First results from the CERN axion solar telescope

K. Zioutas; S. Andriamonje; V. Arsov; S. Aune; D. Autiero; F. T. 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; M. D. Hasinoff; F. H. Heinsius; D. H.H. Hoffmann; G. Irastorza; J. Jacoby; D. Kang; K. Königsmann; R. Kotthaus; M. Krčmar; K. Kousouris; M. Kuster; B. Lakić; C. Lasseur; A. Liolios; A. Ljubičić; G. Lutz; G. Luzón; D. W. Miller; A. Morales; J. Morales; M. Mutterer; A. Nikolaidis; A. Ortiz; T. Papaevangelou; A. Placci; G. Raffelt; J. Ruz; H. Riege; M. L. Sarsa; I. Savvidis; W. Serber; P. Serpico; Y. Semertzidis; L. Stewart; J. D. Vieira; J. Villar; L. Walckiers; K. Zachariadou

doi:10.1103/PhysRevLett.94.121301

First results from the CERN axion solar telescope

K. Zioutas
, S. Andriamonje
, V. Arsov
, S. Aune
, D. Autiero
, F. T. 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, M. D. Hasinoff, F. H. Heinsius, D. H.H. Hoffmann, G. Irastorza, J. Jacoby, D. Kang, K. Königsmann, R. Kotthaus, M. Krčmar, K. Kousouris, M. Kuster, B. Lakić, C. Lasseur, A. Liolios, A. Ljubičić, G. Lutz, G. Luzón, D. W. Miller, A. Morales, J. Morales, M. Mutterer, A. Nikolaidis, A. Ortiz, T. Papaevangelou, A. Placci, G. Raffelt, J. Ruz, H. Riege, M. L. Sarsa, I. Savvidis, W. Serber, P. Serpico, Y. Semertzidis, L. Stewart, J. D. Vieira, J. Villar, L. Walckiers, K. Zachariadou

Aristotle University of Thessaloniki
Centre d'Études de Saclay (CEA-Saclay)
Technische Universität Darmstadt
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
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)
Ruder Boskovic Institute
Brookhaven National Laboratory

科研成果: 期刊稿件 › 文章 › 同行评审

393 引用（Scopus）

摘要

Hypothetical axionlike particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field ("axion helioscope"), they would be transformed into x-rays with energies of a few keV. Using a decommissioned Large Hadron Collider test magnet, the CERN Axion Solar Telescope ran for about 6 months during 2003. The first results from the analysis of these data are presented here. No signal above background was observed, implying an upper limit to the axionphoton coupling g_aγ < 1.16 × 10^-10 GeV^-1 at 95% C.L. for m_a ≲ 0.02 eV. This limit, assumption-free, is comparable to the limit from stellar energy-loss arguments and considerably more restrictive than any previous experiment over a broad range of axion masses.

源语言	英语
期刊论文编号	121301
期刊	Physical Review Letters
卷	94
期	12
DOI	https://doi.org/10.1103/PhysRevLett.94.121301
出版状态	已出版 - 1 4月 2005
已对外发布	是

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10.1103/PhysRevLett.94.121301

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Zioutas, K., Andriamonje, S., Arsov, V., Aune, S., Autiero, D., Avignone, F. T., Barth, K., Belov, A., Beltrán, B., Bräuninger, H., Carmona, J. M., Cebrián, S., Chesi, E., Collar, J. I., Creswick, R., Dafni, T., Davenport, M., Di Lella, L., Eleftheriadis, C., ... Zachariadou, K. (2005). First results from the CERN axion solar telescope. Physical Review Letters, 94(12), 期刊论文 121301. https://doi.org/10.1103/PhysRevLett.94.121301

@article{58dac2b781e94639b3dab2064ec75d34,

title = "First results from the CERN axion solar telescope",

abstract = "Hypothetical axionlike particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field ({"}axion helioscope{"}), they would be transformed into x-rays with energies of a few keV. Using a decommissioned Large Hadron Collider test magnet, the CERN Axion Solar Telescope ran for about 6 months during 2003. The first results from the analysis of these data are presented here. No signal above background was observed, implying an upper limit to the axionphoton coupling gaγ < 1.16 {\texttimes} 10-10 GeV-1 at 95\% C.L. for ma ≲ 0.02 eV. This limit, assumption-free, is comparable to the limit from stellar energy-loss arguments and considerably more restrictive than any previous experiment over a broad range of axion masses.",

