Search for supernova neutrino bursts at super-kamiokande

0Citations
Citations of this article
34Readers
Mendeley users who have this article in their library.

Abstract

The result of a search for neutrino bursts from supernova explosions using the Super- Kamiokande detector is reported. Super-Kamiokande is sensitive to core-collapse supernova explosions. The expected number of events comprising such a burst is ∼ 104 and the average energy of the neutrinos is in few tens of MeV range in the case of a core-collapse supernova explosion at the typical distance in our galaxy (10 kiloparsecs). The detection efficiency anywhere within our galaxy and well past the Magellanic Clouds is obtained as 100%. We examined a data set which was taken from May, 1996 to July, 2001 and from December, 2002 to October, 2005 corresponding to 2589.2 live days. However, there is no evidence of such a supernova explosion during the data-taking period. The 90% C.L. upper limit on the rate of core-collapse supernova explosions out to distances of 100 kiloparsecs is found to be 0.32 SN · year-1.

Cite

CITATION STYLE

APA

Ikeda, M., & Takeda, A. (2007). Search for supernova neutrino bursts at super-kamiokande. In Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007 (Vol. 5, pp. 1397–1400). Universidad Nacional Autonoma de Mexico. https://doi.org/10.1086/521547

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free