On some new production processes for [approximate] 1012 eV muons
dc.contributor.author | Ramana Murthy, P. V. | en_US |
dc.date.accessioned | 2006-04-17T15:25:33Z | |
dc.date.available | 2006-04-17T15:25:33Z | |
dc.date.issued | 1968-10-28 | en_US |
dc.identifier.citation | Ramana Murthy, P. V. (1968/10/28)."On some new production processes for [approximate] 1012 eV muons." Physics Letters B 28(1): 38-40. <http://hdl.handle.net/2027.42/33091> | en_US |
dc.identifier.uri | http://www.sciencedirect.com/science/article/B6TVN-473DDYY-60/2/6c060b3790eba1ee596906e7cbc1352f | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/33091 | |
dc.description.abstract | Callan and Glashow and Keuffel have proposed the existence of U and W particles respectively, to explain the lack of zenith angular dependence of cosmic ray muons in the experiment by the Utah group. Arguments are presented to show that both these hypotheses are implausible. | en_US |
dc.format.extent | 230857 bytes | |
dc.format.extent | 3118 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Elsevier | en_US |
dc.title | On some new production processes for [approximate] 1012 eV muons | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Physics | en_US |
dc.subject.hlbsecondlevel | Mathematics | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Physics Department, University of Michigan, Ann Arbor, Michigan 48104, USA | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/33091/1/0000477.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1016/0370-2693(68)90536-4 | en_US |
dc.identifier.source | Physics Letters B | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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