arXiv Analytics

Sign in

arXiv:hep-th/0302170AbstractReferencesReviewsResources

Black Hole Entropy from a Highly Excited Elementary String

Romesh K. Kaul

Published 2003-02-21Version 1

Suggested correspondence between a black hole and a highly excited elementary string is explored. Black hole entropy is calculated by computing the density of states for an open excited string. We identify the square root of oscillator number of the excited string with Rindler energy of black hole to obtain an entropy formula which, not only agrees at the leading order with the Bekenstein-Hawking entropy, but also reproduces the logarithmic correction obtained for black hole entropy in the quantum geometry framework. This provides an additional supporting evidence for correspondence between black holes and strings.

Related articles: Most relevant | Search more
arXiv:hep-th/0611141 (Published 2006-11-14, updated 2006-11-21)
Black Hole Entropy in the presence of Chern-Simons Terms
arXiv:hep-th/9706065 (Published 1997-06-10)
Electromagnetic fields in Schwarzschild and Reissner-Nordström geometry. Quantum corrections to the black hole entropy
arXiv:hep-th/0111224 (Published 2001-11-25, updated 2002-04-12)
The Hamiltonian Dynamics of Bounded Spacetime and Black Hole Entropy: The Canonical Method