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Low-energy neutrino-photon inelastic interactions

The computation of the polarized amplitudes and cross section of the processes $\gamma\nu\to\gamma\gamma \nu$, $\gamma\gamma \to \gamma\nu\bar\nu$ and $\nu\bar\nu \to \gamma\gamma\gamma$ is described. We used an effective lagrangian approach for energies below the threshold for $e^+e^-$ pair product...

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Detalles Bibliográficos
Autores principales: Abada, A., Matias, Joaquim, Pittau, R.
Lenguaje:eng
Publicado: 1999
Materias:
Acceso en línea:http://cds.cern.ch/record/387799
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author Abada, A.
Matias, Joaquim
Pittau, R.
author_facet Abada, A.
Matias, Joaquim
Pittau, R.
author_sort Abada, A.
collection CERN
description The computation of the polarized amplitudes and cross section of the processes $\gamma\nu\to\gamma\gamma \nu$, $\gamma\gamma \to \gamma\nu\bar\nu$ and $\nu\bar\nu \to \gamma\gamma\gamma$ is described. We used an effective lagrangian approach for energies below the threshold for $e^+e^-$ pair production and the complete computation at higher energies for application in supernova dynamics. Leading contributions of physics beyond the SM are also commented.
id cern-387799
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1999
record_format invenio
spelling cern-3877992023-03-14T16:59:00Zhttp://cds.cern.ch/record/387799engAbada, A.Matias, JoaquimPittau, R.Low-energy neutrino-photon inelastic interactionsParticle Physics - PhenomenologyThe computation of the polarized amplitudes and cross section of the processes $\gamma\nu\to\gamma\gamma \nu$, $\gamma\gamma \to \gamma\nu\bar\nu$ and $\nu\bar\nu \to \gamma\gamma\gamma$ is described. We used an effective lagrangian approach for energies below the threshold for $e^+e^-$ pair production and the complete computation at higher energies for application in supernova dynamics. Leading contributions of physics beyond the SM are also commented.The computation of the polarized amplitudes and cross section of the processes $\gamma\nu\to\gamma\gamma \nu$, $\gamma\gamma \to \gamma\nu\bar\nu$ and $\nu\bar\nu \to \gamma\gamma\gamma$ is described. We used an effective lagrangian approach for energies below the threshold for $e^+e^-$ pair production and the complete computation at higher energies for application in supernova dynamics. Leading contributions of physics beyond the SM are also commented.hep-ph/9905380CERN-TH-99-134CERN-TH-99-134oai:cds.cern.ch:3877991999-05-19
spellingShingle Particle Physics - Phenomenology
Abada, A.
Matias, Joaquim
Pittau, R.
Low-energy neutrino-photon inelastic interactions
title Low-energy neutrino-photon inelastic interactions
title_full Low-energy neutrino-photon inelastic interactions
title_fullStr Low-energy neutrino-photon inelastic interactions
title_full_unstemmed Low-energy neutrino-photon inelastic interactions
title_short Low-energy neutrino-photon inelastic interactions
title_sort low-energy neutrino-photon inelastic interactions
topic Particle Physics - Phenomenology
url http://cds.cern.ch/record/387799
work_keys_str_mv AT abadaa lowenergyneutrinophotoninelasticinteractions
AT matiasjoaquim lowenergyneutrinophotoninelasticinteractions
AT pittaur lowenergyneutrinophotoninelasticinteractions