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...
Autores principales: | , , |
---|---|
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 |