The landscape of disc outflows from black hole–neutron star mergers
Abstract
We investigate mass ejection from accretion discs formed in mergers of black holes (BHs) and neutron stars (NSs). The third observing run of the LIGO/Virgo interferometers provided BH–NS candidate events that yielded no electromagnetic (EM) counterparts. The broad range of disc configurations expected from BH–NS mergers motivates a thorough exploration of parameter space to improve EM signal predictions. Here we conduct 27 high-resolution, axisymmetric, long-term hydrodynamic simulations of the viscous evolution of BH accretion discs that include neutrino emission/absorption effects and post-processing with a nuclear reaction network. In the absence of magnetic fields, these simulations provide a lower limit to the fraction of the initial disc mass ejected. We find a nearly linear inverse dependence of this fraction on disc compactness (BH mass over initial disc radius). The dependence is related to the fraction of the disc mass accreted before the ouflow is launched, which depends on the disc position relative to the innermost stable circular orbit. We also characterize a trend of decreasing ejected fraction and decreasing lanthanide/actinide content with increasing disc mass at fixed BH mass. Furthermore, this trend results from a longer time to reach weak freezout and an increasingly dominant role of neutrino absorption at highermore »
- Authors:
-
- Department of Physics, University of Alberta, Edmonton, AB T6G 2E1, Canada
- Department of Physics and Astronomy, University of New Hampshire, Durham, NH 03824, USA
- CCS-2, Los Alamos National Laboratory, Los Alamos, NM 87545, USA, Center for Theoretical Astrophysics, Los Alamos National Laboratory, Los Alamos, NM 87545, USA
- Publication Date:
- Research Org.:
- Univ. of New Hampshire, Durham, NH (United States); Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP); National Science Foundation (NSF); National Aeronautics and Space Administration (NASA)
- OSTI Identifier:
- 1647478
- Alternate Identifier(s):
- OSTI ID: 1681208; OSTI ID: 1784949; OSTI ID: 1844131
- Report Number(s):
- LA-UR-20-23877
Journal ID: ISSN 0035-8711
- Grant/Contract Number:
- SC0020435; PHY-1806278; 80NSSC18K0565; AC02-05CH11231; 89233218CNA000001
- Resource Type:
- Published Article
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 497 Journal Issue: 3; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United Kingdom
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Accretion; accretion discs; dense matter; gravitational waves; hydrodynamics; neutrinos; nuclear reactions; nucleosynthesis; abundances
Citation Formats
Fernández, Rodrigo, Foucart, Francois, and Lippuner, Jonas. The landscape of disc outflows from black hole–neutron star mergers. United Kingdom: N. p., 2020.
Web. doi:10.1093/mnras/staa2209.
Fernández, Rodrigo, Foucart, Francois, & Lippuner, Jonas. The landscape of disc outflows from black hole–neutron star mergers. United Kingdom. https://doi.org/10.1093/mnras/staa2209
Fernández, Rodrigo, Foucart, Francois, and Lippuner, Jonas. Tue .
"The landscape of disc outflows from black hole–neutron star mergers". United Kingdom. https://doi.org/10.1093/mnras/staa2209.
@article{osti_1647478,
title = {The landscape of disc outflows from black hole–neutron star mergers},
author = {Fernández, Rodrigo and Foucart, Francois and Lippuner, Jonas},
abstractNote = {We investigate mass ejection from accretion discs formed in mergers of black holes (BHs) and neutron stars (NSs). The third observing run of the LIGO/Virgo interferometers provided BH–NS candidate events that yielded no electromagnetic (EM) counterparts. The broad range of disc configurations expected from BH–NS mergers motivates a thorough exploration of parameter space to improve EM signal predictions. Here we conduct 27 high-resolution, axisymmetric, long-term hydrodynamic simulations of the viscous evolution of BH accretion discs that include neutrino emission/absorption effects and post-processing with a nuclear reaction network. In the absence of magnetic fields, these simulations provide a lower limit to the fraction of the initial disc mass ejected. We find a nearly linear inverse dependence of this fraction on disc compactness (BH mass over initial disc radius). The dependence is related to the fraction of the disc mass accreted before the ouflow is launched, which depends on the disc position relative to the innermost stable circular orbit. We also characterize a trend of decreasing ejected fraction and decreasing lanthanide/actinide content with increasing disc mass at fixed BH mass. Furthermore, this trend results from a longer time to reach weak freezout and an increasingly dominant role of neutrino absorption at higher disc masses. We estimate the radioactive luminosity from the disc outflow alone available to power kilonovae over the range of configurations studied, finding a spread of two orders of magnitude. For most of the BH–NS parameter space, the disc outflow contribution is well below the kilonova mass upper limits for GW190814.},
doi = {10.1093/mnras/staa2209},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 3,
volume = 497,
place = {United Kingdom},
year = {Tue Jul 28 00:00:00 EDT 2020},
month = {Tue Jul 28 00:00:00 EDT 2020}
}
https://doi.org/10.1093/mnras/staa2209
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