Bounds on the neutrino mixing angles and CP phase for an SO(10) model with lopsided mass matrices -: art. no. 013001

被引:17
作者
Albright, CH [1 ]
机构
[1] No Illinois Univ, Dept Phys, De Kalb, IL 60115 USA
[2] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
来源
PHYSICAL REVIEW D | 2005年 / 72卷 / 01期
关键词
D O I
10.1103/PhysRevD.72.013001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The bounds on the neutrino mixing angles and CP Dirac phase for an SO(10) model with lopsided mass matrices, arising from the presence of 16(H) and 16(H) Higgs representations, are studied by variation of the one real and three unknown complex input parameters for the right-handed Majorana neutrino mass matrix. The scatter plots obtained favor nearly maximal atmospheric neutrino mixing, while the reactor neutrino mixing lies in the range 10(-5) less than or similar to sin(2)theta(13) less than or similar to 1 x 10(-2) with values greater than 10(-3) most densely populated. A rather compelling scenario within the model follows, if we restrict the three unknown complex parameters to their imaginary axes and set two of them equal. We then find the scatter plots are reduced to narrow bands, as the mixing angles and CP phase become highly correlated and predictive. The bounds on the mixing angles and phase then become 0.45 less than or similar to sin(2)theta(23) less than or similar to 0.55, 0.38 less than or similar to tan(2)theta(12) less than or similar to 0.50, 0.002 less than or similar to sin(2)theta(13) less than or similar to 0.003, and 60 degrees less than or similar to +/-delta(CP) less than or similar to 85 degrees. Moreover, successful leptogenesis and subsequent baryogenesis are also obtained, with eta(B) increasing from (2.7 to 6.3) x 10(-10) as sin(2)theta(23) increases from 0.45 to 0.55.
引用
收藏
页码:1 / 12
页数:12
相关论文
共 76 条
[1]  
Aalseth C., HEPPH0412300
[2]   Measurement of the solar neutrino capture rate by SAGE and implications for neutrino oscillations in vacuum [J].
Abdurashitov, JN ;
Bowles, TJ ;
Cherry, ML ;
Cleveland, BT ;
Davis, R ;
Elliott, SR ;
Gavrin, VN ;
Girin, SV ;
Gorbachev, VV ;
Ibragimova, TV ;
Kalikhov, AV ;
Khairnasov, NG ;
Knodel, TV ;
Lande, K ;
Mirmov, IN ;
Nico, JS ;
Shikhin, AA ;
Teasdale, WA ;
Veretenkin, EP ;
Vermul, VM ;
Wark, DL ;
Wildenhain, PS ;
Wilkerson, JF ;
Yants, VE ;
Zatsepin, GT .
PHYSICAL REVIEW LETTERS, 1999, 83 (23) :4686-4689
[3]   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
[4]   Indications of neutrino oscillation in a 250 km long-baseline experiment [J].
Ahn, MH ;
Aoki, S ;
Bhang, H ;
Boyd, S ;
Casper, D ;
Choi, JH ;
Fukuda, S ;
Fukuda, Y ;
Gajewski, W ;
Hara, T ;
Hasegawa, M ;
Hasegawa, T ;
Hayato, Y ;
Hill, J ;
Ichikawa, AK ;
Ikeda, A ;
Inagaki, T ;
Ishida, T ;
Ishii, T ;
Ishitsuka, M ;
Itow, Y ;
Iwashita, T ;
Jang, HI ;
Jang, JS ;
Jeon, EJ ;
Jung, CK ;
Kajita, T ;
Kameda, J ;
Kaneyuki, K ;
Kato, I ;
Kearns, E ;
Kibayashi, A ;
Kielczewska, D ;
Kobayashi, K ;
Kim, BJ ;
Kim, CO ;
Kim, JY ;
Kim, SB ;
Kobayashi, T ;
Kohama, M ;
Koshio, Y ;
Kropp, WR ;
Learned, JG ;
Lim, SH ;
Lim, IT ;
Maesaka, H ;
Martens, K ;
Maruyama, T ;
Matsuno, S ;
Mauger, C .
PHYSICAL REVIEW LETTERS, 2003, 90 (04) :5
[5]   Minimality condition and atmospheric neutrino oscillations [J].
Albright, CH ;
Babu, KS ;
Barr, SM .
PHYSICAL REVIEW LETTERS, 1998, 81 (06) :1167-1170
[6]   Explicit SO(10) supersymmetric grand unified model for the Higgs and Yukawa sectors [J].
Albright, CH ;
Barr, SM .
PHYSICAL REVIEW LETTERS, 2000, 85 (02) :244-247
[7]   Resonant leptogenesis in a predictive SO(10) grand unified model -: art. no. 033013 [J].
Albright, CH ;
Barr, SM .
PHYSICAL REVIEW D, 2004, 70 (03) :033013-1
[8]   Leptogenesis in the type III seesaw mechanism [J].
Albright, CH ;
Barr, SM .
PHYSICAL REVIEW D, 2004, 69 (07) :6
[9]   Normal vs. inverted hierarchy in type I seesaw models [J].
Albright, CH .
PHYSICS LETTERS B, 2004, 599 (3-4) :285-293
[10]   SO(10) GUT models and their present success in explaining mass and mixing data [J].
Albright, CH .
INTERNATIONAL JOURNAL OF MODERN PHYSICS A, 2003, 18 (22) :3947-3955