GALLEX

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References

1 - Solar Neutrinos

[1-1]
Reanalysis of the GALLEX solar neutrino flux and source experiments, F. Kaether, W. Hampel, G. Heusser, J. Kiko, T. Kirsten, Phys. Lett. B685 (2010) 47-54, arXiv:1001.2731.
[Kaether:2010ag]
[1-2]
GALLEX solar neutrino observations: Results for GALLEX IV, W. Hampel et al. (GALLEX), Phys. Lett. B447 (1999) 127-133.
[Hampel:1998xg]
[1-3]
GALLEX solar neutrino observations: Results for GALLEX III., W. Hampel et al. (GALLEX), Phys. Lett. B388 (1996) 384-396.
[Hampel:1996qd]
[1-4]
GALLEX solar neutrino observations: Complete results for GALLEX II, P. Anselmann et al. (GALLEX), Phys. Lett. B357 (1995) 237-247.
[Anselmann:1995ag]
[1-5]
GALLEX results from the first 30 solar neutrino runs, P. Anselmann et al. (GALLEX), Phys. Lett. B327 (1994) 377-385.
[Anselmann:1994cf]
[1-6]
GALLEX solar neutrino observations: The Results from GALLEX-I and early results from GALLEX-II, P. Anselmann et al. (GALLEX), Phys. Lett. B314 (1993) 445-458.
[Anselmann:1993mh]
[1-7]
Implications of the GALLEX determination of the solar neutrino flux, P. Anselmann et al. (GALLEX), Phys. Lett. B285 (1992) 390-397.
[Anselmann:1992kc]
[1-8]
Solar neutrinos observed by GALLEX at Gran Sasso., P. Anselmann et al. (GALLEX), Phys. Lett. B285 (1992) 376-389.
[Anselmann:1992um]

2 - Detector

[2-1]
Data analysis of the solar neutrino experiment GALLEX, Florian Kaether, 2007. PhD Thesis (in German). http://www.ub.uni-heidelberg.de/archiv/7501/.
[Kaether:2007zz]
[2-2]
The muon induced background in the GALLEX experiment, M. Cribier et al. (GALLEX), Astropart. Phys. 6 (1999) 129-141.
[Cribier:1999qe]
[2-3]
Final results of the Cr-51 neutrino source experiments in GALLEX, W. Hampel et al. (GALLEX), Phys. Lett. B420 (1998) 114-126.
From the abstract: The ratio $R$ of the neutrino source strength derived from the measured rate of 71Ge production, divided by the directly determined source strength is $R = 1.01 {}^{+0.12}_{-0.11}$ for the first source and $R = 0.84 {}^{+0.12}_{-0.11}$ for the second one. The combined value of $R$ for the two source experiments is $R = 0.93 \pm 0.08$.
[Hampel:1997fc]
[2-4]
Verification tests of the GALLEX solar neutrino detector, with Ge-71 produced in-situ from the beta-decay of As-71, W. Hampel et al. (GALLEX), Phys. Lett. B436 (1998) 158-173.
[Hampel:1998su]
[2-5]
First results from the Cr-51 neutrino source experiment with the GALLEX detector, P. Anselmann et al. (GALLEX), Phys. Lett. B342 (1995) 440-450.
[Anselmann:1994ar]
[2-6]
The Neutron induced background in GALLEX, M. Cribier et al. (GALLEX), Astropart. Phys. 4 (1995) 23-32.
[Cribier:1995av]

