Fluctuation around horizon on a Schwarzschild
black hole using the null geodesic method

doi:10.1007/s11467-009-0070-2

Front. Phys.

2009, Vol. 4

Issue (4) : 530-533 https://doi.org/10.1007/s11467-009-0070-2

Research articles

Fluctuation around horizon on a Schwarzschild black hole using the null geodesic method

Ji-li HUANG（黄基利）,Wen-biao LIU（刘文彪）,

Department of Physics, Institute of Theoretical Physics, Beijing Normal University, Beijing 100875, China;

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Abstract Using the null geodesic method, Hawking radiation from the horizon of a Schwarzschild black hole is calculated. The thermodynamics can be built successfully on the horizon where the apparent horizon and event horizon are coincident with each other. When a relativistic perturbation is given to the horizon, the first law of thermodynamics can also be constructed at a new supersurface near the horizon successfully. The expressions of the characteristic position and temperature are consistent with the previous result while the thermodynamics was built on the event horizon in a Vaidya black hole. Therefore, the thermodynamics of a dynamical black hole should be constructed on the apparent horizon exactly, and the event horizon thermodynamics is just one of the perturbations near the apparent horizon.

Keywords Hawking radiation thermodynamics dynamical black hole apparent horizon event horizon

Issue Date: 05 December 2009

Cite this article:

Ji-li HUANG（黄基利）,Wen-biao LIU（刘文彪）. Fluctuation around horizon on a Schwarzschild black hole using the null geodesic method[J]. Front. Phys. , 2009, 4(4): 530-533.

URL:

https://academic.hep.com.cn/fop/EN/10.1007/s11467-009-0070-2
https://academic.hep.com.cn/fop/EN/Y2009/V4/I4/530

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