Magnetic reconnection as a mechanism for energy extraction from rotating black holes

Luca Comisso, Felipe A. Asenjo

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

25 Citas (Scopus)

Resumen

Spinning black holes store rotational energy that can be extracted. When a black hole is immersed in an externally supplied magnetic field, reconnection of magnetic field lines within the ergosphere can generate negative energy (relative to infinity) particles that fall into the black hole event horizon while the other accelerated particles escape stealing energy from the black hole. We show analytically that energy extraction via magnetic reconnection is possible when the black hole spin is high (dimensionless spin a∼1) and the plasma is strongly magnetized (plasma magnetization σ0>1/3). The parameter space region where energy extraction is allowed depends on the plasma magnetization and the orientation of the reconnecting magnetic field lines. For σ0≫1, the asymptotic negative energy at infinity per enthalpy of the decelerated plasma that is swallowed by a maximally rotating black hole is found to be ϵ-∞≃-σ0/3. The accelerated plasma that escapes to infinity and takes away black hole energy asymptotes the energy at infinity per enthalpy ϵ+∞≃3σ0. We show that the maximum power extracted from the black hole by the escaping plasma is Pextrmax∼0.1M2σ0w0 (here, M is the black hole mass and w0 is the plasma enthalpy density) for the collisionless plasma regime and one order of magnitude lower for the collisional regime. Energy extraction causes a significant spindown of the black hole when a∼1. The maximum efficiency of the plasma energization process via magnetic reconnection in the ergosphere is found to be ηmax≃3/2. Since fast magnetic reconnection in the ergosphere should occur intermittently in the scenario proposed here, the associated emission within a few gravitational radii from the black hole is expected to display a bursty nature.

Idioma originalInglés
Número de artículo023014
PublicaciónPhysical Review D
Volumen103
N.º2
DOI
EstadoPublicada - 13 ene. 2021
Publicado de forma externa

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