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Review

E6 GUT and Baryon Asymmetry Generation in the E6CHM

I.E.Tamm Theory Department, P.N. Lebedev Physical Institute of the Russian Academy of Sciences, 53 Leninskiy Prospekt, 119991 Moscow, Russia
Universe 2022, 8(1), 33; https://doi.org/10.3390/universe8010033
Submission received: 30 November 2021 / Revised: 26 December 2021 / Accepted: 1 January 2022 / Published: 5 January 2022
(This article belongs to the Special Issue Investigating the Matter-Antimatter Asymmetry)

Abstract

:
Grand unified theories (GUTs) may result in the E 6 -inspired composite Higgs model (E 6 CHM) at low energies, almost stabilizing the electroweak scale. We consider an orbifold GUT in 6 dimensions in which the E 6 -gauge group is broken to the gauge symmetry of the standard model (SM) while different multiplets of the SM fermions come from different 27-plets. The strongly coupled sector of the E 6 CHM is confined on the brane where E 6 is broken down to its S U ( 6 ) subgroup. Near the scale of f 5 TeV , this approximate S U ( 6 ) symmetry is expected to be further broken down to its S U ( 5 ) subgroup, which contains the SM-gauge group. Such a breakdown leads to a set of pseudo-Nambu–Goldstone bosons (pNGBs) that includes an SM-like Higgs doublet. The approximate gauge coupling unification in the E 6 CHM takes place at high energies when the right-handed top quark is a composite fermion. To ensure anomaly cancellation, the weakly coupled sector of this model contains extra exotic matter beyond the SM. We discuss the mechanism of the generation of matter–antimatter asymmetry within the variant of the E 6 CHM in which the baryon number and CP invariance are violated.

1. Introduction

It is well known that the standard model (SM) of elementary particles, which involves all known fundamental bosons and fermions, describes rather precisely the major part of all experimental data. At very high energies, the SM can be embedded into grand unified theories (GUTs) [1]. In the simplest GUTs based on the S U ( 5 ) -gauge group, each SM family of fermions is composed of one antifundamental and one antisymmetric second-rank tensor representation of S U ( 5 ) , i.e., 5 ¯ + 10 . In the case of the S O ( 10 ) GUTs, each family of quarks and leptons fills in a complete single 16-dimensional spinor representation of S O ( 10 ) . This representation also contains the right-handed neutrino, which may be used for the see-saw mechanism [2,3].
Supersymmetry (SUSY) implies that each supermultiplet includes the same number of bosonic and fermionic degrees of freedom. In N = 1 SUSY GUTs with the E 6 -gauge group, the fundamental 27 representation of E 6 decomposes under the S O ( 10 ) × U ( 1 ) ψ subgroup as
27 16 , 1 24 10 , 2 24 1 , 4 24 ,
where the first and second quantities in brackets are the S O ( 10 ) representation and its U ( 1 ) ψ charge. As before, the supermultiplet 16 , 1 24 can include one family of quarks and leptons. The doublet of the Higgs bosons may form components of the supermultiplet 10 , 2 24 . The SM-gauge bosons are assigned to the adjoint representation of E 6 , i.e., a 78-plet. In N = 2 SUSY GUTs based on the E 8 -gauge symmetry, all SM bosons and SM fermions may belong to a single 248 representation of E 8 which decomposes under the E 6 subgroup of E 8 , as follows:
248 78 3 × 27 3 × 27 ¯ 8 × 1 .
In Equation (2), 3 generations of the SM fermions can be associated with 3 27-plets which may also contain the doublet of the Higgs bosons, while some components of the 78-plet may form the multiplets of the SM-gauge bosons.
The breakdown of gauge symmetry within the SUSY GUTs near some high energy scale M X 10 16 10 17 GeV can result in the gauge group and field content of the SM. In this case, below the scale of M X , the Higgs scalar potential takes the form
V ( H ) = m H 2 H H + λ ( H H ) 2 + .
In order to ensure that, at low energies, the doublet of the Higgs fields acquires vacuum expectation value (VEV) H = v / 2 174   GeV breaking the electroweak (EW) symmetry, | m H 2 | is required to be of the order of ( 100   GeV ) 2 . On the other hand, most commonly, | m H 2 | is about M X 2 , and an enormous amount of fine tuning is needed to keep | m H 2 | ( 100   GeV ) 2 .
Such enormous fine tuning can be avoided if the breakdown of gauge symmetry in SUSY GUTs leads to the extension of the SM with softly broken supersymmetry. The cancellation of quadratic divergences [4,5,6,7] within the minimal supersymmetric standard model (MSSM) stabilises the EW scale, solving the hierarchy problem [8,9] (for a review see [10]). N = 1 SUSY also facilitates the high-energy convergence of the SM-gauge couplings [11,12,13,14] which allows the SM-gauge group, i.e., S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y , to be embedded into SUSY GUTs. Theories with flat [15,16] and warped [17,18] extra spatial dimensions provide new insight into gauge coupling unification [19,20] and also permit the hierarchy between the EW and Planck scales to be explained.
Alternatively, the Higgs boson can be a composite state. Composite Higgs models include two sectors (for a review, see ref. [21]). One of them involves weakly-coupled elementary particles with the quantum numbers of all SM-gauge bosons and SM fermions. The second strongly coupled sector gives rise to a set of bound states that, in particular, contains Higgs doublet. The corresponding idea was proposed in the 1970s [22,23] and 1980s [24,25,26,27,28,29,30,31]. This implies that the EW scale is generated dynamically in a strongly interacting sector, in analogy with the origin of the QCD scale. In general, these models lead to a relatively large quartic coupling λ at the EW scale, and the composite Higgs state tends to be quite heavy. The rather small values of the parameters λ 0.13 and m H 2 ( 90   GeV ) 2 in Equation (3), which are associated with the measured Higgs mass m h 125–126 GeV , indicate that the Higgs doublet may emerge as a set of pseudo-Nambu–Goldstone bosons (pNGB). The appearance of such pNGB states can be caused by the spontaneous breakdown of an approximate global symmetry of the strongly coupled sector.
In SUSY GUTs with the E 8 × G 0 (or E 6 × G 0 )-gauge group, the breakdown of gauge symmetry at high energies down to the S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y × G subgroup may lead to the S U ( 6 ) global symmetry in the strongly interacting sector [32,33,34,35,36,37]. Hereafter, it is assumed that fields, which compose the strongly coupled sector, can be charged under both the E 8 ( E 6 )- and G 0 (G)-gauge symmetries, whereas the elementary states belonging to the weakly coupled sector participate in the E 8 ( E 6 ) interactions only. The scenario mentioned above is realised if, for instance, in the strongly interacting sector, E 8 is broken to E 6 , with sequential breakdown of E 6 to its S U ( 6 ) subgroup near the GUT scale M X . The spontaneous S U ( 6 ) symmetry, breaking at much lower energies to S U ( 5 ) , which contains the SM-gauge group, gives rise to the 11 pNGBs in this E 6 -inspired composite Higgs model (E 6 CHM) [32,33,34,35,36,37]. The corresponding set of the pNGBs involves the Higgs doublet. It is worth noting that the E 6 CHM can not appear as a low energy limit of the heterotic superstring theory with E 8 × E 8 -gauge symmetry. Some phenomenological consequences of the heterotic string model were discussed in [38,39].
This review paper is organised as follows. In the next Section, we briefly review the composite Higgs models and specify the E 6 CHM. To suppress the proton decay rate and the Majorana masses of the left-handed neutrino within the E 6 CHM, the elementary fermions with different baryon and lepton numbers should stem from different fundamental representations of E 6 , whereas all other components of the corresponding 27-plets are expected to gain masses of the order of M X . In this context, in Section 3, we present a six-dimensional ( 6 D ) orbifold GUT model based on the E 6 × G 0 -gauge group in which the appropriate splitting of the fundamental representations of E 6 can be achieved. The observed baryon asymmetry in the universe stimulates the exploration of different extensions of the SM. This asymmetry can be created dynamically within the scenarios satisfying Sakharov conditions [40]. A number of such new physics scenarios were proposed, including GUT baryogenesis [41,42,43,44,45,46,47], baryogenesis via leptogenesis [48], the Affleck–Dine mechanism [49,50], electroweak baryogenesis [51], etc. In Section 4 we consider the process of the baryon asymmetry generation in the framework of the E 6 CHM with explicitly broken U ( 1 ) B baryon symmetry. The sizeable baryon number asymmetry can be induced in this model if CP is violated. Section 5 concludes the paper.

2. Composite Higgs Models and E 6 CHM

2.1. Composite Higgs Models—A Brief Review

The strongly interacting sector of the minimal composite Higgs model (MCHM) possesses a global S O ( 5 ) × U ( 1 ) X symmetry [52]. It is expected that, near the scale f 1–10 TeV , this global symmetry is broken down to S O ( 4 ) × U ( 1 ) X S U ( 2 ) W × S U ( 2 ) R × U ( 1 ) X , which includes the S U ( 2 ) W × U ( 1 ) Y -gauge group as a subgroup. Such a breakdown gives rise to a set of pNGBs which form the Higgs doublet. Via the AdS/CFT correspondence, such composite Higgs scenarios are dual to the Randall–Sundrum (RS) extra-dimensional scenarios, with the SM fields in the bulk [52,53]. In the RS scenarios, Kaluza–Klein excitations of the SM fields are associated with the bound states at the compositeness scale, f [52,53,54,55].
Thus, the strongly coupled sector in the composite Higgs models should result in a set of massive fields with quantum numbers of all SM particles, which are the so-called composite partners of the SM states. The elementary states from the weakly coupled sector mix with their composite partners. Therefore, at low energies, those states identified with SM fermions (bosons) are superpositions of the elementary fermionic (bosonic) states and their fermionic (bosonic) composite partners. Such partial compositeness [55,56] implies that the SM states couple to the composite Higgs with a strength which is determined by the fraction of the compositeness of this state. As consequence, the effective up- and down-quark Yukawa couplings ( y i j u and y i j d ) are given by
y i j u = s q i Y i j u s u j , y i j d = s q i Y i j d s d j ,
where s q i , s u j and s d j are the fractions of compositeness of the left-handed SM quarks as well as the right-handed SM quarks of up- and down-types, whereas i , j = 1 , 2 , 3 . In Equation (4), Y i j u and Y i j d are the effective Yukawa couplings of the composite Higgs field to the composite partners of the up- and down-quarks. The couplings of the elementary states to the operators of the strongly interacting sector explicitly break its global symmetry. In these models, the Higgs potential arises from loops containing elementary states. This results in the suppression of the effective quartic Higgs coupling. The contributions of the composite partners of the SM states to the EW observables, including the S ^ and T ^ parameters, were examined in [57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79,80,81,82,83,84]. Within the MCHM, the custodial symmetry S U ( 2 ) c u s t S O ( 4 ) S U ( 2 ) W × S U ( 2 ) R [85] protects the Peskin–Takeuchi T ^ parameter [86] against the contributions of new composite states.
In the phenomenologically viable composite Higgs models, the fractions of compositeness of the first and second generation fermions should be rather small. If this is the case, the corresponding states have small couplings to the Higgs doublet and therefore tend to be light. In other words, the observed mass hierarchy in the quark and lepton sectors can be reproduced if the couplings of the elementary fermions associated with the first and second generations to the states from the strongly interacting sector are very weak. Such weak couplings result in some suppression of flavour-changing processes and modifications of the W and Z couplings [55,87], playing the role of the generalization of the Glashow–Iliopoulos–Maiani (GIM) mechanism of the SM [88]. Although this generalization of the GIM mechanism reduces the contributions of new composite states to the off-diagonal flavour transitions in the quark and lepton sectors, this suppression is not sufficient. To avoid dangerous flavour-changing processes, the composite Higgs models have to satisfy a set of constraints which were examined in [81,82,83,84,89,90,91,92,93,94,95,96,97]. If the matrices of effective Yukawa couplings in the strongly interacting sector, such as Y i j u and Y i j d , are structureless, then the adequate suppression of the non-diagonal flavour transitions can be achieved only if f is larger than 10 TeV [81,82,83,89,90,91,94,95]. At the same time, in the composite Higgs models with flavour symmetries [79,80,81,89,92,93,98,99,100], under which the third-generation elementary fermions transform as singlets while the first two generations of elementary fermions form different U ( 2 ) doublets, the corresponding constraints can be fulfilled even if f 1 TeV [92,93].
When f 10 TeV , approximate U ( 1 ) B and U ( 1 ) L symmetries, which ensure the conservation of the baryon and lepton numbers, should be imposed in the strongly interacting sector of the composite Higgs models. These symmetries are needed to suppress the operators that give rise to the Majorana masses of the left-handed neutrinos and the baryon number violation. The implications of the composite Higgs models were considered for Higgs physics [73,74,75,76,77,78,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124], gauge coupling unification [125,126], dark matter [57,107,127,128] and collider phenomenology [70,71,72,73,79,80,89,93,123,124,129,130,131,132,133,134,135,136,137,138,139,140,141,142,143,144,145,146,147,148,149,150,151,152,153]. Non-minimal composite Higgs models were explored in [57,101,102,103,104,105,106,107,127,128,154,155,156,157,158,159,160,161,162,163].
Since the top quark is rather heavy, the left-handed and right-handed top quarks (t and t c ) should have substantial fractions of compositeness. In the case when t c is in an entirely composite state, the approximate unification of the SM-gauge couplings in the composite Higgs models may take place if all multiplets in the strongly coupled sector form complete representations of S U ( 5 ) , while the weakly coupled sector includes the following set of matter multiplets [32,164]:
( q i , d i c , i , e i c ) + u α c + q ¯ + d c ¯ + ¯ + e c ¯ ,
where i = 1 , 2 , 3 runs over all 3 generations and α = 1 , 2 runs over the first 2 generations. Here, we have denoted the right-handed charged leptons and the right-handed down- and up-type quarks by e i c , d i c and u α c , whereas i and q i are associated with the left-handed lepton and quark doublets. In Equation (5), e c ¯ , d c ¯ , q ¯ and ¯ correspond to the exotic fermions which have opposite S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y quantum numbers compared to the right-handed charged leptons, right-handed down-type quarks, as well as left-handed quark and left-handed lepton doublets, respectively. The set of elementary states (5) contains all SM fermions except t c . The particle content of the weakly coupled sector is chosen so that anomaly cancellation takes place.
The phenomenological viability of such composite Higgs models implies that the strongly coupled sector leads to a set of composite fermions that form 10 + 5 ¯ multiplets of S U ( 5 ) . All of them, except the components of the 10-plet associated with the composite t c , get combined with q ¯ , d c ¯ , ¯ and e c ¯ , composing vector-like states. The composite S U ( 3 ) C triplet identified with t c survives to the EW scale.
The presence of exotic vector-like fermions facilitates the convergence of the SM-gauge couplings at high energies. In the one-loop approximation, the renormalisation group (RG) flow of the SM-gauge couplings is described by a system of RG equations (RGEs), which can be written in the following form:
d α i d t = β i α i 2 ( 2 π ) ,
where b i are one-loop beta functions with the index i running from 1 to 3, corresponding to U ( 1 ) Y , S U ( 2 ) W and S U ( 3 ) C interactions, t = ln μ / M Z and μ is a renormalisation scale. Then, using the solutions of the RGEs (6), one can find α 3 ( M Z ) , for which the exact gauge coupling unification takes place
1 α 3 ( M Z ) = 1 b 1 b 2 b 1 b 3 α 2 ( M Z ) b 2 b 3 α 1 ( M Z ) .
If all bound states in the strongly interacting sector compose complete S U ( 5 ) multiplets, they contribute equally to b i . Because of this, the inclusion of the composite sector fields does not change the differential running. In other words, in the one-loop approximation, ( b i b j ) are determined by the particle content of the weakly coupled sector (5). Then, from Equation (7), it follows that for sin 2 θ W = 0.231 , α ( M Z ) = 1 / 127.9 and the values of ( b i b j ) corresponding to the elementary particle spectrum (5), the exact gauge coupling unification may be obtained if α 3 ( M Z ) 0.109 . Such unification of the SM-gauge couplings takes place near the scale M X 10 15 10 16 GeV . Despite the fact that α 3 ( M Z ) 0.109 is considerably lower than the central measured value of this coupling, this estimation indicates that, in the composite Higgs model with a composite t c , an approximate unification of the SM-gauge couplings can be attained.

