Search for solar axions: CAST

Biljana Lakić; S. Andriamonje; V. Arsov; S. Aune; D. Autiero; F. Avignone; K. Barth; A. Belov; B. Beltrán; H. Bräuninger; J. M. Carmona; S. Cebrián; E. Chesi; J. I. Collar; R. Creswick; T. Dafni; M. Davenport; L. Di Lella; C. Eleftheriadis; J. Englhauser; G. Fanourakis; H. Farach; E. Ferrer; H. Fischer; J. Franz; P. Friedrich; T. Geralis; I. Giomataris; S. Gninenko; N. Goloubev; R. Hartmann; M. D. Hasinoff; F. H. Heinsius; D. H.H. Hoffmann; I. G. Irastorza; J. Jacoby; D. Kang; K. Königsmann; R. Kotthaus; M. Krčmar; K. Kousouris; M. Kuster; C. Lasseur; A. Liolios; A. Ljubičić; G. Lutz; G. Luzón; D. W. Miller; A. Morales; J. Morales; A. Ortiz; T. Papaevangelou; A. Placci; G. Raffelt; J. Ruz; H. Riege; M. L. Sarsa; I. Savvidis; P. Serpico; Y. Semertzidis; L. Stewart; J. D. Vieira; J. Villar; L. Walckiers; K. Zachariadou; K. Zioutas

Search for solar axions: CAST

Biljana Lakić
, S. Andriamonje
, V. Arsov
, S. Aune
, D. Autiero
, F. Avignone
, K. Barth
, A. Belov
, B. Beltrán
, H. Bräuninger
, J. M. Carmona
, S. Cebrián
, E. Chesi
, J. I. Collar
, R. Creswick
, T. Dafni
, M. Davenport
, L. Di Lella
, C. Eleftheriadis
, J. Englhauser

G. Fanourakis, H. Farach, E. Ferrer, H. Fischer, J. Franz, P. Friedrich, T. Geralis, I. Giomataris, S. Gninenko, N. Goloubev, R. Hartmann, M. D. Hasinoff, F. H. Heinsius, D. H.H. Hoffmann, I. G. Irastorza, J. Jacoby, D. Kang, K. Königsmann, R. Kotthaus, M. Krčmar, K. Kousouris, M. Kuster, C. Lasseur, A. Liolios, A. Ljubičić, G. Lutz, G. Luzón, D. W. Miller, A. Morales, J. Morales, A. Ortiz, T. Papaevangelou, A. Placci, G. Raffelt, J. Ruz, H. Riege, M. L. Sarsa, I. Savvidis, P. Serpico, Y. Semertzidis, L. Stewart, J. D. Vieira, J. Villar, L. Walckiers, K. Zachariadou, K. Zioutas

Ruder Boskovic Institute
Centre d'Études de Saclay (CEA-Saclay)
Goethe University Frankfurt
CERN
Institute de Physique Nucléaire
University of South Carolina
Russian Academy of Sciences
University of Zaragoza
Max Planck Institute for Extraterrestrial Physics
The University of Chicago
Technische Universität Darmstadt
Scuola Normale Superiore di Pisa
Demokritos National Centre for Scientific Research
University of Freiburg
University of British Columbia
Max Planck Institute for Physics (Werner Heisenberg Institute)
Aristotle University of Thessaloniki
Brookhaven National Laboratory
University of Patras

科研成果: 期刊稿件 › 会议文章 › 同行评审

摘要

The CERN Axion Solar Telescope (CAST) is searching for axions produced in the Sun’s core by the Primakoff process. CAST is using a decommissioned Large Hadron Collider (LHC) test magnet where axions could be converted back into X-rays with energies up to 10 keV. Analysis of the 2003 data showed no signal above background implying an upper limit for the axion-photon coupling constant ga_γγ < 1.16 × 10⁻¹⁰ GeV⁻¹ at 95% C.L. for m_a 0.02 eV [1]. The higher quality 2004 data is presently under analysis. CAST Phase II is scheduled to start in late 2005. This will be the first step in extending CAST’s sensitivity to axion rest masses up to ∼ 1 eV.

