Abstract
A comprehensive study of the atmospheric neutrino flux in the energy region from sub-GeV up to several TeV using the Super-Kamiokande (SK) water Cherenkov detector is presented in this paper. The energy and azimuthal spectra, and variation over time, of the atmospheric νe+νe and νμ+νμ fluxes are measured. The energy spectra are obtained using an iterative unfolding method by combining various event topologies with differing energy responses. The azimuthal spectra depending on energy and zenith angle, and their modulation by geomagnetic effects, are also studied. A predicted east-west asymmetry is observed in both the νe and νμ samples at 8.0σ and 6.0σ significance, respectively, and an indication that the asymmetry dipole angle changes depending on the zenith angle was seen at the 2.2σ level. The measured energy and azimuthal spectra are consistent with the current flux models within the estimated systematic uncertainties. A study of the long-term correlation between the atmospheric neutrino flux and the solar magnetic activity cycle is performed, and a weak preference for a correlation was seen at the 1.1σ level, using SK-I-SK-IV data spanning a 20-year period. For several particularly strong solar activity periods, corresponding to Forbush decrease events, no theoretical prediction is available but a deviation below the typical neutrino event rate is seen at the 2.4σ level. The seasonal modulation of the neutrino flux is also examined, but the change in flux at the SK site is predicted to be negligible, and, as expected, no evidence for a seasonal correlation is seen.
| Original language | English |
|---|---|
| Article number | 052001 |
| Journal | Physical Review D |
| Volume | 94 |
| Issue number | 5 |
| DOIs | |
| Publication status | Published - Sep 2 2016 |
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ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)
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Measurements of the atmospheric neutrino flux by Super-Kamiokande : Energy spectra, geomagnetic effects, and solar modulation. / (Super-Kamiokande Collaboration).
In: Physical Review D, Vol. 94, No. 5, 052001, 02.09.2016.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Measurements of the atmospheric neutrino flux by Super-Kamiokande
T2 - Energy spectra, geomagnetic effects, and solar modulation
AU - (Super-Kamiokande Collaboration)
AU - Richard, E.
AU - Okumura, K.
AU - Abe, K.
AU - Haga, Y.
AU - Hayato, Y.
AU - Ikeda, M.
AU - Iyogi, K.
AU - Kameda, J.
AU - Kishimoto, Y.
AU - Miura, M.
AU - Moriyama, S.
AU - Nakahata, M.
AU - Nakajima, T.
AU - Nakano, Y.
AU - Nakayama, S.
AU - Orii, A.
AU - Sekiya, H.
AU - Shiozawa, M.
AU - Takeda, A.
AU - Tanaka, H.
AU - Tomura, T.
AU - Wendell, R. A.
AU - Akutsu, R.
AU - Irvine, T.
AU - Kajita, T.
AU - Kaneyuki, K.
AU - Nishimura, Y.
AU - Labarga, L.
AU - Fernandez, P.
AU - Gustafson, J.
AU - Kachulis, C.
AU - Kearns, E.
AU - Raaf, J. L.
AU - Stone, J. L.
AU - Sulak, L. R.
AU - Berkman, S.
AU - Nantais, C. M.
AU - Tanaka, H. A.
AU - Tobayama, S.
AU - Goldhaber, M.
AU - Kropp, W. R.
AU - Mine, S.
AU - Weatherly, P.
AU - Smy, M. B.
AU - Sobel, H. W.
AU - Takhistov, V.
AU - Ganezer, K. S.
AU - Ishino, Hirokazu
AU - Koshio, Yusuke
AU - Sakuda, Makoto
PY - 2016/9/2
Y1 - 2016/9/2
N2 - A comprehensive study of the atmospheric neutrino flux in the energy region from sub-GeV up to several TeV using the Super-Kamiokande (SK) water Cherenkov detector is presented in this paper. The energy and azimuthal spectra, and variation over time, of the atmospheric νe+νe and νμ+νμ fluxes are measured. The energy spectra are obtained using an iterative unfolding method by combining various event topologies with differing energy responses. The azimuthal spectra depending on energy and zenith angle, and their modulation by geomagnetic effects, are also studied. A predicted east-west asymmetry is observed in both the νe and νμ samples at 8.0σ and 6.0σ significance, respectively, and an indication that the asymmetry dipole angle changes depending on the zenith angle was seen at the 2.2σ level. The measured energy and azimuthal spectra are consistent with the current flux models within the estimated systematic uncertainties. A study of the long-term correlation between the atmospheric neutrino flux and the solar magnetic activity cycle is performed, and a weak preference for a correlation was seen at the 1.1σ level, using SK-I-SK-IV data spanning a 20-year period. For several particularly strong solar activity periods, corresponding to Forbush decrease events, no theoretical prediction is available but a deviation below the typical neutrino event rate is seen at the 2.4σ level. The seasonal modulation of the neutrino flux is also examined, but the change in flux at the SK site is predicted to be negligible, and, as expected, no evidence for a seasonal correlation is seen.
AB - A comprehensive study of the atmospheric neutrino flux in the energy region from sub-GeV up to several TeV using the Super-Kamiokande (SK) water Cherenkov detector is presented in this paper. The energy and azimuthal spectra, and variation over time, of the atmospheric νe+νe and νμ+νμ fluxes are measured. The energy spectra are obtained using an iterative unfolding method by combining various event topologies with differing energy responses. The azimuthal spectra depending on energy and zenith angle, and their modulation by geomagnetic effects, are also studied. A predicted east-west asymmetry is observed in both the νe and νμ samples at 8.0σ and 6.0σ significance, respectively, and an indication that the asymmetry dipole angle changes depending on the zenith angle was seen at the 2.2σ level. The measured energy and azimuthal spectra are consistent with the current flux models within the estimated systematic uncertainties. A study of the long-term correlation between the atmospheric neutrino flux and the solar magnetic activity cycle is performed, and a weak preference for a correlation was seen at the 1.1σ level, using SK-I-SK-IV data spanning a 20-year period. For several particularly strong solar activity periods, corresponding to Forbush decrease events, no theoretical prediction is available but a deviation below the typical neutrino event rate is seen at the 2.4σ level. The seasonal modulation of the neutrino flux is also examined, but the change in flux at the SK site is predicted to be negligible, and, as expected, no evidence for a seasonal correlation is seen.
UR - http://www.scopus.com/inward/record.url?scp=84990859007&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84990859007&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.94.052001
DO - 10.1103/PhysRevD.94.052001
M3 - Article
AN - SCOPUS:84990859007
VL - 94
JO - Physical Review D
JF - Physical Review D
SN - 2470-0010
IS - 5
M1 - 052001
ER -