Search for neutrino-induced cascades with the AMANDA detector
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 e...
Ausführliche Beschreibung
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2003 |
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Online-Ressource 10 |
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APS Digital Backfile Archive 1893-2003 |
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Enthalten in: Physical review / D - [S.l.] : Soc., 1970, 67(2003), 1 |
| Übergeordnetes Werk: |
volume:67 ; year:2003 ; number:1 ; extent:10 |
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NLEJ249943921 |
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| 520 | |a 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 νμ-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 νe+νμ+ντ+ν¯e+ν¯μ+ν¯τ is E2(dΦ/dE)<9.8×10-6 GeV cm-2 s-1 sr-1, assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of νe+ν¯e is E2(dΦ/dE)<6.5×10-6 GeV cm-2 s-1 sr-1, independent of the assumed neutrino flavor flux ratio. | ||
| 533 | |f APS Digital Backfile Archive 1893-2003 | ||
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(DE-627)NLEJ249943921 (DE-601)aps:14861df0a14f6e038a0a4e415eb1258bc608fcb2 DE-627 ger DE-627 rakwb Search for neutrino-induced cascades with the AMANDA detector 2003 Online-Ressource 10 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 νμ-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 νe+νμ+ντ+ν¯e+ν¯μ+ν¯τ is E2(dΦ/dE)<9.8×10-6 GeV cm-2 s-1 sr-1, assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of νe+ν¯e is E2(dΦ/dE)<6.5×10-6 GeV cm-2 s-1 sr-1, independent of the assumed neutrino flavor flux ratio. APS Digital Backfile Archive 1893-2003 Ahrens, J. oth Bai, X. oth Barouch, G. oth Barwick, S. W. oth Bay, R. C. oth Becka, T. oth Becker, K.-H. oth Bertrand, D. oth Binon, F. oth Biron, A. oth Böser, S. oth Booth, J. oth Botner, O. oth Bouchta, A. oth Bouhali, O. oth Boyce, M. M. oth Burgess, T. oth Carius, S. oth Chen, A. oth Chirkin, D. oth Conrad, J. oth Cooley, J. oth Costa, C. G. oth Cowen, D. F. oth Davour, A. oth De Clercq, C. oth DeYoung, T. oth Desiati, P. oth Dewulf, J.-P. oth Doksus, P. oth Ekström, P. oth Feser, T. oth Frère, J.-M. oth Gaisser, T. K. oth Gaug, M. oth Geenen, H. oth Goldschmidt, A. oth Hallgren, A. oth Halzen, F. oth Hanson, K. oth Hardtke, R. oth Hauschildt, T. oth Hellwig, M. oth Hill, G. C. oth Hulth, P. O. oth Hultqvist, K. oth Hundertmark, S. oth Jacobsen, J. oth Karle, A. oth Kim, J. oth Koci, B. oth Köpke, L. oth Kowalski, M. oth Lamoureux, J. I. oth Leich, H. oth Leuthold, M. oth Lindahl, P. oth Liubarsky, I. oth Lowder, D. M. oth Madsen, J. oth Marciniewski, P. oth Matis, H. S. oth McParland, C. P. oth Messarius, T. oth Miller, T. C. oth Minaeva, Y. oth Miočinović, P. oth Mock, P. C. oth Morse, R. oth Neunhöffer, T. oth Niessen, P. oth Nygren, D. R. oth Ogelman, H. oth Olbrechts, Ph. oth Pérez de los Heros, C. oth Pohl, A. C. oth Porrata, R. oth Price, P. B. oth Przybylski, G. T. oth Rawlins, K. oth Reed, C. oth Resconi, E. oth Rhode, W. oth Ribordy, M. oth Richter, S. oth Rodríguez Martino, J. oth Romenesko, P. oth Ross, D. oth Sander, H.