Zobrazeno 1 - 10
of 132
pro vyhledávání: '"I. Dostrovsky"'
Autor:
P. Anselmann, W. Hampel, G. Heusser, J. Kiko, T. Kirsten, E. Pernicka, R. Plaga, U. Rönn, M. Sann, C. Schlosser, R. Wink, M. Wójcik, R. von Ammon, K.H. Ebert, T. Fritsch, K. Hellriegel, E. Henrich, L. Stieglitz, F. Weyrich, M. Balata, E. Bellotti, N. Ferrari, H. Lalla, T. Stolarczyk, C. Cattadori, O. Cremonesi, E. Fiorini, S. Pezzoni, L. Zanotti, F. von Feilitzsch, R. Mößbauer, U. Schanda, G. Berthomieu, E. Schatzman, I. Carmi, I. Dostrovsky, C. Bacci, P. Belli, R. Bernabei, S. d’Angelo, L. Paoluzi, S. Charbit, M. Cribier, G. Dupont, L. Gösset, J. Rich, M. Spiro, C. Tao, D. Vignaud, R.L. Hahn, F.X. Hartmann, J.K. Rowley, R.W. Stoenner, J. Weneser
Publikováno v:
Solar Neutrinos ISBN: 9780429502811
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f0752c170011438b31b180a587155e41
https://doi.org/10.1201/9780429502811-50
https://doi.org/10.1201/9780429502811-50
Autor:
T.A. Kirsten, W. Hampel, J. Handt, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, W. Rau, U. Rönn, M. Wojcik, Y. Zakharov, R.v. Ammon, K.H. Ebert, T. Fritsch, D. Heidt, E. Henrich, L. Stieglitz, F. Weirich, M. Balata, M. Sann, F.X. Hartmann, E. Bellotti, C. Cattadori, O. Cremonesi, N. Ferrari, E. Fiorini, L. Zanotti, M. Altmann, F.v. Feilitzsch, R. Möβbauer, S. Wänninger, G. Berthomieu, E. Schatzman, I. Carmi, I. Dostrovsky, C. Bacci, P. Belli, R. Bernabei, S. d'Angelo, L. Paoluzi, M. Cribier, J. Rich, M. Spiro, C. Tao, D. Vignaud, J. Boger, R.L. Hahn, J.K. Rowley, R.W. Stoenner, J. Weneser, E. Burkert, H. Richter, F.X. Hartman
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 77:26-34
We describe the results of the GALLEX solar neutrino experiment after completion of the project. In particular, we summarize the results for GALLEX IV (12 solar runs) and for our 71As - spiking experiments. The integral GALLEX result for all 65 solar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e1050bc01ad3f2c2030c8616f2da262f
https://doi.org/10.1016/s0920-5632(99)00389-8
https://doi.org/10.1016/s0920-5632(99)00389-8
Autor:
M. Cribier, W. Hampel, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, W. Rau, U. Rönn, C. Schlosser, M. Wójcik, R.v. Ammon, K.H. Ebert, T. Fritsch, D. Heidt, E. Henrich, L. Stieglitz, F. Weirich, M. Balata, F.X. Hartmann, M. Sann, E. Bellotti, C. Cattadori, O. Cremonesi, N. Ferrari, E. Fiorini, L. Zanotti, M. Altmann, F.v. Feilitzsch, R. Möβbauer, S. Waenninger, G. Berthomieu, E. Schatzman, I. Carmi, I. Dostrovsky, C. Bacci, P. Belli, R. Bernabei, S. d'Angelo, L. Paoluzi, A. Bevilacqua, L. Gosset, J. Rich, M. Spiro, C. Tao, D. Vignaud, J. Boger, R.L. Hahn, J.K. Rowley, R.W. Stoenner, J. Weneser
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 70:284-291
After 5.5 years of data taking, GALLEX ended its experimental phase. The solar neutrino production rate, 76.4 ± 8 SNU, represents about 55% of the predicted rate. The As tests prove, at the 1% level, the reliability of the technique and the detectio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c205edea86da25685eded4db46903b5
https://doi.org/10.1016/s0920-5632(98)00438-1
https://doi.org/10.1016/s0920-5632(98)00438-1
Autor:
