The IAXO Helioscope

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ID: 115046
2015
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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.
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Authors 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,Theopisti Dafni,M Davenport,A. V. Derbin,K Desch,A Diago,B Döbrich,I Dratchnev,A Dudarev,C Eleftheriadis,G. Fanourakis,Javier Galán,J A García,J G Garza,T. Geralis,B Gimeno,I Giomataris,S Gninenko,H. Gómez,D Gonzalez-Diaz,Eduardo I. Guendelman,C J. Hailey,T Hiramatsu,D.H.H. Hoffmann,D. Horns,F.J. Iguaz,I G Irastorza,J. Isern,K Imai,J Jaeckel,Anders C. Jakobsen,K. Jakovčić,J Kaminski,M Kawasaki,Marin Karuza,M. Krčmar,K. Kousouris,Christoph Krieger,B. Lakić,O. Limousin,A Lindner,A Liolios,G. Luzón,S. Matsuki,V N Muratova,C Nones,I Ortega,Thomas 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 Tomàs,S. Troitsky,T Vafeiadis,K Van Bibber,P Védrine,J.A. Villar,J. K. Vogel,L Walckiers,A Weltman,W Wester,S C. Yildiz,Konstantin Zioutas;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;Theopisti Dafni;M Davenport;A. V. Derbin;K Desch;A Diago;B Döbrich;I Dratchnev;A Dudarev;C Eleftheriadis;G. Fanourakis;Javier Galán;J A García;J G Garza;T. Geralis;B Gimeno;I Giomataris;S Gninenko;H. Gómez;D Gonzalez-Diaz;Eduardo I. Guendelman;C J. Hailey;T Hiramatsu;D.H.H. Hoffmann;D. Horns;F.J. Iguaz;I G Irastorza;J. Isern;K Imai;J Jaeckel;Anders C. Jakobsen;K. Jakovčić;J Kaminski;M Kawasaki;Marin Karuza;M. Krčmar;K. Kousouris;Christoph Krieger;B. Lakić;O. Limousin;A Lindner;A Liolios;G. Luzón;S. Matsuki;V N Muratova;C Nones;I Ortega;Thomas 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 Tomàs;S. Troitsky;T Vafeiadis;K Van Bibber;P Védrine;J.A. Villar;J. K. Vogel;L Walckiers;A Weltman;W Wester;S C. Yildiz;Konstantin Zioutas;
Journal journal of physics: conference series
Year 2015
DOI
10.1088/1742-6596/650/1/012009
URL
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