Quantum Field Theory, 2nd Edition

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Foundations of Quantum Mechanics and Quantum Gravity".

Deadline for manuscript submissions: 28 February 2025 | Viewed by 3508

Special Issue Editor


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Guest Editor
Theoretical High Energy Physics, University of Heidelberg, Heidelberg, Germany
Interests: quantum field theory; pure Yang-Mills theory and the foundations of quantum mechanics
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Special Issue Information

Dear Colleagues,

Quantum field theory is a convincing framework used to address a variety of subatomic processes, high-energy particle reactions, and the effective physics of condensed matter systems. In particular, quantum gauge theory has acquired a prominent status. This Special Issue aims to present the latest developments in local quantum field theory, perturbatively and nonperturbatively and largely analytically describing systems of the variable spacetime dimension D=d+1 and signature, as well as field content. Examples include non-perturbative and analytical approaches to gauge theory (semi-classical approximation, non-perturbative a priori estimates) and conformal field theory in d=1,2,3, as well as approaches to quantum field theory that exploit a weak–strong coupling duality. We also welcome submissions that discuss resummation schemes of small-coupling expansions, operator product expansions, numerical approaches such as lattice gauge theory, quantum field theoretic investigations on strongly curved spacetime backgrounds and at finite temperature, and the various approaches to quantum gravity.

One of the second Special Issue’s focuses is the investigation of implications of an analytical approach to 4D Euclidean Yang–Mills thermodynamics (gauge groups SU(2) and SU(3)) developed by the editor and his collaborators. In particular, we encourage contributions that discuss the temperature dependence of ultralight Planck-scale axions by referring to matrix models on the spectrum of the Dirac operator, direct or indirect (e.g., field-strength correlator) lattice computations or effective chiral field-theory techniques. In the context of astrophysical/cosmological axion physics, we welcome numerical investigations of self-gravitating axion lumps (fuzzy dark matter) for a single axion species and/or several components either treated entirely by the Poisson–Schrödinger system or partly in terms of classical N-body components. Here, it is also highly interesting to include relativistic corrections to study the potential onset of collapse. Emulator-based and effective field theoretic approaches to the non-linear growth of small-scale structure are important tools to learn about the nature of dark matter (possibly in the framework of fuzzy dark matter based on ultralight axions), and we welcome submissions in this field.

The Special Issue would also benefit from contributions that target the process of thermalization and mixing of several Yang–Mills theories subject to hierarchical Yang–Mills scales.  To this end, a revisit of big-bang nucleosynthesis and the investigation of a partial photon-induced disintegration of already formed light elements due to a Hagedorn transition at a temperature of ~10 keV would be insightful. On the basis of the Yang–Mills theory, this topic is tightly connected to understanding why electroweak symmetry breaking is so effectively and successfully realized in the Standard Model. It also touches upon issues of plasma instabilities in terrestrial nuclear-fusion experiments for both inertial and magnetic confinement.

There are interesting questions to be addressed concerning the ranking of multi-loop diagrams in deconfining SU(2) Yang–Mills thermodynamics, and it would be useful if sharper tools than those that already exist could be developed in this regard. 

The editor hopes that the quantum thermodynamics of Yang–Mills theory could shed more light on how quantum gravitational processes work within black-hole thermodynamics when studying the microscopic interplay of both ingredients. Here, we particularly welcome speculative ideas. 

Finally, we encourage authors that specialize in 2D strongly correlated electrons to contribute to this Special Issue in elucidating the non-local electronic properties (e.g. spin-charge separation and long-range magnetic correlations).

