Constraining Properties of the Next Nearby Core-collapse Supernova with Multimessenger Signals
Abstract
With the advent of modern neutrino and gravitational wave (GW) detectors, the promise of multimessenger detections of the next galactic core-collapse supernova (CCSN) has become very real. Such detections will give insight into the CCSN mechanism and the structure of the progenitor star, and may resolve longstanding questions in fundamental physics. In order to properly interpret these detections, a thorough understanding of the landscape of possible CCSN events, and their multimessenger signals, is needed. We present detailed predictions of neutrino and GW signals from 1D simulations of stellar core collapse, spanning the landscape of core-collapse progenitors from 9 to 120 M⊙. In order to achieve explosions in 1D, we use the Supernova Turbulence In Reduced-dimensionality model, which includes the effects of turbulence and convection in 1D supernova simulations to mimic the 3D explosion mechanism. We study the GW emission from the 1D simulations using an astroseismology analysis of the protoneutron star. We find that the neutrino and GW signals are strongly correlated with the structure of the progenitor star and remnant compact object. Using these correlations, future detections of the first few seconds of neutrino and GW emission from a galactic CCSN may be able to provide constraints on stellarmore »
- Authors:
-
[1];
[2];
[3];
[4]
- North Carolina State Univ., Raleigh, NC (United States). Dept. of Physics; Michigan State Univ., East Lansing, MI (United States). Dept. of Physics and Astronomy. Joint Inst. for Nuclear Astrophysics. Center for the Evolution of the Elements
- Michigan State Univ., East Lansing, MI (United States). Dept. of Physics and Astronomy. Joint Inst. for Nuclear Astrophysics. Center for the Evolution of the Elements. Dept. of Computational Mathematics, Science, and Engineering. National Superconducting Cyclotron Lab.
- Stockholm Univ. (Sweden). Dept. of Astronomy. Oskar Klein Centre
- Pennsylvania State Univ., University Park, PA (United States). Dept. of Physics
- Publication Date:
- Research Org.:
- Michigan State Univ., East Lansing, MI (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP)
- OSTI Identifier:
- 1802779
- Grant/Contract Number:
- SC0015904; SC0017955
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 898; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; core-collapse supernovae; gravitational wave astronomy; gravitational wave sources; neutrino astronomy; supernova neutrinos
Citation Formats
Warren, MacKenzie L., Couch, Sean M., O’Connor, Evan P., and Morozova, Viktoriya. Constraining Properties of the Next Nearby Core-collapse Supernova with Multimessenger Signals. United States: N. p., 2020.
Web. doi:10.3847/1538-4357/ab97b7.
Warren, MacKenzie L., Couch, Sean M., O’Connor, Evan P., & Morozova, Viktoriya. Constraining Properties of the Next Nearby Core-collapse Supernova with Multimessenger Signals. United States. https://doi.org/10.3847/1538-4357/ab97b7
Warren, MacKenzie L., Couch, Sean M., O’Connor, Evan P., and Morozova, Viktoriya. Fri .
"Constraining Properties of the Next Nearby Core-collapse Supernova with Multimessenger Signals". United States. https://doi.org/10.3847/1538-4357/ab97b7. https://www.osti.gov/servlets/purl/1802779.
