Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos

J. Ahrens; J. N. Bahcall; X. Bai; R. C. Bay; T. Becka; K. H. Becker; D. Berley; E. Bernardini; D. Bertrand; D. Z. Besson; A. Biron; E. Blaufuss; D. J. Boersma; S. Böser; C. Bohm; O. Botner; A. Bouchta; O. Bouhali; T. Burgess; W. Carithers; T. Castermans; J. Cavin; W. Chinowsky; D. Chirkin; B. Collin; J. Conrad; J. Cooley; D. F. Cowen; A. Davour; C. de Clercq; T. DeYoung; P. Desiati; R. Ehrlich; R. W. Ellsworth; P. A. Evenson; A. R. Fazely; T. Feser; T. K. Gaisser; J. Gallagher; R. Ganugapati; H. Geenen; A. Goldschmidt; J. A. Goodman; R. M. Gunasingha; A. Hallgren; F. Halzen; K. Hanson; R. Hardtke; T. Hauschildt; D. Hays; K. Helbing; M. Hellwig; P. Herquet; G. C. Hill; D. Hubert; B. Hughey; P. O. Hulth; K. Hultqvist; S. Hundertmark; J. Jacobsen; G. S. Japaridze; A. Jones; A. Karle; H. Kawai; M. Kestel; N. Kitamura; R. Koch; L. Köpke; M. Kowalski; J. I. Lamoureux; H. Leich; M. Leuthold; I. Liubarsky; J. Madsen; H. S. Matis; C. P. McParland; T. Messarius; P. Mészáros; Y. Minaeva; R. H. Minor; P. Miočinović; H. Miyamoto; R. Morse; R. Nahnhauer; T. Neunhöffer; P. Niessen; D. R. Nygren; H. Ögelman; P. Olbrechts; S. Patton; R. Paulos; C. Pérez de los Heros; A. C. Pohl; J. Pretz; P. B. Price; G. T. Przybylski; K. Rawlins; S. Razzaque; E. Resconi; W. Rhode; M. Ribordy; S. Richter; H. G. Sander; K. Schinarakis; S. Schlenstedt; T. Schmidt; D. Schneider; R. Schwarz; D. Seckel; A. J. Smith; M. Solarz; G. M. Spiczak; C. Spiering; M. Stamatikos; T. Stanev; D. Steele; P. Steffen; T. Stezelberger; R. G. Stokstad; K. H. Sulanke; G. W. Sullivan; T. J. Sumner; I. Taboada; S. Tilav; N. van Eijndhoven; W. Wagner; C. Walck; R. R. Wang; C. H. Wiebusch; C. Wiedemann; R. Wischnewski; H. Wissing; K. Woschnagg; S. Yoshida

doi:10.1016/j.astropartphys.2003.09.003

Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos

J. Ahrens
, J. N. Bahcall
, X. Bai
, R. C. Bay
, T. Becka
, K. H. Becker
, D. Berley
, E. Bernardini
, D. Bertrand
, D. Z. Besson
, A. Biron
, E. Blaufuss
, D. J. Boersma
, S. Böser
, C. Bohm
, O. Botner
, A. Bouchta
, O. Bouhali
, T. Burgess
, W. Carithers

T. Castermans, J. Cavin, W. Chinowsky, D. Chirkin, B. Collin, J. Conrad, J. Cooley, D. F. Cowen, A. Davour, C. de Clercq, T. DeYoung, P. Desiati, R. Ehrlich, R. W. Ellsworth, P. A. Evenson, A. R. Fazely, T. Feser, T. K. Gaisser, J. Gallagher, R. Ganugapati, H. Geenen, A. Goldschmidt, J. A. Goodman, R. M. Gunasingha, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Hauschildt, D. Hays, K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, D. Hubert, B. Hughey, P. O. Hulth, K. Hultqvist, S. Hundertmark, J. Jacobsen, G. S. Japaridze, A. Jones, A. Karle, H. Kawai, M. Kestel, N. Kitamura, R. Koch, L. Köpke, M. Kowalski, J. I. Lamoureux, H. Leich, M. Leuthold, I. Liubarsky, J. Madsen, H. S. Matis, C. P. McParland, T. Messarius, P. Mészáros, Y. Minaeva, R. H. Minor, P. Miočinović, H. Miyamoto, R. Morse, R. Nahnhauer, T. Neunhöffer, P. Niessen, D. R. Nygren, H. Ögelman, P. Olbrechts, S. Patton, R. Paulos, C. Pérez de los Heros, A. C. Pohl, J. Pretz, P. B. Price, G. T. Przybylski, K. Rawlins, S. Razzaque, E. Resconi, W. Rhode, M. Ribordy, S. Richter, H. G. Sander, K. Schinarakis, S. Schlenstedt, T. Schmidt, D. Schneider, R. Schwarz, D. Seckel, A. J. Smith, M. Solarz, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, D. Steele, P. Steffen, T. Stezelberger, R. G. Stokstad, K. H. Sulanke, G. W. Sullivan, T. J. Sumner, I. Taboada, S. Tilav, N. van Eijndhoven, W. Wagner, C. Walck, R. R. Wang, C. H. Wiebusch, C. Wiedemann, R. Wischnewski, H. Wissing, K. Woschnagg, S. Yoshida

