4-dimensional dilaton black holes with cosmological constant
Tadashi Okai

TL;DR
This paper investigates static, spherically symmetric dilaton black hole solutions with a cosmological constant, deriving a power series solution and analyzing the maximum number of horizons, revealing notable differences from known Reissner-Nordström-de Sitter black holes.
Contribution
It provides a formal power series solution for dilaton black holes with cosmological constant and proves bounds on the number of horizons, highlighting differences from classical solutions.
Findings
Maximum of 2 horizons for positive cosmological constant
Maximum of 1 horizon for negative cosmological constant
Contrast with Reissner-Nordström-de Sitter black holes with 3 horizons
Abstract
Static and spherically symmetric black hole solutions with non-zero cosmological constant are investigated. A formal power series solution is found. It is proved that the number of regular horizons is less than or equal to 2 for positive cosmological constant and is less than or equal to 1 for negative cosmological constant. This shows a striking contrast to the fact that the Reissner-Nordstr{\o}m-de Sitter black hole with positive cosmological horizon has 3 regular horizons.
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Taxonomy
TopicsRelativity and Gravitational Theory · Black Holes and Theoretical Physics · Cosmology and Gravitation Theories
