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Einstein Static Universe in Exponential $f(T)$ Gravity

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arxiv 1302.2688 v2 pith:M6T6SUE3 submitted 2013-02-12 gr-qc astro-ph.CO

Jung-Tsung Li , Chung-Chi Lee , Chao-Qiang Geng This is my paper · ORCID
classification gr-qcastro-ph.CO
keywords universeeinsteinexponentialgravitystablestatictheoriesallowed
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abstract

We analyze the stability of the Einstein static closed and open universe in two types of exponential $f(T)$ gravity theories. We show that the stable solutions exist in these two models. In particular, we find that large regions of parameter space in equation of state $w=p/\rho$ for the stable universe are allowed in the $f(T)$ theories.

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Cited by 1 Pith paper

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  1. Apparent horizon thermodynamics in an exponential $f(Q)$ gravity model

    gr-qc 2026-08 conditional novelty 5.0 of 10

    In an exponential f(Q) model, apparent-horizon entropy gains exponentially suppressed corrections to the area law, and the generalized second law excludes parameter values b>0.26 in the future-redshift region.

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