2.2. E 6 CHM

Hereafter, we assume that the weakly coupled sector of the E 6 CHM involves all elementary states specified in Equation (5). Since the strongly coupled sector of the E 6 CHM possesses an approximate global S U ( 6 ) symmetry, which is expected to be broken down to its S U ( 5 ) subgroup near some scale f v 246 GeV so that the S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y -gauge symmetry remains intact, all composite states must come in complete S U ( 5 ) multiplets. Therefore, an approximate gauge coupling unification may be achieved. Because the Lagrangian of the strongly interacting sector of the E 6 CHM does not possess any custodial symmetry that may protect the Peskin–Takeuchi T ^ parameter against contributions of extra composite states, | T ^ | should be of the order ξ v 2 / f 2 [57]. In this case, the electroweak precision measurements, which constrain | T ^ | 0.002 , result in the lower bound
f 5 TeV .
In the model under consideration, more stringent restrictions on the scale f can be avoided. Indeed, the non-diagonal flavour transitions can be suppressed by imposing approximate flavour symmetry. Due to the mixing between the elementary states and their composite partners, the interactions in the strongly coupled sector may also induce the dimension-5 operators of the form i j H H / f , which give rise to overly large Majorana neutrino masses, as well as a set of baryon number-violating operators. All these operators are suppressed by the small fractions of compositeness of the SM fermions and by the relatively large scale f. Nevertheless such suppression is not sufficient if f 10 TeV . The baryon- and lepton number-violating operators can be forbidden by postulating the conservation of baryon and lepton numbers in the E 6 CHM. In principle, the corresponding U ( 1 ) B and U ( 1 ) L symmetries can be part of the symmetries of the composite sector. The G 0 -gauge symmetry associated with the strongly coupled sector might be broken down to its subgroup G so that the U ( 1 ) B and U ( 1 ) L symmetries are preserved to very good approximations. As a consequence, at low energies, the Lagrangian of the strongly interacting sector of the E 6 CHM respects the approximate S U ( 6 ) × U ( 1 ) B × U ( 1 ) L global symmetry.
The global U ( 1 ) L symmetry has to be broken down to
Z 2 L = ( 1 ) L ,
where L is a lepton number. This breakdown allows the left-handed neutrinos to gain non-zero Majorana masses. When Z 2 L remains in almost exact discrete symmetry, it forbids all operators that lead to rapid proton decay.
Near the scale f, the approximate global S U ( 6 ) symmetry of the strongly coupled sector is broken down to S U ( 5 ) in the E 6 CHM. The S U ( 6 ) and S U ( 5 ) groups have 35 and 24 generators, t a , respectively, which are normalised so that Tr t a t b = 1 2 δ a b . Here, we denote the 11 broken generators from the coset S U ( 6 ) / S U ( 5 ) by T a ^ . The generators of the unbroken S U ( 5 ) subgroup of S U ( 6 ) are denoted by T a . The 11 pNGB states can be parameterised in terms of a 6-component unit vector Ω [32]
Ω T = Ω 0 T Σ T = e i ϕ 0 15 f C ϕ 1 C ϕ 2 C ϕ 3 C ϕ 4 C ϕ 5 cos ϕ ˜ 2 f + 3 10 C ϕ 0 , C = i ϕ ˜ sin ϕ ˜ 2 f , ϕ ˜ = 3 10 ϕ 0 2 + | ϕ 1 | 2 + | ϕ 2 | 2 + | ϕ 3 | 2 + | ϕ 4 | 2 + | ϕ 5 | 2 ,
where
Ω 0 T = ( 0 0 0 0 0 1 ) , Σ = e i Π / f , Π = Π a ^ T a ^ .
In Equation (10), ϕ 0 is a real field, whereas ϕ 1 ϕ 2 ϕ 3 ϕ 4 and ϕ 5 are complex fields. Taking into account that ϕ 0 and ϕ ˜ are invariant under the S U ( 5 ) symmetry transformations, vector Ω can be decomposed into 5 + 1 under the unbroken S U ( 5 ) symmetry. Thus, it is convenient to introduce a 5-component multiplet H ˜ = ( ϕ 1 , ϕ 2 , ϕ 3 , ϕ 4 , ϕ 5 ) and A = ϕ 0 , which is a SM singlet field. The first two components of H ˜ compose an S U ( 2 ) W doublet. Therefore these components can be associated with the SM-like Higgs doublet H. A total of 3 other components, T = ( ϕ 3 , ϕ 4 , ϕ 5 ) , form an S U ( 3 ) C triplet. Since in the SM the Higgs doublet does not carry any baryon and/or lepton numbers (B and L), all components of the vector Ω have B = L = 0 . The Lagrangian that describes the interactions of these pNGBs is given by
L p N G B = f 2 2 | D μ Ω | 2 .
Integrating out composite partners of the SM states and exotic fermions, one can obtain the pNGB effective potential V e f f ( H ˜ , T , ϕ 0 ) . This potential is induced by the interactions of the SM states with their composite partners that break S U ( 6 ) symmetry. In the exact S U ( 6 ) symmetry limit, it vanishes. The investigation of the pNGB potentials within similar models revealed that there exists a large part of the parameter space where the EW symmetry is broken, while S U ( 3 ) C is preserved [57,127]. Nevertheless, a significant tuning, ∼0.01%, is required in order to get a 125 GeV Higgs state in E 6 CHM because f 5 TeV . It was shown that the appropriate quadratic term m H 2 | H | 2 in the pNGB effective potential can be induced [127]. The analysis performed in the models, which are similar to the E 6 CHM, indicated that, in the corresponding part of the parameter space, the S U ( 3 ) C triplet scalar T is considerably heavier than the SM-like Higgs boson.
As mentioned before, the weakly coupled sector of the E 6 CHM includes a set of elementary states (5), whereas the right-handed top quark t c is a composite state. Such a scenario implies that the dynamics of the strongly interacting sector results in the formation of the composite 10 + 5 ¯ multiplets of S U ( 5 ) . These S U ( 5 ) multiplets get combined with ¯ , e c ¯ , q ¯ and d c ¯ , leading to a set of massive vector-like fermions as well as composite t c . The composite 10 + 5 ¯ multiplets of S U ( 5 ) may originate from two 6 ¯ -plets ( 6 ¯ 1 and 6 ¯ 2 ) and one 15 -plet of S U ( 6 ) . The 15 -plet and 6 ¯ -plet have the following decomposition in terms of S U ( 5 ) representations:
15 10 5 , 6 ¯ 5 ¯ 1 .
The components of 6 ¯ 1 , 6 ¯ 2 and 15 decompose under S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y × U ( 1 ) B × U ( 1 ) L as follows:
15 Q = 3 , 2 , 1 6 , 1 3 , 0 , t c = 3 , 1 , 2 3 , 1 3 , 0 , E c = 1 , 1 , 1 , 1 3 , 0 , D = 3 , 1 , 1 3 , 1 3 , 0 , L ¯ = 1 , 2 , 1 2 , 1 3 , 0 ; 6 ¯ 2 D 2 c = 3 ¯ , 1 , 1 3 , 1 3 , 0 , L 2 = 1 , 2 , 1 2 , 1 3 , 0 , N 2 = 1 , 1 , 0 , 1 3 , 0 , 6 ¯ 1 D 1 c = 3 ¯ , 1 , 1 3 , B 6 ¯ 1 , L 6 ¯ 1 , L 1 = 1 , 2 , 1 2 , B 6 ¯ 1 , L 6 ¯ 1 , N 1 = 1 , 1 , 0 , B 6 ¯ 1 , L 6 ¯ 1 .
In Equation (12), the first and second quantities in brackets are the S U ( 3 ) C and S U ( 2 ) W representations, while the third, fourth and fifth quantities are the U ( 1 ) Y , U ( 1 ) B and U ( 1 ) L charges, respectively. Since the right-handed top quark belongs to the 15 -plet, all components of this multiplet should carry the same baryon and lepton numbers as t c , i.e., B 15 = 1 / 3 and L 15 = 0 . After the S U ( 6 ) symmetry breaking, a 5 ¯ -plet from the 6 ¯ 2 and 5 -plet from the 15 -plet should compose vector-like states. This can be possible only if B 6 ¯ 2 = 1 / 3 and L 6 ¯ 2 = 0 . Although the baryon and lepton numbers of the components of the 6 ¯ 1 multiplet are not fixed in the E 6 CHM, the S U ( 5 ) singlet components of 6 ¯ 1 and 6 ¯ 2 may gain mass through the interaction ( 6 ¯ 1 Ω ) ( Ω 6 ¯ 2 ) if B 6 ¯ 1 = 1 / 3 and L 6 ¯ 1 = 0 .
As pointed out before, in the composite Higgs models, the elementary fermions acquire masses through mixing with their composite partners. From the conservation of baryon and lepton numbers, it follows that in the E 6 CHM, different multiplets of elementary fermions should come from different representations of the GUT-gauge group. All other components of the corresponding GUT multiplets have to be extremely heavy. Therefore, elementary fermions appear at low energies as incomplete GUT multiplets. In the case of the simplest S U ( 5 ) GUT, the elementary fermions constitute the following set of incomplete S U ( 5 ) multiplets:
u α c 10 α u = 10 , 1 3 , 0 α q i 10 i q = 10 , 1 3 , 0 i d i c 5 ¯ i d = 5 ¯ , 1 3 , 0 i e i c 10 i e = 10 , 0 , 1 i i 5 ¯ i = 5 ¯ , 0 , 1 i ,
where the first, second and third quantities in brackets are the S U ( 5 ) representation and the U ( 1 ) B and U ( 1 ) L charges. In Equation (13), α = 1 , 2 and i = 1 , 2 , 3 . The Higgs doublet h is normally embedded into the fundamental representation of S U ( 5 ) , i.e., h 5 h . In this scenario, the Yukawa interactions of the SM, which induce the masses of the up-type quarks at low energies, have the following S U ( 5 ) structure:
L S U ( 5 ) u h α i u 10 α u 10 i q 5 h .
In the simplest S U ( 5 ) models, the masses of the charged leptons and down-type quarks are generated through the Yukawa interactions
L S U ( 5 ) d h i j e 10 i e 5 ¯ j 5 ¯ h + h i j d 10 i q 5 ¯ j d 5 ¯ h .
The composite partners of the elementary quarks and leptons must be embedded into the representations of the S U ( 6 ) group so that the Yukawa interactions (14) and (15) are allowed. In this case, the Higgs multiplet 5 h has to be replaced by the unit vector Ω . Moreover, instead of 10 α u and 10 i q of S U ( 5 ) , one needs to include two S U ( 6 ) multiplets which involve an S U ( 5 ) decuplet. The simplest S U ( 6 ) multiplet of this type is an antisymmetric second-rank tensor field 15 . The next-simplest S U ( 6 ) representation that contains an S U ( 5 ) decuplet is a totally antisymmetric third-rank tensor 20 that has the following decomposition in terms of S U ( 5 ) representations: 20 = 10 10 ¯ . The generalisation of the Yukawa interaction (14) to the case of S U ( 6 ) symmetry can be written as
L S U ( 6 ) u 20 × 15 × 6 .
In Equation (16), the 6 -plet has to be identified with the unit vector Ω . Thus, there are two different scenarios. In scenario A, the composite partners of u α c and q i ( U α and Q i ) are components of 15 ( U α ) and 20 ( Q i ) representations of S U ( 6 ) , while in scenario B, the composite partners of u α c and q i belong to 20 ( U α ) and 15 ( Q i ) , respectively. Below scale f, the mixing between incomplete S U ( 5 ) representations ( 10 α u and 10 i q ) and their composite partners is induced, and the Yukawa interactions (14) are reproduced.
In scenario A, the S U ( 6 ) generalisation of the Yukawa interactions (15) is given by
L S U ( 6 ) d 20 × 15 ¯ × 6 ¯ ,
where 6 ¯ Ω . In Equation (17), the 20 -plet is associated with the S U ( 6 ) representations involving the composite partners of q i , i.e., 20 ( Q i ) , while the 15 ¯ -plet involves the 5 ¯ multiplet of the S U ( 5 ) group that should include the composite partners of d i c , i.e., 15 ¯ 15 ¯ ( D i ) .
In scenario B, the S U ( 6 ) generalisation of the S U ( 5 ) structure of the Yukawa interactions (15) takes the form:
L S U ( 6 ) d 15 × 6 ¯ × 6 ¯ .
In this case, again, the 6 ¯ in Equation (18) must be identified with Ω . The 15 -plet corresponds to 15 ( Q i ) , which contains the composite partners of q i , whereas the 6 ¯ -plet has to involve the composite partners of d i c ( D i ), i.e., 6 ¯ 6 ¯ ( D i ) . After the breakdown of the S U ( 6 ) global symmetry near the scale f, Equation (18) should lead to the Yukawa interactions (15).
The interactions (18) can also be used to generate the masses of charged leptons in both scenarios A and B. In this case, 15 ( E i ) and 6 ¯ ( L i ) should contain the composite partners of e i c and i , respectively. In the simplest S U ( 5 ) GUT, the masses of the left-handed neutrinos can be induced through the interactions
L S U ( 5 ) ν k i j 5 ¯ i 5 h 5 ¯ j 5 h .
The S U ( 6 ) generalisation of the interactions (19) takes the form:
L S U ( 6 ) ν ϰ i j 6 ¯ × 6 6 ¯ × 6 ,
where 6 ¯ should be associated with 6 ¯ ( L i ) , and 6 Ω . The inclusion of interactions (20) implies that global U ( 1 ) L symmetry is broken down to Z 2 L = ( 1 ) L . Since, in the E 6 CHM, the lepton number is preserved to a very good approximation, ϰ i j are expected to be very small, giving rise to tiny masses of the left-handed neutrinos.

3. From E 6 Orbifold GUT to the E 6 CHM

As previously noted, the nearly exact conservation of the baryon and lepton numbers at low energies requires different multiplets of elementary quarks and leptons to stem from different representations of the GUT group. In this sense, the U ( 1 ) B and U ( 1 ) L charges of the corresponding GUT multiplets are determined by the baryon and lepton numbers of the fermion components of these representations that survive to low energies. All other components of these GUT multiplets must gain huge masses. In this section, we focus on the SUSY GUTs with the E 6 -gauge group and assume that elementary fermions originate from different 27 -plets and 27 ¯ -plets of E 6 . The complete set of the S U ( 6 ) and E 6 representations associated with the multiplets of elementary fermions is given by
q ¯ 15 ¯ q ¯ = 15 ¯ , 1 3 , 0 27 ¯ q ¯ = 27 ¯ , 1 3 , 0 , e c ¯ 15 ¯ e ¯ = 15 ¯ , 1 3 , 0 27 ¯ e ¯ = 27 ¯ , 1 3 , 0 , d c ¯ 6 d ¯ = 6 , B 6 ¯ 2 , L 6 ¯ 2 27 ¯ d ¯ = 27 ¯ , B 6 ¯ 2 , L 6 ¯ 2 , ¯ 6 ¯ = 6 , B 6 ¯ 2 , L 6 ¯ 2 27 ¯ ¯ = 27 ¯ , B 6 ¯ 2 , L 6 ¯ 2 , u α c 15 α u = 15 , 1 3 , 0 α 27 α u = 27 , 1 3 , 0 α , q i 15 i q = 15 , 1 3 , 0 i 27 i q = 27 , 1 3 , 0 i , e i c 15 i e = 15 , 0 , 1 i 27 i e = 27 , 0 , 1 i , d i c 6 ¯ i d = 6 ¯ , 1 3 , 0 i 27 i d = 27 , 1 3 , 0 i , i 6 ¯ i = 6 ¯ , 0 , 1 i 27 i = 27 , 0 , 1 i .
In Equation (21), the first quantity in brackets is either the S U ( 6 ) or E 6 representation, whereas the second and third quantities are the U ( 1 ) B and U ( 1 ) L charges. It is rather problematic to get the desirable splitting of the 27 -plets and 27 ¯ -plets within four-dimensional E 6 GUTs. Nevertheless, the appropriate splitting of these E 6 representations can occur in the orbifold GUTs with extra dimensions.
Orbifolding in higher-dimensional theories offers new possibilities for gauge symmetry breaking which have been explored within the SUSY GUT models in five dimensions [165,166,167,168,169,170,171,172,173,174,175,176,177,178,179,180,181,182,183,184,185,186,187,188,189,190,191,192,193] and six dimensions [188,189,190,191,192,193,194,195,196,197,198,199,200,201,202,203,204,205,206,207,208]. Initially, in the string-motivated work [209,210,211,212,213,214,215], it was pointed out that the breakdown of the gauge symmetry can be caused by identifications imposed on the gauge fields under the spacetime symmetries of an orbifold. More recently, it was argued that the orbifold compactifications of the heterotic string may lead to five-dimensional or six-dimensional GUT structures which are similar to orbifold GUT models [216,217,218,219,220,221,222]. The unification of gauge couplings in the 5 D and 6 D orbifold GUTs was examined in [179,180,181,182,183,184,185,186,187,206,207]. The models of composite fermions were studied in the context of Sherk–Schwarz compactification in [223].
In this section, an N = 1 SUSY GUT in 6 D , which results in a set of elementary fermions given by Equation (5), is considered. This SUSY GUT is based on the E 6 × G 0 -gauge group. Near some high energy scale M X , the E 6 and G 0 groups are broken down to S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y and G, respectively. The elementary bosons and fermions participate in the E 6 interactions only. Fields from the composite sector are charged under both the G 0 (G) and E 6 -gauge symmetries. The phenomenological viability of such a model requires the adequate suppression of operators which give rise to proton decay. In the context of orbifold GUTs, the proton stability was discussed in [176,177,178,180,181,182,183,184,185,208]. It was shown that the experimental lower limit on the proton lifetime can be satisfied if M X 10 16 GeV [208].
All elementary fermions in the model under consideration are components of the bulk 27-plets. In the four-dimensional N = 1 SUSY GUT, the fundamental 27-dimensional representation of E 6 contains components Φ n ( n = 1 , 2 , , 27 ) associated with the supermultiplets of one generation of ordinary matter, including the right-handed neutrino ( ν c ), i.e., q, , u c , d c , e c and ν c . In addition, it also involves the supermultiplets that correspond to the charged ± 1 / 3 exotic quarks (h and h c ), 2 S U ( 2 ) W doublets ( h d and h u ) as well as a SM singlet s. Each 6 D fermion state is formed by 2 4 D Weyl fermions, ψ and ψ c . The minimal N = 1 SUSY in 6 D implies that each 6 D superfield involves one 6 D fermion field and two complex scalars, ϕ and ϕ c . These fields compose a 4 D N = 2 hypermultiplet that contains 2 4 D N = 1 chiral superfields, Φ = ( ϕ , ψ ) and Φ ¯ = ( ϕ c , ψ c ) , with opposite quantum numbers. Therefore, each 6 D 27-plet Φ ^ n includes two 4 D N = 1 supermultiplets, Φ n (27-plet) and Φ ¯ n ( 27 ¯ -plet). In other words, the N = 1 SUSY in 6 D corresponds to N = 2 supersymmetry in 4 D .
The E 6 -gauge supermultiplet which should exist in the bulk must include vector bosons A M ( M = 0 , 1 , 2 , 3 , 5 , 6 ) as well as 6 D Weyl fermions (gauginos). Each 6 D gaugino is formed by 2 4 D Weyl fermions, λ and λ . The components of vector bosons and gauginos can be grouped into chiral and vector supermultiplets of the N = 1 SUSY in 4 D , i.e.,
V = ( A μ , λ ) , Σ = ( A 5 + i A 6 ) / 2 , λ .
In Equation (22), μ = 0 , 1 , 2 , 3 , whereas λ , λ , A M , V and Σ are matrices in the adjoint E 6 representation. The N = 1 supermultiplets (22) compose an N = 2 vector supermultiplet in 4 D .
We assume that 2 extra dimensions z ( = x 6 ) and y ( = x 5 ) are compact with z ( π R 6 , π R 6 ] and y ( π R 5 , π R 5 ] that corresponds to the compactification of extra dimensions on a torus T 2 with fixed radii R 5 and R 6 , where R 5 and R 6 are defined by the scale M X . Using Z 2 symmetry, the orbifold T 2 / Z 2 can be obtained. The Z 2 transformation acts on T 2 according to z z and y y . The components of the bulk supermultiplets also transform under Z 2 symmetry, while the Lagrangian of the model under consideration has to be invariant under this transformation. The Z 2 symmetry allows the physical region to be reduced to a pillow with the 4 fixed points as corners: ( 0 , 0 ) , ( π R 5 , 0 ) , ( 0 , π R 6 ) and ( π R 5 , π R 6 ) .

