The CERN Axion Solar Telescope (CAST)

C. E. Aalseth; E. Arik; D. Autiero; F. T. Avignone; K. Barth; S. M. Bowyer; H. Brauninger; R. L. Brodzinski; J. M. Carmona; S. Cebrian; G. Celebi; S. Cetin; J. I. Collar; R. Creswick; A. Delbart; M. Delattre; L. DiLella; R. De Oliveira; Ch Eleftheriadis; N. Erdutan; G. Fanourakis; H. A. Farach; C. Fiorini; Th Geralis; I. Giomataris; T. A. Girard; S. N. Gninenko; N. A. Golubev; M. Hasinoff; D. Hoffmann; I. G. Irastorza; J. Jacoby; F. Jeanneau; M. A. Knopf; A. V. Kovzelev; R. Kotthaus; M. Krčmar; Z. Krečak; B. Lakić; A. Liolios; A. Ljubičić; G. Lutz; A. Longoni; G. Luzon; A. Mailov; V. A. Matveev; H. S. Miley; A. Morales; J. Morales; M. Mutterer; A. Nikolaidis; S. Nussinov; A. Ortiz; W. K. Pitts; A. Placci; V. E. Postoev; G. G. Raffelt; H. Riege; M. Sampieto; M. Sarsa; I. Savvidis; M. Stipčević; C. W. Thomas; R. C. Thompson; P. Valco; J. A. Villar; B. Villierme; L. Walckiers; W. Wilcox; K. Zachariadou; K. Zioutas

doi:10.1016/s0920-5632(02)01459-7

The CERN Axion Solar Telescope (CAST)

C. E. Aalseth
, E. Arik
, D. Autiero
, F. T. Avignone
, K. Barth
, S. M. Bowyer
, H. Brauninger
, R. L. Brodzinski
, J. M. Carmona
, S. Cebrian
, G. Celebi
, S. Cetin
, J. I. Collar
, R. Creswick
, A. Delbart
, M. Delattre
, L. DiLella
, R. De Oliveira
, Ch Eleftheriadis
, N. Erdutan

G. Fanourakis, H. A. Farach, C. Fiorini, Th Geralis, I. Giomataris, T. A. Girard, S. N. Gninenko, N. A. Golubev, M. Hasinoff, D. Hoffmann, I. G. Irastorza, J. Jacoby, F. Jeanneau, M. A. Knopf, A. V. Kovzelev, R. Kotthaus, M. Krčmar, Z. Krečak, B. Lakić, A. Liolios, A. Ljubičić, G. Lutz, A. Longoni, G. Luzon, A. Mailov, V. A. Matveev, H. S. Miley, A. Morales, J. Morales, M. Mutterer, A. Nikolaidis, S. Nussinov, A. Ortiz, W. K. Pitts, A. Placci, V. E. Postoev, G. G. Raffelt, H. Riege, M. Sampieto, M. Sarsa, I. Savvidis, M. Stipčević, C. W. Thomas, R. C. Thompson, P. Valco, J. A. Villar, B. Villierme, L. Walckiers, W. Wilcox, K. Zachariadou, K. Zioutas

Pacific Northwest National Laboratory
University of South Carolina
Bogazici University
CERN
Max Planck Institute for Extraterrestrial Physics
University of Zaragoza
The University of Chicago
Centre d'Etudes de Saclay
Aristotle University of Thessaloniki
Natl. Res. Center for Physical Sci.
Polytechnic University of Milan
University of Lisbon
Russian Academy of Sciences
University of British Columbia
Technische Universität Darmstadt
Max Planck Institute for Physics (Werner Heisenberg Institute)
Ruder Boskovic Institute
Tel Aviv University

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

15 Scopus citations

Abstract

A decommissioned LHC test magnet 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 ±8⁰ vertically and ±45⁰, horizontally. A sensitivity in axion-photon coupling g_aγγ < 5 × 10^-11 GeV^-1 can be reached for m_a ≤ 10^-2eV, and with a gas filled tube-can reach g_aγγ ≤ 10^-10GeV^-1 for axion masses m_a < 2eV.

