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dc.contributor.authorYahlali, Nadia-
dc.contributor.authorDíaz Medina, José-
dc.contributor.authorMatulewicz, T.-
dc.contributor.authorDelagrange, H.-
dc.contributor.authorPiasecki, K.-
dc.contributor.authorD'Enterria, D. G.-
dc.contributor.authorFernández Moreno, Francisco-
dc.contributor.authorKugler, A.-
dc.contributor.authorLohner, H.-
dc.contributor.authorMartínez García, Ginés-
dc.contributor.authorOstendorf, R. W.-
dc.contributor.authorSchutz, Y.-
dc.contributor.authorTlusty, P.-
dc.contributor.authorTurrisi, R.-
dc.contributor.authorWagner, V.-
dc.contributor.authorWilschut, H. W.-
dc.date.accessioned2010-09-30T12:19:43Z-
dc.date.available2010-09-30T12:19:43Z-
dc.date.issued2010-05-28-
dc.identifier.citationPhysical Review - Section C - Nuclear Physics 81 (5): 054912 (2010)en_US
dc.identifier.issn0556-2813-
dc.identifier.urihttp://hdl.handle.net/10261/28111-
dc.description.abstractDifferential cross sections of neutral pions emitted in Ta-181+Au-197 collisions at a beam energy of 39.5A Me V have been measured with the two-arm photon spectrometer (TAPS). The kinetic energy and transverse momentum spectra of neutral pions cannot be properly described in the framework of the thermal model, nor when the reabsorption of pions is accounted for in a phenomenological model. However, high energy and high momentum tails of the pion spectra can be well fitted through thermal distributions with unexpectedly soft temperature parameters below 10 MeV.en_US
dc.description.sponsorshipWe thank the GANIL accelerator staff for delivering a high quality beam. This research was supported in part by the Polish State Commitee for Scientific Research (KBN) under grant 2P03B 102 25, and by the Spanish Ministerio de Educación y Ciencia under contract FPA2006-12120-C03-02.en_US
dc.format.extent207777 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoengen_US
dc.publisherAmerican Physical Societyen_US
dc.rightsopenAccessen_US
dc.titleEmission patterns of neutral pions in 40A MeV Ta plus Au reactionsen_US
dc.typeartículoen_US
dc.identifier.doi10.1103/PhysRevC.81.054912-
dc.description.peerreviewedPeer revieweden_US
dc.relation.publisherversionhttp://dx.doi.org/10.1103/PhysRevC.81.054912en_US
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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