Generating primordial fluctuations from modified teleparallel gravity with local Lorentz-symmetry breaking
In the context of modified teleparallel gravity, we study the generation of primordial density fluctuations in a general scalar-torsion theory whose Lagrangian density is an arbitrary function f(T,ϕ) of the torsion scalar T and a scalar field ϕ, plus the kinetic term of this latter. It is well known...
Main Authors: | , |
---|---|
Format: | Article |
Language: | English |
Published: |
Elsevier
2020-10-01
|
Series: | Physics Letters B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269320304998 |
id |
doaj-e5d74f4e48434098abd58adf83146597 |
---|---|
record_format |
Article |
spelling |
doaj-e5d74f4e48434098abd58adf831465972020-11-25T02:06:07ZengElsevierPhysics Letters B0370-26932020-10-01809135696Generating primordial fluctuations from modified teleparallel gravity with local Lorentz-symmetry breakingManuel Gonzalez-Espinoza0Giovanni Otalora1Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4950, Valparaíso, ChileCorresponding author.; Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4950, Valparaíso, ChileIn the context of modified teleparallel gravity, we study the generation of primordial density fluctuations in a general scalar-torsion theory whose Lagrangian density is an arbitrary function f(T,ϕ) of the torsion scalar T and a scalar field ϕ, plus the kinetic term of this latter. It is well known that generic modifications of teleparallel gravity are not invariant under six-parameter local Lorentz transformations. In order to restore the local Lorentz symmetry, we have incorporated six additional degrees of freedom in the form of Goldstone modes of the symmetry breaking through a Lorentz rotation of the tetrad field. After integrating out all the auxiliary modes, we obtain a second order action for the scalar and tensor propagating modes and their power spectrum generated during inflation. It is found that an explicit mass term emerges in the second order action for curvature perturbation, describing the imprints of local Lorentz violation at first-order of slow-roll. We show that only inflationary models with nonminimal coupling functions f(T,ϕ) which are non-linear in T, including the case of f(T) gravity with minimally coupled scalar field, can generate primordial fluctuations. For a concrete model of inflation, we study the power-law potential by using the latest Planck data.http://www.sciencedirect.com/science/article/pii/S0370269320304998 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Manuel Gonzalez-Espinoza Giovanni Otalora |
spellingShingle |
Manuel Gonzalez-Espinoza Giovanni Otalora Generating primordial fluctuations from modified teleparallel gravity with local Lorentz-symmetry breaking Physics Letters B |
author_facet |
Manuel Gonzalez-Espinoza Giovanni Otalora |
author_sort |
Manuel Gonzalez-Espinoza |
title |
Generating primordial fluctuations from modified teleparallel gravity with local Lorentz-symmetry breaking |
title_short |
Generating primordial fluctuations from modified teleparallel gravity with local Lorentz-symmetry breaking |
title_full |
Generating primordial fluctuations from modified teleparallel gravity with local Lorentz-symmetry breaking |
title_fullStr |
Generating primordial fluctuations from modified teleparallel gravity with local Lorentz-symmetry breaking |
title_full_unstemmed |
Generating primordial fluctuations from modified teleparallel gravity with local Lorentz-symmetry breaking |
title_sort |
generating primordial fluctuations from modified teleparallel gravity with local lorentz-symmetry breaking |
publisher |
Elsevier |
series |
Physics Letters B |
issn |
0370-2693 |
publishDate |
2020-10-01 |
description |
In the context of modified teleparallel gravity, we study the generation of primordial density fluctuations in a general scalar-torsion theory whose Lagrangian density is an arbitrary function f(T,ϕ) of the torsion scalar T and a scalar field ϕ, plus the kinetic term of this latter. It is well known that generic modifications of teleparallel gravity are not invariant under six-parameter local Lorentz transformations. In order to restore the local Lorentz symmetry, we have incorporated six additional degrees of freedom in the form of Goldstone modes of the symmetry breaking through a Lorentz rotation of the tetrad field. After integrating out all the auxiliary modes, we obtain a second order action for the scalar and tensor propagating modes and their power spectrum generated during inflation. It is found that an explicit mass term emerges in the second order action for curvature perturbation, describing the imprints of local Lorentz violation at first-order of slow-roll. We show that only inflationary models with nonminimal coupling functions f(T,ϕ) which are non-linear in T, including the case of f(T) gravity with minimally coupled scalar field, can generate primordial fluctuations. For a concrete model of inflation, we study the power-law potential by using the latest Planck data. |
url |
http://www.sciencedirect.com/science/article/pii/S0370269320304998 |
work_keys_str_mv |
AT manuelgonzalezespinoza generatingprimordialfluctuationsfrommodifiedteleparallelgravitywithlocallorentzsymmetrybreaking AT giovanniotalora generatingprimordialfluctuationsfrommodifiedteleparallelgravitywithlocallorentzsymmetrybreaking |
_version_ |
1724934923738939392 |