Gravity and Cosmology: Exploring the Mysteries of f(T) Gravity

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Gravitation".

Deadline for manuscript submissions: closed (20 December 2024) | Viewed by 1485

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Divisão de Astrofísica, Instituto Nacional de Pesquisas Espaciais, São José dos Campos 12227-010, Brasil
Interests: gravitation; compact stars; cosmology

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Guest Editor
1. Instituto Federal Fluminense (IFF) , Campus Quissamã, Av. Amilcar Pereira da Silva, 727 Piteiras, Quissamã 28735-000, RJ, Brasil
2. Divisão de Astrofísica, Instituto Nacional de Pesquisas Espaciais, São José dos Campos 12227-010, Brasil
Interests: gravitation; compact stars; field theory

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Guest Editor
1. National Observatory of Athens, Lofos Nymfon, 11852 Athens, Greece
2. CAS Key Laboratory for Researches in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, China
3. Departamento de Matemáticas, Universidad Católica del Norte, Avda. Angamos 0610, Casilla, Antofagasta 1280, Chile
Interests: ark energy formulation; modified theories of gravity; inflationary cosmology; brane cosmology; observational cosmology
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Special Issue Information

Dear Colleagues,

The search for a consistent and complete theory of gravity is one of the great ambitions of this century. General Relativity (GR), despite its overwhelming success, has been confronted with the latest data from cosmological discoveries, for example, the supernovae observations, which indicate an accelerated expansion of the universe. In this sense, it appears to be inevitable to consider some modifications in GR. Dark energy is a possible factor to be included in GR in order to explain such an accelerated expansion, although its origin or composition is not known. In this search for the most suitable theory of gravity, it is natural to consider not only direct extensions of GR itself but also take into account different formulations, which, besides the scalar curvature R, involve other geometric invariants, such as the models with scalar torsion T.

The Teleparallel equivalent of General Relativity (TEGR) is a theory where gravitation is due to torsion and not due to curvature but it is dynamically equivalent to GR, i.e., cannot be distinguished through classical experiments. It is possible to build extended theories of gravity by modifying both GR and Teleparallel theories. Modifications in TEGR by considering the Lagrangian density as a more general function of the torsion scalar, namely, f(T), lead to second order field equations, simpler than those from alternative models, f(R), generated by extensions of curvature-based formulations. Recent works on f(T) have presented interesting cosmological and astrophysical solutions, providing alternative interpretations for the acceleration phases of the universe, for example.

The aim of this Special Issue is to explore different aspects of f(T) Gravity and related issues. Thus, it is expected to have contributions on cosmology and compact stars, as well as relevant topics related to the theory itself, i.e., what are well established issues and putative ambiguities.


Dr. Jose Carlos Neves De Araujo
Dr. Hemily Gomes Marciano Fortes
Dr. Emmanuel N. Saridakis
Guest Editors

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Keywords

  • gravity
  • general relativity
  • teleparallel theory
  • torsion
  • extended teleparallel theory
  • cosmology
  • compact stars

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Published Papers (2 papers)

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Research

20 pages, 1799 KiB  
Article
Impact of Charge on Strange Compact Stars in Rastall Theory
by Malick Sallah and Muhammad Sharif
Universe 2025, 11(1), 25; https://doi.org/10.3390/universe11010025 - 16 Jan 2025
Viewed by 346
Abstract
Within the framework of Rastall theory, we investigate the impact of charge on the structural development of different types of spherically symmetric anisotropic stars. To do so, we present modified field equations based upon the Finch–Skea metric potentials expressed in terms of three [...] Read more.
Within the framework of Rastall theory, we investigate the impact of charge on the structural development of different types of spherically symmetric anisotropic stars. To do so, we present modified field equations based upon the Finch–Skea metric potentials expressed in terms of three parameters (A,B,C). These constants are determined using suitable matching conditions and observational data for compact objects which include Her X-1, SAX J 1808.4-3658, PSR J038-0842, LMC X-4 and SMC X-1. The equation of state offered by the MIT bag model for quark–gluon plasma is used to investigate the inner structure and other characteristics of these compact objects. For a fixed bag constant, B=60MeV/fm3, and two sets of the Rastall and charge parameters, ζ=0.255,0.259 and Q˜=0.2,0.7, respectively, we analyze the consistency of the matter variables in the model and other physical parameters such as energy conditions, stellar mass, compactness, and surface redshift. In addition, we assess the stability of the constructed model through two different approaches. It is found that the obtained model is physically viable and stable. Full article
(This article belongs to the Special Issue Gravity and Cosmology: Exploring the Mysteries of f(T) Gravity)
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17 pages, 1035 KiB  
Article
Mapping the ΛsCDM Scenario to f(T) Modified Gravity: Effects on Structure Growth Rate
by Mateus S. Souza, Ana M. Barcelos, Rafael C. Nunes, Özgür Akarsu and Suresh Kumar
Universe 2025, 11(1), 2; https://doi.org/10.3390/universe11010002 - 25 Dec 2024
Viewed by 519
Abstract
The concept of a rapidly sign-switching cosmological constant, interpreted as a mirror AdS-dS transition in the late universe and known as the ΛsCDM, has significantly improved the fit to observational data, offering a promising framework for alleviating major cosmological tensions such [...] Read more.
The concept of a rapidly sign-switching cosmological constant, interpreted as a mirror AdS-dS transition in the late universe and known as the ΛsCDM, has significantly improved the fit to observational data, offering a promising framework for alleviating major cosmological tensions such as the H0 and S8 tensions. However, when considered within general relativity, this scenario does not predict any effects on the evolution of the matter density contrast beyond modifications to the background functions. In this work, we propose a new gravitational model in which the background dynamics predicted by the ΛsCDM framework are mapped into f(T) gravity, dubbed f(T)-ΛsCDM, rendering the models indistinguishable at the background level. However, in this new scenario, the sign-switching cosmological constant dynamics modify the evolution of linear matter perturbations through an effective gravitational constant, Geff. We investigate the evolution of the growth rate and derive new observational constraints for this scenario using RSD measurements. We also present new constraints in the standard ΛsCDM case, incorporating the latest Type Ia supernovae data samples available in the literature, along with BAO data from DESI. Our findings indicate that the new corrections expected at the linear perturbative level, as revealed through RSD samples, can provide significant evidence in favor of this new scenario. Additionally, this model may be an excellent candidate for resolving the current S8 tension. Full article
(This article belongs to the Special Issue Gravity and Cosmology: Exploring the Mysteries of f(T) Gravity)
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