Preliminary Design Document

By Section | Whole Paper | PDF (233 pages, ~6.62mb)

References

• [1] M. Nagano et al. J. Phys. G10 (1984) 1295.
• [2] Yu. A. Fomin et al., Proc. 22nd Int. Cosmic Ray Conf. (Dublin) vol. 2 (1991) 85.
• [3] M. Takeda et al., Phys. Rev. Lett. 81 (1998) 1163.
• [4] M.A. Lawrence, R.J.O. Reid & A.A. Watson, J. Phys. G17 (1991) 733.
• [5] M.I. Pravdin et al., Proc. 26th Int. Cosmic Ray Conf. (Salt Lake City, 1999) vol. 3, p. 292.
• [6] D.J. Bird et al., Astrophys. J. 424 (1994) 491.
• [7] D.J. Bird et al., Phys. Rev. Letters 71 (1993) 3401.
• [8] E. Waxman & J. Bahcall, Phys. Rev. D 59 (1999) 023002.
• [9] J. Bahcall & E. Waxman, Phys. Rev. D 64 (2001) 023002.
• [10] G.R. Farrar & T. Piran, Phys. Rev. Letters 84 (2000) 3527.
• [11] K. Griesen, Phys. Rev. Lett. 16 (1966) 748; G.T. Zatsepin and V.A. Kuzmin, JETPh Lett. 4 (1966) 78.
• [12] A. Achterberg in High Energy Gamma-Ray Astronomy, (A.I.P. Conf. Proc. 558, ed. Felix A. Aharonian & Heinz J. Völk, γ2000) 392.
• [13] J. Bednarz & M. Ostrowski, Phys. Rev. Letters 80 (1998) 3911.
• [14] J.G. Kirk, A.W. Guthmann, Y.A. Gallant & A. Achterberg, Ap.J. 542 (2000) 235.
• [15] T. K. Gaisser, in Observing Ultra-high energy Cosmic Rays from Space and Earth (A.I.P. Conf. Proc. 566, ed. Humberto Salazar, Luis Villaseñor & Arnulfo Zepeda, Metepec, Puebla, Mexico, August 9-12, 2000), p. 238.
• [16] R. Gandhi, C. Quigg, M.H. Reno & I. Sarcevic, Astropart. Phys. 5 (1996) 81.
• [17] T.K. Gaisser, astro-ph/9707283.
• [18] Mannheim, Protheroe & Rachen, astro-ph/9812398; J.P. Rachen, R.J. Protheroe & K. Mannheim, astro-ph/9908031.
• [19] J. Learned & K. Mannheim, Ann. Revs. Nuclear and Particle Physics.
• [20] C. Schuster, M. Pohl & R. Schlickeiser, submitted to Astronomy and Astrophysics.
• [21] M. Pohl & R. Schlickeiser, Astron. & Astrophys. 354 (2000) 395.
• [22] F.A. Aharonian et al., Astron. Astrophys. 349 (1999) 11.
• [23] F.W. Samuelson et al., Ap.J. 501 (1998) L17.
• [24] A. Djannati-Atai et al. Astron. Astrophys. 350 (1999) 17.
• [25] Eli Waxman & John Bahcall, Phys. Rev. Letters 78 (1997) 2292.
• [26] J. Rachen & P. Mészáros, Phys. Rev. D58 (1998) 123005.
• [27] P. Mészáros & E. Waxman, astro-ph/0103275.
• [28] A.K. Konopelko, J.G. Kirk, F.W. Stecker & A. Mastichiadis, Ap.J. 518 (1999) L13.
• [29] W. Bednarek & R.J. Protheroe, Phys. Rev. Letters 79 (1997) 2616.
• [30] R.J. Protheroe and T. Stanev, Phys. Rev. Lett. 77, 3708 (1996) and Erratum 78, 3420 (1997).
• [31] G. Gelmini and A. Kusenko, Phys. Rev. Lett. 84, 1378 (2000).
• [32] M. Birkel and S. Sarkar, Astropart. Phys. 9, 297 (1998).
• [33] T. Weiler, Astropart. Phys. 11, 303 (1999); D. Fargion, B. Mele and A. Salis, Astrophys. J. 517, 725 (1999).
