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Neutrinos from SN 1987A and cooling of the nascent neutron starThe implications of the detection of neutrinos from SN 1987A for the cooling of the nascent neutron star are considered. The nu-bar(e) number N, the apparent temperature, the cooling time scale measured by the Kamioka and IMB detectors, and the inferred neutron star apparent radius and binding energy are all found to provide striking verification of current supernova theory.
Document ID
19890041505
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Lamb, D. Q. (Chicago Univ. Chicago, IL, United States)
Loredo, Thomas J. (Chicago, University IL, United States)
Melia, Fulvio (Northwestern University Evanston, IL, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Subject Category
Astrophysics
Meeting Information
Meeting: Geroge Mason Astrophysics Workshop
Location: Fairfax, VA
Country: United States
Start Date: October 12, 1987
End Date: October 14, 1987
Sponsors: NASA
Accession Number
89A28876
Funding Number(s)
CONTRACT_GRANT: NAGW-830
Distribution Limits
Public
Copyright
Other

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