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1. New solar axion search using the CERN Axion Solar Telescope withHe4filling

Author

M. Arik, S. Aune, K. Barth, A. Belov, H. Bräuninger, J. Bremer, V. Burwitz, G. Cantatore, J. M. Carmona, S. A. Cetin, J. I. Collar, E. Da Riva, T. Dafni, M. Davenport, A. Dermenev, C. Eleftheriadis, N. Elias, G. Fanourakis, E. Ferrer-Ribas, J. Galán, J. A. García, A. Gardikiotis, J. G. Garza, E. N. Gazis, T. Geralis, E. Georgiopoulou, I. Giomataris, S. Gninenko, M. Gómez Marzoa, M. D. Hasinoff, D. H. H. Hoffmann, F. J. Iguaz, I. G. Irastorza, J. Jacoby, K. Jakovčić, M. Karuza, M. Kavuk, M. Krčmar, M. Kuster, B. Lakić, J. M. Laurent, A. Liolios, A. Ljubičić, G. Luzón, S. Neff, T. Niinikoski, A. Nordt, I. Ortega, T. Papaevangelou, M. J. Pivovaroff, G. Raffelt, A. Rodríguez, M. Rosu, J. Ruz, I. Savvidis, I. Shilon, S. K. Solanki, L. Stewart, A. Tomás, T. Vafeiadis, J. Villar, J. K. Vogel, S. C. Yildiz, and K. Zioutas

Published
2015
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2. Search for Solar Axions by the CERN Axion Solar Telescope withHe3Buffer Gas: Closing the Hot Dark Matter Gap

Author

M. Arik, S. Aune, K. Barth, A. Belov, S. Borghi, H. Bräuninger, G. Cantatore, J. M. Carmona, S. A. Cetin, J. I. Collar, E. Da Riva, T. Dafni, M. Davenport, C. Eleftheriadis, N. Elias, G. Fanourakis, E. Ferrer-Ribas, P. Friedrich, J. Galán, J. A. García, A. Gardikiotis, J. G. Garza, E. N. Gazis, T. Geralis, E. Georgiopoulou, I. Giomataris, S. Gninenko, H. Gómez, M. Gómez Marzoa, E. Gruber, T. Guthörl, R. Hartmann, S. Hauf, F. Haug, M. D. Hasinoff, D. H. H. Hoffmann, F. J. Iguaz, I. G. Irastorza, J. Jacoby, K. Jakovčić, M. Karuza, K. Königsmann, R. Kotthaus, M. Krčmar, M. Kuster, B. Lakić, P. M. Lang, J. M. Laurent, A. Liolios, A. Ljubičić, G. Luzón, S. Neff, T. Niinikoski, A. Nordt, T. Papaevangelou, M. J. Pivovaroff, G. Raffelt, H. Riege, A. Rodríguez, M. Rosu, J. Ruz, I. Savvidis, I. Shilon, P. S. Silva, S. K. Solanki, L. Stewart, A. Tomás, M. Tsagri, K. van Bibber, T. Vafeiadis, J. Villar, J. K. Vogel, S. C. Yildiz, and K. Zioutas

Published
2014
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3. Search for Sub-eV Mass Solar Axions by the CERN Axion Solar Telescope withHe3Buffer Gas

Author

M. Arik, S. Aune, K. Barth, A. Belov, S. Borghi, H. Bräuninger, G. Cantatore, J. M. Carmona, S. A. Cetin, J. I. Collar, T. Dafni, M. Davenport, C. Eleftheriadis, N. Elias, C. Ezer, G. Fanourakis, E. Ferrer-Ribas, P. Friedrich, J. Galán, J. A. García, A. Gardikiotis, E. N. Gazis, T. Geralis, I. Giomataris, S. Gninenko, H. Gómez, E. Gruber, T. Guthörl, R. Hartmann, F. Haug, M. D. Hasinoff, D. H. H. Hoffmann, F. J. Iguaz, I. G. Irastorza, J. Jacoby, K. Jakovčić, M. Karuza, K. Königsmann, R. Kotthaus, M. Krčmar, M. Kuster, B. Lakić, J. M. Laurent, A. Liolios, A. Ljubičić, V. Lozza, G. Lutz, G. Luzón, J. Morales, T. Niinikoski, A. Nordt, T. Papaevangelou, M. J. Pivovaroff, G. Raffelt, T. Rashba, H. Riege, A. Rodríguez, M. Rosu, J. Ruz, I. Savvidis, P. S. Silva, S. K. Solanki, L. Stewart, A. Tomás, M. Tsagri, K. van Bibber, T. Vafeiadis, J. A. Villar, J. K. Vogel, S. C. Yildiz, and K. Zioutas

Published
2011
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4. First Results on the Search for Chameleons with the KWISP Detector at CAST

Author

C. Krieger, Sami K. Solanki, K. Barth, B. Döbrich, S. Neff, Michael J. Pivovaroff, J. Castel, A. Belov, I. Tsagris, E. Ruiz Chóliz, Marc Schumann, A. Ozbey, A. V. Dermenev, A. Bayirli, L. Stewart, S. C. Yildiz, J. Ruz, J. G. Garza, L. Miceli, Serkant Ali Cetin, S. Arguedas Cuendis, T. Dafni, Giovanni Cantatore, J. M. Laurent, F.J. Iguaz, T. Vafeiadis, J. M. Carmona, Klaus Kurt Desch, I. G. Irastorza, M. Maroudas, M. D. Hasinoff, S. N. Gninenko, Biljana Lakić, I. Ortega, H. Bräuninger, M. Vretenar, Konstantin Zioutas, Søren Schmidt, Marin Karuza, Sebastian Baum, Julia Vogel, G. Luzón, A. Gardikiotis, Yannis K. Semertzidis, J. Baier, M. Davenport, Krešimir Jakovčić, M. Rosu, H. Fischer, Wolfgang Funk, J. A. García, Dieter Hoffmann, J. Kaminski, Arguedas Cuendis, S., Baier, J., Barth, K., Baum, S., Bayirli, A., Belov, A., Brauninger, H., Cantatore, G., Carmona, J. M., Castel, J. F., Cetin, S. A., Dafni, T., Davenport, M., Dermenev, A., Desch, K., Dobrich, B., Fischer, H., Funk, W., Garcia, J. A., Gardikiotis, A., Garza, J. G., Gninenko, S., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jakovcic, K., Kaminski, J., Karuza, M., Krieger, C., Lakic, B., Laurent, J. M., Luzon, G., Maroudas, M., Miceli, L., Neff, S., Ortega, I., Ozbey, A., Pivovaroff, M. J., Rosu, M., Ruz, J., Choliz, E. R., Schmidt, S., Schumann, M., Semertzidis, Y. K., Solanki, S. K., Stewart, L., Tsagris, I., Vafeiadis, T., Vogel, J. K., Vretenar, M., Yildiz, S. C., Zioutas, K., and İÜC

Subjects
Astrophysics and Astronomy, Physics - Instrumentation and Detectors, Photon, Cosmology and Nongalactic Astrophysics (astro-ph.CO), astro-ph.SR, Physics::Instrumentation and Detectors, Chameleons, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 7. Clean energy, High Energy Physics - Experiment, law.invention, Telescope, High Energy Physics - Experiment (hep-ex), Optics, law, Opto-mechanical sensor, 0103 physical sciences, Chameleon, Dark energy, Detectors and Experimental Techniques, 010306 general physics, chameleons, dark energy, opto-mechanical sensor, interferometry, Axion, physics.ins-det, Solar and Stellar Astrophysics (astro-ph.SR), Physics, Coupling, 010308 nuclear & particles physics, business.industry, hep-ex, Detector, Michelson interferometer, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), Interferometry, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, astro-ph.CO, Direct coupling, business, Particle Physics - Experiment, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We report on a first measurement with a sensitive opto-mechanical force sensor designed for the direct detection of coupling of real chameleons to matter. These dark energy candidates could be produced in the Sun and stream unimpeded to Earth. The KWISP detector installed on the CAST axion search experiment at CERN looks for tiny displacements of a thin membrane caused by the mechanical effect of solar chameleons. The displacements are detected by a Michelson interferometer with a homodyne readout scheme. The sensor benefits from the focusing action of the ABRIXAS X-ray telescope installed at CAST, which increases the chameleon flux on the membrane. A mechanical chopper placed between the telescope output and the detector modulates the incoming chameleon stream. We present the results of the solar chameleon measurements taken at CAST in July 2017, setting an upper bound on the force acting on the membrane of $80$~pN at 95\% confidence level. The detector is sensitive for direct coupling to matter $10^4 \leq\beta_m \leq 10^8$, where the coupling to photons is locally bound to $\beta_\gamma \leq 10^{11}$., Comment: 21 pages, 12 figures

Published
2019

5. An update on the Axion Helioscopes front: current activities at CAST and the IAXO project

Author

Joachim Jacoby, J. I. Collar, H. Ten Kate, Fritz Caspers, Julia Vogel, J. Kaminski, H. Silva, Giovanni Cantatore, Benito Gimeno, S. C. Yildiz, M. Betz, Alexey Dudarev, Georg G. Raffelt, A. Belov, F.J. Iguaz, Rainer Kotthaus, Javier Redondo, F. Haug, K. Barth, G. Luzón, Klaus Kurt Desch, C. Eleftheriadis, S. Caspi, P. Brax, Georgios Fanourakis, W. C. Wester, Hector Gomez, J. M. Laurent, N. Breijnholt, I. Dratchnev, Toyokazu Sekiguchi, S. Neff, L. Stewart, Joerg Jaeckel, Amanda Weltman, Marin Karuza, C. Krieger, Pierre Sikivie, A. Tomás, S. Aune, C. Nones, Heinrich Bräuninger, Serkant Ali Cetin, M. Rosu, I. G. Irastorza, J. M. Carmona, Babette Döbrich, Krešimir Jakovčić, Steffen Hauf, Takashi Hiramatsu, Biljana Lakić, Milica Krčmar, Evangelos Gazis, M. Davenport, Dieter H. H. Hoffmann, T. Papaevangelou, J.A. Villar, A. V. Derbin, Ante Ljubičić, Dieter Horns, S. N. Gninenko, A. Diago, I. Ortega, S. Matsuki, E. Gruber, Sergey Troitsky, T. Dafni, J. G. Garza, I. Savvidis, Andreas Ringwald, A. Lindner, Jordi Isern, M. Arik, Javier Galan, Ken'ichi Saikawa, E. Georgiopoulou, T. Guthörl, Eduardo Guendelman, Adriane De Assis Lawisch Rodriguez, I. Shilon, D. Chelouche, S. Russenschuck, Kenichi Imai, V. N. Muratova, P. Vedrine, F.E. Christensen, T. O. Niinikoski, E. Ferrer-Ribas, F. T. Avignone, Charles J. Hailey, M. D. Hasinoff, Peter Friedrich, M. J. Pivovaroff, Konstantin Zioutas, Sami K. Solanki, Louis Walckiers, H. Riege, Pierre Brun, Konstantinos Kousouris, Markus Kuster, A. Dael, T. Geralis, Gianpaolo Carosi, J. A. Garcia, A. Gardikiotis, Yannis K. Semertzidis, Eric Armengaud, Raimo Hartmann, Theodoros Vafeiadis, J. Ruz, K. Königsmann, Masahiro Kawasaki, D. González-Díaz, I. Giomataris, K. van Bibber, Olivier Limousin, A.C. Jakobsen, A. Liolios, Dafni, T, Arik, M., Armengaud, E., Aune, S., Avignone, F. T., Barth, K., Belov, A., Betz, M., Bräuninger, H., Brax, P., Breijnholt, N., Brun, P., Cantatore, Giovanni, Carmona, J. M., Carosi, G. P., Caspers, F., Caspi, S., Cetin, S. A., Chelouche, D., Christensen, F. E., Collar, J. I., Dael, A., Davenport, M., Derbin, A. V., Desch, K., Diago, A., Döbrich, B., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer Ribas, E., Friedrich, P., Galán, J., García, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Georgiopoulou, E., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gómez, H., González Díaz, D., Gruber, E., Guendelman, E., Guthörl, T., Hailey, C. J., Hartmann, R., Hauf, S., Haug, F., Hasinoff, M. D., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Irastorza, I. G., Isern, J., Imai, K., Jacoby, J., Jaeckel, J., Jakobsen, A. C., Jakovcić, K., Kaminski, J., Kawasaki, M., Karuza, M., Königsmann, K., Kotthaus, R., Krcmar, M., Kousouris, K., Krieger, C., Kuster, M., Lakić, B., Laurent, J. M., Limousin, O., Lindner, A., Liolios, A., Ljubicić, A., Luzón, G., Matsuki, S., Muratova, V. N., Neff, S., Niinikoski, T., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Riege, H., Ringwald, A., Rodríguez, A., Rosu, M., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., Solanki, S. K., Stewart, L., ten Kate, H. H. J., Tomas, A., Troitsky, S., Vafeiadis, T., van Bibber, K., Vedrine, P., Villar, J. A., Vogel, J. K., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., Zioutas, K., Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Arık, Metin, and Yıldız, Süleyman Cenk