3 - Conference Proceedings

[3-1]
GALLEX solar neutrino results and status of GNO, T. A. Kirsten (GALLEX and GNO), Nucl. Phys. Proc. Suppl. 77 (1999) 26-34.
[Kirsten:1999cx]
[3-2]
Final results of the GALLEX solar neutrino experiment, D. Vignaud (GALLEX), 1998. Contributed to 29th International Conference on High-Energy Physics (ICHEP 98), Vancouver, Canada, 23-29 Jul 1998.
[Vignaud:1998fn]
[3-3]
GALLEX solar neutrino results, T. A. Kirsten, Prog. Part. Nucl. Phys. 40 (1998) 85-99.
[Kirsten:1998py]
[3-4]
Implications of the GALLEX results after the chromium source experiment, R. Bernabei et al. (GALLEX), Nucl. Phys. Proc. Suppl. 48 (1996) 304-308.
[Bernabei:1996wh]
[3-5]
Proportional counters with shaped cathodes for the GALLEX experiment: Performance and potential, U. Ronn, 1995. In 'Baksan Valley 1995, Particles and cosmology' 77-80.
[Ronn:1995bk]
[3-6]
Recent results from the GALLEX experiment, C. Tao (GALLEX), 1995. Prepared for 30th Rencontres de Moriond: Euroconferences: Clustering in the Universe, Les Arcs, Savoie, France, 11-18 Mar 1995.
[Tao:1995cv]
[3-7]
Update of GALLEX solar neutrino results and implications, P. Anselmann et al. (GALLEX), Nucl. Phys. Proc. Suppl. 38 (1995) 68-76.
[Anselmann:1995uv]
[3-8]
The 62 PBq Cr-51 artificial neutrino source for the GALLEX experiment, D. Vignaud, 1995. In 'Baksan Valley 1995, Particles and cosmology' 60-69.
[Vignaud:1995bi]
[3-9]
GALLEX and the Be-7 solar neutrino problem, T. Kirsten (GALLEX), 1995. In 'Osaka 1995, Weak and electromagnetic interactions in nuclei' 135-143.
[Kirsten:1995nj]
[3-10]
GALLEX solar neutrino results: An update, O. Cremonesi (GALLEX), 1994. In 'Vulcano 1994, Frontier objects in astrophysics and particle physics' 377-385.
[Cremonesi:1994rf]
[3-11]
GALLEX results from the first 30 solar neutrino runs, P. Anselmann (GALLEX), 1994. In 'Meribel les Allues 1994, Electroweak interactions and unified theories' 585-592.
[Anselmann:1994yj]
[3-12]
GALLEX solar neutrino results and their implications, T. A. Kirsten (GALLEX), Prog. Part. Nucl. Phys. 32 (1994) 33-34.
[Kirsten:1994jx]
[3-13]
Solar neutrinos observed by GALLEX at Gran Sasso, P. Anselmann et al. (GALLEX), Nucl. Phys. Proc. Suppl. 31 (1993) 117-124.
[Anselmann:1993ct]
[3-14]
Status report on the GALLEX experiment, R. Bernabei et al., 1993. Prepared for 5th International Symposium on Neutrino Telescopes, Venice, Italy, 2-4 Mar 1993.
[Bernabei:1993fc]
[3-15]
Status report on the GALLEX experiment, P. Anselmann et al. (GALLEX.), Nuovo Cim. C15 (1992) 917-929.
[Anselmann:1992wu]
[3-16]
GALLEX status report as of November, 1991, T. Kirsten (GALLEX), Nucl. Phys. Proc. Suppl. 28A (1992) 82-87.
[Kirsten:1992ig]
[3-17]
The observation of solar neutrinos by GALLEX at Gran Sasso, E. Bellotti et al., 1992. Given at 3rd International Symposium on Weak and Electromagnetic Interactions in Nuclei (WEIN 92), Dubna, USSR, 16-22 June 1992.
[Bellotti:1992zt]
[3-18]
Results from the GALLEX solar neutrino experiment: GALLEX- I, T. Kirsten (GALLEX.), 1992. In 'Kyoto 1992, Proceedings, The frontier of nuclear spectroscopy' 251-260.
[Kirsten:1992vi]
[3-19]
Status report on the GALLEX experiment, L. Zanotti et al., 1992. Prepared for 12th Moriond Workshop: Progress in Atomic Physics, Neutrinos and Gravitation, Les Arcs, France, 25 Jan - 1 Feb 1992.
[Zanotti:1992rk]
[3-20]
Advances in GALLEX till spring 1991, R. Plaga et al. (GALLEX.), 1991. In 'Boston 1991, Proceedings, Particles, strings and cosmology' 107-121.
[Plaga:1991bh]
[3-21]
Status of the GALLEX solar neutrino experiment, E. Bellotti et al. (GALLEX), 1991. Prepared for International Workshop on Neutrino Telescopes, 3rd, Venice, Italy, 26-28 Feb 1991.
[Bellotti:1991ep]
[3-22]
Characteristics of the GALLEX spectrometer, P. Anselmann et al. (GALLEX), 1991. Given at 2nd International Conference on Trends in Astroparticle Physics, Aachen, Germany, 10-12 Oct 1991.
[Anselmann:1991hw]
[3-23]
The status of GALLEX, R. Wink et al. (GALLEX), Nucl. Phys. Proc. Suppl. 19 (1991) 77-83.
[Wink:1991ef]
[3-24]
GALLEX status report as of August, 1991, T. Kirsten et al. (GALLEX), 1991. Prepared for Particles and Fields 91: Meeting of the Division of Particles and Fields of the APS, Vancouver, Canada, 18-22 Aug 1991.
[Kirsten:1991gq]
[3-25]
The GALLEX experiment: Status report, T. Kirsten (GALLEX), 1990. In 'Venice 1990, Proceedings, Neutrino telescopes' 61-71.
[Kirsten:1990cn]
[3-26]
Neutrino physics and astrophysics with the GALLEX solar neutrino experiment, J. Rich et al. (GALLEX), 1987. IN 'SYracuse 1987, Proceedings, Grand Unification' 109-125.
[Rich:1987hp]
[3-27]
Progress report on the 'Gallex' solar neutrino project, T. Kirsten (GALLEX), 1986. In 'Sendai 1986, Proceedings, Neutrino '86' 317-329.
[Kirsten:1986hj]
[3-28]
Status report on the proposed gallium solar neutrino experiment, T. Kirsten (GAllium Solar Neutrino), 1979. In 'Bergen 1979, Proceedings, Neutrino '79, Vol.2', 452- 460.
[Kirsten:1979rj]

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Authors:
Stefano Gariazzo / gariazzo@to.infn.it
Carlo Giunti / giunti@to.infn.it
Marco Laveder / marco.laveder@pd.infn.it
Last Update: Wed 20 Sep 2017, 09:48:54 UTC