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Title: Gravitational Waves from Gravitational Collapse

Abstract

Gravitational-wave emission from stellar collapse has been studied for nearly four decades. Current state-of-the-art numerical investigations of collapse include those that use progenitors with more realistic angular momentum profiles, properly treat microphysics issues, account for general relativity, and examine non-axisymmetric effects in three dimensions. Such simulations predict that gravitational waves from various phenomena associated with gravitational collapse could be detectable with ground-based and space-based interferometric observatories. This review covers the entire range of stellar collapse sources of gravitational waves: from the accretion-induced collapse of a white dwarf through the collapse down to neutron stars or black holes of massive stars to the collapse of supermassive stars.

Authors:
 [1];  [1]
+ Show Author Affiliations
  1. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Publication Date:
Research Org.:
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
810413
Report Number(s):
LA-UR-02-3583
Journal ID: ISSN 2367-3613
Grant/Contract Number:  
W-7405-ENG-36
Resource Type:
Accepted Manuscript
Journal Name:
Living Reviews in Relativity
Additional Journal Information:
Journal Volume: 6; Journal Issue: 1; Journal ID: ISSN 2367-3613
Publisher:
Springer Nature
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 79 ASTRONOMY AND ASTROPHYSICS; Black Hole; Neutron Star; Gravitational Wave; White Dwarf; Core Collapse

Citation Formats

Fryer, Chris L., and New, Kimberly C. B. Gravitational Waves from Gravitational Collapse. United States: N. p., 2003. Web. doi:10.12942/lrr-2003-2.
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Fryer, Chris L., & New, Kimberly C. B. Gravitational Waves from Gravitational Collapse. United States. https://doi.org/10.12942/lrr-2003-2
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Fryer, Chris L., and New, Kimberly C. B. Mon . "Gravitational Waves from Gravitational Collapse". United States. https://doi.org/10.12942/lrr-2003-2. https://www.osti.gov/servlets/purl/810413.
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@article{osti_810413,
title = {Gravitational Waves from Gravitational Collapse},
author = {Fryer, Chris L. and New, Kimberly C. B.},
abstractNote = {Gravitational-wave emission from stellar collapse has been studied for nearly four decades. Current state-of-the-art numerical investigations of collapse include those that use progenitors with more realistic angular momentum profiles, properly treat microphysics issues, account for general relativity, and examine non-axisymmetric effects in three dimensions. Such simulations predict that gravitational waves from various phenomena associated with gravitational collapse could be detectable with ground-based and space-based interferometric observatories. This review covers the entire range of stellar collapse sources of gravitational waves: from the accretion-induced collapse of a white dwarf through the collapse down to neutron stars or black holes of massive stars to the collapse of supermassive stars.},
doi = {10.12942/lrr-2003-2},
journal = {Living Reviews in Relativity},
number = 1,
volume = 6,
place = {United States},
year = {2003},
month = {3}
}
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https://doi.org/10.12942/lrr-2003-2
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Figure 1 Figure 1: Diagram of the convective engine for supernova explosions.
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A New Class of Unstable Modes of Rotating Relativistic Stars
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Nonlinear Development of the Secular Bar‐Mode Instability in Rotating Neutron Stars
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Formation of supermassive black holes by direct collapse in pre-galactic haloes
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Nonlinear Evolution of the r -Modes in Neutron Stars
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Numerical evolutions of nonlinear r -modes in neutron stars
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Gravitational radiation from 3D gravitational stellar core collapse
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Nonlinear mode coupling in rotating stars and the r -mode instability in neutron stars
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Gravitational wave astronomy
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Neutron Star Kicks from Asymmetric Collapse
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Nonlinear r -Modes in Rapidly Rotating Relativistic Stars
journal, February 2001

Axisymmetric simulations of magneto-rotational core collapse: dynamics and gravitational wave signal
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Accretion-driven gravitational radiation from nonrotating compact objects: Infalling quadrupolar shells
journal, June 2004

Comment on β€œGravitational Radiation Instability in Hot Young Neutron Stars”
journal, February 2001

Gravitational waves from newly born, hot neutron stars
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Conditions for accretion-induced collapse of white dwarfs
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Evolution of Differentially Rotating Supermassive Stars to the Onset of Bar Instability
journal, February 2001

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The Magnetorotational Instability in Core‐Collapse Supernova Explosions
journal, February 2003

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Effect of hyperon bulk viscosity on neutron-star r -modes
journal, March 2002

Nonlinear r-Modes in Rapidly Rotating Relativistic Stars
text, January 2001

Theory and Astrophysical Consequences of a Magnetized Torus around a Rapidly Rotating Black Hole
journal, February 2003

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Death rate of massive stars at redshiftΒ $\mathsf{\sim}$0.3
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A Radio Survey of Type Ib and Ic Supernovae: Searching for Engine‐driven Supernovae
journal, December 2003

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Rapidly Rotating Stars. VIII. Zero-Viscosity Polytropic Sequences
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Supermassive Black Holes and Galaxy Morphology
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Axial Instability of Rotating Relativistic Stars
journal, August 1998

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Nonaxisymmetric Dynamic Instabilities of Rotating Polytropes. II. Torques, Bars, and Mode Saturation with Applications to Protostars and Fizzlers
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The Hydrodynamic Behavior of Supernovae Explosions
journal, January 1966

