| dc.contributor.author |
Narayan M. |
|
| dc.contributor.author |
Rajasekaran G. |
|
| dc.contributor.author |
Sinha R. |
|
| dc.contributor.author |
Burgess C.P. |
|
| dc.date.accessioned |
2023-10-13T12:37:30Z |
|
| dc.date.available |
2023-10-13T12:37:30Z |
|
| dc.date.issued |
1999 |
|
| dc.identifier |
10.1103/PhysRevD.60.073006 |
|
| dc.identifier.issn |
15507998 |
|
| dc.identifier.uri |
https://dspace.imsc.res.in/xmlui/handle/123456789/733 |
|
| dc.identifier.uri |
https://doi.org/10.1103/PhysRevD.60.073006 |
|
| dc.description.abstract |
The solar neutrino counting rate in a real time detector such as Super-Kamiokanda, SNO, or Borexino is enhanced due to neutrino oscillations in the Moon during a partial or total solar eclipse. The enhancement is calculated as a function of the neutrino parameters in the case of three flavor mixing. This enhancement, if seen, can further help to determine the neutrino parameters. © 1999 The American Physical Society. |
|
| dc.language.iso |
en |
|
| dc.relation.ispartof |
Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 60, Issue. 7 |
|
| dc.rights |
Copyrighted by the Publisher |
|
| dc.source |
Physical Review D - Particles, Fields, Gravitation and Cosmology |
|
| dc.title |
Solar neutrinos and the eclipse effect |
|
| dc.relation.url |
https://doi.org/10.1103/PhysRevD.60.073006 |
|
| dc.type |
Article |
|