Cargando…

Cross-sections for neutrino-nucleus interactions on $^{12}C$ and $^{16}O$

We calculate cross sections for neutral current quasi-elastic neutrino-nucleus scattering within a continuum RPA model, based on a Green's function approach. As residual interaction a Skyrme force is used. The unperturbed single particle wave functions are generated using either a Woods-Saxon p...

Descripción completa

Detalles Bibliográficos
Autores principales: Jachowicz, N, Rombouts, S, Heyde, Kris L G
Lenguaje:eng
Publicado: 1998
Materias:
Acceso en línea:http://cds.cern.ch/record/366781
_version_ 1780892940517769216
author Jachowicz, N
Rombouts, S
Heyde, Kris L G
author_facet Jachowicz, N
Rombouts, S
Heyde, Kris L G
author_sort Jachowicz, N
collection CERN
description We calculate cross sections for neutral current quasi-elastic neutrino-nucleus scattering within a continuum RPA model, based on a Green's function approach. As residual interaction a Skyrme force is used. The unperturbed single particle wave functions are generated using either a Woods-Saxon potential or a Hartree-Fock calculation. These calculations have interesting applications. Neutrinos play an important role in supernova nucleosynthesis. To obtain more information about these processes, cross sections are folded with a Fermi-Dirac distribution with temperatures of approximately 10 9 K.
id cern-366781
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1998
record_format invenio
spelling cern-3667812019-09-30T06:29:59Zhttp://cds.cern.ch/record/366781engJachowicz, NRombouts, SHeyde, Kris L GCross-sections for neutrino-nucleus interactions on $^{12}C$ and $^{16}O$Nuclear Physics - ExperimentWe calculate cross sections for neutral current quasi-elastic neutrino-nucleus scattering within a continuum RPA model, based on a Green's function approach. As residual interaction a Skyrme force is used. The unperturbed single particle wave functions are generated using either a Woods-Saxon potential or a Hartree-Fock calculation. These calculations have interesting applications. Neutrinos play an important role in supernova nucleosynthesis. To obtain more information about these processes, cross sections are folded with a Fermi-Dirac distribution with temperatures of approximately 10 9 K.CERN-EP-98-141oai:cds.cern.ch:3667811998-09-09
spellingShingle Nuclear Physics - Experiment
Jachowicz, N
Rombouts, S
Heyde, Kris L G
Cross-sections for neutrino-nucleus interactions on $^{12}C$ and $^{16}O$
title Cross-sections for neutrino-nucleus interactions on $^{12}C$ and $^{16}O$
title_full Cross-sections for neutrino-nucleus interactions on $^{12}C$ and $^{16}O$
title_fullStr Cross-sections for neutrino-nucleus interactions on $^{12}C$ and $^{16}O$
title_full_unstemmed Cross-sections for neutrino-nucleus interactions on $^{12}C$ and $^{16}O$
title_short Cross-sections for neutrino-nucleus interactions on $^{12}C$ and $^{16}O$
title_sort cross-sections for neutrino-nucleus interactions on $^{12}c$ and $^{16}o$
topic Nuclear Physics - Experiment
url http://cds.cern.ch/record/366781
work_keys_str_mv AT jachowiczn crosssectionsforneutrinonucleusinteractionson12cand16o
AT romboutss crosssectionsforneutrinonucleusinteractionson12cand16o
AT heydekrislg crosssectionsforneutrinonucleusinteractionson12cand16o