首页|Energy exchange between charged relativistic fluids in f(T)gravity

Energy exchange between charged relativistic fluids in f(T)gravity

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This study focuses on the effects of a polytropic fluid on a charged gravitational source within f(T)gravity,where T is the torsion scalar.We investigate how the electromagnetic field affects the flow of energy in spherically symmetric and static celestial objects that contain relativistic fluids.By using the gravitational decoupling technique,we analyze the effects of polytropic fluid on the dynamics of the gravitational source,accompanied by the matching of the interior geometry with an exterior at the hypersurface Σ.Finally,with the help of the Tolman Ⅳsolution,we observe the conduct of energy conditions with the existence of charge using f(T)field equations and got the intended outcomes.

complexityhydrodynamicsanisotropyself-gravitating systemsenergy exchange

Z Yousaf、U A Khokhar、Nasser Bin Turki、T Suzuki

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Department of Mathematics,University of the Punjab,Quaid-i-Azam Campus,Lahore-54590,Pakistan

Department of Mathematics,College of Science,King Saud University,PO Box 2455,Riyadh,11451,Saudi Arabia

Department of Regional Management,Faculty of Management,Fukushima College,Fukushima 960-0181,Japan

King Saud University,Riyadh,Saudi Arabia

RSP2024R413

2024

理论物理通讯(英文版)
中国科学院理论物理研究所 中国物理学会

理论物理通讯(英文版)

CSTPCD
影响因子:0.333
ISSN:0253-6102
年,卷(期):2024.76(10)