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Journal articles on the topic 'GALLEX'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

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1

Hampel, W., J. Handt, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, et al. "GALLEX solar neutrino observations: results for GALLEX IV." Physics Letters B 447, no. 1-2 (February 1999): 127–33. http://dx.doi.org/10.1016/s0370-2693(98)01579-2.

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2

Hampel, W., G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, W. Rau, et al. "GALLEX solar neutrino observations: Results for GALLEX III." Physics Letters B 388, no. 2 (November 1996): 384–96. http://dx.doi.org/10.1016/s0370-2693(96)01121-5.

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3

Anselmann, P., W. Hampel, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, et al. "GALLEX solar neutrino observations. The results from GALLEX I and early results from GALLEX II." Physics Letters B 314, no. 3-4 (September 1993): 445–58. http://dx.doi.org/10.1016/0370-2693(93)91264-n.

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4

Anselmann, P., W. Hampel, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, et al. "GALLEX solar neutrino observations: complete results for GALLEX II." Physics Letters B 357, no. 1-2 (August 1995): 237–47. http://dx.doi.org/10.1016/0370-2693(95)00897-t.

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5

Kirsten, T., M. Breitenbach, W. Hampel, G. Heusser, J. Kiko, T. Kirsten, H. Lalla, et al. "The GALLEX Project." International Astronomical Union Colloquium 121 (1990): 187–99. http://dx.doi.org/10.1017/s0252921100067944.

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AbstractThe GALLEX collaboration aims at the detection of solar neutrinos in a radiochemical experiment employing 30 tons of Gallium in form of concentrated aqueous Gallium-chloride solution. The detector is primarily sensitive to the otherwise inaccessible pp-neutrinos. Details of the experiment have been repeatedly described before [1-7]. Here we report the present status of implementation in the Laboratori Nazionali del Gran Sasso (Italy). So far, 12.2 tons of Gallium are at hand. The present status of development allows to start the first full scale run at the time when 30 tons of Gallium become available. This date is expected to be January, 1990.

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6

Kirsten, Till. "GALLEX mißt Sonnenneutrinos." Physik in unserer Zeit 23, no. 6 (1992): 246–55. http://dx.doi.org/10.1002/piuz.19920230607.

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7

Kirsten, T. A. "GALLEX solar neutrino results." Progress in Particle and Nuclear Physics 40 (January 1998): 85–99. http://dx.doi.org/10.1016/s0146-6410(98)00013-1.

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8

Kirsten, T. "Retrospect of GALLEX/GNO." Journal of Physics: Conference Series 120, no. 5 (July 1, 2008): 052013. http://dx.doi.org/10.1088/1742-6596/120/5/052013.

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9

Kirsten, Till, E. Bellotti, P. Anselmann, M. Breitenbach, W. Hampel, G. Heusser, J. Kiko, et al. "The status of gallex." Nuclear Physics B - Proceedings Supplements 19 (April 1991): 77–83. http://dx.doi.org/10.1016/0920-5632(91)90190-p.

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10

Vignaud, D. "The GALLEX solar neutrino experiment." Nuclear Physics B - Proceedings Supplements 60, no. 3 (January 1998): 20–29. http://dx.doi.org/10.1016/s0920-5632(97)00498-2.

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11

Hampel, W. "Erste Sonnenneutrino-Messung durch GALLEX." Physik Journal 48, no. 11 (November 1992): 901–5. http://dx.doi.org/10.1002/phbl.19920481107.

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12

Cribier, M., W. Hampel, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, et al. "Results of the whole GALLEX experiment." Nuclear Physics B - Proceedings Supplements 70, no. 1-3 (January 1999): 284–91. http://dx.doi.org/10.1016/s0920-5632(98)00438-1.

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13

Cribler, M., B. Pichard, J. P. Soirat, M. Spiro, Th Stolarczyk, C. Tao, D. Vignaud, P. Belli, S. d'Angelo, and R. Wink. "The neutron induced background in GALLEX." Astroparticle Physics 4, no. 1 (October 1995): 23–32. http://dx.doi.org/10.1016/0927-6505(95)00025-c.

