Search for neutrino-induced cascades with five years of AMANDA data

R. Abbasi; Y. Abdou; T. Abu-Zayyad; O. Actis; J. Adams; J. A. Aguilar; M. Ahlers; K. Andeen; J. Auffenberg; X. Bai; M. Baker; S. W. Barwick; R. Bay; J. L. Bazo Alba; K. Beattie; J. J. Beatty; S. Bechet; J. K. Becker; K. H. Becker; M. L. Benabderrahmane; J. Berdermann; P. Berghaus; D. Berley; E. Bernardini; D. Bertrand; D. Z. Besson; M. Bissok; E. Blaufuss; D. J. Boersma; C. Bohm; S. Böser; O. Botner; L. Bradley; J. Braun; S. Buitink; M. Carson; D. Chirkin; B. Christy; J. Clem; F. Clevermann; S. Cohen; C. Colnard; D. F. Cowen; M. V. D'Agostino; M. Danninger; J. C. Davis; C. De Clercq; L. Demirörs; O. Depaepe; F. Descamps; P. Desiati; G. De Vries-Uiterweerd; T. Deyoung; J. C. Díaz-Vélez; J. Dreyer; J. P. Dumm; M. R. Duvoort; R. Ehrlich; J. Eisch; R. W. Ellsworth; O. Engdegrd; S. Euler; P. A. Evenson; O. Fadiran; A. R. Fazely; T. Feusels; K. Filimonov; C. Finley; M. M. Foerster; B. D. Fox; A. Franckowiak; R. Franke; T. K. Gaisser; J. Gallagher; R. Ganugapati; M. Geisler; L. Gerhardt; L. Gladstone; T. Glüsenkamp; A. Goldschmidt; J. A. Goodman; D. Grant; T. Griesel; A. Groß; S. Grullon; R. M. Gunasingha; M. Gurtner; C. Ha; A. Hallgren; F. Halzen; K. Han; K. Hanson; K. Helbing; P. Herquet; S. Hickford; G. C. Hill; K. D. Hoffman; A. Homeier; K. Hoshina; D. Hubert; W. Huelsnitz; J. P. Hülß; P. O. Hulth; K. Hultqvist; S. Hussain; R. L. Imlay; A. Ishihara; J. Jacobsen; G. S. Japaridze; H. Johansson; J. M. Joseph; K. H. Kampert; A. Kappes; T. Karg; A. Karle; J. L. Kelley; N. Kemming; P. Kenny; J. Kiryluk; F. Kislat; S. R. Klein; S. Knops; J. H. Köhne; G. Kohnen; H. Kolanoski; L. Köpke; D. J. Koskinen; M. Kowalski; T. Kowarik; M. Krasberg; T. Krings; G. Kroll; K. Kuehn; T. Kuwabara; M. Labare; S. Lafebre; K. Laihem; H. Landsman; R. Lauer; R. Lehmann; D. Lennarz; J. Lünemann; J. Madsen; P. Majumdar; R. Maruyama; K. Mase; H. S. Matis; M. Matusik; K. Meagher; M. Merck; P. Mészáros; T. Meures; E. Middell; N. Milke; J. Miller; T. Montaruli; R. Morse; S. M. Movit; R. Nahnhauer; J. W. Nam; U. Naumann; P. Nießen; D. R. Nygren; S. Odrowski; A. Olivas; M. Olivo; M. Ono; S. Panknin; L. Paul; C. Pérez De Los Heros; J. Petrovic; A. Piegsa; D. Pieloth; R. Porrata; J. Posselt; P. B. Price; M. Prikockis; G. T. Przybylski; K. Rawlins; P. Redl; E. Resconi; W. Rhode; M. Ribordy; A. Rizzo; J. P. Rodrigues; P. Roth; F. Rothmaier; C. Rott; C. Roucelle; T. Ruhe; D. Rutledge; B. Ruzybayev; D. Ryckbosch; H. G. Sander; S. Sarkar; K. Schatto; S. Schlenstedt; T. Schmidt; D. Schneider; A. Schukraft; A. Schultes; O. Schulz; M. Schunck; D. Seckel; B. Semburg; S. H. Seo; Y. Sestayo; S. Seunarine; A. Silvestri; A. Slipak; G. M. Spiczak; C. Spiering; M. Stamatikos; T. Stanev; G. Stephens; T. Stezelberger; R. G. Stokstad; S. Stoyanov; E. A. Strahler; T. Straszheim; G. W. Sullivan; Q. Swillens; I. Taboada; A. Tamburro; A. Tepe; S. Ter-Antonyan; S. Tilav; P. A. Toale; D. Tosi; D. Turčan; N. Van Eijndhoven; J. Vandenbroucke; A. Van Overloop; J. Van Santen; B. Voigt; C. Walck; T. Waldenmaier; M. Wallraff; M. Walter; C. Wendt; S. Westerhoff; N. Whitehorn; K. Wiebe; C. H. Wiebusch; G. Wikström; D. R. Williams; R. Wischnewski; H. Wissing; K. Woschnagg; C. Xu; X. W. Xu; G. Yodh; S. Yoshida; P. Zarzhitsky