@article{osti_1802779,
title = {Constraining Properties of the Next Nearby Core-collapse Supernova with Multimessenger Signals},
author = {Warren, MacKenzie L. and Couch, Sean M. and O’Connor, Evan P. and Morozova, Viktoriya},
abstractNote = {With the advent of modern neutrino and gravitational wave (GW) detectors, the promise of multimessenger detections of the next galactic core-collapse supernova (CCSN) has become very real. Such detections will give insight into the CCSN mechanism and the structure of the progenitor star, and may resolve longstanding questions in fundamental physics. In order to properly interpret these detections, a thorough understanding of the landscape of possible CCSN events, and their multimessenger signals, is needed. We present detailed predictions of neutrino and GW signals from 1D simulations of stellar core collapse, spanning the landscape of core-collapse progenitors from 9 to 120 M⊙. In order to achieve explosions in 1D, we use the Supernova Turbulence In Reduced-dimensionality model, which includes the effects of turbulence and convection in 1D supernova simulations to mimic the 3D explosion mechanism. We study the GW emission from the 1D simulations using an astroseismology analysis of the protoneutron star. We find that the neutrino and GW signals are strongly correlated with the structure of the progenitor star and remnant compact object. Using these correlations, future detections of the first few seconds of neutrino and GW emission from a galactic CCSN may be able to provide constraints on stellar evolution independent of preexplosion imaging and the mass of the compact object remnant prior to fallback accretion.},
doi = {10.3847/1538-4357/ab97b7},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 898,
place = {United States},
year = {Fri Jul 31 00:00:00 EDT 2020},
month = {Fri Jul 31 00:00:00 EDT 2020}
}
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- Fröhlich, C.; Hix, W. R.; Martínez-Pinedo, G.
- New Astronomy Reviews, Vol. 50, Issue 7-8
Very low Energy Supernovae from Neutrino mass loss
journal, May 2013
- Lovegrove, Elizabeth; Woosley, S. E.
- The Astrophysical Journal, Vol. 769, Issue 2
The Dominance of Neutrino-Driven Convection in Core-Collapse Supernovae
journal, June 2013
- Murphy, Jeremiah W.; Dolence, Joshua C.; Burrows, Adam
- The Astrophysical Journal, Vol. 771, Issue 1
Pushing Core-Collapse Supernovae to Explosions in Spherical Symmetry. i. the Model and the case of sn 1987a
journal, June 2015
- Perego, A.; Hempel, M.; Fröhlich, C.
- The Astrophysical Journal, Vol. 806, Issue 2
Monte Carlo Study of Supernova Neutrino Spectra Formation
journal, June 2003
- Keil, Mathias Th.; Raffelt, Georg G.; Janka, Hans‐Thomas
- The Astrophysical Journal, Vol. 590, Issue 2
Towards asteroseismology of core-collapse supernovae with gravitational-wave observations – I. Cowling approximation
journal, November 2017
- Torres-Forné, Alejandro; Cerdá-Durán, Pablo; Passamonti, Andrea
- Monthly Notices of the Royal Astronomical Society, Vol. 474, Issue 4
Conservative general relativistic variable Eddington tensor radiation transport equations
journal, May 2013
- Cardall, Christian Y.; Endeve, Eirik; Mezzacappa, Anthony
- Physical Review D, Vol. 87, Issue 10
Universal Relations for Gravitational-Wave Asteroseismology of Protoneutron Stars
journal, July 2019
- Torres-Forné, Alejandro; Cerdá-Durán, Pablo; Obergaulinger, Martin
- Physical Review Letters, Vol. 123, Issue 5
Convection-aided Explosions in One-dimensional Core-collapse Supernova Simulations. I. Technique and Validation
journal, December 2019
- Mabanta, Quintin A.; Murphy, Jeremiah W.; Dolence, Joshua C.
- The Astrophysical Journal, Vol. 887, Issue 1
Neutrino signals of core-collapse supernovae in underground detectors
journal, August 2018
- Seadrow, Shaquann; Burrows, Adam; Vartanyan, David
- Monthly Notices of the Royal Astronomical Society, Vol. 480, Issue 4
Identifying the neutrino mass spectrum from a supernova neutrino burst
journal, July 2000
- Dighe, Amol S.; Smirnov, Alexei Yu.
- Physical Review D, Vol. 62, Issue 3
A simple approach to the supernova progenitor–explosion connection
journal, May 2016
- Müller, Bernhard; Heger, Alexander; Liptai, David
- Monthly Notices of the Royal Astronomical Society, Vol. 460, Issue 1
Core-collapse supernovae in the hall of mirrors: A three-dimensional code-comparison project
journal, November 2018
- Cabezón, Rubén M.; Pan, Kuo-Chuan; Liebendörfer, Matthias
- Astronomy & Astrophysics, Vol. 619