-G. oth Schinarakis, K. oth Schmidt, T. oth Schneider, D. oth Schwarz, R. oth Silvestri, A. oth Solarz, M. oth Spiczak, G. M. oth Spiering, C. oth Starinsky, N. oth Steele, D. oth Steffen, P. oth Stokstad, R. G. oth Sulanke, K.-H. oth Taboada, I. oth Thollander, L. oth Tilav, S. oth Vander Donckt, M. oth Wagner, W. oth Walck, C. oth Weinheimer, C. oth Wiebusch, C. H. oth Widemann, C. oth Wischnewski, R. oth Wissing, H. oth Woschnagg, K. oth Wu, W. oth Yodh, G. oth Young, S. oth Enthalten in Physical review / D [S.l.] : Soc., 1970 67(2003), 1 Online-Ressource (DE-627)NLEJ248237861 (DE-600)1461167-3 1550-2368 nnns volume:67 year:2003 number:1 extent:10 https://www.tib.eu/de/suchen/id/aps%3A14861df0a14f6e038a0a4e415eb1258bc608fcb2 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 67 2003 1 10 |
| spelling |
(DE-627)NLEJ249943921 (DE-601)aps:14861df0a14f6e038a0a4e415eb1258bc608fcb2 DE-627 ger DE-627 rakwb Search for neutrino-induced cascades with the AMANDA detector 2003 Online-Ressource 10 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 νμ-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 νe+νμ+ντ+ν¯e+ν¯μ+ν¯τ is E2(dΦ/dE)<9.8×10-6 GeV cm-2 s-1 sr-1, assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of νe+ν¯e is E2(dΦ/dE)<6.5×10-6 GeV cm-2 s-1 sr-1, independent of the assumed neutrino flavor flux ratio. APS Digital Backfile Archive 1893-2003 Ahrens, J. oth Bai, X. oth Barouch, G. oth Barwick, S. W. oth Bay, R. C. oth Becka, T. oth Becker, K.-H. oth Bertrand, D. oth Binon, F. oth Biron, A. oth Böser, S. oth Booth, J. oth Botner, O. oth Bouchta, A. oth Bouhali, O. oth Boyce, M. M. oth Burgess, T. oth Carius, S. oth Chen, A. oth Chirkin, D. oth Conrad, J. oth Cooley, J. oth Costa, C. G. oth Cowen, D. F. oth Davour, A. oth De Clercq, C. oth DeYoung, T. oth Desiati, P. oth Dewulf, J.-P. oth Doksus, P. oth Ekström, P. oth Feser, T. oth Frère, J.-M. oth Gaisser, T. K. oth Gaug, M. oth Geenen, H. oth Goldschmidt, A. oth Hallgren, A. oth Halzen, F. oth Hanson, K. oth Hardtke, R. oth Hauschildt, T. oth Hellwig, M. oth Hill, G. C. oth Hulth, P. O. oth Hultqvist, K. oth Hundertmark, S. oth Jacobsen, J. oth Karle, A. oth Kim, J. oth Koci, B. oth Köpke, L. oth Kowalski, M. oth Lamoureux, J. I. oth Leich, H. oth Leuthold, M. oth Lindahl, P. oth Liubarsky, I. oth Lowder, D. M. oth Madsen, J. oth Marciniewski, P. oth Matis, H. S. oth McParland, C. P. oth Messarius, T. oth Miller, T. C. oth Minaeva, Y. oth Miočinović, P. oth Mock, P. C. oth Morse, R. oth Neunhöffer, T. oth Niessen, P. oth Nygren, D. R. oth Ogelman, H. oth Olbrechts, Ph. oth Pérez de los Heros, C. oth Pohl, A. C. oth Porrata, R. oth Price, P. B. oth Przybylski, G. T. oth Rawlins, K. oth Reed, C. oth Resconi, E. oth Rhode, W. oth Ribordy, M. oth Richter, S. oth Rodríguez Martino, J. oth Romenesko, P. oth Ross, D. oth Sander, H.-G. oth Schinarakis, K. oth Schmidt, T. oth Schneider, D. oth Schwarz, R. oth Silvestri, A. oth Solarz, M. oth Spiczak, G. M. oth Spiering, C. oth Starinsky, N. oth Steele, D. oth Steffen, P. oth Stokstad, R. G. oth Sulanke, K.