Vaidya spacetime in Brans-Dicke gravity's rainbow

被引:7
作者
Rudra, Prabir [1 ]
Maity, Sayani [2 ]
机构
[1] Asutosh Coll, Dept Math, Kolkata 700026, India
[2] Techno India Salt Lake, Dept Math, Sect 5, Kolkata 700091, India
来源
EUROPEAN PHYSICAL JOURNAL C | 2018年 / 78卷 / 10期
关键词
BLACK-HOLE; GRAVITATIONAL COLLAPSE; THERMAL FLUCTUATIONS; INHOMOGENEOUS DUST; HAWKING RADIATION; QUANTUM-GRAVITY; THERMODYNAMICS; SINGULARITIES; SATURN; TIME;
D O I
10.1140/epjc/s10052-018-6304-0
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
In this note we study an energy dependent deformation of a time dependent geometry in the background of Brans-Dicke gravity theory. The study is performed using the gravity's rainbow formalism. We compute the field equations in Brans-Dicke gravity's rainbow using Vaidya metric which is a time dependent geometry. We study a star collapsing under such conditions. Our prime objective is to determine the nature of singularity formed as a result of gravitational collapse and its strength. The idea is to test the validity of the cosmic censorship hypothesis for our model. We have also studied the effect of such a deformation on the thermalization process. In this regard we have calculated the important thermodynamical quantities such as thermalization temperature, Helmholtz free energy, specific heat and analyzed the behavior of such quantities.
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页数:13
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