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Core-Collapse Supernovae, Neutrinos, and Gravitational Waves

Ott, C. D. and O'Connor, E. P. and Gossan, S. and Abdikamalov, E. and Gamma, U. C. T. and Drasco, S. (2013) Core-Collapse Supernovae, Neutrinos, and Gravitational Waves. Nuclear Physics B - Proceedings Supplements, 235-36 . pp. 381-387. ISSN 0920-5632 . http://resolver.caltech.edu/CaltechAUTHORS:20130208-113632514

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Abstract

Core-collapse supernovae are among the most energetic cosmic cataclysms. They are prodigious emitters of neutrinos and quite likely strong galactic sources of gravitational waves. Observation of both neutrinos and gravitational waves from the next galactic or near extragalactic core-collapse supernova will yield a wealth of information on the explosion mechanism, but also on the structure and angular momentum of the progenitor star, and on aspects of fundamental physics such as the equation of state of nuclear matter at high densities and low entropies. In this contribution to the proceedings of the Neutrino 2012 conference, we summarize recent progress made in the theoretical understanding and modeling of core-collapse supernovae. In this, our emphasis is on multi-dimensional processes involved in the explosion mechanism such as neutrino-driven convection and the standing accretion shock instability. As an example of how supernova neutrinos can be used to probe fundamental physics, we discuss how the rise time of the electron antineutrino flux observed in detectors can be used to probe the neutrino mass hierarchy. Finally, we lay out aspects of the neutrino and gravitational-wave signature of core-collapse supernovae and discuss the power of combined analysis of neutrino and gravitational wave data from the next galactic core-collapse supernova.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1212.4250v1arXivDiscussion Paper
http://dx.doi.org/10.1016/j.nuclphysbps.2013.04.036DOIArticle
http://www.sciencedirect.com/science/article/pii/S0920563213001576PublisherArticle
http://neu2012.kek.jp/OrganizationConference Website
Additional Information:© 2013 Elsevier B.V. We acknowledge helpful interactions at Neutrino 2012 with John Beacom, Ryan Patterson, Kate Scholberg, and Mark Vagins. This research is partially supported by NSF grant nos. AST-1212170, PHY-1151197, PHY-1068881, and OCI-0905046, by the Alfred P. Sloan Foundation, and by the Sherman Fairchild Foundation. Some of the results presented here were obtained on supercomputers of the NSF XSEDE network under computer time allocation TG-PHY100033.
Group:TAPIR
Funders:
Funding AgencyGrant Number
NSFAST-1212170
NSFPHY-1151197
NSFPHY-1068881
NSFOCI-0905046
Alfred P. Sloan FoundationUNSPECIFIED
Sherman Fairchild FoundationUNSPECIFIED
NSFTG-PHY100033
Subject Keywords:Core-Collapse Supernovae, Neutrinos, and Gravitational Waves
Record Number:CaltechAUTHORS:20130208-113632514
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20130208-113632514
Official Citation:C.D. Ott, E.P. OʼConnor, S. Gossan, E. Abdikamalov, U.C.T. Gamma, S. Drasco, Core-Collapse Supernovae, Neutrinos, and Gravitational Waves, Nuclear Physics B - Proceedings Supplements, Volumes 235–236, February–March 2013, Pages 381-387, ISSN 0920-5632, http://dx.doi.org/10.1016/j.nuclphysbps.2013.04.036.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:36822
Collection:CaltechAUTHORS
Deposited By: JoAnn Boyd
Deposited On:13 Feb 2013 19:17
Last Modified:12 Aug 2013 15:30

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