-H. oth Taboada, I. oth Thollander, L. oth Tilav, S. oth Vander Donckt, M. oth Wagner, W. oth Walck, C. oth Weinheimer, C. oth Wiebusch, C. H. oth Widemann, C. oth Wischnewski, R. oth Wissing, H. oth Woschnagg, K. oth Wu, W. oth Yodh, G. oth Young, S. oth Enthalten in Physical review / D [S.l.] : Soc., 1970 67(2003), 1 Online-Ressource (DE-627)NLEJ248237861 (DE-600)1461167-3 1550-2368 nnns volume:67 year:2003 number:1 extent:10 https://www.tib.eu/de/suchen/id/aps%3A14861df0a14f6e038a0a4e415eb1258bc608fcb2 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 67 2003 1 10 |
| allfields_unstemmed |
(DE-627)NLEJ249943921 (DE-601)aps:14861df0a14f6e038a0a4e415eb1258bc608fcb2 DE-627 ger DE-627 rakwb Search for neutrino-induced cascades with the AMANDA detector 2003 Online-Ressource 10 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 νμ-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 νe+νμ+ντ+ν¯e+ν¯μ+ν¯τ is E2(dΦ/dE)<9.8×10-6 GeV cm-2 s-1 sr-1, assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of νe+ν¯e is E2(dΦ/dE)<6.5×10-6 GeV cm-2 s-1 sr-1, independent of the assumed neutrino flavor flux ratio. APS Digital Backfile Archive 1893-2003 Ahrens, J. oth Bai, X. oth Barouch, G. oth Barwick, S. W. oth Bay, R. C. oth Becka, T. oth Becker, K.-H. oth Bertrand, D. oth Binon, F. oth Biron, A. oth Böser, S. oth Booth, J. oth Botner, O. oth Bouchta, A. oth Bouhali, O. oth Boyce, M. M. oth Burgess, T. oth Carius, S. oth Chen, A. oth Chirkin, D. oth Conrad, J. oth Cooley, J. oth Costa, C. G. oth Cowen, D. F. oth Davour, A. oth De Clercq, C. oth DeYoung, T. oth Desiati, P. oth Dewulf, J.-P. oth Doksus, P. oth Ekström, P. oth Feser, T. oth Frère, J.-M. oth Gaisser, T. K. oth Gaug, M. oth Geenen, H. oth Goldschmidt, A. oth Hallgren, A. oth Halzen, F. oth Hanson, K. oth Hardtke, R. oth Hauschildt, T. oth Hellwig, M. oth Hill, G. C. oth Hulth, P. O. oth Hultqvist, K. oth Hundertmark, S. oth Jacobsen, J. oth Karle, A. oth Kim, J. oth Koci, B. oth Köpke, L. oth Kowalski, M. oth Lamoureux, J. I. oth Leich, H. oth Leuthold, M. oth Lindahl, P. oth Liubarsky, I. oth Lowder, D. M. oth Madsen, J. oth Marciniewski, P. oth Matis, H. S. oth McParland, C. P. oth Messarius, T. oth Miller, T. C. oth Minaeva, Y. oth Miočinović, P. oth Mock, P. C. oth Morse, R. oth Neunhöffer, T. oth Niessen, P. oth Nygren, D. R. oth Ogelman, H. oth Olbrechts, Ph. oth Pérez de los Heros, C. oth Pohl, A. C. oth Porrata, R. oth Price, P. B. oth Przybylski, G. T. oth Rawlins, K. oth Reed, C. oth Resconi, E. oth Rhode, W. oth Ribordy, M. oth Richter, S. oth Rodríguez Martino, J. oth Romenesko, P. oth Ross, D. oth Sander, H.-G. oth Schinarakis, K. oth Schmidt, T. oth Schneider, D. oth Schwarz, R. oth Silvestri, A. oth Solarz, M. oth Spiczak, G. M. oth Spiering, C. oth Starinsky, N. oth Steele, D. oth Steffen, P. oth Stokstad, R. G. oth Sulanke, K.-H. oth Taboada, I. oth Thollander, L. oth Tilav, S. oth Vander Donckt, M. oth Wagner, W. oth Walck, C. oth Weinheimer, C. oth Wiebusch, C. H. oth Widemann, C. oth Wischnewski, R. oth Wissing, H. oth Woschnagg, K. oth Wu, W. oth Yodh, G. oth Young, S. oth Enthalten in Physical review / D [S.l.] : Soc., 1970 67(2003), 1 Online-Ressource (DE-627)NLEJ248237861 (DE-600)1461167-3 1550-2368 nnns volume:67 year:2003 number:1 extent:10 https://www.tib.eu/de/suchen/id/aps%3A14861df0a14f6e038a0a4e415eb1258bc608fcb2 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 67 2003 1 10 |