Original language	English
Pages (from-to)	85-87
Number of pages	3
Journal	Nuclear Physics B - Proceedings Supplements
Volume	110
DOIs	https://doi.org/10.1016/s0920-5632(02)01459-7
State	Published - Jul 2002
Externally published	Yes

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Aalseth, C. E., Arik, E., Autiero, D., Avignone, F. T., Barth, K., Bowyer, S. M., Brauninger, H., Brodzinski, R. L., Carmona, J. M., Cebrian, S., Celebi, G., Cetin, S., Collar, J. I., Creswick, R., Delbart, A., Delattre, M., DiLella, L., De Oliveira, R., Eleftheriadis, C., ... Zioutas, K. (2002). The CERN Axion Solar Telescope (CAST). Nuclear Physics B - Proceedings Supplements, 110, 85-87. https://doi.org/10.1016/s0920-5632(02)01459-7

@article{813cedafa12f4721ac2bb18d348674e7,

title = "The CERN Axion Solar Telescope (CAST)",

abstract = "A decommissioned LHC test magnet 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 ±80 vertically and ±450, horizontally. A sensitivity in axion-photon coupling gaγγ < 5 × 10-11 GeV-1 can be reached for ma ≤ 10-2eV, and with a gas filled tube-can reach gaγγ ≤ 10-10GeV-1 for axion masses ma < 2eV.",

author = "Aalseth, \{C. E.\} and E. Arik and D. Autiero and Avignone, \{F. T.\} and K. Barth and Bowyer, \{S. M.\} and H. Brauninger and Brodzinski, \{R. L.\} and Carmona, \{J. M.\} and S. Cebrian and G. Celebi and S. Cetin and Collar, \{J. I.\} and R. Creswick and A. Delbart and M. Delattre and L. DiLella and \{De Oliveira\}, R. and Ch Eleftheriadis and N. Erdutan and G. Fanourakis and Farach, \{H. A.\} and C. Fiorini and Th Geralis and I. Giomataris and Girard, \{T. A.\} and Gninenko, \{S. N.\} and Golubev, \{N. A.\} and M. Hasinoff and D. Hoffmann and Irastorza, \{I. G.\} and J. Jacoby and F. Jeanneau and Knopf, \{M. A.\} and Kovzelev, \{A. V.\} and R. Kotthaus and M. Kr{\v c}mar and Z. Kre{\v c}ak and B. Laki{\'c} and A. Liolios and A. Ljubi{\v c}i{\'c} and G. Lutz and A. Longoni and G. Luzon and A. Mailov and Matveev, \{V. A.\} and Miley, \{H. S.\} and A. Morales and J. Morales and M. Mutterer and A. Nikolaidis and S. Nussinov and A. Ortiz and Pitts, \{W. K.\} and A. Placci and Postoev, \{V. E.\} and Raffelt, \{G. G.\} and H. Riege and M. Sampieto and M. Sarsa and I. Savvidis and M. Stip{\v c}evi{\'c} and Thomas, \{C. W.\} and Thompson, \{R. C.\} and P. Valco and Villar, \{J. A.\} and B. Villierme and L. Walckiers and W. Wilcox and K. Zachariadou and K. Zioutas",

