Absence of Relativistic Stars in f(T) Gravity
作者： Cemsinan Deliduman , Baris Yapiskan
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摘要: In this work we investigate the structure of neutron stars in modified f(T) gravity models. We find that, unlike f(R) models, equations motion put a rather strict constraint on possible functions. Specifically, after analyzing problem two different choice coordinates with spherical symmetry, conclude that relativistic star solution models is only if linear function torsion scalar T, case Teleparallel Equivalent General Relativity.
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