3.1. The E 6 Symmetry Breaking to S U ( 4 ) × S U ( 2 ) W × S U ( 2 ) N × U ( 1 )

In this section, we consider a 6 D SUSY GUT compactified on the orbifold T 2 / ( Z 2 × Z 2 I × Z 2 I I ) , where Z 2 , Z 2 I and Z 2 I I are reflections. In particular, a Z 2 transformation is defined as before, i.e., z z and y y . The reflection Z 2 I acts as z z and y y , where y = y π R 5 / 2 . The reflection Z 2 I I is defined by z z and y y , where z = z π R 6 / 2 . The reflection symmetries Z 2 I and Z 2 I I introduce additional fixed points, resulting in the physical region in which z [ 0 , π R 6 / 2 ] and y [ 0 , π R 5 / 2 ] . The irreducible space is a pillow limited by fixed points with 4 4 D branes (walls) which are located at its corners.
The Lagrangian of this 6 D SUSY GUT must be invariant under the transformations of Z 2 , Z 2 I and Z 2 I I symmetries. Each reflection has its own orbifold parity, i.e., P, P I and P I I . The components Φ n and Φ ¯ n of 6 D 27-plets transform under Z 2 , Z 2 I and Z 2 I I reflections as follows:
Φ n ( x , y , z ) = P n n Φ n ( x , y , z ) , Φ ¯ n ( x , y , z ) = P n n Φ ¯ n ( x , y , z ) , Φ n ( x , y , z ) = P n n I Φ ^ n ( x , y , z ) , Φ ¯ n ( x , y , z ) = P n n I Φ ¯ n ( x , y , z ) , Φ n ( x , y , z ) = P n n I I Φ ^ n ( x , y , z ) , Φ ¯ n ( x , y , z ) = P n n I I Φ ¯ n ( x , y , z ) .
In Equation (23), P, P I and P I I are diagonal matrices which have eigenvalues ± 1 . The diagonal elements of these matrices can be written as
( P ) i i = σ exp { 2 π i Δ α i } , ( P I ) i i = σ I exp { 2 π i Δ I α i } , ( P I I ) i i = σ I I exp { 2 π i Δ I I α i } ,
where σ , σ I , σ I I { + , } are parities of the 6 D 27-plets and α i are E 6 weights which are well-known [193]. The gauge shifts Δ , Δ I and Δ I I associated with Z 2 , Z 2 I and Z 2 I I reflections are chosen so that
Δ = 0 , 0 , 0 , 1 2 , 0 , 0 , Δ I = 1 2 , 1 2 , 1 2 , 1 2 , 1 2 , 0 , Δ I I = 1 2 , 1 2 , 1 2 , 0 , 1 2 , 0 .
The corresponding orbifold parity assignments are shown in Table 1.
The components of the E 6 -gauge supermultiplet (V and Σ ) transform under reflections Z 2 , Z 2 I and Z 2 I I as follows:
V ( x , y , z ) = P V ( x , y , z ) P 1 , V ( x , y , z ) = P I V ( x , y , z ) ( P I ) 1 , V ( x , y , z ) = P I I V ( x , y , z ) ( P I I ) 1 , Σ ( x , y , z ) = P Σ ( x , y , z ) P 1 , Σ ( x , y , z ) = P I Σ ( x , y , z ) ( P I ) 1 , Σ ( x , y , z ) = P I I Σ ( x , y , z ) ( P I I ) 1 ,
where Σ ( x , y , z ) = Σ A ( x , y , z ) T A and V ( x , y , z ) = V A ( x , y , z ) T A , while T A are the E 6 generators. In the orbifold GUT under consideration, the 4 D N = 2 SUSY is broken down to 4 D N = 1 supersymmetry because components Φ n and Φ ¯ n as well as V and Σ transform differently under the reflections. Since P, P I and P I I are not unit matrices, they do not commute with all generators of E 6 . As a consequence, the E 6 -gauge symmetry is broken as well.
From the P parity assignment, it follows that near the fixed point y = z = 0 (brane O) associated with the Z 2 reflection, the E 6 -gauge group is broken down to S U ( 6 ) × S U ( 2 ) N . Indeed, the fundamental representation of E 6 decomposes under S U ( 6 ) × S U ( 2 ) N as follows:
27 ( 15 , 1 ) + ( 6 ¯ , 2 ) .
In Equation (27), the first and second quantities in brackets are the S U ( 6 ) and S U ( 2 ) N representations. From Table 1, one can see that ( 6 ¯ , 2 ) is formed by two S U ( 2 ) W doublets and h d , two SM singlets ν c and s as well as two S U ( 3 ) C triplets d c and h c . Indeed, these components of the 27-plet transform differently under the Z 2 reflection as compared with the other components of the fundamental representation of E 6 which compose the ( 15 , 1 ) supermultiplet of S U ( 6 ) . The unbroken S U ( 6 ) group contains a S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y subgroup. It is assumed that all fields of the strongly interacting sector are localised on the O brane.
At the fixed point y = π R 5 / 2 , z = 0 (brane O I ) of the Z 2 I reflection the E 6 group is broken to its S U ( 6 ) × S U ( 2 ) W subgroup. According to the P I parity assignment, all S U ( 2 ) W doublets from the 27-plet transform differently as compared with the other components of the fundamental representation of E 6 . These S U ( 2 ) W doublets compose the ( 6 , 2 ) representation of S U ( 6 ) . All other components of the 27-plet form ( 15 ¯ , 1 ) of S U ( 6 ) . In this case, the unbroken S U ( 6 ) includes a S U ( 3 ) C subgroup. It is assumed that 2 pairs of ( 15 , 1 ) and ( 15 ¯ , 1 ) of S U ( 6 ) are localised on the brane O I . They are needed to ensure the appropriate breakdown of the E 6 -gauge group to its S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y subgroup.
Near the fixed point y = 0 , z = π R 6 / 2 (brane O I I ) associated with the Z 2 I I reflection the E 6 -gauge group is also broken to S O ( 10 ) × U ( 1 ) . Indeed, the P I I parity assignment indicates that the 16 components of the fundamental representation of E 6 , i.e., q, d c , ν c , h u , h c and s, are odd, composing a 16-dimensional spinor representation of S O ( 10 ) . All other components of the 27-plet are even. Because, in the orbifold GUTs, the mechanism of gauge symmetry breaking preserves the ranks of the group, the unbroken subgroup of the E 6 group has to be S O ( 10 ) × U ( 1 ) . The unbroken S O ( 10 ) contains a S U ( 3 ) C × S U ( 2 ) W subgroup. The 10 components of the 27-plet, i.e., u c , , h d and h, constitute a 10-dimensional vector representation of S O ( 10 ) while the e c component of the 27-plet is an S O ( 10 ) singlet. It is worth noting that the spinor representation of the ordinary S O ( 10 ) and S O ( 10 ) are composed by different components of the 27-plets. This means that S O ( 10 ) and S O ( 10 ) are different subgroups of E 6 . We assume that, on the brane O I I , a 45-dimensional representation of S O ( 10 ) as well as 3 pairs of e i c and e i c ¯ superfields are confined.
At the corner of the physical region, i.e., y = π R 5 / 2 , z = π R 6 / 2 , a fourth fixed point (brane O I I I ) is located. It is associated with the Z 2 I I I symmetry, which is obtained by combining reflections Z 2 , Z 2 I and Z 2 I I . The corresponding parity assignment P I I I = P P I P I I is just an identity matrix. Therefore, near this fixed point, the E 6 -gauge group remains intact, whereas N = 2 SUSY is broken to N = 1 supersymmetry. We assume that two 27-plets reside on the brane O I I I .
The intersection of the E 6 subgroups, which remain intact near the branes O, O I , O I I and O I I I , represents the unbroken gauge group of the effective 4 D theory. The intersection of the E 6 subgroups S U ( 6 ) × S U ( 2 ) N , S U ( 6 ) × S U ( 2 ) W and S O ( 10 ) × U ( 1 ) is S U ( 4 ) × S U ( 2 ) W × S U ( 2 ) N × U ( 1 ) , where the S U ( 4 ) group includes a S U ( 3 ) C subgroup. The S U ( 4 ) group is also a subgroup of S U ( 6 ) and S O ( 10 ) . In Table 2, the charges associated with the U ( 1 ) symmetry are specified.

3.2. The Breakdown of S U ( 4 ) × S U ( 2 ) W × S U ( 2 ) N × U ( 1 ) to S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y

According to Table 1, the bulk 27-plets contain components which have even and odd parities with respect to the transformations of the Z 2 , Z 2 I and Z 2 I I symmetries. At the same time, only components that have all even parities are allowed to have zero modes which may survive below the scale M X . In particular, the elementary fermions, u α c , e i c and e c ¯ , can stem from the bulk 27-plets Φ ^ i u , Φ ^ i u ¯ , Φ ^ i e and Φ ^ i e ¯ . Hereafter, index i = 1 , 2 , 3 runs over three generations. These bulk 27-plets decompose as follows:
Φ ^ i u = 27 , + , + , + , + , Φ ^ i u ¯ = 27 , , , , , Φ ^ i e = 27 , + , + , + , + , Φ ^ i e ¯ = 27 , , , , ,
In Equation (28), the quantities in brackets are the parities of the bulk 27-plets σ , σ I , σ I I and σ I I I as well as the E 6 representations of these 6 D supermultiplets. The parities of Φ ^ i u are such that only the components u i c , e i c and h i of Φ i u have zero modes. Since the parities of the components of Φ i u and Φ ¯ i u are opposite, the N = 1 supermultiplet Φ ¯ i u does not lead to zero modes. On the other hand, the Kaluza–Klein (KK) expansion of Φ ^ i u ¯ involves only the zero modes of components u c ¯ i , e c ¯ i and h ¯ i . The bulk 27-plets Φ ^ i e and Φ ^ i e ¯ result in a similar set of zero modes.
The 45-dimensional representation of S O ( 10 ) that resides on the brane O I I involves one component, φ , corresponding to the generator of the U ˜ ( 1 ) subgroup of S O ( 10 ) , the charges of which are specified in Table 2. It is assumed that φ acquires a non-zero vacuum expectation value (VEV), φ 0 , and couples to Φ ^ i e and Φ ^ i e ¯ . This VEV, which is smaller than the scale M X , breaks the S U ( 4 ) × S U ( 2 ) W × S U ( 2 ) N × U ( 1 ) -gauge symmetry to S U ( 3 ) C × S U ( 2 ) W × S U ( 2 ) N × U ˜ ( 1 ) × U ( 1 ) , generating masses of the the zero modes u i c , u c ¯ i , h i and h ¯ i of supermultiplets Φ ^ i e and Φ ^ i e ¯ . In this case, only zero modes associated with the components e i c and e c ¯ i remain massless. The couplings of other 6 D supermultiplets to φ are expected to be forbidden. Because supermultiplet φ is confined on the brane O I I , the VEV φ 0 does not directly break the S U ( 6 ) × S U ( 2 ) N global symmetry of the strongly interacting sector which is localised on the brane O.
At the same time, the superfield e i c , which resides on brane O I I , can be combined with the corresponding zero modes of Φ ^ i u ¯ , giving rise to vector-like states with masses of order of M X . In the same way, e i c ¯ and the appropriate zero modes of Φ ^ i u can form vector-like states that gain masses set by the scale M X . As a result, only zero modes of the components of Φ ^ i u ¯ and Φ ^ i u with the quantum numbers of u c ¯ i , h ¯ i , u i c and h i remain massless.
The zero modes with the quantum numbers of q i , d i c , q ¯ and d c ¯ can originate from the bulk supermultiplets
Φ ^ i q = 27 , + , , , + , Φ ^ i q ¯ = 27 , , + , + , , Φ ^ i d = 27 , , + , , + , Φ ^ i d ¯ = 27 , + , , + , .
Using the parity assignments given in Table 1, it is easy to check that all parities of d i c , h i c , s i and ν i c components of Φ ^ i d , d i c ¯ , h i c ¯ , s i ¯ and ν i c ¯ components of Φ ^ i d ¯ , h i u and q i components of Φ ^ i q as well as h i u ¯ and q i ¯ and components of Φ ^ i q ¯ are positive. Therefore, the corresponding KK expansions include zero modes.
In order to obtain the zero modes associated with the i and ¯ components of the 27-plets and 27 ¯ -plet, the set of the 6 D supermultiplets has to be supplemented by
Φ ^ i = 27 , , , + , + , Φ ^ i ¯ = 27 , + , + , , .
Again, one can check that all parities of h i d and i components of Φ ^ i as well as h i d ¯ and i ¯ components of Φ ^ i ¯ are positive, resulting in the corresponding set of zero modes. The full set of the bulk supermultiplets, as well as their zero modes, which remain massless below φ = φ 0 , are given in Table 3. We assume here that the mass terms associated with the zero modes with opposite quantum numbers are forbidden.
Below the scale φ 0 , the 6 D supermultiplets result in the set of zero modes which involves 3 pairs of N = 1 chiral 27 and 27 ¯ -plets. The model under consideration implies that 2 27 ¯ -plets associated with i = 1 , 2 and 2 27 supermultiplets which are confined on the O I I I brane compose vector-like states with masses M 0 φ 0 . It is also expected that 2 pairs of 15 ¯ and 15 of S U ( 6 ) that reside on the brane O I acquire VEVs of the order of ϕ 0 M 0 . The VEVs of the ν c ¯ and ν c components of one pair of 15 and 15 ¯ break the S U ( 3 ) C × S U ( 2 ) W × S U ( 2 ) N × U ˜ ( 1 ) × U ( 1 ) -gauge group to S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y × U ( 1 ) N . Different phenomenological aspects of the SUSY extensions of the SM based on the S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y × U ( 1 ) N -gauge symmetry were explored in [224,225,226,227,228,229,230,231,232,233,234,235,236,237,238,239,240,241,242,243,244,245,246,247,248,249,250]. The VEVs of the s ¯ and s components of another pair of 15 and 15 ¯ break the S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y × U ( 1 ) N -gauge group to S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y . The VEVs of ν c ¯ , ν c , s ¯ and s also induce the set of the mass terms in the superpotential as follows:
δ W m a s s = M i j η h i h j c + M i j ζ h i u h j d + M i j ξ s i s j + M i j ν ν i c ν j c + M ¯ η h ¯ h c ¯ + M ¯ ζ h u ¯ h d ¯ + M ¯ ξ s ¯ 2 + M ¯ ν ν c ¯ 2 ,
where i , j = 1 , 2 , 3 and M i j η M i j ζ M i j ξ M i j ν M ¯ η M ¯ ζ M ¯ ξ M ¯ ν ϕ 0 . The pairs of 15 and 15 ¯ of S U ( 6 ) compose vector-like states with masses which are close to ϕ 0 . These states reside on the brane O I and do not interact directly with the supermultiplets which are localised on the brane O. Therefore, the S U ( 6 ) global symmetry of the strongly interacting sector may remain unbroken.
In the six-dimensional orbifold GUTs, there are two types of anomalies: bulk anomalies [251,252,253,254,255] and 4 D anomalies at orbifold fixed points [256,257,258]. Bulk anomalies are induced by box diagrams, the contributions of which are proportional to the trace of four generators. This trace includes a part which may be reduced to the product involving traces of two generators. It corresponds to the reducible anomaly that can be canceled by the Green–Schwarz mechanism [259]. Another nonfactorizable part is associated with the irreducible gauge anomaly. The E 6 orbifold GUT model in six dimensions does not have irreducible anomaly [254,255]. The 4 D anomalies at the fixed points reduces to the anomalies associated with the unbroken subgroup of the E 6 -gauge group in the vicinity of such points. These anomalies are determined by the sum of the contributions that come from the zero modes confined on the brane [251,252,253,260,261,262]. In the orbifold GUT under consideration, the corresponding brane anomalies are cancelled automatically.
Finally, near the scale M S , which is somewhat lower than ϕ 0 , SUSY gets broken. As a consequence, the scalar components of all superfields gain masses of the order of M S . At the scale of M S , the SM singlet superfield S develops a non-zero VEV. This superfield interacts only with the components of Φ ^ 3 u and Φ ^ 3 u ¯ . The interactions of the superfield S with the components of other bulk supermultiplets can be forbidden by the discrete Z 2 S symmetry, under which only Φ ^ 3 u ¯ and S are odd, whereas all other bulk 27-plets are even. The VEV of S gives rise to the masses of zero modes u 3 and u 3 ¯ . Thus, below scale M S , the weakly coupled elementary sector includes a set of the fermion states given by Equation (5). Since different fermion multiplets are the zero modes of different bulk supermultiplets, they are allowed to have different baryon and lepton numbers in this case.