Subjects
X-Ray Focusing Devices, X-ray detector, Particle physics, Nuclear and High Energy Physics, X-ray focusing device, Axions, Dark matter, Magnet Development, Micromegas detector, axions, dark matter, x-ray, detectors, micromegas detectors, x-ray focusing devices, magnet development, CAST, IAXO, 01 natural sciences, Axion, Primary (astronomy), Observatory, 0103 physical sciences, Dark Matter, X-Ray Detectors, 010306 general physics, Physics, Helioscope, Micromegas Detectors, 010308 nuclear & particles physics, Magnet development, Micromegas detectors, X-ray detectors, X-ray focusing devices, Orders of magnitude (time), Experimental methods, CERN Axion Solar Telescope
Abstract

Çetin, Serkant Ali (Dogus Author) -- Arık, Metin (Dogus Author) -- Yıldız, Süleyman Cenk (Dogus Author) Although they have not yet been detected, axions and axion-like particles (ALPs) continue to maintain the interest (even increasingly so) of the rare-event searches community as viable candidates for the Dark Matter of the Universe but also as a solution for several other puzzles of astrophysics. Their property of coupling to photons has inspired different experimental methods for their detection, one of which is the helioscope technique. The CERN Axion Solar Telescope (CAST) is the most sensitive helioscope built up to date and has recently published part of the latest data taken with the magnet bores gradually filled with He-3, probing the mass range up to 1.17 eV. The International AXion Observatory (IAXO) is being proposed as a facility where different axion studies can be performed, with the primary goal to study axions coming from the Sun. Designed to maximize sensitivity, it will improve the levels reached by CAST by almost 5 orders of magnitude in signal detection, that is more than one order of magnitude in terms of gay. Here we will summarize the most important aspects of the helioscopes, and focus mainly on IAXO, based on the recent papers [1, 2].

Published
2016
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6. The Next Generation of Axion Helioscopes: The International Axion Observatory (IAXO)

Author

Javier Redondo, Biljana Lakić, Eduardo Guendelman, K. van Bibber, A. Diago, S. Matsuki, Hector Gomez, Marin Karuza, C. Eleftheriadis, Olivier Limousin, H. H. J. ten Kate, Eric Armengaud, T. Dafni, Finn Erland Christensen, I. Ortega, Pierre Sikivie, Anders Clemen Jakobsen, F.J. Iguaz, Charles J. Hailey, Diego González-Díaz, Theodoros Vafeiadis, Milica Krčmar, Takashi Hiramatsu, V. N. Muratova, Dieter H. H. Hoffmann, J.A. Villar, S. C. Yildiz, Klaus Kurt Desch, I. Shilon, B. Döbrich, Javier Galan, J. G. Garza, Pierre Brun, A. Dael, S. Gninenko, F. T. Avignone, A. Tomás, W. C. Wester, C. Krieger, I. G. Irastorza, Masahiro Kawasaki, A. Lindner, A. Dudarev, Andreas Ringwald, Michael J. Pivovaroff, M. Betz, A. V. Derbin, P. Brax, C. Nones, D. Chelouche, Ioannis Giomataris, I. Savvidis, Yannis K. Semertzidis, S. Russenschuck, Kenichi Imai, Konstantin Zioutas, Theodoros Geralis, Serkant Ali Cetin, Giovanni Cantatore, Julia Vogel, Jordi Isern, H. Silva, E. Ferrer-Ribas, Ken'ichi Saikawa, G. Luzón, Dieter Horns, P. Vedrine, G. Fanourakis, Toyokazu Sekiguchi, Fritz Caspers, J. A. Garcia, Joerg Jaeckel, Amanda Weltman, J. Ruz, M. Davenport, J. Kaminski, L. Walckiers, Krešimir Jakovčić, Gianpaolo Carosi, A. Liolios, B. Gimeno, Georg G. Raffelt, T. Papaevangelou, J. M. Carmona, S. Caspi, Konstantinos Kousouris, I. Dratchnev, Sergey Troitsky, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Vogel, J. K., Armengaud, E., Avignone, F. T., Betz, M., Brax, P., Brun, P., Cantatore, Giovanni, 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., Diago, A., Döbrich, B., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer Ribas, E., Galán, J., García, J. A., Garza, J. G., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gómez, H., González Díaz, D., Guendelman, E., Hailey, C. J., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Irastorza, I. G., Isern, J., Imai, K., Jakobsen, A. C., Jaeckel, J., 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, V. N., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Ringwald, A., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., ten Kate, H., Tomas, A., Troitsky, S., Vafeiadis, T., van Bibber, K., Vedrine, P., Villar, J. A., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., and Zioutas, K.

Subjects
QCD axion, Particle physics, Physics::Instrumentation and Detectors, Dark matter, Physics and Astronomy(all), 01 natural sciences, 7. Clean energy, magnetic helioscope, High Energy Physics::Theory, QCD axions, Astroparticle Physics, Axion, Observatory, 0103 physical sciences, dark matter, Dark Matter, ddc:530, Detectors and Experimental Techniques, 010306 general physics, Astroparticle physics, Physics, Helioscope, 010308 nuclear & particles physics, Axion Dark Matter Experiment, High Energy Physics::Phenomenology, Strong CP problem, IAXO, Strong CP Problem, ALP, CERN Axion Solar Telescope, Particle Physics - Experiment, Helioscopes
Abstract

Çetin, Serkant Ali (Dogus Author) -- Conference full title: 13th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2013; Asilomar Conference Grounds Monterey Peninsula; United States; 8 September 2013 through 13 September 2013. The International Axion Observatory (IAXO) is a proposed 4th-generation axion helioscope with the primary physics research goal to search for solar axions via their Primakoff conversion into photons of 1 - 10 keV energies in a strong magnetic field. IAXO will achieve a sensitivity to the axion-photon coupling gaγ down to a few ×10-12 GeV-1 for a wide range of axion masses up to ∼ 0.25 eV. This is an improvement over the currently best (3rd generation) axion helioscope, the CERN Axion Solar Telescope (CAST), of about 5 orders of magnitude in signal strength, corresponding to a factor ∼ 20 in the axion photon coupling. IAXO's sensitivity relies on the construction of a large superconducting 8-coil toroidal magnet of 20 m length optimized for axion research. Each of the eight 60 cm diameter magnet bores is equipped with x-ray optics focusing the signal photons into ∼ 0.2 cm2 spots that are imaged by very low background x-ray detectors. The magnet will be built into a structure with elevation and azimuth drives that will allow solar tracking for 12 hours each day. This contribution is a summary of our papers [1-3] and we refer to these for further details.

Published
2015
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7. New micromegas for axion searches in CAST

Author

Hector Gomez, S. Aune, I. G. Irastorza, G. Luzón, T. Geralis, T. Vafeiadis, J. Ruz, I. Giomataris, Georgios Fanourakis, A. Gardikiotis, A. Tomás, J. Morales, A Rodríguez, Javier Galan, S. C. Yildiz, T. Papaevangelou, T. Dafni, F.J. Iguaz, E. Ferrer-Ribas, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, and Yıldız, Süleyman Cenk

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, 010308 nuclear & particles physics, Axions, Detector, X-ray detector, MicroMegas detector, Gas Micropattern Detectors, Low Background, 01 natural sciences, 0103 physical sciences, Cast, X-ray Detectors, 010306 general physics, Instrumentation, Axion, Micromegas
Abstract

Yıldız, Süleyman Cenk (Dogus Author) Micromegas detectors have been taking data in the CAST experiment since 2002, occupying one opening (out of the two looking for sunrise axions) of the magnet and showing good performance and stability. Currently, three of the four X-ray detectors used in the experiment are micromegas. The new detectors are of the Microbulk technology, which have attracted a lot of attention because of the advantages they present, among them the low-material construction, high radiopurity and good energy resolution. Here, their performance during the last year will be commented. In particular, the low background levels reached in some detectors have triggered a set of studies in order to understand the effect.

Published
2011
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8. New solar axion search using the CERN Axion Solar Telescope withHe4filling

Author

T. Papaevangelou, S. C. Yildiz, I. Savvidis, M. D. Hasinoff, Biljana Lakić, J. M. Carmona, I. Giomataris, A. Belov, Evangelos Gazis, T. O. Niinikoski, V. Burwitz, José Villar, L. Stewart, S. Neff, E. Da Riva, Theodoros Vafeiadis, J. Bremer, F.J. Iguaz, Ante Ljubičić, Dieter Hoffmann, Sami K. Solanki, M. Rosu, Markus Kuster, Sergei Gninenko, A. Tomás, T. Geralis, Krešimir Jakovčić, J. G. Garza, Joachim Jacoby, M. Gomez Marzoa, T. Dafni, Georgios Fanourakis, C. Eleftheriadis, M. Kavuk, M. J. Pivovaroff, Konstantin Zioutas, Julia Vogel, Heinrich Bräuninger, J. M. Laurent, Giovanni Cantatore, S. Aune, A. Liolios, Serkant Ali Cetin, K. Barth, G. Luzón, Milica Krčmar, M. Davenport, Marin Karuza, J. A. Garcia, I. Ortega, N. Elias, I. Shilon, Metin Arik, A. V. Dermenev, E. Georgiopoulou, Javier Galan, Georg G. Raffelt, I. G. Irastorza, J. Ruz, J. I. Collar, Adriane De Assis Lawisch Rodriguez, E. Ferrer-Ribas, A. Gardikiotis, and A. Nordt

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, Large Hadron Collider, Photon, Dark matter, chemistry.chemical_element, Superconducting magnet, 7. Clean energy, chemistry, CERN Axion Solar Telescope, Axion, Helium, Line (formation)
Abstract

The CERN Axion Solar Telescope (CAST) searches for a -> gamma conversion in the 9 T magnetic field of a refurbished LHC test magnet that can be directed toward the Sun. Two parallel magnet bores can be filled with helium of adjustable pressure to match the x-ray refractive mass m(gamma) to the axion search mass m(a). After the vacuum phase (2003-2004), which is optimal for m(a) less than or similar to 0.02 eV, we used He-4 in 2005-2007 to cover the mass range of 0.02-0.39 eV and He-3 in 2009-2011 to scan from 0.39 to 1.17 eV. After improving the detectors and shielding, we returned to He-4 in 2012 to investigate a narrow m(a) range around 0.2 eV ("candidate setting" of our earlier search) and 0.39-0.42 eV, the upper axion mass range reachable with He-4, to "cross the axion line" for the KSVZ model. We have improved the limit on the axion-photon coupling to g(a gamma) < 1.47 x 10(-10) GeV-1 (95% C.L.), depending on the pressure settings. Since 2013, we have returned to the vacuum and aim for a significant increase in sensitivity.

