The IAXO Helioscope

E. Ferrer Ribas; E. Armengaud; F. T. Avignone; M. Betz; P. Brax; P. Brun; G. Cantatore; J. M. Carmona; G. P. Carosi; F. Caspers; S. Caspi; S. A. Cetin; D. Chelouche; F. E. Christensen; A. Dael; T. Dafni; M. Davenport; A. V. Derbin; K. Desch; A. Diago; B. Döbrich; I. Dratchnev; A. Dudarev; C. Eleftheriadis; G. Fanourakis; J. Galán; J. A. García; J. G. Garza; T. Geralis; B. Gimeno; I. Giomataris; S. Gninenko; H. Gómez; D. González-Diaz; E. Guendelman; C. J. Hailey; T. Hiramatsu; D. H.H. Hoffmann; D. Horns; F. J. Iguaz; I. G. Irastorza; J. Isern; K. Imai; J. Jaeckel; A. C. Jakobsen; K. Jakovčić; J. Kaminski; M. Kawasaki; M. Karuza; M. Krčmar; K. Kousouris; C. Krieger; B. Lakić; O. Limousin; A. Lindner; A. Liolios; G. Luzón; S. Matsuki; V. N. Muratova; C. Nones; I. Ortega; T. Papaevangelou; M. J. Pivovaroff; G. Raffelt; J. Redondo; A. Ringwald; S. Russenschuck; J. Ruz; K. Saikawa; I. Savvidis; T. Sekiguchi; Y. K. Semertzidis; I. Shilon; P. Sikivie; H. Silva; H. H.J. Ten Kate; A. Tomas; S. Troitsky; T. Vafeiadis; K. Van Bibber; P. Vedrine; J. A. Villar; J. K. Vogel; L. Walckiers; A. Weltman; W. Wester; S. C. Yildiz; K. Zioutas

doi:10.1088/1742-6596/650/1/012009

The IAXO Helioscope

E. Ferrer Ribas
, E. Armengaud
, F. T. Avignone
, M. Betz
, P. Brax
, P. Brun
, G. Cantatore
, J. M. Carmona
, G. P. Carosi
, F. Caspers
, S. Caspi
, S. A. Cetin
, D. Chelouche
, F. E. Christensen
, A. Dael
, T. Dafni
, M. Davenport
, A. V. Derbin
, K. Desch
, A. Diago

B. Döbrich, I. Dratchnev, A. Dudarev, C. Eleftheriadis, G. Fanourakis, J. Galán, J. A. García, J. G. Garza, T. Geralis, B. Gimeno, I. Giomataris, S. Gninenko, H. Gómez, D. González-Diaz, E. Guendelman, C. J. Hailey, T. Hiramatsu, D. H.H. Hoffmann, D. Horns, F. J. Iguaz, I. G. Irastorza, J. Isern, K. Imai, J. Jaeckel, A. C. Jakobsen, K. Jakovčić, J. Kaminski, M. Kawasaki, M. Karuza, M. Krčmar, K. Kousouris, C. Krieger, B. Lakić, O. Limousin, A. Lindner, A. Liolios, G. Luzón, S. Matsuki, V. N. Muratova, C. Nones, I. Ortega, T. Papaevangelou, M. J. Pivovaroff, G. Raffelt, J. Redondo, A. Ringwald, S. Russenschuck, J. Ruz, K. Saikawa, I. Savvidis, T. Sekiguchi, Y. K. Semertzidis, I. Shilon, P. Sikivie, H. Silva, H. H.J. Ten Kate, A. Tomas, S. Troitsky, T. Vafeiadis, K. Van Bibber, P. Vedrine, J. A. Villar, J. K. Vogel, L. Walckiers, A. Weltman, W. Wester, S. C. Yildiz, K. Zioutas

