On the Hawking wormhole horizon entropy

Details On the Hawking wormhole horizon entropy On the Hawking wormhole horizon entropy

2004-09-07

arxiv.org/abs/hep-th/0409079v4

Physics

High Energy Physics

High Energy Physics - Theory

6 pages, typos corrected, revised version

Scientific paper

The entropy S of the horizon $theta = pi/2$ of the Hawking wormhole written in spherical Rindler coordinates is computed in this letter. Using Padmanabhan's prescription,we found that the surface gravity of the horizon equals the proper acceleration of the Rindler observer. S is a monotonic function of the radial coordinate $xi$ and vanishes when $xi$ equals the Planck length. In addition, its expression is similar with the Kaul - Majumdar one for the black hole entropy, including logarithmic corrections in quantum gravity scenarios.

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