doi:10.1016/j.astropartphys.2010.10.007

Search for neutrino-induced cascades with five years of AMANDA data

R. Abbasi
, Y. Abdou
, T. Abu-Zayyad
, O. Actis
, J. Adams
, J. A. Aguilar
, M. Ahlers
, K. Andeen
, J. Auffenberg
, X. Bai
, M. Baker
, S. W. Barwick
, R. Bay
, J. L. Bazo Alba
, K. Beattie
, J. J. Beatty
, S. Bechet
, J. K. Becker
, K. H. Becker
, M. L. Benabderrahmane

J. Berdermann, P. Berghaus, D. Berley, E. Bernardini, D. Bertrand, D. Z. Besson, M. Bissok, E. Blaufuss, D. J. Boersma, C. Bohm, S. Böser, O. Botner, L. Bradley, J. Braun, S. Buitink, M. Carson, D. Chirkin, B. Christy, J. Clem, F. Clevermann, S. Cohen, C. Colnard, D. F. Cowen, M. V. D'Agostino, M. Danninger, J. C. Davis, C. De Clercq, L. Demirörs, O. Depaepe, F. Descamps, P. Desiati, G. De Vries-Uiterweerd, T. Deyoung, J. C. Díaz-Vélez, J. Dreyer, J. P. Dumm, M. R. Duvoort, R. Ehrlich, J. Eisch, R. W. Ellsworth, O. Engdegrd, S. Euler, P. A. Evenson, O. Fadiran, A. R. Fazely, T. Feusels, K. Filimonov, C. Finley, M. M. Foerster, B. D. Fox, A. Franckowiak, R. Franke, T. K. Gaisser, J. Gallagher, R. Ganugapati, M. Geisler, L. Gerhardt, L. Gladstone, T. Glüsenkamp, A. Goldschmidt, J. A. Goodman, D. Grant, T. Griesel, A. Groß, S. Grullon, R. M. Gunasingha, M. Gurtner, C. Ha, A. Hallgren, F. Halzen, K. Han, K. Hanson, K. Helbing, P. Herquet, S. Hickford, G. C. Hill, K. D. Hoffman, A. Homeier, K. Hoshina, D. Hubert, W. Huelsnitz, J. P. Hülß, P. O. Hulth, K. Hultqvist, S. Hussain, R. L. Imlay, A. Ishihara, J. Jacobsen, G. S. Japaridze, H. Johansson, J. M. Joseph, K. H. Kampert, A. Kappes, T. Karg, A. Karle, J. L. Kelley, N. Kemming, P. Kenny, J. Kiryluk, F. Kislat, S. R. Klein, S. Knops, J. H. Köhne, G. Kohnen, H. Kolanoski, L. Köpke, D. J. Koskinen, M. Kowalski, T. Kowarik, M. Krasberg, T. Krings, G. Kroll, K. Kuehn, T. Kuwabara, M. Labare, S. Lafebre, K. Laihem, H. Landsman, R. Lauer, R. Lehmann, D. Lennarz, J. Lünemann, J. Madsen, P. Majumdar, R. Maruyama, K. Mase, H. S. Matis, M. Matusik, K. Meagher, M. Merck, P. Mészáros, T. Meures, E. Middell, N. Milke, J. Miller, T. Montaruli, R. Morse, S. M. Movit, R. Nahnhauer, J. W. Nam, U. Naumann, P. Nießen, D. R. Nygren, S. Odrowski, A. Olivas, M. Olivo, M. Ono, S. Panknin, L. Paul, C. Pérez De Los Heros, J. Petrovic, A. Piegsa, D. Pieloth, R. Porrata, J. Posselt, P. B. Price, M. Prikockis, G. T. Przybylski, K. Rawlins, P. Redl, E. Resconi, W. Rhode, M. Ribordy, A. Rizzo, J. P. Rodrigues, P. Roth, F. Rothmaier, C. Rott, C. Roucelle, T. Ruhe, D. Rutledge, B. Ruzybayev, D. Ryckbosch, H. G. Sander, S. Sarkar, K. Schatto, S. Schlenstedt, T. Schmidt, D. Schneider, A. Schukraft, A. Schultes, O. Schulz, M. Schunck, D. Seckel, B. Semburg, S. H. Seo, Y. Sestayo, S. Seunarine, A. Silvestri, A. Slipak, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, G. Stephens, T. Stezelberger, R. G. Stokstad, S. Stoyanov, E. A. Strahler, T. Straszheim, G. W. Sullivan, Q. Swillens, I. Taboada, A. Tamburro, A. Tepe, S. Ter-Antonyan, S. Tilav, P. A. Toale, D. Tosi, D. Turčan, N. Van Eijndhoven, J. Vandenbroucke, A. Van Overloop, J. Van Santen, B. Voigt, C. Walck, T. Waldenmaier, M. Wallraff, M. Walter, C. Wendt, S. Westerhoff, N. Whitehorn, K. Wiebe, C. H. Wiebusch, G. Wikström, D. R. Williams, R. Wischnewski, H. Wissing, K. Woschnagg, C. Xu, X. W. Xu, G. Yodh, S. Yoshida, P. Zarzhitsky

