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Cosmic ray results on the A dependence of multiplicity and angular distributions in proton nuclear interactions above 100 GeV
dc.contributor.authorVishwanath, P. R.en_US
dc.contributor.authorBussian, A. E.en_US
dc.contributor.authorJones, Lawrence W.en_US
dc.contributor.authorLyon, Jr. , D. E.en_US
dc.contributor.authorLearned, J. G.en_US
dc.contributor.authorReeder, D. D.en_US
dc.contributor.authorWilkes, R. J.en_US
dc.date.accessioned2006-04-07T16:40:27Z
dc.date.available2006-04-07T16:40:27Z
dc.date.issued1975-01-06en_US
dc.identifier.citationVishwanath, P. R., Bussian, A. E., Jones, L. W., Lyon, Jr., D. E., Learned, J. G., Reeder, D. D., Wilkes, R. J. (1975/01/06)."Cosmic ray results on the A dependence of multiplicity and angular distributions in proton nuclear interactions above 100 GeV." Physics Letters B 53(5): 479-483. <http://hdl.handle.net/2027.42/22150>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6TVN-46YKPW5-2BR/2/7b3e6779036b1d45bad5c6ace73cd5c4en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/22150
dc.description.abstractA calorimeter-spark chamber system was used to collect data on several hundred proton-nucleus interactions above 100 GeV using targets of C, Al, Fe, Sn and Pb. The average charged prong multiplicity is found to depend on atomic mass number as nc&gt; = nc&gt;(p-p)Ax where X = 0.129 +/- 0.004, with the dominant increase in multiplicity occuring in the backward (p-p c.m.) hemisphere. The value of x shows no significant energy dependence.en_US
dc.format.extent363227 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleCosmic ray results on the A dependence of multiplicity and angular distributions in proton nuclear interactions above 100 GeVen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbsecondlevelMathematicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, Michigan 48104, USAen_US
dc.contributor.affiliationotherDivision of Science and Mathematics, Community College of Denver, Red Rocks Campus, Lakewood, Colorado 80215, USA.en_US
dc.contributor.affiliationotherStanford Linear Accelerator Center, Stanford, California 94305, USA.en_US
dc.contributor.affiliationotherStanford Linear Accelerator Center, Stanford, California 94305, USA.en_US
dc.contributor.affiliationotherUniversity of Wisconsin, Madison, Wisconsin 53706, USAen_US
dc.contributor.affiliationotherUniversity of Wisconsin, Madison, Wisconsin 53706, USAen_US
dc.contributor.affiliationotherCERN, 1211 Geneva 23, Switzerlanden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/22150/1/0000579.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0370-2693(75)90222-1en_US
dc.identifier.sourcePhysics Letters Ben_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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