IAXO - The International Axion Observatory

J. K. Vogel; F. T. Avignone; G. Cantatore; J. M. Carmona; S. Caspi; S. A. Cetin; F. E. Christensen; A. Dael; T. Dafni; M. Davenport; A. V. Derbin; K. Desch; A. Diago; A. Dudarev; C. Eleftheriadis; G. Fanourakis; E. Ferrer-Ribas; J. Galán; J. A. García; J. G. Garza; T. Geralis; B. Gimeno; I. Giomataris; S. Gninenko; H. Gómez; C. J. Hailey; T. Hiramatsu; D. H.H. Hoffmann; F. J. Iguaz; I. G. Irastorza; J. Isern; J. Jaeckel; K. Jakovčić; J. Kaminski; M. Kawasaki; M. Krčmar; C. Krieger; B. Lakić; A. Lindner; A. Liolios; G. Luzón; I. Ortega; T. Papaevangelou; M. J. Pivovaroff; G. Raffelt; J. Redondo; A. Ringwald; S. Russenschuck; J. Ruz; K. Saikawa; I. Savvidis; T. Sekiguchi; I. Shilon; H. Silva; H. H.J. ten Kate; A. Tomas; S. Troitsky; K. van Bibber; P. Vedrine; J. A. Villar; L. Walckiers; W. Wester; S. C. Yildiz; K. Zioutas

IAXO - The International Axion Observatory

J. K. Vogel
, F. T. Avignone
, G. Cantatore
, J. M. Carmona
, S. Caspi
, S. A. Cetin
, F. E. Christensen
, A. Dael
, T. Dafni
, M. Davenport
, A. V. Derbin
, K. Desch
, A. Diago
, A. Dudarev
, C. Eleftheriadis
, G. Fanourakis
, E. Ferrer-Ribas
, J. Galán
, J. A. García
, J. G. Garza

T. Geralis, B. Gimeno, I. Giomataris, S. Gninenko, H. Gómez, C. J. Hailey, T. Hiramatsu, D. H.H. Hoffmann, F. J. Iguaz, I. G. Irastorza, J. Isern, J. Jaeckel, K. Jakovčić, J. Kaminski, M. Kawasaki, M. Krčmar, C. Krieger, B. Lakić, A. Lindner, A. Liolios, G. Luzón, I. Ortega, T. Papaevangelou, M. J. Pivovaroff, G. Raffelt, J. Redondo, A. Ringwald, S. Russenschuck, J. Ruz, K. Saikawa, I. Savvidis, T. Sekiguchi, I. Shilon, H. Silva, H. H.J. ten Kate, A. Tomas, S. Troitsky, K. van Bibber, P. Vedrine, J. A. Villar, L. Walckiers, W. Wester, S. C. Yildiz, K. Zioutas

Chem./Materials Science Directorate
University of South Carolina
University of Trieste
University of Zaragoza
LBL
Dogus University
Technical University of Denmark
Centre d' Etudes Nucléaires de Saclay (CEA-Saclay)
CERN
St. Petersburg Nuclear Physics Institute
University of Bonn
Aristotle University of Thessaloniki
Demokritos National Centre for Scientific Research
University of Valencia
Russian Academy of Sciences
Columbia University
Kyoto University
Technische Universität Darmstadt
Facultat de Ciències
Heidelberg University
Ruder Boskovic Institute
The University of Tokyo
German Electron Synchrotron
Max Planck Institute for Physics (Werner Heisenberg Institute)
University of California at Berkeley
Fermi National Accelerator Laboratory
University of Patras

科研成果: 书/报告/会议事项章节 › 会议稿件 › 同行评审

6 引用（Scopus）

摘要

The International Axion Observatory (IAXO) is a next generation axion helioscope aiming at a sensitivity to the axion-photon coupling of a few 10⁻¹² GeV⁻¹, i.e. 1-1.5 orders of magnitude beyond sensitivities achieved by the currently most sensitive axion helioscope, the CERN Axion Solar Telescope (CAST). Crucial factors in improving the sensitivity for IAXO are the increase of the magnetic field volume together with the extensive use of x-ray focusing optics and low background detectors, innovations already successfully tested at CAST. Electron-coupled axions invoked to explain the white dwarf cooling, relic axions, and a large variety of more generic axion-like particles (ALPs) along with other novel excitations at the low-energy frontier of elementary particle physics could provide additional physics motivation for IAXO.