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14

Peterson, I. "At Last, Neutrino Results from GALLEX." Science News 141, no. 24 (June 13, 1992): 388. http://dx.doi.org/10.2307/3976516.

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15

Gough, Douglas. "New astronomy from GALLEX and SAGE?" Physics World 5, no. 7 (July 1992): 21–22. http://dx.doi.org/10.1088/2058-7058/5/7/22.

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16

Stodolsky, L. "Comment on the gallex mixing solutions." Nuclear Physics B - Proceedings Supplements 31 (April 1993): 135. http://dx.doi.org/10.1016/0920-5632(93)90125-p.

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17

Henrich, E. "Chemistry of the Gallex Solar Neutrino Experiment." Interdisciplinary Science Reviews 18, no. 3 (September 1993): 295–305. http://dx.doi.org/10.1179/isr.1993.18.3.295.

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18

Kirsten, Till A. "GALLEX solar neutrino results and their implications." Progress in Particle and Nuclear Physics 32 (January 1994): 33–34. http://dx.doi.org/10.1016/0146-6410(94)90005-1.

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19

Kirsten, Till, P. Anselmann, W. Hampel, G. Heusser, J. Kiko, T. Kirsten, G. Monninger, et al. "Gallex status report as of November, 1991." Nuclear Physics B - Proceedings Supplements 28, no. 1 (July 1992): 82–87. http://dx.doi.org/10.1016/0920-5632(92)90150-q.

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20

Kirsten, T. A., W. Hampel, J. Handt, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, et al. "GALLEX solar neutrino results and status of GNO." Nuclear Physics B - Proceedings Supplements 77, no. 1-3 (May 1999): 26–34. http://dx.doi.org/10.1016/s0920-5632(99)00389-8.

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21

Cribier, M., B. Pichard, J. Rich, J. P. Soirat, M. Spiro, Th Stolarczyk, C. Tao, et al. "The muon induced background in the GALLEX experiment." Astroparticle Physics 6, no. 2 (February 1997): 129–41. http://dx.doi.org/10.1016/s0927-6505(96)00049-7.

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22

Anselmann, P., W. Hampel, G. Heusser, J. Kiko, T. Kirsten, E. Pernicka, R. Plaga, et al. "Solar neutrinos observed by GALLEX at Gran Sasso." Nuclear Physics B - Proceedings Supplements 31 (April 1993): 117–24. http://dx.doi.org/10.1016/0920-5632(93)90122-m.

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23

Anselmann, P., W. Hampel, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, et al. "Update of GALLEX solar neutrino results and implications." Nuclear Physics B - Proceedings Supplements 38, no. 1-3 (January 1995): 68–76. http://dx.doi.org/10.1016/0920-5632(94)00735-e.

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24

Anselmann, P., W. Hampel, G. Heusser, J. Kiko, T. Kirsten, E. Pernicka, R. Plaga, et al. "Solar neutrinos observed by GALLEX at Gran Sasso." Physics Letters B 285, no. 4 (July 1992): 376–89. http://dx.doi.org/10.1016/0370-2693(92)91521-a.

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25

Anselmann, P., W. Hampel, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, et al. "GALLEX results from the first 30 solar neutrino runs." Physics Letters B 327, no. 3-4 (May 1994): 377–85. http://dx.doi.org/10.1016/0370-2693(94)90744-7.

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26

Von Ammon, Reinhard. "Solar neutrino measurement with the radiochemical gallium detector (GALLEX)." Astrophysics and Space Science 214, no. 1-2 (April 1994): 35–47. http://dx.doi.org/10.1007/bf00982323.

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27

Sturrock, P. A. "Reexamination of Possible Bimodality of GALLEX Solar-Neutrino Data." Solar Physics 260, no. 2 (October 27, 2009): 245–50. http://dx.doi.org/10.1007/s11207-009-9462-2.

