| 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 |