التفاصيل البيبلوغرافية
العنوان:
RECENT RESULTS FROM AMANDA
المؤلفون:
W. Wu , E. Schneider , D. M. Lowder , G. C. Hill , D. Schneider , Y. D. He , K. Rawlins , P. Askebjer , P. B. Price , D. Bierenbaum , T. Scheider , T. O. B. Schmidt , James Madsen , M. Hellwig , E. Andres , H. G. Sander , Glenn Spiczak , H. Rubinstein , Kurt Woschnagg , P. Ekström , M. M. Boyce , R. Schwarz , F. M. Newcomer , C. Walck , R. Hardtke , R. Porrata , G. B. Yodh , C. Pérez de los Heros , Albrecht Karle , I. Liubarsky , A. Mihalyi , Staffan Carius , P. Lindahl , R. C. Bay , P. Niessen , S. Young , P. Romenesko , Ariel Goobar , Christian Spiering , N. Starinsky , B. Erlandsson , H. S. Matis , D. Steele , D. F. Cowen , D. Chirkin , S. Hundertmark , A. Biron , Stefan Richter , Marek Kowalski , M. Solarz , T. Mikolajski , S. Tilav , H. Heukenkamp , P. C. Mock , P. Miocinovic , C. H. Wiebusch , J. Ludvig , D. Ross , K. H. Becker , L. Gray , Xinhua Bai , J. Booth , L. Thollander , A. Silvestri , I. Taboada , R. G. Stokstad , R. Wischnewski , H. Leich , T. C. Miller , R. Morse , J. E. Jacobsen , B. Koci , T. Thon , Lars Bergström , Kael Hanson , J. Rodríguez Martino , Hakki Ögelman , Adam Bouchta , Steven W. Barwick , A. Richards , Francis Halzen , Paolo Desiati , Allan Hallgren , J. P Dewulf , Ole Streicher , T. Neunhöffer , M. Vander Donckt , Olga Botner , V. Kandhadai , Wolfgang Rhode , P. Loaiza , A. Goldschmidt , Y. Minaeva , G. Barouch , M. Gaug , Caroline Costa , Ch. Weinheimer , Matthias Leuthold , D. R. Nygren , P. Steffen , L. Köpke , Jan Conrad , T. Feser , H. Haase , Jodi Cooley , E. Dalberg , D. Bertrand , A. Chen , Joakim Edsjö , Q. Sun , C. Reed , J. Dailing , P. Doksus , Nicholas G. Usechak , J. Kim , T. De Young , P. O. Hulth , H. Wissing , Pawel Marciniewski
المصدر:
International Journal of Modern Physics A . 16:1013-1015
بيانات النشر:
World Scientific Pub Co Pte Lt, 2001.
سنة النشر:
2001
مصطلحات موضوعية:
Physics , Nuclear and High Energy Physics , Muon , Physics::Instrumentation and Detectors , Astrophysics::High Energy Astrophysical Phenomena , Solar neutrino , Astrophysics::Instrumentation and Methods for Astrophysics , Astronomy , Astronomy and Astrophysics , Astrophysics , Solar neutrino problem , Atomic and Molecular Physics, and Optics , Neutrino detector , Measurements of neutrino speed , High Energy Physics::Experiment , Neutrino , Neutrino oscillation , Physics::Atmospheric and Oceanic Physics , Charged current
الوصف:
We present results based on data taken in 1997 with the 302-PMT Antarctic Muon and Neutrino Detector Array-B10 ("AMANDA-B10") array. Atmospheric neutrinos created in the northern hemisphere are observed indirectly through their charged current interactions which produce relativistic, Cherenkov-light-emitting upgoing muons in the South Pole ice cap. The reconstructed angular distribution of these events is in good agreement with expectation and demonstrates the viability of this ice-based device as a neutrino telescope.
تدمد:
1793-656X
URL الوصول:
https://explore.openaire.eu/search/publication?articleId=doi_________::b1656c81b78dd4e42721cb3de5f71de6 https://doi.org/10.1142/s0217751x01008746
رقم الأكسشن:
edsair.doi...........b1656c81b78dd4e42721cb3de5f71de6
قاعدة البيانات:
OpenAIRE