源语言	英语
主期刊名	8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012
出版商	Deutsches Elektronen-Synchrotron (DESY)
ISBN（电子版）	9783935702690
出版状态	已出版 - 2012
已对外发布	是
活动	8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012 - Chicago, 美国期限: 18 7月 2012 → 22 7月 2012

出版系列

姓名	8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012

会议

会议	8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012
国家/地区	美国
市	Chicago
时期	18/07/12 → 22/07/12

其它文件与链接

链接到 Scopus 的出版物

引用此

Vogel, J. K., Avignone, F. T., Cantatore, G., Carmona, J. M., Caspi, S., Cetin, S. A., Christensen, F. E., Dael, A., Dafni, T., Davenport, M., Derbin, A. V., Desch, K., Diago, A., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer-Ribas, E., Galán, J., García, J. A., ... Zioutas, K. (2012). IAXO - The International Axion Observatory. 在 8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012 (8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012). Deutsches Elektronen-Synchrotron (DESY).

@inproceedings{b2e1af00ac5d4ec4aed1d4a2f26fdaf3,

title = "IAXO - The International Axion Observatory",

abstract = "The International Axion Observatory (IAXO) is a next generation axion helioscope aiming at a sensitivity to the axion-photon coupling of a few 10−12 GeV−1, i.e. 1-1.5 orders of magnitude beyond sensitivities achieved by the currently most sensitive axion helioscope, the CERN Axion Solar Telescope (CAST). Crucial factors in improving the sensitivity for IAXO are the increase of the magnetic field volume together with the extensive use of x-ray focusing optics and low background detectors, innovations already successfully tested at CAST. Electron-coupled axions invoked to explain the white dwarf cooling, relic axions, and a large variety of more generic axion-like particles (ALPs) along with other novel excitations at the low-energy frontier of elementary particle physics could provide additional physics motivation for IAXO.",

author = "Vogel, \{J. K.\} and Avignone, \{F. T.\} and G. Cantatore and Carmona, \{J. M.\} and S. Caspi and Cetin, \{S. A.\} and Christensen, \{F. E.\} and A. Dael and T. Dafni and M. Davenport and Derbin, \{A. V.\} and K. Desch and A. Diago and A. Dudarev and C. Eleftheriadis and G. Fanourakis and E. Ferrer-Ribas and J. Gal{\'a}n and Garc{\'i}a, \{J. A.\} and Garza, \{J. G.\} and T. Geralis and B. Gimeno and I. Giomataris and S. Gninenko and H. G{\'o}mez and Hailey, \{C. J.\} and T. Hiramatsu and Hoffmann, \{D. H.H.\} and Iguaz, \{F. J.\} and Irastorza, \{I. G.\} and J. Isern and J. Jaeckel and K. Jakov{\v c}i{\'c} and J. Kaminski and M. Kawasaki and M. Kr{\v c}mar and C. Krieger and B. Laki{\'c} and A. Lindner and A. Liolios and G. Luz{\'o}n and I. Ortega and T. Papaevangelou and Pivovaroff, \{M. J.\} and G. Raffelt and J. Redondo and A. Ringwald and S. Russenschuck and J. Ruz and K. Saikawa and I. Savvidis and T. Sekiguchi and I. Shilon and H. Silva and \{ten Kate\}, \{H. H.J.\} and A. Tomas and S. Troitsky and \{van Bibber\}, K. and P. Vedrine and Villar, \{J. A.\} and L. Walckiers and W. Wester and Yildiz, \{S. C.\} and K. Zioutas",

note = "Publisher Copyright: {\textcopyright} 2012 8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012. All Rights Reserved.; 8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012 ; Conference date: 18-07-2012 Through 22-07-2012",

year = "2012",

language = "英语",

series = "8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012",

publisher = "Deutsches Elektronen-Synchrotron (DESY)",

booktitle = "8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012",

}

Vogel, JK, Avignone, FT, Cantatore, G, Carmona, JM, Caspi, S, Cetin, SA, Christensen, FE, Dael, A, Dafni, T, Davenport, M, Derbin, AV, Desch, K, Diago, A, Dudarev, A, Eleftheriadis, C, Fanourakis, G, Ferrer-Ribas, E, Galán, J, García, JA, Garza, JG, Geralis, T, Gimeno, B, Giomataris, I, Gninenko, S, Gómez, H, Hailey, CJ, Hiramatsu, T, Hoffmann, DHH, Iguaz, FJ, Irastorza, IG, Isern, J, Jaeckel, J, Jakovčić, K, Kaminski, J, Kawasaki, M, Krčmar, M, Krieger, C, Lakić, B, Lindner, A, Liolios, A, Luzón, G, Ortega, I, Papaevangelou, T, Pivovaroff, MJ, Raffelt, G, Redondo, J, Ringwald, A, Russenschuck, S, Ruz, J, Saikawa, K, Savvidis, I, Sekiguchi, T, Shilon, I, Silva, H, ten Kate, HHJ, Tomas, A, Troitsky, S, van Bibber, K, Vedrine, P, Villar, JA, Walckiers, L, Wester, W, Yildiz, SC & Zioutas, K 2012, IAXO - The International Axion Observatory. 在 8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012. 8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012, Deutsches Elektronen-Synchrotron (DESY), 8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012, Chicago, 美国, 18/07/12.

