The CERN Axion Solar Telescope (CAST): An update

S. Andriamonje; V. Arsov; S. Aune; T. Aune; F. T. Avignone; K. Barth; A. Belov; B. Beltran; H. Bräuninger; J. Carmona; S. Cebrián; E. Chesi; G. Cipolla; J. Collar; R. Creswick; T. Dafni; M. Davenport; S. Dedousis; M. Delattre; A. Delbart; R. DeOliveira; L. DiLella; C. Eleftheriadis; J. Engelhauser; G. Fanourakis; H. Farach; E. Ferrer; H. Fischer; F. Formenti; J. Franz; P. Friedrich; T. Geralis; I. Giomataris; S. Gninenko; N. Golubev; R. Hartmann; M. Hasinoff; F. H. Heinsius; D. H.H. Hoffmann; I. Irastorza; J. Jacoby; J. N. Joux; D. Kang; K. Königsmann; R. Kotthaus; M. Krcmar; M. Kuster; B. Lakic; C. Lasseur; A. Liolios; A. Lippitsch; A. Ljubicic; G. Lutz; G. Luzon; A. Morales; J. Morales; M. Mutterer; A. Nikolaidis; A. Ortiz de Solorzano; T. Papaevangelou; A. Placci; G. Raffelt; P. Rammos; J. P. Robert; J. Ruz; M. Sarsa; C. Schill; W. Serber; Y. Semertzidis; J. Vieira; J. Villar; B. Vullierme; L. Walckiers; K. Zioutas

doi:10.1016/j.nuclphysbps.2004.11.008

The CERN Axion Solar Telescope (CAST): An update

S. Andriamonje
, V. Arsov
, S. Aune
, T. Aune
, F. T. Avignone
, K. Barth
, A. Belov
, B. Beltran
, H. Bräuninger
, J. Carmona
, S. Cebrián
, E. Chesi
, G. Cipolla
, J. Collar
, R. Creswick
, T. Dafni
, M. Davenport
, S. Dedousis
, M. Delattre
, A. Delbart

R. DeOliveira, L. DiLella, C. Eleftheriadis, J. Engelhauser, G. Fanourakis, H. Farach, E. Ferrer, H. Fischer, F. Formenti, J. Franz, P. Friedrich, T. Geralis, I. Giomataris, S. Gninenko, N. Golubev, R. Hartmann, M. Hasinoff, F. H. Heinsius, D. H.H. Hoffmann, I. Irastorza, J. Jacoby, J. N. Joux, D. Kang, K. Königsmann, R. Kotthaus, M. Krcmar, M. Kuster, B. Lakic, C. Lasseur, A. Liolios, A. Lippitsch, A. Ljubicic, G. Lutz, G. Luzon, A. Morales, J. Morales, M. Mutterer, A. Nikolaidis, A. Ortiz de Solorzano, T. Papaevangelou, A. Placci, G. Raffelt, P. Rammos, J. P. Robert, J. Ruz, M. Sarsa, C. Schill, W. Serber, Y. Semertzidis, J. Vieira, J. Villar, B. Vullierme, L. Walckiers, K. Zioutas

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

6 Scopus citations

Abstract

The CERN Axion Solar Telescope (CAST), a 10 meter long LHC, 9 Tesla, test magnet is mounted on a moving platform that tracks the sun about 1.5 hours during sunrise, again during sunset. It moves ±8⁰ vertically and ±40⁰ horizontally. It has been taking data continuously since July 10, 2003. Data analyzed thus far yield an upper bound on the photon-axion coupling constant, g_aγγ ≤ 3 × 10^-10 GeV^-1 for axion masses less than 5 × 10^-2 eV.

