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Dynamics of dissipative self-gravitating source in Rastall gravity
International Journal of Modern Physics A ( IF 1.6 ) Pub Date : 2021-07-13 , DOI: 10.1142/s0217751x21501530
M. Tahir 1 , G. Abbas 2 , Kazuharu Bamba 3 , M. R. Shahzad 4
Affiliation  

The dynamics of dissipative gravitational collapse of a source is explored in Rastall gravity. The field equations are derived for the geometry and collapsing matter. The dynamical equations are formulated for the heat flux and diffusion approximation. The heat transportation equation is derived by using Müller–Israel–Stewart approach to investigate the effects of heat flux on the collapsing source. Moreover, an equation is found by combining the dynamical and heat transport equation, the consequences of this equation are discussed in detail. Furthermore, the Rastall parameter λ effect is analyzed for the collapse of sphere.

中文翻译:

Rastall 引力中耗散自引力源的动力学

在 Rastall 引力中探讨了源耗散引力坍缩的动力学。为几何和坍缩物质推导出场方程。动力学方程是为热通量和扩散近似制定的。通过使用 Müller-Israel-Stewart 方法来研究热通量对塌陷源的影响,推导出热传输方程。此外,通过结合动力和热传输方程找到了一个方程,并详细讨论了该方程的结果。此外,Rastall 参数λ分析球体坍塌的影响。
更新日期:2021-07-13
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