Physics potential of the CERN-MEMPHYS neutrino oscillation project

被引:67
作者
Campagne, Jean-Eric [1 ]
Maltoni, Michele
Mezzetto, Mauro
Schwetz, Thomas
机构
[1] Univ Paris 11, Lab Accelerateur Lineaire, IN2P3, CNRS, BP 34, F-91898 Orsay, France
[2] Abdus Salaam Int Ctr Theoret Phys, I-31014 Trieste, Italy
[3] Univ Autonoma Madrid, Dept Fis Teor, Fac Ciencias, E-28049 Madrid, Spain
[4] Univ Autonoma Madrid, Inst Fis Teor, Fac Ciencias, E-28049 Madrid, Spain
[5] Ist Nazl Fis Nucl, Sez Padova, I-35100 Padua, Italy
[6] Scuola Int Super Studi Avanzati, I-34014 Trieste, Italy
[7] CERN, Dept Phys, Div Theory, CH-1211 Geneva 23, Switzerland
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2007年 / 04期
关键词
neutrino physics; solar and atmospheric neutrinos;
D O I
10.1088/1126-6708/2007/04/003
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We consider the physics potential of CERN based neutrino oscillation experiments consisting of a Beta Beam (beta B) and a Super Beam (SPL) sending neutrinos to MEMPHYS, a 440 kt water. Cerenkov detector at Frejus, at a distance of 130 km from CERN. The theta(13) discovery reach and the sensitivity to CP violation are investigated, including a detailed discussion of parameter degeneracies and systematical errors. For SPL sensitivities similar to the ones of the phase II of the T2K experiment (T2HK) are obtained, whereas the beta B may reach significantly better sensitivities, depending on the achieved number of total ion decays. The results for the CERN-MEMPHYS experiments are less affected by systematical uncertainties than T2HK. We point out that by a combination of data from beta B and SPL a measurement with antineutrinos is not necessary and hence the same physics results can be obtained within about half of the measurement time compared to one single experiment. Furthermore, it is shown how including data from atmospheric neutrinos in the MEMPHYS detector allows to resolve parameter degeneracies and, in particular, provides sensitivity to the neutrino mass hierarchy and the octant of theta(23).
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页数:35
相关论文
共 97 条
[1]  
ABDURASHITOV JN, 2002, SOV PHYS JETP, V95, P181
[2]  
Acquistapace G., CERN9802
[3]  
Aguilar A, 2001, PHYS REV D, V64, DOI 10.1103/PhysRevD.64.112007
[4]   Electron energy spectra, fluxes, and day-night asymmetries of 8B solar neutrinos from measurements with NaCl dissolved in the heavy-water detector at the Sudbury Neutrino Observatory -: art. no. 055502 [J].
Aharmim, B ;
Ahmed, SN ;
Anthony, AE ;
Beier, EW ;
Bellerive, A ;
Bergevin, M ;
Biller, SD ;
Boger, J ;
Boulay, MG ;
Bowler, MG ;
Bullard, TV ;
Chan, YD ;
Chen, M ;
Chen, X ;
Cleveland, BT ;
Cox, GA ;
Currat, CA ;
Dai, X ;
Dalnoki-Veress, F ;
Deng, H ;
Doe, PJ ;
Dosanjh, RS ;
Doucas, G ;
Duba, CA ;
Duncan, FA ;
Dunford, M ;
Dunmore, JA ;
Earle, ED ;
Elliott, SR ;
Evans, HC ;
Ewan, GT ;
Farine, J ;
Fergani, H ;
Fleurot, F ;
Formaggio, JA ;
Frame, K ;
Frati, W ;
Fulsom, BG ;
Gagnon, N ;
Graham, K ;
Grant, DR ;
Hahn, RL ;
Hall, JC ;
Hallin, AL ;
Hallman, ED ;
Handler, WB ;
Hargrove, CK ;
Harvey, PJ ;
Hazama, R ;
Heeger, KM .
PHYSICAL REVIEW C, 2005, 72 (05)
[5]   Measurement of day and night neutrino energy spectra at SNO and constraints on neutrino mixing parameters -: art. no. 011302 [J].
Ahmad, QR ;
Allen, RC ;
Andersen, TC ;
Anglin, JD ;
Barton, JC ;
Beier, EW ;
Bercovitch, M ;
Bigu, J ;
Biller, SD ;
Black, RA ;
Blevis, I ;
Boardman, RJ ;
Boger, J ;
Bonvin, E ;
Boulay, MG ;
Bowler, MG ;
Bowles, TJ ;
Brice, SJ ;
Browne, MC ;
Bullard, TV ;
Bühler, G ;
Cameron, J ;
Chan, YD ;
Chen, HH ;
Chen, M ;
Chen, X ;
Cleveland, BT ;
Clifford, ETH ;
Cowan, JHM ;
Cowen, DF ;
Cox, GA ;
Dai, X ;
Dalnoki-Veress, F ;
Davidson, WF ;
Doe, PJ ;
Doucas, G ;
Dragowsky, MR ;
Duba, CA ;
Duncan, FA ;
Dunford, M ;
Dunmore, JA ;
Earle, ED ;
Elliott, SR ;
Evans, HC ;
Ewan, GT ;
Farine, J ;
Fergani, H ;
Ferraris, AP ;
Ford, RJ ;
Formaggio, JA .
PHYSICAL REVIEW LETTERS, 2002, 89 (01)
[6]   Atmospheric neutrinos at super-Kamiokande and parametric resonance in neutrino oscillations [J].
Akhmedov, EK ;
Dighe, A ;
Lipari, P ;
Smirnov, AY .
NUCLEAR PHYSICS B, 1999, 542 (1-2) :3-30
[7]   Parametric resonance of neutrino oscillations and passage of solar and atmospheric neutrinos through the earth [J].
Akhmedov, EK .
NUCLEAR PHYSICS B, 1999, 538 (1-2) :25-51
[8]  
ALBRIGTH C, NEUTRINO FACTORY BET, P91601
[9]  
ALBROW MG, PHYS FERMILAB PROTON, P91601
[10]   Evidence for muon neutrino oscillation in an accelerator-based experiment [J].
Aliu, E ;
Andringa, S ;
Aoki, S ;
Argyriades, J ;
Asakura, K ;
Ashie, R ;
Berns, H ;
Bhang, H ;
Blondel, A ;
Borghi, S ;
Bouchez, J ;
Burguet-Castell, J ;
Casper, D ;
Cavata, C ;
Cervera, A ;
Cho, KO ;
Choi, JH ;
Dore, U ;
Espinal, X ;
Fechner, M ;
Fernandez, E ;
Fukuda, Y ;
Gomez-Cadenas, J ;
Gran, R ;
Hara, T ;
Hasegawa, M ;
Hasegawa, T ;
Hayashi, K ;
Hayato, Y ;
Helmer, RL ;
Hill, J ;
Hiraide, K ;
Hosaka, J ;
Ichikawa, AK ;
Iinuma, M ;
Ikeda, A ;
Inagaki, T ;
Ishida, T ;
Ishihara, K ;
Ishii, T ;
Ishitsuka, M ;
Itow, Y ;
Iwashita, T ;
Jang, HI ;
Jeon, EJ ;
Jeong, IS ;
Joo, K ;
Jover, G ;
Jung, CK ;
Kajita, T .
PHYSICAL REVIEW LETTERS, 2005, 94 (08)