Gravitational Wave Eigenfrequencies from Neutrino-driven Core-collapse Supernovae
Abstract
Abstract Core-collapse supernovae (CCSNe) are predicted to produce gravitational waves (GWs) that may be detectable by Advanced LIGO/Virgo. These GW signals carry information from the heart of these cataclysmic events, where matter reaches nuclear densities. Recent studies have shown that it may be possible to infer the properties of the proto-neutron star (PNS) via GWs generated by hydrodynamic perturbations of the PNS. However, we lack a comprehensive understanding of how these relationships may change with the properties of CCSNe. In this work, we build a self-consistent suite of over 1000 exploding CCSNe from a grid of progenitor masses and metallicities combined with six different nuclear equations of state (EOS). Performing a linear perturbation analysis on each model, we compute the resonant GW frequencies of the PNS, and we motivate a time-agnostic method for identifying characteristic frequencies of the dominant GW emission. From this, we identify two characteristic frequencies, of the early- and late-time signal, that measure the surface gravity of the cold remnant neutron star, and simultaneously constrain the hot nuclear EOS. However, we find that the details of the CCSN model, such as the treatment of gravity or the neutrino transport, and whether it explodes, noticeably change the magnitudemore »
- Publication Date:
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1998001
- Grant/Contract Number:
- FG02-02ER41216
- Resource Type:
- Published Article
- Journal Name:
- The Astrophysical Journal
- Additional Journal Information:
- Journal Name: The Astrophysical Journal Journal Volume: 954 Journal Issue: 2; Journal ID: ISSN 0004-637X
- Publisher:
- American Astronomical Society
- Country of Publication:
- United States
- Language:
- English
Citation Formats
Wolfe, Noah E., Fröhlich, Carla, Miller, Jonah M., Torres-Forné, Alejandro, and Cerdá-Durán, Pablo. Gravitational Wave Eigenfrequencies from Neutrino-driven Core-collapse Supernovae. United States: N. p., 2023.
Web. doi:10.3847/1538-4357/ace693.
Wolfe, Noah E., Fröhlich, Carla, Miller, Jonah M., Torres-Forné, Alejandro, & Cerdá-Durán, Pablo. Gravitational Wave Eigenfrequencies from Neutrino-driven Core-collapse Supernovae. United States. https://doi.org/10.3847/1538-4357/ace693
Wolfe, Noah E., Fröhlich, Carla, Miller, Jonah M., Torres-Forné, Alejandro, and Cerdá-Durán, Pablo. Mon .
"Gravitational Wave Eigenfrequencies from Neutrino-driven Core-collapse Supernovae". United States. https://doi.org/10.3847/1538-4357/ace693.
@article{osti_1998001,
title = {Gravitational Wave Eigenfrequencies from Neutrino-driven Core-collapse Supernovae},
author = {Wolfe, Noah E. and Fröhlich, Carla and Miller, Jonah M. and Torres-Forné, Alejandro and Cerdá-Durán, Pablo},
abstractNote = {Abstract Core-collapse supernovae (CCSNe) are predicted to produce gravitational waves (GWs) that may be detectable by Advanced LIGO/Virgo. These GW signals carry information from the heart of these cataclysmic events, where matter reaches nuclear densities. Recent studies have shown that it may be possible to infer the properties of the proto-neutron star (PNS) via GWs generated by hydrodynamic perturbations of the PNS. However, we lack a comprehensive understanding of how these relationships may change with the properties of CCSNe. In this work, we build a self-consistent suite of over 1000 exploding CCSNe from a grid of progenitor masses and metallicities combined with six different nuclear equations of state (EOS). Performing a linear perturbation analysis on each model, we compute the resonant GW frequencies of the PNS, and we motivate a time-agnostic method for identifying characteristic frequencies of the dominant GW emission. From this, we identify two characteristic frequencies, of the early- and late-time signal, that measure the surface gravity of the cold remnant neutron star, and simultaneously constrain the hot nuclear EOS. However, we find that the details of the CCSN model, such as the treatment of gravity or the neutrino transport, and whether it explodes, noticeably change the magnitude and evolution of the PNS eigenfrequencies.},
doi = {10.3847/1538-4357/ace693},
journal = {The Astrophysical Journal},
number = 2,
volume = 954,
place = {United States},
year = {Mon Sep 04 00:00:00 EDT 2023},
month = {Mon Sep 04 00:00:00 EDT 2023}
}
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