• [34] D. Cline and F.W. Stecker, contributed to OWL/AW Neutrino Workshop on Observing Ultrahigh Energy Neutrinos, Los Angeles, California, Nov. 1999, astro-ph/0003459.
• [35] V. Berezinsky, M. Kachelreiß and A. Vilenkin, Phys. Rev. Lett. 79, 4302 (1997).
• [36] J. Alvarez-Muñiz and F. Halzen, Phys. Rev. D 63, 037302 (2001).
• [37] F.W. Stecker et al., Phys. Rev. Lett., 66, 2697 (1991).
• [38] J. Alvarez-Muñiz and F. Halzen, First International Workshop on Radio Detection of High-Energy Particles (RADHEP 2000), Los Angeles, California, astro-ph/0102106
• [39] Super-Kamiokande Collaboration, Y. Fukuda et al., Phys. Rev. Lett. 81 (1998) 1562.
• [40] Sudbury Neutrino Observatory (SNO) Collaboration, Q.R. Ahmad et al., submitted to Phys. Rev. Lett. (nucl-ex/0106015).
• [41] J.G. Learned and S. Pakvasa, Astrop. Phys. 3 (1995) pp 267-274.
• [42] F. Halzen & D. Saltzberg, Phys. Rev. Letters 81 (1998) 4305.
• [43] H. Athar, G. Parente & E. Zas, Phys. Rev. D62 (2000) 093010.
• [44] A.P. Szabo & R.J. Protheroe, Astropart. Phys. 2 (1994) 375.
• [45] J. Edsjo, WIMP searches with IceCube, Amanda Internal report, Jan.7, 2000.
• [46] J. Bahcall and P. Meszaros, hep-ph/0004019.
• [47] AMANDA supernova search paper, A. Bouchta et al.
• [48] see K.Scholberg, Nucl.Phys.Proc.Suppl. 91 (2000) 331-337.
• [49] A. Loeb and E. Waxman, astro-ph/0007049.
• [50] T.K. Gaisser, F. Halzen, T. Stanev, Phys. Rep. 258 (1995) 173.
• [51] F.W. Stecker, O.C. de Jager, Astron. Astrophys. 334, L85 (1998).
• [52] E.N. Parker, Astrophys. J. 160 (1970) 383.
• [53] E. Andrés et al. (AMANDA Collaboration), Astropart. Phys. 13 (2000) 1–20.
• [54] E. Andrés et al. (The AMANDA Collaboration), Nature 410 (2001) 441.
• [55] Bai et al., Proceedings of 27th Int. Conf. on Cosmic Rays, Hamburg 2001.
• [56] T. R. DeYoung, Observation of atmospheric neutrinos with AMANDA, Dissertation, University of Wisconsin-Madison, April 2001
• [57] Ch. Wiebusch, Muon Reconstruction with AMANDA, DESY-PROC 1999-01, July 1999
• [58] G. C. Hill, proceedings of the XXXVIth Recontres de Moriond, Electroweak Interactions and Unified Theories, March 2001.
• [59] V. Agrawal, T. Gaisser, P. Lipari, and T. Stanev, Phys. Rev. D53 (1996) 1314.
• [60] Nellen, L., Mannheim, K., & Biermann, P.L. Neutrino Production through Hadronic Cascades in AGN Accretion Disks. Phys. Rev. D47, 5270-5274 (1993).
• [61] W. Bednarek and R. J. Protheroe, Mon. Not. Roy. Astro. Soc. 287(1997) 560.
• [62] S. Colafrancesco, and P. Blasi, Astropart. Physics 9 (1998) 219
• [63] Stecker, F.W. & Salamon, M.H. High-Energy Neutrinos from Quasars. Space Sci. Rev. 75, 341-355 (1996).
• [64] T.K. Gaisser, R.J. Protheroe, and T. Stanev, Ap. J. 492 (1998) 219.
• [65] E. Andrés et al. (The AMANDA Collaboration), Proceedings of Neutrino 2000 Conference, Sudbury, e-print: astro-ph/0009242.
