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dc.contributor.authorCatanesi, M. G.-
dc.contributor.authorBurguet Castell, Jordi-
dc.contributor.authorCervera Villanueva, Anselmo-
dc.contributor.authorGómez Cadenas, Juan José-
dc.contributor.authorMartín-Albo, Justo-
dc.contributor.authorNovella, Pau-
dc.contributor.authorSorel, Michel-
dc.contributor.authorApollonio, M.-
dc.contributor.authorHARP Collaboration-
dc.date.accessioned2011-11-23T09:43:40Z-
dc.date.available2011-11-23T09:43:40Z-
dc.date.issued2008-05-
dc.identifier.citationAstroparticle Physics 29 (4): 257-281 (2008)es_ES
dc.identifier.issn0927-6505-
dc.identifier.urihttp://hdl.handle.net/10261/42698-
dc.description.abstractThe results of the measurements of the double-differential production cross-sections of pions, d(2)sigma(pi)/dpd Omega, in p-C and pi(+/-)-C interactions using the forward spectrometer of the HARP experiment are presented. The incident particles are 12 GeV/c protons and charged pions directed onto a carbon target with a thickness of 5% of a nuclear interaction length. For p-C interactions the analysis is performed using 100,035 reconstructed secondary tracks, while the corresponding numbers of tracks for pi(-)-C and pi(+)-C analyses are 106,534 and 10,122, respectively. Cross-section results are presented in the kinematic range 0.5 GeV/c <= p(pi) < 8 GeV/c and 30 mrad <= theta(pi) < 240 mrad in the laboratory frame. The measured cross-sections have a direct impact on the precise calculation of atmospheric neutrino fluxes and on the improved reliability of extensive air shower simulations by reducing the uncertainties of hadronic interaction models in the low energy range.es_ES
dc.description.sponsorshipWe gratefully acknowledge the help and support of the PS beam staff and of the numerous technical collaborators who contributed to the detector design, construction, commissioning and operation. In particular, we would like to thank G. Barichello, R. Brocard, K. Burin, V. Carassiti, F. Chignoli, D. Conventi, G. Decreuse, M. Delattre, C. Detraz, A. Domeniconi, M. Dwuznik, F. Evangelisti, B. Friend, A. Iaciofano, I. Krasin, D. Lacroix, J.-C. Legrand, M. Lobello, M. Lollo, J. Loquet, F. Marinilli, J. Mulon, L. Musa, R. Nicholson, A. Pepato, P. Petev, X. Pons, I. Rusinov, M. Scandurra, E. Usenko, and R. van der Vlugt, for their support in the construction of the detector. The collaboration acknowledges the major contributions and advice of M. Baldo-Ceolin, L. Linssen, M.T. Muciaccia and A. Pullia during the construction of the experiment. The collaboration is indebted to V. Ableev, F. Bergsma, P. Binko, E. Boter, M. Calvi, C. Cavion, A. Chukanov, M. Doucet, D. Du¨ llmann, V. Ermilova, W. Flegel, Y. Hayato, A. Ichikawa, A. Ivanchenko, O. Klimov, T. Kobayashi, D. Kustov, M. Laveder, M. Mass, H. Meinhard, A. Menegolli, T. Nakaya, K. Nishikawa, M. Pasquali, M. Placentino, V. Serdiouk, S. Simone, S. Troquereau, S. Ueda and A. Valassi for their contributions to the experiment. We acknowledge the contributions of V. Ammosov, G. Chelkov, D. Dedovich, F. Dydak, M. Gostkin, A. Guskov, D. Khartchenko, V. Koreshev, Z. Kroumchtein, I. Nefedov, A. Semak, J. Wotschack, V. Zaets and A. Zhemchugov to the work described in this paper. The experiment was made possible by grants from the Institut Interuniversitaire des Sciences Nucle´aires and the Interuniversitair Instituut voor Kernwetenschappen (Belgium), Ministerio de Educacion y Ciencia, Grant FPA2003-06921-c02-02 and Generalitat Valenciana, grant GV00-054-1, CERN (Geneva, Switzerland), the German Bundesministerium fu¨ r Bildung und Forschung (Germany), the Istituto Nazionale di Fisica Nucleare (Italy), INR RAS (Moscow) and the Particle Physics and Astronomy Research Council (UK). We gratefully acknowledge their support.es_ES
dc.language.isoenges_ES
dc.publisherElsevieres_ES
dc.rightsopenAccesses_ES
dc.titleMeasurement of the production cross-sections of pi(+/-) in p-C and pi(+/-)-C interactions at 12 GeV/ces_ES
dc.typeartículoes_ES
dc.identifier.doi10.1016/j.astropartphys.2008.02.002-
dc.description.peerreviewedPeer reviewedes_ES
dc.relation.publisherversionhttp://dx.doi.org/10.1016/j.astropartphys.2008.02.002es_ES
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.openairetypeartículo-
item.grantfulltextopen-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
item.languageiso639-1en-
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