Stefan-Boltzmann's law of the Dirac field of static spherically symmetric black holes | Zendy

Meng Qing-miao | Zendy

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Stefan-Boltzmann's law of the Dirac field of static spherically symmetric black holes

Author(s) -

Meng Qing-miao

Publication year - 2003

Publication title -

acta physica sinica

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.199

H-Index - 47

ISSN - 1000-3290

DOI - 10.7498/aps.52.2102

Subject(s) - physics , event horizon , black hole (networking) , boltzmann constant , quartic function , nonsingular black hole models , entropy (arrow of time) , extremal black hole , mathematical physics , classical mechanics , charged black hole , quantum mechanics , spacetime , mathematics , computer network , routing protocol , routing (electronic design automation) , computer science , pure mathematics , link state routing protocol

Using the statistical entropy of the Dirac field of static spherically symmetric black hole, the Stefan-Boltzmann's law of static spherically symmetric black ho les is calculated, and we obtain a conclusion that the radiant emittance of a bl ack hole is proportionate to quartic power of temperature of the event horizon o f the black hole. It is found that the value of Stefan-Boltzmann constant in curved space-time is different from that in Euclidean space-time, and the constant has different value in different space-time.

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