Does the neutrino magnetic moment have an impact on solar neutrino physics?

被引：33

作者：

Balantekin, AB

Volpe, C

机构：

[1] Inst Phys Nucl, F-91406 Orsay, France

[2] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA

来源：

PHYSICAL REVIEW D | 2005年 / 72卷 / 03期

关键词：

D O I：

10.1103/PhysRevD.72.033008

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Solar neutrino observations coupled with the recent KamLAND data suggest that spin-flavor precession scenario does not play a major role in neutrino propagation in the solar matter. We provide approximate analytical formulas and numerical results to estimate the contribution of the spin-flavor precession, if any, to the electron neutrino survival probability when the magnetic moment and magnetic field combination is small.

引用

页码：1 / 7

页数：7

共 48 条

[1] Solar fusion cross sections [J].

Adelberger, EG ;

Austin, SM ;

Bahcall, JN ;

Balantekin, AB ;

Bogaert, G ;

Brown, LS ;

Buchmann, L ;

Cecil, FE ;

Champagne, AE ;

de Braeckeleer, L ;

Duba, CA ;

Elliott, SR ;

Freedman, SJ ;

Gai, M ;

Goldring, G ;

Gould, CR ;

Gruzinov, A ;

Haxton, WC ;

Heeger, KM ;

Henley, E ;

Johnson, CW ;

Kamionkowski, M ;

Kavanagh, RW ;

Koonin, SE ;

Kubodera, K ;

Langanke, K ;

Motobayashi, T ;

Pandharipande, V ;

Parker, P ;

Robertson, RGH ;

Rolfs, C ;

Sawyer, RF ;

Shaviv, N ;

Shoppa, TD ;

Snover, KA ;

Swanson, E ;

Tribble, RE ;

Turck-Chieze, S ;

Wilkerson, JF .

REVIEWS OF MODERN PHYSICS, 1998, 70 (04) :1265-1291

[2] Solar neutrino oscillations and bounds on neutrino magnetic moment and solar magnetic field [J].

Akhmedov, EK ;

Pulido, J .

PHYSICS LETTERS B, 2003, 553 (1-2) :7-17

[3] RESONANT AMPLIFICATION OF NEUTRINO SPIN ROTATION IN MATTER AND THE SOLAR-NEUTRINO PROBLEM [J].

AKHMEDOV, EK .

PHYSICS LETTERS B, 1988, 213 (01) :64-68

[4] ANTINEUTRINOS FROM THE SUN [J].

AKHMEDOV, EK .

PHYSICS LETTERS B, 1991, 255 (01) :84-88

[5]

Antia HM, 2000, ASTRON ASTROPHYS, V360, P335

[6] 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)

[7]

Bahcall J.N., 1989, Neutrino Astrophysics

[8] What do we (not) know theoretically about solar neutrino fluxes? [J].

Bahcall, JN ;

Pinsonneault, MH .

PHYSICAL REVIEW LETTERS, 2004, 92 (12) :121301-1

[9] Solar models: Current epoch and time dependences, neutrinos, and helioseismological properties [J].

Bahcall, JN ;

Pinsonneault, MH ;

Basu, S .

ASTROPHYSICAL JOURNAL, 2001, 555 (02) :990-1012

[10] SOLAR AND SUPERNOVA NEUTRINO PHYSICS WITH SUDBURY-NEUTRINO-OBSERVATORY [J].

BALANTEKIN, AB ;

LORETI, F .

PHYSICAL REVIEW D, 1992, 45 (04) :1059-1065

← 1 2 3 4 5 →