Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Klimushin, S. I."'
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
The description of muon propagation through large depths of matter, based on a concept of the correction factor, is proposed. The results of Monte-Carlo calculations of this correction factor are presented. The parametrizations for continuous energy
Externí odkaz:
http://arxiv.org/abs/hep-ph/0106010
Publikováno v:
Phys.Rev.D64:014016,2001
The analytical expression for angular integral flux of atmospheric muons in matter with the explicit relation of its parameters with those of the sea level spectrum is obtained. The fitting formula for the sea level muon spectrum at different zenith
Externí odkaz:
http://arxiv.org/abs/hep-ph/0012032
Knowledge of atmospheric muon flux intensity at large depths is extremely important for neutrino telescopes located deep under ground, water or ice. One of the methods to transform muon sea-level spectrum into depth one is to apply Monte Carlo techni
Externí odkaz:
http://arxiv.org/abs/hep-ph/0010323
Publikováno v:
Phys.Rev.D64:074015,2001
We present a new Monte Carlo muon propagation algorithm MUM (MUons+Medium) which possesses some advantages over analogous algorithms presently in use. The most important features of algorithm are described. Results on the test for accuracy of treatme
Externí odkaz:
http://arxiv.org/abs/hep-ph/0010322
Autor:
Belolaptikov, I. A., Bezrukov, L. B., Budnev, N. M., Bugaev, E. V., Djilkibaev, Zh. -A. M., Domogatsky, G. V., Doroshenko, A. A., Klabukov, A. M., Klimushin, S. I., Kuzmichev, L. A., Panfilov, A. I., Parfenov, Yu. V., Sokalski, I. A.
Supersymmetric models allow for stable non-topological solitons, Q-balls, which can be produced in the early Universe and contribute to dark matter. Experimental signature of electrically neutral Q-balls is, in fact, the same as is expected for super
Externí odkaz:
http://arxiv.org/abs/astro-ph/9802223
Autor:
Bagduev, R. I., Balkanov, V., Golikov, A. V., Glukhovskoi, B. M., Heller, R., Kabikov, V. B., Khripunova, M. P., Klabukov, A. M., Klimushin, S. I., Koshechkin, A. P., Kuzmichov, L. A., Lisovsky, G. V., Belolaptikov, I. A., Lubsandorzhev, B. K., Mikolajski, T., Osipova, E. A., Pokhil, P. G., Pokolev, P. A., Putilov, P. A., Spiering, C., Stepanenko, Z. I., Streicher, O., Thon, T., Bezrukov, Leonid B., Vorobev, A. A., Wischnewski, R., BAIKAL Collaboration, Budnev, N. M., Borisovets, B. A., Domogatsky, G. V., Donskich, L. A., Doroshenko, A. A., Garus, A. A.
30 pp. (1999).
A deep underwater Cherenkov telescope has been operating since 1993 in stages of growing size at 1.1 km depth in Lake Baikal. The key component of the telescope is the Optical Module (OM) which houses the highly sensitive phototub
A deep underwater Cherenkov telescope has been operating since 1993 in stages of growing size at 1.1 km depth in Lake Baikal. The key component of the telescope is the Optical Module (OM) which houses the highly sensitive phototub
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::66d203d52ac3fa59997fa392cea19fd2