源语言	英语
期刊	Proceedings of Science
卷	21
出版状态	已出版 - 2005
已对外发布	是
活动	2005 International Europhysics Conference on High Energy Physics, HEP 2005 - Lisboa, 葡萄牙期限: 21 7月 2005 → 27 7月 2005

其它文件与链接

链接到 Scopus 的出版物

引用此

@article{1be864744e5b4830961926240e1809f1,

title = "Search for solar axions: CAST",

abstract = "The CERN Axion Solar Telescope (CAST) is searching for axions produced in the Sun{\textquoteright}s core by the Primakoff process. CAST is using a decommissioned Large Hadron Collider (LHC) test magnet where axions could be converted back into X-rays with energies up to 10 keV. Analysis of the 2003 data showed no signal above background implying an upper limit for the axion-photon coupling constant gaγγ < 1.16 × 10−10 GeV−1 at 95\% C.L. for ma 0.02 eV [1]. The higher quality 2004 data is presently under analysis. CAST Phase II is scheduled to start in late 2005. This will be the first step in extending CAST{\textquoteright}s sensitivity to axion rest masses up to ∼ 1 eV.",

author = "Biljana Laki{\'c} and S. Andriamonje and V. Arsov and S. Aune and D. Autiero and F. Avignone and K. Barth and A. Belov and B. Beltr{\'a}n and H. Br{\"a}uninger and Carmona, \{J. M.\} and S. Cebri{\'a}n and E. Chesi and Collar, \{J. I.\} and R. Creswick and T. Dafni and M. Davenport and \{Di Lella\}, L. and C. Eleftheriadis and J. Englhauser and G. Fanourakis and H. Farach and E. Ferrer and H. Fischer and J. Franz and P. Friedrich and T. Geralis and I. Giomataris and S. Gninenko and N. Goloubev and R. Hartmann and Hasinoff, \{M. D.\} and Heinsius, \{F. H.\} and Hoffmann, \{D. H.H.\} and Irastorza, \{I. G.\} and J. Jacoby and D. Kang and K. K{\"o}nigsmann and R. Kotthaus and M. Kr{\v c}mar and K. Kousouris and M. Kuster and C. Lasseur and A. Liolios and A. Ljubi{\v c}i{\'c} and G. Lutz and G. Luz{\'o}n and Miller, \{D. W.\} and A. Morales and J. Morales and A. Ortiz and T. Papaevangelou and A. Placci and G. Raffelt and J. Ruz and H. Riege and Sarsa, \{M. L.\} and I. Savvidis and P. Serpico and Y. Semertzidis and L. Stewart and Vieira, \{J. D.\} and J. Villar and L. Walckiers and K. Zachariadou and K. Zioutas",

note = "Publisher Copyright: {\textcopyright} Copiright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.; 2005 International Europhysics Conference on High Energy Physics, HEP 2005 ; Conference date: 21-07-2005 Through 27-07-2005",

year = "2005",

language = "英语",

volume = "21",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

Lakić, B, Andriamonje, S, Arsov, V, Aune, S, Autiero, D, Avignone, F, Barth, K, Belov, A, Beltrán, B, Bräuninger, H, Carmona, JM, Cebrián, S, Chesi, E, Collar, JI, Creswick, R, Dafni, T, Davenport, M, Di Lella, L, Eleftheriadis, C, Englhauser, J, Fanourakis, G, Farach, H, Ferrer, E, Fischer, H, Franz, J, Friedrich, P, Geralis, T, Giomataris, I, Gninenko, S, Goloubev, N, Hartmann, R, Hasinoff, MD, Heinsius, FH, Hoffmann, DHH, Irastorza, IG, Jacoby, J, Kang, D, Königsmann, K, Kotthaus, R, Krčmar, M, Kousouris, K, Kuster, M, Lasseur, C, Liolios, A, Ljubičić, A, Lutz, G, Luzón, G, Miller, DW, Morales, A, Morales, J, Ortiz, A, Papaevangelou, T, Placci, A, Raffelt, G, Ruz, J, Riege, H, Sarsa, ML, Savvidis, I, Serpico, P, Semertzidis, Y, Stewart, L, Vieira, JD, Villar, J, Walckiers, L, Zachariadou, K & Zioutas, K 2005, 'Search for solar axions: CAST', Proceedings of Science, 卷 21.

