On the gravitational energy of the Hawking wormhole

Details On the gravitational energy of the Hawking wormhole On the gravitational energy of the Hawking wormhole

2002-09-10

arxiv.org/abs/hep-th/0209083v3

Int.J.Mod.Phys. A18 (2003) 4251-4256

Physics

High Energy Physics

High Energy Physics - Theory

9 pages, chapter 4 removed, to appear in Int. Jour. Mod. Phys. A

Scientific paper

10.1142/S0217751X03016124

The surface energy for a conformally flat spacetime which represents the Hawking wormhole in spherical (static) Rindler coordinates is computed using the Hawking - Hunter formalism for non asymptotically - flat spacetimes. The physical gravitational Hamiltonian is proportional to the Rindler acceleration g of the hyperbolic observer and is finite on the event horizon ksi = b (b-the Planck length, ksi - the Minkowski interval). The corresponding temperature of the system of particles associated to the massless scalar field Psi, coupled conformally to Einstein's equations, is given by the Davies - Unruh temperature up to a constant factor of order unity.

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