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Future galactic supernova neutrino signal: What can we learn?

Vogel, P. (2002) Future galactic supernova neutrino signal: What can we learn? Progress in Particle and Nuclear Physics, 48 (1). pp. 29-37. ISSN 0146-6410. doi:10.1016/S0146-6410(02)00108-4. https://resolver.caltech.edu/CaltechAUTHORS:20170711-132837202

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Abstract

The next supernova in our galaxy will be detected by a variety of neutrino detectors. In this lecture I discuss the set of observables needed to constrain the models of supernova neutrino emission. They are the flux normalizations, and average energies, of each of the three expected components of the neutrino flux: ν_e, ν_e, and ν_x (all the other four flavors combined). I show how the existing, or soon to be operational, neutrino detectors will be able to determine the magnitude of these observables, and estimate the corresponding rates.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1016/S0146-6410(02)00108-4DOIArticle
http://www.sciencedirect.com/science/article/pii/S0146641002001084PublisherArticle
ORCID:
AuthorORCID
Vogel, P.0000-0003-0587-5466
Additional Information:© 2002 Elsevier B.V. Received 8 November 2001, Available online 21 June 2002.
Issue or Number:1
DOI:10.1016/S0146-6410(02)00108-4
Record Number:CaltechAUTHORS:20170711-132837202
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170711-132837202
Official Citation:P. Vogel, Future galactic supernova neutrino signal: What can we learn?, Progress in Particle and Nuclear Physics, Volume 48, Issue 1, 2002, Pages 29-37, ISSN 0146-6410, https://doi.org/10.1016/S0146-6410(02)00108-4. (http://www.sciencedirect.com/science/article/pii/S0146641002001084)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:78953
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:11 Jul 2017 21:01
Last Modified:15 Nov 2021 17:44

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