4. Generation of Matter–Antimatter Asymmetry in the E 6 CHM

In this section, we restrict our consideration to the scenarios with f 10 TeV . The U ( 1 ) B symmetry can be explicitly broken in the strongly coupled sector in this case, since Z 2 L can be nearly exact, forbidding all operators which lead to the proton decay. When scale f is so high, all other operators that violate baryon number are sufficiently strongly suppressed. This suppression is caused by the small mixing between elementary fermions and their composite partners as well as by the large value of f. For instance, the effective operators in the SM, which give rise to the processes with Δ B = 2 and Δ L = 0 , are given by
L Δ B = 2 = 1 Λ 5 q i q j q k q m ( d n c d l c ) + u i c d j c d k c u m c d n c d l c ,
where i , j , k , m , n , l = 1 , 2 , 3 are the generation indices. The n n ¯ mixing mass δ m and n n ¯ oscillation time τ n n ¯ can be estimated as
δ m ϰ Λ Q C D 6 Λ 5 , τ n n ¯ 1 δ m .
In Equation (33), ϰ 1 and Λ Q C D 200 MeV . The n n ¯ oscillation time becomes close to the experimental limit 10 8 s . Refs. [263,264] for Λ f e w × 100 TeV . The operators (32) also induce the process of the annihilation of the two nucleons N N K K , resulting in rare nuclear decays. The searches for such decays set a lower bound on Λ of around 200–300 TeV. At the same time, in the E 6 CHM with f 10 TeV , the value of Λ f e w × 100 TeV .
Here we assume that the effective Lagrangian of the E 6 CHM possesses an approximate Z 2 B symmetry. This discrete symmetry is a subgroup of U ( 1 ) B , i.e.,
Z 2 B = ( 1 ) 3 B .
In Equation (34), B is the baryon number of the multiplet. The Z 2 B discrete symmetry forbids proton decay, but it does not suppress the baryon-number-violating operators (32) Thus, in this case, the Lagrangian of the strongly interacting sector of the E 6 CHM respects the approximate S U ( 6 ) × U ( 1 ) L × Z 2 B symmetry.
In the scenario under consideration, after the breakdown of the S U ( 6 ) global symmetry to its S U ( 5 ) subgroup, all composite states and exotic fermions, including the components of the S U ( 6 ) multiplets 6 ¯ 1 , 6 ¯ 2 , 15 as well as q ¯ , d c ¯ , ¯ and e c ¯ , gain masses which are several times larger than f. The only exceptions are the components of the 15-plet which are identified with t c . These components survive to the EW scale. As follows from Equation (12), all components of the 15 -plet and 6 ¯ 2 multiplet as well as q ¯ and e c ¯ are odd under the Z 2 B symmetry. The components of the 6 ¯ 1 multiplet, q ¯ and ¯ can be either odd or even under the Z 2 B symmetry. Hereafter, it is assumed that these fermions are Z 2 B -even.
The N 1 and N 2 components of 6 ¯ 1 and 6 ¯ 2 multiplets acquire Majorana masses through the interactions ( 6 ¯ 1 Ω ) ( Ω 6 ¯ 1 ) and ( 6 ¯ 2 Ω ) ( Ω 6 ¯ 2 ) , respectively. These operators are allowed by the approximate Z 2 B symmetry. Nevertheless, this symmetry suppresses the mixing between N 1 and N 2 . We further assume that N 1 is substantially lighter than other composite and exotic fermions and has a mass of order of f.
The pNGB states have masses which are considerably lower than f 10 TeV . Therefore these resonances are the lightest composite particles in the E 6 CHM spectrum. All pNGB states are even under the Z 2 B symmetry because the Higgs boson manifests itself in interactions with SM particles as a Z 2 B -even state. The Z 2 B and gauge symmetries permit the decays of the S U ( 3 ) C triplet of scalar fields T into up and down antiquarks. On the other hand, almost exact Z 2 L symmetry forbids the decays of T into either a neutrino and a down quark or a charged lepton and an up quark. The decay mode T t ¯ b ¯ should be the dominant one because the first and second generation quarks have quite small fractions of compositeness. For E f , all operators that violate baryon number are suppressed, and T manifests itself in the interactions with other particles as a diquark with B = 2 / 3 . At the LHC, the S U ( 3 ) C triplet can be pair produced, resulting in four heavy quarks in the final state, i.e., p p T T ¯ t t ¯ b b ¯ . A somewhat similar signature arises in the R-parity-violating SUSY models. It is associated with the lightest squark in these models. Nowadays, scenarios with the mass of the S U ( 3 ) C triplet T below 700 GeV are disfavored by the LHC constraints on the masses of such squarks [265].
Although at low energies E f the baryon number violating processes are suppressed within the E 6 CHM, a sizeable baryon number asymmetry may still be generated via the out-of-equilibrium decays of N 1 if N 1 has a mass which is substantially lower than the masses of all other composite and exotic fermions. This can happen if CP is violated and the mass of the S U ( 3 ) C triplet T ( m T ) is in the multi TeV range, provided m T m N 1 f and the decays N 1 T + d i and N 1 T + d ¯ i are allowed. The Lagrangian that describes the decays of N 1 and N 2 into down-type quarks and the pNGB state T is given by
L N = i = 1 3 g i 1 T d i c N 1 + g i 2 T d i c N 2 + h . c . .
When Z 2 B symmetry is exact, the coupling g i 1 vanishes. Therefore, one can expect that, in the case of the approximate Z 2 B symmetry, | g i 1 | | g i 2 | . Because the pNGB state T decays mostly into t ¯ b ¯ , the decays of the Majorana fermion N 1 lead to the final states with B = ± 1 . The baryon asymmetry generation via the neutral fermion decays into scalar diquark and quark was considered in [266,267,268,269,270,271,272,273,274,275,276,277,278,279,280,281].
The generation of the baryon asymmetry is determined by the flavour CP asymmetries ε 1 , k
ε 1 , k = Γ N 1 d k Γ N 1 d ¯ k m Γ N 1 d m + Γ N 1 d ¯ m ,
where k , m = 1 , 2 , 3 , whereas Γ N 1 d ¯ k and Γ N 1 d k are partial decay widths of N 1 d ¯ k + T and N 1 d k + T . There are three CP (decay) asymmetries that correspond to three quark flavours, i.e., d , s and b. At the tree level,
Γ N 1 d k = Γ N 1 d ¯ k = 3 | g k 1 | 2 32 π M 1 ,
and the decay asymmetries (36) vanish in this approximation. In Equation (37), M 1 is the mass of N 1 . The interference of the tree-level decay amplitudes of N 1 with the one-loop corrections to them yields the non-zero values of the CP asymmetries (36) if CP invariance is violated. The corresponding tree-level and one-loop diagrams can be found in [250]. Assuming that m T m N 1 , and using the results obtained in the case of thermal leptogenesis [48,282,283,284,285,286], the direct calculation of all these diagrams gives
ε 1 , i = 1 ( 8 π ) 1 ( m = 1 3 | g m 1 | 2 ) [ n = 1 3 Im ( g i 1 g i 2 g n 1 g n 2 ) x ( 3 2 ( 1 x ) + 1 ( 1 + x ) ln 1 + x x ) + n = 1 3 Im ( g i 1 g i 2 g n 1 g n 2 ) 3 2 ( 1 x ) ] ,
where M 2 is the mass of N 2 and x = ( M 2 / M 1 ) 2 .
To compute the baryon asymmetries generated by the decays of N 1 , one needs to solve the system of Boltzmann equations that determine the evolution of baryon number densities. Since the corresponding solution has to be similar to the solutions in the case of thermal leptogenesis, the induced baryon asymmetry relative to the entropy density Y Δ B can be approximately estimated as (see [286])
Y Δ B 10 3 k = 1 3 ε 1 , k η k , Y Δ B = n B n B ¯ s | 0 = ( 8.75 ± 0.23 ) × 10 11 .
where η k are efficiency factors that vary from 0 to 1, and s is the entropy density. In the limit, when washout processes can be neglected, η k = 1 . Here we ignore sphaleron processes that partially convert baryon asymmetry into lepton asymmetry.
It is expected that | g 32 | | g 22 | , | g 12 | and | g 31 | | g 21 | , | g 11 | because s- and d-quarks are almost elementary fermions which couple very weakly to the operators of the strongly interacting sector. Such hierarchical structure of the Yukawa couplings ensures that ε 1 , 2 and ε 1 , 1 are negligibly small. To simplify our analysis, we set M 2 = 10 · M 1 . In the limit x 1 for ε 1 , 3 , one finds
ε 1 , 3 1 ( 4 π ) | g 32 | 2 x sin 2 Δ φ , Δ φ = φ 32 φ 31 ,
where the phases φ 32 and φ 31 are defined as g 32 = | g 32 | e i φ 32 and g 31 = | g 31 | e i φ 31 . When CP invariance is preserved, i.e., all Yukawa couplings are real, the decay asymmetry (40) goes to zero. The maximum absolute value of ε 1 , 3 is attained for Δ φ = ± π / 4 .
The efficiency factor η 3 can be of the order of unity in the E 6 CHM. Indeed, in the strong washout scenario η 3 may be estimated as follows (see, for example [286])
η 3 H ( T = M 1 ) / Γ 3 , Γ 3 = Γ N 1 d 3 + Γ N 1 d ¯ 3 = 3 | g 31 | 2 16 π M 1 , H = 1.66 g 1 / 2 T 2 M P l ,
where g = n b + 7 8 n f is the number of relativistic degrees of freedom in the thermal bath and H is the Hubble expansion rate. In the SM, g = 106.75 , while in the E 6 CHM, g = 113.75 for T f . From Equation (41), one can see that the efficiency factor η 3 increases with diminishing of | g 31 | , and for sufficiently small values of | g 31 | , it may become close to unity. For instance, in the case when M 1 10 TeV and | g 31 | 10 6 , this factor is around 0.25 .
When η 3 1 , the generated baryon asymmetry is defined by the CP asymmetry ε 1 , 3 which does not depend on | g 31 | . From Equation (40), it follows that for a given ratio M 2 / M 1 and negligibly small absolute values of the Yukawa couplings | g 11 | , | g 21 | , | g 12 | and | g 22 | , the decay asymmetry ε 1 , 3 is set by the combination of phases Δ φ and | g 32 | . Because g 32 is not suppressed by the Z 2 B discrete symmetry, it is expected that | g 32 | 0.1 . In Figure 1, the dependence of | ε 1 , 3 | on Δ φ is shown for two different values of | g 32 | , i.e., | g 32 | = 1 and | g 32 | = 0.1 . Figure 1 illustrates that | ε 1 , 3 | increases when | g 32 | grows and attains its maximal possible value for Δ φ π / 4 . Near its maximum, the value of | ε 1 , 3 | is so large that a phenomenologically acceptable baryon density is induced only for η 3 10 3 . If | g 32 | 0.1 and η 3 1 , then the appropriate matter–antimatter asymmetry, corresponding to ε 1 , 3 10 7 10 6 , can be obtained only in the limit when Δ φ 0.01 . This demonstrates that, in the E 6 CHM, the observed baryon density can be induced even if CP is approximately preserved. For Δ φ 1 and ( M 2 / M 1 ) = 10 , phenomenologically acceptable matter–antimatter asymmetry can be also generated when | g 32 | varies from 0.01 to 0.1 .

5. Conclusions

The breakdown of gauge symmetry within GUTs can lead, at low energies, to the E 6 -inspired composite Higgs model (E 6 CHM), which almost allows the mass hierarchy to be stabilized. In particular, the E 6 CHM can originate from the SUSY GUT based on the E 6 × G 0 -gauge symmetry. In the vicinity of some high energy scale M X , the E 6 × G 0 group can be broken down to the S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y × G subgroup, where G and G 0 are associated with the strongly interacting sector. We consider a six-dimensional orbifold SUSY GUT in which all fields of the strongly coupled sector reside on the brane where E 6 is broken down to S U ( 6 ) . It is expected that, in the E 6 CHM S U ( 6 ) , there still remains an approximate symmetry of the strongly interacting sector even at low energies, and this gets spontaneously broken around the scale f 5 TeV to S U ( 5 ) , which contains the S U ( 3 ) C × S U ( 2 ) W × U ( 1 ) Y -gauge group as a subgroup. The E 6 orbifold GUTs in six dimensions do not have irreducible bulk anomaly. In the orbifold SUSY GUT under consideration, brane anomalies are cancelled. Within this E 6 model, different multiplets of the elementary quarks and leptons stem from different bulk 27-plets. All other components of these 27-plets gain huge masses which are somewhat close to M X . As a consequence, the low energy Lagrangian of the E 6 CHM can be invariant with respect to the global U ( 1 ) L and U ( 1 ) B symmetries, which guarantee the conservation of the lepton and baryon charges to a very good approximation. To ensure that the left-handed neutrinos acquire non-zero Majorana masses, the U ( 1 ) L symmetry should be broken down to its Z 2 L discrete subgroup, which forbids all operators giving rise to rapid proton decay.
The S U ( 6 ) symmetry breaking to S U ( 5 ) in the E 6 CHM results in eleven pNGB states. Four of these states form the SM-like Higgs doublet H. One of these pNGBs is a SM singlet boson A. Six others are associated with the S U ( 3 ) C triplet of scalar field T. The pNGB states mentioned above do not carry any lepton and/or baryon numbers. A significant fine-tuning, ∼0.01%, is required to obtain a Higgs boson with mass around 125 GeV in this model because v f .
The masses of the SM fermions in the E 6 CHM are induced through the mixing between elementary states and their composite partners. There are two different scenarios of quark mass generation. In scenario A, the composite partners of the right-handed down-type quarks, left-handed quarks and right-handed up-type quarks are components of 15 ¯ , 20 and 15 representations of S U ( 6 ) . Scenario B implies that the composite partners of the right-handed down-type quarks, left-handed quarks and right-handed up-type quarks belong to 6 ¯ , 15 and 20 representations of the S U ( 6 ) group. In the case of the lepton sector, the corresponding masses can be generated if the composite partners of the right-handed charged leptons and left-handed leptons are components of the 15 and 6 ¯ representations of S U ( 6 ) .
The embedding of the E 6 CHM into an orbifold GUT with the E 6 -gauge group implies that, at some high energy scale, the SM-gauge couplings are approximately equal. This can be achieved when the dynamics of the strongly coupled sector lead to the composite right-handed top quark t c . In addition to the SM fields (without t c ), the weakly coupled sector in this case must involve a set of exotic fermions that also permits anomalies to be canceled. In particular, this set of exotic particles contains two SM singlet Majorana fermions N 2 and N 1 . In general, all exotic fermions and all composite resonances except the pNGB states gain masses which are a few times larger than f. The pNGB states have masses which tend to be considerably lower than f. Therefore, they are the lightest composite resonances in the E 6 CHM spectrum. In our analysis, N 1 is assumed to be the lightest exotic fermion; it has a mass around 10 TeV . The discrete Z 2 B symmetry, which is a subgroup of U ( 1 ) B , forbids all couplings that allow N 1 to decay. When Z 2 B is an approximate symmetry, N 1 can be a long-lived composite state.
When the S U ( 6 ) symmetry-breaking scale f 10 TeV and Z 2 L symmetry are almost exact, all operators that violate baryon number are sufficiently strongly suppressed even if U ( 1 ) B is explicitly broken. In this variant of the E 6 CHM, the out-of-equilibrium decays N 1 T + b and N 1 T + b ¯ can induce the observed baryon asymmetry if CP is violated. This scenario implies that the lifetime of N 1 is less than 10 15 s . Phenomenologically acceptable matter–antimatter asymmetry can be obtained, even in the limit when all CP-violating phases are small (≲0.01). The electric dipole moments (EDMs) of atoms, neutrons and elementary states, which have not been observed in different experiments, are suppressed if CP invariance is approximately preserved. These EDMs, as well as baryon-number-violating processes, such as neutron-antineutron oscillations, are going to be searched for in the near future [263,264].
The lightest exotic fermion N 1 becomes absolutely stable if Z 2 L and Z 2 B are exact symmetries. In this limit, N 1 can account for all or some of the observed cold dark matter density if it has a mass M 1 which is much smaller than the scale f. In particular, when M 1 is close to half the mass of the SM singlet boson A, the annihilation cross section for N 1 N 1 SM   particles can be relatively large, resulting in the cold dark matter density which is smaller than its measured value.
For a large S U ( 6 ) symmetry-breaking scale, i.e., f 5–10 TeV , all exotic fermions and almost all composite resonances are too heavy to be observed at the LHC. Because the deviations of the couplings of the SM-like Higgs boson to the SM particles within the E 6 CHM are determined by v 2 / f 2 , the modifications of the appropriate Higgs branching fractions are negligibly small in this case. Therefore, it is going to be rather problematic to probe such small deviations at the LHC and future e + e collider. Too large a value of f also implies that the interactions of the top quark with the SM particles are very similar to the ones which are predicted by the SM. This makes the top quark with its significant admixture of composite components basically indistinguishable from the corresponding SM state. Nonetheless, the spectrum of the E 6 CHM must contain the S U ( 3 ) C triplet of scalar fields T ( T ) with an electric charge 1 / 3 ( + 1 / 3 ) and a mass which is significantly lower than f. This state predominantly decays into T t ¯ + b ¯ . If this S U ( 3 ) C triplet T has a mass in the few TeV range, then it can be pair produced at the LHC, resulting in some enhancement of the cross section of p p t t ¯ b b ¯ . The discovery of such a colour state will provide a smoking gun signal of the composite Higgs model under consideration.