Dr. Ralf Hofmann
Guest Editor

Manuscript Submission Information

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Keywords

  • ultralight axions
  • Peccei–Quinn at finite temperature
  • spectral densities
  • mixing of Yang–Mills theories
  • electroweak symmetry breaking
  • coarse-graining of Euclidean field theory gradient flow cooling

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Published Papers (3 papers)

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Research

14 pages, 306 KiB  
Article
The Quantum Electromagnetic Field in the Weyl–Wigner Representation
by Emilio Santos
Universe 2024, 10(12), 452; https://doi.org/10.3390/universe10120452 - 9 Dec 2024
Viewed by 561
Abstract
The quantum electromagnetic (EM) field is formulated in the Weyl–Wigner representation (WW), which is equivalent to the standard Hilbert space one (HS). In principle, it is possible to interpret within WW all experiments involving the EM field interacting with macroscopic bodies, the latter [...] Read more.
The quantum electromagnetic (EM) field is formulated in the Weyl–Wigner representation (WW), which is equivalent to the standard Hilbert space one (HS). In principle, it is possible to interpret within WW all experiments involving the EM field interacting with macroscopic bodies, the latter treated classically. In the WW formalism, the essential difference between classical electrodynamics and the quantum theory of the EM field is just the assumption that there is a random EM field-filling space, i.e., the existence of a zero-point field with a Gaussian distribution for the field amplitudes. I analyze a typical optical test of a Bell inequality. The model admits an interpretation compatible with local realism, modulo a number of assumptions assumed plausible. Full article
(This article belongs to the Special Issue Quantum Field Theory, 2nd Edition)
10 pages, 284 KiB  
Article
Topological Susceptibility of the Gluon Plasma in the Stochastic-Vacuum Approach
by Dmitry Antonov
Universe 2024, 10(9), 377; https://doi.org/10.3390/universe10090377 - 23 Sep 2024
Cited by 1 | Viewed by 679
Abstract
Topological susceptibility of the SU(3) gluon plasma is calculated by accounting for both factorized and non-factorized contributions to the two-point correlation function of topological-charge densities. It turns out that, while the factorized contribution keeps this correlation function non-positive away from the origin, the [...] Read more.
Topological susceptibility of the SU(3) gluon plasma is calculated by accounting for both factorized and non-factorized contributions to the two-point correlation function of topological-charge densities. It turns out that, while the factorized contribution keeps this correlation function non-positive away from the origin, the non-factorized contribution makes it positive at the origin, in accordance with the reflection positivity condition. Matching the obtained result for topological susceptibility to its lattice value at the deconfinement critical temperature, we fix the parameters of the quartic cumulant of gluonic field strengths, and calculate the contribution of that cumulant to the string tension. This contribution reduces the otherwise too large value of the string tension, which stems from the quadratic cumulant, making it much closer to the standard phenomenological value. Full article
(This article belongs to the Special Issue Quantum Field Theory, 2nd Edition)
20 pages, 1110 KiB  
Article
Quantum Field Theory of Neutrino Mixing in Spacetimes with Torsion
by Antonio Capolupo, Giuseppe De Maria, Simone Monda, Aniello Quaranta and Raoul Serao
Universe 2024, 10(4), 170; https://doi.org/10.3390/universe10040170 - 3 Apr 2024
Cited by 5 | Viewed by 1581
Abstract
In the framework of quantum field theory, we analyze the neutrino oscillations in the presence of a torsion background. We consider the Einstein–Cartan theory and we study the cases of constant torsion and of linearly time-dependent torsion. We derive new neutrino oscillation formulae [...] Read more.
In the framework of quantum field theory, we analyze the neutrino oscillations in the presence of a torsion background. We consider the Einstein–Cartan theory and we study the cases of constant torsion and of linearly time-dependent torsion. We derive new neutrino oscillation formulae which depend on the spin orientation. Indeed, the energy splitting induced by the torsion influences oscillation amplitudes and frequencies. This effect is maximal for values of torsion of the same order of the neutrino masses and for very low momenta, and disappears for large values of torsion. Moreover, neutrino oscillation is inhibited for intensities of torsion term much larger than neutrino masses and momentum. The modifications induced by torsion on the CP-asymmetry are also presented. Future experiments, such as PTOLEMY, which have as a goal the analysis of the cosmological background of neutrino (which have very low momenta), can provide insights into the effect shown here. Full article
(This article belongs to the Special Issue Quantum Field Theory, 2nd Edition)
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