year = "2002",

month = jul,

doi = "10.1016/s0920-5632(02)01459-7",

language = "英语",

volume = "110",

pages = "85--87",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

publisher = "Elsevier",

}

Aalseth, CE, Arik, E, Autiero, D, Avignone, FT, Barth, K, Bowyer, SM, Brauninger, H, Brodzinski, RL, Carmona, JM, 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, HA, Fiorini, C, Geralis, T, Giomataris, I, Girard, TA, Gninenko, SN, Golubev, NA, Hasinoff, M, Hoffmann, D, Irastorza, IG, Jacoby, J, Jeanneau, F, Knopf, MA, Kovzelev, AV, Kotthaus, R, Krčmar, M, Krečak, Z, Lakić, B, Liolios, A, Ljubičić, A, Lutz, G, Longoni, A, Luzon, G, Mailov, A, Matveev, VA, Miley, HS, Morales, A, Morales, J, Mutterer, M, Nikolaidis, A, Nussinov, S, Ortiz, A, Pitts, WK, Placci, A, Postoev, VE, Raffelt, GG, Riege, H, Sampieto, M, Sarsa, M, Savvidis, I, Stipčević, M, Thomas, CW, Thompson, RC, Valco, P, Villar, JA, Villierme, B, Walckiers, L, Wilcox, W, Zachariadou, K & Zioutas, K 2002, 'The CERN Axion Solar Telescope (CAST)', Nuclear Physics B - Proceedings Supplements, vol. 110, pp. 85-87. https://doi.org/10.1016/s0920-5632(02)01459-7

TY - JOUR

T1 - The CERN Axion Solar Telescope (CAST)

AU - Aalseth, C. E.

AU - Arik, E.

AU - Autiero, D.

AU - Avignone, F. T.

AU - Barth, K.

AU - Bowyer, S. M.

AU - Brauninger, H.

AU - Brodzinski, R. L.

AU - Carmona, J. M.

AU - Cebrian, S.

AU - Celebi, G.

AU - Cetin, S.

AU - Collar, J. I.

AU - Creswick, R.

AU - Delbart, A.

AU - Delattre, M.

AU - DiLella, L.

AU - De Oliveira, R.

AU - Eleftheriadis, Ch

AU - Erdutan, N.

AU - Fanourakis, G.

AU - Farach, H. A.

AU - Fiorini, C.

AU - Geralis, Th

AU - Giomataris, I.

AU - Girard, T. A.

AU - Gninenko, S. N.

AU - Golubev, N. A.

AU - Hasinoff, M.

AU - Hoffmann, D.

AU - Irastorza, I. G.

AU - Jacoby, J.

AU - Jeanneau, F.

AU - Knopf, M. A.

AU - Kovzelev, A. V.

AU - Kotthaus, R.

AU - Krčmar, M.

AU - Krečak, Z.

AU - Lakić, B.

AU - Liolios, A.

AU - Ljubičić, A.

AU - Lutz, G.

AU - Longoni, A.

AU - Luzon, G.

AU - Mailov, A.

AU - Matveev, V. A.

AU - Miley, H. S.

AU - Morales, A.

AU - Morales, J.

AU - Mutterer, M.

AU - Nikolaidis, A.

AU - Nussinov, S.

AU - Ortiz, A.

AU - Pitts, W. K.

AU - Placci, A.

AU - Postoev, V. E.

AU - Raffelt, G. G.

AU - Riege, H.

AU - Sampieto, M.

AU - Sarsa, M.

AU - Savvidis, I.

AU - Stipčević, M.

AU - Thomas, C. W.

AU - Thompson, R. C.

AU - Valco, P.

AU - Villar, J. A.

AU - Villierme, B.

AU - Walckiers, L.

AU - Wilcox, W.

AU - Zachariadou, K.

AU - Zioutas, K.

PY - 2002/7

Y1 - 2002/7

N2 - A decommissioned LHC test magnet 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 ±80 vertically and ±450, horizontally. A sensitivity in axion-photon coupling gaγγ < 5 × 10-11 GeV-1 can be reached for ma ≤ 10-2eV, and with a gas filled tube-can reach gaγγ ≤ 10-10GeV-1 for axion masses ma < 2eV.

AB - A decommissioned LHC test magnet 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 ±80 vertically and ±450, horizontally. A sensitivity in axion-photon coupling gaγγ < 5 × 10-11 GeV-1 can be reached for ma ≤ 10-2eV, and with a gas filled tube-can reach gaγγ ≤ 10-10GeV-1 for axion masses ma < 2eV.

UR - https://www.scopus.com/pages/publications/0036666732

U2 - 10.1016/s0920-5632(02)01459-7

DO - 10.1016/s0920-5632(02)01459-7

M3 - 文章

AN - SCOPUS:0036666732

SN - 0920-5632

VL - 110

SP - 85

EP - 87

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

ER -

The CERN Axion Solar Telescope (CAST)

Abstract

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