TY - GEN

T1 - IAXO - The International Axion Observatory

AU - Vogel, J. K.

AU - Avignone, F. T.

AU - Cantatore, G.

AU - Carmona, J. M.

AU - Caspi, S.

AU - Cetin, S. A.

AU - Christensen, F. E.

AU - Dael, A.

AU - Dafni, T.

AU - Davenport, M.

AU - Derbin, A. V.

AU - Desch, K.

AU - Diago, A.

AU - Dudarev, A.

AU - Eleftheriadis, C.

AU - Fanourakis, G.

AU - Ferrer-Ribas, E.

AU - Galán, J.

AU - García, J. A.

AU - Garza, J. G.

AU - Geralis, T.

AU - Gimeno, B.

AU - Giomataris, I.

AU - Gninenko, S.

AU - Gómez, H.

AU - Hailey, C. J.

AU - Hiramatsu, T.

AU - Hoffmann, D. H.H.

AU - Iguaz, F. J.

AU - Irastorza, I. G.

AU - Isern, J.

AU - Jaeckel, J.

AU - Jakovčić, K.

AU - Kaminski, J.

AU - Kawasaki, M.

AU - Krčmar, M.

AU - Krieger, C.

AU - Lakić, B.

AU - Lindner, A.

AU - Liolios, A.

AU - Luzón, G.

AU - Ortega, I.

AU - Papaevangelou, T.

AU - Pivovaroff, M. J.

AU - Raffelt, G.

AU - Redondo, J.

AU - Ringwald, A.

AU - Russenschuck, S.

AU - Ruz, J.

AU - Saikawa, K.

AU - Savvidis, I.

AU - Sekiguchi, T.

AU - Shilon, I.

AU - Silva, H.

AU - ten Kate, H. H.J.

AU - Tomas, A.

AU - Troitsky, S.

AU - van Bibber, K.

AU - Vedrine, P.

AU - Villar, J. A.

AU - Walckiers, L.

AU - Wester, W.

AU - Yildiz, S. C.

AU - Zioutas, K.

PY - 2012

Y1 - 2012

N2 - The International Axion Observatory (IAXO) is a next generation axion helioscope aiming at a sensitivity to the axion-photon coupling of a few 10−12 GeV−1, i.e. 1-1.5 orders of magnitude beyond sensitivities achieved by the currently most sensitive axion helioscope, the CERN Axion Solar Telescope (CAST). Crucial factors in improving the sensitivity for IAXO are the increase of the magnetic field volume together with the extensive use of x-ray focusing optics and low background detectors, innovations already successfully tested at CAST. Electron-coupled axions invoked to explain the white dwarf cooling, relic axions, and a large variety of more generic axion-like particles (ALPs) along with other novel excitations at the low-energy frontier of elementary particle physics could provide additional physics motivation for IAXO.

AB - The International Axion Observatory (IAXO) is a next generation axion helioscope aiming at a sensitivity to the axion-photon coupling of a few 10−12 GeV−1, i.e. 1-1.5 orders of magnitude beyond sensitivities achieved by the currently most sensitive axion helioscope, the CERN Axion Solar Telescope (CAST). Crucial factors in improving the sensitivity for IAXO are the increase of the magnetic field volume together with the extensive use of x-ray focusing optics and low background detectors, innovations already successfully tested at CAST. Electron-coupled axions invoked to explain the white dwarf cooling, relic axions, and a large variety of more generic axion-like particles (ALPs) along with other novel excitations at the low-energy frontier of elementary particle physics could provide additional physics motivation for IAXO.

UR - https://www.scopus.com/pages/publications/85183857464

M3 - 会议稿件

AN - SCOPUS:85183857464

T3 - 8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012

BT - 8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012

PB - Deutsches Elektronen-Synchrotron (DESY)

T2 - 8th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2012

Y2 - 18 July 2012 through 22 July 2012

ER -

IAXO - The International Axion Observatory

摘要

出版系列

会议

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学术指纹

引用此