Centre d' Etudes Nucléaires de Saclay (CEA-Saclay)
University of South Carolina
CERN
Centre d'Études de Saclay (CEA-Saclay)
University of Trieste
University of Zaragoza
Chem./Materials Science Directorate
LBL
Dogus University
University of Haifa
Technical University of Denmark
St. Petersburg Nuclear Physics Institute
University of Bonn
German Electron Synchrotron
Aristotle University of Thessaloniki
Demokritos National Centre for Scientific Research
University of Valencia
Russian Academy of Sciences
Ben-Gurion University of the Negev
Columbia University
Kyoto University
Technische Universität Darmstadt
University of Hamburg
Facultat de Ciències
Japan Atomic Energy Agency
Heidelberg University
Ruder Boskovic Institute
The University of Tokyo
University of Rijeka
Max Planck Institute for Physics (Werner Heisenberg Institute)
Korea Advanced Institute of Science and Technology
University of Florida
University of California at Berkeley
University of Cape Town
Fermi National Accelerator Laboratory
University of Patras

Research output: Contribution to journal › Conference article › peer-review

3 Scopus citations

Abstract

The IAXO (International Axion Experiment) is a fourth generation helioscope with a sensitivity, in terms of detectable signal counts, at least 10⁴ better than CAST phase-I, resulting in sensitivity on g_aγ one order of magnitude better. To achieve this performance IAXO will count on a 8-coil toroidal magnet with 60 cm diameter bores and equipped with X-ray focusing optics into 0.20 cm² spots coupled to ultra-low background Micromegas X-ray detectors. The magnet will be on a platform that will allow solar tracking for 12 hours per day. The next short term objectives are to prepare a Technical Design Report and to construct the first prototypes of the hardware main ingredients: demonstration coil, X-ray optics and low background detector while refining the physics case and studying the feasibility studies for Dark Matter axions.

Original language	English
Article number	012009
Journal	Journal of Physics: Conference Series
Volume	650
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/650/1/012009
State	Published - 16 Nov 2015
Externally published	Yes
Event	7th International Symposium on Large TPCs for Low-Energy Rare Event Detection - Paris, France Duration: 15 Dec 2014 → 17 Dec 2014

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10.1088/1742-6596/650/1/012009

Cite this

Ribas, E. F., Armengaud, E., Avignone, F. T., Betz, M., Brax, P., Brun, P., Cantatore, G., Carmona, J. M., Carosi, G. P., Caspers, F., Caspi, S., Cetin, S. A., Chelouche, D., Christensen, F. E., Dael, A., Dafni, T., Davenport, M., Derbin, A. V., Desch, K., ... Zioutas, K. (2015). The IAXO Helioscope. Journal of Physics: Conference Series, 650(1), Article 012009. https://doi.org/10.1088/1742-6596/650/1/012009

@article{f73d602cd1234fe7aed23ad17a03390f,

title = "The IAXO Helioscope",

abstract = "The IAXO (International Axion Experiment) is a fourth generation helioscope with a sensitivity, in terms of detectable signal counts, at least 104 better than CAST phase-I, resulting in sensitivity on gaγ one order of magnitude better. To achieve this performance IAXO will count on a 8-coil toroidal magnet with 60 cm diameter bores and equipped with X-ray focusing optics into 0.20 cm2 spots coupled to ultra-low background Micromegas X-ray detectors. The magnet will be on a platform that will allow solar tracking for 12 hours per day. The next short term objectives are to prepare a Technical Design Report and to construct the first prototypes of the hardware main ingredients: demonstration coil, X-ray optics and low background detector while refining the physics case and studying the feasibility studies for Dark Matter axions.",

