The quantum horizon of the Garfinkle—Horowitz—Strominger dilatonic blackhole

Details The quantum horizon of the Garfinkle—Horowitz—Strominger dilatonic blackhole The quantum horizon of the Garfinkle—Horowitz—Strominger dilatonic blackhole

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006gregr..38..963g&link_type=abstract

General Relativity and Gravitation, Volume 38, Issue 5, pp.963-970

Computer Science

4

Quantum States, Brown&Mdash, York'S Quasi-Local Gravitational Energy, Hawking Temperature

Scientific paper

Treating macro-black hole as quantum states, and using Brown York's quasi-local gravitational energy definition and Heisenberg uncertainty principle, the GHS black hole's quantum horizon is constructed. The Hawking temperature is computed naturally, and the entropy can also be figured out without introducing the cutoff factor h. The Φ-field mode number is predicted too. The result is consistent with that of the Schwarzschild and R-N black hole.

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