Solar neutrino results from Super-Kamiokande

Details Solar neutrino results from Super-Kamiokande Solar neutrino results from Super-Kamiokande

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nuphs..77...35s&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 77, Issue 1-3, p. 35-42.

Physics

Nuclear Physics

73

Scientific paper

The recent results from the solar neutrino observation in Super-Kamiokande is presented. From the 504 days of data, taken between the 31st of May, 1996 and the 25th of March, 1998, we have obtained the 8B-solar neutrino flux ratio to the prediction of the standard solar model of BP98 to be 0.474+0.010-0.009+0.017- 0.014 (0.506+0.011-0.010+0.018- 0.015 for TC98). We found no significant difference between day and nighttime flux. The spectrum shape is compared with the expected from the 8B-neutrino spectrum, the neutrino interaction and the detector response, and we have obtained χ2 of 25.3 (15 d.o.f), corresponding to a 4.6% C.L. Implications of these measurements to neutrino oscillations are discussed.

Affiliated with

Also associated with

No associations

Rating

Solar neutrino results from Super-Kamiokande does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Solar neutrino results from Super-Kamiokande, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar neutrino results from Super-Kamiokande will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1193131