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f(T) gravity: background dependence and propagating degrees of freedom

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F25%3A00635570" target="_blank" >RIV/68378271:_____/25:00635570 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1103/PhysRevD.111.104023" target="_blank" >https://doi.org/10.1103/PhysRevD.111.104023</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1103/PhysRevD.111.104023" target="_blank" >10.1103/PhysRevD.111.104023</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    f(T) gravity: background dependence and propagating degrees of freedom

  • Original language description

    The standard cosmological model, rooted in general relativity (GR), has achieved remarkable success, yet it still faces unresolved issues like the nature of dark matter, dark energy, and the Hubble tension. These challenges might imply the need for alternative gravitational theories. Teleparallel gravity offers a compelling framework by reformulating the gravitational interaction using torsion, rather than curvature, as its fundamental geometrical property. This paper delves into f(T) gravity, an extension of the teleparallel equivalent of general relativity (TEGR), which introduces nonlinear modifications of the torsion scalar T. We focus on the role of spacetime-dependent Lorentz transformations in the vierbein formalism, examining their impact on both background solutions and perturbation dynamics. Special attention is given to the homogeneous and isotropic Friedmann-Lemaître-Robertson-Walker (FLRW) spacetime, as well as the anisotropic Bianchi I spacetime. Furthermore, the analysis of the propagating degrees of freedom on these spacetimes is performed. While it is well established that TEGR reproduces the same results as GR, the propagating degrees of freedom in its nonlinear extension, f(T) gravity, is still debated in the literature. In this work, we find that only two fields propagate in the gravity sector, independent of the background spacetime considered, either FLRW or Bianchi I. Although not definitive, this paper provides fresh insights into the issue of the propagating degrees of freedom in f(T) gravity, opening the door to intriguing new directions for further investigation.n

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/LUC23115" target="_blank" >LUC23115: Spin 2 WISPers from the laboratory to the cosmos</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2025

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Physical Review D

  • ISSN

    2470-0010

  • e-ISSN

    2470-0029

  • Volume of the periodical

    111

  • Issue of the periodical within the volume

    10

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    17

  • Pages from-to

    104023

  • UT code for WoS article

    001491244000009

  • EID of the result in the Scopus database

    2-s2.0-105005275100