Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae
Abstract
We explore the influence of progenitor mass and rotation on the gravitational-wave (GW) emission from core-collapse supernovae, during the postbounce, preexplosion, accretion phase. We present the results from 15 two-dimensional (2D) neutrino radiation-hydrodynamic simulations from initial stellar collapse to ~300 ms after core bounce. We examine the features of the GW signals for four zero-age main sequence (ZAMS) progenitor masses ranging from 12 M⊙ to 60 M⊙ and four core rotation rates from 0 to 3 rad s-1. We find that GW strain immediately around core bounce is fairly independent of ZAMS mass and—consistent with previous findings—that it is more heavily dependent on the core angular momentum. At later times, all nonrotating progenitors exhibit loud GW emission, which we attribute to vibrational g-modes of the protoneutron star (PNS) excited by convection in the postshock layer and the standing accretion shock instability (SASI). We find that increasing rotation rates results in muting of the accretion-phase GW signal due to centrifugal effects that inhibit convection in the postshock region, quench the SASI, and slow the rate at which the PNS peak vibrational frequency increases. Finally, we verify the efficacy of our approximate general relativistic (GR) effective potential treatment of gravity by comparingmore »
- Authors:
-
[1];
[1];
[2];
[3]
- Michigan State Univ., East Lansing, MI (United States)
- National Tsing Hua Univ., Hsinchu (Taiwan)
- Stockholm Univ., Stockholm (Sweden)
- Publication Date:
- Research Org.:
- Michigan State Univ., East Lansing, MI (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP)
- OSTI Identifier:
- 1612345
- Grant/Contract Number:
- SC0015904; SC0017955; TM7-18005X
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 878; Journal Issue: 1; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; astronomy & astrophysics; gravitational waves; stars; supernovae
Citation Formats
Pajkos, Michael A., Couch, Sean M., Pan, Kuo-Chuan, and O’Connor, Evan P. Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae. United States: N. p., 2019.
Web. doi:10.3847/1538-4357/ab1de2.
Pajkos, Michael A., Couch, Sean M., Pan, Kuo-Chuan, & O’Connor, Evan P. Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae. United States. https://doi.org/10.3847/1538-4357/ab1de2
Pajkos, Michael A., Couch, Sean M., Pan, Kuo-Chuan, and O’Connor, Evan P. Fri .
"Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae". United States. https://doi.org/10.3847/1538-4357/ab1de2. https://www.osti.gov/servlets/purl/1612345.
@article{osti_1612345,
title = {Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae},
author = {Pajkos, Michael A. and Couch, Sean M. and Pan, Kuo-Chuan and O’Connor, Evan P.},
abstractNote = {We explore the influence of progenitor mass and rotation on the gravitational-wave (GW) emission from core-collapse supernovae, during the postbounce, preexplosion, accretion phase. We present the results from 15 two-dimensional (2D) neutrino radiation-hydrodynamic simulations from initial stellar collapse to ~300 ms after core bounce. We examine the features of the GW signals for four zero-age main sequence (ZAMS) progenitor masses ranging from 12 M⊙ to 60 M⊙ and four core rotation rates from 0 to 3 rad s-1. We find that GW strain immediately around core bounce is fairly independent of ZAMS mass and—consistent with previous findings—that it is more heavily dependent on the core angular momentum. At later times, all nonrotating progenitors exhibit loud GW emission, which we attribute to vibrational g-modes of the protoneutron star (PNS) excited by convection in the postshock layer and the standing accretion shock instability (SASI). We find that increasing rotation rates results in muting of the accretion-phase GW signal due to centrifugal effects that inhibit convection in the postshock region, quench the SASI, and slow the rate at which the PNS peak vibrational frequency increases. Finally, we verify the efficacy of our approximate general relativistic (GR) effective potential treatment of gravity by comparing our core bounce GW strains with the recent 2D GR results of other groups.},
doi = {10.3847/1538-4357/ab1de2},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 878,
place = {United States},
year = {Fri Jun 07 00:00:00 EDT 2019},
month = {Fri Jun 07 00:00:00 EDT 2019}
}
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- Couch, Sean M.; Ott, Christian D.