Johannes Gutenberg University Mainz
Institute for Advanced Studies
University of Delaware
University of California at Berkeley
University of Wuppertal
University of Maryland, College Park
German Electron Synchrotron
Université libre de Bruxelles
University of Kansas
Stockholm University
Uppsala University
Lawrence Berkeley National Laboratory
Universite de Mons
University of Wisconsin-Madison
Pennsylvania State University
Vrije Universiteit Brussel
George Mason University
Southern University and A&M College
Clark Atlanta University
Chiba University
Imperial College London
University of Wisconsin-River Falls
Universidad Simón Bolívar
Utrecht University

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

407 Citations (Scopus)

Abstract

We present results of a Monte Carlo study of the sensitivity of the planned IceCube detector to predicted fluxes of muon neutrinos at TeV to PeV energies. A complete simulation of the detector and data analysis is used to study the detector's capability to search for muon neutrinos from potential sources such as active galaxies and gamma-ray bursts (GRBs). We study the effective area and the angular resolution of the detector as a function of muon energy and angle of incidence. We present detailed calculations of the sensitivity of the detector to both diffuse and pointlike neutrino fluxes, including an assessment of the sensitivity to neutrinos detected in coincidence with GRB observations. After three years of data taking, IceCube will be able to detect a point-source flux of E_ν²× dN_ν/dE_ν=7×10^-9 cm^-2s^-1 GeV at a 5σ significance, or, in the absence of a signal, place a 90% c.l. limit at a level of E_ν²×dN_ν/dE_ν= 2×10^-9 cm^-2 s^-1 GeV. A diffuse E^-2 flux would be detectable at a minimum strength of E_ν²×dN_ν/dE_ν =10^-8 cm^-2-1 sr^-1 GeV. A GRB model following the formulation of Waxman and Bahcall would result in a 5σ effect after the observation of 200 bursts in coincidence with satellite observations of the gamma rays.

Original language	English
Pages (from-to)	507-532
Number of pages	26
Journal	Astroparticle Physics
Volume	20
Issue number	5
DOIs	https://doi.org/10.1016/j.astropartphys.2003.09.003
Publication status	Published - Feb 2004
Externally published	Yes

Keywords

IceCube
Neutrino astronomy
Neutrino telescope

Access to Document

10.1016/j.astropartphys.2003.09.003

Cite this

Ahrens, J., Bahcall, J. N., Bai, X., Bay, R. C., Becka, T., Becker, K. H., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Biron, A., Blaufuss, E., Boersma, D. J., Böser, S., Bohm, C., Botner, O., Bouchta, A., Bouhali, O., Burgess, T., ... Yoshida, S. (2004). Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos. Astroparticle Physics, 20(5), 507-532. https://doi.org/10.1016/j.astropartphys.2003.09.003

@article{bab51d5d4157474fa9817d53c188b9c0,

title = "Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos",

abstract = "We present results of a Monte Carlo study of the sensitivity of the planned IceCube detector to predicted fluxes of muon neutrinos at TeV to PeV energies. A complete simulation of the detector and data analysis is used to study the detector's capability to search for muon neutrinos from potential sources such as active galaxies and gamma-ray bursts (GRBs). We study the effective area and the angular resolution of the detector as a function of muon energy and angle of incidence. We present detailed calculations of the sensitivity of the detector to both diffuse and pointlike neutrino fluxes, including an assessment of the sensitivity to neutrinos detected in coincidence with GRB observations. After three years of data taking, IceCube will be able to detect a point-source flux of Eν2× dNν/dEν=7×10-9 cm-2s-1 GeV at a 5σ significance, or, in the absence of a signal, place a 90\% c.l. limit at a level of Eν2×dNν/dEν= 2×10-9 cm-2 s-1 GeV. A diffuse E-2 flux would be detectable at a minimum strength of Eν2×dNν/dEν =10-8 cm-2-1 sr-1 GeV. A GRB model following the formulation of Waxman and Bahcall would result in a 5σ effect after the observation of 200 bursts in coincidence with satellite observations of the gamma rays.",

