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

[1] GALLEX solar neutrino observations:: results for GALLEX IV
Hampel, W
Handt, J
Heusser, G
Kiko, J
Kirsten, T
Laubenstein, M
Pernicka, E
Rau, W
Wojcik, M
Zakharov, Y
Ammon, RV
Ebert, KH
Fritsch, T
Heidt, D
Henrich, E
Stielglitz, L
Weirich, F
Balata, M
Sann, M
Hartmann, FX
Bellotti, E
Cattadori, C
Cremonesi, O
Ferrari, N
Fiorini, E
Zanotti, L
Altmann, M
von Feilitzsch, F
Mössbauer, R
Wänninger, S
Berthomieu, G
Schatzman, E
Carmi, I
Dostrovsky, I
Bacci, C
Belli, P
Bernabei, R
d'Angelo, S
Paoluzi, L
Cribier, M
Rich, J
Spiro, M
Tao, C
Vignaud, D
Boger, J
Hahn, RL
Rowley, JK
Stoenner, RW
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[J]. PHYSICS LETTERS B, 1999, 447 (1-2) : 127 - 133
[2] GALLEX SOLAR-NEUTRINO OBSERVATIONS - COMPLETE RESULTS FOR GALLEX-II
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CHARBIT, S
CRIBIER, M
GOSSET, L
RICH, J
SPIRO, M
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TAO, C
VIGNAUD, D
[J]. PHYSICS LETTERS B, 1995, 357 (1-2) : 237 - 247
[3] GALLEX solar neutrino results
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[J]. PROGRESS IN PARTICLE AND NUCLEAR PHYSICS, VOL 40: NEUTRINOS IN ASTRO, PARTICLE AND NUCLEAR PHYSICS, 1998, 40 : 85 - 99
[4] GALLEX SOLAR-NEUTRINO OBSERVATIONS - THE RESULTS FROM GALLEX-I AND EARLY RESULTS FROM GALLEX-II
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SANN, M
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CHARBIT, S
CRIBIER, M
DUPONT, G
GOSSET, L
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[J]. PHYSICS LETTERS B, 1993, 314 (3-4) : 445 - 458
[5] GALLEX solar neutrino results: An update
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[J]. VULCANO WORKSHOP 1996 - FRONTIER OBJECTS IN ASTROPHYSICS AND PARTICLE PHYSICS, 1997, 57 : 495 - 502
[6] GALLEX solar neutrino results and status of GNO
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[J]. NEUTRINO PHYSICS AND ASTROP HYSICS, 1999, : 26 - 34
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[J]. ASTROPHYSICAL LETTERS & COMMUNICATIONS, 1996, 33 (1-5) : 11 - 18
[8] GALLEX solar neutrino results and status of GNO
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[J]. NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 1999, 77 : 26 - 34
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[J]. ABSTRACTS OF PAPERS OF THE AMERICAN CHEMICAL SOCIETY, 1994, 208 : 59 - NUCL
[10] GALLEX SOLAR-NEUTRINO RESULTS AND THEIR IMPLICATIONS
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[J]. PROGRESS IN PARTICLE AND NUCLEAR PHYSICS, VOL 32: NEUTRINOS IN COSMOLOGY, ASTRO, PARTICLE AND NUCLEAR PHYSICS, 1994, 32 : 33 - 34

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