author = "Ribas, \{E. Ferrer\} and E. Armengaud and Avignone, \{F. T.\} and M. Betz and P. Brax and P. Brun and G. Cantatore and Carmona, \{J. M.\} and Carosi, \{G. P.\} and F. Caspers and S. Caspi and Cetin, \{S. A.\} and D. Chelouche and Christensen, \{F. E.\} and A. Dael and T. Dafni and M. Davenport and Derbin, \{A. V.\} and K. Desch and A. Diago and B. D{\"o}brich and I. Dratchnev and A. Dudarev and C. Eleftheriadis and G. Fanourakis 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 D. Gonz{\'a}lez-Diaz and E. Guendelman and Hailey, \{C. J.\} and T. Hiramatsu and Hoffmann, \{D. H.H.\} and D. Horns and Iguaz, \{F. J.\} and Irastorza, \{I. G.\} and J. Isern and K. Imai and J. Jaeckel and Jakobsen, \{A. C.\} and K. Jakov{\v c}i{\'c} and J. Kaminski and M. Kawasaki and M. Karuza and M. Kr{\v c}mar and K. Kousouris and C. Krieger and B. Laki{\'c} and O. Limousin and A. Lindner and A. Liolios and G. Luz{\'o}n and S. Matsuki and Muratova, \{V. N.\} and C. Nones 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 Semertzidis, \{Y. K.\} and I. Shilon and P. Sikivie and H. Silva and \{Ten Kate\}, \{H. H.J.\} and A. Tomas and S. Troitsky and T. Vafeiadis and \{Van Bibber\}, K. and P. Vedrine and Villar, \{J. A.\} and Vogel, \{J. K.\} and L. Walckiers and A. Weltman and W. Wester and Yildiz, \{S. C.\} and K. Zioutas",

note = "Publisher Copyright: {\textcopyright} Published under licence by IOP Publishing Ltd.; 7th International Symposium on Large TPCs for Low-Energy Rare Event Detection ; Conference date: 15-12-2014 Through 17-12-2014",

year = "2015",

month = nov,

day = "16",

doi = "10.1088/1742-6596/650/1/012009",

language = "英语",

volume = "650",

journal = "Journal of Physics: Conference Series",

issn = "1742-6588",

publisher = "IOP Publishing Ltd.",

number = "1",

}

Ribas, EF, Armengaud, E, Avignone, FT, Betz, M, Brax, P, Brun, P, Cantatore, G, Carmona, JM, Carosi, GP, Caspers, F, Caspi, S, Cetin, SA, Chelouche, D, Christensen, FE, Dael, A, Dafni, T, Davenport, M, Derbin, AV, Desch, K, Diago, A, Döbrich, B, Dratchnev, I, Dudarev, A, Eleftheriadis, C, Fanourakis, G, Galán, J, García, JA, Garza, JG, Geralis, T, Gimeno, B, Giomataris, I, Gninenko, S, Gómez, H, González-Diaz, D, Guendelman, E, Hailey, CJ, Hiramatsu, T, Hoffmann, DHH, Horns, D, Iguaz, FJ, Irastorza, IG, Isern, J, Imai, K, Jaeckel, J, Jakobsen, AC, Jakovčić, K, Kaminski, J, Kawasaki, M, Karuza, M, Krčmar, M, Kousouris, K, Krieger, C, Lakić, B, Limousin, O, Lindner, A, Liolios, A, Luzón, G, Matsuki, S, Muratova, VN, Nones, C, Ortega, I, Papaevangelou, T, Pivovaroff, MJ, Raffelt, G, Redondo, J, Ringwald, A, Russenschuck, S, Ruz, J, Saikawa, K, Savvidis, I, Sekiguchi, T, Semertzidis, YK, Shilon, I, Sikivie, P, Silva, H, Ten Kate, HHJ, Tomas, A, Troitsky, S, Vafeiadis, T, Van Bibber, K, Vedrine, P, Villar, JA, Vogel, JK, Walckiers, L, Weltman, A, Wester, W, Yildiz, SC & Zioutas, K 2015, 'The IAXO Helioscope', Journal of Physics: Conference Series, vol. 650, no. 1, 012009. https://doi.org/10.1088/1742-6596/650/1/012009

TY - JOUR

T1 - The IAXO Helioscope

AU - Ribas, E. Ferrer

AU - Armengaud, E.

AU - Avignone, F. T.

AU - Betz, M.

AU - Brax, P.

AU - Brun, P.