• [66] Bolesta J.W. et al., Proc. 25-th ICRC, Durban South Africa, 7:29 (1997)
• [67] Porrata et al., Proc. 25-th ICRC, Durban South Africa, 7:9 (1997)
• [68] Rhode W. et al. (Frejus-Coll.), AstroPart. Phys. 4:217 (1996)
• [69] Protheroe RJ, astro-ph/9809144 (1998)
• [70] C.Spiering, Nucl.Phys.Proc.Suppl. 91 (2000) 445-452.
• [71] Balkanov,V.A. et al., Astropart. Phys. 14, 61-67 (2000). See also http://www-zeuthen.desy.de/baikal/baikalhome.html.
• [72] Nucl.Phys.Proc.Suppl. 87 (2000) 436-438. See also http://antares.in2p3.fr/.
• [73] G.V.Domogatsky (for BAIKAL Collaboration), Nucl. Phys. Proc. Suppl. 91 (2000) 438-444.
• [74] See http://www.nestor.org.gr/.
• [75] Zh.-A. Dzhilkibaev (for BAIKAL Collaboration), these proceedings, Int. Conf. on Neutrino Telesopes, Venice, 2001, astro-ph/0105269.
• [76] Waxman, E. & Bahcall, J.N. High-Energy Neutrinos from Cosmological Gamma Ray Burst Fireballs. Phys. Rev. Lett. 78, 2292-2295 (1997).
• [77] Waxman, E. & Bahcall, J.N. High Energy Neutrinos from Astrophysical Sources: An Upper Bound. Phys. Rev. D59, 023002 (1999).
• [78] E. Waxman and J.N. Bahcall, Phys. Rev. Lett. 78, 2292 (1997).
• [79] AMANDA Collaboration (Bai et al.), Sep 2000. 7pp. Contrib. to the proc. of 3rd Int. Workshop on the Identification of Dark Matter (IDM2000), York, England, 18-22 Sep 2000. e-Print: astro-ph/0012285
• [80] Paper in preparation.
• [81] Ahrens et al. (AMANDA collaboration), Search for Supernova Neutrino Bursts with the AMANDA detector, accepted for publication, AstroParticle Physics, April 2001.
• [82] http://www-zeuthen.desy.de/nuastro/publications/others/proposal.shtml
• [83] http://www.ssec.wisc.edu/a3ri/icecube/proposal/
• [84] http://www-zeuthen.desy.de/nuastro/
• [85] The Origin of Cosmic Rays, V.L. Ginzburg & S.I. Syrovatskii (Pergamon Press, 1964).
• [86] M. Nagano et al. J. Phys. G10 (1984) 1295.
• [87] Yu. A. Fomin et al., Proc. 22nd Int. Cosmic Ray Conf. (Dublin) vol. 2 (1991) 85.
• [88] M. Takeda et al., Phys. Rev. Lett. 81 (1998) 1163.
• [89] M.A. Lawrence, R.J.O. Reid & A.A. Watson, J. Phys. G17 (1991) 733.
• [90] M.I. Pravdin et al., Proc. 26th Int. Cosmic Ray Conf. (Salt Lake City, 1999) vol. 3, p. 292.
• [91] D.J. Bird et al., Astrophys. J. 424 (1994) 491.
• [92] E.G. Berezhko & H.J. Völk, Astroparticle Phys. 7 (1997) 183.
• [93] T.K. Gaisser, F. Halzen, T. Stanev, Phys. Rep. 258 (1995) 173.
• [94] E. Waxman & J. Bahcall, Phys. Rev. D 59 (1999) 023002.
• [95] P.Lipari, Astropart. Phys. 1 (1993) 195-227.
• [96] G.R. Farrar & T. Piran, Phys. Rev. Letters 84 (2000) 3527.
• [97] T. K. Gaisser, to be published in Proceedings of the International Workshop on Observing Ultra-high energy Cosmic Rays from Space and Earth (Metepec, Puebla, Mexico, August 9-12, 2000), astro-ph/0011525.
• [98] T.K. Gaisser, Talk given at the OECD Megascience Forum Workshop, Taormina, Sicily, 22/23 May, 1997, astro-ph/9707283.
