Energy of a spherically symmetric charged dilaton black hole

1996/02/02 by A. Chamorro, K. S. Virbhadra, Chamorro, A. +1
Physics and Astronomy · #Astrophysics (astro-ph) #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #High Energy Physics - Theory (hep-th) #Relativity and Gravitational Theory #astro-ph #gr-qc #hep-th

paper · pdf · doi:10.48550/arxiv.gr-qc/9602005

3 pages, LaTex, Published in "Inhomogeneous Cosmological Models", (Eds. A Molina and J M M Senovilla, World Scientific, Singapore 1995), Pages 230-232

arxiv created 1996/02/02 · openalex publication_date 1996/02/02 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

The energy associated with a static and spherically symmetric charged dilaton black hole is obtained for arbitrary value of the coupling parameter (which regulates the strength of the coupling of the dilaton to the Maxwell field) β. The energy distribution depends on β, whereas the total energy is independent of this and is given by the mass parameter of the black hole.

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