Physics and Astronomy

University of Wisconsin-Madison
Ghent University
University of Wisconsin-River Falls
German Electron Synchrotron
University of Canterbury
University of Oxford
University of Wuppertal
University of Delaware
University of California at Irvine
University of California at Berkeley
Lawrence Berkeley National Laboratory
Ohio State University
Université libre de Bruxelles
Ruhr University Bochum
University of Maryland, College Park
University of Kansas
RWTH Aachen University
Oskar Klein Centre
University of Bonn
Uppsala University
Pennsylvania State University
TU Dortmund University
Swiss Federal Institute of Technology Lausanne
Max Planck Institute for Nuclear Physics
Vrije Universiteit Brussel
Utrecht University
Clark Atlanta University
Southern University and A&M College
Humboldt University of Berlin
University of Alberta
Johannes Gutenberg University Mainz
Universite de Mons
Chiba University
Friedrich-Alexander University Erlangen-Nürnberg
University of Bari
University of Alaska Anchorage
The University of the West Indies
NASA Goddard Space Flight Center
Georgia Institute of Technology
University of Alabama

Research output: Contribution to journal › Article › peer-review

22 Scopus citations

Abstract

We report on the search for electromagnetic and hadronic showers ("cascades") produced by a diffuse flux of extraterrestrial neutrinos in the AMANDA neutrino telescope. Data for this analysis were recorded during 1001 days of detector livetime in the years 2000-2004. The observed event rates are consistent with the background expectation from atmospheric neutrinos and muons. An upper limit is derived for the diffuse flux of neutrinos of all flavors assuming a flavor ratio of ν_e:ν_μ: ν_τ = 1:1:1 at the detection site. The all-flavor flux of neutrinos with an energy spectrum Φ ∝ E^-2 is less than 5.0 × 10^-7 GeV s^-1 sr^-1 cm^-2 at a 90% C.L. Here, 90% of the simulated signal would fall within the energy range 40 TeV to 9 PeV. We discuss flux limits in the context of several specific models of extraterrestrial and prompt atmospheric neutrino production.

