Time evolving fluid from Vaidya spacetime

被引:0
|
作者
Wu, Bin [1 ,3 ,4 ]
Hao, Xin [2 ]
Zhao, Liu [2 ]
机构
[1] Northwest Univ Xian, Inst Modern Phys, Xian 710069, Shaanxi, Peoples R China
[2] Nankai Univ, Sch Phys, Tianjin 300071, Peoples R China
[3] Northwest Univ Xian, Sch Phys, Xian 710069, Shaanxi, Peoples R China
[4] Shaanxi Key Lab Theoret Phys Frontiers, Xian 710069, Shaanxi, Peoples R China
基金
中国国家自然科学基金;
关键词
BLACK-HOLES; VISCOSITY;
D O I
10.1103/PhysRevD.96.046010
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
' A time evolving fluid system is constructed on a timelike boundary hypersurface at finite cutoff in Vaidya spacetime. The approach used to construct the fluid equations is a direct extension of the ordinary gravity/fluid correspondence under the constrained fluctuation obeying Petrov type I conditions. The explicit relationships between the time dependent fluctuation modes and the fluid quantities such as density, velocity field and kinematic viscosity parameters are established, and the resulting fluid system is governed by a system of a sourced continuity equation and a compressible Navier-Stokes equation with nontrivial time evolution.
引用
收藏
页数:8
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