keywords = "IceCube, Neutrino astronomy, Neutrino telescope",

author = "J. Ahrens and Bahcall, \{J. N.\} and X. Bai and Bay, \{R. C.\} and T. Becka and Becker, \{K. H.\} and D. Berley and E. Bernardini and D. Bertrand and Besson, \{D. Z.\} and A. Biron and E. Blaufuss and Boersma, \{D. J.\} and S. B{\"o}ser and C. Bohm and O. Botner and A. Bouchta and O. Bouhali and T. Burgess and W. Carithers and T. Castermans and J. Cavin and W. Chinowsky and D. Chirkin and B. Collin and J. Conrad and J. Cooley and Cowen, \{D. F.\} and A. Davour and \{de Clercq\}, C. and T. DeYoung and P. Desiati and R. Ehrlich and Ellsworth, \{R. W.\} and Evenson, \{P. A.\} and Fazely, \{A. R.\} and T. Feser and Gaisser, \{T. K.\} and J. Gallagher and R. Ganugapati and H. Geenen and A. Goldschmidt and Goodman, \{J. A.\} and Gunasingha, \{R. M.\} and A. Hallgren and F. Halzen and K. Hanson and R. Hardtke and T. Hauschildt and D. Hays and K. Helbing and M. Hellwig and P. Herquet and Hill, \{G. C.\} and D. Hubert and B. Hughey and Hulth, \{P. O.\} and K. Hultqvist and S. Hundertmark and J. Jacobsen and Japaridze, \{G. S.\} and A. Jones and A. Karle and H. Kawai and M. Kestel and N. Kitamura and R. Koch and L. K{\"o}pke and M. Kowalski and Lamoureux, \{J. I.\} and H. Leich and M. Leuthold and I. Liubarsky and J. Madsen and Matis, \{H. S.\} and McParland, \{C. P.\} and T. Messarius and P. M{\'e}sz{\'a}ros and Y. Minaeva and Minor, \{R. H.\} and P. Mio{\v c}inovi{\'c} and H. Miyamoto and R. Morse and R. Nahnhauer and T. Neunh{\"o}ffer and P. Niessen and Nygren, \{D. R.\} and H. {\"O}gelman and P. Olbrechts and S. Patton and R. Paulos and \{P{\'e}rez de los Heros\}, C. and Pohl, \{A. C.\} and J. Pretz and Price, \{P. B.\} and Przybylski, \{G. T.\} and K. Rawlins and S. Razzaque and E. Resconi and W. Rhode and M. Ribordy and S. Richter and Sander, \{H. G.\} and K. Schinarakis and S. Schlenstedt and T. Schmidt and D. Schneider and R. Schwarz and D. Seckel and Smith, \{A. J.\} and M. Solarz and Spiczak, \{G. M.\} and C. Spiering and M. Stamatikos and T. Stanev and D. Steele and P. Steffen and T. Stezelberger and Stokstad, \{R. G.\} and Sulanke, \{K. H.\} and Sullivan, \{G. W.\} and Sumner, \{T. J.\} and I. Taboada and S. Tilav and \{van Eijndhoven\}, N. and W. Wagner and C. Walck and Wang, \{R. R.\} and Wiebusch, \{C. H.\} and C. Wiedemann and R. Wischnewski and H. Wissing and K. Woschnagg and S. Yoshida",

year = "2004",

month = feb,

doi = "10.1016/j.astropartphys.2003.09.003",

language = "English",

volume = "20",

pages = "507--532",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier B.V.",

