GALLEX

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References

  1 - Solar Neutrinos

  2 - Neutrino Oscillations

  3 - Detector

  4 - Conference Proceedings

The references in each group are listed in approximate inverted chronological order.
Click on the reference label to search it in inSPIRE.

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.
[1-2]
GALLEX solar neutrino observations: Results for GALLEX IV, Hampel, W. et al. (GALLEX), Phys. Lett. B447 (1999) 127-133.
[1-3]
GALLEX solar neutrino observations: Results for GALLEX III., Hampel, W. et al. (GALLEX), Phys. Lett. B388 (1996) 384-396.
[1-4]
GALLEX solar neutrino observations: Complete results for GALLEX II, Anselmann, P. et al. (GALLEX), Phys. Lett. B357 (1995) 237-247.
[1-5]
GALLEX results from the first 30 solar neutrino runs, Anselmann, P. et al. (GALLEX), Phys. Lett. B327 (1994) 377-385.
[1-6]
GALLEX solar neutrino observations: The Results from GALLEX-I and early results from GALLEX-II, Anselmann, P. et al. (GALLEX), Phys. Lett. B314 (1993) 445-458.
[1-7]
Implications of the GALLEX determination of the solar neutrino flux, Anselmann, P. et al. (GALLEX), Phys. Lett. B285 (1992) 390-397.
[1-8]
Solar neutrinos observed by GALLEX at Gran Sasso., Anselmann, P. et al. (GALLEX), Phys. Lett. B285 (1992) 376-389.

2 - Neutrino Oscillations

[2-1]
Final results of the Cr-51 neutrino source experiments in GALLEX, Hampel, W. 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 +- 0.08.
From the article: Update limits on short-baseline \nu_e disappearance. See also [arXiv:hep-ph/9411414].
Comment: In reality, limits are relaxed in the high \Delta m^2 region, due to the result of the second source run, to the value \sin^2 2 \theta < 0.4 at 90% CL. [M.L.].

3 - Detector

[3-1]
Data analysis of the solar neutrino experiment GALLEX, Kaether, Florian, 2007. PhD Thesis (in German). http://www.ub.uni-heidelberg.de/archiv/7501/.
[3-2]
The muon induced background in the GALLEX experiment, Cribier, M. et al. (GALLEX), Astropart. Phys. 6 (1999) 129-141.
[3-3]
Verification tests of the GALLEX solar neutrino detector, with Ge-71 produced in-situ from the beta-decay of As-71, Hampel, W. et al. (GALLEX), Phys. Lett. B436 (1998) 158-173.
[3-4]
Final results of the Cr-51 neutrino source experiments in GALLEX, Hampel, W. 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 +- 0.08.
[3-5]
The Neutron induced background in GALLEX, Cribier, M. et al. (GALLEX), Astropart. Phys. 4 (1995) 23-32.
[3-6]
First results from the Cr-51 neutrino source experiment with the GALLEX detector, Anselmann, P. et al. (GALLEX), Phys. Lett. B342 (1995) 440-450.

4 - Conference Proceedings

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

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Authors:
Carlo Giunti / giunti@to.infn.it
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Last Update: Tue 15 May 2012, day 136 of the year 2012, 09:42:10 UTC