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(DE-627)NLEJ249943921 (DE-601)aps:14861df0a14f6e038a0a4e415eb1258bc608fcb2 DE-627 ger DE-627 rakwb Search for neutrino-induced cascades with the AMANDA detector 2003 Online-Ressource 10 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 νμ-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 νe+νμ+ντ+ν¯e+ν¯μ+ν¯τ is E2(dΦ/dE)<9.8×10-6 GeV cm-2 s-1 sr-1, assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of νe+ν¯e is E2(dΦ/dE)<6.5×10-6 GeV cm-2 s-1 sr-1, independent of the assumed neutrino flavor flux ratio. APS Digital Backfile Archive 1893-2003 Ahrens, J. oth Bai, X. oth Barouch, G. oth Barwick, S. W. oth Bay, R. C. oth Becka, T. oth Becker, K.-H. oth Bertrand, D. oth Binon, F. oth Biron, A. oth Böser, S. oth Booth, J. oth Botner, O. oth Bouchta, A. oth Bouhali, O. oth Boyce, M. M. oth Burgess, T. oth Carius, S. oth Chen, A. oth Chirkin, D. oth Conrad, J. oth Cooley, J. oth Costa, C. G. oth Cowen, D. F. oth Davour, A. oth De Clercq, C. oth DeYoung, T. oth Desiati, P. oth Dewulf, J.-P. oth Doksus, P. oth Ekström, P. oth Feser, T. oth Frère, J.-M. oth Gaisser, T. K. oth Gaug, M. oth Geenen, H. oth Goldschmidt, A. oth Hallgren, A. oth Halzen, F. oth Hanson, K. oth Hardtke, R. oth Hauschildt, T. oth Hellwig, M. oth Hill, G. C. oth Hulth, P. O. oth Hultqvist, K. oth Hundertmark, S. oth Jacobsen, J. oth Karle, A. oth Kim, J. oth Koci, B. oth Köpke, L. oth Kowalski, M. oth Lamoureux, J. I. oth Leich, H. oth Leuthold, M. oth Lindahl, P. oth Liubarsky, I. oth Lowder, D. M. oth Madsen, J. oth Marciniewski, P. oth Matis, H. S. oth McParland, C. P. oth Messarius, T. oth Miller, T. C. oth Minaeva, Y. oth Miočinović, P. oth Mock, P. C. oth Morse, R. oth Neunhöffer, T. oth Niessen, P. oth Nygren, D. R. oth Ogelman, H. oth Olbrechts, Ph. oth Pérez de los Heros, C. oth Pohl, A. C. oth Porrata, R. oth Price, P. B. oth Przybylski, G. T. oth Rawlins, K. oth Reed, C. oth Resconi, E. oth Rhode, W. oth Ribordy, M. oth Richter, S. oth Rodríguez Martino, J. oth Romenesko, P. oth Ross, D. oth Sander, H.-G. oth Schinarakis, K. oth Schmidt, T. oth Schneider, D. oth Schwarz, R. oth Silvestri, A. oth Solarz, M. oth Spiczak, G. M. oth Spiering, C. oth Starinsky, N. oth Steele, D. oth Steffen, P. oth Stokstad, R. G. oth Sulanke, K.-H. oth Taboada, I. oth Thollander, L. oth Tilav, S. oth Vander Donckt, M. oth Wagner, W. oth Walck, C. oth Weinheimer, C. oth Wiebusch, C. H. oth Widemann, C. oth Wischnewski, R. oth Wissing, H. oth Woschnagg, K. oth Wu, W. oth Yodh, G. oth Young, S. oth Enthalten in Physical review / D [S.l.] : Soc., 1970 67(2003), 1 Online-Ressource (DE-627)NLEJ248237861 (DE-600)1461167-3 1550-2368 nnns volume:67 year:2003 number:1 extent:10 https://www.tib.eu/de/suchen/id/aps%3A14861df0a14f6e038a0a4e415eb1258bc608fcb2 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 67 2003 1 10 |
