Neutron Stars in Modified Teleparallel Gravity
arXiv:2301.06432 · doi:10.1088/1475-7516/2023/04/044
Abstract
We investigate compact objects in modified teleparallel gravity with realistic equations of state. We propose a modification of Teleparallel Equivalent to General Relativity, then an appropriate tetrad is applied to the field equations. A specific set of relations showing an equivalency between our gravitational model and the New General Relativity is found. The conservation equation implies that our Tolman-Oppenheimer-Volkoff equations are presented with an effective gravitational coupling constant. Numerical analysis using realistic equations of state is made, and the behavior of mass, radius, and the relation mass-radius as functions of a free parameter of our model is also investigated.
9 pages, 5 figures
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Cited by in corpus (6)
- Mass of compact stars in f(T) gravity
- Static spherically symmetric solutions in New General Relativity
- Black hole solutions surrounded by anisotropic fluid in f(T,T) gravity
- Dark matter effects in modified teleparallel gravity
- Distinctive Features of Hairy Black Holes in Teleparallel Gauss-Bonnet Gravity
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