Conserved masses in GHS Einstein and string black holes

Details Conserved masses in GHS Einstein and string black holes Conserved masses in GHS Einstein and string black holes

1996-04-29

arxiv.org/abs/gr-qc/9604055v1

Phys.Rev. D54 (1996) 3892-3899

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

16 pages REVTeX with packages amsfonts and amssymb

Scientific paper

10.1103/PhysRevD.54.3892

We analyze the relationship between quasilocal masses calculated for solutions of conformally related theories. We show that the ADM mass of a static, spherically symmetric solution is conformally invariant (up to a constant factor) only if the background action functional is conformally invariant. Thus, the requirement of conformal invariance places restrictions on the choice of reference spacetimes. We calculate the mass of the black hole solutions obtained by Garfinkle, Horowitz, and Strominger (GHS) for both the string and the Einstein metrics. In addition, the quasilocal thermodynamic quantities in the string metrics are computed and discussed.

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