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(DE-627)NLEJ249943921 (DE-601)aps:14861df0a14f6e038a0a4e415eb1258bc608fcb2 DE-627 ger DE-627 rakwb Search for neutrino-induced cascades with the AMANDA detector 2003 Online-Ressource 10 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier 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 νμ-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 νe+νμ+ντ+ν¯e+ν¯μ+ν¯τ is E2(dΦ/dE)<9.8×10-6 GeV cm-2 s-1 sr-1, assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of νe+ν¯e is E2(dΦ/dE)<6.5×10-6 GeV cm-2 s-1 sr-1, independent of the assumed neutrino flavor flux ratio. APS Digital Backfile Archive 1893-2003 Ahrens, J. oth Bai, X. oth Barouch, G. oth Barwick, S. W. oth Bay, R. C. oth Becka, T. oth Becker, K.-H. oth Bertrand, D. oth Binon, F. oth Biron, A. oth Böser, S. oth Booth, J. oth Botner, O. oth Bouchta, A. oth Bouhali, O. oth Boyce, M. M. oth Burgess, T. oth Carius, S. oth Chen, A. oth Chirkin, D. oth Conrad, J. oth Cooley, J. oth Costa, C. G. oth Cowen, D. F. oth Davour, A. oth De Clercq, C. oth DeYoung, T. oth Desiati, P. oth Dewulf, J.-P. oth Doksus, P. oth Ekström, P. oth Feser, T. oth Frère, J.-M. oth Gaisser, T. K. oth Gaug, M. oth Geenen, H. oth Goldschmidt, A. oth Hallgren, A. oth Halzen, F. oth Hanson, K. oth Hardtke, R. oth Hauschildt, T. oth Hellwig, M. oth Hill, G. C. oth Hulth, P. O. oth Hultqvist, K. oth Hundertmark, S. oth Jacobsen, J. oth Karle, A. oth Kim, J. oth Koci, B. oth Köpke, L. oth Kowalski, M. oth Lamoureux, J. I. oth Leich, H. oth Leuthold, M. oth Lindahl, P. oth Liubarsky, I. oth Lowder, D. M. oth Madsen, J. oth Marciniewski, P. oth Matis, H. S. oth McParland, C. P. oth Messarius, T. oth Miller, T. C. oth Minaeva, Y. oth Miočinović, P. oth Mock, P. C. oth Morse, R. oth Neunhöffer, T. oth Niessen, P. oth Nygren, D. R. oth Ogelman, H. oth Olbrechts, Ph. oth Pérez de los Heros, C. oth Pohl, A. C. oth Porrata, R. oth Price, P. B. oth Przybylski, G. T. oth Rawlins, K. oth Reed, C. oth Resconi, E. oth Rhode, W. oth Ribordy, M. oth Richter, S. oth Rodríguez Martino, J. oth Romenesko, P. oth Ross, D. oth Sander, H.-G. oth Schinarakis, K. oth Schmidt, T. oth Schneider, D. oth Schwarz, R. oth Silvestri, A. oth Solarz, M. oth Spiczak, G. M. oth Spiering, C. oth Starinsky, N. oth Steele, D. oth Steffen, P. oth Stokstad, R. G. oth Sulanke, K.-H. oth Taboada, I. oth Thollander, L. oth Tilav, S. oth Vander Donckt, M. oth Wagner, W. oth Walck, C. oth Weinheimer, C. oth Wiebusch, C. H. oth Widemann, C. oth Wischnewski, R. oth Wissing, H. oth Woschnagg, K. oth Wu, W. oth Yodh, G. oth Young, S. oth Enthalten in Physical review / D [S.l.] : Soc., 1970 67(2003), 1 Online-Ressource (DE-627)NLEJ248237861 (DE-600)1461167-3 1550-2368 nnns volume:67 year:2003 number:1 extent:10 https://www.tib.eu/de/suchen/id/aps%3A14861df0a14f6e038a0a4e415eb1258bc608fcb2 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 67 2003 1 10 |