number = "5",

}

Ahrens, J, Bahcall, JN, Bai, X, Bay, RC, Becka, T, Becker, KH, Berley, D, Bernardini, E, Bertrand, D, Besson, DZ, Biron, A, Blaufuss, E, Boersma, DJ, Böser, S, Bohm, C, Botner, O, Bouchta, A, Bouhali, O, Burgess, T, Carithers, W, Castermans, T, Cavin, J, Chinowsky, W, Chirkin, D, Collin, B, Conrad, J, Cooley, J, Cowen, DF, Davour, A, de Clercq, C, DeYoung, T, Desiati, P, Ehrlich, R, Ellsworth, RW, Evenson, PA, Fazely, AR, Feser, T, Gaisser, TK, Gallagher, J, Ganugapati, R, Geenen, H, Goldschmidt, A, Goodman, JA, Gunasingha, RM, Hallgren, A, Halzen, F, Hanson, K, Hardtke, R, Hauschildt, T, Hays, D, Helbing, K, Hellwig, M, Herquet, P, Hill, GC, Hubert, D, Hughey, B, Hulth, PO, Hultqvist, K, Hundertmark, S, Jacobsen, J, Japaridze, GS, Jones, A, Karle, A, Kawai, H, Kestel, M, Kitamura, N, Koch, R, Köpke, L, Kowalski, M, Lamoureux, JI, Leich, H, Leuthold, M, Liubarsky, I, Madsen, J, Matis, HS, McParland, CP, Messarius, T, Mészáros, P, Minaeva, Y, Minor, RH, Miočinović, P, Miyamoto, H, Morse, R, Nahnhauer, R, Neunhöffer, T, Niessen, P, Nygren, DR, Ögelman, H, Olbrechts, P, Patton, S, Paulos, R, Pérez de los Heros, C, Pohl, AC, Pretz, J, Price, PB, Przybylski, GT, Rawlins, K, Razzaque, S, Resconi, E, Rhode, W, Ribordy, M, Richter, S, Sander, HG, Schinarakis, K, Schlenstedt, S, Schmidt, T, Schneider, D, Schwarz, R, Seckel, D, Smith, AJ, Solarz, M, Spiczak, GM, Spiering, C, Stamatikos, M, Stanev, T, Steele, D, Steffen, P, Stezelberger, T, Stokstad, RG, Sulanke, KH, Sullivan, GW, Sumner, TJ, Taboada, I, Tilav, S, van Eijndhoven, N, Wagner, W, Walck, C, Wang, RR, Wiebusch, CH, Wiedemann, C, Wischnewski, R, Wissing, H, Woschnagg, K & Yoshida, S 2004, 'Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos', Astroparticle Physics, vol. 20, no. 5, pp. 507-532. https://doi.org/10.1016/j.astropartphys.2003.09.003

TY - JOUR

T1 - Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos

AU - Ahrens, J.

AU - Bahcall, J. N.

AU - Bai, X.

AU - Bay, R. C.

AU - Becka, T.

AU - Becker, K. H.

AU - Berley, D.

AU - Bernardini, E.

AU - Bertrand, D.

AU - Besson, D. Z.

AU - Biron, A.

AU - Blaufuss, E.

AU - Boersma, D. J.

AU - Böser, S.

AU - Bohm, C.

AU - Botner, O.

AU - Bouchta, A.

AU - Bouhali, O.

AU - Burgess, T.

AU - Carithers, W.

AU - Castermans, T.

AU - Cavin, J.

AU - Chinowsky, W.

AU - Chirkin, D.

AU - Collin, B.

AU - Conrad, J.

AU - Cooley, J.

AU - Cowen, D. F.

AU - Davour, A.

AU - de Clercq, C.

AU - DeYoung, T.

AU - Desiati, P.

AU - Ehrlich, R.

AU - Ellsworth, R. W.

AU - Evenson, P. A.

AU - Fazely, A. R.

AU - Feser, T.

AU - Gaisser, T. K.

AU - Gallagher, J.

AU - Ganugapati, R.

AU - Geenen, H.

AU - Goldschmidt, A.

AU - Goodman, J. A.

AU - Gunasingha, R. M.

AU - Hallgren, A.

AU - Halzen, F.

AU - Hanson, K.

AU - Hardtke, R.

AU - Hauschildt, T.

AU - Hays, D.

AU - Helbing, K.

AU - Hellwig, M.

AU - Herquet, P.

AU - Hill, G. C.

AU - Hubert, D.

AU - Hughey, B.

AU - Hulth, P. O.

AU - Hultqvist, K.

AU - Hundertmark, S.

AU - Jacobsen, J.

AU - Japaridze, G. S.

AU - Jones, A.

AU - Karle, A.

AU - Kawai, H.

AU - Kestel, M.

AU - Kitamura, N.

AU - Koch, R.

AU - Köpke, L.

AU - Kowalski, M.

AU - Lamoureux, J. I.

AU - Leich, H.

AU - Leuthold, M.

AU - Liubarsky, I.

AU - Madsen, J.

AU - Matis, H. S.

AU - McParland, C. P.

AU - Messarius, T.

AU - Mészáros, P.

AU - Minaeva, Y.

AU - Minor, R. H.

