Dilatonic interpolation between Reissner-Nordstrom and Bertotti-Robinson spacetimes with physical consequences

Abstract

We give a general class of static, spherically symmetric, non-asymptotically flat and asymptotically non-(anti) de Sitter black hole solutions in Einstein-Maxwell-Dilaton (EMD) theory of gravity in 4-dimensions. In this general study we couple a magnetic Maxwell field with a general dilaton potential, while double Liouville-type potentials are coupled with the gravity. We show that the dilatonic parameters play the key role in switching between the Bertotti-Robinson and Reissner-Nordström spacetimes. We study the stability of such black holes under a linear radial perturbation, and in this sense we find exceptional cases that the EMD black holes are unstable. In continuation we give a detailed study of the spin-weighted harmonics in dilatonic Hawking radiation spectrum and compare our results with the previously known ones. Finally, we investigate the status of resulting naked singularities of our general solution when probed with quantum test particles.

27 pages, 4 figures, to appear in CQG.

References in corpus (4)

• Hawking radiation of linear dilaton black holes
• Black Hole solutions in Einstein-Maxwell-Yang-Mills-Gauss-Bonnet Theory
• Quantum Singularities in Spacetimes with Spherical and Cylindrical Topological Defects
• Black Holes in Models with Dilaton Field and Electric or Electric and Magnetic Charges

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