Funding

This research received no external funding.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

Data sharing is not applicable to this article.

Acknowledgments

R.N. thanks A.W. Thomas for sharing his valuable ideas in connection with composite Higgs models. R.N. acknowledges fruitful discussions with E. Akhmedov, E. Boos, M. Dubinin, S. Duplij, D. Gorbunov, D. Kazakov, V. Novikov, V. Rubakov, M. Vasiliev, M. Vysotsky and E. Zhemchugov.

Conflicts of Interest

The author declares no conflict of interest.

References

  1. Georgi, H.; Glashow, S.L. Unity Of All Elementary Particle Forces. Phys. Rev. Lett. 1974, 32, 438. [Google Scholar] [CrossRef] [Green Version]
  2. Minkowski, P. μeγ at a Rate of One Out of 109 Muon Decays? Phys. Lett. B 1977, 67, 421. [Google Scholar] [CrossRef]
  3. Mohapatra, R.N.; Senjanovic, G. Neutrino Mass and Spontaneous Parity Nonconservation. Phys. Rev. Lett. 1980, 44, 912. [Google Scholar] [CrossRef] [Green Version]
  4. Witten, E. Dynamical Breaking of Supersymmetry. Nucl. Phys. B 1981, 188, 513. [Google Scholar] [CrossRef]
  5. Sakai, N. Naturalness in Supersymmetric GUTs. Z. Phys. C 1981, 11, 153. [Google Scholar] [CrossRef]
  6. Dimopoulos, S.; Georgi, H. Softly Broken Supersymmetry and SU(5). Nucl. Phys. B 1981, 193, 150. [Google Scholar] [CrossRef] [Green Version]
  7. Kaul, R.K.; Majumdar, P. Cancellation of Quadratically Divergent Mass Corrections in Globally Supersymmetric Spontaneously Broken Gauge Theories. Nucl. Phys. B 1982, 199, 36. [Google Scholar] [CrossRef]
  8. Gildener, E.; Weinberg, S. Symmetry Breaking and Scalar Bosons. Phys. Rev. D 1976, 13, 3333. [Google Scholar] [CrossRef]
  9. Gildener, E. Gauge Symmetry Hierarchies. Phys. Rev. D 1976, 14, 1667. [Google Scholar] [CrossRef]
  10. Chung, D.J.H.; Everett, L.L.; Kane, G.L.; King, S.F.; Lykken, J.; Wang, L.T. The soft supersymmetry-breaking Lagrangian: Theory and applications. Phys. Rept. 2005, 407, 1. [Google Scholar] [CrossRef] [Green Version]
  11. Ellis, J.R.; Kelley, S.; Nanopoulos, D.V. Probing the desert using gauge coupling unification. Phys. Lett. B 1991, 260, 131. [Google Scholar] [CrossRef] [Green Version]
  12. Langacker, P.; Luo, M.X. Implications of precision electroweak experiments for Mt, ρ0, sin2θW and grand unification. Phys. Rev. D 1991, 44, 817. [Google Scholar] [CrossRef] [PubMed]
  13. Amaldi, U.; de Boer, W.; Furstenau, H. Comparison of grand unified theories with electroweak and strong coupling constants measured at LEP. Phys. Lett. B 1991, 260, 447. [Google Scholar] [CrossRef] [Green Version]
  14. Anselmo, F.; Cifarelli, L.; Peterman, A.; Zichichi, A. The Effective experimental constraints on M(susy) and M(gut). Nuovo Cim. A 1991, 104, 1817. [Google Scholar] [CrossRef] [Green Version]
  15. Arkani-Hamed, N.; Dimopoulos, S.; Dvali, G.R. The Hierarchy problem and new dimensions at a millimeter. Phys. Lett. B 1998, 429, 263. [Google Scholar] [CrossRef] [Green Version]
  16. Antoniadis, I.; Arkani-Hamed, N.; Dimopoulos, S.; Dvali, G.R. New dimensions at a millimeter to a Fermi and superstrings at a TeV. Phys. Lett. B 1998, 436, 257. [Google Scholar] [CrossRef] [Green Version]
  17. Randall, L.; Sundrum, R. A Large mass hierarchy from a small extra dimension. Phys. Rev. Lett. 1999, 83, 3370. [Google Scholar] [CrossRef] [Green Version]
  18. Randall, L.; Sundrum, R. An Alternative to compactification. Phys. Rev. Lett. 1999, 83, 4690. [Google Scholar] [CrossRef] [Green Version]
  19. Dienes, K.R.; Dudas, E.; Gherghetta, T. Extra space-time dimensions and unification. Phys. Lett. B 1998, 436, 55. [Google Scholar] [CrossRef] [Green Version]
  20. Dienes, K.R.; Dudas, E.; Gherghetta, T. Grand unification at intermediate mass scales through extra dimensions. Nucl. Phys. B 1999, 537, 47. [Google Scholar] [CrossRef] [Green Version]
  21. Bellazzini, B.; Csáki, C.; Serra, J. Composite Higgses. Eur. Phys. J. C 2014, 74, 2766. [Google Scholar] [CrossRef] [Green Version]
  22. Terazawa, H.; Akama, K.; Chikashige, Y. Unified Model of the Nambu-Jona-Lasinio Type for All Elementary Particle Forces. Phys. Rev. D 1977, 15, 480. [Google Scholar] [CrossRef]
  23. Terazawa, H. Subquark Model of Leptons and Quarks. Phys. Rev. D 1980, 22, 184. [Google Scholar] [CrossRef]
  24. Dimopoulos, S.; Preskill, J. Massless Composites With Massive Constituents. Nucl. Phys. B 1982, 199, 206. [Google Scholar] [CrossRef] [Green Version]
  25. Kaplan, D.B.; Georgi, H. SU(2) × U(1) Breaking by Vacuum Misalignment. Phys. Lett. B 1984, 136, 183. [Google Scholar] [CrossRef]
  26. Kaplan, D.B.; Georgi, H.; Dimopoulos, S. Composite Higgs Scalars. Phys. Lett. B 1984, 136, 187. [Google Scholar] [CrossRef]
  27. Georgi, H.; Kaplan, D.B.; Galison, P. Calculation of the Composite Higgs Mass. Phys. Lett. B 1984, 143, 152. [Google Scholar] [CrossRef]
  28. Banks, T. Constraints on SU(2) × U(1) Breaking by Vacuum Misalignment. Nucl. Phys. B 1984, 243, 125. [Google Scholar] [CrossRef]
  29. Georgi, H.; Kaplan, D.B. Composite Higgs and Custodial SU(2). Phys. Lett. B 1984, 145, 216. [Google Scholar] [CrossRef]
  30. Dugan, M.J.; Georgi, H.; Kaplan, D.B. Anatomy of a Composite Higgs Model. Nucl. Phys. B 1985, 254, 299. [Google Scholar] [CrossRef]
  31. Georgi, H. A Tool Kit for Builders of Composite Models. Nucl. Phys. B 1986, 266, 274. [Google Scholar] [CrossRef]
  32. Nevzorov, R.; Thomas, A.W. E6 inspired composite Higgs model. Phys. Rev. D 2015, 92, 075007. [Google Scholar] [CrossRef] [Green Version]
  33. Nevzorov, R.; Thomas, A.W. LHC signatures of neutral pseudo-Goldstone boson in the E6CHM. J. Phys. G 2017, 44, 075003. [Google Scholar] [CrossRef] [Green Version]
  34. Nevzorov, R.; Thomas, A.W. E6 inspired composite Higgs model and 750 GeV diphoton excess. EPJ Web Conf. 2016, 125, 02021. [Google Scholar] [CrossRef]
  35. Nevzorov, R.; Thomas, A.W. Baryon asymmetry generation in the E6CHM. Phys. Lett. B 2017, 774, 123. [Google Scholar] [CrossRef]
  36. Nevzorov, R.; Thomas, A.W. Generation of baryon asymmetry in the E6CHM. EPJ Web Conf. 2018, 191, 02004. [Google Scholar] [CrossRef] [Green Version]
  37. Nevzorov, R.; Thomas, A.W. E6 Inspired Composite Higgs Model and Baryon Asymmetry Generation. Phys. Part. Nucl. 2020, 51, 709. [Google Scholar] [CrossRef]
  38. Khlopov, M.Y.; Shibaev, K.I. New physics from superstring phenomenology. Grav. Cosmol. Suppl. 2002, 8, 45. [Google Scholar]
  39. Khlopov, M.Y. What comes after the Standard model? Prog. Part. Nucl. Phys. 2021, 116, 103824. [Google Scholar] [CrossRef]
  40. Sakharov, A.D. Violation of CP invariance, C asymmetry, and baryon asymmetry of the universe. JETP Lett. 1967, 5, 24. [Google Scholar]
  41. Ignatiev, A.Y.; Krasnikov, N.V.; Kuzmin, V.A.; Tavkhelidze, A.N. Universal CP Noninvariant Superweak Interaction and Baryon Asymmetry of the Universe. Phys. Lett. B 1978, 76, 436. [Google Scholar] [CrossRef]
  42. Yoshimura, M. Unified Gauge Theories and the Baryon Number of the Universe. Phys. Rev. Lett. 1978, 41, 281. [Google Scholar] [CrossRef]
  43. Toussaint, D.; Treiman, S.B.; Wilczek, F.; Zee, A. Matter - Antimatter Accounting, Thermodynamics, and Black Hole Radiation. Phys. Rev. D 1979, 19, 1036. [Google Scholar] [CrossRef]
  44. Weinberg, S. Cosmological production of baryons. Phys. Rev. Lett. 1979, 42, 850. [Google Scholar] [CrossRef]
  45. Yoshimura, M. Origin of Cosmological Baryon Asymmetry. Phys. Lett. B 1979, 88, 294. [Google Scholar] [CrossRef]
  46. Barr, S.M.; Segre, G.; Weldon, H.A. The Magnitude of the Cosmological Baryon Asymmetry. Phys. Rev. D 1979, 20, 2494. [Google Scholar] [CrossRef]
  47. Nanopoulos, D.V.; Weinberg, S. Mechanisms for Cosmological Baryon Production. Phys. Rev. D 1979, 20, 2484. [Google Scholar] [CrossRef]
  48. Fukugita, M.; Yanagida, T. Baryogenesis Without Grand Unification. Phys. Lett. B 1986, 174, 45. [Google Scholar] [CrossRef]
  49. Affleck, I.; Dine, M. A New Mechanism for Baryogenesis. Nucl. Phys. B 1985, 249, 361. [Google Scholar] [CrossRef]
  50. Dine, M.; Randall, L.; Thomas, S.D. Baryogenesis from flat directions of the supersymmetric standard model. Nucl. Phys. B 1996, 458, 291. [Google Scholar] [CrossRef] [Green Version]
  51. Riotto, A.; Trodden, M. Recent progress in baryogenesis. Ann. Rev. Nucl. Part. Sci. 1999, 49, 35. [Google Scholar] [CrossRef] [Green Version]
  52. Agashe, K.; Contino, R.; Pomarol, A. The Minimal composite Higgs model. Nucl. Phys. B 2005, 719, 165. [Google Scholar] [CrossRef] [Green Version]
  53. Contino, R.; Nomura, Y.; Pomarol, A. Higgs as a holographic pseudoGoldstone boson. Nucl. Phys. B 2003, 671, 148. [Google Scholar] [CrossRef] [Green Version]
  54. Agashe, K.; Delgado, A.; May, M.J.; Sundrum, R. RS1, custodial isospin and precision tests. J. High Energy Phys. 2003, 308, 50. [Google Scholar] [CrossRef] [Green Version]
  55. Contino, R.; Kramer, T.; Son, M.; Sundrum, R. Warped/composite phenomenology simplified. J. High Energy Phys. 2007, 705, 74. [Google Scholar] [CrossRef] [Green Version]
  56. Kaplan, D.B. Flavor at SSC energies: A New mechanism for dynamically generated fermion masses. Nucl. Phys. B 1991, 365, 259. [Google Scholar] [CrossRef]
  57. Frigerio, M.; Serra, J.; Varagnolo, A. Composite GUTs: Models and expectations at the LHC. J. High Energy Phys. 2011, 1106, 29. [Google Scholar] [CrossRef] [Green Version]
  58. Agashe, K.; Contino, R. The Minimal composite Higgs model and electroweak precision tests. Nucl. Phys. B 2006, 742, 59. [Google Scholar] [CrossRef] [Green Version]
  59. Agashe, K.; Contino, R.; Da Rold, L.; Pomarol, A. A Custodial symmetry for Zb b ¯ . Phys. Lett. B 2006, 641, 62. [Google Scholar] [CrossRef] [Green Version]
  60. Giudice, G.F.; Grojean, C.; Pomarol, A.; Rattazzi, R. The Strongly-Interacting Light Higgs. J. High Energy Phys. 2007, 706, 45. [Google Scholar] [CrossRef] [Green Version]
  61. Barbieri, R.; Bellazzini, B.; Rychkov, V.S.; Varagnolo, A. The Higgs boson from an extended symmetry. Phys. Rev. D 2007, 76, 115008. [Google Scholar] [CrossRef] [Green Version]
  62. Lodone, P. Vector-like quarks in a ‘composite’ Higgs model. J. High Energy Phys. 2008, 0812, 029. [Google Scholar] [CrossRef]
  63. Gillioz, M. A Light composite Higgs boson facing electroweak precision tests. Phys. Rev. D 2009, 80, 055003. [Google Scholar] [CrossRef] [Green Version]
  64. Anastasiou, C.; Furlan, E.; Santiago, J. Realistic Composite Higgs Models. Phys. Rev. D 2009, 79, 075003. [Google Scholar] [CrossRef] [Green Version]
  65. Panico, G.; Wulzer, A. The Discrete Composite Higgs Model. J. High Energy Phys. 2011, 1109, 135. [Google Scholar] [CrossRef] [Green Version]
  66. De Curtis, S.; Redi, M.; Tesi, A. The 4D Composite Higgs. J. High Energy Phys. 2012, 1204, 42. [Google Scholar] [CrossRef] [Green Version]
  67. Marzocca, D.; Serone, M.; Shu, J. General Composite Higgs Models. J. High Energy Phys. 2012, 1208, 013. [Google Scholar] [CrossRef] [Green Version]
  68. Orgogozo, A.; Rychkov, S. The S parameter for a Light Composite Higgs: A Dispersion Relation Approach. J. High Energy Phys. 2013, 1306, 14. [Google Scholar] [CrossRef] [Green Version]
  69. Grojean, C.; Matsedonskyi, O.; Giuliano, P. Light top partners and precision physics. J. High Energy Phys. 2013, 1310, 160. [Google Scholar] [CrossRef] [Green Version]
  70. Carena, M.; Ponton, E.; Santiago, J.; Wagner, C.E.M. Light Kaluza Klein States in Randall-Sundrum Models with Custodial SU(2). Nucl. Phys. B 2006, 759, 202. [Google Scholar] [CrossRef] [Green Version]
  71. Pomarol, A.; Serra, J. Top Quark Compositeness: Feasibility and Implications. Phys. Rev. D 2008, 78, 074026. [Google Scholar] [CrossRef] [Green Version]
  72. Pappadopulo, D.; Thamm, A.; Torre, R. A minimally tuned composite Higgs model from an extra dimension. J. High Energy Phys. 2013, 1307, 58. [Google Scholar] [CrossRef] [Green Version]
  73. Bellazzini, B.; Csaki, C.; Hubisz, J.; Serra, J.; Terning, J. Composite Higgs Sketch. J. High Energy Phys. 2012, 1211, 3. [Google Scholar] [CrossRef] [Green Version]
  74. Gillioz, M.; Grober, R.; Grojean, C.; Muhlleitner, M.; Salvioni, E. Higgs Low-Energy Theorem (and its corrections) in Composite Models. J. High Energy Phys. 2012, 1210, 4. [Google Scholar] [CrossRef] [Green Version]
  75. Azatov, A.; Galloway, J. Electroweak Symmetry Breaking and the Higgs Boson: Confronting Theories at Colliders. Int. J. Mod. Phys. A 2013, 28, 1330004. [Google Scholar] [CrossRef] [Green Version]
  76. Falkowski, A.; Riva, F.; Urbano, A. Higgs at last. J. High Energy Phys. 2013, 1311, 111. [Google Scholar] [CrossRef] [Green Version]
  77. Azatov, A.; Contino, R.; Di Iura, A.; Galloway, J. New Prospects for Higgs Compositeness in hZγ. Phys. Rev. D 2013, 88, 075019. [Google Scholar] [CrossRef] [Green Version]
  78. Gillioz, M.; Gröber, R.; Kapuvari, A.; Mühlleitner, M. Vector-like Bottom Quarks in Composite Higgs Models. J. High Energy Phys. 2014, 1403, 37. [Google Scholar] [CrossRef] [Green Version]