L. Paoluzi, S. d'Angelo, R. Fockenbrock, R. von Ammon, R. Bernabei, E. Schatzman, K.H. Ebert, J. Kiko, F.X. Hartmann, C. Schlosser, M. Balata, D. Vignaud, S. Charbit, F. Weirich, I. Carmi, R.W. Stoenner, Marcin Wójcik, G. Berthomieu, Matthias Laubenstein, J. Weneser, H. Lalla, J. Boger, C. Cattadori, E. Bellotti, Th. Stolarczyk, J.K. Rowley, M. Cribier, N. Ferrari, J. Rich, Charling Tao, E. Henrich, C. Bacci, U. Schanda, Ettore Fiorini, S. Pezzoni, Oliviero Cremonesi, U. Roenn, Ernst Pernicka, L. Zanotti, R. Mossbauer, G. Dupont, L. Gosset, M. Sann, P. Anselmann, I. Dostrovsky, M. Altmann, R. Wink, G. Heusser, F. von Feilitzsch, F. Spielker, P. Belli, L. Stieglitz, Michel Spiro, Till Kirsten, T. Fritsch, R.L. Hahn, D. Heidt, W. Hampel, A. Bevilacqua
Publikováno v:
Scopus-Elsevier
Since May 1991, the GALLEX experiment — installed in the Gran Sasso Underground Laboratory — is continuously monitoring the solar neutrino signal by measuring the 71 Ge production rate in a target of 30.3 tons of nat Ga. The measured signal 77.1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c9bc6752de2a2c4d1d727a8bb836d55
https://doi.org/10.1016/0920-5632(96)00265-4
https://doi.org/10.1016/0920-5632(96)00265-4
Autor:
T. Kirsten, M. Breitenbach, W. Hampel, G. Heusser, J. Kiko, H. Lalla, A. Lenzing, E. Pernicka, R. Plaga, B. Povh, C. Schlosser, H. Völk, R. Wink, K. Zuber, R.v. Ammon, K. Ebert, E. Henrich, L. Stieglitz, E. Bellotti, O. Cremonesi, E. Fiorini, C. Liguori, S. Ragazzi, L. Zanotti, R. Mössbauer, A. Urban, G. Berthomieu, E. Schatzman, S. d’Angelo, C. Bacci, P. Belli, R. Bernabei, L. Paoluzi, R. Santonico, M. Cribier, G. Dupont, B. Pichard, J. Rich, M. Spiro, T. Stolarczyk, C. Tao, D. Vignaud, I. Dostrovsky, G. Friedlander, R.L. Hahn, J.K. Rowley, R.W. Stoenner, J. Weneser
Publikováno v:
International Astronomical Union Colloquium. 121:187-199
The 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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::742d14bb5015486f4c504cd68c01f0d1
https://doi.org/10.1017/s0252921100067944
https://doi.org/10.1017/s0252921100067944
Publikováno v:
1999 ISES Solar World Congress
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dae5f145ecbabe20b49fb7d03bca7864
https://doi.org/10.1016/b978-008043895-5/50157-0
https://doi.org/10.1016/b978-008043895-5/50157-0
Autor:
E. Henrich, M. Balata, R. Mößbauer, I. Dostrovsky, E. Bellotti, W. Hampel, Marcin Wójcik, R.L. Hahn, D. Heidt, C. Cattadori, L. Paoluzi, F. Weirich, R.W. Stoenner, F. Hartmann, P. Belli, M. Cribier, R.v. Ammon, A. Bevilacqua, S. d'Angelo, Matthias Laubenstein, U. Rönn, L. Stieglitz, Ettore Fiorini, Y. Zakharov, F.v. Feilitzsch, C. Bacci, L. Zanotti, G. Heusser, M. Sann, R. Bernabei, Michel Spiro, M. Altmann, L. Gosset, J. Kiko, E. Schatzman, Charling Tao, W. Rau, Till Kirsten, T. Fritsch, J.K. Rowley, K.H. Ebert, I. Carmi, Ernst Pernicka, J. Rich, D. Vignaud, C. Schlosser, N. Ferrari, Oliviero Cremonesi, G. Berthomieu, J. Boger, J. Weneser
Publikováno v:
Scopus-Elsevier
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 (s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a896e6311406be477a7ca81347fbac9d
http://cds.cern.ch/record/387170
http://cds.cern.ch/record/387170
Autor:
