Cargando…

Equalization of Response Functions of SK and SNO

We have studied the equalization of the response functions of the SK and SNO for total event rate and event rate for the energy bins. To calculate the response functions of SNO, we have used the latest theoretical values of the cross section of the neutrino-deuteron CC process. By using these new th...

Descripción completa

Detalles Bibliográficos
Autores principales: Akram, F, Rashid, H
Lenguaje:eng
Publicado: 2004
Materias:
Acceso en línea:http://cds.cern.ch/record/720006
_version_ 1780903570743230464
author Akram, F
Rashid, H
author_facet Akram, F
Rashid, H
author_sort Akram, F
collection CERN
description We have studied the equalization of the response functions of the SK and SNO for total event rate and event rate for the energy bins. To calculate the response functions of SNO, we have used the latest theoretical values of the cross section of the neutrino-deuteron CC process. By using these new theoretical values, we find that the trigger threshold of the SK at which its response function is equalized to the response function of SNO (at the trigger threshold of 6.75 MeV), is 8.5 MeV. This value is 0.1 MeV smaller than the value calculated using the old theoretical values of the cross section of neutrino-deuteron process. The use of these new theoretical values also produces a small change in the range of the energy bins where the response functions are equalized.
id cern-720006
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2004
record_format invenio
spelling cern-7200062019-09-30T06:29:59Zhttp://cds.cern.ch/record/720006engAkram, FRashid, HEqualization of Response Functions of SK and SNOAstrophysics and AstronomyWe have studied the equalization of the response functions of the SK and SNO for total event rate and event rate for the energy bins. To calculate the response functions of SNO, we have used the latest theoretical values of the cross section of the neutrino-deuteron CC process. By using these new theoretical values, we find that the trigger threshold of the SK at which its response function is equalized to the response function of SNO (at the trigger threshold of 6.75 MeV), is 8.5 MeV. This value is 0.1 MeV smaller than the value calculated using the old theoretical values of the cross section of neutrino-deuteron process. The use of these new theoretical values also produces a small change in the range of the energy bins where the response functions are equalized.EXT-2004-019oai:cds.cern.ch:7200062004-02-16
spellingShingle Astrophysics and Astronomy
Akram, F
Rashid, H
Equalization of Response Functions of SK and SNO
title Equalization of Response Functions of SK and SNO
title_full Equalization of Response Functions of SK and SNO
title_fullStr Equalization of Response Functions of SK and SNO
title_full_unstemmed Equalization of Response Functions of SK and SNO
title_short Equalization of Response Functions of SK and SNO
title_sort equalization of response functions of sk and sno
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/720006
work_keys_str_mv AT akramf equalizationofresponsefunctionsofskandsno
AT rashidh equalizationofresponsefunctionsofskandsno