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Ahrens, J. @@oth@@ Bai, X. @@oth@@ Barouch, G. @@oth@@ Barwick, S. W. @@oth@@ Bay, R. C. @@oth@@ Becka, T. @@oth@@ Becker, K.-H. @@oth@@ Bertrand, D. @@oth@@ Binon, F. @@oth@@ Biron, A. @@oth@@ Böser, S. @@oth@@ Booth, J. @@oth@@ Botner, O. @@oth@@ Bouchta, A. @@oth@@ Bouhali, O. @@oth@@ Boyce, M. M. @@oth@@ Burgess, T. @@oth@@ Carius, S. @@oth@@ Chen, A. @@oth@@ Chirkin, D. @@oth@@ Conrad, J. @@oth@@ Cooley, J. @@oth@@ Costa, C. G. @@oth@@ Cowen, D. F. @@oth@@ Davour, A. @@oth@@ De Clercq, C. @@oth@@ DeYoung, T. @@oth@@ Desiati, P. @@oth@@ Dewulf, J.-P. @@oth@@ Doksus, P. @@oth@@ Ekström, P. @@oth@@ Feser, T. @@oth@@ Frère, J.-M. @@oth@@ Gaisser, T. K. @@oth@@ Gaug, M. @@oth@@ Geenen, H. @@oth@@ Goldschmidt, A. @@oth@@ Hallgren, A. @@oth@@ Halzen, F. @@oth@@ Hanson, K. @@oth@@ Hardtke, R. @@oth@@ Hauschildt, T. @@oth@@ Hellwig, M. @@oth@@ Hill, G. C. @@oth@@ Hulth, P. O. @@oth@@ Hultqvist, K. @@oth@@ Hundertmark, S. @@oth@@ Jacobsen, J. @@oth@@ Karle, A. @@oth@@ Kim, J. @@oth@@ Koci, B. @@oth@@ Köpke, L. @@oth@@ Kowalski, M. @@oth@@ Lamoureux, J. I. @@oth@@ Leich, H. @@oth@@ Leuthold, M. @@oth@@ Lindahl, P. @@oth@@ Liubarsky, I. @@oth@@ Lowder, D. M. @@oth@@ Madsen, J. @@oth@@ Marciniewski, P. @@oth@@ Matis, H. S. @@oth@@ McParland, C. P. @@oth@@ Messarius, T. @@oth@@ Miller, T. C. @@oth@@ Minaeva, Y. @@oth@@ Miočinović, P. @@oth@@ Mock, P. C. @@oth@@ Morse, R. @@oth@@ Neunhöffer, T. @@oth@@ Niessen, P. @@oth@@ Nygren, D. R. @@oth@@ Ogelman, H. @@oth@@ Olbrechts, Ph. @@oth@@ Pérez de los Heros, C. @@oth@@ Pohl, A. C. @@oth@@ Porrata, R. @@oth@@ Price, P. B. @@oth@@ Przybylski, G. T. @@oth@@ Rawlins, K. @@oth@@ Reed, C. @@oth@@ Resconi, E. @@oth@@ Rhode, W. @@oth@@ Ribordy, M. @@oth@@ Richter, S. @@oth@@ Rodríguez Martino, J. @@oth@@ Romenesko, P. @@oth@@ Ross, D. @@oth@@ Sander, H.-G. @@oth@@ Schinarakis, K. @@oth@@ Schmidt, T. @@oth@@ Schneider, D. @@oth@@ Schwarz, R. @@oth@@ Silvestri, A. @@oth@@ Solarz, M. @@oth@@ Spiczak, G. M. @@oth@@ Spiering, C. @@oth@@ Starinsky, N. @@oth@@ Steele, D. @@oth@@ Steffen, P. @@oth@@ Stokstad, R. G. @@oth@@ Sulanke, K.-H. @@oth@@ Taboada, I. @@oth@@ Thollander, L. @@oth@@ Tilav, S. @@oth@@ Vander Donckt, M. @@oth@@ Wagner, W. @@oth@@ Walck, C. @@oth@@ Weinheimer, C. @@oth@@ Wiebusch, C. H. @@oth@@ Widemann, C. @@oth@@ Wischnewski, R. @@oth@@ Wissing, H. @@oth@@ Woschnagg, K. @@oth@@ Wu, W. @@oth@@ Yodh, G. @@oth@@ Young, S. @@oth@@ |
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Search for neutrino-induced cascades with the AMANDA detector |
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search for neutrino-induced cascades with the amanda detector |
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Search for neutrino-induced cascades with the AMANDA detector |
| abstract |
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 νμ-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 νe+νμ+ντ+ν¯e+ν¯μ+ν¯τ is E2(dΦ/dE)<9.8×10-6 GeV cm-2 s-1 sr-1, assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of νe+ν¯e is E2(dΦ/dE)<6.5×10-6 GeV cm-2 s-1 sr-1, independent of the assumed neutrino flavor flux ratio. |
| abstractGer |
