Energy Extraction via Magnetic Reconnection in the Ergosphere of a rotating non-Kerr Black Hole
arXiv:2204.07338 · doi:10.3847/1538-4357/ac3de3
Abstract
Magnetic reconnection process in the ergosphere is investigated for a relativistic plasma around a rotating non-Kerr black hole. For a rotating non-Kerr black hole immersed in magnetic field generated by an externally material, anti-parallel magnetic field line could form in the ergosphere due to the frame dragging. Therefore, magnetic reconnection could occur in the ergosphere. Such magnetic reconnection may generate negative energy at infinity by redistributing the angular momentum during the process. The results show that, with the effect of the deformed parameter, extraction of energy from a rotating non-Kerr black hole by magnetic reconnection could be enhanced in the presence of a positive deformed parameter.
arXiv comment7 pages, 4 figures. Published in ApJ
References in corpus (40)
- Collapsars - Gamma-Ray Bursts and Explosions in "Failed Supernovae"
- First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
- First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon
- A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair Theorem
- Apparent shape of super-spinning black holes
- Fast variability of TeV gamma-rays from the radio galaxy M 87
- Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes
- High-resolution magnetohydrodynamics simulation of black hole-neutron star merger: Mass ejection and short gamma-ray burst
- Constraining the quadrupole moment of stellar-mass black-hole candidates with the continuum fitting method
- Imaging Bright Spots in the Accretion Flow Near the Black Hole Horizon of Sgr A*
- On The Nature of the Variable Infrared Emission from Sgr A*
- A code to compute the emission of thin accretion disks in non-Kerr space-times and test the nature of black hole candidates
- Measurement of the spin of the M87 black hole from its observed twisted light
- Testing the space-time geometry around black hole candidates with the analysis of the broad K iron line
- A powerful flare from Sgr A* confirms the synchrotron nature of the X-ray emission
- Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum. III. Quasi-Periodic Variability
- Testing the No-Hair Theorem with Observations in the Electromagnetic Spectrum: I. Properties of a Quasi-Kerr Spacetime
- How to observe a non-Kerr spacetime
- An observable signature of a background deviating from Kerr
- Time Dependent Models of Flares from Sagittarius A*
- Tests of General Relativity in the Strong Gravity Regime Based on X-Ray Spectropolarimetric Observations of Black Holes in X-Ray Binaries
- Particle Acceleration and the Origin of X-ray Flares in GRMHD simulations of Sgr A*
- Testing the Kerr-nature of stellar-mass black hole candidates by combining the continuum-fitting method and the power estimate of transient ballistic jets
- Spinning Loop Black Holes
- Magnetic Reconnection as a Mechanism for Energy Extraction from Rotating Black Holes
- Reconnection in Marginally Collisionless Accretion Disk Coronae
- VERITAS Observations of day-scale flaring of M87 in 2010 April
- Energy Extraction from a Rotating Black Hole by Magnetic Reconnection in Ergosphere
- VERITAS 2008 - 2009 monitoring of the variable gamma-ray source M87
- Effects of spin on magnetized binary neutron star mergers and jet launching
- Attempt to find a correlation between the spin of stellar-mass black hole candidates and the power of steady jets: relaxing the Kerr black hole hypothesis
- Strong gravitational lensing by a rotating non-Kerr compact object
- Constraint on the quadrupole moment of super-massive black hole candidates from the estimate of the mean radiative efficiency of AGN
- Can an astrophysical black hole have a topologically non-trivial event horizon?
- Variations in emission from episodic plasmoid ejecta around black holes
- Properties of a thin accretion disk around a rotating non-Kerr black hole
- A magnetohydrodynamic model for multi-wavelength flares from Sagittarius~A (I): model and the near-infrared and X-ray flares
- Rotating non-Kerr black hole and energy extraction
- Horizon-Penetrating Transonic Accretion Disks around Rotating Black Holes
- A nonthermal bomb explains the near-infrared superflare of Sgr A*
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