GALLEX solar neutrino observations: Results for GALLEX III

被引：0

作者：

Hampel, W

Heusser, G

Kiko, J

Kirsten, T

Laubenstein, M

Pernicka, E

Rau, W

Ronn, U

Schlosser, C

Wojcik, M

Zakharov, Y

vonAmmon, R

Ebert, KH

Fritsch, T

Heidt, D

Henrich, E

Stieglitz, L

Weirich, F

Balata, M

Sann, M

Hartmann, FX

Bellotti, E

Cattadori, C

Cremonesi, O

Ferrari, N

Fiorini, E

Zanotti, L

Altmann, M

vonFeilitzsch, F

Mossbauer, R

Berthomieu, G

Schatzman, E

Carmi, I

Dostrovsky, I

Bacci, C

Belli, P

Bernabei, R

dAngelo, S

Paoluzi, L

Bevilacqua, A

Cribier, M

Gosset, L

Rich, J

Spiro, M

Tao, C

Vignaud, D

Boger, J

Hahn, RL

Rowley, JK

Stoenner, RW

机构：

[1] FORSCHUNGSZENTRUM KARLSRUHE,INST CHEM TECH,D-76021 KARLSRUHE,GERMANY

[2] LAB NAZL GRAN SASSO,I-67010 LAQUILA,ITALY

[3] UNIV MILAN,DIPARTIMENTO FIS,I-20133 MILAN,ITALY

[4] IST NAZL FIS NUCL,I-20133 MILAN,ITALY

[5] TECH UNIV MUNICH,PHYS DEPT E15,D-85748 GARCHING,GERMANY

[6] OBSERV COTE AZUR,DEPT CASSINI,F-06004 NICE 4,FRANCE

[7] WEIZMANN INST SCI,DEPT ENVIRONM SCI & ENERGY RES,IL-76100 REHOVOT,ISRAEL

[8] UNIV ROMA TOR VERGATA,DIPARTIMENTO FIS,I-00133 ROME,ITALY

[9] IST NAZL FIS NUCL,SEZ ROMA 2,I-00133 ROME,ITALY

[10] CENS,SERV PHYS PARTICULES,DAPNIA,F-91191 GIF SUR YVETTE,FRANCE

[11] BROOKHAVEN NATL LAB,UPTON,NY 11973

[12] JAGIELLONIAN UNIV,INST PHYS,PL-30059 KRAKOW,POLAND

[13] RUSSIAN ACAD SCI,INST NUCL RES,MOSCOW 117312,RUSSIA

[14] UNIV ROMA 3,DIPARTIMENTO FIS,I-00100 ROME,ITALY

[15] CEN,SAPR,SRS,F-38041 GRENOBLE,FRANCE

[16] COLL FRANCE,LPC,F-75005 PARIS,FRANCE

来源：

PHYSICS LETTERS B | 1996年 / 388卷 / 02期

关键词：

D O I：

10.1016/S0370-2693(96)01121-5

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report the GALLEX solar neutrino results for the measuring period GALLEX III, the period from 12 October 1994-4 October 1995. Counting for these runs was completed on 29 March 1996. The GALLEX III result (14 runs) is [53.9 +/- 10.6(stat.) +/- 3.1 (syst.)] SNU (1 sigma). This is 15.8 SNU below but statistically compatible with the new combined result for GALLEX (I+II+III) (53 runs), which is [69.7 +/- 6.7 (stat.)(-4.5)(+3.9) (syst.)] SNU (1 sigma) or (69.7(-8.1)(+7.8)) SNU With errors quadratically added. We also give the preliminary result from our second Cr-51-source experiment: the measured detector response is 83 +/- 10% of expectation. The combined result from both GALLEX Cr-51-source experiments is 92 +/- 8% of expectation.

引用

页码：384 / 396

页数：13

共 50 条

[21] Comparative analysis of GALLEX and GNO solar neutrino data
Sturrock, P. A.
Caldwell, D. O.
Scargle, J. D.
[J]. ASTROPARTICLE PHYSICS, 2006, 26 (03) : 174 - 185
[22] Reanalysis of the GALLEX solar neutrino flux and source experiments
Kaether, F.
Hampel, W.
Heusser, G.
Kiko, J.
Kirsten, T.
[J]. PHYSICS LETTERS B, 2010, 685 (01) : 47 - 54
[23] SOLAR NEUTRINOS AT GALLEX
HAMPEL, W
[J]. PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 1994, 346 (1678): : 3 - 13
[24] IMPLICATIONS OF THE GALLEX SOURCE EXPERIMENT FOR THE SOLAR-NEUTRINO PROBLEM
HATA, N
HAXTON, W
[J]. PHYSICS LETTERS B, 1995, 353 (04) : 422 - 431
[25] GALLEX RESULTS FROM THE 1ST 30 SOLAR-NEUTRINO RUNS
ANSELMANN, P
HAMPEL, W
HEUSSER, G
KIKO, J
KIRSTEN, T
LAUBENSTEIN, M
PERNICKA, E
PEZZONI, S
RONN, U
SANN, M
SCHLOSSER, C
WINK, R
WOJCIK, M
VONAMMON, R
EBERT, KH
FRITSCH, T
HELLRIEGEL, K
HENRICH, E
STIEGLITZ, L
WEIRICH, F
BALATA, M
FERRARI, N
LALLA, H
BELLOTTI, E
CATTADORI, C
CREMONESI, O
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
GOSSET, L
RICH, J
SPIRO, M
STOLARCZYK, T
TAO, C
VIGNAUD, D
[J]. PHYSICS LETTERS B, 1994, 327 (3-4) : 377 - 385
[26] Reexamination of Possible Bimodality of GALLEX Solar-Neutrino Data
P. A. Sturrock
[J]. Solar Physics, 2009, 260 : 245 - 250
[27] Search for time modulations in the Gallex/GNO solar neutrino data
Pandola, L
[J]. ASTROPARTICLE PHYSICS, 2004, 22 (02) : 219 - 226
[28] Reexamination of Possible Bimodality of GALLEX Solar-Neutrino Data
Sturrock, P. A.
[J]. SOLAR PHYSICS, 2009, 260 (02) : 245 - 250
[29] Time – Frequency Analysis of GALLEX and GNO Solar Neutrino Data
P. A. Sturrock
[J]. Solar Physics, 2008, 252 : 1 - 18
[30] SOLAR-NEUTRINO MEASUREMENT WITH THE RADIOCHEMICAL GALLIUM DETECTOR (GALLEX)
VONAMMON, R
[J]. ASTROPHYSICS AND SPACE SCIENCE, 1994, 214 (1-2) : 35 - 47

← 1 2 3 4 5 →