Original language	English
Pages (from-to)	420-430
Number of pages	11
Journal	Astroparticle Physics
Volume	34
Issue number	6
DOIs	https://doi.org/10.1016/j.astropartphys.2010.10.007
State	Published - Jan 2011

Keywords

Cascades
Neutrinos

Access to Document

10.1016/j.astropartphys.2010.10.007

Cite this

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Actis, O., Adams, J., Aguilar, J. A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S. W., Bay, R., Bazo Alba, J. L., Beattie, K., Beatty, J. J., Bechet, S., Becker, J. K., Becker, K. H., ... Zarzhitsky, P. (2011). Search for neutrino-induced cascades with five years of AMANDA data. Astroparticle Physics, 34(6), 420-430. https://doi.org/10.1016/j.astropartphys.2010.10.007

@article{f8bb8eec798047a9b6306816270febef,

title = "Search for neutrino-induced cascades with five years of AMANDA data",

abstract = "We report on the search for electromagnetic and hadronic showers ({"}cascades{"}) produced by a diffuse flux of extraterrestrial neutrinos in the AMANDA neutrino telescope. Data for this analysis were recorded during 1001 days of detector livetime in the years 2000-2004. The observed event rates are consistent with the background expectation from atmospheric neutrinos and muons. An upper limit is derived for the diffuse flux of neutrinos of all flavors assuming a flavor ratio of νe:νμ: ντ = 1:1:1 at the detection site. The all-flavor flux of neutrinos with an energy spectrum Φ ∝ E-2 is less than 5.0 {\texttimes} 10-7 GeV s-1 sr-1 cm-2 at a 90\% C.L. Here, 90\% of the simulated signal would fall within the energy range 40 TeV to 9 PeV. We discuss flux limits in the context of several specific models of extraterrestrial and prompt atmospheric neutrino production.",

