Search for neutrino-induced cascades with the AMANDA detector

J. Ahrens, X. Bai, G. Barouch, S. W. Barwick, R. C. Bay, T. Becka, K. H. Becker, D. Bertrand, F. Binon, A. Biron, S. Böser, J. Booth, O. Botner, A. Bouchta, O. Bouhali, M. M. Boyce, T. Burgess, S. Carius, A. Chen, D. ChirkinJ. Conrad, J. Cooley, C. G.S. Costa, D. F. Cowen, A. Davour, C. De Clercq, T. DeYoung, P. Desiati, J. P. Dewulf, P. Doksus, P. Ekström, T. Feser, J. M. Frère, T. K. Gaisser, M. Gaug, H. Geenen, A. Goldschmidt, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Hauschildt, M. Hellwig, G. C. Hill, P. O. Hulth, K. Hultqvist, 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, D. M. Lowder, J. Madsen, P. Marciniewski, H. S. Matis, C. P. McParland, T. Messarius, T. C. Miller, Y. Minaeva, P. Miočinović, P. C. Mock, R. Morse, T. Neunhöffer, P. Niessen, D. R. Nygren, H. Ogelman, Ph Olbrechts, C. Pérez de los Heros, A. C. Pohl, R. Porrata, P. B. Price, G. T. Przybylski, K. Rawlins, C. Reed, E. Resconi, W. Rhode, M. Ribordy, S. Richter, J. Rodríguez Martino, P. Romenesko, D. Ross, H. G. Sander, K. Schinarakis, T. Schmidt, D. Schneider, R. Schwarz, A. Silvestri, M. Solarz, G. M. Spiczak, C. Spiering, N. Starinsky, D. Steele, P. Steffen, R. G. Stokstad, K. H. Sulanke, I. Taboada, L. Thollander, S. Tilav, M. Vander Donckt, W. Wagner, C. Walck, C. Weinheimer, C. H. Wiebusch, C. Widemann, R. Wischnewski, H. Wissing, K. Woschnagg, W. Wu, G. Yodh, S. Young

Research output: Contribution to journalArticlepeer-review

47 Scopus citations


We report on a search for electromagnetic and/or hadronic showers (cascades) induced by a diffuse flux of neutrinos with energies between 5 TeV and 300 TeV from extraterrestrial sources. Cascades may be produced by matter interactions of all flavors of neutrinos, and contained cascades have better energy resolution and afford better background rejection than throughgoing (Formula presented)-induced muons. Data taken in 1997 with the AMANDA detector were searched for events with a high-energy cascadelike signature. The observed events are consistent with expected backgrounds from atmospheric neutrinos and catastrophic energy losses from atmospheric muons. Effective volumes for all flavors of neutrinos, which allow the calculation of limits for any neutrino flux model, are presented. The limit on cascades from a diffuse flux of (Formula presented) is (Formula presented) assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of (Formula presented) is (Formula presented) independent of the assumed neutrino flavor flux ratio.

Original languageEnglish (US)
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Issue number1
StatePublished - Jan 10 2003

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)


Dive into the research topics of 'Search for neutrino-induced cascades with the AMANDA detector'. Together they form a unique fingerprint.

Cite this