Searching for the Mikheyev-Smirnov-Wolfenstein enhancement

被引：32

作者：

Gelb, JM

Kwong, W

Rosen, SP

机构：

[1] Department of Physics, The University of Texas at Arlington, Arlington, TX

来源：

PHYSICAL REVIEW LETTERS | 1997年 / 78卷 / 12期

关键词：

D O I：

10.1103/PhysRevLett.78.2296

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We point out that the length scale associated with the MSW effect is the radius of the Earth. Therefore to verify matter enhancement of neutrino oscillations, it will be necessary to study neutrinos passing through the Earth. For the parameters of MSW solutions to the solar neutrino problem, the only detectable effects occur in a narrow band of energies from 5 to 10 MeV. We propose that serious consideration be given to mounting an experiment at a location within 9.5 degrees of the equator.

引用

页码：2296 / 2299

页数：4

共 34 条

[1] A HEAVY-WATER DETECTOR TO RESOLVE THE SOLAR NEUTRINO PROBLEM [J].

AARDSMA, G ;

ALLEN, RC ;

ANGLIN, JD ;

BERCOVITCH, M ;

CARTER, AL ;

CHEN, HH ;

DAVIDSON, WF ;

DOE, PJ ;

EARLE, ED ;

EVANS, HC ;

EWAN, GT ;

HALLMAN, ED ;

HARGROVE, CK ;

JAGAM, P ;

KESSLER, D ;

LEE, HW ;

LESLIE, JR ;

MACARTHUR, JD ;

MAK, HB ;

MCDONALD, AB ;

MCLATCHIE, W ;

ROBERTSON, BC ;

SIMPSON, JJ ;

SINCLAIR, D ;

SKENSVED, P ;

STOREY, RS .

PHYSICS LETTERS B, 1987, 194 (02) :321-325

[2] FIRST RESULTS FROM THE CR-51 NEUTRINO SOURCE EXPERIMENT WITH THE GALLEX DETECTOR [J].

ANSELMANN, P ;

FOCKENBROCK, R ;

HAMPEL, W ;

HEUSSER, G ;

KIKO, J ;

KIRSTEN, T ;

LAUBENSTEIN, M ;

PERNICKA, E ;

PEZZONI, S ;

RONN, U ;

SANN, M ;

SPIELKER, F ;

WINK, R ;

WOJCIK, M ;

AMMON, R ;

EBERT, KH ;

FRITSCH, T ;

HEIDT, D ;

HENRICH, E ;

SCHLOSSER, C ;

STIEGLITZ, L ;

WEIRICH, F ;

BALATA, M ;

LALLA, H ;

BELLOTTI, E ;

CATTADORI, C ;

CREMONESI, O ;

FERRARI, N ;

FIORINI, E ;

ZANOTTI, L ;

ALTMANN, M ;

VONFEILITZSCH, F ;

MOSSBAUER, R ;

SCHANDA, U ;

BERTHOMIEU, G ;

SCHATZMAN, E ;

CARMI, I ;

DOSTROVSKY, I ;

BACCI, C ;

BELLI, P ;

BERNABEI, R ;

DANGELO, S ;

PAOLUZI, L ;

BEVILACQUA, A ;

CHARBIT, S ;

CRIBIER, M ;

DUPONT, G ;

GOSSET, L ;

RICH, J ;

SPIRO, M .

PHYSICS LETTERS B, 1995, 342 (1-4) :440-450

[3]

Bahcall J.N., 1989, Neutrino Astrophysics

[4] How well do we (and will we) know solar neutrino fluxes and oscillation parameters? [J].

Bahcall, JN ;

Krastev, PI .

PHYSICAL REVIEW D, 1996, 53 (08) :4211-4225

[5]

BAHCALL JN, 1994, PHYS LETT B, V338, P276, DOI 10.1016/0370-2693(94)91378-1

[6] MIKHEYEV-SMIRNOV-WOLFENSTEIN EFFECT IN ELECTRON-NEUTRINO SCATTERING EXPERIMENTS [J].

BAHCALL, JN ;

GELB, JM ;

ROSEN, SP .

PHYSICAL REVIEW D, 1987, 35 (10) :2976-2982

[7] IMPLICATION OF GALLIUM RESULTS ON THE POSSIBILITY OF OBSERVING DAY-NIGHT MATTER OSCILLATIONS AT SNO, SUPER-KAMIOKANDE, AND BOREXINO [J].

BALTZ, AJ ;

WENESER, J .

PHYSICAL REVIEW D, 1994, 50 (09) :5971-5979

[8] EFFECT OF TRANSMISSION THROUGH THE EARTH ON NEUTRINO OSCILLATIONS [J].

BALTZ, AJ ;

WENESER, J .

PHYSICAL REVIEW D, 1987, 35 (02) :528-535

[9] MATTER OSCILLATIONS - NEUTRINO TRANSFORMATION IN THE SUN AND REGENERATION IN THE EARTH [J].

BALTZ, AJ ;

WENESER, J .

PHYSICAL REVIEW D, 1988, 37 (12) :3364-3377

[10] POSSIBILITY OF RADIOCHEMICAL OBSERVATION OF DAY-NIGHT MATTER OSCILLATIONS IN LIGHT OF CURRENT SOLAR-NEUTRINO RESULTS [J].

BALTZ, AJ ;

WENESER, J .

PHYSICAL REVIEW D, 1995, 51 (07) :3960-3961

← 1 2 3 4 →