keywords = "Cascades, Neutrinos",

author = "R. Abbasi and Y. Abdou and T. Abu-Zayyad and O. Actis and J. Adams and Aguilar, \{J. A.\} and M. Ahlers and K. Andeen and J. Auffenberg and X. Bai and M. Baker and Barwick, \{S. W.\} and R. Bay and \{Bazo Alba\}, \{J. L.\} and K. Beattie and Beatty, \{J. J.\} and S. Bechet and Becker, \{J. K.\} and Becker, \{K. H.\} and Benabderrahmane, \{M. L.\} and J. Berdermann and P. Berghaus and D. Berley and E. Bernardini and D. Bertrand and Besson, \{D. Z.\} and M. Bissok and E. Blaufuss and Boersma, \{D. J.\} and C. Bohm and S. B{\"o}ser and O. Botner and L. Bradley and J. Braun and S. Buitink and M. Carson and D. Chirkin and B. Christy and J. Clem and F. Clevermann and S. Cohen and C. Colnard and Cowen, \{D. F.\} and D'Agostino, \{M. V.\} and M. Danninger and Davis, \{J. C.\} and \{De Clercq\}, C. and L. Demir{\"o}rs and O. Depaepe and F. Descamps and P. Desiati and \{De Vries-Uiterweerd\}, G. and T. Deyoung and D{\'i}az-V{\'e}lez, \{J. C.\} and J. Dreyer and Dumm, \{J. P.\} and Duvoort, \{M. R.\} and R. Ehrlich and J. Eisch and Ellsworth, \{R. W.\} and O. Engdegrd and S. Euler and Evenson, \{P. A.\} and O. Fadiran and Fazely, \{A. R.\} and T. Feusels and K. Filimonov and C. Finley and Foerster, \{M. M.\} and Fox, \{B. D.\} and A. Franckowiak and R. Franke and Gaisser, \{T. K.\} and J. Gallagher and R. Ganugapati and M. Geisler and L. Gerhardt and L. Gladstone and T. Gl{\"u}senkamp and A. Goldschmidt and Goodman, \{J. A.\} and D. Grant and T. Griesel and A. Gro{\ss} and S. Grullon and Gunasingha, \{R. M.\} and M. Gurtner and C. Ha and A. Hallgren and F. Halzen and K. Han and K. Hanson and K. Helbing and P. Herquet and S. Hickford and Hill, \{G. C.\} and Hoffman, \{K. D.\} and A. Homeier and K. Hoshina and D. Hubert and W. Huelsnitz and H{\"u}l{\ss}, \{J. P.\} and Hulth, \{P. O.\} and K. Hultqvist and S. Hussain and Imlay, \{R. L.\} and A. Ishihara and J. Jacobsen and Japaridze, \{G. S.\} and H. Johansson and Joseph, \{J. M.\} and Kampert, \{K. H.\} and A. Kappes and T. Karg and A. Karle and Kelley, \{J. L.\} and N. Kemming and P. Kenny and J. Kiryluk and F. Kislat and Klein, \{S. R.\} and S. Knops and K{\"o}hne, \{J. H.\} and G. Kohnen and H. Kolanoski and L. K{\"o}pke and Koskinen, \{D. J.\} and M. Kowalski and T. Kowarik and M. Krasberg and T. Krings and G. Kroll and K. Kuehn and T. Kuwabara and M. Labare and S. Lafebre and K. Laihem and H. Landsman and R. Lauer and R. Lehmann and D. Lennarz and J. L{\"u}nemann and J. Madsen and P. Majumdar and R. Maruyama and K. Mase and Matis, \{H. S.\} and M. Matusik and K. Meagher and M. Merck and P. M{\'e}sz{\'a}ros and T. Meures and E. Middell and N. Milke and J. Miller and T. Montaruli and R. Morse and Movit, \{S. M.\} and R. Nahnhauer and Nam, \{J. W.\} and U. Naumann and P. Nie{\ss}en and Nygren, \{D. R.\} and S. Odrowski and A. Olivas and M. Olivo and M. Ono and S. Panknin and L. Paul and \{P{\'e}rez De Los Heros\}, C. and J. Petrovic and A. Piegsa and D. Pieloth and R. Porrata and J. Posselt and Price, \{P. B.\} and M. Prikockis and Przybylski, \{G. T.\} and K. Rawlins and P. Redl and E. Resconi and W. Rhode and M. Ribordy and A. Rizzo and Rodrigues, \{J. P.\} and P. Roth and F. Rothmaier and C. Rott and C. Roucelle and T. Ruhe and D. Rutledge and B. Ruzybayev and D. Ryckbosch and Sander, \{H. G.\} and S. Sarkar and K. Schatto and S. Schlenstedt and T. Schmidt and D. Schneider and A. Schukraft and A. Schultes and O. Schulz and M. Schunck and D. Seckel and B. Semburg and Seo, \{S. H.\} and Y. Sestayo and S. Seunarine and A. Silvestri and A. Slipak and Spiczak, \{G. M.\} and C. Spiering and M. Stamatikos and T. Stanev and G. Stephens and T. Stezelberger and Stokstad, \{R. G.\} and S. Stoyanov and Strahler, \{E. A.\} and T. Straszheim and Sullivan, \{G. W.\} and Q. Swillens and I. Taboada and A. Tamburro and A. Tepe and S. Ter-Antonyan and S. Tilav and Toale, \{P. A.\} and D. Tosi and D. Tur{\v c}an and \{Van Eijndhoven\}, N. and J. Vandenbroucke and \{Van Overloop\}, A. and \{Van Santen\}, J. and B. Voigt and C. Walck and T. Waldenmaier and M. Wallraff and M. Walter and C. Wendt and S. Westerhoff and N. Whitehorn and K. Wiebe and Wiebusch, \{C. H.\} and G. Wikstr{\"o}m and Williams, \{D. R.\} and R. Wischnewski and H. Wissing and K. Woschnagg and C. Xu and Xu, \{X. W.\} and G. Yodh and S. Yoshida and P. Zarzhitsky",