AU - Cantatore, G.

AU - Carmona, J. M.

AU - Carosi, G. P.

AU - Caspers, F.

AU - Caspi, S.

AU - Cetin, S. A.

AU - Chelouche, D.

AU - Christensen, F. E.

AU - Dael, A.

AU - Dafni, T.

AU - Davenport, M.

AU - Derbin, A. V.

AU - Desch, K.

AU - Diago, A.

AU - Döbrich, B.

AU - Dratchnev, I.

AU - Dudarev, A.

AU - Eleftheriadis, C.

AU - Fanourakis, G.

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 - González-Diaz, D.

AU - Guendelman, E.

AU - Hailey, C. J.

AU - Hiramatsu, T.

AU - Hoffmann, D. H.H.

AU - Horns, D.

AU - Iguaz, F. J.

AU - Irastorza, I. G.

AU - Isern, J.

AU - Imai, K.

AU - Jaeckel, J.

AU - Jakobsen, A. C.

AU - Jakovčić, K.

AU - Kaminski, J.

AU - Kawasaki, M.

AU - Karuza, M.

AU - Krčmar, M.

AU - Kousouris, K.

AU - Krieger, C.

AU - Lakić, B.

AU - Limousin, O.

AU - Lindner, A.

AU - Liolios, A.

AU - Luzón, G.

AU - Matsuki, S.

AU - Muratova, V. N.

AU - Nones, C.

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 - Semertzidis, Y. K.

AU - Shilon, I.

AU - Sikivie, P.

AU - Silva, H.

AU - Ten Kate, H. H.J.

AU - Tomas, A.

AU - Troitsky, S.

AU - Vafeiadis, T.

AU - Van Bibber, K.

AU - Vedrine, P.

AU - Villar, J. A.

AU - Vogel, J. K.

AU - Walckiers, L.

AU - Weltman, A.

AU - Wester, W.

AU - Yildiz, S. C.

AU - Zioutas, K.

PY - 2015/11/16

Y1 - 2015/11/16

N2 - The IAXO (International Axion Experiment) is a fourth generation helioscope with a sensitivity, in terms of detectable signal counts, at least 104 better than CAST phase-I, resulting in sensitivity on gaγ one order of magnitude better. To achieve this performance IAXO will count on a 8-coil toroidal magnet with 60 cm diameter bores and equipped with X-ray focusing optics into 0.20 cm2 spots coupled to ultra-low background Micromegas X-ray detectors. The magnet will be on a platform that will allow solar tracking for 12 hours per day. The next short term objectives are to prepare a Technical Design Report and to construct the first prototypes of the hardware main ingredients: demonstration coil, X-ray optics and low background detector while refining the physics case and studying the feasibility studies for Dark Matter axions.

AB - The IAXO (International Axion Experiment) is a fourth generation helioscope with a sensitivity, in terms of detectable signal counts, at least 104 better than CAST phase-I, resulting in sensitivity on gaγ one order of magnitude better. To achieve this performance IAXO will count on a 8-coil toroidal magnet with 60 cm diameter bores and equipped with X-ray focusing optics into 0.20 cm2 spots coupled to ultra-low background Micromegas X-ray detectors. The magnet will be on a platform that will allow solar tracking for 12 hours per day. The next short term objectives are to prepare a Technical Design Report and to construct the first prototypes of the hardware main ingredients: demonstration coil, X-ray optics and low background detector while refining the physics case and studying the feasibility studies for Dark Matter axions.

UR - https://www.scopus.com/pages/publications/84957837713

U2 - 10.1088/1742-6596/650/1/012009

DO - 10.1088/1742-6596/650/1/012009

M3 - 会议文章

AN - SCOPUS:84957837713

SN - 1742-6588

VL - 650

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - 1

M1 - 012009

T2 - 7th International Symposium on Large TPCs for Low-Energy Rare Event Detection

Y2 - 15 December 2014 through 17 December 2014

ER -

The IAXO Helioscope

Abstract

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