Flux limits on ultra high energy neutrinos with AMANDA-B10

M. Ackermann; J. Ahrens; H. Albrecht; D. Atlee; X. Bai; R. Bay; M. Bartelt; S. W. Barwick; T. Becka; K. H. Becker; J. K. Becker; E. Bernardini; D. Bertrand; D. J. Boersma; S. Böser; O. Botner; A. Bouchta; O. Bouhali; J. Braun; C. Burgess; T. Burgess; T. Castermans; D. Chirkin; T. Coarasa; B. Collin; J. Conrad; J. Cooley; D. F. Cowen; A. Davour; C. De Clercq; T. De Young; P. Desiati; P. Ekström; T. Feser; T. K. Gaisser; R. Ganugapati; H. Geenen; L. Gerhardt; A. Goldschmidt; A. Groß; A. Hallgren; F. Halzen; K. Hanson; D. Hardtke; R. Hardtke; T. Harenberg; T. Hauschildt; K. Helbing; M. Hellwig; P. Herquet; G. C. Hill; J. Hodges; D. Hubert; B. Hughey; P. O. Hulth; K. Hultqvist; Stephan Hundertmark; J. Jacobsen; K. H. Kampert; A. Karle; J. Kelley; M. Kestel; L. Köpke; M. Kowalski; M. Krasberg; K. Kuehn; H. Leich; M. Leuthold; J. Lundberg; J. Madsen; K. Mandli; P. Marciniewski; H. S. Matis; C. P. McParland; T. Messarius; Y. Minaeva; P. Miočinović; R. Morse; S. Movit; K. Münich; R. Nahnhauer; J. W. Nam; T. Neunhöffer; P. Niessen; D. R. Nygren; H. Ögelman; Ph Olbrechts; C. Pérez de los Heros; A. C. Pohl; R. Porrata; P. B. Price; G. T. Przybylski; K. Rawlins; E. Resconi; W. Rhode; M. Ribordy; S. Richter; J. Rodríguez Martino; D. Rutledge

doi:10.1016/j.astropartphys.2004.09.008

Flux limits on ultra high energy neutrinos with AMANDA-B10

M. Ackermann
, J. Ahrens
, H. Albrecht
, D. Atlee
, X. Bai
, R. Bay
, M. Bartelt
, S. W. Barwick
, T. Becka
, K. H. Becker
, J. K. Becker
, E. Bernardini
, D. Bertrand
, D. J. Boersma
, S. Böser
, O. Botner
, A. Bouchta
, O. Bouhali
, J. Braun
, C. Burgess

T. Burgess, T. Castermans, D. Chirkin, T. Coarasa, B. Collin, J. Conrad, J. Cooley, D. F. Cowen, A. Davour, C. De Clercq, T. De Young, P. Desiati, P. Ekström, T. Feser, T. K. Gaisser, R. Ganugapati, H. Geenen, L. Gerhardt, A. Goldschmidt, A. Groß, A. Hallgren, F. Halzen, K. Hanson, D. Hardtke, R. Hardtke, T. Harenberg, T. Hauschildt, K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, J. Hodges, D. Hubert, B. Hughey, P. O. Hulth, K. Hultqvist, Stephan Hundertmark^*, J. Jacobsen, K. H. Kampert, A. Karle, J. Kelley, M. Kestel, L. Köpke, M. Kowalski, M. Krasberg, K. Kuehn, H. Leich, M. Leuthold, J. Lundberg, J. Madsen, K. Mandli, P. Marciniewski, H. S. Matis, C. P. McParland, T. Messarius, Y. Minaeva, P. Miočinović, R. Morse, S. Movit, K. Münich, R. Nahnhauer, J. W. Nam, T. Neunhöffer, P. Niessen, D. R. Nygren, H. Ögelman, Ph Olbrechts, C. Pérez de los Heros, A. C. Pohl, R. Porrata, P. B. Price, G. T. Przybylski, K. Rawlins, E. Resconi, W. Rhode, M. Ribordy, S. Richter, J. Rodríguez Martino, D. Rutledge