year = "2011",

month = jan,

doi = "10.1016/j.astropartphys.2010.10.007",

language = "English",

volume = "34",

pages = "420--430",

journal = "Astroparticle Physics",

issn = "0927-6505",

number = "6",

}

Abbasi, R, Abdou, Y, Abu-Zayyad, T, Actis, O, Adams, J, Aguilar, JA, Ahlers, M, Andeen, K, Auffenberg, J, Bai, X, Baker, M, Barwick, SW, Bay, R, Bazo Alba, JL, Beattie, K, Beatty, JJ, Bechet, S, Becker, JK, Becker, KH, Benabderrahmane, ML, Berdermann, J, Berghaus, P, Berley, D, Bernardini, E, Bertrand, D, Besson, DZ, Bissok, M, Blaufuss, E, Boersma, DJ, Bohm, C, Böser, S, Botner, O, Bradley, L, Braun, J, Buitink, S, Carson, M, Chirkin, D, Christy, B, Clem, J, Clevermann, F, Cohen, S, Colnard, C, Cowen, DF, D'Agostino, MV, Danninger, M, Davis, JC, De Clercq, C, Demirörs, L, Depaepe, O, Descamps, F, Desiati, P, De Vries-Uiterweerd, G, Deyoung, T, Díaz-Vélez, JC, Dreyer, J, Dumm, JP, Duvoort, MR, Ehrlich, R, Eisch, J, Ellsworth, RW, Engdegrd, O, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Feusels, T, Filimonov, K, Finley, C, Foerster, MM, Fox, BD, Franckowiak, A, Franke, R, Gaisser, TK, Gallagher, J, Ganugapati, R, Geisler, M, Gerhardt, L, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Goodman, JA, Grant, D, Griesel, T, Groß, A, Grullon, S, Gunasingha, RM, Gurtner, M, Ha, C, Hallgren, A, Halzen, F, Han, K, Hanson, K, Helbing, K, Herquet, P, Hickford, S, Hill, GC, Hoffman, KD, Homeier, A, Hoshina, K, Hubert, D, Huelsnitz, W, Hülß, JP, Hulth, PO, Hultqvist, K, Hussain, S, Imlay, RL, Ishihara, A, Jacobsen, J, Japaridze, GS, Johansson, H, Joseph, JM, Kampert, KH, Kappes, A, Karg, T, Karle, A, Kelley, JL, Kemming, N, Kenny, P, Kiryluk, J, Kislat, F, Klein, SR, Knops, S, Köhne, JH, Kohnen, G, Kolanoski, H, Köpke, L, Koskinen, DJ, Kowalski, M, Kowarik, T, Krasberg, M, Krings, T, Kroll, G, Kuehn, K, Kuwabara, T, Labare, M, Lafebre, S, Laihem, K, Landsman, H, Lauer, R, Lehmann, R, Lennarz, D, Lünemann, J, Madsen, J, Majumdar, P, Maruyama, R, Mase, K, Matis, HS, Matusik, M, Meagher, K, Merck, M, Mészáros, P, Meures, T, Middell, E, Milke, N, Miller, J, Montaruli, T, Morse, R, Movit, SM, Nahnhauer, R, Nam, JW, Naumann, U, Nießen, P, Nygren, DR, Odrowski, S, Olivas, A, Olivo, M, Ono, M, Panknin, S, Paul, L, Pérez De Los Heros, C, Petrovic, J, Piegsa, A, Pieloth, D, Porrata, R, Posselt, J, Price, PB, Prikockis, M, Przybylski, GT, Rawlins, K, Redl, P, Resconi, E, Rhode, W, Ribordy, M, Rizzo, A, Rodrigues, JP, Roth, P, Rothmaier, F, Rott, C, Roucelle, C, Ruhe, T, Rutledge, D, Ruzybayev, B, Ryckbosch, D, Sander, HG, Sarkar, S, Schatto, K, Schlenstedt, S, Schmidt, T, Schneider, D, Schukraft, A, Schultes, A, Schulz, O, Schunck, M, Seckel, D, Semburg, B, Seo, SH, Sestayo, Y, Seunarine, S, Silvestri, A, Slipak, A, Spiczak, GM, Spiering, C, Stamatikos, M, Stanev, T, Stephens, G, Stezelberger, T, Stokstad, RG, Stoyanov, S, Strahler, EA, Straszheim, T, Sullivan, GW, Swillens, Q, Taboada, I, Tamburro, A, Tepe, A, Ter-Antonyan, S, Tilav, S, Toale, PA, Tosi, D, Turčan, D, Van Eijndhoven, N, Vandenbroucke, J, Van Overloop, A, Van Santen, J, Voigt, B, Walck, C, Waldenmaier, T, Wallraff, M, Walter, M, Wendt, C, Westerhoff, S, Whitehorn, N, Wiebe, K, Wiebusch, CH, Wikström, G, Williams, DR, Wischnewski, R, Wissing, H, Woschnagg, K, Xu, C, Xu, XW, Yodh, G, Yoshida, S & Zarzhitsky, P 2011, 'Search for neutrino-induced cascades with five years of AMANDA data', Astroparticle Physics, vol. 34, no. 6, pp. 420-430. https://doi.org/10.1016/j.astropartphys.2010.10.007

TY - JOUR

T1 - Search for neutrino-induced cascades with five years of AMANDA data

AU - Abbasi, R.

