GALLEX results from the first 30 solar neutrino runs

Physics Letters B

Volumn 327, Issue 3-4, 1994, Pages 377-385

  Anselmann, P ^a   Hampel, W ^a   Heusser, G ^a   Kiko, J ^a   Kirsten, T ^a   Laubenstein, M ^a   Pernicka, E ^a   Pezzoni, S ^a   Rönn, U ^a   Sann, M ^a   Schlosser, C ^a   Wink, R ^a   Wojcik, M ^a   Ammon, R v ^b   Ebert, K H ^b   Fritsch, T ^b   Hellriegel, K ^b   Henrich, E ^b   Stieglitz, L ^b   Weirich, F ^b   Balata, M ^c   Ferrari, N ^c   Lalla, H ^c   Bellotti, E ^d   Cattadori, C ^d   Cremonesi, O ^d   Fiorini, E ^d   Zanotti, L ^d   Altmann, M ^e   Feilitzsch, F v ^e   Mößbauer, R ^e   Schanda, U ^e   Berthomieu, G ^f   Schatzman, E ^f   Carmi, I ^g   Dostrovsky, I ^g   Bacci, C ^h   Belli, P ^h   Bernabei, R ^h   d'Angelo, S ^h   Paoluzi, L ^h   Bevilacqua, A ⁱ   Charbit, S ⁱ   Cribier, M ⁱ   Gosset, L ⁱ   Rich, J ⁱ   Spiro, M ⁱ   Stolarczyk, T ⁱ   Tao, C ⁱ   Vignaud, D ⁱ   Hahn, R L ^j   Hartmann, F X ^j   Rowley, J K ^j   Stoenner, R W ^j   Weneser, J ^j   more..

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b KARLSRUHE INSTITUTE OF TECHNOLOGY   (Germany)

^c LABORATORI NAZIONALI DEL GRAN SASSO   (Italy)

^d UNIVERSITY OF MILAN   (Italy)

^e TECHNICAL UNIVERSITY OF MUNICH   (Germany)

^f UNIVERSITÉ CÔTE D'AZUR   (France)

^g WEIZMANN INSTITUTE OF SCIENCE   (Israel)

^h UNIVERSITY OF ROME TOR VERGATA   (Italy)

ⁱ DAPNIA/Service de Physique des Particules CE Saclay F 91191 Gif sur Yvette Cedex France3 ^*

^j BROOKHAVEN NATIONAL LABORATORY   (United States)

more..

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0642356182     PISSN: 03702693     EISSN: None     Source Type: Journal    
DOI: 10.1016/0370-2693(94)90744-7     Document Type: Article

References (40)

1. Statistical treatment of the low-level counting data in GALLEX
2. Status of the GALLEX solar neutrino experiment with emphasis on error treatment and on blank runs
3. Recent results from SAGE
4. On the exclusion of an astrophysical solution to the solar neutrino problem
5. Are there astrophysical solutions to the solar neutrino puzzle?
6. Future solar neutrino spectroscopy and neutrino properties
7. Solar model uncertainties, MSW analysis and future solar neutrino experiments