Relativistic compact stars in $f(T)$ gravity admitting conformal motion

Abstract

We provide a set of exact spherically symmetric solutions describing the interior of a relativistic star under f(T) modified gravity. To tackle the problem with lucidity we also assume the existence of a conformal Killing vector field within this f(T) gravity. We study several cases of interest to explore physically valid features of the solutions.

9 pages, 7 figues, Accepted in Astrophysics and Space Science

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Cited by in corpus (9)

• Compact stars in $f(R,T)$ gravity
• Exploring physical properties of minimally deformed strange star model and constraints on maximum mass limit in $f(\mathcal{Q})$ gravity
• Stability of motion and thermodynamics in charged black holes in $f(T)$ gravity
• Quasinormal modes of black holes in f(T) gravity
• Compact stars with specific mass function
• Big Bang Nucleosynthesis constraints on $f(T,T_G)$ gravity
• Unimodular $f(G)$ gravity
• Self-similarity in static axially symmetric relativistic fluids
• Neutron Stars in Mimetic Gravity