AU - Abdou, Y.

AU - Abu-Zayyad, T.

AU - Actis, O.

AU - Adams, J.

AU - Aguilar, J. A.

AU - Ahlers, M.

AU - Andeen, K.

AU - Auffenberg, J.

AU - Bai, X.

AU - Baker, M.

AU - Barwick, S. W.

AU - Bay, R.

AU - Bazo Alba, J. L.

AU - Beattie, K.

AU - Beatty, J. J.

AU - Bechet, S.

AU - Becker, J. K.

AU - Becker, K. H.

AU - Benabderrahmane, M. L.

AU - Berdermann, J.

AU - Berghaus, P.

AU - Berley, D.

AU - Bernardini, E.

AU - Bertrand, D.

AU - Besson, D. Z.

AU - Bissok, M.

AU - Blaufuss, E.

AU - Boersma, D. J.

AU - Bohm, C.

AU - Böser, S.

AU - Botner, O.

AU - Bradley, L.

AU - Braun, J.

AU - Buitink, S.

AU - Carson, M.

AU - Chirkin, D.

AU - Christy, B.

AU - Clem, J.

AU - Clevermann, F.

AU - Cohen, S.

AU - Colnard, C.

AU - Cowen, D. F.

AU - D'Agostino, M. V.

AU - Danninger, M.

AU - Davis, J. C.

AU - De Clercq, C.

AU - Demirörs, L.

AU - Depaepe, O.

AU - Descamps, F.

AU - Desiati, P.

AU - De Vries-Uiterweerd, G.

AU - Deyoung, T.

AU - Díaz-Vélez, J. C.

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PY - 2011/1

Y1 - 2011/1

N2 - We report on the search for electromagnetic and hadronic showers ("cascades") produced by a diffuse flux of extraterrestrial neutrinos in the AMANDA neutrino telescope. Data for this analysis were recorded during 1001 days of detector livetime in the years 2000-2004. The observed event rates are consistent with the background expectation from atmospheric neutrinos and muons. An upper limit is derived for the diffuse flux of neutrinos of all flavors assuming a flavor ratio of νe:νμ: ντ = 1:1:1 at the detection site. The all-flavor flux of neutrinos with an energy spectrum Φ ∝ E-2 is less than 5.0 × 10-7 GeV s-1 sr-1 cm-2 at a 90% C.L. Here, 90% of the simulated signal would fall within the energy range 40 TeV to 9 PeV. We discuss flux limits in the context of several specific models of extraterrestrial and prompt atmospheric neutrino production.

AB - We report on the search for electromagnetic and hadronic showers ("cascades") produced by a diffuse flux of extraterrestrial neutrinos in the AMANDA neutrino telescope. Data for this analysis were recorded during 1001 days of detector livetime in the years 2000-2004. The observed event rates are consistent with the background expectation from atmospheric neutrinos and muons. An upper limit is derived for the diffuse flux of neutrinos of all flavors assuming a flavor ratio of νe:νμ: ντ = 1:1:1 at the detection site. The all-flavor flux of neutrinos with an energy spectrum Φ ∝ E-2 is less than 5.0 × 10-7 GeV s-1 sr-1 cm-2 at a 90% C.L. Here, 90% of the simulated signal would fall within the energy range 40 TeV to 9 PeV. We discuss flux limits in the context of several specific models of extraterrestrial and prompt atmospheric neutrino production.

KW - Cascades

KW - Neutrinos

UR - https://www.scopus.com/pages/publications/78650518728

U2 - 10.1016/j.astropartphys.2010.10.007

DO - 10.1016/j.astropartphys.2010.10.007

M3 - Article

AN - SCOPUS:78650518728

SN - 0927-6505

VL - 34

SP - 420

EP - 430

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 6

ER -

Search for neutrino-induced cascades with five years of AMANDA data

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