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dc.creatorRuiz Simo, I.es
dc.creatorAlbertus, C.es
dc.creatorAmaro Soriano, José Enriquees
dc.creatorBarbaro, M. B.es
dc.creatorCaballero Carretero, Juan Antonioes
dc.creatorDonnelly, T. W.es
dc.date.accessioned2017-07-17T13:06:22Z
dc.date.available2017-07-17T13:06:22Z
dc.date.issued2014-09-22
dc.identifier.citationRuiz Simo, I., Albertus, C., Amaro Soriano, J.E., Barbaro, M.B., Caballero Carretero, J.A. y Donnelly, T.W. (2014). Angular distribution in two-particle emission induced by neutrinos and electrons. Physical Review D - Particles, Fields, Gravitation and Cosmology, 90 (5), 053010-1-053010-8.
dc.identifier.issn1550-7998 (impreso)es
dc.identifier.issn1550-2368 (electrónico)es
dc.identifier.urihttp://hdl.handle.net/11441/62592
dc.description.abstractThe angular distribution of the phase space arising in two-particle emission reactions induced by electrons and neutrinos is computed in the laboratory (Lab) system by boosting the isotropic distribution in the center of mass (CM) system used in Monte Carlo generators. The Lab distribution has a singularity for some angular values, coming from the Jacobian of the angular transformation between CM and Lab systems. We recover the formula we obtained in a previous calculation for the Lab angular distribution. This is in accordance with the Monte Carlo method used to generate two-particle events for neutrino scattering [J. T. Sobczyk, Phys. Rev. C 86, 015504 (2012)]. Inversely, by performing the transformation to the CM system, it can be shown that the phase-space function, which is proportional to the two-particle-two-hole (2p-2h) hadronic tensor for a constant current operator, can be computed analytically in the frozen nucleon approximation, if Pauli blocking is absent. The results in the CM frame confirm our previous work done using an alternative approach in the Lab frame. The possibilities of using this method to compute the hadronic tensor by a boost to the CM system are analyzed.es
dc.description.sponsorshipDGI FIS2011-28738-C02-01es
dc.description.sponsorshipJunta de Andalucía QM-225 FQM-160es
dc.description.sponsorshipU.S. Department of Energy E-FC02-94ER40818es
dc.formatapplication/pdfes
dc.language.isoenges
dc.publisherAmerican Physical Societyes
dc.relation.ispartofPhysical Review D - Particles, Fields, Gravitation and Cosmology, 90 (5), 053010-1-053010-8.
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleAngular distribution in two-particle emission induced by neutrinos and electronses
dc.typeinfo:eu-repo/semantics/articlees
dcterms.identifierhttps://ror.org/03yxnpp24
dc.type.versioninfo:eu-repo/semantics/publishedVersiones
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses
dc.contributor.affiliationUniversidad de Sevilla. Departamento de Física Atómica, Molecular y Nucleares
dc.relation.projectIDFIS2011-28738-C02-01es
dc.relation.projectIDQM-225 FQM-160es
dc.relation.projectIDE-FC02-94ER40818es
dc.relation.publisherversionhttps://doi.org/10.1103/PhysRevD.90.053010es
dc.identifier.doi10.1103/PhysRevD.90.053010es
idus.format.extent8 p.es
dc.journaltitlePhysical Review D - Particles, Fields, Gravitation and Cosmologyes
dc.publication.volumen90es
dc.publication.issue5es
dc.publication.initialPage053010-1es
dc.publication.endPage053010-8es

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