^*Corresponding author for this work

German Electron Synchrotron
Johannes Gutenberg University Mainz
Pennsylvania State University
University of Delaware
University of California at Berkeley
University of Wuppertal
University of California at Irvine
Université libre de Bruxelles
Uppsala University
University of Wisconsin-Madison
Stockholm University
Universite de Mons
Vrije Universiteit Brussel
University of Maryland, College Park
Lawrence Berkeley National Laboratory
University of Wisconsin-River Falls
Linnaeus University

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

80 Citations (Scopus)

Abstract

Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of all flavors with energies above 10¹⁶eV. At these energies the Earth is opaque to neutrinos, and thus neutrino induced events are concentrated at the horizon. The background are large muon bundles from down-going atmospheric air shower events. No excess events above the background expectation are observed and a neutrino flux following E^-2, with an equal mix of all flavors, is limited to E²φ(10¹⁵eV < E < 3 × 10¹⁸eV) ≤ 0.99 × 10^-6GeV cm^-2 s^-1 sr^-1 at 90% confidence level. This is the most restrictive experimental bound placed by any neutrino detector at these energies. Bounds to specific extra-terrestrial eutrino flux predictions are also presented.

Original language	English
Pages (from-to)	339-353
Number of pages	15
Journal	Astroparticle Physics
Volume	22
Issue number	5-6
DOIs	https://doi.org/10.1016/j.astropartphys.2004.09.008
Publication status	Published - Jan 2005
Externally published	Yes

Keywords

AMANDA
Neutrino astronomy
Neutrino telescopes
UHE neutrinos

Access to Document

10.1016/j.astropartphys.2004.09.008

Cite this

Ackermann, M., Ahrens, J., Albrecht, H., Atlee, D., Bai, X., Bay, R., Bartelt, M., Barwick, S. W., Becka, T., Becker, K. H., Becker, J. K., Bernardini, E., Bertrand, D., Boersma, D. J., Böser, S., Botner, O., Bouchta, A., Bouhali, O., Braun, J., ... Rutledge, D. (2005). Flux limits on ultra high energy neutrinos with AMANDA-B10. Astroparticle Physics, 22(5-6), 339-353. https://doi.org/10.1016/j.astropartphys.2004.09.008

@article{5a08d144be37404ea5d9e394828c4b65,

title = "Flux limits on ultra high energy neutrinos with AMANDA-B10",

abstract = "Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of all flavors with energies above 1016eV. At these energies the Earth is opaque to neutrinos, and thus neutrino induced events are concentrated at the horizon. The background are large muon bundles from down-going atmospheric air shower events. No excess events above the background expectation are observed and a neutrino flux following E-2, with an equal mix of all flavors, is limited to E2φ(1015eV < E < 3 × 1018eV) ≤ 0.99 × 10-6GeV cm-2 s-1 sr-1 at 90\% confidence level. This is the most restrictive experimental bound placed by any neutrino detector at these energies. Bounds to specific extra-terrestrial eutrino flux predictions are also presented.",

keywords = "AMANDA, Neutrino astronomy, Neutrino telescopes, UHE neutrinos",

author = "M. Ackermann and J. Ahrens and H. Albrecht and D. Atlee and X. Bai and R. Bay and M. Bartelt and Barwick, \{S. W.\} and T. Becka and Becker, \{K. H.\} and Becker, \{J. K.\} and E. Bernardini and D. Bertrand and Boersma, \{D. J.\} and S. B{\"o}ser and O. Botner and A. Bouchta and O. Bouhali and J. Braun and C. Burgess and T. Burgess and T. Castermans and D. Chirkin and T. Coarasa and B. Collin and J. Conrad and J. Cooley and Cowen, \{D. F.\} and A. Davour and \{De Clercq\}, C. and \{De Young\}, T. and P. Desiati and P. Ekstr{\"o}m and T. Feser and Gaisser, \{T. K.\} and R. Ganugapati and H. Geenen and L. Gerhardt and A. Goldschmidt and A. Gro{\ss} and A. Hallgren and F. Halzen and K. Hanson and D. Hardtke and R. Hardtke and T. Harenberg and T. Hauschildt and K. Helbing and M. Hellwig and P. Herquet and Hill, \{G. C.\} and J. Hodges and D. Hubert and B. Hughey and Hulth, \{P. O.\} and K. Hultqvist and Stephan Hundertmark and J. Jacobsen and Kampert, \{K. H.\} and A. Karle and J. Kelley and M. Kestel and L. K{\"o}pke and M. Kowalski and M. Krasberg and K. Kuehn and H. Leich and M. Leuthold and J. Lundberg and J. Madsen and K. Mandli and P. Marciniewski and Matis, \{H. S.\} and McParland, \{C. P.\} and T. Messarius and Y. Minaeva and P. Mio{\v c}inovi{\'c} and R. Morse and S. Movit and K. M{\"u}nich and R. Nahnhauer and Nam, \{J. W.\} and T. Neunh{\"o}ffer and P. Niessen and Nygren, \{D. R.\} and H. {\"O}gelman and Ph Olbrechts and \{de los Heros\}, \{C. P{\'e}rez\} and Pohl, \{A. C.\} and R. Porrata and Price, \{P. B.\} and Przybylski, \{G. T.\} and K. Rawlins and E. Resconi and W. Rhode and M. Ribordy and S. Richter and Martino, \{J. Rodr{\'i}guez\} and D. Rutledge",