  79. Barbieri, R.; Isidori, G.; Pappadopulo, D. Composite fermions in Electroweak Symmetry Breaking. J. High Energy Phys. 2009, 902, 29. [Google Scholar] [CrossRef] [Green Version]
  80. Matsedonskyi, O. On Flavour and Naturalness of Composite Higgs Models. J. High Energy Phys. 2015, 1502, 154. [Google Scholar] [CrossRef] [Green Version]
  81. Barbieri, R.; Buttazzo, D.; Sala, F.; Straub, D.M.; Tesi, A. A 125 GeV composite Higgs boson versus flavour and electroweak precision tests. J. High Energy Phys. 2013, 1305, 69. [Google Scholar] [CrossRef] [Green Version]
  82. Csaki, C.; Falkowski, A.; Weiler, A. The Flavor of the Composite Pseudo-Goldstone Higgs. J. High Energy Phys. 2008, 809, 8. [Google Scholar] [CrossRef] [Green Version]
  83. Agashe, K.; Azatov, A.; Zhu, L. Flavor Violation Tests of Warped/Composite SM in the Two-Site Approach. Phys. Rev. D 2009, 79, 056006. [Google Scholar] [CrossRef] [Green Version]
  84. Vignaroli, N. Δ F=1 constraints on composite Higgs models with LR parity. Phys. Rev. D 2012, 86, 115011. [Google Scholar] [CrossRef] [Green Version]
  85. Sikivie, P.; Susskind, L.; Voloshin, M.B.; Zakharov, V.I. Isospin Breaking in Technicolor Models. Nucl. Phys. B 1980, 173, 189. [Google Scholar] [CrossRef]
  86. Peskin, M.E.; Takeuchi, T. Estimation of oblique electroweak corrections. Phys. Rev. D 1992, 46, 381. [Google Scholar] [CrossRef] [Green Version]
  87. Agashe, K.; Perez, G.; Soni, A. Flavor structure of warped extra dimension models. Phys. Rev. D 2005, 71, 016002. [Google Scholar] [CrossRef] [Green Version]
  88. Glashow, S.L.; Iliopoulos, J.; Maiani, L. Weak Interactions with Lepton-Hadron Symmetry. Phys. Rev. D 1970, 2, 1285. [Google Scholar] [CrossRef]
  89. Redi, M.; Weiler, A. Flavor and CP Invariant Composite Higgs Models. J. High Energy Phys. 2011, 1111, 108. [Google Scholar] [CrossRef] [Green Version]
  90. Blanke, M.; Buras, A.J.; Duling, B.; Gori, S.; Weiler, A. Δ F = 2 Observables and Fine-Tuning in a Warped Extra Dimension with Custodial Protection. J. High Energy Phys. 2009, 903, 1. [Google Scholar] [CrossRef] [Green Version]
  91. Gedalia, O.; Isidori, G.; Perez, G. Combining Direct & Indirect Kaon CP Violation to Constrain the Warped KK Scale. Phys. Lett. B 2009, 682, 200. [Google Scholar]
  92. Barbieri, R.; Buttazzo, D.; Sala, F.; Straub, D.M. Flavour physics from an approximate U(2)3 symmetry. J. High Energy Phys. 2012, 1207, 181. [Google Scholar] [CrossRef] [Green Version]
  93. Redi, M. Leptons in Composite MFV. J. High Energy Phys. 2013, 1309, 60. [Google Scholar] [CrossRef] [Green Version]
  94. Agashe, K.; Blechman, A.E.; Petriello, F. Probing the Randall-Sundrum geometric origin of flavor with lepton flavor violation. Phys. Rev. D 2006, 74, 053011. [Google Scholar] [CrossRef] [Green Version]
  95. Csaki, C.; Grossman, Y.; Tanedo, P.; Tsai, Y. Warped penguin diagrams. Phys. Rev. D 2011, 83, 073002. [Google Scholar] [CrossRef] [Green Version]
  96. Csaki, C.; Delaunay, C.; Grojean, C.; Grossman, Y. A Model of Lepton Masses from a Warped Extra Dimension. J. High Energy Phys. 2008, 0810, 055. [Google Scholar] [CrossRef] [Green Version]
  97. del Aguila, F.; Carmona, A.; Santiago, J. Neutrino Masses from an A4 Symmetry in Holographic Composite Higgs Models. J. High Energy Phys. 2010, 1008, 127. [Google Scholar] [CrossRef] [Green Version]
  98. Cacciapaglia, G.; Csaki, C.; Galloway, J.; Marandella, G.; Terning, J.; Weiler, A. A GIM Mechanism from Extra Dimensions. J. High Energy Phys. 2008, 804, 6. [Google Scholar] [CrossRef] [Green Version]
  99. Redi, M. Composite MFV and Beyond. Eur. Phys. J. C 2012, 72, 2030. [Google Scholar] [CrossRef] [Green Version]
  100. König, M.; Neubert, M.; Straub, D.M. Dipole operator constraints on composite Higgs models. Eur. Phys. J. C 2014, 74, 2945. [Google Scholar] [CrossRef] [Green Version]
  101. Gripaios, B.; Pomarol, A.; Riva, F.; Serra, J. Beyond the Minimal Composite Higgs Model. J. High Energy Phys. 2009, 904, 70. [Google Scholar] [CrossRef] [Green Version]
  102. Mrazek, J.; Pomarol, A.; Rattazzi, R.; Redi, M.; Serra, J.; Wulzer, A. The Other Natural Two Higgs Doublet Model. Nucl. Phys. B 2011, 853, 1. [Google Scholar] [CrossRef] [Green Version]
  103. Redi, M.; Tesi, A. Implications of a Light Higgs in Composite Models. J. High Energy Phys. 2012, 1210, 166. [Google Scholar] [CrossRef] [Green Version]
  104. Bertuzzo, E.; Ray, T.S.; de Sandes, H.; Savoy, C.A. On Composite Two Higgs Doublet Models. J. High Energy Phys. 2013, 1305, 153. [Google Scholar] [CrossRef] [Green Version]
  105. Montull, M.; Riva, F. Higgs discovery: The beginning or the end of natural EWSB? J. High Energy Phys. 2012, 1211, 18. [Google Scholar] [CrossRef] [Green Version]
  106. Chala, M. hγγ excess and Dark Matter from Composite Higgs Models. J. High Energy Phys. 2013, 1301, 122. [Google Scholar] [CrossRef] [Green Version]
  107. Frigerio, M.; Pomarol, A.; Riva, F.; Urbano, A. Composite Scalar Dark Matter. J. High Energy Phys. 2012, 1207, 15. [Google Scholar] [CrossRef] [Green Version]
  108. Contino, R.; Grojean, C.; Moretti, M.; Piccinini, F.; Rattazzi, R. Strong Double Higgs Production at the LHC. J. High Energy Phys. 2010, 1005, 89. [Google Scholar] [CrossRef] [Green Version]
  109. Low, I.; Vichi, A. On the production of a composite Higgs boson. Phys. Rev. D 2011, 84, 045019. [Google Scholar] [CrossRef] [Green Version]
  110. Contino, R.; Marzocca, D.; Pappadopulo, D.; Rattazzi, R. On the effect of resonances in composite Higgs phenomenology. J. High Energy Phys. 2011, 1110, 81. [Google Scholar] [CrossRef] [Green Version]
  111. Azatov, A.; Galloway, J. Light Custodians and Higgs Physics in Composite Models. Phys. Rev. D 2012, 85, 055013. [Google Scholar] [CrossRef] [Green Version]
  112. Contino, R.; Ghezzi, M.; Moretti, M.; Panico, G.; Piccinini, F.; Wulzer, A. Anomalous Couplings in Double Higgs Production. J. High Energy Phys. 2012, 1208, 154. [Google Scholar] [CrossRef] [Green Version]
  113. Contino, R.; Ghezzi, M.; Grojean, C.; Muhlleitner, M.; Spira, M. Effective Lagrangian for a light Higgs-like scalar. J. High Energy Phys. 2013, 1307, 35. [Google Scholar] [CrossRef] [Green Version]
  114. Delaunay, C.; Grojean, C.; Perez, G. Modified Higgs Physics from Composite Light Flavors. J. High Energy Phys. 2013, 1309, 90. [Google Scholar] [CrossRef] [Green Version]
  115. Banfi, A.; Martin, A.; Sanz, V. Probing top-partners in Higgs+jets. J. High Energy Phys. 2014, 1408, 53. [Google Scholar] [CrossRef] [Green Version]
  116. Montull, M.; Riva, F.; Salvioni, E.; Torre, R. Higgs Couplings in Composite Models. Phys. Rev. D 2013, 88, 095006. [Google Scholar] [CrossRef] [Green Version]
  117. Contino, R.; Grojean, C.; Pappadopulo, D.; Rattazzi, R.; Thamm, A. Strong Higgs Interactions at a Linear Collider. J. High Energy Phys. 2014, 1402, 6. [Google Scholar] [CrossRef] [Green Version]
  118. Flacke, T.; Kim, J.H.; Lee, S.J.; Lim, S.H. Constraints on composite quark partners from Higgs searches. J. High Energy Phys. 2014, 1405, 123. [Google Scholar] [CrossRef] [Green Version]
  119. Grojean, C.; Salvioni, E.; Schlaffer, M.; Weiler, A. Very boosted Higgs in gluon fusion. J. High Energy Phys. 2014, 1405, 22. [Google Scholar] [CrossRef] [Green Version]
  120. Carena, M.; Da Rold, L.; Pontón, E. Minimal Composite Higgs Models at the LHC. J. High Energy Phys. 2014, 1406, 159. [Google Scholar] [CrossRef] [Green Version]
  121. Carmona, A.; Goertz, F. A naturally light Higgs without light Top Partners. J. High Energy Phys. 2015, 1505, 2. [Google Scholar] [CrossRef] [Green Version]
  122. Buchalla, G.; Cata, O.; Krause, C. A Systematic Approach to the SILH Lagrangian. Nucl. Phys. B 2015, 894, 602. [Google Scholar] [CrossRef] [Green Version]
  123. Pomarol, A.; Riva, F. The Composite Higgs and Light Resonance Connection. J. High Energy Phys. 2012, 1208, 135. [Google Scholar] [CrossRef] [Green Version]
  124. Matsedonskyi, O.; Panico, G.; Wulzer, A. Light Top Partners for a Light Composite Higgs. J. High Energy Phys. 2013, 1301, 164. [Google Scholar] [CrossRef] [Green Version]
  125. Agashe, K.; Delgado, A.; Sundrum, R. Grand unification in RS1. Ann. Phys. 2003, 304, 145. [Google Scholar] [CrossRef] [Green Version]
  126. Gherghetta, T. Partly supersymmetric grand unification. Phys. Rev. D 2005, 71, 065001. [Google Scholar] [CrossRef] [Green Version]
  127. Barnard, J.; Gherghetta, T.; Ray, T.S.; Spray, A. The Unnatural Composite Higgs. J. High Energy Phys. 2015, 1501, 67. [Google Scholar] [CrossRef] [Green Version]
  128. Asano, M.; Kitano, R. Partially Composite Dark Matter. J. High Energy Phys. 2014, 1409, 171. [Google Scholar] [CrossRef] [Green Version]
  129. Agashe, K.; Belyaev, A.; Krupovnickas, T.; Perez, G.; Virzi, J. LHC Signals from Warped Extra Dimensions. Phys. Rev. D 2008, 77, 015003. [Google Scholar] [CrossRef] [Green Version]
  130. Lillie, B.; Randall, L.; Wang, L.T. The Bulk RS KK-gluon at the LHC. J. High Energy Phys. 2007, 0709, 074. [Google Scholar] [CrossRef] [Green Version]
  131. Agashe, K.; Davoudiasl, H.; Gopalakrishna, S.; Han, T.; Huang, G.Y.; Perez, G.; Si, Z.G.; Soni, A. LHC Signals for Warped Electroweak Neutral Gauge Bosons. Phys. Rev. D 2007, 76, 115015. [Google Scholar] [CrossRef] [Green Version]
  132. Carena, M.; Medina, A.D.; Panes, B.; Shah, N.R.; Wagner, C.E.M. Collider phenomenology of gauge-Higgs unification scenarios in warped extra dimensions. Phys. Rev. D 2008, 77, 076003. [Google Scholar] [CrossRef] [Green Version]
  133. Contino, R.; Servant, G. Discovering the top partners at the LHC using same-sign dilepton final states. J. High Energy Phys. 2008, 0806, 026. [Google Scholar] [CrossRef] [Green Version]
  134. Agashe, K.; Gopalakrishna, S.; Han, T.; Huang, G.Y.; Soni, A. LHC Signals for Warped Electroweak Charged Gauge Bosons. Phys. Rev. D 2009, 80, 075007. [Google Scholar] [CrossRef] [Green Version]
  135. Aguilar-Saavedra, J.A. Identifying top partners at LHC. J. High Energy Phys. 2009, 0911, 030. [Google Scholar] [CrossRef] [Green Version]
  136. Mrazek, J.; Wulzer, A. A Strong Sector at the LHC: Top Partners in Same-Sign Dileptons. Phys. Rev. D 2010, 81, 075006. [Google Scholar] [CrossRef] [Green Version]
  137. Agashe, K.; Azatov, A.; Han, T.; Li, Y.; Si, Z.G.; Zhu, L. LHC Signals for Coset Electroweak Gauge Bosons in Warped/Composite PGB Higgs Models. Phys. Rev. D 2010, 81, 096002. [Google Scholar] [CrossRef] [Green Version]
  138. Dissertori, G.; Furlan, E.; Moortgat, F.; Nef, P. Discovery potential of top-partners in a realistic composite Higgs model with early LHC data. J. High Energy Phys. 2010, 1009, 19. [Google Scholar] [CrossRef] [Green Version]
  139. Vignaroli, N. Early discovery of top partners and test of the Higgs nature. Phys. Rev. D 2012, 86, 075017. [Google Scholar] [CrossRef] [Green Version]
  140. Cacciapaglia, G.; Deandrea, A.; Panizzi, L.; Perries, S.; Sordini, V. Heavy Vector-like quark with charge 5/3 at the LHC. J. High Energy Phys. 2013, 1303, 4. [Google Scholar] [CrossRef] [Green Version]
  141. De Simone, A.; Matsedonskyi, O.; Rattazzi, R.; Wulzer, A. A First Top Partner Hunter’s Guide. J. High Energy Phys. 2013, 1304, 4. [Google Scholar] [CrossRef] [Green Version]
  142. Li, J.; Liu, D.; Shu, J. Towards the fate of natural composite Higgs model through single t search at the 8 TeV LHC. J. High Energy Phys. 2013, 1311, 47. [Google Scholar] [CrossRef] [Green Version]
  143. Redi, M.; Sanz, V.; de Vries, M.; Weiler, A. Strong Signatures of Right-Handed Compositeness. J. High Energy Phys. 2013, 1308, 8. [Google Scholar] [CrossRef] [Green Version]
  144. Delaunay, C.; Flacke, T.; Gonzalez-Fraile, J.; Lee, S.J.; Panico, G.; Perez, G. Light Non-degenerate Composite Partners at the LHC. J. High Energy Phys. 2014, 1402, 55. [Google Scholar] [CrossRef] [Green Version]
  145. Matsedonskyi, O.; Riva, F.; Vantalon, T. Composite Charge 8/3 Resonances at the LHC. J. High Energy Phys. 2014, 1404, 59. [Google Scholar] [CrossRef] [Green Version]
  146. Cheng, H.C.; Gu, J. Top seesaw with a custodial symmetry, and the 126 GeV Higgs. J. High Energy Phys. 2014, 1410, 2. [Google Scholar] [CrossRef] [Green Version]
  147. Gripaios, B.; Müller, T.; Parker, M.A.; Sutherland, D. Search Strategies for Top Partners in Composite Higgs models. J. High Energy Phys. 2014, 1408, 171. [Google Scholar] [CrossRef] [Green Version]
  148. Azatov, A.; Panico, G.; Perez, G.; Soreq, Y. On the Flavor Structure of Natural Composite Higgs Models & Top Flavor Violation. J. High Energy Phys. 2014, 1412, 82. [Google Scholar]
  149. Backović, M.; Flacke, T.; Kim, J.H.; Lee, S.J. Boosted Event Topologies from TeV Scale Light Quark Composite Partners. J. High Energy Phys. 2015, 1504, 82. [Google Scholar] [CrossRef] [Green Version]
  150. Kanemura, S.; Kaneta, K.; Machida, N.; Shindou, T. New resonance scale and fingerprint identification in minimal composite Higgs models. Phys. Rev. D 2015, 91, 115016. [Google Scholar] [CrossRef] [Green Version]