TY - JOUR

T1 - Search for solar axions

T2 - 2005 International Europhysics Conference on High Energy Physics, HEP 2005

AU - Lakić, Biljana

AU - Andriamonje, S.

AU - Arsov, V.

AU - Aune, S.

AU - Autiero, D.

AU - Avignone, F.

AU - Barth, K.

AU - Belov, A.

AU - Beltrán, B.

AU - Bräuninger, H.

AU - Carmona, J. M.

AU - Cebrián, S.

AU - Chesi, E.

AU - Collar, J. I.

AU - Creswick, R.

AU - Dafni, T.

AU - Davenport, M.

AU - Di Lella, L.

AU - Eleftheriadis, C.

AU - Englhauser, J.

AU - Fanourakis, G.

AU - Farach, H.

AU - Ferrer, E.

AU - Fischer, H.

AU - Franz, J.

AU - Friedrich, P.

AU - Geralis, T.

AU - Giomataris, I.

AU - Gninenko, S.

AU - Goloubev, N.

AU - Hartmann, R.

AU - Hasinoff, M. D.

AU - Heinsius, F. H.

AU - Hoffmann, D. H.H.

AU - Irastorza, I. G.

AU - Jacoby, J.

AU - Kang, D.

AU - Königsmann, K.

AU - Kotthaus, R.

AU - Krčmar, M.

AU - Kousouris, K.

AU - Kuster, M.

AU - Lasseur, C.

AU - Liolios, A.

AU - Ljubičić, A.

AU - Lutz, G.

AU - Luzón, G.

AU - Miller, D. W.

AU - Morales, A.

AU - Morales, J.

AU - Ortiz, A.

AU - Papaevangelou, T.

AU - Placci, A.

AU - Raffelt, G.

AU - Ruz, J.

AU - Riege, H.

AU - Sarsa, M. L.

AU - Savvidis, I.

AU - Serpico, P.

AU - Semertzidis, Y.

AU - Stewart, L.

AU - Vieira, J. D.

AU - Villar, J.

AU - Walckiers, L.

AU - Zachariadou, K.

AU - Zioutas, K.

N1 - Publisher Copyright: © Copiright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.

PY - 2005

Y1 - 2005

N2 - The CERN Axion Solar Telescope (CAST) is searching for axions produced in the Sun’s core by the Primakoff process. CAST is using a decommissioned Large Hadron Collider (LHC) test magnet where axions could be converted back into X-rays with energies up to 10 keV. Analysis of the 2003 data showed no signal above background implying an upper limit for the axion-photon coupling constant gaγγ < 1.16 × 10−10 GeV−1 at 95% C.L. for ma 0.02 eV [1]. The higher quality 2004 data is presently under analysis. CAST Phase II is scheduled to start in late 2005. This will be the first step in extending CAST’s sensitivity to axion rest masses up to ∼ 1 eV.

AB - The CERN Axion Solar Telescope (CAST) is searching for axions produced in the Sun’s core by the Primakoff process. CAST is using a decommissioned Large Hadron Collider (LHC) test magnet where axions could be converted back into X-rays with energies up to 10 keV. Analysis of the 2003 data showed no signal above background implying an upper limit for the axion-photon coupling constant gaγγ < 1.16 × 10−10 GeV−1 at 95% C.L. for ma 0.02 eV [1]. The higher quality 2004 data is presently under analysis. CAST Phase II is scheduled to start in late 2005. This will be the first step in extending CAST’s sensitivity to axion rest masses up to ∼ 1 eV.

UR - https://www.scopus.com/pages/publications/85056279174

M3 - 会议文章

AN - SCOPUS:85056279174

SN - 1824-8039

VL - 21

JO - Proceedings of Science

JF - Proceedings of Science

Y2 - 21 July 2005 through 27 July 2005

ER -

Search for solar axions: CAST

摘要

其它文件与链接

学术指纹

引用此