year = "2005",

month = jan,

doi = "10.1016/j.astropartphys.2004.09.008",

language = "English",

volume = "22",

pages = "339--353",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier B.V.",

number = "5-6",

}

Ackermann, M, Ahrens, J, Albrecht, H, Atlee, D, Bai, X, Bay, R, Bartelt, M, Barwick, SW, Becka, T, Becker, KH, Becker, JK, Bernardini, E, Bertrand, D, Boersma, DJ, Böser, S, Botner, O, Bouchta, A, Bouhali, O, Braun, J, Burgess, C, Burgess, T, Castermans, T, Chirkin, D, Coarasa, T, Collin, B, Conrad, J, Cooley, J, Cowen, DF, Davour, A, De Clercq, C, De Young, T, Desiati, P, Ekström, P, Feser, T, Gaisser, TK, Ganugapati, R, Geenen, H, Gerhardt, L, Goldschmidt, A, Groß, A, Hallgren, A, Halzen, F, Hanson, K, Hardtke, D, Hardtke, R, Harenberg, T, Hauschildt, T, Helbing, K, Hellwig, M, Herquet, P, Hill, GC, Hodges, J, Hubert, D, Hughey, B, Hulth, PO, Hultqvist, K, Hundertmark, S, Jacobsen, J, Kampert, KH, Karle, A, Kelley, J, Kestel, M, Köpke, L, Kowalski, M, Krasberg, M, Kuehn, K, Leich, H, Leuthold, M, Lundberg, J, Madsen, J, Mandli, K, Marciniewski, P, Matis, HS, McParland, CP, Messarius, T, Minaeva, Y, Miočinović, P, Morse, R, Movit, S, Münich, K, Nahnhauer, R, Nam, JW, Neunhöffer, T, Niessen, P, Nygren, DR, Ögelman, H, Olbrechts, P, de los Heros, CP, Pohl, AC, Porrata, R, Price, PB, Przybylski, GT, Rawlins, K, Resconi, E, Rhode, W, Ribordy, M, Richter, S, Martino, JR & Rutledge, D 2005, 'Flux limits on ultra high energy neutrinos with AMANDA-B10', Astroparticle Physics, vol. 22, no. 5-6, pp. 339-353. https://doi.org/10.1016/j.astropartphys.2004.09.008

TY - JOUR

T1 - Flux limits on ultra high energy neutrinos with AMANDA-B10

AU - Ackermann, M.

AU - Ahrens, J.

AU - Albrecht, H.

AU - Atlee, D.

AU - Bai, X.

AU - Bay, R.

AU - Bartelt, M.

AU - Barwick, S. W.

AU - Becka, T.

AU - Becker, K. H.

AU - Becker, J. K.

AU - Bernardini, E.

AU - Bertrand, D.

AU - Boersma, D. J.

AU - Böser, S.

AU - Botner, O.

AU - Bouchta, A.

AU - Bouhali, O.

AU - Braun, J.

AU - Burgess, C.

AU - Burgess, T.

AU - Castermans, T.