• [99] Mannheim, Protheroe & Rachen, Phys.Rev. D63 (2001) 023003, astro-ph/9812398; J.P. Rachen, R.J. Protheroe & K. Mannheim, Comment presented at the 19th Texas Symposium, Paris, December 1998, astro-ph/9908031.
• [100] J. Alvarez-Muñiz and F. Halzen, Phys. Rev. D 63, 037302 (2001).
• [101] L.V. Volkova, Yad. Fiz. 31, 1510 (1980) [Sov. J. Nucl. Phys. 31, 784 (1980)]. (1999).
• [102] D. Cline and F.W. Stecker, science white paper from UCLA Workshop on High Energy Neutrino Astrophysics, astro-ph/0003459.
• [103] R.J. Protheroe and T. Stanev, Phys. Rev. Lett. 77, 3708 (1996) and Erratum 78, 3420 (1997).
• [104] G. Gelmini and A. Kusenko, Phys. Rev. Lett. 84, 1378 (2000).
• [105] The Detection of Faint Light in Deep Underwater Neutrino Telescopes, C. Wiebusch, Ph.D. Thesis, PITHA 95/37, RWTH Aachen, Dec. 1995.
• [106] M. Birkel and S. Sarkar, Astropart. Phys. 9, 297 (1998).
• [107] Supernova Neutrino-Burst Detection with the AMANDA Detector, to be published.
• [108] F. Halzen, J.E. Jacobsen: Possibility that High Energy Neutrinos Telescopes could detect Supernovae, Phys. Rev. D49, 1758 (1994).
• [109] K. Scholberg, SNEWS: the Supernova Early Warning System, Conference proceedings paper of the 3rd Amaldi Conference on Gravitational Waves, astro-ph/9911359.
• [110] Christian Weinheimer and Lutz Köpke, AMANDA internal note 20000203.
• [111] Marc Hellwig et al., AMANDA internal note 20010301.
• [112] T. Neunhöffer for the AMANDA Collaboration, contributed paper to ICRC 2001.
• [113] P. Bauleo et al., UV-enhancement of photomultiplier response, a study of wavelength shifters for the AMANDA/IceCube detector, August 99.
• [114] J.F. Beacom and P. Vogel, Phys. Rev. D60, 33007 (1999).
• [115] T. Weiler, Astropart. Phys. 11, 303 (1999); D. Fargion, B. Mele and A. Salis, Astrophys. J. 517, 725 (1999).
• [116] V. Berezinsky, M. Kachelreiß and A. Vilenkin, Phys. Rev. Lett. 79, 4302 (1997).
• [117] F.W. Stecker et al., Phys. Rev. Lett., 66, 2697 (1991).
• [118] J.G. Learned and S. Pakvasa, Astrop. Phys. 3 (1995) pp 267-274.
• [119] H. Athar, G. Parente and E. Zas, in preparation.
• [120] I.Belolaptikov et al., Astropart.Phys. 7 (1997) 263.
• [121] J.Edsjo, WIMP searches with IceCube, Amanda Internal report, Jan.7, 2000.
• [122] K.Dick et al., Nucl.Phys. B588 (2000) 101-109 and Nucl.Phys. B598 (2001) 543-553.
• [123] J.G.Learned, K.Mannheim, High Energy Neutrino Astrophysics, Ann.Rev.Nucl.Phys. (2000).
• [124] M.Leuthold, Proc.Simulation and Analysis Methods for Large Neutrino Telescopes, DESY Zeuthen, 1998, DESY-PROC-1999-01 (ed. C.Spiering), 484.
• [125] M.Leuthold, IceCube Performance Studies, Amanda Internal Report, Nov.1999.
• [126] J.Krabi, C.Spiering et al., preprint PHE 91-03, Zeuthen 1991.
• [127] E. Waxman & J. Bahcall, Phys. Rev. Lett. 78 (1997) 2292.
• [128] E. Waxman & J. Bahcall, Phys. Rev. D 59 (1999) 023002.
• [129] C.Hettlage and K.Mannheim, to appear in the Proceedings of the XXIst Moriond Workshop Very High Energy Phenomena in the Universe, Les Arcs, France, January 20-27 2001, astro-ph/0103499
• [130] T.Gaisser, to be published in Proceedings of the International Workshop on Observing Ultra-high energy Cosmic Rays from Space and Earth (Metepec, Puebla, Mexico, August 9-12, 2000), astro-ph/0011525.
