Please use this identifier to cite or link to this item: http://hdl.handle.net/2307/366
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dc.contributor.authorAielli, G.-
dc.contributor.authorBacci, Cesare-
dc.contributor.authorBartoli, B.-
dc.contributor.authorBernardini, P.-
dc.contributor.authorBi, X. J.-
dc.contributor.authorBleve, C.-
dc.contributor.authorBranchini, Paolo-
dc.contributor.authorBudano, A.-
dc.contributor.authorBussino, Severino-
dc.contributor.authorCalabrese Melcarne, A. K.-
dc.contributor.authorCamarri, P.-
dc.contributor.authorCao, Z.-
dc.contributor.authorCappa, A.-
dc.contributor.authorCardarelli, R.-
dc.contributor.authorCatalanotti, S.-
dc.contributor.authorCattaneo, C.-
dc.contributor.authorCelio, Paola-
dc.contributor.authorChen, S. Z.-
dc.contributor.authorChen, Y.-
dc.contributor.authorCheng, N.-
dc.contributor.authorCreti, P.-
dc.contributor.authorCui, S. W.-
dc.contributor.authorDai, B. Z.-
dc.contributor.authorD'Ali Staiti, G.-
dc.contributor.authorDanzengluobu-
dc.contributor.authorDattoli, M.-
dc.contributor.authorDe Mitri, I.-
dc.contributor.authorD'Ettorre Piazzoli, B.-
dc.contributor.authorDe Vincenzi, Mario-
dc.contributor.authorDi Girolamo, T.-
dc.contributor.authorDing, X. H.-
dc.contributor.authorDi Sciascio, G.-
dc.contributor.authorFeng, C. F.-
dc.contributor.authorFeng, Zhaoyang-
dc.contributor.authorFeng, Zhenyong-
dc.contributor.authorGaleazzi, Fulvio-
dc.contributor.authorGaleotti, P.-
dc.contributor.authorGargana, Riccardo-
dc.contributor.authorGou, Q. B.-
dc.contributor.authorGuo, Y. Q.-
dc.contributor.authorHe, H. H.-
dc.contributor.authorHu, Haibing-
dc.contributor.authorHu, Hongbo-
dc.contributor.authorHuang, Q.-
dc.contributor.authorIacovacci, M.-
dc.contributor.authorIuppa, R.-
dc.contributor.authorJames, Irina-
dc.contributor.authorJia, H. Y.-
dc.contributor.authorLabaciren-
dc.contributor.authorLi, H. J.-
dc.contributor.authorLi, J. Y.-
dc.contributor.authorLi, X. X.-
dc.contributor.authorLiberti, B.-
dc.contributor.authorLiguori, G.-
dc.contributor.authorLiu, C.-
dc.contributor.authorLiu, C. Q.-
dc.contributor.authorLiu, M. Y.-
dc.contributor.authorLiu, J.-
dc.contributor.authorLu, H.-
dc.contributor.authorMa, X. H.-
dc.contributor.authorMancarella, G.-
dc.contributor.authorMari, Stefano Maria-
dc.contributor.authorMarsella, G.-
dc.contributor.authorMartello, D.-
dc.contributor.authorMastroianni, Stefano-
dc.contributor.authorMeng, X. R.-
dc.contributor.authorMontini, Paolo-
dc.contributor.authorNing, C. C.-
dc.contributor.authorPagliaro, A.-
dc.contributor.authorPanareo, M.-
dc.contributor.authorPerrone, L.-
dc.contributor.authorPistilli, Pio-
dc.contributor.authorQu, X. B.-
dc.contributor.authorRossi, E.-
dc.contributor.authorRuggieri, Federico-
dc.contributor.authorSaggese, L.-
dc.contributor.authorSalvini, P.-
dc.contributor.authorSantonico, R.-
dc.contributor.authorShen, P. R.-
dc.contributor.authorSheng, X. D.-
dc.contributor.authorShi, F.-
dc.contributor.authorStanescu, Cristian-
dc.contributor.authorSurdo, A.-
dc.contributor.authorTan, Y. H.-
dc.contributor.authorVallania, P.-
dc.contributor.authorVernetto, S.-
dc.contributor.authorVigorito, C.-
dc.contributor.authorWang, B.-
dc.contributor.authorWang, H.-
dc.contributor.authorWu, C. Y.-
dc.contributor.authorWu, H. R.-
dc.contributor.authorXu, B.-
dc.contributor.authorXue, L.-
dc.contributor.authorYan, Y. X.-
dc.contributor.authorYang, Q. Y.-
dc.contributor.authorYang, X. C.-
dc.contributor.authorYuan, A. F.-
dc.contributor.authorZha, M.-
dc.contributor.authorZhang, H. M.-
dc.contributor.authorZhang, JiLong-
dc.contributor.authorZhang, JianLi-
dc.contributor.authorZhang, L.-
dc.contributor.authorZhang, P.-
dc.contributor.authorZhang, X. Y.-
dc.contributor.authorZhang, Y.-
dc.contributor.authorZhaxisangzhu-
dc.contributor.authorZhou, X. X.-
dc.contributor.authorZhu, F. R.-
dc.contributor.authorZhu, Q. Q.-
dc.contributor.authorZizzi, G.-
dc.date.accessioned2010-07-28T13:27:30Z-
dc.date.available2010-07-28T13:27:30Z-
dc.date.issued2009-11-16-
dc.identifier.issn1550-7998-
dc.identifier.urihttp://hdl.handle.net/2307/366-
dc.description.abstractThe proton-air cross section in the energy range 1-100 TeV has been measured by the ARGO-YBJ cosmic ray experiment. The analysis is based on the primary cosmic ray flux attenuation for different atmospheric depths (i.e. zenith angles) and exploits the detector capabilities of selecting the shower development stage by means of hit multiplicity, density and lateral profile measurements at ground. The effects of shower fluctuations, the contribution of heavier primaries and the uncertainties of the hadronic interaction models, have been taken into account. The results have been used to estimate the total proton-proton cross section at center-of-mass energies between 70 and 500 GeV, where no accelerator data are currently available.en
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.relation.ispartofPhysical Review Den
dc.rightsThe American Physical Societyen
dc.subjectHADRONIC-INTERACTIONSen
dc.subjectp-p CROSS SECTIONen
dc.subjectAIR SHOWER EXPERIMENTSen
dc.subjectASTROPARTICLE PHYSICSen
dc.subjectCOSMIC RAYSen
dc.titleProton-air cross section measurement with the ARGO-YBJ cosmic ray experimenten
dc.typeArticleen
dc.subject.miurSettori Disciplinari MIUR::Scienze fisiche::FISICA SPERIMENTALEen
dc.subject.isicruiCategorie ISI-CRUI::Scienze fisiche::Physicsen
dc.subject.anagraferoma3Scienze fisicheen
dc.relation.volumenumber80en
dc.relation.pagenumber092004en
dc.identifier.doi10.1103/PhysRevD.80.092004-
dc.relation.issuenumber9en
item.languageiso639-1other-
item.fulltextWith Fulltext-
item.grantfulltextrestricted-
Appears in Collections:A - Articolo su rivista
X_Dipartimento di Fisica 'Edoardo Amaldi'
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