新山 雅之
   所属   京都産業大学  理学部 物理科学科
   職種   教授
発行・発表の年月 2013/10
形態種別 その他
標題 Proposal: A Search for Sterile Neutrino at J-PARC Materials and Life Science Experimental Facility
執筆形態 その他
著者・共著者 M. Harada,S. Hasegawa,Y. Kasugai,S. Meigo,K. Sakai,S. Sakamoto,K. Suzuya,E. Iwai,T. Maruyama,K. Nishikawa,R. Ohta,M. Niiyama,S. Ajimura,T. Hiraiwa,T. Nakano,M. Nomachi,T. Shima,T. J. C. Bezerra,E. Chauveau,T. Enomoto,H. Furuta,H. Sakai,F. Suekane,M. Yeh,G. T. Garvey,W. C. Louis,G. B. Mills,R. Van de Water
概要 We propose a definite search for sterile neutrinos at the J-PARC Materials
and Life Science Experimental Facility (MLF). With the 3 GeV Rapid Cycling
Synchrotron (RCS) and spallation neutron target, an intense neutrino beam from
muon decay at rest (DAR) is available. Neutrinos come from \mu+ decay, and the
oscillation to be searched for is (anti \nu \mu -> anti \nu e) which is
detected by the inverse \beta decay interaction (anti \nu e + p -> e+ + n),
followed by a gamma from neutron capture.
The unique features of the proposed experiment, compared with the LSND and
experiments using horn focused beams, are;
(1) The pulsed beam with about 600 ns spill width from J-PARC RCS and muon
long lifetime allow us to select neutrinos from \mu DAR only.
(2) Due to nuclear absorption of \pi- and \mu-, neutrinos from \mu- decay are
suppressed to about the $10^{-3}$ level.
(3) Neutrino cross sections are well known. The inverse \beta decay cross
section is known to be a few percent accuracy.
(4) The neutrino energy can be calculated from positron energy by adding ~1.8
MeV.
(5) The anti \nu \mu and \nu e fluxes have different and well defined
spectra. This allows us to separate oscillated signals from those due to \mu-
decay contamination.
We propose to proceed with the oscillation search in steps since the region
of \Delta m^2 to be searched can be anywhere between sub-eV^2 to several tens
of eV^2. We start to examine the large \Delta m^2 region, which can be done
with short baseline at first. At close distance to the MLF target gives a high
neutrino flux, and allows us to use relatively small detector.
If no definitive positive signal is found, a future option exists to cover
small \Delta m^2 region. This needs a relatively long baseline and requires a
large detector to compensate for the reduced neutrino flux.
PermalinkURL http://arxiv.org/abs/1310.1437v1
researchmap用URL http://arxiv.org/pdf/1310.1437v1