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28

Sturrock, P. A., D. O. Caldwell, and J. D. Scargle. "Comparative analysis of GALLEX and GNO solar neutrino data." Astroparticle Physics 26, no. 3 (October 2006): 174–85. http://dx.doi.org/10.1016/j.astropartphys.2006.06.001.

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29

Hampel, W., G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, W. Rau, et al. "Final results of the 51Cr neutrino source experiments in GALLEX." Physics Letters B 420, no. 1-2 (February 1998): 114–26. http://dx.doi.org/10.1016/s0370-2693(97)01562-1.

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30

Kaether, F., W. Hampel, G. Heusser, J. Kiko, and T. Kirsten. "Reanalysis of the Gallex solar neutrino flux and source experiments." Physics Letters B 685, no. 1 (February 2010): 47–54. http://dx.doi.org/10.1016/j.physletb.2010.01.030.

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31

Wänninger, S., M. Altmann, F. v. Feilitzsch, C. Hagner, B. Kemmather, L. Oberauer, and J. Schnagl. "Probing Neutrino Vacuum Oscillations with the GALLEX Solar Neutrino Results." Physical Review Letters 83, no. 6 (August 9, 1999): 1088–91. http://dx.doi.org/10.1103/physrevlett.83.1088.

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32

Anselmann, P., and F. X. Hartmann. "Statistical treatment of the low-level counting data in GALLEX." Progress in Particle and Nuclear Physics 32 (January 1994): 35–40. http://dx.doi.org/10.1016/0146-6410(94)90006-x.

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33

Sturrock, P. A. "Time – Frequency Analysis of GALLEX and GNO Solar Neutrino Data." Solar Physics 252, no. 1 (September 10, 2008): 1–18. http://dx.doi.org/10.1007/s11207-008-9254-0.

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34

Anselmann, P., R. Fockenbrock, W. Hampel, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, et al. "Implications of the GALLEX results after the Chromium source experiment." Nuclear Physics B - Proceedings Supplements 48, no. 1-3 (May 1996): 304–8. http://dx.doi.org/10.1016/0920-5632(96)00265-4.

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35

Anselmann, P., W. Hampel, G. Heusser, J. Kiko, T. Kirsten, E. Pernicka, R. Plaga, et al. "Implications of the GALLEX determination of the solar neutrino flux." Physics Letters B 285, no. 4 (July 1992): 390–97. http://dx.doi.org/10.1016/0370-2693(92)91522-b.

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36

Schwarzschild, Bertram. "Gallex Data Can't Quite Lay the Solar Neutrino Problem to Rest." Physics Today 45, no. 8 (August 1992): 17–20. http://dx.doi.org/10.1063/1.2809767.

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37

Henrich, Edmund, and Klaus H. Ebert. "Die Chemie von GALLEX – Messung von Sonnenneutrinos mit einem radiochemischen Galliumdetektor." Angewandte Chemie 104, no. 10 (October 1992): 1310–24. http://dx.doi.org/10.1002/ange.19921041005.

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38

Bahcall, J. N., P. I. Krastev, and E. Lisi. "Limits on electron-neutrino oscillations from the GALLEX 51Cr source experiment." Physics Letters B 348, no. 1-2 (March 1995): 121–23. http://dx.doi.org/10.1016/0370-2693(95)00111-w.

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39

d'Angelo, Silio. "Performance test of low-noise proportional counters for the GALLEX experiment." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 279, no. 1-2 (July 1989): 148–51. http://dx.doi.org/10.1016/0168-9002(89)91075-9.

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40

Kiko, J. "The GALLEX solar neutrino experiment at the Gran Sasso Underground Laboratory." Astrophysics and Space Science 228, no. 1-2 (June 1995): 107–12. http://dx.doi.org/10.1007/bf00984970.

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41

Hata, Naoya, and Wick Haxton. "Implications of the GALLEX source experiment for the solar neutrino problem." Physics Letters B 353, no. 4 (July 1995): 422–31. http://dx.doi.org/10.1016/0370-2693(95)00598-f.

