Neutrino mass spectrum and future beta decay experiments

被引:77
作者
Farzan, Y
Peres, OLG
Smirnov, AY
机构
[1] Scuola Int Super Studi Avanzati, I-34014 Trieste, Italy
[2] Univ Estadual Campinas, UNICAMP, Inst Fis Gleb Wataghin, BR-13083970 Campinas, SP, Brazil
[3] Abdus Salam Int Ctr Theoret Phys, I-34100 Trieste, Italy
[4] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
基金
巴西圣保罗研究基金会;
关键词
neutrino masses and mixing; beta decay;
D O I
10.1016/S0550-3213(01)00361-3
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 study the discovery potential of future beta decay experiments on searches for the neutrino mass in the sub-eV range. and, in particular, KATRIN experiment with sensitivity m > 0.3 eV. Effects of neutrino mass and mixing on the beta decay spectrum in the neutrino schemes which explain the solar and atmospheric neutrino data are discussed. The schemes which lead to observable effects contain one or two sets of quasi-degenerate states. Future beta decay measurements will allow to check the three-neutrino scheme with mass degeneracy, moreover, the possibility appears to measure the CP-violating Majorana phase. Effects in the four-neutrino schemes which can also explain the LSND data are strongly restricted by the results of Bugey and CHOOZ oscillation experiments: apart from bending of the spectrum and the shift of the end point one expects appearance of small kink of (< 2%) size or suppressed tail after bending of the spectrum with rate below 2% of the expected rate for zero neutrino mass. We consider possible implications of future beta decay experiments for the neutrino mass spectrum, the determination of the absolute scale of neutrino mass and for establishing the nature of neutrinos. We show that beta decay measurements in combination with data from the oscillation and double beta decay experiments will allow to establish the structure of the scheme (hierarchical or non-hierarchical), the type of the hierarchy or ordering of states (normal or inverted) and to measure the relative CP-violating phase in the solar pair of states. (C) 2001 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:59 / 97
页数:39
相关论文
共 84 条
[1]   SEARCH FOR NEUTRINO OSCILLATIONS AT 15, 40 AND 95 METERS FROM A NUCLEAR-POWER-REACTOR AT BUGEY [J].
ACHKAR, B ;
ALEKSAN, R ;
AVENIER, M ;
BAGIEU, G ;
BOUCHEZ, J ;
BRISSOT, R ;
CAVAIGNAC, JF ;
COLLOT, J ;
COUSINOU, MC ;
CUSSONNEAU, JP ;
DECLAIS, Y ;
DUFOUR, Y ;
FAVIER, J ;
GARCIAZ, F ;
KAJFASZ, E ;
DEKERRET, H ;
KOANG, DH ;
LEFIEVRE, B ;
LESQUOY, E ;
MALLET, J ;
METREF, A ;
NAGY, E ;
PESSARD, H ;
PIERRE, F ;
OBOLENSKY, M ;
STUTZ, A ;
WUTHRICK, JP .
NUCLEAR PHYSICS B, 1995, 434 (03) :503-532
[2]   Constraints on mixing angles of Majorana neutrinos [J].
Adhikari, R ;
Rajasekaran, G .
PHYSICAL REVIEW D, 2000, 61 (03)
[3]  
AGUILAR A, HEPEX0104049
[4]   Limits on neutrino oscillations from the CHOOZ experiment [J].
Apollonio, I ;
Baldini, A ;
Bemporad, C ;
Caffau, E ;
Cei, F ;
Déclais, Y ;
de Kerret, H ;
Dieterle, B ;
Etenko, A ;
George, J ;
Giannini, G ;
Grassi, M ;
Kozlov, Y ;
Kropp, W ;
Kryn, D ;
Laiman, M ;
Lane, CE ;
Lefièvre, B ;
Machulin, I ;
Martemyanov, A ;
Martemyanov, V ;
Mikaelyan, L ;
Nicolò, D ;
Obolensky, M ;
Pazzi, R ;
Pieri, G ;
Price, L ;
Riley, S ;
Reeder, R ;
Sabelnikov, A ;
Santin, G ;
Skorokhvatov, M ;
Sobel, H ;
Steele, J ;
Steinberg, R ;
Sukhotin, S ;
Tomshaw, S ;
Veron, D ;
Vyrodov, V .
PHYSICS LETTERS B, 1999, 466 (2-4) :415-430
[5]  
ASEEV V, 2001, INT WORKSH NEUTR MAS
[6]   Correlations of solar neutrino observables for SNO [J].
Bahcall, JN ;
Krastev, PI ;
Smirnov, AY .
PHYSICAL REVIEW D, 2001, 63 (05)
[7]  
BALAJI KRS, HEPPH0101005
[8]   Majorana neutrino masses from neutrinoless double beta decay and cosmology [J].
Barger, V ;
Whisnant, K .
PHYSICS LETTERS B, 1999, 456 (2-4) :194-200
[9]   Resolving the solar neutrino problem with KamLAND [J].
Barger, V ;
Marfatia, D ;
Wood, BP .
PHYSICS LETTERS B, 2001, 498 (1-2) :53-61
[10]  
BARGER V, HEPPH0104166