- arXiv
An Open-Source Neutrino Radiation Hydrodynamics Code for Core-Collapse Supernovae
text, January 2014
- O'Connor, Evan
- arXiv
Two Dimensional Core-Collapse Supernova Explosions Aided by General Relativity with Multidimensional Neutrino Transport
text, January 2015
- O'Connor, Evan; Couch, Sean
- arXiv
Neutrino-nucleon scattering in supernova matter from the virial expansion
text, January 2016
- Horowitz, C. J.; Caballero, O. L.; Lin, Zidu
- arXiv
Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport
text, January 2017
- Nagakura, Hiroki; Iwakami, Wakana; Furusawa, Shun
- arXiv
Protomagnetar and black hole formation in high-mass stars
text, January 2017
- Obergaulinger, Martin; Aloy, Miguel-Ángel
- arXiv
Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition
text, January 2017
- Summa, A.; Janka, H. -Th.; Melson, T.
- arXiv
Core-Collapse Supernova Simulations including Neutrino Interactions from the Virial EOS
text, January 2017
- O'Connor, Evan; Horowitz, C. J.; Lin, Zidu
- arXiv
Core collapse with magnetic fields and rotation
text, January 2018
- Obergaulinger, M.; Just, O.; Aloy, M. Á.
- arXiv
Radiation hydrodynamics with neutrinos: Variable Eddington factor method for core-collapse supernova simulations
text, January 2002
- Rampp, Markus; Janka, H. -Thomas
- arXiv
Relativistic simulations of rotational core collapse. II. Collapse dynamics and gravitational radiation
text, January 2002
- Dimmelmeier, Harald; Font, Jose A.; Mueller, Ewald
- arXiv
Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae
text, January 2002
- Blondin, John M.; Mezzacappa, Anthony; DeMarino, Christine
- arXiv
Towards Gravitational Wave Signals from Realistic Core Collapse Supernova Models
text, January 2003
- Mueller, Ewald; Rampp, Markus; Buras, Robert
- arXiv
A simple parameterization of the consequences of deleptonization for simulations of stellar core collapse
text, January 2005
- Liebendoerfer, M.
- arXiv
Numerical Analysis on Standing Accretion Shock Instability with Neutrino Heating in the Supernova Cores
text, January 2005
- Ohnishi, Naofumi; Kotake, Kei; Yamada, Shoichi
- arXiv
Instability of a stalled accretion shock: evidence for the advective-acoustic cycle
text, January 2006
- Foglizzo, T.; Galletti, P.; Scheck, L.
- arXiv
Simulations of Magnetically-Driven Supernova and Hypernova Explosions in the Context of Rapid Rotation
text, January 2007
- Burrows, Adam; Dessart, Luc; Livne, Eli
- arXiv
General relativistic simulations of pasive-magneto-rotational core collapse with microphysics
text, January 2007
- Cerdá-Durán, P.; Font, J. A.; Dimmelmeier, H.
- arXiv
Presupernova Evolution of Rotating Massive Stars I: Numerical Method and Evolution of the Internal Stellar Structure
text, January 1999
- Heger, A.; Langer, N.; Woosley, S. E.
- arXiv
A full general relativistic neutrino radiation-hydrodynamics simulation of a collapsing very massive star and the formation of a black hole
text, January 2018
- Kuroda, Takami; Kotake, Kei; Takiwaki, Tomoya
- arXiv
Works referencing / citing this record:
Temporal and angular variations of 3D core-collapse supernova emissions and their physical correlations
journal, August 2019
- Vartanyan, David; Burrows, Adam; Radice, David
- Monthly Notices of the Royal Astronomical Society, Vol. 489, Issue 2
Gravitational waves from supernova mass loss and natal kicks in close binaries
journal, October 2019
- Holgado, A. Miguel; Ricker, Paul M.
- Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 4