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42

Pandola, L. "Search for time modulations in the Gallex/GNO solar neutrino data." Astroparticle Physics 22, no. 2 (November 2004): 219–26. http://dx.doi.org/10.1016/j.astropartphys.2004.07.007.

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43

Altmann, M., F. v. Feilitzsch, and U. Schanda. "A parameterized pulse shape analysis method for the GALLEX solar neutrino experiment." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 381, no. 2-3 (November 1996): 398–412. http://dx.doi.org/10.1016/s0168-9002(96)00738-3.

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44

Cribier, M., L. Gosset, P. Lamare, J. C. Languillat, P. Perrin, M. Renard, J. Rich, et al. "Production of a 62 PBq 51Cr low energy neutrino source for GALLEX." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 378, no. 1-2 (August 1996): 233–50. http://dx.doi.org/10.1016/0168-9002(96)00464-0.

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45

Anselmann, P., R. Fockenbrock, W. Hampel, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, et al. "First results from the 51Cr neutrino source experiment with the GALLEX detector." Physics Letters B 342, no. 1-4 (January 1995): 440–50. http://dx.doi.org/10.1016/0370-2693(94)01586-2.

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46

DREINER, H., G. K. LEONTARIS, and N. D. TRACAS. "ANSATZ FOR QUARK, CHARGED LEPTON, AND NEUTRINO MASSES IN SUSY GUTs." Modern Physics Letters A 08, no. 22 (July 20, 1993): 2099–109. http://dx.doi.org/10.1142/s0217732393001811.

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We extend a fermion mass matrix ansatz by Giudice to include neutrino masses. The previous predictions are maintained. With two additional parameters, a large Majorana neutrino mass and a hierarchy factor, we have seven further low energy predictions: the masses of the neutrinos, the mixing angles and the phase in the leptonic sector. We choose a reasonable hierarchy of Majorana masses and fit the overall mass scale according to a solution of the solar neutrino problem via the MSW mechanism, which is in agreement with the 37 Cl , Kamiokande, SAGE and GALLEX data. We then also obtain a cosmologically interesting tau-neutrino mass.

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47

KIM, Y. E., J. H. YOON, and M. RABINOWITZ. "CONDENSED MATTER EFFECTS ON FUSION NEUTRINO PRODUCTION RATES." Modern Physics Letters B 07, no. 13n14 (June 20, 1993): 953–65. http://dx.doi.org/10.1142/s0217984993000965.

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Condensed matter effects (CME) influence nuclear fusion rates in astrophysical settings. As potential energy is a significant component of the total energy in dense plasmas or condensed matter, the mean kinetic energy (and hence effective flux velocity) is reduced. Additional CME are due to a high density interference effect. Both CME reduce the flux in elastic scattering with a significantly larger reduction in fusion rates for the higher Z nuclei. Our CME predictions are consistent with neutrino experiments including the recent GALLEX measurements. CME have broad ranging astrophysical implications, and may be testable in laboratory beam fusion experiments with solid targets.

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48

Henrich, Edmund, and Klaus H. Ebert. "The Chemistry of GALLEX—Measurement of Solar Neutrinos with a Radiochemical Gallium Detector." Angewandte Chemie International Edition in English 31, no. 10 (October 1992): 1283–97. http://dx.doi.org/10.1002/anie.199212831.

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49

Schneider, Dirk, and Donald M. Engelman. "GALLEX, a Measurement of Heterologous Association of Transmembrane Helices in a Biological Membrane." Journal of Biological Chemistry 278, no. 5 (November 21, 2002): 3105–11. http://dx.doi.org/10.1074/jbc.m206287200.

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50

Sturrock, P. A. "Analysis of Bimodality in Histograms Formed from GALLEX and GNO Solar Neutrino Data." Solar Physics 249, no. 1 (April 5, 2008): 1–10. http://dx.doi.org/10.1007/s11207-008-9170-3.

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