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 νμ-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 νe+νμ+ντ+ν¯e+ν¯μ+ν¯τ is E2(dΦ/dE)<9.8×10-6 GeV cm-2 s-1 sr-1, assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of νe+ν¯e is E2(dΦ/dE)<6.5×10-6 GeV cm-2 s-1 sr-1, independent of the assumed neutrino flavor flux ratio. |
| abstract_unstemmed |
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 νμ-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 νe+νμ+ντ+ν¯e+ν¯μ+ν¯τ is E2(dΦ/dE)<9.8×10-6 GeV cm-2 s-1 sr-1, assuming a neutrino flavor flux ratio of 1:1:1 at the detector. The limit on cascades from a diffuse flux of νe+ν¯e is E2(dΦ/dE)<6.5×10-6 GeV cm-2 s-1 sr-1, independent of the assumed neutrino flavor flux ratio. |
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Search for neutrino-induced cascades with the AMANDA detector |
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Ahrens, J. Bai, X. Barouch, G. Barwick, S. W. Bay, R. C. Becka, T. Becker, K.-H. Bertrand, D. Binon, F. Biron, A. Böser, S. Booth, J. Botner, O. Bouchta, A. Bouhali, O. Boyce, M. M. Burgess, T. Carius, S. Chen, A. Chirkin, D. Conrad, J. Cooley, J. Costa, C. G. Cowen, D. F. Davour, A. De Clercq, C. DeYoung, T. Desiati, P. Dewulf, J.-P. Doksus, P. Ekström, P. Feser, T. Frère, J.-M. Gaisser, T. K. Gaug, M. Geenen, H. Goldschmidt, A. Hallgren, A. Halzen, F. Hanson, K. Hardtke, R. Hauschildt, T. Hellwig, M. Hill, G. C. Hulth, P. O. Hultqvist, K. Hundertmark, S. Jacobsen, J. Karle, A. Kim, J. Koci, B. Köpke, L. Kowalski, M. Lamoureux, J. I. Leich, H. Leuthold, M. Lindahl, P. Liubarsky, I. Lowder, D. M. Madsen, J. Marciniewski, P. Matis, H. S. McParland, C. P. Messarius, T. Miller, T. C. Minaeva, Y. Miočinović, P. Mock, P. C. Morse, R. Neunhöffer, T. Niessen, P. Nygren, D. R. Ogelman, H. Olbrechts, Ph Pérez de los Heros, C. Pohl, A. C. Porrata, R. Price, P. B. Przybylski, G. T. Rawlins, K. Reed, C. Resconi, E. Rhode, W. Ribordy, M. Richter, S. Rodríguez Martino, J. Romenesko, P. Ross, D. Sander, H.-G. Schinarakis, K. Schmidt, T. Schneider, D. Schwarz, R. Silvestri, A. Solarz, M. Spiczak, G. M. Spiering, C. Starinsky, N. Steele, D. Steffen, P. Stokstad, R. G. Sulanke, K.-H. Taboada, I. Thollander, L. Tilav, S. Vander Donckt, M. Wagner, W. Walck, C. Weinheimer, C. Wiebusch, C. H. Widemann, C. Wischnewski, R. Wissing, H. Woschnagg, K. Wu, W. Yodh, G. Young, S. |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000naa a22002652 4500</leader><controlfield tag="001">NLEJ249943921</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20231114103226.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">231114s2003 xx |||||o 00| ||und c</controlfield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)NLEJ249943921</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-601)aps:14861df0a14f6e038a0a4e415eb1258bc608fcb2</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Search for neutrino-induced cascades with the AMANDA detector</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2003</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">10</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">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. 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