Possible role of magnetic reconnection in the electromagnetic counterpart of binary black hole merger
arXiv:1603.01950 · doi:10.1088/1475-7516/2018/04/054
Abstract
We propose a qualitative scenario to interpret the argued association between the direct measurement of the gravitational wave event GW150914 by Laser Interferometer Gravitational Wave Observatory (LIGO)-Virgo collaborations and the hard -ray transient detected by Fermi-Gamma-ray Burst Monitor (GBM) sec after. In a binary system of two gravitationally collapsing objects with a non-vanishing electric charge, the compenetration of the two magnetospheres occurring during the coalescence, through magnetic reconnection, produces a highly collimated relativistic outflow that becomes optically thin and shines in the GBM field of view. We propose that this process should be expected as a commonplace in the future joint gravitational/electromagnetic detections and, in case of neutron star-neutron star merger event, might lead to detectable - or -ray precursors to, or transients associated with, the gravitational bursts.
8 pages; 1 figure. JCAP, in press
References in corpus (11)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- The Physics of Gamma-Ray Bursts and Relativistic Jets
- Astrophysical Implications of the Binary Black-Hole Merger GW150914
- Fermi GBM Observations of LIGO Gravitational Wave event GW150914
- Electromagnetic Counterparts to Black Hole Mergers Detected by LIGO
- Short Gamma-Ray Bursts from the Merger of Two Black Holes
- Mergers of Charged Black Holes: Gravitational Wave Events, Short Gamma-Ray Bursts, and Fast Radio Bursts
- Relativistic magnetic reconnection in pair plasmas and its astrophysical applications
- Stellar explosions powered by the Blandford-Znajek mechanism
- Accurate Simulations of Binary Black-Hole Mergers in Force-Free Electrodynamics
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- Charged Compact Binary Coalescence Signal and Electromagnetic Counterpart of Plunging BH-NS mergers
- Analysis of Sub-threshold Short Gamma-ray Bursts in Fermi GBM Data
- Limits on electromagnetic counterparts of gravitational wave-detected binary black hole mergers
- On neutralization of charged black holes
- A First Search for Prompt Radio Emission from a Gravitational-Wave Event
- Initial data for general relativistic simulations of multiple electrically charged black holes with linear and angular momenta
- Merger estimates for Kerr-Sen black holes
- H.E.S.S. follow-up observations of Binary Black Hole Coalescence events during the second and third Gravitational Waves observing runs of Advanced LIGO and Advanced Virgo
- Strongly lensed gravitational waves as the probes to test the cosmic distance duality relation
- Electromagnetic Emission post Spinning Black Hole-Magnetized Neutron Star Mergers
- The cosmological distribution of compact object mergers from dynamical interactions with SMBH binaries
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