Published
2015
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9. Lowering the background level and the energy threshold of Micromegas x-ray detectors for axion searches

Author

S. Aune, J. G. Garza, A. Tomás, D. Jourde, Ioannis Giomataris, Esther Ferrer Ribas, Javier Galan, F. Aznar, T. Papaevangelou, I. G. Irastorza, I. Ortega, M. Davenport, J. F. Castel, T. Dafni, Adriane De Assis Lawisch Rodriguez, S. C. Yildiz, Theodoros Vafeiadis, J. A. Garcia, and Francisco Jose Iguaz Gutierrez

Subjects
Physics, Astrophysics and Astronomy, Range (particle radiation), Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Canfranc Underground Laboratory, Detector, X-ray detector, FOS: Physical sciences, MicroMegas detector, Instrumentation and Detectors (physics.ins-det), 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, Electromagnetic shielding, Astrophysics - Instrumentation and Methods for Astrophysics, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Axion, Energy (signal processing)
Abstract

Axion helioscopes search for solar axions by their conversion in x-rays in the presence of high magnetic fields. The use of low background x-ray detectors is an essential component contributing to the sensitivity of these searches. In this work, we review the recent advances on Micromegas detectors used in the CERN Axion Solar Telescope (CAST) and proposed for the future International Axion Observatory (IAXO). The actual setup in CAST has achieved background levels below 10$^{-6}$ keV$^{-1}$ cm$^{-2}$ s$^{-1}$, a factor 100 lower than the first generation of Micromegas detectors. This reduction is based on active and passive shielding techniques, the selection of radiopure materials, offline discrimination techniques and the high granularity of the readout. We describe in detail the background model of the detector, based on its operation at CAST site and at the Canfranc Underground Laboratory (LSC), as well as on Geant4 simulations. The best levels currently achieved at LSC are low than 10$^{-7}$ keV$^{-1}$ cm$^{-2}$ s$^{-1}$ and show good prospects for the application of this technology in IAXO. Finally, we present some ideas and results for reducing the energy threshold of these detectors below 1 keV, using high-transparent windows, autotrigger electronics and studying the cluster shape at different energies. As a high flux of axion-like-particles is expected in this energy range, a sub-keV threshold detector could enlarge the physics case of axion helioscopes., Comment: Proceedings of 3rd International Conference on Technology and Instrumentation in Particle Physics (TIPP 2014)

Published
2015
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10. Future axion searches with the International Axion Observatory (IAXO)

Author

C. Krieger, A. Lindner, Javier Redondo, Biljana Lakić, L. Walckiers, Pierre Sikivie, Joerg Jaeckel, A. Tomás, Ioannis Giomataris, Iratxe Ortega, K Saikawa, Hector Gomez, Jochen Kaminski, Takashi Hiramatsu, F.J. Iguaz, H. H. J. ten Kate, Milica Krčmar, Anders Clemen Jakobsen, Dieter H. H. Hoffmann, F. T. Avignone, Theodoros Vafeiadis, Krešimir Jakovčić, H. Silva, J.A. Villar, Javier Galan, B. Döbrich, I. Shilon, C. J. Hailey, Jordi Isern, J. G. Garza, A. Diago, Michael J. Pivovaroff, Konstantin Zioutas, S. C. Yildiz, W. C. Wester, Theodoros Geralis, S. Caspi, A. Dael, S. Gninenko, Julia Vogel, K. van Bibber, Toyokazu Sekiguchi, G. Luzón, M. Davenport, Georg G. Raffelt, Finn Erland Christensen, Sergey Troitsky, J. Ruz, Masahiro Kawasaki, Giovanni Cantatore, A. V. Derbin, A. Liolios, C. Eleftheriadis, Dieter Horns, B. Gimeno, T. Papaevangelou, J. M. Carmona, A. Dudarev, Eduardo Guendelman, Andreas Ringwald, Serkant Ali Cetin, I. G. Irastorza, P. Vedrine, G. Fanourakis, I. Savvidis, T. Dafni, S. Russenschuck, E. Ferrer-Ribas, Klaus Kurt Desch, J. A. Garcia, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, I. G., Irastorza, F. T., Avignone, Cantatore, Giovanni, J. M., Carmona, S., Caspi, S. A., Cetin, F. E., Christensen, A., Dael, T., Dafni, M., Davenport, A. V., Derbin, K., Desch, A., Diago, B., Döbrich, A., Dudarev, C., Eleftheriadi, G., Fanouraki, E., Ferrer Riba, J., Galán, J. A., García, J. G., Garza, T., Gerali, B., Gimeno, I., Giomatari, S., Gninenko, H., Gómez, E., Guendelman, C. J., Hailey, T., Hiramatsu, D. H. H., Hoffmann, D., Horn, F. J., Iguaz, J., Isern, A. C., Jakobsen, J., Jaeckel, K., Jakovčić, J., Kaminski, M., Kawasaki, M., Krčmar, C., Krieger, B., Lakić, A., Lindner, A., Liolio, G., Luzón, I., Ortega, T., Papaevangelou, M. J., Pivovaroff, G., Raffelt, J., Redondo, A., Ringwald, S., Russenschuck, J., Ruz, K., Saikawa, I., Savvidi, T., Sekiguchi, I., Shilon, P., Sikivie, H., Silva, H., ten Kate, A., Toma, S., Troitsky, T., Vafeiadi, K., van Bibber, P., Vedrine, J. A., Villar, J. K., Vogel, L., Walckier, W., Wester, S. C., Yildiz, and K., Zioutas

Subjects
Physics, History, Particle physics, solar axion, Orders of Magnitude, 010308 nuclear & particles physics, Rare event detection, Single photon detectors, Low Background Detectors, 01 natural sciences, dark matter, White Dwarfs, Computer Science Applications, Education, Low energy, Observatory, 0103 physical sciences, solar axions, ddc:530, X-ray Focusing Optics, 010306 general physics, Axion
Abstract

Çetin, Serkant Ali (Dogus Author) -- Conference full title: 6th Symposium on Large TPCs for Low Energy Rare Event Detection; Paris; France; 17 December 2012 through 19 December 2012. The International Axion Observatory (IAXO) is a new generation axion helioscope aiming at a sensitivity to the axion-photon coupling of gaγ ∼ few × 10-12 GeV-1, i.e. 1-1.5 orders of magnitude beyond the one achieved by CAST, currently the most sensitive axion helioscope. The main elements of IAXO are an increased magnetic field volume together with extensive use of x-ray focusing optics and low background detectors, innovations already successfully tested in CAST. Additional physics cases of IAXO could include the detection of electron-coupled axions invoked to explain the white dwarf cooling, relic axions, and a large variety of more generic axion-like particles (ALPs) and other novel excitations at the low-energy frontier of elementary particle physics.

Published
2013
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11. Status and perspectives of the CAST experiment

Author

Biljana Lakić, José Villar, C. Ezer, J. I. Collar, T. Dafni, S. Borghi, Giovanni Cantatore, T. Geralis, F.J. Iguaz, S. C. Yildiz, Theodoros Vafeiadis, M. Davenport, S. N. Gninenko, J. Ruz, Sami K. Solanki, Evangelos Gazis, M. Rosu, Georgios Fanourakis, Hector Gomez, Joachim Jacoby, Georg G. Raffelt, G. Lutz, Julia Vogel, Marin Karuza, Markus Kuster, K. Barth, G. Luzón, A. Liolios, A. Gardikiotis, Timur Rashba, A. Belov, S. Aune, T. Papaevangelou, E. Ferrer-Ribas, N. Elias, F. Haug, M. D. Hasinoff, Peter Friedrich, M Tsagri, I. Savvidis, Raimo Hartmann, H. Riege, Rainer Kotthaus, T. O. Niinikoski, J. M. Carmona, I. G. Irastorza, M. J. Pivovaroff, Dieter H. H. Hoffmann, A Rodríguez, Konstantin Zioutas, J. Morales, E. Gruber, J. A. Garcia, Krešimir Jakovčić, V. Lozza, K. Königsmann, L. Stewart, I. Giomataris, C. Eleftheriadis, A. Nordt, J. M. Laurent, A. Tomás, P. S. Silva, M. Arik, Ante Ljubičić, Javier Galan, Heinrich Bräuninger, Milica Krčmar, Serkant Ali Cetin, T. Guthörl, K. van Bibber, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR144760, Arık, Metin, B., Lakić, M., Arik, S., Aune, K., Barth, A., Belov, S., Borghi, H., Bräuninger, Cantatore, Giovanni, J. M., Carmona, S. A., Cetin, J. I., Collar, T., Dafni, M., Davenport, C., Eleftheriadi, N., Elia, C., Ezer, G., Fanouraki, E., Ferrer Riba, P., Friedrich, J., Galán, J. A., García, A., Gardikioti, E. N., Gazi, T., Gerali, I., Giomatari, S., Gninenko, H., Gómez, E., Gruber, T., Guthörl, R., Hartmann, F., Haug, M. D., Hasinoff, D. H. H., Hoffmann, F. J., Iguaz, I. G., Irastorza, J., Jacoby, K., Jakovčić, M., Karuza, K., Königsmann, R., Kotthau, M., Krčmar, M., Kuster, J. M., Laurent, A., Liolio, A., Ljubičić, V., Lozza, G., Lutz, G., Luzón, J., Morale, T., Niinikoski, A., Nordt, T., Papaevangelou, M. J., Pivovaroff, G., Raffelt, T., Rashba, H., Riege, A., Rodríguez, M., Rosu, J., Ruz, I., Savvidi, P. S., Silva, S. K., Solanki, L., Stewart, A., Tomá, M., Tsagri, K., van Bibber, T., Vafeiadi, J., Villar, J. K., Vogel, S. C., Yildiz, and K., Zioutas

Subjects
History, Particle physics, solar axion, Physics::Instrumentation and Detectors, 01 natural sciences, 7. Clean energy, Education, Nuclear physics, High Energy Physics::Theory, Phase I, Solar core, 0103 physical sciences, Buffer Gas, 010306 general physics, CERN Axion Solar Telescopes, Axion, Coupling constant, Physics, Coupling Constants, Helioscope, Various Densities, Large Hadron Collider, 010308 nuclear & particles physics, Axion Dark Matter Experiment, X-Rays, High Energy Physics::Phenomenology, Single photon detectors, Phase II, axions, solar physics, dark matter, Computer Science Applications, solar axions, Magnet, X-Ray, CERN Axion Solar Telescope
Abstract

Arık, Metin (Dogus Author) -- The conference paper was firstly submitted to 12th International Conference on Topics in Astroparticle and Underground Physics. The CERN Axion Solar Telescope (CAST) is currently the most sensitive axion helioscope designed to search for axions produced by the Primakoff process in the solar core. CAST is using a Large Hadron Collider (LHC) test magnet where axions could be converted into X-rays with energies up to 10 keV. During the phase I, the experiment operated with vacuum inside the magnet bores and covered axion masses up to 0.02 eV. In the phase II, the magnet bores were filled with a buffer gas (first 4He and later 3He) at various densities in order to extend the sensitivity to higher axion masses (up to f .18 eV). The phase II data taking was completed in 2011. So far, no evidence of axion signal has been found and CAST set the most restrictive experimental limit on the axion-photon coupling constant over a broad range of axion masses. The latest CAST results with 3He data in the mass range 0.39 eV < m a < 0.64 eV will be presented.

