Time-of-night variation of solar neutrinos

Show simple item record

dc.contributor.author Narayan M.
dc.contributor.author Rajasekaran G.
dc.contributor.author Sinha R.
dc.date.accessioned 2023-10-13T12:37:30Z
dc.date.available 2023-10-13T12:37:30Z
dc.date.issued 1998
dc.identifier 10.1142/S0217732398002023
dc.identifier.issn 2177323
dc.identifier.uri https://dspace.imsc.res.in/xmlui/handle/123456789/734
dc.identifier.uri https://doi.org/10.1142/S0217732398002023
dc.description.abstract We investigate the time-of-night variation of solar neutrino rate which will be of relevance to super-Kamioka and Sudbury neutrino detectors in the framework of oscillations among the three flavors. An analytical method of computing the regeneration in the earth is presented. If day-night effect is seen, we show how the study of the time-of-night variation will allow the determination of the neutrino parameters.
dc.language.iso en
dc.relation.ispartof Modern Physics Letters A, Vol. 13, Issue. 24
dc.rights Copyrighted by the Publisher
dc.source Modern Physics Letters A
dc.title Time-of-night variation of solar neutrinos
dc.description.pages 1915 - 1922
dc.relation.url https://doi.org/10.1142/S0217732398002023
dc.publisher World Scientific Publishing Co. Pte Ltd
dc.type Article


Files in this item

Files Size Format View

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record

Search DSpace


Advanced Search

Browse

My Account