A Micromegas-based low-background x-ray detector coupled to a slumped-glass telescope for axion research
Abstract
Here, we report on the design, construction and operation of a low background x-ray detection line composed of a shielded Micromegas detector of the microbulk technology. The detector is made from radiopure materials and is placed at the focal point of a ~ 5 cm diameter, 1.5 m focal-length, cone-approximation Wolter I x-ray telescope (XRT) assembled from thermally-formed (or "slumped") glass substrates deposited with multilayer coatings. The system has been conceived as a technological pathfinder for the future International Axion Observatory (IAXO), as it combines two of the techniques (optic and detector) proposed in the conceptual design of the project. It is innovative for two reasons: it is the first time an x-ray optic has been designed and fabricated specifically for axion research, and the first time a Micromegas detector has been operated with an x-ray optic. The line has been installed at one end of the CERN Axion Solar Telescope (CAST) magnet and is currently looking for solar axions. Furthermore, the combination of the XRT and Micromegas detector provides the best signal-to-noise ratio obtained so far by any detection system of the CAST experiment with a background rate of 5.4×10–3 counts per hour in the energy region-of-interest and signalmore »
- Authors:
-
more »
- Univ. de Zaragoza, Zaragoza (Spain)
- Technical Univ. of Denmark. Lyngby (Denmark)
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- CEA, Gif-sur-Yvette (France)
- Columbia Univ., New York, NY (United States)
- Aristotle Univ. of Thessaloniki, Thessaloniki (Greece)
- Publication Date:
- Research Org.:
- Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA)
- OSTI Identifier:
- 1476208
- Report Number(s):
- LLNL-JRNL-747464
Journal ID: ISSN 1475-7516; 932504
- Grant/Contract Number:
- AC52-07NA27344
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Cosmology and Astroparticle Physics
- Additional Journal Information:
- Journal Volume: 2015; Journal Issue: 12; Journal ID: ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; axions; dark matter detectors; dark matter experiments; X-ray telescopes
Citation Formats
Aznar, F., Castel, J., Christensen, F. E., Dafni, T., Decker, T. A., Ferrer-Ribas, E., Garcia, J. A., Giomataris, I., Garza, J. G., Hailey, C. J., Hill, R. M., Iguaz, F. J., Irastorza, I. G., Jakobsen, A. C., Luzon, G., Mirallas, H., Papaevangelou, T., Pivovaroff, M. J., Ruz, J., Vafeiadis, T., and Vogel, J. K. A Micromegas-based low-background x-ray detector coupled to a slumped-glass telescope for axion research. United States: N. p., 2015.
Web. doi:10.1088/1475-7516/2015/12/008.
Aznar, F., Castel, J., Christensen, F. E., Dafni, T., Decker, T. A., Ferrer-Ribas, E., Garcia, J. A., Giomataris, I., Garza, J. G., Hailey, C. J., Hill, R. M., Iguaz, F. J., Irastorza, I. G., Jakobsen, A. C., Luzon, G., Mirallas, H., Papaevangelou, T., Pivovaroff, M. J., Ruz, J., Vafeiadis, T., & Vogel, J. K. A Micromegas-based low-background x-ray detector coupled to a slumped-glass telescope for axion research. United States. https://doi.org/10.1088/1475-7516/2015/12/008
Aznar, F., Castel, J., Christensen, F. E., Dafni, T., Decker, T. A., Ferrer-Ribas, E., Garcia, J. A., Giomataris, I., Garza, J. G., Hailey, C. J., Hill, R. M., Iguaz, F. J., Irastorza, I. G., Jakobsen, A. C., Luzon, G., Mirallas, H., Papaevangelou, T., Pivovaroff, M. J., Ruz, J., Vafeiadis, T., and Vogel, J. K. Thu .
"A Micromegas-based low-background x-ray detector coupled to a slumped-glass telescope for axion research". United States. https://doi.org/10.1088/1475-7516/2015/12/008. https://www.osti.gov/servlets/purl/1476208.
@article{osti_1476208,
title = {A Micromegas-based low-background x-ray detector coupled to a slumped-glass telescope for axion research},
author = {Aznar, F. and Castel, J. and Christensen, F. E. and Dafni, T. and Decker, T. A. and Ferrer-Ribas, E. and Garcia, J. A. and Giomataris, I. and Garza, J. G. and Hailey, C. J. and Hill, R. M. and Iguaz, F. J. and Irastorza, I. G. and Jakobsen, A. C. and Luzon, G. and Mirallas, H. and Papaevangelou, T. and Pivovaroff, M. J. and Ruz, J. and Vafeiadis, T. and Vogel, J. K.},
abstractNote = {Here, we report on the design, construction and operation of a low background x-ray detection line composed of a shielded Micromegas detector of the microbulk technology. The detector is made from radiopure materials and is placed at the focal point of a ~ 5 cm diameter, 1.5 m focal-length, cone-approximation Wolter I x-ray telescope (XRT) assembled from thermally-formed (or "slumped") glass substrates deposited with multilayer coatings. The system has been conceived as a technological pathfinder for the future International Axion Observatory (IAXO), as it combines two of the techniques (optic and detector) proposed in the conceptual design of the project. It is innovative for two reasons: it is the first time an x-ray optic has been designed and fabricated specifically for axion research, and the first time a Micromegas detector has been operated with an x-ray optic. The line has been installed at one end of the CERN Axion Solar Telescope (CAST) magnet and is currently looking for solar axions. Furthermore, the combination of the XRT and Micromegas detector provides the best signal-to-noise ratio obtained so far by any detection system of the CAST experiment with a background rate of 5.4×10–3 counts per hour in the energy region-of-interest and signal spot area.},
doi = {10.1088/1475-7516/2015/12/008},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 12,
volume = 2015,
place = {United States},
year = {Thu Dec 03 00:00:00 EST 2015},
month = {Thu Dec 03 00:00:00 EST 2015}
}
Web of Science
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