Saved in:
Bibliographic Details
Main Authors: Zhang, Feng-Yi, Zhai, Rongrong, Chen, Li-Yang
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2508.16530
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866913074268602368
author Zhang, Feng-Yi
Zhai, Rongrong
Chen, Li-Yang
author_facet Zhang, Feng-Yi
Zhai, Rongrong
Chen, Li-Yang
contents We reassess single-field slow-roll inflation in teleparallel gravity with $f(T)=C\,T^{2δ+1}$, motivated by recent measurements from the Atacama Cosmology Telescope (ACT) that indicate a modest upward shift in the scalar spectral index $n_s$. Using analytic approximations together with high-precision numerical calculations, we compute primordial predictions for representative potentials: power-law monomials, hilltop models, and $E$-type plateaus. We find that torsional corrections controlled by $δ$ generically suppress $r$ while keeping $n_s$ near its slow-roll value. As a result, modest positive $δ$ can restore viability to sub-quadratic monomials and hilltop models that are disfavored in general relativity (GR), whereas $E$-type plateaus remain compatible only in a limited range of $δ$: small $δ$ may improve the fit but moderate $δ$ drives the dynamics toward quadratic-like behaviour and increases $r$. These signatures are observationally testable: improved cosmic microwave background (CMB) B-mode measurements will further discriminate among potential classes and place quantitative bounds on torsional deviations from GR.
format Preprint
id arxiv_https___arxiv_org_abs_2508_16530
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle ACT-Era Constraints on Single-Field Inflation in $f(T)$ Teleparallel Gravity
Zhang, Feng-Yi
Zhai, Rongrong
Chen, Li-Yang
General Relativity and Quantum Cosmology
We reassess single-field slow-roll inflation in teleparallel gravity with $f(T)=C\,T^{2δ+1}$, motivated by recent measurements from the Atacama Cosmology Telescope (ACT) that indicate a modest upward shift in the scalar spectral index $n_s$. Using analytic approximations together with high-precision numerical calculations, we compute primordial predictions for representative potentials: power-law monomials, hilltop models, and $E$-type plateaus. We find that torsional corrections controlled by $δ$ generically suppress $r$ while keeping $n_s$ near its slow-roll value. As a result, modest positive $δ$ can restore viability to sub-quadratic monomials and hilltop models that are disfavored in general relativity (GR), whereas $E$-type plateaus remain compatible only in a limited range of $δ$: small $δ$ may improve the fit but moderate $δ$ drives the dynamics toward quadratic-like behaviour and increases $r$. These signatures are observationally testable: improved cosmic microwave background (CMB) B-mode measurements will further discriminate among potential classes and place quantitative bounds on torsional deviations from GR.
title ACT-Era Constraints on Single-Field Inflation in $f(T)$ Teleparallel Gravity
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2508.16530