Generation of large flavor mixing from radiative corrections

被引:75
作者
Balaji, KRS [1 ]
Dighe, AS
Mohapatra, RN
Parida, MK
机构
[1] Inst Math Sci, Madras 600113, Tamil Nadu, India
[2] CERN, Div Theory, CH-1211 Geneva 23, Switzerland
[3] Univ Maryland, Dept Phys, College Pk, MD 20742 USA
[4] N Eastern Hill Univ, Dept Phys, Shillong 793022, Meghalaya, India
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevLett.84.5034
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We provide a model independent criterion which would guarantee a large flavor mixing of two quasi-degenerate Majorana neutrinos at the low scale, irrespective of the mixing at the high scale. We also show that such a situation is realizable for a phenomenologically interesting range of parameters of the weak scale theory. We further claim that for a similar condition to be implementable for the three generation case, the CP parity of one of the neutrinos needs to be opposite to that of the others.
引用
收藏
页码:5034 / 5037
页数:4
相关论文
共 19 条
[1]   Initial results from the CHOOZ long baseline reactor neutrino oscillation experiment [J].
Apollonio, M ;
Baldini, A ;
Bemporad, C ;
Caffau, E ;
Cei, F ;
Declais, Y ;
de Kerret, H ;
Dieterle, B ;
Etenko, A ;
George, J ;
Giannini, G ;
Grassi, M ;
Kozlov, Y ;
Kropp, W ;
Kryn, D ;
Laiman, M ;
Lane, CE ;
Lefievre, B ;
Machulin, I ;
Martemyanov, A ;
Martemyanov, V ;
Mikaelyan, L ;
Nicolo, 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, 1998, 420 (3-4) :397-404
[2]   RENORMALIZATION OF THE NEUTRINO MASS OPERATOR [J].
BABU, KS ;
LEUNG, CN ;
PANTALEONE, J .
PHYSICS LETTERS B, 1993, 319 (1-3) :191-198
[3]   Where do we stand with solar neutrino oscillations? art. no. 096016 [J].
Bahcall, JN ;
Krastev, PI ;
Smirnov, AY .
PHYSICAL REVIEW D, 1998, 58 (09)
[4]  
BARGER V, HEPPH9911524
[5]  
BILENKY SM, HEPPH9802201
[6]  
CASAS JA, HEPPH9905381
[7]   RENORMALIZATION-GROUP EQUATIONS FOR SEESAW NEUTRINO MASSES [J].
CHANKOWSKI, PH ;
PLUCIENNIK, Z .
PHYSICS LETTERS B, 1993, 316 (2-3) :312-317
[8]  
DIGHE AS, HEPPH9907423
[9]   Can neutrinos be degenerate in mass? [J].
Ellis, J ;
Lola, S .
PHYSICS LETTERS B, 1999, 458 (2-3) :310-321
[10]   Super-Kamiokande atmospheric neutrino data, zenith distributions, and three-flavor oscillations [J].
Fogli, GL ;
Lisi, E ;
Marrone, A ;
Scioscia, G .
PHYSICAL REVIEW D, 1999, 59 (03)