KamLAND neutrino spectra in energy and time: Indications for reactor power variations and constraints

被引:21
作者
Fogli, GL
Lisi, E
Palazzo, A
Rotunno, AM
机构
[1] Univ Bari, Dipartmento Fis, I-70126 Bari, Italy
[2] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy
关键词
D O I
10.1016/j.physletb.2005.07.064
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Kamioka liquid scintillator anti-neutrino detector (KamLAND) is sensitive to the neutrino event spectrum from (mainly Japanese) nuclear reactors in both the energy domain and the time domain. While the energy spectrum of KamLAND events allows the determination of the neutrino oscillation parameters, the time spectrum can be used to monitor known and unknown neutrino sources. By using available monthly-binned data on event-by-event energies in KamLAND and on reactor powers in Japan, we perform a likelihood analysis of the neutrino event spectra in energy and time, and find significant indications in favor of time variations of the known reactor sources, as compared with the hypothetical case of constant reactor neutrino flux. We also find that the KamLAND data place interesting upper limits on the power of a speculative nuclear reactor operating in the Earth's core (the so-called georeactor); such limits are strengthened by including solar neutrino constraints on the neutrino mass and mixing parameters. Our results corroborate the standard interpretation of the KamLAND signal as due to oscillating neutrinos from known reactor sources. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:80 / 92
页数:13
相关论文
共 55 条
[1]  
ABARMIM B, NUCLEX10502021
[2]   Solar neutrino flux measurements by the Soviet-American gallium experiment (SAGE) for half the 22-year solar cycle [J].
Abdurashitov, JN ;
Veretenkin, EP ;
Vermul, VM ;
Gavrin, VN ;
Girin, SV ;
Gorbachev, VV ;
Gurkina, PP ;
Zatsepin, GT ;
Ibragimova, TV ;
Kalikhov, AV ;
Knodel, TV ;
Mirmov, IN ;
Khairnasov, NG ;
Shikhin, AA ;
Yants, VE ;
Bowles, TJ ;
Teasdale, WA ;
Nico, JS ;
Wilkerson, JF ;
Cleveland, BT ;
Elliott, SR .
JOURNAL OF EXPERIMENTAL AND THEORETICAL PHYSICS, 2002, 95 (02) :181-193
[3]  
ABDURASHITOV JN, 2002, ZH EKSP TEOR FIZ, V122, P211
[4]   Measurement of the total active 8B solar neutrino flux at the sudbury neutrino observatory with enhanced neutral current sensitivity -: art. no. 181301 [J].
Ahmed, SN ;
Anthony, AE ;
Beier, EW ;
Bellerive, A ;
Biller, SD ;
Boger, J ;
Boulay, MG ;
Bowler, MG ;
Bowles, TJ ;
Brice, SJ ;
Bullard, TV ;
Chan, YD ;
Chen, M ;
Chen, X ;
Cleveland, BT ;
Cox, GA ;
Dai, X ;
Dalnoki-Veress, F ;
Doe, PJ ;
Dosanjh, RS ;
Doucas, G ;
Dragowsky, MR ;
Duba, CA ;
Duncan, FA ;
Dunford, M ;
Dunmore, JA ;
Earle, ED ;
Elliott, SR ;
Evans, HC ;
Ewan, GT ;
Farine, J ;
Fergani, H ;
Fleurot, F ;
Formaggio, JA ;
Fowler, MM ;
Frame, K ;
Fulsom, BG ;
Gagnon, N ;
Graham, K ;
Grant, DR ;
Hahn, RL ;
Hall, JC ;
Hallin, AL ;
Hallman, ED ;
Hamer, AS ;
Handler, WB ;
Hargrove, CK ;
Harvey, PJ ;
Hazama, R ;
Heeger, KM .
PHYSICAL REVIEW LETTERS, 2004, 92 (18) :181301-1
[5]   Neutrino mass parameters from Kamland, SNO, and other solar evidence [J].
Aliani, P ;
Antonelli, V ;
Picariello, M ;
Torrente-Lujan, E .
PHYSICAL REVIEW D, 2004, 69 (01)
[6]   Complete results for five years of GNO solar neutrino observations [J].
Altmann, M ;
Balata, M ;
Belli, P ;
Bellotti, E ;
Bernabei, R ;
Burkert, E ;
Cattadori, C ;
Cerulli, R ;
Chiarini, M ;
Cribier, M ;
d'Angelo, S ;
Del Re, G ;
Ebert, KH ;
von Feilitzsch, F ;
Ferrari, N ;
Hampel, W ;
Hartmann, FX ;
Henrich, E ;
Heusser, G ;
Kaether, F ;
Kiko, J ;
Kirsten, T ;
Lachenmaier, T ;
Lanfranchi, J ;
Laubenstein, M ;
Lützenkirchen, K ;
Mayer, K ;
Moegel, P ;
Motta, D ;
Nisi, S ;
Oehm, J ;
Pandola, L ;
Petricca, F ;
Potzel, W ;
Richter, H ;
Schoenert, S ;
Wallenius, M ;
Wojcik, M ;
Zanotti, L .
PHYSICS LETTERS B, 2005, 616 (3-4) :174-190
[7]  
*AM PHYS SOC, 2004, MULT NEUTR STUD REP
[8]  
ANDERSON D, ENERGETICS EARTH MIS
[9]   Measurement of neutrino oscillation with KamLAND: Evidence of spectral distortion [J].
Araki, T ;
Eguchi, K ;
Enomoto, S ;
Furuno, K ;
Ichimura, K ;
Ikeda, H ;
Inoue, K ;
Ishihara, K ;
Iwamoto, T ;
Kawashima, T ;
Kishimoto, Y ;
Koga, M ;
Koseki, Y ;
Maeda, T ;
Mitsui, T ;
Motoki, M ;
Nakajima, K ;
Ogawa, H ;
Owada, K ;
Ricol, JS ;
Shimizu, I ;
Shirai, J ;
Suekane, F ;
Suzuki, A ;
Tada, K ;
Tajima, O ;
Tamae, K ;
Tsuda, Y ;
Watanabe, H ;
Busenitz, J ;
Classen, T ;
Djurcic, Z ;
Keefer, G ;
McKinny, K ;
Mei, DM ;
Piepke, A ;
Yakushev, E ;
Berger, BE ;
Chan, YD ;
Decowski, MP ;
Dwyer, DA ;
Freedman, SJ ;
Fu, Y ;
Fujikawa, BK ;
Goldman, J ;
Gray, F ;
Heeger, KM ;
Lesko, KT ;
Luk, KB ;
Murayama, H .
PHYSICAL REVIEW LETTERS, 2005, 94 (08)
[10]  
Bahcall J.N., 1989, Neutrino Astrophysics