Published
2012
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12. Latest results and prospects of the CERN Axion Solar Telescope

Author

I. Giomataris, C. Eleftheriadis, T. Guthörl, S. C. Yildiz, José Villar, A. Tomás, G Lutz, I. G. Irastorza, F.J. Iguaz, Georgios Fanourakis, Biljana Lakić, L. Stewart, Javier Galan, S. Aune, Hector Gomez, J. M. Carmona, Marin Karuza, Dieter H. H. Hoffmann, V. Lozza, Milica Krčmar, Ante Ljubičić, K. Königsmann, M. Davenport, Theodoros Vafeiadis, E. Gruber, J. M. Laurent, Joachim Jacoby, S. Borghi, F. Haug, Timur Rashba, T. Papaevangelou, M. Tsagri, M. D. Hasinoff, I. Savvidis, Heinrich Bräuninger, P. S. Silva, M. Rosu, Peter Friedrich, M. J. Pivovaroff, Serkant Ali Cetin, T. Geralis, Konstantin Zioutas, T. O. Niinikoski, Giovanni Cantatore, S. N. Gninenko, K. van Bibber, A. Gardikiotis, Raimo Hartmann, J. Ruz, A. Liolios, N. Elias, Sami K. Solanki, Markus Kuster, A Nordt, E. Ferrer-Ribas, Julia Vogel, K. Barth, G. Luzón, H. Riege, C. Ezer, T. Dafni, A Rodríguez, Krešimir Jakovčić, Evangelos Gazis, Georg G. Raffelt, Regina Soufli, A. Belov, J. Morales, Rainer Kotthaus, J. I. Collar, I. G., Irastorza, S., Aune, K., Barth, A., Belov, S., Borghi, H., Bräuninger, Cantatore, Giovanni, J. M., Carmona, S. A., Cetin, J. I., Collar, T., Dafni, M., Davenport, C., Eleftheriadi, N., Elia, C., Ezer, G., Fanouraki, E., Ferrer Riba, P., Friedrich, J., Galán, A., Gardikioti, E. N., Gazi, T., Gerali, I., Giomatari, S., Gninenko, H., Gómez, E., Gruber, T., Guthörl, R., Hartmann, F., Haug, M. D., Hasinoff, D. H. H., Hoffmann, F. J., Iguaz, J., Jacoby, K., Jakovčić, M., Karuza, K., Königsmann, R., Kotthau, M., Krčmar, M., Kuster, B., Lakić, J. M., Laurent, A., Liolio, A., Ljubičić, Lozza, Valentina, G., Lutz, G., Luzón, J., Morale, T., Niinikoski, A., Nordt, T., Papaevangelou, M. J., Pivovaroff, G., Raffelt, T., Rashba, H., Riege, A., Rodríguez, M., Rosu, J., Ruz, I., Savvidi, P. S., Silva, S. K., Solanki, R., Soufli, L., Stewart, A., Tomá, M., Tsagri, Bibber, K. v. a. n., T., Vafeiadi, J., Villar, J. K., Vogel, S. C., Yildiz, K., Zioutas, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Ezer, C., and Yıldız, Süleyman Cenk

Subjects
History, Particle physics, axions, Physics::Instrumentation and Detectors, Dark matter, 01 natural sciences, 7. Clean energy, dark matter, Education, Phase I, 0103 physical sciences, 010306 general physics, CERN Axion Solar Telescopes, Axion, Primakoff effect, solar physics, Physics, High Magnetic Fields, Helioscope, Large Hadron Collider, 010308 nuclear & particles physics, Axion Dark Matter Experiment, solar physic, Solar physics, Computer Science Applications, ddc, axion, CERN Axion Solar Telescope
Abstract

Çetin, Serkant Ali (Dogus Author) -- Ezer, C. (Dogus Author) -- Yıldız, Süleyman Cenk (Dogus Author) The CERN Axion Solar Telescope (CAST) experiment searches for axions from the Sun converted into few keV photons via the inverse Primakoff effect in the high magnetic field of a superconducting Large Hadron Collider (LHC) decommissioned test magnet. After results obtained with vacuum in the magnet pipes (phase I of the experiment) as well as with 4He the collaboration is now immersed in the data taking with 3He, to be finished in 2011. The status of the experiment will be presented, including a preliminary exclusion plot of the first 3He data. CAST is currently sensitive to realistic QCD axion models at the sub-eV scale, and with axion-photon couplings down to the ∼ 2 × 10-10 GeV -1, compatible with solar life limits. Future plans include revisiting vaccuum and 4He configurations with improved sensitivity, as well as possible additional search for non-standard signals from chamaleons, paraphotons or other WISPs. For the longer term, we study the feasibility of an altogether improved version of the axion helioscope concept, with a jump in sensitivity of about one order of magnitude in gaγ beyond CAST.

Published
2011

13. Probing the eV-Mass range for solar axions with CAST

Author

S Aune, K Barth, A Belov, S Borghi, H Brauninger, G Cantatore, J M Carmona, S A Cetin, J I Collar, T Dafni, M Davenport, C Eleftheriadis, N Elias, C Ezer, G Fanourakis, E Ferrer-Ribas, H Fischer, J Franz, P Friedrich, J Galan, A Gardikiotis, E N Gazis, T Geralis, I Giomataris, S Gninenko, H Gomez, E Gruber, T Guthorl, R Hartmann, F Haug, M D Hasinoff, D H H Hoffmann, F J Iguaz, I G Irastorza, J Jacoby, K Jakovcic, D Kang, T Karageorgopoulou, M Karuza, K Konigsmann, R Kotthaus, M Krcmar, K Kousouris, M Kuster, B Lakic, P Lang, C Lasseur, J M Laurent, A Liolios, A Ljubicic, V Lozza, G Lutz, G Luzon, D W Miller, A Mirizzi, J Morales, T Niinikoski, A Nordt, T Papaevangelou, M J Pivovaroff, G Raiteri, G Raffelt, T Rashba, H Riege, A Rodriguez, M Rosu, J Ruz, I Savvidis, Y Semertzidis, P Serpico, P S Silva, S K Solanki, R Soufli, L Stewart, A Tomas, M Tsagri, K van Bibber, T Vafeiadis, J Villar, Julia K Vogel, L Walckiers, Y Y Y Wong, S C Yildiz, K Zioutas, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, TR144753, Çetin, Serkant Ali, Yıldız, Süleyman Cenk, S., Aune, K., Barth, A., Belov, S., Borghi, H., Brauninger, Cantatore, Giovanni, J. M., Carmona, S. A., Cetin, J. I., Collar, T. Dafni M., Davenport, C., Eleftheriadi, N., Elia, C., Ezer, G., Fanouraki, E., Ferrer Riba, H., Fischer, J., Franz, P., Friedrich, J., Galan, A., Gardikioti, E. N., Gazi, T., Gerali, I., Giomatari, S., Gninenko, H., Gomez, E., Gruber, T., Guthorl, R., Hartmann, F., Haug, M. D., Hasinoff, D. H. H., Hoffmann, F. J., Iguaz, I. G., Irastorza, J., Jacoby, K., Jakovcic, D., Kang, T., Karageorgopoulou, M., Karuza, K., Konigsmann, R., Kotthau, M., Krcmar, K., Kousouri, M., Kuster, B., Lakic, P., Lang, C., Lasseur, J. M., Laurent, A., Liolio, A., Ljubicic, V., Lozza, G., Lutz, G., Luzon, D. W., Miller, A., Mirizzi, J., Morale, T., Niinikoski, A., Nordt, T., Papaevangelou, M. J., Pivovaroff, G., Raiteri, G., Raffelt, T., Rashba, H., Riege, A., Rodriguez, M., Rosu, J., Ruz, I., Savvidi, Y., Semertzidi, P., Serpico, P. S., Silva, S. K., Solanki, R., Soufli, L., Stewart, A., Toma, M., Tsagri, K., Van Bibber, T., Vafeiadi, J., Villar, J. K., Vogel, L., Walckier, Y. Y. Y., Wong, S. C., Yildiz, and K., Zioutas

Subjects
Particle physics, solar axion, Second Phase, Physics::Instrumentation and Detectors, Dark matter, dark matter, X-ray Detector, Helium Gas, Phase Spaces, Current Status, Dark Matter, CERN Axion Solar Telescopes, Axion, Primakoff effect, Coupling Constants, Physics, Large Hadron Collider, Mass Regions, Axion Dark Matter Experiment, Gas Density Distribution, Solar Axions, Upper Limits, X-ray Photons, Massless particle, Strong CP Problem, solar axions, Photon detection, Strong CP problem, CERN Axion Solar Telescope, High Pressure
Abstract

Çetin, Serkant Ali (Dogus Author) -- Yıldız, Süleyman Cenk (Dogus Author) -- Conference full title: 2010 IEEE Nuclear Science Symposium conference record (NSS/MIC 2010) : [including the 2010 IEEE Nuclear Science Symposium, Medical Imaging Conference, and the 17th International Workshop on Room-Temperature Semiconductor X-Ray and Gamma-Ray Detectors (RTSD)]; Knoxville, Tennessee, USA, 30 October - 6 November 2010 The CERN Axion Solar Telescope (CAST) is searching for solar axions which could be produced in the core of the Sun via the so-called Primakoff effect. Not only would these hypothetical particles solve the strong CP problem, but they are also one of the favored candidates for dark matter. In order to look for axions originating from the Sun, CAST uses a decommissioned LHC prototype magnet. In its 10 m long magnetic field region of 9 Tesla, axions could be reconverted into X-ray photons. Different X-ray detectors are installed on both ends of the magnet, which is mounted on a structure built to follow the Sun during sunrise and sunset for a total of about 3 hours per day. The analysis of the data acquired during the first phase of the experiment with vacuum in the magnetic field region yielded the most restrictive experimental upper limit on the axion-to-photon coupling constant for axion masses up to about 0.02 eV. In order to extend the sensitivity of the experiment to a wider mass range, the CAST experiment continues its search for axions with helium in the magnet bores. In this way it is possible to restore coherence of conversion for larger masses. Changing the pressure of the helium gas enables the experiment to scan different axion masses in the range of up to about 1.2 eV. Especially at high pressures, a precise knowledge of the gas density distribution is crucial to obtain accurate results. In the first part of this second phase of CAST, 4He was used and the axion mass region was extended up to 0.39 eV, a part of phase space favored by axion models. In CAST's ongoing 3He phase the studied mass range is now being extended further. In this contribution the final results of CAST's 4He phase will be presented and the current status of the 3He run will be given. This includes latest results as well as prospects of future axion experiments. Nucl. Plasma Sci. Soc. Inst. Electr. Electron. Eng. (NPSS)

Published
2010
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14. Search for chameleons with CAST

Author

J. I. Collar, M. Arik, F.J. Iguaz, Milica Krčmar, Javier Galan, Philippe Brax, José Villar, S. C. Yildiz, Marin Karuza, Julia Vogel, K. Barth, G. Luzón, Biljana Lakić, M. Davenport, M. Kavuk, I. Ortega, Joachim Jacoby, Heinrich Bräuninger, Serkant Ali Cetin, T. Geralis, Georg G. Raffelt, E. Ferrer-Ribas, M. Rosu, H. Riege, T. Papaevangelou, J. G. Garza, Theodoros Vafeiadis, A. Belov, I. G. Irastorza, S. Aune, A. Gardikiotis, Krešimir Jakovčić, F. Haug, I. Savvidis, J. M. Laurent, Dieter H. H. Hoffmann, Peter Friedrich, S. Neff, Charles J. Hailey, M. J. Pivovaroff, Konstantin Zioutas, T. Dafni, Vassilis Anastassopoulos, J. Ruz, I. Giomataris, Klaus Kurt Desch, I. Lavrentyev, Finn Erland Christensen, C. Eleftheriadis, Ante Ljubičić, A. V. Dermenev, A. Upadhye, C. Krieger, Sami K. Solanki, J. M. Carmona, M. D. Hasinoff, Georgios Fanourakis, G. Cantatore, Evangelos Gazis, Jochen Kaminski, Anders Clemen Jakobsen, A. Krüger, A. Liolios, J. A. Garcia, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Anastassopoulos, V, Arik, M., Aune, S., Barth, K., Belov, A., Bräuninger, H., Cantatore, Giovanni, Carmona, J. M., Cetin, S. A., Christensen, F., Collar, J. I., Dafni, T., Davenport, M., Desch, K., Dermenev, A., Eleftheriadis, C., Fanourakis, G., Ferrer Ribas, E., Friedrich, P., Galán, J., García, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Geralis, T., Giomataris, I., Hailey, C., Haug, F., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jacoby, J., Jakobsen, A., Jakovčić, K., Kaminski, J., Karuza, M., Kavuk, M., Krčmar, M., Krieger, C., Krüger, A., Lakić, B., Laurent, J. M., Liolios, A., Ljubičić, A., Luzón, G., Neff, S., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Riege, H., Rosu, M., Ruz, J., Savvidis, I., Solanki, S. K., Vafeiadis, T., Villar, J. A., Vogel, J. K., Yildiz, S. C., Zioutas, K., Brax, P., Lavrentyev, I., and Upadhye, A.

