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The International Conference DARK 2000 Heidelberg, Germany, 10–14 July 2000 | 2001

Status of the Neutrino Telescope AMANDA: Monopoles and WIMPS

X. Bai; G. Barouch; S. W. Barwick; R. Bay; K. Becker; Lars Bergström; D. Bertrand; A. Biron; O. Botner; A. Bouchta; M. M. Boyce; Staffan Carius; A. Chen; D. Chirkin; J. M. Conrad; J. Cooley; C. G. S. Costa; D. F. Cowen; J. Dailing; E. Dalberg; T. DeYoung; P. Desiati; J.-P. Dewulf; P. Doksus; Joakim Edsjö; P. Ekström; T. Feser; M. Gaug; A. Goldschmidt; Ariel Goobar

The neutrino telescope AMANDA has been set up at the geographical South Pole as first step to a neutrino telescope of the scale of one cubic kilometer, which is the canonical size for a detector sensitive to neutrinos from Active Galactic Nuclei (AGN), Gamma Ray Bursts (GRB) and Topological Defects (TD). The location and depth in which the detector is installed is given by the requirement to detect neutrinos by the Cherenkov light produced by their reaction products and to keep the background due to atmospheric muons as small as possible. However, a detector optimized for this purpose is also capable to detect the bright Cherenkov light from relativistic Monopoles and neutrino signals from regions with high gravitational potential, where WIMPS are accumulated and possibly annihilate. Both hypothetical particles might contribute to the amount of dark matter. Therefore here a report about the status of the experiment (autumn 2000) and about the status of the search for these particles with the AMANDA B10 sub-detector is given.


arXiv: Astrophysics | 2001

WIMP searches with AMANDA-B10

X. Bai; J. Rodrguez Martino; Jeongwoo Kim; G. Yodh; R. Schwarz; P. Romenesko; R. Hardtke; E. Dalberg; Ch. Weinheimer; A. Bouchta; W. Wu; L. Köpke; P. Ekström; D. Steele; D. F. Cowen; H. G. Sander; M. Vander Donckt; F. Halzen; P. Desiati; C. G. S. Costa; K. Rawlins; P. Niessen; A. Silvestri; T. Schmidt; A. Biron; Ariel Goobar; D. Schneider; B. Koci; J. Jacobsen; P. Steffen

We report on the search for nearly vertical up-going muon neutrinos from WIMP annihilations in the center of the Earth with the AMANDA-B10 detector. The whole data sample collected in 1997, 10^9 events, has been analyzed and a final sample of 15 up-going events is found in a restricted zenith angular region where a signal from WIMP annihilations is expected. A preliminary upper limit at 90% confidence level on the annihilation rate of WIMPs in the center of the Earth is presented.


Archive | 2005

The IceCube Collaboration

A. Achterberg; M. Ackermann; J. Ahrens; X. Bai; B. Baret; M. Bartelt; R. Bay; K. Beattie; T. Becka; P. Berghaus; D. Berley; E. Bernardini; Daniel Bertrand; E. Blaufuss; O. Botner; A. Bouchta; Jürgen Braun; T. Burgess; T. Castermans; D. Chirkin; J. Clem; J. M. Conrad; Anna Davour; C. De Clercq; P. Desiati; T. DeYoung; J. Dreyer; R. Ehrlich; T. Feser; K. Filimonov


9th International Workshop, Venice, Italy, March 6-9, 2001 | 2001

Results from AMANDA

J. Ahrens; Ch. Weinheimer; J. Kim; Ph. Olbrechts; R. Hardtke; L. Gerhardt; A. Bouchta; L. Köpke; P. Ekström; D. Steele; D. F. Cowen; H. Wissing; H. G. Sander; M. Vander Donckt; F. Halzen; P. Desiati; C. G. S. Costa; K. Rawlins; P. Niessen; C. De Clercq; A. Silvestri; T. Schmidt; J. Booth; A. Biron; O. Botner; D. Schneider; B. Koci; J. Jacobsen; P. Steffen; P. Herquet


Proceedings of the 28th International Cosmic Ray Conference, Tsukuba, Japan, 31 July - 7 August 2003 | 2003

Search for Diffuse Fluxes of Extraterrestrial Muon- Neutrinos with the AMANDA Detectors

Gary C. Hill; Matthias J. Leuthold; Jodi A. Cooley; J. Ahrens; X. Bai; T. Becka; E. Bernardini; D. Bertrand; A. Biron; O. Botner; A. Bouchta; O. Bouhali; T. Burgess; Staffan Carius; T. Castermans; A. Chen; D. Chirkin; B. Collin; J. Conrad; Anna Davour; T. DeYoung; P. Desiati; P. Doksus; T. Feser; R. Ganugapati; H. Geenen; L. Gerhardt; Axel Groß; A. Goldschmidt; A. Hallgren


23rd Johns Hopkins Workshop on current problems in particle theory, Baltimore, USA, June 10-12, 1999 | 1999

From AMANDA to IceCube : Current and future high energy neutrino telescopes at the South Pole

Timothy Miller; G.M. Spiczak; A. Biron; A. Bouchta; P. Desiati; M. Gaug; S. Hundertmark; M. Kowalski; H. Leich; M. Leuthold; P. Niessen; T. Schmidt; A. Silvestri; C. Spiering; P. Steffen; O. Streicher; T. Thron; C. Wienbusch; R. Wischnewski; Staffan Carius; P. Lindahl; L. Berstrom; E. Dalberg; Joakim Edsjö; P. Ekström; A. Goodbar; P. O. Hulth; J. Rodriguez Martino; H. Rubenstein; C. Walck


21st Rencontres de Moriond Workshop on Very High-Energy Phenomena in the Universe, 20-27 Jan 2001. Les Arcs, France | 2001

Initial results from AMANDA

J. Ahrens; X. Bai; G. Barouch; S. W. Barwick; R. Bay; T. Becka; K. Becker; D. Bertrand; A. Biron; J. Booth; O. Botner; A. Bouchta; M. M. Boyce; Staffan Carius; A. Chen; D. Chirkin; J. Conrad; J. Cooley; C. G. S. Costa; D. F. Cowen; E. Dalberg; T. DeYoung; P. Desiati; J.-P. Dewulf; P. Doksus; Joakim Edsjö; P. Ekström; T. Feser; M. Gaug; A. Goldschmidt

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P. Desiati

University of Wisconsin-Madison

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X. Bai

University of Delaware

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C. G. S. Costa

University of Wisconsin-Madison

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D. Chirkin

University of Wisconsin-Madison

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D. F. Cowen

Pennsylvania State University

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