AU - Miočinović, P.

AU - Miyamoto, H.

AU - Morse, R.

AU - Nahnhauer, R.

AU - Neunhöffer, T.

AU - Niessen, P.

AU - Nygren, D. R.

AU - Ögelman, H.

AU - Olbrechts, P.

AU - Patton, S.

AU - Paulos, R.

AU - Pérez de los Heros, C.

AU - Pohl, A. C.

AU - Pretz, J.

AU - Price, P. B.

AU - Przybylski, G. T.

AU - Rawlins, K.

AU - Razzaque, S.

AU - Resconi, E.

AU - Rhode, W.

AU - Ribordy, M.

AU - Richter, S.

AU - Sander, H. G.

AU - Schinarakis, K.

AU - Schlenstedt, S.

AU - Schmidt, T.

AU - Schneider, D.

AU - Schwarz, R.

AU - Seckel, D.

AU - Smith, A. J.

AU - Solarz, M.

AU - Spiczak, G. M.

AU - Spiering, C.

AU - Stamatikos, M.

AU - Stanev, T.

AU - Steele, D.

AU - Steffen, P.

AU - Stezelberger, T.

AU - Stokstad, R. G.

AU - Sulanke, K. H.

AU - Sullivan, G. W.

AU - Sumner, T. J.

AU - Taboada, I.

AU - Tilav, S.

AU - van Eijndhoven, N.

AU - Wagner, W.

AU - Walck, C.

AU - Wang, R. R.

AU - Wiebusch, C. H.

AU - Wiedemann, C.

AU - Wischnewski, R.

AU - Wissing, H.

AU - Woschnagg, K.

AU - Yoshida, S.

PY - 2004/2

Y1 - 2004/2

N2 - We present results of a Monte Carlo study of the sensitivity of the planned IceCube detector to predicted fluxes of muon neutrinos at TeV to PeV energies. A complete simulation of the detector and data analysis is used to study the detector's capability to search for muon neutrinos from potential sources such as active galaxies and gamma-ray bursts (GRBs). We study the effective area and the angular resolution of the detector as a function of muon energy and angle of incidence. We present detailed calculations of the sensitivity of the detector to both diffuse and pointlike neutrino fluxes, including an assessment of the sensitivity to neutrinos detected in coincidence with GRB observations. After three years of data taking, IceCube will be able to detect a point-source flux of Eν2× dNν/dEν=7×10-9 cm-2s-1 GeV at a 5σ significance, or, in the absence of a signal, place a 90% c.l. limit at a level of Eν2×dNν/dEν= 2×10-9 cm-2 s-1 GeV. A diffuse E-2 flux would be detectable at a minimum strength of Eν2×dNν/dEν =10-8 cm-2-1 sr-1 GeV. A GRB model following the formulation of Waxman and Bahcall would result in a 5σ effect after the observation of 200 bursts in coincidence with satellite observations of the gamma rays.

AB - We present results of a Monte Carlo study of the sensitivity of the planned IceCube detector to predicted fluxes of muon neutrinos at TeV to PeV energies. A complete simulation of the detector and data analysis is used to study the detector's capability to search for muon neutrinos from potential sources such as active galaxies and gamma-ray bursts (GRBs). We study the effective area and the angular resolution of the detector as a function of muon energy and angle of incidence. We present detailed calculations of the sensitivity of the detector to both diffuse and pointlike neutrino fluxes, including an assessment of the sensitivity to neutrinos detected in coincidence with GRB observations. After three years of data taking, IceCube will be able to detect a point-source flux of Eν2× dNν/dEν=7×10-9 cm-2s-1 GeV at a 5σ significance, or, in the absence of a signal, place a 90% c.l. limit at a level of Eν2×dNν/dEν= 2×10-9 cm-2 s-1 GeV. A diffuse E-2 flux would be detectable at a minimum strength of Eν2×dNν/dEν =10-8 cm-2-1 sr-1 GeV. A GRB model following the formulation of Waxman and Bahcall would result in a 5σ effect after the observation of 200 bursts in coincidence with satellite observations of the gamma rays.

KW - IceCube

KW - Neutrino astronomy

KW - Neutrino telescope

UR - https://www.scopus.com/pages/publications/1642503175

U2 - 10.1016/j.astropartphys.2003.09.003

DO - 10.1016/j.astropartphys.2003.09.003

M3 - Article

AN - SCOPUS:1642503175

SN - 0927-6505

VL - 20

SP - 507

EP - 532

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 5

ER -

Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos

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