W. Hampel, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, W. Rau, U. Rönn, C. Schlosser, M. Wojcik, Y. Zakharov, R.v. Ammon, K.H. Ebert, T. Fritsch, D. Heidt, E. Henrich, L. Stieglitz, F. Weirich, M. Balata, M. Sann, F.X. Hartmann, E. Bellotti, C. Cattadori, O. Cremonesi, N. Ferrari, E. Fiorini, L. Zanotti, M. Altmann, F.v. Feilitzsch, R. Mößbauer, G. Berthomieu, E. Schatzman, I. Carmi, I. Dostrovsky, C. Bacci, P. Belli, R. Bernabei, S. d'Angelo, L. Paoluzi, A. Bevilacqua, M. Cribier, L. Gosset, J. Rich, M. Spiro, C. Tao, D. Vignaud, J. Boger, R.L. Hahn, J.K. Rowley, R.W. Stoenner, J. Weneser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ca7b28551d1f6641dad077795c8f812
http://cds.cern.ch/record/308967
http://cds.cern.ch/record/308967
Autor:
D. Vignaud, G. Berthomieu, Charling Tao, U. Rönn, Till Kirsten, T. Fritsch, U. Schanda, G. Heusser, Matthias Laubenstein, J. Boger, L. Zanotti, M. Cribier, L. Paoluzi, Th. Stolarczyk, F. Weirich, S. d'Angelo, R. Wink, L. Gosset, R.L. Hahn, D. Heidt, Ernst Pernicka, R.W. Stoenner, S. Pezzoni, A. Bevilacqua, M. Sann, H. Lalla, Ettore Fiorini, J. Kiko, W. Hampel, R. Bernabei, I. Dostrovsky, F. Spielker, S. Charbit, N. Ferrari, R. Mößbauer, C. Cattadori, F.v. Feilitzsch, P. Anselmann, K.H. Ebert, J. Rich, Michel Spiro, G. Dupont, C. Bacci, E. Henrich, I. Carmi, J.K. Rowley, J. Weneser, P. Belli, M. M. Wojcik, E. Bellotti, F.X. Hartmann, Oliviero Cremonesi, R.v. Ammon, R. Fockenbrock, C. Schlosser, E. Schatzman, M. Balata, M. Altmann, L. Stieglitz
The radiochemical GALLEX experiment, which has been measuring the solar neutrino flux since May 1991, has performed an investigation with an intense man-made 51 Cr neutrino source (61.9 ± 1.2 PBq). The source, produced via neutron irradiation of ≈
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::59e71ec3e1230e288e15100336a3a266
http://hdl.handle.net/2108/24709
http://hdl.handle.net/2108/24709
Autor:
P. Anselmann, W. Hampel, G. Heusser, J. Kiko, T. Kirsten, M. Laubenstein, E. Pernicka, S. Pezzoni, U. Rönn, M. Sann, C. Schlosser, R. Wink, M. Wójcik, R. von Ammon, K.H. Ebert, T. Fritsch, K. Hellriegel, E. Henrich, L. Stieglitz, F. Weirich, M. Balata, N. Ferrari, H. Lalla, E. Bellotti, C. Cattadori, O. Cremonesi, E. Fiorini, L. Zanotti, M. Altmann, F. von Feilitzsch, R. Möβbauer, U. Schanda, G. Berthomieu, E. Schatzman, I. Carmi, I. Dostrovsky, C. Bacci, P. Belli, R. Bernabei, S. d'Angelo, L. Paoluzi, A. Bevilacqua, S. Charbit, M. Cribier, L. Gosset, J. Rich, M. Spiro, T. Stolarczyk, C. Tao, D. Vignaud, R.L. Hahn, F.X. Hartmann, J.K. Rowley, R.W. Stoenner, J. Weneser
Publikováno v:
Nuclear Physics B-Proceedings Supplements
Nuclear Physics B-Proceedings Supplements, 1995, 38 (1-3), pp.68-76. ⟨10.1016/0920-5632(94)00735-E⟩
Nuclear Physics B-Proceedings Supplements, Elsevier, 1995, 38 (1-3), pp.68-76. ⟨10.1016/0920-5632(94)00735-E⟩
Nuclear Physics B-Proceedings Supplements, 1995, 38 (1-3), pp.68-76. ⟨10.1016/0920-5632(94)00735-E⟩
Nuclear Physics B-Proceedings Supplements, Elsevier, 1995, 38 (1-3), pp.68-76. ⟨10.1016/0920-5632(94)00735-E⟩
The galliumchloride detector operated by the GALLEX-collaboration in the Gran Sasso Underground Laboratory responds primarily to pp-neutrinos. They are produced in the primary fusion reaction of hydrogen into deuterium and directly coupled to the sol
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c0fce524ec50a558859be38487311f9a
https://hal.science/hal-03094691
https://hal.science/hal-03094691