• [131] P. L. Biermann et al., Nucl. Phys. Proc. Suppl. 87 (2000) 417, astro-ph/0008063
• [132] G.C. Hill, K. Rawlins, Amanda Internal Report
• [133] G.C. Hill Astropart. Phys. 6 (1997) 215.
• [134] G.C. Hill. PhD thesis, University of Adelaide (1996)
• [135] G.C. Hill &. K. Rawlins Presentation at NSF Hartill Icecube Review, June 2000
• [136] A.Hillas et al., Astrophys.J. 503, 744.
• [137] T.Weekes, to be included in proceedings of the International Symposium on High Energy Gamma-Ray Astronomy, Heidelberg, June 2000, astrop-ph/0010431.
• [138] K.Wang et al., A survey of the Northern sky for TeV point sources, astro-ph/0103353
• [139] M.Leuthold, C.Spiering, H.Wissing, Amanda Internal Report.
• [140] G.Feldman, J.Cousins, Phys.Rev. D57 (1998) 3873.
• [141] S.Barwick, HENAP meeting (Venice, Feb. 2001), Amanda collaboration meeting in March 2001.
• [142] S.Hundertmark, Amanda collaboration meeting in Oct. 2000.
• [143] P.Meszaros and E.Waxman, astro-ph/0103275.
• [144] D.Guetta, Review talk, to appear in the Proc. of the XXIst Rencontres de Moriond "Very High Energy Phenomena in the Universe", Les Arcs, France, Jan. 20-27 (2001), astroph/0104045.
• [145] C.Schuster, M.Pohl, R.Schlickeiser, Neutrinos from AGN as diagnostic tool, submitted to A&A
• [146] E.Waxman, submitted to PRL, astro-ph/0102317.
• [147] T.Weiler, submitted to Astro. Part. Phys, astro-ph/0001233.
• [148] D.Bakari et al., hep-ex/0004019.
• [149] G.Giacomelli and L.Patrizii, Lecture at the Fifth School on Non-Accelerator Particle Astrophysics, Trieste, 29 June - 10 July 1998, hep-ex/0002032.
• [150] E.Andres et al., Astropart.Phys.13 (2000) 1.
• [151] see report on neutrino analysis on Zeuthen IceCube webpage.
• [152] C.Spiering, Nucl.Phys.Proc.Suppl. 91 (2000) 445-452.
• [153] L.Köpke and C.Weinheimer, Amanda Internal report.
• [154] K.Scholberg, Nucl.Phys.Proc.Suppl. 91 (2000) 331-337.
• [155] Pierre Auger Observatory, see http://www.auger.org/.
• [156] J.E. Dickinson et al., NIM A440 (2000) 95.
• [157] D. Nygren et al., Digital Optical Module & System Design for a km-Scale Neutrino Detector in Ice, LBNL INPA Internal Report, March 20, 1998.
• [158] R. G. Stokstad, RAP - A Method for Absolute Time Calibration of a Large Array based on a digital Optical Module System, LBNL-43200, October 9, 1998.
• [159] R. G. Stokstad, Consequences of a Local Coincidence for a Large Array in Ice, LBNL-41476, May 1998.
• [160] J. Jacobsen and R. G. Stokstad, Consequences of a Local Coincidence for a Large Array in Ice II: Local Coincidences in AMANDA B-10 1997 Data, LBNL INPA Internal Report, October 9, 1998.
• [161] J. Jacobsen and R. G. Stokstad, Consequences of a Local Coincidence for a Large Array in Ice III: Monte Carlo Simulations, LBNL INPA Internal Report, October 24, 1998.
• [162] See http://www.rational.com/products/rose for details about the Rational Rose model-driven software development system.
• [163] See http://www.sf.net for details about the Sourceforge software development system.
• [164] See http://cedar.web.cern.ch/CEDAR/ for details about the EDMS document handling system.
• [165] For Gaudi documentation, see http://proj-gaudi.web.cern.ch/proj-gaudi.

Table of Contents

Last modified: July 17, 2007

Contact the Webmaster: webmaster@icecube.wisc.edu