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High-resolution for IAXO: MMC-based X-ray detectors
Axion helioscopes like the planned International Axion Observatory (IAXO) search for evidence of axions and axion-like particles (ALPs) from the Sun. A strong magnetic field is used to convert ALPs into photons via the generic ALP-photon coupling. To observe the resulting photons, X-ray detectors wi...
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Published in: | Journal of instrumentation 2021-06, Vol.16 (6), p.P06006 |
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Main Authors: | , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Axion helioscopes like the planned International Axion
Observatory (IAXO) search for evidence of axions and axion-like
particles (ALPs) from the Sun. A strong magnetic field is used to
convert ALPs into photons via the generic ALP-photon coupling. To
observe the resulting photons, X-ray detectors with low background
and high efficiency are necessary. In addition, good energy
resolution and low energy threshold would allow for investigating
the ALP properties by studying the X-ray spectrum after its
discovery. We propose to use low temperature metallic magnetic
calorimeters (MMCs). Here we present the first detector system based
on MMCs developed for IAXO and discuss the results of the
characterization. The detector consists of a two-dimensional
64-pixel array covering an active area of
16mm
2
with a fill factor of
93%. We achieve an average energy resolution of
6.1 eV FWHM allowing for energy thresholds below
100 eV. This detector is the first step towards a
larger 1 cm
2
array matching the IAXO X-ray
optics. We determine the background rate for an unshielded detector
system in the energy range between 1 keV and
10 keV to be
3.2(1) Ă— 10
-4
keV
-1
cm
-2
s
-1
from events acquired over 30 days. In the future, active and
passive shields will significantly reduce the background induced by
cosmic muons and natural radioactivity. Our results demonstrate that
MMCs are a promising technology for helioscopes to discover and
study ALPs. |
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ISSN: | 1748-0221 1748-0221 |
DOI: | 10.1088/1748-0221/16/06/P06006 |