Original language	English
Pages (from-to)	41-44
Number of pages	4
Journal	Nuclear Physics B - Proceedings Supplements
Volume	138
Issue number	1-3
DOIs	https://doi.org/10.1016/j.nuclphysbps.2004.11.008
State	Published - Jan 2005
Externally published	Yes

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10.1016/j.nuclphysbps.2004.11.008

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Andriamonje, S., Arsov, V., Aune, S., Aune, T., Avignone, F. T., Barth, K., Belov, A., Beltran, B., Bräuninger, H., Carmona, J., Cebrián, S., Chesi, E., Cipolla, G., Collar, J., Creswick, R., Dafni, T., Davenport, M., Dedousis, S., Delattre, M., ... Zioutas, K. (2005). The CERN Axion Solar Telescope (CAST): An update. Nuclear Physics B - Proceedings Supplements, 138(1-3), 41-44. https://doi.org/10.1016/j.nuclphysbps.2004.11.008

@article{92bdbb62530e41098843008fb6fbaecc,

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

abstract = "The CERN Axion Solar Telescope (CAST), a 10 meter long LHC, 9 Tesla, test magnet is mounted on a moving platform that tracks the sun about 1.5 hours during sunrise, again during sunset. It moves ±80 vertically and ±400 horizontally. It has been taking data continuously since July 10, 2003. Data analyzed thus far yield an upper bound on the photon-axion coupling constant, gaγγ ≤ 3 × 10-10 GeV-1 for axion masses less than 5 × 10-2 eV.",

author = "S. Andriamonje and V. Arsov and S. Aune and T. Aune and Avignone, \{F. T.\} and K. Barth and A. Belov and B. Beltran and H. Br{\"a}uninger and J. Carmona and S. Cebri{\'a}n and E. Chesi and G. Cipolla and J. Collar and R. Creswick and T. Dafni and M. Davenport and S. Dedousis and M. Delattre and A. Delbart and R. DeOliveira and L. DiLella and C. Eleftheriadis and J. Engelhauser and G. Fanourakis and H. Farach and E. Ferrer and H. Fischer and F. Formenti and J. Franz and P. Friedrich and T. Geralis and I. Giomataris and S. Gninenko and N. Golubev and R. Hartmann and M. Hasinoff and Heinsius, \{F. H.\} and Hoffmann, \{D. H.H.\} and I. Irastorza and J. Jacoby and Joux, \{J. N.\} and D. Kang and K. K{\"o}nigsmann and R. Kotthaus and M. Krcmar and M. Kuster and B. Lakic and C. Lasseur and A. Liolios and A. Lippitsch and A. Ljubicic and G. Lutz and G. Luzon and A. Morales and J. Morales and M. Mutterer and A. Nikolaidis and \{de Solorzano\}, \{A. Ortiz\} and T. Papaevangelou and A. Placci and G. Raffelt and P. Rammos and Robert, \{J. P.\} and J. Ruz and M. Sarsa and C. Schill and W. Serber and Y. Semertzidis and J. Vieira and J. Villar and B. Vullierme and L. Walckiers and K. Zioutas",

year = "2005",

month = jan,

doi = "10.1016/j.nuclphysbps.2004.11.008",

language = "英语",

volume = "138",

pages = "41--44",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

publisher = "Elsevier",

number = "1-3",

}

Andriamonje, S, Arsov, V, Aune, S, Aune, T, Avignone, FT, Barth, K, Belov, A, Beltran, B, Bräuninger, H, Carmona, J, Cebrián, S, Chesi, E, Cipolla, G, Collar, J, Creswick, R, Dafni, T, Davenport, M, Dedousis, S, Delattre, M, Delbart, A, DeOliveira, R, DiLella, L, Eleftheriadis, C, Engelhauser, J, Fanourakis, G, Farach, H, Ferrer, E, Fischer, H, Formenti, F, Franz, J, Friedrich, P, Geralis, T, Giomataris, I, Gninenko, S, Golubev, N, Hartmann, R, Hasinoff, M, Heinsius, FH, Hoffmann, DHH, Irastorza, I, Jacoby, J, Joux, JN, Kang, D, Königsmann, K, Kotthaus, R, Krcmar, M, Kuster, M, Lakic, B, Lasseur, C, Liolios, A, Lippitsch, A, Ljubicic, A, Lutz, G, Luzon, G, Morales, A, Morales, J, Mutterer, M, Nikolaidis, A, de Solorzano, AO, Papaevangelou, T, Placci, A, Raffelt, G, Rammos, P, Robert, JP, Ruz, J, Sarsa, M, Schill, C, Serber, W, Semertzidis, Y, Vieira, J, Villar, J, Vullierme, B, Walckiers, L & Zioutas, K 2005, 'The CERN Axion Solar Telescope (CAST): An update', Nuclear Physics B - Proceedings Supplements, vol. 138, no. 1-3, pp. 41-44. https://doi.org/10.1016/j.nuclphysbps.2004.11.008

TY - JOUR

T1 - The CERN Axion Solar Telescope (CAST)

T2 - An update

AU - Andriamonje, S.