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Relativistic simulations of rotational core collapse I. Methods, initial models, and code tests
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Determining gravitational radiation from Newtonian self-gravitating systems
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Dynamical Rotational Instability at Low [ITAL]T[/ITAL]/[ITAL]W[/ITAL]
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Gravitational wave background from a cosmological population of core-collapse supernovae
journal, February 1999

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Magnetorotational collapse of very massive stars to black holes in full general relativity
journal, October 2007

Collapsing white dwarfs
journal, September 1987

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Gravitational-Wave Emission from Rotating Gravitational Collapse
journal, August 1985

Surface Hydrogen-burning Modeling of Supersoft X-Ray Binaries: Are They Type Ia Supernova Progenitors?
journal, August 2004

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Stellar Core Collapse and Supernova, b
journal, May 1986

Nonlinear couplings of R-modes: Energy transfer and saturation amplitudes at realistic timescales
journal, December 2004

The generation of gravitational radiation by escaping supernova neutrinos
journal, August 1978

The linear and nonlinear dynamic stability of rotating N = 3/2 polytropes
journal, November 1985

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Gravitational Radiation from Nonaxisymmetric Collisions of Neutron Stars
journal, October 1993

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Numerical Methods for the Simulation of Dynamical Mass Transfer in Binaries
journal, January 2002

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One‐armed Spiral Instability in Differentially Rotating Stars
journal, September 2003

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The Spin Periods and Rotational Profiles of Neutron Stars at Birth
journal, May 2006

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Asymptotic Giant Branch Evolution and Beyond
journal, September 1983

Long Gamma-Ray Burst Progenitors: Boundary Conditions and Binary Models
text, January 2007

A compact star rotating at 1122 Hz and the r-mode instability
text, January 2007

Magnetorotational collapse of very massive stars to black holes in full general relativity
text, January 2007

A new general relativistic magnetohydrodynamics code for dynamical spacetimes
text, January 2008

Criteria for Core-Collapse Supernova Explosions by the Neutrino Mechanism
text, January 2008

The gravitational wave burst signal from core collapse of rotating stars
text, January 2008

Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle Recombination
text, January 2008

A Model for Gravitational Wave Emission from Neutrino-Driven Core-Collapse Supernovae
text, January 2009

Gravitational waves from relativistic rotational core collapse
text, January 2001

Relativistic simulations of rotational core collapse. I. Methods, initial models, and code tests
text, January 2002

Gravitational waves from newly born, hot neutron stars
text, January 2002

Towards Gravitational Wave Signals from Realistic Core Collapse Supernova Models
text, January 2003

Neutron Star Kicks from Asymmetric Collapse
text, January 2003

Nonlinear Development of the Secular Bar-mode Instability in Rotating Neutron Stars
text, January 2004

Explosion Mechanism, Neutrino Burst, and Gravitational Wave in Core-Collapse Supernovae
text, January 2005

Numerical Simulations of the Onset and Stability of Dynamical Mass Transfer in Binaries
text, January 2005

Supernova Fallback: A Possible Site for the r-Process
text, January 2006

Gamma-Ray Bursts as the Death Throes of Massive Binary Stars
text, January 1992

Hyper-Accreting Black Holes and Gamma-Ray Bursts
text, January 1998

The Formation and Fragmentation of Primordial Molecular Clouds
preprint, January 1998

Quasinormal ringing of Kerr black holes: The excitation factors
text, January 2006

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    Non-linear pulsations in differentially rotating neutron stars: mass-shedding-induced damping and splitting of the fundamental mode
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    • Stergioulas, Nikolaos; Apostolatos, Theocharis A.; Font, JosΓ© A.
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    All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run
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    Spectral Methods for Numerical Relativity
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    • Living Reviews in Relativity, Vol. 12, Issue 1
    • DOI: 10.12942/lrr-2009-1

    Gravitational Radiation from Standing Accretion Shock Instability in Core‐Collapse Supernovae
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    • Kotake, Kei; Ohnishi, Naofumi; Yamada, Shoichi
    • The Astrophysical Journal, Vol. 655, Issue 1
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    Gravitational waves from supernova mass loss and natal kicks in close binaries
    journal, October 2019

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    Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo
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    All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run
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    • Abadie, J.; Affeldt, C.; Allen, Bruce
    • College Park, MD : American Physical Society
    • DOI: 10.15488/2140

    Current status of numerical-relativity simulations in Kyoto
    journal, January 2012

    • Sekiguchi, Yuichiro; Kiuchi, Kenta; Kyutoku, Koutarou
    • Progress of Theoretical and Experimental Physics, Vol. 2012, Issue 1
    • DOI: 10.1093/ptep/pts011

    Parametrized 3D models of neutrino-driven supernova explosions: Neutrino emission asymmetries and gravitational-wave signals
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    Exploring the sensitivity of next generation gravitational wave detectors
    journal, January 2017

    • Abbott, B. P.; Abbott, R.; Abbott, T. D.
    • Classical and Quantum Gravity, Vol. 34, Issue 4
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    Towards asteroseismology of core-collapse supernovae with gravitational wave observations – II. Inclusion of space–time perturbations
    journal, October 2018

    • Torres-FornΓ©, Alejandro; CerdΓ‘-DurΓ‘n, Pablo; Passamonti, Andrea
    • Monthly Notices of the Royal Astronomical Society, Vol. 482, Issue 3
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    IGEC2: A 17-month search for gravitational wave bursts in 2005–2007
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    The gravitational-wave signature of core-collapse supernovae
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    Quasinormal modes of black holes and black branes
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    Current Status of Numerical-Relativity Simulations in Kyoto
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