dc.contributor.author |
Sivaram, C |
|
dc.date.accessioned |
2008-11-15T11:57:38Z |
|
dc.date.available |
2008-11-15T11:57:38Z |
|
dc.date.issued |
1989-09 |
|
dc.identifier.citation |
Progress of Theoretical Physics, Vol. 82, No. 2, pp. 215 - 216 |
en |
dc.identifier.issn |
0033-068X |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4004 |
|
dc.description.abstract |
It was recentrly shown that the bunching in time of the neutrinos detected from SN1987A in LMC implies among other things that the neutrino electric charge q is 10/sup(-17) times as small as the electron charge. We point out that limits on q several orders more stringent than this can be obtained from other astrophysical considerations, for neutrinos with small rest mass. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Japan Science and Technology Agency |
en |
dc.relation.uri |
http://ptp.ipap.jp/link?PTP/82/215/ |
en |
dc.subject |
Astrophysical Limits |
en |
dc.subject |
Neutrino Electric Charge |
en |
dc.title |
Astrophysical Limits on the Neutrino Electric Charge |
en |
dc.type |
Article |
en |