Subjects
Nuclear and High Energy Physics, Astrophysics and Astronomy, Photon, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, Tachocline, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, SDD, X-ray, High Energy Physics - Phenomenology (hep-ph), 0103 physical sciences, Chameleon, Dark energy, 010306 general physics, Axion, Solar and Stellar Astrophysics (astro-ph.SR), Primakoff effect, Coupling constant, Coupling, Physics, CAST, 010308 nuclear & particles physics, Instrumentation and Detectors (physics.ins-det), lcsh:QC1-999, High Energy Physics - Phenomenology, Astrophysics - Solar and Stellar Astrophysics, CERN Axion Solar Telescope, lcsh:Physics
Abstract

In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ($\beta_{\rm m}$) and to photons ($\beta_{\gamma}$) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1$\,$keV to 400$\,$eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600$\,$eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of $\beta_{\gamma}\!\lesssim\!10^{11}$ for $1, Comment: 8 pages, 12 figures

Published
2015
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15. The IAXO Helioscope

Author

I. Savvidis, I. G. Irastorza, I. Ortega, Toyokazu Sekiguchi, K Saikawa, M. Davenport, Serkant Ali Cetin, C. Eleftheriadis, C. Krieger, D. Chelouche, O. Limousin, Charles J. Hailey, P. Vedrine, G. Fanourakis, S. Caspi, Gianpaolo Carosi, Javier Redondo, A. Tomás, Ioannis Giomataris, Javier Galan, Hector Gomez, Pierre Sikivie, A.C. Jakobsen, S. Russenschuck, J. G. Garza, F.J. Iguaz, Kenichi Imai, K. van Bibber, Pierre Brun, Marin Karuza, A. Dael, Takashi Hiramatsu, S. Gninenko, A. Lindner, M. Betz, Dieter H. H. Hoffmann, A. Liolios, Jochen Kaminski, E. Ferrer Ribas, Theodoros Geralis, V. N. Muratova, Julia Vogel, Yannis K. Semertzidis, Theodoros Vafeiadis, Babette Döbrich, Sergey Troitsky, G. Luzón, A. V. Derbin, D. González-Díaz, Michael J. Pivovaroff, F. T. Avignone, J. A. Garcia, Joerg Jaeckel, Amanda Weltman, W. C. Wester, Georg G. Raffelt, Masahiro Kawasaki, A. Dudarev, Andreas Ringwald, Krešimir Jakovčić, T. Dafni, Milica Krčmar, J.A. Villar, A. Diago, Eduardo Guendelman, Konstantin Zioutas, Dieter Horns, Klaus Kurt Desch, J. Ruz, J. M. Carmona, Giovanni Cantatore, Benito Gimeno, F.E. Christensen, P. Brax, T. Papaevangelou, L. Walckiers, Jordi Isern, Konstantinos Kousouris, I. Dratchnev, I. Shilon, Fritz Caspers, C. Nones, S. Matsuki, S. C. Yildiz, Biljana Lakić, H. H. J. ten Kate, E. Armengaud, H. Silva, Ribas, E. Ferrer, Armengaud, E., Avignone, F. T., Betz, M., Brax, P., Brun, P., Cantatore, Giovanni, 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., Diago, A., Döbrich, B., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Galán, J., García, J. A., Garza, J. G., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gómez, H., González Diaz, D., Guendelman, E., Hailey, C. J., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Irastorza, I. G., Isern, J., Imai, K., Jaeckel, J., Jakobsen, A. C., 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, V. N., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Ringwald, A., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., Ten Kate, H. H. J., Tomas, A., Troitsky, S., Vafeiadis, T., Van Bibber, K., Vedrine, P., Villar, J. A., Vogel, J. K., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., Zioutas, K., Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, and Çetin, Serkant Ali

Subjects
History, Particle physics, QCD axion, Dark matter, X-ray optics, Detectable Signal, 7. Clean energy, magnetic helioscope, dark matter, Education, Solar tracker, Optics, QCD axions, ddc:530, Detectors and Experimental Techniques, Axion, Physics, Helioscope, Fourth Generation, business.industry, Technical Design, Detector, MicroMegas detector, Toroidal Magnets, Low Background Detectors, Computer Science Applications, Magnet, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Feasibility Studies, X-ray Focusing Optics, business
Abstract

Çetin, Serkant Ali (Dogus Author) -- Conference full title: 7th International Symposium on Large TPCs for Low-Energy Rare Event Detection; Institute of Astroparticle Physics (APC) Campus - Paris Diderot UniversityParis; France; 15 December 2014 through 17 December 2014 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.

Published
2015
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16. Search for Solar Axions by the CERN Axion Solar Telescope withHe3Buffer Gas: Closing the Hot Dark Matter Gap

Author

M. Tsagri, T. Guthörl, M. Gomez Marzoa, S. C. Yildiz, J. G. Garza, T. Dafni, M. Davenport, S. Borghi, J. M. Laurent, M. D. Hasinoff, Steffen Hauf, N. Elias, P. S. Silva, Sami K. Solanki, S. Aune, Joachim Jacoby, Markus Kuster, Evangelos Gazis, T. Vafeiadis, F.J. Iguaz, P. M. Lang, E. Da Riva, Peter Friedrich, A. Liolios, Dieter H. H. Hoffmann, Georg G. Raffelt, T. O. Niinikoski, Georgios Fanourakis, M. J. Pivovaroff, Konstantin Zioutas, A. Nordt, C. Eleftheriadis, Ioannis Giomataris, Heinrich Bräuninger, J. Ruz, T. Geralis, Serkant Ali Cetin, Milica Krčmar, K. Königsmann, G. Cantatore, Ante Ljubičić, J. I. Collar, Biljana Lakić, T. Papaevangelou, J. M. Carmona, I. Savvidis, K. van Bibber, S. Neff, A. Tomás, E. Georgiopoulou, S. N. Gninenko, M. Arik, E. Gruber, A. Belov, Javier Galan, Rainer Kotthaus, F. Haug, A Rodríguez, L. Stewart, J. A. Garcia, Hector Gomez, Marin Karuza, E. Ferrer-Ribas, I. G. Irastorza, H. Riege, A. Gardikiotis, Raimo Hartmann, Julia Vogel, K. Barth, G. Luzón, Krešimir Jakovčić, M. Rosu, I. Shilon, and José Villar

Subjects
Physics, Helioscope, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Axion Dark Matter Experiment, Hot dark matter, Buffer gas, Dark matter, General Physics and Astronomy, Astrophysics, 7. Clean energy, 01 natural sciences, Observatory, 0103 physical sciences, Astrophysics::Earth and Planetary Astrophysics, 010306 general physics, CERN Axion Solar Telescope, Axion
Abstract

The CERN Axion Solar Telescope has finished its search for solar axions with He-3 buffer gas, covering the search range 0.64 eV less than or similar to ma less than or similar to 1.17 eV. This closes the gap to the cosmological hot dark matter limit and actually overlaps with it. From the absence of excess x rays when the magnet was pointing to the Sun we set a typical upper limit on the axion-photon coupling of g(a gamma) less than or similar to 3.3 x 10(-10) GeV-1 at 95% C.L., with the exact value depending on the pressure setting. Future direct solar axion searches will focus on increasing the sensitivity to smaller values of g(a gamma), for example by the currently discussed next generation helioscope International AXion Observatory.

Published
2014
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17. Low background x-ray detection with Micromegas for axion research

Author

Ioannis Giomataris, I. Ortega, S. C. Yildiz, F.J. Iguaz, A. Tomás, A Rodríguez, A. Diago, J. G. Garza, Javier Galan, J. A. Garcia, T. Papaevangelou, I. G. Irastorza, A. Gardikiotis, Theodoros Vafeiadis, E. Ferrer-Ribas, and T. Dafni

Subjects
Physics, History, Particle physics, 010308 nuclear & particles physics, Detector, X-ray detector, MicroMegas detector, 01 natural sciences, Computer Science Applications, Education, Background level, Signal strength, 0103 physical sciences, 010306 general physics, Axion
Abstract

We have studied low-background techniques in order to improve the background level for Micromegas detectors. These detectors are good candidates for rare event searches thanks to the low mass and the radiopurity of the materials used in the construction; moreover they have good discrimination capabilities. The motivation of these studies is the reduction of the background level in the CAST experiment where three of the four detectors operating currently are Micromegas of the microbulk type. The last result of the experience acquired in low-background techniques has been the reduction of the background level by a factor 4.5 for two detectors in the CAST experiment, corresponding to an improvement of a factor 2 in signal strength.

Published
2014
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18. Conceptual design of the International Axion Observatory (IAXO)

Author

A. Liolios, P. Vedrine, G. Fanourakis, Doron Chelouche, Klaus Kurt Desch, Serkant Ali Cetin, I. G. Irastorza, Konstantin Zioutas, Gianpaolo Carosi, Javier Redondo, I. Dratchnev, Ken'ichi Saikawa, Ioannis Giomataris, B. Gimeno, Pierre Brun, Eduardo Guendelman, A. Dael, B. Döbrich, S. Gninenko, E. Ferrer-Ribas, C. Krieger, L. Walckiers, J. Ruz, J. A. García, S. Matsuki, Milica Krčmar, I. Shilon, S. Russenschuck, Kenichi Imai, J.A. Villar, I. Ortega, A. Diago, J. Galán, Sergey Troitsky, V. N. Muratova, Joerg Jaeckel, I. Savvidis, Ph. Brax, Amanda Weltman, H. Silva, C. Nones, Charles J. Hailey, Haley Louise Gomez, Dieter Horns, K. van Bibber, Krešimir Jakovčić, S. C. Yildiz, Olivier Limousin, Jordi Isern, Finn Erland Christensen, T. Vafeiadis, William Wester, C. Eleftheriadis, Michael J. Pivovaroff, Theodoros Geralis, Biljana Lakić, Julia Vogel, A. Dudarev, Andreas Ringwald, Fritz Caspers, A. V. Derbin, K. Kousouris, G. Luzón, T. Papaevangelou, J. M. Carmona, J. Kaminski, Anders Clemen Jakobsen, H. H. J. ten Kate, T. Dafni, A. Lindner, M. Betz, Georg G. Raffelt, Marin Karuza, S. Caspi, Masahiro Kawasaki, Giovanni Cantatore, Eric Armengaud, J. G. Garza, F.J. Iguaz, F. T. Avignone, A. Tomás, T. Sekiguchi, M. Davenport, Pierre Sikivie, Takashi Hiramatsu, Dieter H. H. Hoffmann, Diego González-Díaz, Yannis K. Semertzidis, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Armengaud, E., Avignone, F. T., Betz, M., Brax, P., Brun, P., Cantatore, Giovanni, 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., Diago, A., Döbrich, B., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer Ribas, E., Galán, J., García, J. A., Garza, J. G., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gómez, H., Gonźlez Díaz, D., Guendelman, E., Hailey, C. J., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Irastorza, I. G, Isern, J., Imai, K., Jakobsen, A. C., Jaeckel, J., 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, V. N., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Ringwald, A., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., Kate, H. Ten, Tomas, A., Troitsky, S., Vafeiadis, T., Bibber, K. Van, Vedrine, P., Villar, J. A., Vogel, J. K., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., and Zioutas, K.

