Core-collapse supernovae and gravitational waves

C. Y. Cardall

doi:10.1016/j.nuclphysbps.2004.11.100

Core-collapse supernovae and gravitational waves

C. Y. Cardall

Theoretical and Computational Physics

Research output: Contribution to journal › Article › peer-review

1 Scopus citations

Abstract

Core-collapse supernovae are dramatic events with a rich phenomenology, including gravitational radiation. Simulations of these events in multiple spatial dimensions with energy- and angle-dependent neutrino transport are still in their infancy. Core collapse and bounce in a supernova in our galaxy may well be visible by first-generation LIGO, but detailed understanding waits on improvements in modeling both stellar progenitors and the supernova process.

Original language	English
Pages (from-to)	436-438
Number of pages	3
Journal	Nuclear Physics B - Proceedings Supplements
Volume	138
Issue number	1-3
DOIs	https://doi.org/10.1016/j.nuclphysbps.2004.11.100
State	Published - Jan 2005

Funding

∗This work was supportedby ScientificDiscovery Through Advanced Computing (SciDAC), a program of the Office of Science of the U.S. Department of Energy (DoE); and by Oak Ridge National Laboratory, managed by UT-Battelle, LLC, for the DoE under contract DE-AC05-00OR22725.

Access to Document

10.1016/j.nuclphysbps.2004.11.100

Cite this

@article{27ec153b2f744ce7b227fe4236fd0e32,

title = "Core-collapse supernovae and gravitational waves",

abstract = "Core-collapse supernovae are dramatic events with a rich phenomenology, including gravitational radiation. Simulations of these events in multiple spatial dimensions with energy- and angle-dependent neutrino transport are still in their infancy. Core collapse and bounce in a supernova in our galaxy may well be visible by first-generation LIGO, but detailed understanding waits on improvements in modeling both stellar progenitors and the supernova process.",

author = "Cardall, \{C. Y.\}",

year = "2005",

month = jan,

doi = "10.1016/j.nuclphysbps.2004.11.100",

language = "English",

volume = "138",

pages = "436--438",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

publisher = "Elsevier",

number = "1-3",

}

TY - JOUR

T1 - Core-collapse supernovae and gravitational waves

AU - Cardall, C. Y.

PY - 2005/1

Y1 - 2005/1

N2 - Core-collapse supernovae are dramatic events with a rich phenomenology, including gravitational radiation. Simulations of these events in multiple spatial dimensions with energy- and angle-dependent neutrino transport are still in their infancy. Core collapse and bounce in a supernova in our galaxy may well be visible by first-generation LIGO, but detailed understanding waits on improvements in modeling both stellar progenitors and the supernova process.

AB - Core-collapse supernovae are dramatic events with a rich phenomenology, including gravitational radiation. Simulations of these events in multiple spatial dimensions with energy- and angle-dependent neutrino transport are still in their infancy. Core collapse and bounce in a supernova in our galaxy may well be visible by first-generation LIGO, but detailed understanding waits on improvements in modeling both stellar progenitors and the supernova process.

UR - https://www.scopus.com/pages/publications/26644455506

U2 - 10.1016/j.nuclphysbps.2004.11.100

DO - 10.1016/j.nuclphysbps.2004.11.100

M3 - Article

AN - SCOPUS:26644455506

SN - 0920-5632

VL - 138

SP - 436

EP - 438

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

IS - 1-3

ER -

Core-collapse supernovae and gravitational waves

Abstract

Funding

Access to Document

Other files and links

Fingerprint

Cite this