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Anisotropic compact star models in f (T) gravity with Tolman-Kuchowicz spacetime

Author
Ditta, Allah
Azmat, Hina
GÜDEKLİ, Ertan
Bhar, Piyali
Zubair, M.
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Abstract
© 2021 World Scientific Publishing Company.The purpose of this work is to present stellar models for anisotropic matter distribution in the framework of f(T) gravity with torsion scalar T. In this regard, we use the interior geometry of Tolman-Kuchowicz spacetime having the potential components of the form ψ = Br2 + 2ln C and χ =ln(1 + ar2 + br4), where a, b, B and C are constants which have been evaluated with the aid of matching conditions on the surface of interior and exterior spacetimes. Off-diagonal tetrad is used to obtain the modified Field Equations (FEs). We use power law of f(T) gravity to get all the physical parameters such as principal stresses, density. We discuss anisotropy of the system and its effects on the system. The physical analysis is also presented by measuring speeds of sound, equilibrium conditions, energy conditions and redshift, etc. We choose some compact star models to present graphical description of the solution.
URI
http://hdl.handle.net/20.500.12627/1736
https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85100813147&origin=inward
https://doi.org/10.1142/s0219887821500602
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Creative Commons Lisansı

İstanbul Üniversitesi Akademik Arşiv Sistemi (ilgili içerikte aksi belirtilmediği sürece) Creative Commons Alıntı-GayriTicari-Türetilemez 4.0 Uluslararası Lisansı ile lisanslanmıştır.

DSpace software copyright © 2002-2016  DuraSpace
Contact Us | Send Feedback
Theme by 
Atmire NV