Subjects
MICROPIC, Physics - Instrumentation and Detectors, Photon, axions, Parameter space, 7. Clean energy, High Energy Physics - Experiment, Dark Matter detectors (WIMPs, axions, etc.), High Energy Physics - Experiment (hep-ex), Observatory, etc.), Micropattern gaseous detectors (MSGC, GEM, THGEM, RETHGEM, MHSP, MICROPIC, MICROMEGAS, InGrid, etc), Detectors and Experimental Techniques, Instrumentation, Mathematical Physics, Physics, GEM, solar [axion], Dark Matter Detectors (Wimps, Axions, etc.), MicroMegas detector, X-ray detectors, Instrumentation and Detectors (physics.ins-det), Large detector systems for particle and astroparticle physics, solar, observatory, MICROMEGAS, MHSP, axion-like particles, proposed experiment, dark matter detectors, x-ray detectors, Micropattern gaseous detectors, large detector systems for particle and astroparticle physics, Micromegas, X-ray detector, Particle physics, optics [X-ray], FOS: Physical sciences, Superconducting magnet, Micropattern gaseous detectors (MSGC, ddc:610, Axion, activity report, Dark Matter detectors (WIMPs, superconductivity [magnet], etc), Helioscope, sensitivity, InGrid, RETHGEM, Orders of magnitude (time), axion, Large detector systems for particle and astroparticle physic, THGEM, Micropattern Gaseous Detectors (MSGC, Gem, THGEM, Rethgem, MHSP, Micropic, Micromegas, In Grid
Abstract

The International Axion Observatory (IAXO) will be a forth generation axion helioscope. As its primary physics goal, IAXO will look for axions or axion-like particles (ALPs) originating in the Sun via the Primakoff conversion of the solar plasma photons. In terms of signal-to-noise ratio, IAXO will be about 4-5 orders of magnitude more sensitive than CAST, currently the most powerful axion helioscope, reaching sensitivity to axion-photon couplings down to a few $\times 10^{-12}$ GeV$^{-1}$ and thus probing a large fraction of the currently unexplored axion and ALP parameter space. IAXO will also be sensitive to solar axions produced by mechanisms mediated by the axion-electron coupling $g_{ae}$ with sensitivity $-$for the first time$-$ to values of $g_{ae}$ not previously excluded by astrophysics. With several other possible physics cases, IAXO has the potential to serve as a multi-purpose facility for generic axion and ALP research in the next decade. In this paper we present the conceptual design of IAXO, which follows the layout of an enhanced axion helioscope, based on a purpose-built 20m-long 8-coils toroidal superconducting magnet. All the eight 60cm-diameter magnet bores are equipped with focusing x-ray optics, able to focus the signal photons into $\sim 0.2$ cm$^2$ spots that are imaged by ultra-low-background Micromegas x-ray detectors. The magnet is built into a structure with elevation and azimuth drives that will allow for solar tracking for $\sim$12 h each day., Comment: 47 pages, submitted to JINST

Published
2014
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19. X-ray detection with Micromegas with background levels below 10-6keV-1cm-2s-1

Author

D.C. Herrera, F. Aznar, E. Ferrer-Ribas, D. Calvet, T. Geralis, S. Aune, J. Galán, A. Gardikiotis, A Rodríguez, J.P. Mols, Haley Louise Gomez, G. Luzón, D. Jourde, J. A. García, G. Fanourakis, T. Vafeiadis, L. Segui, T. Dafni, J. G. Garza, A. Diago, Diego González-Díaz, F. Druillole, F.J. Iguaz, A. Tomás, T. Papaevangelou, H. Mirallas, I. G. Irastorza, Ioannis Giomataris, S. C. Yildiz, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR144753, and Yıldız, Süleyman Cenk

Subjects
Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, 01 natural sciences, Nuclear physics, 0103 physical sciences, Detectors and Experimental Techniques, X-ray Detectors, 010306 general physics, Instrumentation, Axion, Mathematical Physics, Physics, Helioscope, COSMIC cancer database, Muon, Gaseous Detectors, Micropattern Gaseous Detectors, 010308 nuclear & particles physics, Detector, X-ray, MicroMegas detector, Instrumentation and Detectors (physics.ins-det), Dark Matter Detectors, High Energy Physics::Experiment, Beam (structure)
Abstract

Micromegas detectors are an optimum technological choice for the detection of low energy x-rays. The low background techniques applied to these detectors yielded remarkable background reductions over the years, being the CAST experiment beneficiary of these developments. In this document we report on the latest upgrades towards further background reductions and better understanding of the detectors' response. The upgrades encompass the readout electronics, a new detector design and the implementation of a more efficient cosmic muon veto system. Background levels below 10$^{-6}$keV$^{-1}$cm$^{-2}$s$^{-1}$ have been obtained at sea level for the first time, demonstrating the feasibility of the expectations posed by IAXO, the next generation axion helioscope. Some results obtained with a set of measurements conducted in the x-ray beam of the CAST Detector Laboratory will be also presented and discussed. Micromegas detectors are an optimum technological choice for the detection of low energy x-rays. The low background techniques applied to these detectors yielded remarkable background reductions over the years, being the CAST experiment beneficiary of these developments. In this document we report on the latest upgrades towards further background reductions and better understanding of the detectors' response. The upgrades encompass the readout electronics, a new detector design and the implementation of a more efficient cosmic muon veto system. Background levels below 10−6keV-1cm-2s-1 have been obtained at sea level for the first time, demonstrating the feasibility of the expectations posed by IAXO, the next generation axion helioscope. Some results obtained with a set of measurements conducted in the x-ray beam of the CAST Detector Laboratory will be also presented and discussed. Micromegas detectors are an optimum technological choice for the detection of low energy x-rays. The low background techniques applied to these detectors yielded remarkable background reductions over the years, being the CAST experiment beneficiary of these developments. In this document we report on the latest upgrades towards further background reductions and better understanding of the detectors' response. The upgrades encompass the readout electronics, a new detector design and the implementation of a more efficient cosmic muon veto system. Background levels below 10$^{-6}$keV$^{-1}$cm$^{-2}$s$^{-1}$ have been obtained at sea level for the first time, demonstrating the feasibility of the expectations posed by IAXO, the next generation axion helioscope. Some results obtained with a set of measurements conducted in the x-ray beam of the CAST Detector Laboratory will be also presented and discussed.

Published
2013

20. CAST microbulk micromegas in the Canfranc Underground Laboratory

Author

L. Segui, A Rodríguez, J. A. Garcia, S. C. Yildiz, Hector Gomez, I. Giomataris, T. Papaevangelou, T. Geralis, A. Tomás, J. G. Garza, J. Ruz, Javier Galan, G. Luzón, S. Aune, I. G. Irastorza, T. Vafeiadis, D.C. Herrera, Georgios Fanourakis, A. Gardikiotis, F.J. Iguaz, E. Ferrer-Ribas, and T. Dafni

Subjects
Physics, Physics - Instrumentation and Detectors, axions, microbulk, 010308 nuclear & particles physics, Canfranc Underground Laboratory, Underground Physics, Detector, FOS: Physical sciences, MicroMegas detector, ultra-low background, Instrumentation and Detectors (physics.ins-det), Physics and Astronomy(all), 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Astrophysics - Solar and Stellar Astrophysics, 0103 physical sciences, Electromagnetic shielding, Rare Event Searches, Detectors and Experimental Techniques, 010306 general physics, Micromegas, Solar and Stellar Astrophysics (astro-ph.SR)
Abstract

During the last taking data campaigns of the CAST experiment, the micromegas detectors have achieved background levels of $\approx 5 \times 10^{-6}$keV$^{-1}$cm$^{-2}$s$^{-1}$ between 2 and 9 keV. This performance has been possible thanks to the introduction of the microbulk technology, the implementation of a shielding and the development of discrimination algorithms. It has motivated new studies towards a deeper understanding of CAST detectors background. One of the working lines includes the construction of a replica of the set-up used in CAST by micromegas detectors and its installation in the Canfranc Underground Laboratory. Thanks to the comparison between the performance of the detectors underground and at surface, shielding upgrades, etc, different contributions to the detectors background have been evaluated. In particular, an upper limit $< 2 \times 10^{-7}$keV$^{-1}$cm$^{-2}$s$^{-1}$ for the intrinsic background of the detector has been obtained. This work means a first evaluation of the potential of the newest micromegas technology in an underground laboratory, the most suitable environment for Rare Event Searches., 6 pages, 8 figures. To appear in the proceedings of the 2nd International Conference on Technology and Instrumentation for Particle Physics (TIPP 2011)

Published
2012
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21. Rare event searches based on micromegas detectors: The T-REX project

Author

I. Giomataris, A. Gardikiotis, A Rodríguez, J. G. Garza, J. Ruz, T. Papaevangelou, J. A. Garcia, S. C. Yildiz, A. Tomás, G. Luzón, Javier Galan, Georgios Fanourakis, T. Dafni, Theodoros Vafeiadis, Hector Gomez, F.J. Iguaz, T. Geralis, L. Segui, S. Aune, S. Cebrián, D.C. Herrera, I. G. Irastorza, E. Ferrer-Ribas, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, and Yıldız, Süleyman Cenk

Subjects
Physics, Micromegas Detector, History, Particle physics, Helioscope, 010308 nuclear & particles physics, Gain Stability, Detector, MicroMegas detector, Rare Event, 01 natural sciences, Computer Science Applications, Education, Time Projection Chambers, Double beta decay, 0103 physical sciences, Rare events, Energy Resolutions, 010306 general physics, Double Beta Decay, Axion, Micromegas
Abstract

Yıldız, Süleyman Cenk (Dogus Author) -- The conference paper was firstly submitted to 12th International Conference on Topics in Astroparticle and Underground Physics. Micromegas readouts are an attractive option for many of the rare event searches, due to their performance regarding energy resolution, gain stability, homogeneity and material budget. The T-REX project aims at developing further these novel readout techniques for Time Projection Chambers and their potential use in experiments searching for rare events. Here we will refer to the latest results regarding the use and prospects of Micromegas read-outs in axion physics (CAST and the future helioscope), as well as the R&D carried out within NEXT, to search for the neutrinoless double-beta decay.

Published
2012

22. Search for Sub-eV Mass Solar Axions by the CERN Axion Solar Telescope withHe3Buffer Gas

Author

K. Königsmann, T. Dafni, J. M. Laurent, Joachim Jacoby, Sergei Gninenko, Milica Krčmar, Ante Ljubičić, Biljana Lakić, Hector Gomez, F. Haug, Marin Karuza, Evangelos Gazis, T. Guthörl, C. Eleftheriadis, H. Riege, J. Morales, A. Liolios, N. Elias, Heinrich Bräuninger, José Villar, Serkant Ali Cetin, G. Lutz, S. Aune, A. Tomás, A. Nordt, V. Lozza, M. Arik, T. Geralis, I. Giomataris, K. van Bibber, T. Papaevangelou, I. Savvidis, Javier Galan, Dieter Hoffmann, M. Tsagri, J. Ruz, Sami K. Solanki, J. A. Garcia, M. Rosu, Markus Kuster, Krešimir Jakovčić, T. O. Niinikoski, Peter Friedrich, P. S. Silva, M. J. Pivovaroff, Konstantin Zioutas, A. Gardikiotis, M. Davenport, Raimo Hartmann, Julia Vogel, J. I. Collar, Theodoros Vafeiadis, K. Barth, G. Luzón, Adriane De Assis Lawisch Rodriguez, E. Ferrer-Ribas, C. Ezer, A. Belov, Rainer Kotthaus, L. Stewart, I. G. Irastorza, Georg G. Raffelt, Georgios Fanourakis, S. C. Yildiz, Timur Rashba, M. D. Hasinoff, J. M. Carmona, E. Gruber, S. Borghi, Giovanni Cantatore, and F.J. Iguaz

Subjects
Physics, Helioscope, Particle physics, Solar energetic particles, 010308 nuclear & particles physics, Hot dark matter, Dark matter, General Physics and Astronomy, Astrophysics, 01 natural sciences, 7. Clean energy, Massless particle, 0103 physical sciences, Strong CP problem, 010306 general physics, CERN Axion Solar Telescope, Axion
Abstract

The CERN Axion Solar Telescope (CAST) has extended its search for solar axions by using (3)He as a buffer gas. At T=1.8 K this allows for larger pressure settings and hence sensitivity to higher axion masses than our previous measurements with (4)He. With about 1 h of data taking at each of 252 different pressure settings we have scanned the axion mass range 0.39 eV≲m(a)≲0.64 eV. From the absence of excess x rays when the magnet was pointing to the Sun we set a typical upper limit on the axion-photon coupling of g(aγ)≲2.3×10(-10) GeV(-1) at 95% C.L., the exact value depending on the pressure setting. Kim-Shifman-Vainshtein-Zakharov axions are excluded at the upper end of our mass range, the first time ever for any solar axion search. In the future we will extend our search to m(a)≲1.15 eV, comfortably overlapping with cosmological hot dark matter bounds.

