Spherically symmetric black-hole entropy without brick walls

Details Spherically symmetric black-hole entropy without brick walls Spherically symmetric black-hole entropy without brick walls

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cqgra..20.4885r&link_type=abstract

Classical and Quantum Gravity, Volume 20, Issue 22, pp. 4885-4890 (2003).

Physics

9

Scientific paper

Properties of the thermal radiation of black holes are discussed using a new equation of state density motivated by the generalized uncertainty relation in quantum gravity. There is no burst at the last stage of emission from a spherically symmetric black hole. When the new equation of state density is used to investigate the entropy of a bosonic field and fermionic field outside the horizon of a static spherically symmetric black hole, the divergence that appears in the brick-wall model is removed without any cutoff. The entropy proportional to the horizon area is derived from the contribution from the vicinity of the horizon.

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