Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Home
Search
Quick Search
Advanced
Fulltext
Browse
Collections
Persons
My eDoc
Session History
Login
Name:
Password:
Documentation
Help
Support Wiki
Direct access to
document ID:


          Institute: MPI für extraterrestrische Physik     Collection: High Energy Astrophysics at MPE     Display Documents



  history
ID: 5827.0, MPI für extraterrestrische Physik / High Energy Astrophysics at MPE
The CERN Axion Solar Telescope (CAST)
Authors:Aalseth, C.E; Arik, E.; Autiero, D.; Avignone, F.T; Barth, K.; Bowyer, S.M; Bräuninger, H.; Brodzinski, R.L; Carmona, J.M; Cebrian, S.; Celebi, G.; Cetin, S.; Collar, JI.; Creswick, R.; Delbart, A.; Delattre, M.; DiLella, L.; De Oliveira, R.; Eleftheriadis, C.; Erdutan, N.; Fanourakis, G.; Farach, H.A; Fiorini, C.; Geralis, T.; Giomataris, I.; Girard, T.A; Gninenko, S.N; Golubev, N.A; Hasinoff, M.; Hoffmann, D.; Irastorza, I.G; Jacoby, J.; Jeanneau, F.; Knopf, M.A; Kovzelev, A.V; Kotthaus, R.; Krcmar, M.; Krecak, Z.; Lakic, B.; Liolios, A.; Ljubicic, A.; Lutz, G.; Longoni, A.; Luzon, G; Mailov, A.; Matveev, V.A; Miley, H.S; Morales, A.; Morales, J.; Mutterer, M.; Nikolaidis, A.; Nussinov, S.; Ortiz, A.; Pitts, W.K; Placci, A.; Postoev, V.E; Raffelt, G.G; Riege, H.; Sampieto, M.; Sarsa, M.; Savvidis, I.; Stipcevic, M.; Thomas, C.W; Thompson, R.C; Valco, P.; Villar, J.A; Villierme, B.; Walckiers, L.; Wilcox, W.; Zachariadou, K.; Zioutas, K
Language:English
Date of Publication (YYYY-MM-DD):2002-07
Title of Journal:Nuclear Physics B (Proceedings Supplement)
Journal Abbrev.:Nucl. Phys. B (Proc. Suppl.)
Volume:110
Start Page:85
End Page:87
Review Status:Peer-review
Audience:Experts Only
Abstract / Description:A decommissioned LHC test magnets is being prepared as the CERN Axion Solar Telescope (CAST) experiment. The magnet has a field of 9.6 Tesla and length of 10 meters. It is being mounted on a platform to track the sun over +/-8(0) vertically and +/-45(0), horizontally. A sensitivity in axion-photon coupling g(agammagamma) < 5 x 10(-11)GeV(-1) can be reached for m(a) less than or equal to 10(-2) eV, and with a gas filled tube-can reach g(agammagamma) less than or equal to 10(-10)GeV(-1) for axion masses m(a) < 2eV.
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für extraterrestrische Physik
External Affiliations:Pacific NW Natl Lab, Richland, WA 99352 USA; Pacific NW Natl Lab, Richland, WA 99352 USA; Univ S Carolina, Columbia, SC 29208 USA; Bogazici Univ, Istanbul, Turkey; CERN, European Org Nucl Res, CH-1211 Geneva, Switzerland; Max Planck Inst Extraterr Phys, Garching, Germany; Univ Zaragoza, Zaragoza 50009, Spain; Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA; Ctr Etud Saclay, F-91191 Gif Sur Yvette, France; Aristotle Univ Thessaloniki, GR-54006 Thessaloniki, Greece; Natl Res Ctr Phys Sci, Demokritos 60228, Greece; Politecn Milan, I-20133 Milan, Italy; Univ Lisbon, Lisbon, Portugal; Inst Nucl Res, Moscow, Russia; Univ British Columbia, Vancouver, BC V5Z 1M9, Canada; Tech Univ Darmstadt, Inst Kernphys, D-64289 Darmstadt, Germany; Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany; Rudjer Boskovic Inst, HR-10002 Zagreb, Croatia; Tel Aviv Univ, IL-69978 Tel Aviv, Israel; Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, D-80805 Munich, Germany; Univ Thessaloniki, GR-54006 Thessaloniki, Greece
Identifiers:ISSN:0920-5632
LOCALID:7032
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.