AU - Chirkin, D.

AU - Coarasa, T.

AU - Collin, B.

AU - Conrad, J.

AU - Cooley, J.

AU - Cowen, D. F.

AU - Davour, A.

AU - De Clercq, C.

AU - De Young, T.

AU - Desiati, P.

AU - Ekström, P.

AU - Feser, T.

AU - Gaisser, T. K.

AU - Ganugapati, R.

AU - Geenen, H.

AU - Gerhardt, L.

AU - Goldschmidt, A.

AU - Groß, A.

AU - Hallgren, A.

AU - Halzen, F.

AU - Hanson, K.

AU - Hardtke, D.

AU - Hardtke, R.

AU - Harenberg, T.

AU - Hauschildt, T.

AU - Helbing, K.

AU - Hellwig, M.

AU - Herquet, P.

AU - Hill, G. C.

AU - Hodges, J.

AU - Hubert, D.

AU - Hughey, B.

AU - Hulth, P. O.

AU - Hultqvist, K.

AU - Hundertmark, Stephan

AU - Jacobsen, J.

AU - Kampert, K. H.

AU - Karle, A.

AU - Kelley, J.

AU - Kestel, M.

AU - Köpke, L.

AU - Kowalski, M.

AU - Krasberg, M.

AU - Kuehn, K.

AU - Leich, H.

AU - Leuthold, M.

AU - Lundberg, J.

AU - Madsen, J.

AU - Mandli, K.

AU - Marciniewski, P.

AU - Matis, H. S.

AU - McParland, C. P.

AU - Messarius, T.

AU - Minaeva, Y.

AU - Miočinović, P.

AU - Morse, R.

AU - Movit, S.

AU - Münich, K.

AU - Nahnhauer, R.

AU - Nam, J. W.

AU - Neunhöffer, T.

AU - Niessen, P.

AU - Nygren, D. R.

AU - Ögelman, H.

AU - Olbrechts, Ph

AU - de los Heros, C. Pérez

AU - Pohl, A. C.

AU - Porrata, R.

AU - Price, P. B.

AU - Przybylski, G. T.

AU - Rawlins, K.

AU - Resconi, E.

AU - Rhode, W.

AU - Ribordy, M.

AU - Richter, S.

AU - Martino, J. Rodríguez

AU - Rutledge, D.

PY - 2005/1

Y1 - 2005/1

N2 - Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of all flavors with energies above 1016eV. At these energies the Earth is opaque to neutrinos, and thus neutrino induced events are concentrated at the horizon. The background are large muon bundles from down-going atmospheric air shower events. No excess events above the background expectation are observed and a neutrino flux following E-2, with an equal mix of all flavors, is limited to E2φ(1015eV < E < 3 × 1018eV) ≤ 0.99 × 10-6GeV cm-2 s-1 sr-1 at 90% confidence level. This is the most restrictive experimental bound placed by any neutrino detector at these energies. Bounds to specific extra-terrestrial eutrino flux predictions are also presented.

AB - Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of all flavors with energies above 1016eV. At these energies the Earth is opaque to neutrinos, and thus neutrino induced events are concentrated at the horizon. The background are large muon bundles from down-going atmospheric air shower events. No excess events above the background expectation are observed and a neutrino flux following E-2, with an equal mix of all flavors, is limited to E2φ(1015eV < E < 3 × 1018eV) ≤ 0.99 × 10-6GeV cm-2 s-1 sr-1 at 90% confidence level. This is the most restrictive experimental bound placed by any neutrino detector at these energies. Bounds to specific extra-terrestrial eutrino flux predictions are also presented.

KW - AMANDA

KW - Neutrino astronomy

KW - Neutrino telescopes

KW - UHE neutrinos

UR - https://www.scopus.com/pages/publications/19944430055

U2 - 10.1016/j.astropartphys.2004.09.008

DO - 10.1016/j.astropartphys.2004.09.008

M3 - Article

AN - SCOPUS:19944430055

SN - 0927-6505

VL - 22

SP - 339

EP - 353

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 5-6

ER -

Flux limits on ultra high energy neutrinos with AMANDA-B10

Abstract

Keywords

Access to Document

Other files and links

Fingerprint

Cite this