Langanke, K. and Vogel, P. and Kolbe, E. (1996) Signal for supernova νμ and ντ neutrinos in water Čerenkov detectors. Physical Review Letters, 76 (15). pp. 2629-2632. ISSN 0031-9007. http://resolver.caltech.edu/CaltechAUTHORS:LANprl96
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We suggest that photons with energies between 5 and 10 MeV, generated by the ( ν,ν′pγ) and ( ν,ν′nγ) reactions on 16O, constitute a signal which allows a unique identification of supernova νμ and ντ neutrinos in water Čerenkov detectors. We calculate the yield of such γ events and estimate that a few hundred of them would be detected in Superkamiokande for a supernova at 10 kpc distance.
|Additional Information:||©1996 The American Physical Society. Received 27 November 1995. We are grateful to F.-K. Thielemann for providing us with his statistical model code SMOKER. We thank Y.-Z. Qian and F.-K. Thielemann for helpful discussions. This work was supported by the U.S. National Science Foundation (Grants No. PHY94-12818 and No. PHY94-20470), by the U.S. Department of Energy (Contract No. DEFG03-88ER-40397), and by the Swiss Nationalfonds.|
|Subject Keywords:||II SUPERNOVAE; EMISSION; BURST|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Tony Diaz|
|Deposited On:||06 Oct 2006|
|Last Modified:||18 Sep 2014 18:11|
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