Inferring core-collapse supernova physics with gravitational waves

Logue, J.; Ott, C. D.; Heng, I. S.; Kalmus, P.; Scargill, J. H. C.

doi:10.1103/PhysRevD.86.044023

Title: Inferring core-collapse supernova physics with gravitational waves

Full Record
Other Related Research

Authors:: Logue, J.; Ott, C. D.; Heng, I. S.; Kalmus, P.; Scargill, J. H. C.

Publication Date:: 2012-08-17

Sponsoring Org.:: USDOE

OSTI Identifier:: 1103146

Resource Type:: Publisher's Accepted Manuscript

Journal Name:: Physical Review D

Additional Journal Information:: Journal Volume: 86; Journal Issue: 4; Journal ID: ISSN 1550-7998

Publisher:: American Physical Society

Country of Publication:: United States

Language:: English

Citation Formats


                    Logue, J., Ott, C. D., Heng, I. S., Kalmus, P., and Scargill, J. H. C. Inferring core-collapse supernova physics with gravitational waves.  United States: N. p., 2012. 
Web.  doi:10.1103/PhysRevD.86.044023.

Copy to clipboard


                    Logue, J., Ott, C. D., Heng, I. S., Kalmus, P., & Scargill, J. H. C. Inferring core-collapse supernova physics with gravitational waves.  United States.  https://doi.org/10.1103/PhysRevD.86.044023

Copy to clipboard


                    Logue, J., Ott, C. D., Heng, I. S., Kalmus, P., and Scargill, J. H. C. Fri .  
"Inferring core-collapse supernova physics with gravitational waves".  United States.  https://doi.org/10.1103/PhysRevD.86.044023.

Copy to clipboard


                    
@article{osti_1103146,

  title        = {Inferring core-collapse supernova physics with gravitational waves},

  author       = {Logue, J. and Ott, C. D. and Heng, I. S. and Kalmus, P. and Scargill, J. H. C.},

  abstractNote = {},

  doi          = {10.1103/PhysRevD.86.044023},

  journal      = {Physical Review D},

  number       = 4,

  volume       = 86,

  place        = {United States},

  year         = {2012},

  month        = {8}

}

Copy to clipboard

Journal Article:

Free Publicly Available Full Text

Accepted Manuscript (Publisher)

Publisher's Version of Record
https://doi.org/10.1103/PhysRevD.86.044023

Other availability

Search WorldCat to find libraries that may hold this journal

Citation Metrics:

Cited by: 32 works

Citation information provided by
Web of Science

Save / Share:

Export Metadata

Save to My Library

Similar Records in DOE PAGES and OSTI.GOV collections:

Detection prospects of core-collapse supernovae with supernova-optimized third-generation gravitational-wave detectors

Journal Article Srivastava, Varun ; Ballmer, Stefan ; Brown, Duncan A. ; ... - Physical Review D

We discuss how to optimize the third-generation gravitational-wave detector to maximize the range to detect core-collapse supernovae. Based on three-dimensional simulations for core-collapse and the corresponding gravitational-wave waveform emitted, the corresponding detection range for these waveforms is limited to within our Galaxy even in the era of third-generation detectors. The corresponding event rate is two per century. We find from the waveforms that to detect core-collapse supernovae with an event rate of one per year, the gravitational-wave detectors need a strain sensitivity of 3 × 10^-27 Hz^-1/2 in a frequency range from 100 to 1500 Hz. We also explore detectormore »« less
Cited by 4
https://doi.org/10.1103/physrevd.100.043026

Full Text Available
A NEW MULTI-DIMENSIONAL GENERAL RELATIVISTIC NEUTRINO HYDRODYNAMICS CODE OF CORE-COLLAPSE SUPERNOVAE. III. GRAVITATIONAL WAVE SIGNALS FROM SUPERNOVA EXPLOSION MODELS

Journal Article Mueller, Bernhard ; Janka, Hans-Thomas ; Marek, Andreas - Astrophysical Journal

We present a detailed theoretical analysis of the gravitational wave (GW) signal of the post-bounce evolution of core-collapse supernovae (SNe), employing for the first time relativistic, two-dimensional explosion models with multi-group, three-flavor neutrino transport based on the ray-by-ray-plus approximation. The waveforms reflect the accelerated mass motions associated with the characteristic evolutionary stages that were also identified in previous works: a quasi-periodic modulation by prompt post-shock convection is followed by a phase of relative quiescence before growing amplitudes signal violent hydrodynamical activity due to convection and the standing accretion shock instability during the accretion period of the stalled shock. Finally, amore »« less
https://doi.org/10.1088/0004-637X/766/1/43
The neutrino gravitational memory from a core collapse supernova: phenomenology and physics potential

Journal Article Mukhopadhyay, Mainak ; Cardona, Carlos ; Lunardini, Cecilia - Journal of Cosmology and Astroparticle Physics

Not provided.
https://doi.org/10.1088/1475-7516/2021/07/055
Toward Computing the Gravitational Wave Signatures of Core Collapse Supernovae

Conference Mezzacappa, Anthony ; Yakunin, Konstantin ; Marronetti, Pedro ; ...

No abstract prepared.
The Gravitational Wave Signal from Core-collapse Supernovae

Journal Article Morozova, Viktoriya ; Radice, David ; Burrows, Adam ; ... - The Astrophysical Journal (Online)

We report on gravitational waves (GWs) from a set of 2D multigroup neutrino radiation hydrodynamic simulations of core-collapse supernovae (CCSNe). Our aim is to systematize the current knowledge about the post-bounce CCSN GW signal and recognize the templatable features that could be used by the ground-based laser interferometers. We demonstrate that, starting from ~400 ms after core bounce, the dominant GW signal represents the fundamental quadrupole (l = 2) oscillation mode (f-mode) of the proto–neutron star (PNS), which can be accurately reproduced by a linear perturbation analysis of the angle-averaged PNS profile. Before that, in the time interval between ~200more »« less
Cited by 25
https://doi.org/10.3847/1538-4357/aac5f1

Full Text Available

Similar Records