author = "K. Zioutas and S. Andriamonje and V. Arsov and S. Aune and D. Autiero and Avignone, \{F. T.\} 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 Hasinoff, \{M. D.\} and Heinsius, \{F. H.\} and Hoffmann, \{D. H.H.\} and G. Irastorza 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 B. Laki{\'c} 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 M. Mutterer and A. Nikolaidis 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 W. Serber and P. Serpico and Y. Semertzidis and L. Stewart and Vieira, \{J. D.\} and J. Villar and L. Walckiers and K. Zachariadou",

year = "2005",

month = apr,

day = "1",

doi = "10.1103/PhysRevLett.94.121301",

language = "英语",

volume = "94",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "12",

}

Zioutas, K, Andriamonje, S, Arsov, V, Aune, S, Autiero, D, Avignone, FT, 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, Hasinoff, MD, Heinsius, FH, Hoffmann, DHH, Irastorza, G, Jacoby, J, Kang, D, Königsmann, K, Kotthaus, R, Krčmar, M, Kousouris, K, Kuster, M, Lakić, B, Lasseur, C, Liolios, A, Ljubičić, A, Lutz, G, Luzón, G, Miller, DW, Morales, A, Morales, J, Mutterer, M, Nikolaidis, A, Ortiz, A, Papaevangelou, T, Placci, A, Raffelt, G, Ruz, J, Riege, H, Sarsa, ML, Savvidis, I, Serber, W, Serpico, P, Semertzidis, Y, Stewart, L, Vieira, JD, Villar, J, Walckiers, L & Zachariadou, K 2005, 'First results from the CERN axion solar telescope', Physical Review Letters, 卷 94, 号码 12, 121301. https://doi.org/10.1103/PhysRevLett.94.121301

TY - JOUR

T1 - First results from the CERN axion solar telescope

AU - Zioutas, K.

AU - Andriamonje, S.

AU - Arsov, V.

AU - Aune, S.

AU - Autiero, D.

AU - Avignone, F. T.

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 - Hasinoff, M. D.

AU - Heinsius, F. H.

AU - Hoffmann, D. H.H.

AU - Irastorza, G.

AU - Jacoby, J.

AU - Kang, D.

AU - Königsmann, K.

AU - Kotthaus, R.

AU - Krčmar, M.

AU - Kousouris, K.

AU - Kuster, M.

AU - Lakić, B.

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 - Mutterer, M.

AU - Nikolaidis, A.

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 - Serber, W.

AU - Serpico, P.

AU - Semertzidis, Y.

AU - Stewart, L.

AU - Vieira, J. D.

AU - Villar, J.

AU - Walckiers, L.

AU - Zachariadou, K.

PY - 2005/4/1

Y1 - 2005/4/1

N2 - Hypothetical axionlike particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field ("axion helioscope"), they would be transformed into x-rays with energies of a few keV. Using a decommissioned Large Hadron Collider test magnet, the CERN Axion Solar Telescope ran for about 6 months during 2003. The first results from the analysis of these data are presented here. No signal above background was observed, implying an upper limit to the axionphoton coupling gaγ < 1.16 × 10-10 GeV-1 at 95% C.L. for ma ≲ 0.02 eV. This limit, assumption-free, is comparable to the limit from stellar energy-loss arguments and considerably more restrictive than any previous experiment over a broad range of axion masses.

AB - Hypothetical axionlike particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field ("axion helioscope"), they would be transformed into x-rays with energies of a few keV. Using a decommissioned Large Hadron Collider test magnet, the CERN Axion Solar Telescope ran for about 6 months during 2003. The first results from the analysis of these data are presented here. No signal above background was observed, implying an upper limit to the axionphoton coupling gaγ < 1.16 × 10-10 GeV-1 at 95% C.L. for ma ≲ 0.02 eV. This limit, assumption-free, is comparable to the limit from stellar energy-loss arguments and considerably more restrictive than any previous experiment over a broad range of axion masses.

UR - https://www.scopus.com/pages/publications/18244395576

U2 - 10.1103/PhysRevLett.94.121301

DO - 10.1103/PhysRevLett.94.121301

M3 - 文章

AN - SCOPUS:18244395576

SN - 0031-9007

VL - 94

JO - Physical Review Letters

JF - Physical Review Letters

IS - 12

M1 - 121301

ER -

First results from the CERN axion solar telescope

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