Energy for accelerating observers in black hole spacetimes

被引:1
|
作者
Major, Seth A. [1 ]
机构
[1] Hamilton Coll, Dept Phys, Clinton, NY 13323 USA
关键词
QUASI-LOCAL ENERGY; LOCALIZATION; INTEGRALS; MASS;
D O I
10.1103/PhysRevD.105.104050
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Energies for constantly accelerating observers in Ba??ados, Teitelboim, and Zanelli; Schwarzschild; and Schwarzschild???de Sitter spacetimes are derived. The expressions are in terms of acceleration, cosmological constant, and area, quantities measurable by the observers. Based on results from quantum fields in curved spacetime for the redshifted Hawking temperature, quasilocal entropy and thermodynamic-like laws are briefly explored in the three spacetimes.
引用
收藏
页数:11
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