Class I stars in the background of \(f(T, \tau)\) cosmological model
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Publication:6542208
DOI10.1016/J.CJPH.2021.12.029zbMATH Open1539.83122MaRDI QIDQ6542208
M. Zubair, Francisco Tello-Ortiz, Allah Ditta, Saira Waheed
Publication date: 21 May 2024
Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
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- Über das Gravitationsfeld einer Kugel aus inkompressibler Flüssigkeit nach der \textit{Einstein}schen Theorie.
- Two diverse models of embedding class one
- The stability of relativistic stars and the role of the adiabatic index
- Study of gravastars under \(f(\mathbb{T})\) gravity
- Existence of relativistic stars in f ( T ) gravity
- Anisotropic stars in general relativity
- Energy conditions in f ( R , L m ) gravity
- ANISOTROPIC COMPACT STARS WITH VARIABLE COSMOLOGICAL CONSTANT
- All static spherically symmetric anisotropic solutions for general relativistic polytropes
- Rotating AdS black holes in Maxwell- f ( T ) gravity
- Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- On Massive Neutron Cores
- Riemannian geometry.
Related Items (2)
A study of bouncing cosmology in framework of \(f(T, \mathcal{T})\) gravity with probing of cosmographic parameters ⋮ Comparative analysis of dark energy compact stars in \(f(T, \mathcal{T})\) and \(f(T)\) gravity theories via conformally flat condition
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