ar X iv : a st ro - p h / 02 05 10 9 v 1 7 M ay 2 00 2 Observation of High Energy Atmospheric Neutrinos with the Antarctic Muon and Neutrino Detector Array
نویسندگان
چکیده
J. Ahrens, E. Andrés, X. Bai, G. Barouch, S.W. Barwick, R.C. Bay, T. Becka, K.-H. Becker, D. Bertrand, F. Binon, A. Biron, J. Booth, O. Botner, A. Bouchta,4∗ O. Bouhali, M.M. Boyce, S. Carius, A. Chen, D. Chirkin, J. Conrad, J. Cooley, C.G.S. Costa, D.F. Cowen, E. Dalberg,14† C. De Clercq, T. DeYoung,11‡ P. Desiati, J.-P. Dewulf, P. Doksus, J. Edsjö, P. Ekström, T. Feser, J.-M. Frère, T.K. Gaisser, M. Gaug4§ A. Goldschmidt, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Hauschildt, M. Hellwig, H. Heukenkamp, G.C. Hill, P.O. Hulth, S. Hundertmark, J. Jacobsen, A. Karle, J. Kim, B. Koci, L. Köpke, M. Kowalski, J.I. Lamoureux, H. Leich, M. Leuthold, P. Lindahl, I. Liubarsky, P. Loaiza, D.M. Lowder,7¶ J. Madsen, P. Marciniewski,13∗∗ H.S. Matis, C.P. McParland, T.C. Miller,1††, Y. Minaeva, P. Miočinović, P.C. Mock,8‡‡, R. Morse, T. Neunhöffer, P. Niessen, D.R. Nygren, H. Ögelman, Ph. Olbrechts, C. Pérez de los Heros, A.C. Pohl, R. Porrata,8§§ P.B. Price, G.T. Przybylski, K. Rawlins, C. Reed,8¶¶, W. Rhode, M. Ribordy, S. Richter, J. Rodŕıguez Martino, P. Romenesko, D. Ross, H.-G. Sander, T. Schmidt, D. Schneider, R. Schwarz, A. Silvestri, M. Solarz, G.M. Spiczak, C. Spiering, N. Starinsky,11∗∗∗, D. Steele, P. Steffen, R.G. Stokstad, O. Streicher, P. Sudhoff, K.-H. Sulanke, I. Taboada, L. Thollander, T. Thon, S. Tilav, M. Vander Donckt, C. Walck, C. Weinheimer, C.H. Wiebusch,4∗ C. Wiedeman, R. Wischnewski, H. Wissing, K. Woschnagg, W. Wu, G. Yodh, S. Young
منابع مشابه
iv : a st ro - p h / 02 05 40 8 v 1 2 3 M ay 2 00 2 High - energy Neutrinos from the Cosmic Accelerator RX J 1713
The observation of TeV-gamma rays of π 0 origin from the supernova remnant RX J1713.7-3946 has revealed the first specific site where protons are accelerated to energies typical of the main component of the cosmic rays. In this letter we calculate the high-energy neutrino flux associated with this source to be at least 40 muon-type neutrinos per kilometer-squared per year. We perform the same c...
متن کاملar X iv : a st ro - p h / 02 05 40 8 v 2 3 0 M ay 2 00 2 High - energy Neutrinos from the Cosmic Accelerator RX J 1713 . 7 - 3946
The observation of TeV-gamma rays of π 0 origin from the supernova remnant RX J1713.7-3946 might have revealed the first specific site where protons are accelerated to energies typical of the main component of the cosmic rays. In this letter we calculate the high-energy neutrino flux associated with this source to be 40 muon-type neutrinos per kilometer-squared per year. We perform the same cal...
متن کاملar X iv : a st ro - p h / 99 02 26 6 v 2 3 A pr 2 00 0 High Energy Cosmic Rays from Neutrinos
We address a class of models in which neutrinos, having a small mass, originate the highest energy cosmic rays interacting with the relic cosmic neutrino background. Assuming lepton number symmetry and an enhanced neutrino
متن کاملar X iv : a st ro - p h / 00 05 56 8 v 1 3 0 M ay 2 00 0 Hot and Cold Dark Matter Search with GENIUS ⋆
GENIUS is a proposal for a large volume detector to search for rare events. An array of 40–400 ’naked’ HPGe detectors will be operated in a tank filled with ultrapure liquid nitrogen. After a description of performed technical studies of detector operation in liquid nitrogen and of Monte Carlo simulations of expected background components, the potential of GENIUS for detecting WIMP dark matter,...
متن کاملar X iv : a st ro - p h / 05 08 67 5 v 1 31 A ug 2 00 5 Search for aDiffuse Flux ofHigh - Energy
We present the results of a search for high energy extraterrestrial neutrinos with the Baikal underwater Cherenkov detector NT200, based on data taken in 1998 2003. Upper limits on the diffuse fluxes of νe + νμ + ντ , predicted by several models of AGN-like neutrino sources, are derived. For an E−2 behavior of the neutrino Preprint submitted to Elsevier Science 1 September 2005 spectrum, our li...
متن کاملar X iv : a st ro - p h / 05 08 67 5 v 1 3 1 A ug 2 00 5 Search for aDiffuse Flux ofHigh - Energy Extraterrestrial Neutrinoswith theNT 200 NeutrinoTelescope
We present the results of a search for high energy extraterrestrial neutrinos with the Baikal underwater Cherenkov detector NT200, based on data taken in 1998 2003. Upper limits on the diffuse fluxes of νe + νμ + ντ , predicted by several models of AGN-like neutrino sources, are derived. For an E−2 behavior of the neutrino Preprint submitted to Elsevier Science 5 February 2008 spectrum, our lim...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2002