  151. Thamm, A.; Torre, R.; Wulzer, A. Future tests of Higgs compositeness: Direct vs indirect. J. High Energy Phys. 2015, 1507, 100. [Google Scholar] [CrossRef] [Green Version]
  152. Azatov, A.; Chowdhury, D.; Ghosh, D.; Ray, T.S. Same sign di-lepton candles of the composite gluons. J. High Energy Phys. 2015, 1508, 140. [Google Scholar] [CrossRef] [Green Version]
  153. Serra, J. Beyond the Minimal Top Partner Decay. J. High Energy Phys. 2015, 1509, 176. [Google Scholar] [CrossRef] [Green Version]
  154. Barnard, J.; Gherghetta, T.; Ray, T.S. UV descriptions of composite Higgs models without elementary scalars. J. High Energy Phys. 2014, 1402, 2, [arXiv:1311.6562 [hep-ph]]. [Google Scholar] [CrossRef] [Green Version]
  155. Ferretti, G.; Karateev, D. Fermionic UV completions of Composite Higgs models. J. High Energy Phys. 2014, 1403, 077. [Google Scholar] [CrossRef] [Green Version]
  156. Cacciapaglia, G.; Sannino, F. Fundamental Composite (Goldstone) Higgs Dynamics. J. High Energy Phys. 2014, 1404, 111. [Google Scholar] [CrossRef] [Green Version]
  157. Hietanen, A.; Lewis, R.; Pica, C.; Sannino, F. Fundamental Composite Higgs Dynamics on the Lattice: SU(2) with Two Flavors. J. High Energy Phys. 2014, 1407, 116. [Google Scholar] [CrossRef] [Green Version]
  158. Ferretti, G. UV Completions of Partial Compositeness: The Case for a SU(4) Gauge Group. J. High Energy Phys. 2014, 1406, 142. [Google Scholar] [CrossRef] [Green Version]
  159. Parolini, A. Phenomenological aspects of supersymmetric composite Higgs models. Phys. Rev. D 2014, 90, 115026. [Google Scholar] [CrossRef] [Green Version]
  160. Geller, M.; Telem, O. Holographic Twin Higgs Model. Phys. Rev. Lett. 2015, 114, 191801. [Google Scholar] [CrossRef] [Green Version]
  161. Gripaios, B.; Nardecchia, M.; Renner, S.A. Composite leptoquarks and anomalies in B-meson decays. J. High Energy Phys. 2015, 1505, 6. [Google Scholar] [CrossRef] [Green Version]
  162. Low, M.; Tesi, A.; Wang, L.T. Twin Higgs mechanism and a composite Higgs boson. Phys. Rev. D 2015, 91, 095012. [Google Scholar] [CrossRef] [Green Version]
  163. Golterman, M.; Shamir, Y. Top quark induced effective potential in a composite Higgs model. Phys. Rev. D 2015, 91, 094506. [Google Scholar] [CrossRef] [Green Version]
  164. Agashe, K.; Contino, R.; Sundrum, R. Top compositeness and precision unification. Phys. Rev. Lett. 2005, 95, 171804. [Google Scholar] [CrossRef] [Green Version]
  165. Kawamura, Y. Triplet doublet splitting, proton stability and extra dimension. Prog. Theor. Phys. 2001, 105, 999. [Google Scholar] [CrossRef] [Green Version]
  166. Altarelli, G.; Feruglio, F. SU(5) grand unification in extra dimensions and proton decay. Phys. Lett. B 2001, 511, 257. [Google Scholar] [CrossRef] [Green Version]
  167. Hebecker, A.; March-Russell, J. A Minimal S1/(Z2 × Z 2 ) orbifold GUT. Nucl. Phys. B 2001, 613, 3. [Google Scholar] [CrossRef] [Green Version]
  168. Barbieri, R.; Hall, L.J.; Nomura, Y. Softly broken supersymmetric desert from orbifold compactification. Phys. Rev. D 2002, 66, 045025. [Google Scholar] [CrossRef] [Green Version]
  169. Haba, N.; Shimizu, Y.; Suzuki, T.; Ukai, K. Fermion mass hierarchy in the grand unified theory on S1/(Z2 × Z 2 ) orbifold. Prog. Theor. Phys. 2002, 107, 151. [Google Scholar] [CrossRef] [Green Version]
  170. Barr, S.M.; Dorsner, I. Unifying flipped SU(5) in five-dimensions. Phys. Rev. D 2002, 66, 065013. [Google Scholar] [CrossRef] [Green Version]
  171. Hebecker, A.; March-Russell, J. The Flavor hierarchy and seesaw neutrinos from bulk masses in 5-d orbifold GUTs. Phys. Lett. B 2002, 541, 338. [Google Scholar] [CrossRef] [Green Version]
  172. Paccetti Correia, F.; Schmidt, M.G.; Tavartkiladze, Z. 5-D SUSY orbifold SU(6) GUT and pseudoGoldstone Higgs doublets. Phys. Lett. B 2002, 545, 153. [Google Scholar] [CrossRef] [Green Version]
  173. Hebecker, A.; March-Russell, J.; Yanagida, T. Higher dimensional origin of heavy sneutrino domination and low scale leptogenesis. Phys. Lett. B 2003, 552, 229. [Google Scholar] [CrossRef] [Green Version]
  174. Kim, H.D.; Raby, S. Neutrinos in 5-D SO(10) unification. J. High Energy Phys. 2003, 0307, 14. [Google Scholar] [CrossRef] [Green Version]
  175. Bhattacharyya, G.; Branco, G.C.; Silva-Marcos, J.I. CP Violation and Flavour Mixings in Orbifold GUTs. Phys. Rev. D 2008, 77, 011901. [Google Scholar] [CrossRef] [Green Version]
  176. Kobakhidze, A.B. Proton stability in TeV scale GUTs. Phys. Lett. B 2001, 514, 131. [Google Scholar] [CrossRef] [Green Version]
  177. Hebecker, A.; March-Russell, J. Proton decay signatures of orbifold GUTs. Phys. Lett. B 2002, 539, 119. [Google Scholar] [CrossRef] [Green Version]
  178. Shafi, Q.; Tavartkiladze, Z. Neutrino democracy and other phenomenology from 5-D SO(10). Nucl. Phys. B 2003, 665, 469. [Google Scholar] [CrossRef] [Green Version]
  179. Hall, L.J.; Nomura, Y. Gauge unification in higher dimensions. Phys. Rev. D 2001, 64, 055003. [Google Scholar] [CrossRef] [Green Version]
  180. Nomura, Y. Strongly coupled grand unification in higher dimensions. Phys. Rev. D 2002, 65, 085036. [Google Scholar] [CrossRef] [Green Version]
  181. Hall, L.J.; Nomura, Y. Gauge coupling unification from unified theories in higher dimensions. Phys. Rev. D 2002, 65, 125012. [Google Scholar] [CrossRef] [Green Version]
  182. Dermisek, R.; Mafi, A. SO(10) grand unification in five-dimensions: Proton decay and the mu problem. Phys. Rev. D 2002, 65, 055002. [Google Scholar] [CrossRef] [Green Version]
  183. Hall, L.J.; Nomura, Y. A Complete theory of grand unification in five-dimensions. Phys. Rev. D 2002, 66, 075004. [Google Scholar] [CrossRef] [Green Version]
  184. Kim, H.D.; Raby, S. Unification in 5-D SO(10). J. High Energy Phys. 2003, 0301, 56. [Google Scholar] [CrossRef] [Green Version]
  185. Dorsner, I. Flipping SU(5) towards five-dimensional unification. Phys. Rev. D 2004, 69, 056003. [Google Scholar] [CrossRef] [Green Version]
  186. Kim, H.-D.; Kim, J.E.; Lee, H.M. Top - bottom mass hierarchy, s - mu puzzle and gauge coupling unification with split multiplets. Eur. Phys. J. C 2002, 24, 159. [Google Scholar] [CrossRef] [Green Version]
  187. Correia, F.P.; Schmidt, M.G.; Tavartkiladze, Z. Gauge coupling unification and phenomenology of selected orbifold 5-D N=1 SUSY models. Nucl. Phys. B 2003, 649, 39. [Google Scholar] [CrossRef] [Green Version]
  188. Hall, L.J.; Nomura, Y.; Tucker-Smith, D. Gauge Higgs unification in higher dimensions. Nucl. Phys. B 2002, 639, 307. [Google Scholar] [CrossRef] [Green Version]
  189. Hall, L.J.; March-Russell, J.; Okui, T.; Tucker-Smith, D. Towards a theory of flavor from orbifold GUTs. J. High Energy Phys. 2004, 0409, 26. [Google Scholar] [CrossRef]
  190. Babu, K.S.; Barr, S.M.; Kyae, B.-S. Family unification in five-dimensions and six-dimensions. Phys. Rev. D 2002, 65, 115008. [Google Scholar] [CrossRef] [Green Version]
  191. Kim, H.D.; Raby, S.; Schradin, L. Quark and lepton masses in 5-D SO(10). J. High Energy Phys. 2005, 0505, 36. [Google Scholar] [CrossRef]
  192. Forste, S.; Nilles, H.P.; Wingerter, A. Geometry of rank reduction. Phys. Rev. D 2005, 72, 026001. [Google Scholar] [CrossRef] [Green Version]
  193. Braam, F.; Knochel, A.; Reuter, J. An Exceptional SSM from E6 Orbifold GUTs with intermediate LR symmetry. J. High Energy Phys. 2010, 1006, 13. [Google Scholar] [CrossRef] [Green Version]
  194. Li, T.-J. GUT breaking on M4 × T2/(Z2 × Z2). Phys. Lett. B 2001, 520, 377. [Google Scholar] [CrossRef] [Green Version]
  195. Asaka, T.; Buchmuller, W.; Covi, L. Gauge unification in six-dimensions. Phys. Lett. B 2001, 523, 199. [Google Scholar] [CrossRef] [Green Version]
  196. Li, T.-J. N=2 supersymmetric GUT breaking on T2 orbifolds. Nucl. Phys. B 2001, 619, 75. [Google Scholar] [CrossRef] [Green Version]
  197. Haba, N.; Kondo, T.; Shimizu, Y. Fermion mass hierarchy in six-dimensional SO(10) grand unified theory on a T2/Z2 orbifold. Phys. Lett. B 2002, 531, 245. [Google Scholar] [CrossRef] [Green Version]
  198. Watari, T.; Yanagida, T. Higher dimensional supersymmetry as an origin of the three families for quarks and leptons. Phys. Lett. B 2002, 532, 252. [Google Scholar] [CrossRef] [Green Version]
  199. Haba, N.; Kondo, T.; Shimizu, Y. Fermion mass hierarchy in six- dimensional SO(10) SUSY GUT. Phys. Lett. B 2002, 535, 271. [Google Scholar] [CrossRef] [Green Version]
  200. Watari, T.; Yanagida, T. Geometric origin of large lepton mixing in a higher dimensional space-time. Phys. Lett. B 2002, 544, 167. [Google Scholar] [CrossRef] [Green Version]
  201. Asaka, T.; Buchmuller, W.; Covi, L. Exceptional coset spaces and unification in six-dimensions. Phys. Lett. B 2002, 540, 295. [Google Scholar] [CrossRef] [Green Version]
  202. Hebecker, A.; Ratz, M. Group theoretical aspects of orbifold and conifold GUTs. Nucl. Phys. B 2003, 670, 3. [Google Scholar] [CrossRef] [Green Version]
  203. Asaka, T.; Buchmuller, W.; Covi, L. Quarks and leptons between branes and bulk. Phys. Lett. B 2003, 563, 209. [Google Scholar] [CrossRef] [Green Version]
  204. Buchmuller, W.; Kersten, J.; Schmidt-Hoberg, K. Squarks and sleptons between branes and bulk. J. High Energy Phys. 2006, 0602, 69. [Google Scholar] [CrossRef] [Green Version]
  205. Buchmuller, W.; Covi, L.; Emmanuel-Costa, D.; Wiesenfeldt, S. CP Violation and Neutrino Masses and Mixings from Quark Mass Hierarchies. J. High Energy Phys. 2007, 0712, 30. [Google Scholar] [CrossRef] [Green Version]
  206. Hall, L.J.; Nomura, Y.; Okui, T.; Tucker-Smith, D. SO(10) unified theories in six-dimensions. Phys. Rev. D 2002, 65, 035008. [Google Scholar] [CrossRef] [Green Version]
  207. Lee, H.M. Gauge coupling unification in six dimensions. Phys. Rev. D 2007, 75, 065009. [Google Scholar] [CrossRef] [Green Version]
  208. Buchmuller, W.; Covi, L.; Emmanuel-Costa, D.; Wiesenfeldt, S. Flavour structure and proton decay in 6D orbifold GUTs. J. High Energy Phys. 2004, 0409, 4. [Google Scholar] [CrossRef]
  209. Candelas, P.; Horowitz, G.T.; Strominger, A.; Witten, E. Vacuum Configurations for Superstrings. Nucl. Phys. B 1985, 258, 46. [Google Scholar] [CrossRef]
  210. Witten, E. Symmetry Breaking Patterns in Superstring Models. Nucl. Phys. B 1985, 258, 75. [Google Scholar] [CrossRef]
  211. Dixon, L.J.; Harvey, J.A.; Vafa, C.; Witten, E. Strings on Orbifolds. Nucl. Phys. B 1985, 261, 678. [Google Scholar] [CrossRef]
  212. Breit, J.D.; Ovrut, B.A.; Segre, G.C. E6 Symmetry Breaking in the Superstring Theory. Phys. Lett. B 1985, 158, 33. [Google Scholar] [CrossRef]
  213. Dixon, L.J.; Harvey, J.A.; Vafa, C.; Witten, E. Strings on Orbifolds 2. Nucl. Phys. B 1986, 274, 285. [Google Scholar] [CrossRef]
  214. Sen, A. Naturally Light Higgs Doublet in Supersymmetric E6 Grand Unified Theory. Phys. Rev. Lett. 1985, 55, 33. [Google Scholar] [CrossRef] [PubMed]
  215. Ibanez, L.E.; Kim, J.E.; Nilles, H.P.; Quevedo, F. Orbifold Compactifications with Three Families of SU(3) × SU(2) × U(1)n. Phys. Lett. B 1987, 191, 282. [Google Scholar] [CrossRef] [Green Version]
  216. Kobayashi, T.; Raby, S.; Zhang, R.-J. Constructing 5-D orbifold grand unified theories from heterotic strings. Phys. Lett. B 2004, 593, 262. [Google Scholar] [CrossRef] [Green Version]
  217. Kobayashi, T.; Raby, S.; Zhang, R.-J. Searching for realistic 4d string models with a Pati-Salam symmetry: Orbifold grand unified theories from heterotic string compactification on a Z(6) orbifold. Nucl. Phys. B 2005, 704, 3. [Google Scholar] [CrossRef] [Green Version]
  218. Buchmuller, W.; Hamaguchi, K.; Lebedev, O.; Ratz, M. Supersymmetric standard model from the heterotic string. Phys. Rev. Lett. 2006, 96, 121602. [Google Scholar] [CrossRef] [PubMed] [Green Version]
  219. Lebedev, O.; Nilles, H.P.; Raby, S.; Ramos-Sanchez, S.; Ratz, M.; Vaudrevange, P.K.S.; Wingerter, A. A Mini-landscape of exact MSSM spectra in heterotic orbifolds. Phys. Lett. B 2007, 645, 88. [Google Scholar] [CrossRef] [Green Version]
  220. Buchmuller, W.; Hamaguchi, K.; Lebedev, O.; Ratz, M. Supersymmetric Standard Model from the Heterotic String (II). Nucl. Phys. B 2007, 785, 149. [Google Scholar] [CrossRef] [Green Version]
  221. Buchmuller, W.; Ludeling, C.; Schmidt, J. Local SU(5) Unification from the Heterotic String. J. High Energy Phys. 2007, 0709, 113. [Google Scholar] [CrossRef] [Green Version]
  222. Lebedev, O.; Nilles, H.P.; Raby, S.; Ramos-Sanchez, S.; Ratz, M.; Vaudrevange, P.K.S.; Wingerter, A. The Heterotic Road to the MSSM with R parity. Phys. Rev. D 2008, 77, 046013. [Google Scholar] [CrossRef] [Green Version]
  223. Chaichian, M.; Chkareuli, J.L.; Kobakhidze, A. Composite quarks and leptons in higher space-time dimensions. Phys. Rev. D 2002, 66, 095013. [Google Scholar] [CrossRef] [Green Version]
  224. Ma, E. Neutrino masses in an extended gauge model with E6 particle content. Phys. Lett. B 1996, 380, 286. [Google Scholar] [CrossRef] [Green Version]
