Explosion and Final State of an Unstable Reissner-Nordström Black Hole

Autor: Nicolas Sanchis-Gual, José A. Font, Pedro J. Montero, Carlos A. R. Herdeiro, Juan Carlos Degollado
Rok vydání: 2016
Předmět:
Zdroj: Physical Review Letters
Repositório Científico de Acesso Aberto de Portugal
Repositório Científico de Acesso Aberto de Portugal (RCAAP)
instacron:RCAAP
ISSN: 0031-9007
0044-4510
0038-5646
DOI: 10.1103/PhysRevLett.116.141101
Popis: A Reissner-Nordstr\"om black hole (BH) is superradiantly unstable against spherical perturbations of a charged scalar field, enclosed in a cavity, with frequency lower than a critical value. We use numerical relativity techniques to follow the development of this unstable system -- dubbed a charged BH bomb -- into the non-linear regime, solving the full Einstein--Maxwell--Klein-Gordon equations, in spherical symmetry. We show that: $i)$ the process stops before all the charge is extracted from the BH; $ii)$ the system settles down into a hairy BH: a charged horizon in equilibrium with a scalar field condensate, whose phase is oscillating at the (final) critical frequency. For low scalar field charge, $q$, the final state is approached smoothly and monotonically. For large $q$, however, the energy extraction overshoots and an explosive phenomenon, akin to a $bosenova$, pushes some energy back into the BH. The charge extraction, by contrast, does not reverse.
Comment: 5 pages, 4 figures; v2: 8 pages, including Supplemental Material; matches published version in Phys. Rev. Lett.; title changed
Databáze: OpenAIRE