Black Hole Entropy Calculation in a Modified Thin Film Model

Details Black Hole Entropy Calculation in a Modified Thin Film Model Black Hole Entropy Calculation in a Modified Thin Film Model

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011japa...32..323z&link_type=abstract

Journal of Astrophysics and Astronomy, Volume 32, Issue 1-2, pp. 323-325

Astronomy and Astrophysics

Astrophysics

Black Hole Entropy, Thin Film Model, Tunnelling Framework, Self-Gravitation., Black Hole Entropy—Thin Film Model—Tunnelling Framework—Self-Gravitation.

Scientific paper

The thin film model is modified to calculate the black hole entropy. The difference from the original method is that the Parikh-Wilczek tunnelling framework is introduced and the self-gravitation of the emission particles is taken into account. In terms of our improvement, if the entropy is still proportional to the area, then the emission energy of the particles will satisfy ω = T/360.

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