  225. Keith, E.; Ma, E. Generic consequences of a supersymmetric U(1) gauge factor at the TeV scale. Phys. Rev. D 1997, 56, 7155. [Google Scholar] [CrossRef] [Green Version]
  226. Suematsu, D. Neutralino decay in the μ problem solvable extra U(1) models. Phys. Rev. D 1998, 57, 1738. [Google Scholar] [CrossRef] [Green Version]
  227. Daikoku, Y.; Suematsu, D. Mass bound of the lightest neutral Higgs scalar in the extra U(1) models. Phys. Rev. D 2000, 62, 095006. [Google Scholar] [CrossRef] [Green Version]
  228. King, S.F.; Moretti, S.; Nevzorov, R. Theory and phenomenology of an exceptional supersymmetric standard model. Phys. Rev. D 2006, 73, 035009. [Google Scholar] [CrossRef] [Green Version]
  229. King, S.F.; Moretti, S.; Nevzorov, R. Exceptional supersymmetric standard model. Phys. Lett. B 2006, 634, 278. [Google Scholar] [CrossRef] [Green Version]
  230. King, S.F.; Moretti, S.; Nevzorov, R. Gauge coupling unification in the exceptional supersymmetric standard model. Phys. Lett. B 2007, 650, 57. [Google Scholar] [CrossRef] [Green Version]
  231. King, S.F.; Moretti, S.; Nevzorov, R. E6SSM. AIP Conf. Proc. 2007, 881, 138. [Google Scholar]
  232. Athron, P.; King, S.F.; Miller, D.J.; Moretti, S.; Nevzorov, R. Predictions of the Constrained Exceptional Supersymmetric Standard Model. Phys. Lett. B 2009, 681, 448. [Google Scholar] [CrossRef] [Green Version]
  233. Athron, P.; King, S.F.; Miller, D.J.; Moretti, S.; Nevzorov, R. The Constrained Exceptional Supersymmetric Standard Model. Phys. Rev. D 2009, 80, 035009. [Google Scholar] [CrossRef]
  234. Athron, P.; Hall, J.P.; Howl, R.; King, S.F.; Miller, D.J.; Moretti, S.; Nevzorov, R. Aspects of the exceptional supersymmetric standard model. Nucl. Phys. Proc. Suppl. 2010, 200–202, 120. [Google Scholar] [CrossRef]
  235. Hall, J.P.; King, S.F.; Nevzorov, R.; Pakvasa, S.; Sher, M. Novel Higgs Decays and Dark Matter in the E6SSM. Phys. Rev. D 2011, 83, 075013. [Google Scholar] [CrossRef] [Green Version]
  236. Athron, P.; King, S.F.; Miller, D.J.; Moretti, S.; Nevzorov, R. LHC Signatures of the Constrained Exceptional Supersymmetric Standard Model. Phys. Rev. D 2011, 84, 055006. [Google Scholar] [CrossRef] [Green Version]
  237. Athron, P.; King, S.F.; Miller, D.J.; Moretti, S.; Nevzorov, R. Constrained Exceptional Supersymmetric Standard Model with a Higgs Near 125 GeV. Phys. Rev. D 2012, 86, 095003. [Google Scholar] [CrossRef] [Green Version]
  238. Nevzorov, R. E6 inspired supersymmetric models with exact custodial symmetry. Phys. Rev. D 2013, 87, 015029. [Google Scholar] [CrossRef] [Green Version]
  239. Nevzorov, R. Quasifixed point scenarios and the Higgs mass in the E6 inspired supersymmetric models. Phys. Rev. D 2014, 89, 055010. [Google Scholar] [CrossRef] [Green Version]
  240. Nevzorov, R.; Pakvasa, S. Exotic Higgs decays in the E6 inspired SUSY models. Phys. Lett. B 2014, 728, 210. [Google Scholar] [CrossRef] [Green Version]
  241. Athron, P.; Mühlleitner, M.; Nevzorov, R.; Williams, A.G. Non-Standard Higgs Decays in U(1) Extensions of the MSSM. J. High Energy Phys. 2015, 1501, 153. [Google Scholar] [CrossRef] [Green Version]
  242. Athron, P.; Harries, D.; Nevzorov, R.; Williams, A.G. E6 Inspired SUSY benchmarks, dark matter relic density and a 125 GeV Higgs. Phys. Lett. B 2016, 760, 19. [Google Scholar] [CrossRef] [Green Version]
  243. Nevzorov, R.; Pakvasa, S. Nonstandard Higgs decays in the E6 inspired SUSY models. Nucl. Part. Phys. Proc. 2016, 273-275, 690. [Google Scholar] [CrossRef] [Green Version]
  244. King, S.F.; Nevzorov, R. 750 GeV Diphoton Resonance from Singlets in an Exceptional Supersymmetric Standard Model. J. High Energy Phys. 2016, 1603, 139. [Google Scholar] [CrossRef] [Green Version]
  245. Athron, P.; Harries, D.; Nevzorov, R.; Williams, A.G. Dark matter in a constrained E6 inspired SUSY model. J. High Energy Phys. 2016, 1612, 128. [Google Scholar] [CrossRef] [Green Version]
  246. Nevzorov, R. Leptogenesis as an origin of hot dark matter and baryon asymmetry in the E6 inspired SUSY models. Phys. Lett. B 2018, 779, 223. [Google Scholar] [CrossRef]
  247. Nevzorov, R. E6 inspired SUSY models with custodial symmetry. Int. J. Mod. Phys. A 2018, 33, 1844007. [Google Scholar] [CrossRef]
  248. King, S.F.; Moretti, S.; Nevzorov, R. A Review of the Exceptional Supersymmetric Standard Model. Symmetry 2020, 12, 557. [Google Scholar] [CrossRef] [Green Version]
  249. Nevzorov, R. Higgs Boson with Mass around 125 GeV in SUSY Extensions of the SM. Phys. Atom. Nucl. 2020, 83, 338. [Google Scholar] [CrossRef]
  250. King, S.F.; Luo, R.; Miller, D.J.; Nevzorov, R. Leptogenesis in the Exceptional Supersymmetric Standard Model: Flavour dependent lepton asymmetries. J. High Energy Phys. 2008, 0812, 042. [Google Scholar] [CrossRef]
  251. Asaka, T.; Buchmuller, W.; Covi, L. Bulk and brane anomalies in six-dimensions. Nucl. Phys. B 2003, 648, 231. [Google Scholar] [CrossRef] [Green Version]
  252. von Gersdorff, G.; Quiros, M. Localized anomalies in orbifold gauge theories. Phys. Rev. D 2003, 68, 105002. [Google Scholar] [CrossRef] [Green Version]
  253. Scrucca, C.A.; Serone, M. Anomalies in field theories with extra dimensions. Int. J. Mod. Phys. A 2004, 19, 2579. [Google Scholar] [CrossRef] [Green Version]
  254. Borghini, N.; Gouverneur, Y.; Tytgat, M.H.G. Anomalies and fermion content of grand unified theories in extra dimensions. Phys. Rev. D 2002, 65, 025017. [Google Scholar] [CrossRef] [Green Version]
  255. von Gersdorff, G. Anomalies on Six Dimensional Orbifolds. J. High Energy Phys. 2007, 703, 83. [Google Scholar] [CrossRef]
  256. Adler, S.L. Axial vector vertex in spinor electrodynamics. Phys. Rev. 1969, 177, 2426. [Google Scholar] [CrossRef]
  257. Adler, S.L.; Bardeen, W.A. Absence of higher order corrections in the anomalous axial vector divergence equation. Phys. Rev. 1969, 182, 1517. [Google Scholar] [CrossRef]
  258. Bell, J.S.; Jackiw, R. A PCAC puzzle: Pi0 –> gamma gamma in the sigma model. Nuovo Cim. A 1969, 60, 47. [Google Scholar] [CrossRef] [Green Version]
  259. Green, M.B.; Schwarz, J.H. Anomaly Cancellation in Supersymmetric D=10 Gauge Theory and Superstring Theory. Phys. Lett. B 1984, 149, 117. [Google Scholar] [CrossRef]
  260. Arkani-Hamed, N.; Cohen, A.G.; Georgi, H. Anomalies on orbifolds. Phys. Lett. B 2001, 516, 395. [Google Scholar] [CrossRef] [Green Version]
  261. Scrucca, C.A.; Serone, M.; Silvestrini, L.; Zwirner, F. Anomalies in orbifold field theories. Phys. Lett. B 2002, 525, 169. [Google Scholar] [CrossRef]
  262. Barbieri, R.; Contino, R.; Creminelli, P.; Rattazzi, R.; Scrucca, C.A. Anomalies, Fayet-Iliopoulos terms and the consistency of orbifold field theories. Phys. Rev. D 2002, 66, 024025. [Google Scholar] [CrossRef] [Green Version]
  263. Phillips, D.G., II; Snow, W.M.; Babu, K.; Banerjee, S.; Baxter, D.V.; Berezhiani, Z.; Bergevin, M.; Bhattacharya, S.; Brooijmans, G.; Castellanos, L. Neutron-Antineutron Oscillations: Theoretical Status and Experimental Prospects. Phys. Rept. 2016, 612, 1. [Google Scholar] [CrossRef] [Green Version]
  264. Kronfeld, A.S.; Tschirhart, R.S.; Al-Binni, U.; Altmannshofer, W.; Ankenbrandt, C.; Babu, K.; Banerjee, S.; Bass, M.; Batell, B.; Baxter, D.V. Project X: Physics Opportunities. arXiv 2013, arXiv:1306.5009. [Google Scholar]
  265. The ATLAS collaboration. A search for pair-produced resonances in four-jet final states at s = 13 TeV with the ATLAS detector. Eur. Phys. J. C 2018, 78, 250. [Google Scholar]
  266. Cline, J.M.; Raby, S. Gravitino induced baryogenesis: A Problem made a virtue. Phys. Rev. D 1991, 43, 1781. [Google Scholar] [CrossRef]
  267. Scherrer, R.J.; Cline, J.M.; Raby, S.; Seckel, D. Gravitino induced baryogenesis, primordial nucleosynthesis, and the Tremaine-Gunn limit. Phys. Rev. D 1991, 44, 3760. [Google Scholar] [CrossRef] [PubMed]
  268. Ma, E.; Raidal, M. Three active and two sterile neutrinos in an E6 model of diquark baryogenesis. J. Phys. G 2002, 28, 95. [Google Scholar] [CrossRef]
  269. Ma, E. Multiplicative conservation of baryon number and baryogenesis. Phys. Lett. B 2008, 661, 273. [Google Scholar] [CrossRef] [Green Version]
  270. Ma, E. Common Origin of (−)L, (−)3B, and Strong CP Conservation. Phys. Rev. D 2008, 78, 047701. [Google Scholar] [CrossRef] [Green Version]
  271. Ma, E. Axionic Extensions of the Supersymmetric Standard Model. Mod. Phys. Lett. A 2009, 24, 1335. [Google Scholar] [CrossRef] [Green Version]
  272. Kohri, K.; Mazumdar, A.; Sahu, N. Inflation, baryogenesis and gravitino dark matter at ultra low reheat temperatures. Phys. Rev. D 2009, 80, 103504. [Google Scholar] [CrossRef] [Green Version]
  273. Cui, Y.; Sundrum, R. Baryogenesis for weakly interacting massive particles. Phys. Rev. D 2013, 87, 116013. [Google Scholar] [CrossRef] [Green Version]
  274. Krauss, L.M.; Long, A.J.; Sabharwal, S. Gravitino Leptogenesis. Phys. Rev. D 2014, 89, 043503. [Google Scholar] [CrossRef] [Green Version]
  275. Rompineve, F. Weak Scale Baryogenesis in a Supersymmetric Scenario with R-parity violation. J. High Energy Phys. 2014, 1408, 014. [Google Scholar] [CrossRef] [Green Version]
  276. Boucenna, S.M.; Morisi, S. Theories relating baryon asymmetry and dark matter: A mini review. Front. Phys. 2014, 1, 33. [Google Scholar] [CrossRef] [Green Version]
  277. Ishiwata, K.; Jeong, K.S.; Takahashi, F. Moduli-induced Baryogenesis. J. High Energy Phys. 2014, 1402, 62. [Google Scholar] [CrossRef] [Green Version]
  278. Dhuria, M.; Hati, C.; Sarkar, U. Explaining the CMS excesses, baryogenesis and neutrino masses in E6 motivated U(1)N model. Phys. Rev. D 2016, 93, 015001. [Google Scholar] [CrossRef] [Green Version]
  279. Cui, Y. A Review of WIMP Baryogenesis Mechanisms. Mod. Phys. Lett. A 2015, 30, 1530028. [Google Scholar] [CrossRef] [Green Version]
  280. Farina, M.; Monteux, A.; Shin, C.S. Twin mechanism for baryon and dark matter asymmetries. Phys. Rev. D 2016, 94, 035017. [Google Scholar] [CrossRef] [Green Version]
  281. Cui, Y.; Okui, T.; Yunesi, A. LHC Signatures of WIMP-triggered Baryogenesis. Phys. Rev. D 2016, 94, 115022. [Google Scholar] [CrossRef] [Green Version]
  282. Luty, M.A. Baryogenesis Via Leptogenesis. Phys. Rev. D 1992, 45, 455. [Google Scholar] [CrossRef] [PubMed]
  283. Flanz, M.; Paschos, E.A.; Sarkar, U. Baryogenesis from a lepton asymmetric universe. Phys. Lett. B 1995, 345, 248. [Google Scholar] [CrossRef] [Green Version]
  284. Plumacher, M. Baryogenesis and lepton number violation. Z. Phys. C 1997, 74, 549. [Google Scholar] [CrossRef] [Green Version]
  285. Buchmuller, W.; Plumacher, M. CP asymmetry in Majorana neutrino decays. Phys. Lett. B 1998, 431, 354. [Google Scholar] [CrossRef] [Green Version]
  286. Davidson, S.; Nardi, E.; Nir, Y. Leptogenesis. Phys. Rept. 2008, 466, 105. [Google Scholar] [CrossRef]
Figure 1. Logarithm (base 10) of the absolute value of the decay asymmetry ε 1 , 3 as a function of logarithm (base 10) of Δ φ for | g 32 | = 1 (solid line) and | g 32 | = 0.1 (dashed line) in the case when g 11 = g 21 = g 12 = g 22 = 0 and M 2 = 10 · M 1 .
Figure 1. Logarithm (base 10) of the absolute value of the decay asymmetry ε 1 , 3 as a function of logarithm (base 10) of Δ φ for | g 32 | = 1 (solid line) and | g 32 | = 0.1 (dashed line) in the case when g 11 = g 21 = g 12 = g 22 = 0 and M 2 = 10 · M 1 .
Universe 08 00033 g001
Table 1. Orbifold parity assignments in the bulk 27 supermultiplet with σ = σ I = σ I I = σ I I I = + 1 .
Table 1. Orbifold parity assignments in the bulk 27 supermultiplet with σ = σ I = σ I I = σ I I I = + 1 .
q d c u c e c ν c h u h d h h c s
Z 2 +++++
Z 2 I +++++++
Z 2 I I +++++
Z 2 I I I +++++++++++
Table 2. The charges ( Q i , Q ˜ i , Q i N and Q i Y ) of the components of the 27-plet associated with the U ( 1 ) , U ˜ ( 1 ) , U ( 1 ) N and U ( 1 ) Y symmetries.
Table 2. The charges ( Q i , Q ˜ i , Q i N and Q i Y ) of the components of the 27-plet associated with the U ( 1 ) , U ˜ ( 1 ) , U ( 1 ) N and U ( 1 ) Y symmetries.
q d c u c e c ν c h u h d h h c s
24 Q i 11 2 2 411 2 2 11
24 Q ˜ i 1 1 2003 3 0 2 1 3
40 Q i N 121210 2 3 2 3 5
5 3 Q i Y 1 6 1 3 2 3 1 2 10 1 2 1 2 1 3 1 3 0
Table 3. The bulk supermultiplets and their zero modes that remain massless below the scales M X , φ 0 and ϕ 0 .
Table 3. The bulk supermultiplets and their zero modes that remain massless below the scales M X , φ 0 and ϕ 0 .
Φ ^ i u Φ ^ i e Φ ^ i q Φ ^ i d Φ ^ i Φ ^ i u ¯ Φ ^ i e ¯ Φ ^ i q ¯ Φ ^ i d ¯ Φ ^ i ¯
E M X u i c , e i c , u i c , e i c , q i , d i c , ν i c , i , u c ¯ i , e c ¯ i , u c ¯ i , e c ¯ i , q i ¯ , d i c ¯ , ν i c ¯ , i ¯ ,
h i h i h i u h i c , s i h i d h ¯ i h ¯ i h i u ¯ h i c ¯ , s i ¯ h i d ¯
E φ 0 u i c , e i c q i , d i c , ν i c , i , u c ¯ i , e c ¯ i q i ¯ , d i c ¯ , ν i c ¯ , i ¯ ,
h i h i u h i c , s i h i d h ¯ i h i u ¯ h i c ¯ , s i ¯ h i d ¯
E ϕ 0 u i c e i c q i d i c i u c ¯ e c ¯ q ¯ d c ¯ ¯
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