AU - Arsov, V.

AU - Aune, S.

AU - Aune, T.

AU - Avignone, F. T.

AU - Barth, K.

AU - Belov, A.

AU - Beltran, B.

AU - Bräuninger, H.

AU - Carmona, J.

AU - Cebrián, S.

AU - Chesi, E.

AU - Cipolla, G.

AU - Collar, J.

AU - Creswick, R.

AU - Dafni, T.

AU - Davenport, M.

AU - Dedousis, S.

AU - Delattre, M.

AU - Delbart, A.

AU - DeOliveira, R.

AU - DiLella, L.

AU - Eleftheriadis, C.

AU - Engelhauser, J.

AU - Fanourakis, G.

AU - Farach, H.

AU - Ferrer, E.

AU - Fischer, H.

AU - Formenti, F.

AU - Franz, J.

AU - Friedrich, P.

AU - Geralis, T.

AU - Giomataris, I.

AU - Gninenko, S.

AU - Golubev, N.

AU - Hartmann, R.

AU - Hasinoff, M.

AU - Heinsius, F. H.

AU - Hoffmann, D. H.H.

AU - Irastorza, I.

AU - Jacoby, J.

AU - Joux, J. N.

AU - Kang, D.

AU - Königsmann, K.

AU - Kotthaus, R.

AU - Krcmar, M.

AU - Kuster, M.

AU - Lakic, B.

AU - Lasseur, C.

AU - Liolios, A.

AU - Lippitsch, A.

AU - Ljubicic, A.

AU - Lutz, G.

AU - Luzon, G.

AU - Morales, A.

AU - Morales, J.

AU - Mutterer, M.

AU - Nikolaidis, A.

AU - de Solorzano, A. Ortiz

AU - Papaevangelou, T.

AU - Placci, A.

AU - Raffelt, G.

AU - Rammos, P.

AU - Robert, J. P.

AU - Ruz, J.

AU - Sarsa, M.

AU - Schill, C.

AU - Serber, W.

AU - Semertzidis, Y.

AU - Vieira, J.

AU - Villar, J.

AU - Vullierme, B.

AU - Walckiers, L.

AU - Zioutas, K.

PY - 2005/1

Y1 - 2005/1

N2 - The CERN Axion Solar Telescope (CAST), a 10 meter long LHC, 9 Tesla, test magnet is mounted on a moving platform that tracks the sun about 1.5 hours during sunrise, again during sunset. It moves ±80 vertically and ±400 horizontally. It has been taking data continuously since July 10, 2003. Data analyzed thus far yield an upper bound on the photon-axion coupling constant, gaγγ ≤ 3 × 10-10 GeV-1 for axion masses less than 5 × 10-2 eV.

AB - The CERN Axion Solar Telescope (CAST), a 10 meter long LHC, 9 Tesla, test magnet is mounted on a moving platform that tracks the sun about 1.5 hours during sunrise, again during sunset. It moves ±80 vertically and ±400 horizontally. It has been taking data continuously since July 10, 2003. Data analyzed thus far yield an upper bound on the photon-axion coupling constant, gaγγ ≤ 3 × 10-10 GeV-1 for axion masses less than 5 × 10-2 eV.

UR - https://www.scopus.com/pages/publications/26644441652

U2 - 10.1016/j.nuclphysbps.2004.11.008

DO - 10.1016/j.nuclphysbps.2004.11.008

M3 - 文章

AN - SCOPUS:26644441652

SN - 0920-5632

VL - 138

SP - 41

EP - 44

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

IS - 1-3

ER -

The CERN Axion Solar Telescope (CAST): An update

Abstract

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