Published
2011
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23. Status of R&D on Micromegas for Rare Event Searches: The T-REX project

Author

Alicia Rodríguez, L. Segui, J. G. Garza, G. Fanourakis, A. Ortiz, Haley Louise Gomez, J.P. Mols, S. C. Yildiz, Theodoros Geralis, Thomas Papaevangelou, D.C. Herrera, S. Cebrián, G. Luzón, L. Esteban, A. Gardikiotis, T. Vafeiadis, J. Galán, J. A. García, E. Ferrer-Ribas, D. Fortuño, J. Ruz, T. Dafni, J. Castel, F.J. Iguaz, A. Tomás, Ioannis Giomataris, and I. G. Irastorza

Subjects
Physics, Helioscope, Particle physics, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, General Engineering, Astronomy and Astrophysics, MicroMegas detector, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, Space and Planetary Science, 0103 physical sciences, 010306 general physics, Axion
Abstract

The T-REX project aims at developing novel readout techniques for Time Projection Chambers in experiments searching for rare events. The enhanced performance of the latest Micromegas readouts in issues like energy resolution, gain stability, homogeneity, material budget, combined with low background techniques, is opening new windows of opportunity for their application in this field. Here we review the latest results regarding the use and prospects of Micromegas readouts in axion physics (CAST and the future helioscope), as well as the R&D carried out within NEXT, to search for the neutrinoless double-beta decay., Comment: Proceedings of the 3rd International conference on Directional Detection of Dark Matter (CYGNUS 2011), Aussois, France, 8-10 June 2011

Published
2011

24. Search for Sub-eV Mass Solar Axions by the CERN Axion Solar Telescope with (3)He Buffer Gas

Author

M, Arik, S, Aune, K, Barth, A, Belov, S, Borghi, H, Bräuninger, G, Cantatore, J M, Carmona, S A, Cetin, J I, Collar, T, Dafni, M, Davenport, C, Eleftheriadis, N, Elias, C, Ezer, G, Fanourakis, E, Ferrer-Ribas, P, Friedrich, J, Galán, J A, García, A, Gardikiotis, E N, Gazis, T, Geralis, I, Giomataris, S, Gninenko, H, Gómez, E, Gruber, T, Guthörl, R, Hartmann, F, Haug, M D, Hasinoff, D H H, Hoffmann, F J, Iguaz, I G, Irastorza, J, Jacoby, K, Jakovčić, M, Karuza, K, Königsmann, R, Kotthaus, M, Krčmar, M, Kuster, B, Lakić, J M, Laurent, A, Liolios, A, Ljubičić, V, Lozza, G, Lutz, G, Luzón, J, Morales, T, Niinikoski, A, Nordt, T, Papaevangelou, M J, Pivovaroff, G, Raffelt, T, Rashba, H, Riege, A, Rodríguez, M, Rosu, J, Ruz, I, Savvidis, P S, Silva, S K, Solanki, L, Stewart, A, Tomás, M, Tsagri, K, van Bibber, T, Vafeiadis, J A, Villar, J K, Vogel, S C, Yildiz, K, Zioutas, Arik, M., Aune, S., Barth, K., Belov, A., Borghi, S., Brauninger, H., Cantatore, Giovanni, Carmona, J. M., Cetin, S. A., Collar, J. I., Dafni, T., Davenport, M., Eleftheriadis, C., Elias, N., Ezer, C., Fanourakis, G., Ferrer Ribas, E., Friedrich, P., Galan, J., Garcia, J. A., Gardikiotis, A., Gazis, E. N., Geralis, T., Giomataris, I., Gninenko, S., Gomez, H., Gruber, E., Guthorl, T., Hartmann, R., Haug, F., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jacoby, J., Jakovcic, K., Karuza, M., Konigsmann, K., Kotthaus, R., Krcmar, M., Kuster, M., Lakic, B., Laurent, J. M., Liolios, A., Ljubicic, A., Lozza, Valentina, Lutz, G., Luzon, G., Morales, J., Niinikoski, T., Nordt, A., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Rashba, T., Riege, H., Rodriguez, A., Rosu, M., Ruz, J., Savvidis, I., Silva, P. S., Solanki, S. K., Stewart, L., Tomas, A., Tsagri, M., van Bibber, K., Vafeiadis, T., Villar, J. A., Vogel, J. K., Yildiz, S. C., and Zioutas, K.

Subjects
solar axion, low background detectors, solar axions, photons, dark matter
Abstract

The CERN Axion Solar Telescope (CAST) has extended its search for solar axions by using (3)He as a buffer gas. At T=1.8 K this allows for larger pressure settings and hence sensitivity to higher axion masses than our previous measurements with (4)He. With about 1 h of data taking at each of 252 different pressure settings we have scanned the axion mass range 0.39 eV≲m(a)≲0.64 eV. From the absence of excess x rays when the magnet was pointing to the Sun we set a typical upper limit on the axion-photon coupling of g(aγ)≲2.3×10(-10) GeV(-1) at 95% C.L., the exact value depending on the pressure setting. Kim-Shifman-Vainshtein-Zakharov axions are excluded at the upper end of our mass range, the first time ever for any solar axion search. In the future we will extend our search to m(a)≲1.15 eV, comfortably overlapping with cosmological hot dark matter bounds.

Published
2011

25. Low background x-ray detection with Micromegas for axion research

Author

J. Castel, T. Vafeiadis, A Rodríguez, J. A. García, A. Gardikiotis, T. Dafni, T. Geralis, J. Galán, Haley Louise Gomez, D. Jourde, M. Davenport, G. Fanourakis, J.P. Mols, S. Aune, D.C. Herrera, L. Segui, S. C. Yildiz, T. Papaevangelou, G. Luzón, I. G. Irastorza, Ioannis Giomataris, F.J. Iguaz, A. Tomás, E. Ferrer-Ribas, J. Ruz, J. G. Garza, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR144753, and Belirlenecek

Subjects
Physics, Particle physics, Helioscope, Canfranc Underground Laboratory, Micropattern Gaseous Detectors (MSGC, GEM, THGEM, RETHGEM, MHSP, MICROPIC, MICROMEGAS, Ingrid, etc), Detector, Dark Matter Detectors (Wimps, Axions, etc.), X-ray detector, MicroMegas detector, Time Projection Chambers (TPC), Observatory, X-Ray Detectors, CERN Axion Solar Telescope, Instrumentation, Axion, Mathematical Physics
Abstract

Axion helioscopes aim at the detection of solar axions through their conversion into x-rays in laboratory magnetic fields. The use of low background x-ray detectors is an essential component contributing to the sensitivity of these searches. Here we review the recent advances on Micromegas detectors used in the CERN Axion Solar Telescope (CAST) and proposed for the future International Axion Observatory (IAXO). The most recent Micromegas setups in CAST have achieved background levels of 1 . 5 x 10(6) keV(-1) cm(-2) s(-1), a factor of more than 100 lower than the ones obtained by the first generation of CAST detectors. This improvement is due to the development of active and passive shielding techniques, offline discrimination techniques allowed by highly granular readout patterns, as well as the use of radiopure detector components. The status of the intensive R&D to reduce the background levels will be described, including the operation of replica detectors in test benches and the detailed Geant4 simulation of the detector setup and the detector response, which has allowed the progressive understanding of background origins. The best levels currently achieved in a test setup operating in the Canfranc Underground Laboratory (LSC) are as low as similar to 10(7) keV(-1) cm(-2) s(-1), showing the good prospects of this technology for application in the future IAXO.

Published
2014
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26. The T-REX project: Micromegas for Rare Event Searches

Author

I. G. Irastorza, F.J. Iguaz, S. Aune, Georgios Fanourakis, J. F. Castel, A. Ortiz, Hector Gomez, T. Geralis, S. C. Yildiz, T. Dafni, G. Luzón, E. Ferrer-Ribas, A. Tomás, A. Gardikiotis, Javier Galan, L. Segui, D.C. Herrera, J. G. Garza, A Rodríguez, T. Papaevangelou, J. A. Garcia, Theodoros Vafeiadis, I. Giomataris, D. Fortuño, S. Cebrián, J.P. Mols, J. Ruz, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, and Yıldız, Şükrü C.

Subjects
Micromegas Detector, Physics, History, Particle physics, 010308 nuclear & particles physics, Event (computing), Time Resolution, Real-time computing, MicroMegas detector, Time resolution, Rare Event, Low Background, 01 natural sciences, Computer Science Applications, Education, Time Projection Chambers, Clouds, Double beta decay, 0103 physical sciences, Rare events, High Energy Physics, Double Beta Decay, 010306 general physics, Projection (set theory), Micromegas
Abstract

Yıldız, Şükrü C. (Dogus Author) -- This paper was firstyly submitted to 2nd International Conference on Particle Physics in Memoriam Engin Arik and Her Colleagues. The T-REX project aims at developing novel readout techniques for Time Projection Chambers for experiments searching for Rare Events. The Micromegas detectors are a good option, because of their good performance regarding low background levels, energy and time resolution, gain and stability of operation. In the present we will shortly refer to two particular cases, on one hand their performance in the CAST experiment and on the other the studies carried out within NEXT, a neutrinoless double-beta decay experiment.

Published
2012
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27. Performance of micromegas detectors in the CAST Experiment

Author

M. Davenport, I. Giomataris, A Rodríguez, F.J. Iguaz, T. Dafni, J. A. Garcia, E. Ferrer-Ribas, S. Aune, S. C. Yildiz, Hector Gomez, T. Papaevangelou, T. Geralis, Theodoros Vafeiadis, A. Gardikiotis, I. G. Irastorza, J. G. Garza, J. Ruz, A. Tomás, Javier Galan, Georgios Fanourakis, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, and Yıldız, Şükrü C.

Subjects
History, Physics::Instrumentation and Detectors, Rare Event, 01 natural sciences, X-ray Detector, Education, Nuclear physics, Optics, 0103 physical sciences, High Energy Physics, CERN Axion Solar Telescopes, 010306 general physics, Axion, Image resolution, Bosons, Physics, Time projection chamber, Expected Energy, 010308 nuclear & particles physics, business.industry, Canfranc Underground Laboratory, Detector, Detectors, MicroMegas detector, Computer Science Applications, Magnetic Fields, Spatial Resolution, High Energy Physics::Experiment, Charge-coupled device, Experiments, business, CERN Axion Solar Telescope, Micromegas
Abstract

Yıldız, Şükrü C. (Dogus Author) -- This paper was firstly submitted to 2nd International Conference on Particle Physics in Memoriam Engin Arik and Her Colleagues. CERN Axion Solar Telescope (CAST) experiment is searching for axions coming from the Sun. Inside transverse magnetic fields, axions can be converted into X-rays, which can be detected by X-ray detectors. The expected energy of the signal in CAST is in the 1-10 keV range. Low noise and low background detectors are necessary to increase the sensitivity of the experiment. Micro Mesh Gaseous Structure (micromegas) detectors have been used in CAST since the beginning, providing good energy and spatial resolution for CAST's needs. CAST has been intensely studying micromegas detectors to develop new technologies. Initially, CAST detectors consisted of a micromegas, a Time Projection Chamber (TPC) and a Charged Couple Device (CCD), however the improvements in micromegas technologies encouraged CAST to replace the TPC with 2 new micromegas detectors. In some periods during CAST run, ultra low background has been observed in one of the micromegas detectors and it is being investigated through simulations and laboratory tests carried out at Canfranc Underground Laboratory. If this low background is indeed not a systematic effect, it can open new possibilities on rare event searches.

