The γ-rays that accompanied GW170817 and the observational signature of a magnetic jet breaking out of NS merger ejecta
Abstract
We present the first relativistic magnetohydrodynamics numerical simulation of a magnetic jet that propagates through and emerges from the dynamical ejecta of a binary neutron star merger. Generated by the magnetized rotation of the merger remnant, the jet propagates through the ejecta and produces an energetic cocoon that expands at mildly relativistic velocities and breaks out of the ejecta. We show that if the ejecta has a low-mass (~10-7 $$M_⊙$$) high-velocity ($$v$$ ~ 0.85c) tail, the cocoon shock breakout will generate γ-ray emission that is comparable to the observed short GRB170817A that accompanied the recent gravitational wave event GW170817. Thus, we propose that this gamma-ray burst (GRB), which is quite different from all other short GRBs observed before, was produced by a different mechanism. We expect, however, that such events are numerous and many will be detected in coming LIGO–Virgo runs.
- Authors:
-
- Tel Aviv Univ., Tel Aviv (Israel). The Raymond and Beverly Sackler School of Physics and Astronomy
- Northwestern Univ., Evanston, IL (United States). Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Dept. of Physics & Astronomy
- Hebrew Univ. of Jerusalem (Israel). Racah Inst. of Physics
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1526488
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 475; Journal Issue: 3; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Bromberg, O., Tchekhovskoy, A., Gottlieb, O., Nakar, E., and Piran, T. The γ-rays that accompanied GW170817 and the observational signature of a magnetic jet breaking out of NS merger ejecta. United States: N. p., 2017.
Web. doi:10.1093/mnras/stx3316.
Bromberg, O., Tchekhovskoy, A., Gottlieb, O., Nakar, E., & Piran, T. The γ-rays that accompanied GW170817 and the observational signature of a magnetic jet breaking out of NS merger ejecta. United States. https://doi.org/10.1093/mnras/stx3316
Bromberg, O., Tchekhovskoy, A., Gottlieb, O., Nakar, E., and Piran, T. Tue .
"The γ-rays that accompanied GW170817 and the observational signature of a magnetic jet breaking out of NS merger ejecta". United States. https://doi.org/10.1093/mnras/stx3316. https://www.osti.gov/servlets/purl/1526488.
@article{osti_1526488,
title = {The γ-rays that accompanied GW170817 and the observational signature of a magnetic jet breaking out of NS merger ejecta},
author = {Bromberg, O. and Tchekhovskoy, A. and Gottlieb, O. and Nakar, E. and Piran, T.},
abstractNote = {We present the first relativistic magnetohydrodynamics numerical simulation of a magnetic jet that propagates through and emerges from the dynamical ejecta of a binary neutron star merger. Generated by the magnetized rotation of the merger remnant, the jet propagates through the ejecta and produces an energetic cocoon that expands at mildly relativistic velocities and breaks out of the ejecta. We show that if the ejecta has a low-mass (~10-7 $M_⊙$) high-velocity ($v$ ~ 0.85c) tail, the cocoon shock breakout will generate γ-ray emission that is comparable to the observed short GRB170817A that accompanied the recent gravitational wave event GW170817. Thus, we propose that this gamma-ray burst (GRB), which is quite different from all other short GRBs observed before, was produced by a different mechanism. We expect, however, that such events are numerous and many will be detected in coming LIGO–Virgo runs.},
doi = {10.1093/mnras/stx3316},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 475,
place = {United States},
year = {Tue Dec 26 00:00:00 EST 2017},
month = {Tue Dec 26 00:00:00 EST 2017}
}
Web of Science
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