Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Sokalski, I. A."'
Autor:
Akindinov, A. V., Anassontzis, E. G., Anton, G., Ardid, M., Aublin, J., Baret, B., Bertin, V., Bourret, S., Bozza, C., Bruchner, M., Bruijn, R., Brunner, J., Chabab, M., Chau, N., Chepurnov, A. S., Molla, M. Colomer, Coyle, P., Creusot, A., de Wasseige, G., Domi, A., Donzaud, C., Eberl, T., Enzenhöfer, A., Faifman, M., Filipović, M. D., Fusco, L., Garkusha, V. I., Gal, T., Gozzini, S. R., Graf, K., Grégoire, T., Grella, G., Hallmann, S., Heijboer, A., Hernández-Rey, J. J., Hofestädt, J., Ivanov, S. V., James, C. W., de Jong, M., de Jong, P., Kalaczyński, P., Kakorin, I. D., Katz, U. F., Chowdhury, N. R. Khan, Kirsanov, M. M., Kouchner, A., Kulikovskiy, V., Kuzmin, K. S., Breton, R. Le, Lebedev, O. P., Lincetto, M., Litvinovich, E., Lopez-Coto, D., Markou, C., Maximov, A. V., Melis, K. W., Muller, R., Naumov, V. A., Navas, S., Nauta, L., Nielsen, C., Novoskoltsev, F. N., Fearraigh, B. Ó, Organokov, M., Papalashvili, G., Perrin-Terrin, M., Poirè, C., Pradier, T., Quinn, L., Samtleben, D. F. E., Sanguineti, M., Seneca, J., Shanidze, R., Shirokov, E. V., Sinopoulou, A., Sinyukov, R. Yu., Skorokhvatov, M. D., Sokalski, I., Sokolov, A. A., Spisso, B., Stellacci, S. M., Strandberg, B., Taiuti, M., Thakore, T., Tzamariudaki, E., Van Elewyck, V., de Wolf, E., Zaborov, D., Zaitsev, A. M., Zornoza, J. D., Zúñiga, J.
Publikováno v:
Eur. Phys. J. C (2019) 79: 758
The Protvino accelerator facility located in the Moscow region, Russia, is in a good position to offer a rich experimental research program in the field of neutrino physics. Of particular interest is the possibility to direct a neutrino beam from Pro
Externí odkaz:
http://arxiv.org/abs/1902.06083
Autor:
Sokalski, I.
Scientific motivations for ultra- and extremely high energy neutrino astronomy are considered. Sources and expected fluxes of EHE/UHE neutrinos are briefly discussed. Operating and planned experiments on astrophysical neutrino detection are reviewed
Externí odkaz:
http://arxiv.org/abs/hep-ex/0501004
Autor:
Sokalski, I.
The ANTARES collaboration aims to build a deep underwater Cherenkov neutrino telescope in the Mediterranean Sea at 2500 m depth, about 40 km off-shore of La Seyne sur Mer, near Toulon. The collaboration was formed in 1996 and the experiment is curren
Externí odkaz:
http://arxiv.org/abs/hep-ex/0501003
Publikováno v:
Phys.Atom.Nucl.67:1177-1181,2004; Yad.Fiz.67N6:1200-1203,2004
We present results of the detailed Monte Carlo calculation of the rates of double-bang events in 1 km$^3$ underwater neutrino telescope with taking into account the effects of $\tau$-neutrino propagation through the Earth. As an input, the moderately
Externí odkaz:
http://arxiv.org/abs/astro-ph/0311086
Autor:
Sokalski, I.
Publikováno v:
Phys.Atom.Nucl.67:1172-1176,2004; Yad.Fiz.67N6:1195-1199,2004
The ANTARES project aims to build a deep underwater Cherenkov neutrino telescope in the Mediterranean Sea. Currently the experiment is in the construction phase and has recently achieved two important milestones. The electro-optical cable to shore an
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310130
If neutrinos produced in astrophysics sources oscillate, neutrino telescopes can have a chance to detect signals from tau-neutrinos. We present an estimate of the 'double bang' event rate produced by tau neutrinos in cubic kilometer scale detectors.<
Externí odkaz:
http://arxiv.org/abs/astro-ph/0305284
We present the formula for angular distribution of integral flux of conventional ($\pi, K$) muons deep under water taking into account the sphericity of the atmosphere and fluctuations of muon energy losses.The accuracy of this formula for various se
Externí odkaz:
http://arxiv.org/abs/hep-ph/0202065
Chain of calculations which have to be performed to predict any kind of signal in a deep underwater/ice neutrino detector necessarily includes the lepton propagation through thick layers of matter, as neutrino can be observed only by means of leptons
Externí odkaz:
http://arxiv.org/abs/hep-ph/0201122
We present a new muon propagation Monte Carlo FORTRAN code MUM (MUons+Medium) which possesses some advantages over analogous codes presently in use. The most important features of the algorithm are described. Data on the test for algorithm accuracy a
Externí odkaz:
http://arxiv.org/abs/hep-ph/0106011
The analytical expression for integral energy spectra and zenith angle distributions of atmospheric muons at large depths is derived. Fluctuations of muon energy losses are described using the parametrized correction factor. The fitting formula for t
Externí odkaz:
http://arxiv.org/abs/hep-ph/0106009