Published
2012
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28. Improved search for solar chameleons with a GridPix detector at CAST

Author

Wolfgang Funk, Milica Krčmar, T. Geralis, M. Maroudas, S. C. Yildiz, I. G. Irastorza, Joachim Jacoby, Sofia Kostoglou, Babette Döbrich, Sergei Gninenko, Giovanni Cantatore, C. Krieger, Søren Schmidt, M. Davenport, Marin Karuza, I. Ortega, M. J. Pivovaroff, Konstantin Zioutas, C. J. Hailey, J. Ruz, S. Neff, L. Miceli, T. Papaevangelou, S. Aune, Georg G. Raffelt, T. Dafni, I. Savvidis, M. Vretenar, Klaus Kurt Desch, Biljana Lakić, A. Liolios, Georgios Fanourakis, Nenad Kralj, Alexander Dermenev, J. F. Castel, A. Belov, Krešimir Jakovčić, L. Stewart, Dieter Hoffmann, Sami K. Solanki, Heinrich Bräuninger, Serkant Ali Cetin, E. Ruiz Chóliz, F.J. Iguaz, Vassilis Anastassopoulos, H. Fischer, A. Gardikiotis, Yannis K. Semertzidis, M. D. Hasinoff, C. Eleftheriadis, Jochen Kaminski, Anders Clemen Jakobsen, K. Paraschou, E. Ferrer-Ribas, J. M. Carmona, Julia Vogel, Theodoros Vafeiadis, J. G. Garza, K. Barth, G. Luzón, Walter Wuensch, I. Giomataris, M. Rosu, P. Brax, Ante Ljubičić, J. M. Laurent, J. A. Garcia, Evangelos Gazis, Finn Erland Christensen, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Théorique - UMR CNRS 3681 (IPHT), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), CAST, Anastassopoulos, V., Aune, S., Barth, K., Belov, A., Bräuninger, H., Cantatore, G., Carmona, J. M., Castel, J. F., Cetin, S. A., Christensen, F., Dafni, T., Davenport, M., Dermenev, A., Desch, K., Döbrich, B., Eleftheriadis, C., Fanourakis, G., Ferrer-Ribas, E., Fischer, H., Funk, W., García, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Geralis, T., Giomataris, I., Gninenko, S., Hailey, C. J., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jakobsen, A., Jacoby, J., Jakovčić, K., Kaminski, J., Karuza, M., Kostoglou, S., Kralj, N., Krčmar, M., Krieger, C., Lakić, B., Laurent, J. M., Liolios, A., Ljubičić, A., Luzón, G., Maroudas, M., Miceli, L., Neff, S., Ortega, I., Papaevangelou, T., Paraschou, K., Pivovaroff, M. J., Raffelt, G., Rosu, M., Ruz, J., Chóliz, E. Ruiz, Savvidis, I., Schmidt, S., Semertzidis, Y. K., Solanki, S. K., Stewart, L., Vafeiadis, T., Vogel, J. K., Vretenar, M., Wuensch, W., Yildiz, S. C., Zioutas, K., and Brax, P.

Subjects
Physics - Instrumentation and Detectors, Photon, Physics::Instrumentation and Detectors, Solar luminosity, magnetic field, Astrophysics, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), photon: coupling, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Astrophysics::Solar and Stellar Astrophysics, Detectors and Experimental Techniques, GridPix, dark energy, modified gravity, physics.ins-det, Solar physics, Physics, dark energy experiments, particle physics - cosmology connection, solar physics, Astronomy and Astrophysics, chameleon: solar, solar physic, Instrumentation and Detectors (physics.ins-det), Coupling (probability), transition: (axion photon), dark energy experiment, Beta (plasma physics), Physics::Space Physics, CAST, Astrophysics::Earth and Planetary Astrophysics, CERN Axion Solar Telescope, Particle Physics - Experiment, chameleon, Modified gravity, Particle physics, CERN Lab, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, photon: spectrum, coupling constant: upper limit, Tachocline, Astrophysics::Cosmology and Extragalactic Astrophysics, X-ray, Dark energy experiments, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Sensitivity (control systems), hep-ex, background, 010308 nuclear & particles physics, magnet, coupling: (axion 2photon), Particle physics - cosmology connection, axion: solar, tachocline, Energy (signal processing), experimental results
Abstract

We report on a new search for solar chameleons with the CERN Axion Solar Telescope (CAST). A GridPix detector was used to search for soft X-ray photons in the energy range from 200 eV to 10 keV from converted solar chameleons. No signiffcant excess over the expected background has been observed in the data taken in 2014 and 2015. We set an improved limit on the chameleon photon coupling, $\beta_\gamma < 5.7\times10^{10}$ for $1, Comment: 19 pages, 12 figures, 3 tables

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29. Search for Solar Axions by the CERN Axion Solar Telescope with He3 Buffer Gas: Closing the Hot Dark Matter Gap

Author

Arik, M., Aune, S., Barth, K., Belov, A., Borghi, S., Brauninger, H., Cantatore, Giovanni, Carmona, J. M., Cetin, S. A., Da Riva, J. I. Collar E., Dafni, T., Davenport, M., Eleftheriadis, C., Elias, N., Fanourakis, G., Ferrer Ribas, E., Friedrich, P., Galan, J., Garcia, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Geralis, T., Georgiopoulou, E., Giomataris, I., Gninenko, S., Gomez, H., Gomez Marzoa, M., Gruber, E., Guthorl, T., Hartmann, R., Hauf, S., Haug, F., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jacoby, J., Jakovcic, K., Karuza, M., Konigsmann, K., Kotthaus, R., Krcmar, M., Kuster, M., Lakic, B., Lang, P. M., Laurent, J. M., Liolios, A., Ljubicic, A., Lozza, V., Luzon, G., Neff, S., Niinikoski, T., Nordt, A., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Riege, H., Rodriguez, A., Rosu, M., Ruz, J., Savvidis, I., Shilon, I., Silva, P. S., Solanki, S. K., Stewart, L., Tomas, A., Tsagri, M., van Bibber, K., Vafeiadis, T., Villar, J., Vogel, J. K., Yildiz, S. C., Zioutas, K., M., Arik, S., Aune, K., Barth, A., Belov, S., Borghi, H., Brauninger, Cantatore, Giovanni, J. M., Carmona, S. A., Cetin, J. I. Collar E., Da Riva, T., Dafni, M., Davenport, C., Eleftheriadi, N., Elia, G., Fanouraki, E., Ferrer Riba, P., Friedrich, J., Galan, J. A., Garcia, A., Gardikioti, J. G., Garza, E. N., Gazi, T., Gerali, E., Georgiopoulou, I., Giomatari, S., Gninenko, H., Gomez, M., Gomez Marzoa, E., Gruber, T., Guthorl, R., Hartmann, S., Hauf, F., Haug, M. D., Hasinoff, D. H. H., Hoffmann, F. J., Iguaz, I. G., Irastorza, J., Jacoby, K., Jakovcic, M., Karuza, K., Konigsmann, R., Kotthau, M., Krcmar, M., Kuster, B., Lakic, P. M., Lang, J. M., Laurent, A., Liolio, A., Ljubicic, V., Lozza, G., Luzon, S., Neff, T., Niinikoski, A., Nordt, T., Papaevangelou, M. J., Pivovaroff, G., Raffelt, H., Riege, A., Rodriguez, M., Rosu, J., Ruz, I., Savvidi, I., Shilon, P. S., Silva, S. K., Solanki, L., Stewart, A., Toma, M., Tsagri, K., van Bibber, T., Vafeiadi, J., Villar, J. K., Vogel, S. C., Yildiz, and K., Zioutas

Subjects
solar axions, dark matter, Photon detection, solar axion, Physics::Instrumentation and Detectors, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics
Abstract

The CERN Axion Solar Telescope (CAST) has finished its search for solar axions with 3^He buffer gas, covering the search range 0.64 eV < m_a

Published
2014

30. CAST: Status and latest results

Author

Dafni, T., Aune, S., Davenport, M., Eleftheriadis, C., Elias, N., Ezer, C., Fanourakis, G., Ferrer-Ribas, E., Friedrich, P., Galan, J., Garcia, J. A., Gardikiotis, A., Barth, K., Gazis, E. N., Geralis, T., Giomataris, I., Gninenko, S., Gomez, H., Gruber, E., Guthorl, T., Hartmann, R., Haug, F., Hasinoff, M. D., Belov, A., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jacoby, J., Jakovcic, K., Karuza, M., Konigsmann, K., Kotthaus, R., Krcmar, M., Kuster, M., Borghi, S., Lakic, B., Laurent, J. M., Liolios, A., Ljubicic, A., Lozza, V., Lutz, G., Luzon, G., Morales, J., Niinikoski, T., Nordt, A., Brauninger, H., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Rashba, T., Riege, H., Rodriguez, A., Rosu, M., Ruz, J., Savvidis, I., Silva, P. S., Cantatore, G., Solanki, S. K., Stewart, L., Tomas, A., Tsagri, M., van Bibber, K., Vafeiadis, T., Villar, J., Vogel, J. K., Yildiz, S. C., Zioutas, K., Carmona, J. M., CAST Collaboration, Cetin, S. A., Collar, J. I., K. Zioutas, M. Schumann, T., Dafni, S., Aune, K., Barth, A., Belov, S., Borghi, H., Brauninger, Cantatore, Giovanni, J. M., Carmona, S. A., Cetin, J. I., Collar, M., Davenport, C., Eleftheriadi, N., Elia, C., Ezer, G., Fanouraki, E., Ferrer Riba, P., Friedrich, J., Galan, J. A., Garcia, A., Gardikioti, E. N., Gazi, T., Gerali, I., Giomatari, S., Gninenko, H., Gomez, E., Gruber, T., Guthorl, R., Hartmann, F., Haug, M. D., Hasinoff, D. H. H., Hoffmann, F. J., Iguaz, I. G., Irastorza, J., Jacoby, K., Jakovcic, M., Karuza, K., Konigsmann, R., Kotthau, M., Krcmar, M., Kuster, B., Lakic, J. M., Laurent, A., Liolio, A., Ljubicic, V., Lozza, G., Lutz, G., Luzon, J., Morale, T., Niinikoski, A., Nordt, T., Papaevangelou, M. J., Pivovaroff, G., Raffelt, T., Rashba, H., Riege, A., Rodriguez, M., Rosu, J., Ruz, I., Savvidi, P. S., Silva, S. K., Solanki, L., Stewart, A., Toma, M., Tsagri, K., van Bibber, T., Vafeiadi, J., Villar, J. K., Vogel, S. C., Yildiz, and K., Zioutas

Subjects
WISPs, solar axion, WISP, Physics, photon detectors, solar axions
Abstract

In July 2011, CAST finished the data-taking of its nominal programme, having scanned axion masses up to ~1.18 eV/c**2. Here we present the first results of the data taken in 2008, first year of the last data-taking campaign when $^3$He was used inside the magnet bores. No excess of signal over background has been recorded, and an upper limit has been set to the axion-to-photon coupling to 2.3*10**-10 GeV**-1 for axion masses between 0.39 and 0.64 eV. CAST remains the most sensitive axion helioscope and for the first time crosses the benchmark line of the KSVZ model at the upper end of the spectrum., Proc. of Patras Workshop on Axions, WIMPs and WISPs, 93 - 97; DESY-PROC-2011-04; ISSN 1435-8077

Published
2011
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