Equation-of-state Dependence of Gravitational Waves in Core-collapse Supernovae
Abstract
Gravitational waves (GWs) provide unobscured insight into the birthplace of neutron stars and black holes in core-collapse supernovae (CCSNe). The nuclear equation of state (EOS) describing these dense environments is yet uncertain, and variations in its prescription affect the proto-neutron star (PNS) and the post-bounce dynamics in CCSN simulations, subsequently impacting the GW emission. In this study, we perform axisymmetric simulations of CCSNe with Skyrme-type EOSs to study how the GW signal and PNS convection zone are impacted by two experimentally accessible EOS parameters, (1) the effective mass of nucleons, m*, which is crucial in setting the thermal dependence of the EOS, and (2) the isoscalar incompressibility modulus, Ksat. While Ksat shows little impact, the peak frequency of the GWs has a strong effective mass dependence due to faster contraction of the PNS for higher values of m* owing to a decreased thermal pressure. These more compact PNSs also exhibit more neutrino heating, which drives earlier explosions and correlates with the GW amplitude via accretion plumes striking the PNS, exciting the oscillations. We investigate the spatial origin of the GWs and show the agreement between a frequency-radial distribution of the GW emission and a perturbation analysis. We do not rulemore »
- Authors:
-
[1];
[1];
[1];
[1];
[2];
[1]
- Stockholm Univ. (Sweden)
- Michigan State Univ., East Lansing, MI (United States)
- Publication Date:
- Research Org.:
- Michigan State Univ., East Lansing, MI (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP); USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR). Scientific Discovery through Advanced Computing (SciDAC); Swedish Research Council (SRC)
- OSTI Identifier:
- 1981233
- Grant/Contract Number:
- SC0015904; SC0017955; 2016-07213
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal
- Additional Journal Information:
- Journal Volume: 923; Journal Issue: 2; Journal ID: ISSN 0004-637X
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; astronomy; astrophysics
Citation Formats
Eggenberger Andersen, Oliver, Zha, Shuai, da Silva Schneider, André, Betranhandy, Aurore, Couch, Sean M., and O’Connor, Evan P. Equation-of-state Dependence of Gravitational Waves in Core-collapse Supernovae. United States: N. p., 2021.
Web. doi:10.3847/1538-4357/ac294c.
Eggenberger Andersen, Oliver, Zha, Shuai, da Silva Schneider, André, Betranhandy, Aurore, Couch, Sean M., & O’Connor, Evan P. Equation-of-state Dependence of Gravitational Waves in Core-collapse Supernovae. United States. https://doi.org/10.3847/1538-4357/ac294c
Eggenberger Andersen, Oliver, Zha, Shuai, da Silva Schneider, André, Betranhandy, Aurore, Couch, Sean M., and O’Connor, Evan P. Wed .
"Equation-of-state Dependence of Gravitational Waves in Core-collapse Supernovae". United States. https://doi.org/10.3847/1538-4357/ac294c. https://www.osti.gov/servlets/purl/1981233.
@article{osti_1981233,
title = {Equation-of-state Dependence of Gravitational Waves in Core-collapse Supernovae},
author = {Eggenberger Andersen, Oliver and Zha, Shuai and da Silva Schneider, André and Betranhandy, Aurore and Couch, Sean M. and O’Connor, Evan P.},
abstractNote = {Gravitational waves (GWs) provide unobscured insight into the birthplace of neutron stars and black holes in core-collapse supernovae (CCSNe). The nuclear equation of state (EOS) describing these dense environments is yet uncertain, and variations in its prescription affect the proto-neutron star (PNS) and the post-bounce dynamics in CCSN simulations, subsequently impacting the GW emission. In this study, we perform axisymmetric simulations of CCSNe with Skyrme-type EOSs to study how the GW signal and PNS convection zone are impacted by two experimentally accessible EOS parameters, (1) the effective mass of nucleons, m*, which is crucial in setting the thermal dependence of the EOS, and (2) the isoscalar incompressibility modulus, Ksat. While Ksat shows little impact, the peak frequency of the GWs has a strong effective mass dependence due to faster contraction of the PNS for higher values of m* owing to a decreased thermal pressure. These more compact PNSs also exhibit more neutrino heating, which drives earlier explosions and correlates with the GW amplitude via accretion plumes striking the PNS, exciting the oscillations. We investigate the spatial origin of the GWs and show the agreement between a frequency-radial distribution of the GW emission and a perturbation analysis. We do not rule out overshoot from below via PNS convection as another moderately strong excitation mechanism in our simulations. We also study the combined effect of effective mass and rotation. In all our simulations we find evidence for a power gap near ~1250 Hz; we investigate its origin and report its EOS dependence.},
doi = {10.3847/1538-4357/ac294c},
journal = {The Astrophysical Journal},
number = 2,
volume = 923,
place = {United States},
year = {Wed Dec 22 00:00:00 EST 2021},
month = {Wed Dec 22 00:00:00 EST 2021}
}
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