A search for solar axion induced signals with COSINE-100

Adhikari, P.; Adhikari, G.; Souza, E. Barbosa de; Carlin, N.; Choi, S.; Djamal, Mitra; Ezeribe, A. C.; Ha, C.; Hahn, I. S.; Jeon, E. J.; Jo, J. H.; Joo, Hyun-Woo; Kang, W. G.; Kauer, M.; Kim, G.S.; Kim, Heonoh; Kim, H.J.; Kim, K.W.; Kim, N.Y.; Kim, S.K.; Kim, Y.D.; Kim, Y.H.; Ko, Y.J.; Kudryavtsev, V. A.; Lee, H.S.; Lee, J.; Lee, J.Y.; Lee, M.H.; Leonard, D. S.; Lynch, W.; Maruyama, R.; Mouton, F.; Olsen, S. L.; Park, B.J.; Park, H.K.; Park, H.S.; Park, K.S.; Pitta, R. L. C.; Prihtiadi, H.; Ra, Sejin; Rott, C.; Shin, K. A.; Scarff, A.; Spooner, N. J. C.; Thompson, W. G.; Yang, L.; Yu, G. H.

doi:10.1016/j.astropartphys.2019.07.004

Cited by 8 publications

(6 citation statements)

References 47 publications

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“…From the analysis of the first 59.5 days of data collected, COSINE-100 excluded the DAMA/LIBRA signal as due to the SI interaction of WIMPs in a standard halo model [65]; these data have been also interpreted in other contexts like Inelastic Boosted DM [66] and WIMP effective models [67]. Results for solar axions have also been derived [68]. A first analysis of annual modulation from 1.7 years of data has been presented [69]; since three crystals were excluded (because of a reduced light yield), the total exposure analyzed is 97.79 kg•y.…”

Section: Annual Modulation Effectmentioning

confidence: 99%

The Role of Small Scale Experiments in the Direct Detection of Dark Matter

Cebrián

2021

Universe

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In the direct detection of the galactic dark matter, experiments using cryogenic solid-state detectors or noble liquids play for years a very relevant role, with increasing target mass and more and more complex detection systems. But smaller projects, based on very sensitive, advanced detectors following new technologies, could help in the exploration of the different proposed dark matter scenarios too. There are experiments focused on the observation of distinctive signatures of dark matter, like an annual modulation of the interaction rates or the directionality of the signal; other ones are intended to specifically investigate low mass dark matter candidates or particular interactions. For this kind of dark matter experiments at small scale, the physics case will be discussed and selected projects will be described, summarizing the basics of their detection methods and presenting their present status, recent results and prospects.

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Section: Annual Modulation Effectmentioning

confidence: 99%

The Role of Small Scale Experiments in the Direct Detection of Dark Matter

Cebrián

2021

Universe

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“…𝑔 𝑎𝑒 𝑔 𝑎𝛾 for Primakoff axions or 𝑔 𝑎𝑒 𝑔 𝑎𝑁 for axions produced in a nuclear transition. A number of searches of this kind have been performed in recent years, see for example EDELWEISS-II [144], XMASS [153], XENON100 [145], PANDA-X [154], LUX [155], CDEX [156], and COSINE-100 [157]. Very recently the XENON1T collaboration has reported an excess of events in the electronic recoil spectrum below 7 keV [158].…”

Section: Axion Searchesmentioning

confidence: 99%

CUORE Opens the Door to Tonne-scale Cryogenics Experiments

Adams,

Alduino,

Alessandria

et al. 2021

Preprint

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The past few decades have seen major developments in the design and operation of cryogenic particle detectors. This technology offers an extremely good energy resolution -comparable to semiconductor detectors -and a wide choice of target materials, making low temperature calorimetric detectors ideal for a variety of particle physics applications. Rare event searches have continued to require ever greater exposures, which has driven them to ever larger cryogenic detectors, with the CUORE experiment being the first to reach a tonne-scale, mK-cooled, experimental mass. CUORE, designed to search for neutrinoless double beta decay, has been operational since 2017 at a temperature of about 10 mK. This result has been attained by the use of an unprecedentedly large cryogenic infrastructure called the CUORE cryostat: conceived, designed and commissioned for this purpose.In this article the main characteristics and features of the cryogenic facility developed for the CUORE experiment are highlighted. A brief introduction of the evolution of the field and of the past cryogenic facilities are given. The motivation behind the design and development of the CUORE cryogenic facility is detailed as are the steps taken toward realization, commissioning, and operation of the CUORE cryostat. The major challenges overcome by the collaboration and the solutions implemented throughout the building of the cryogenic facility will be discussed along with the potential improvements for future facilities.The success of CUORE has opened the door to a new generation of large-scale cryogenic facilities in numerous fields of science. Broader implications of the incredible feat achieved by the CUORE collaboration on the future cryogenic facilities in various fields ranging from neutrino and dark matter experiments to quantum computing will be examined.

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“…The COSINE-100 experiment's aim is to confirm or refute the annual modulation signal observed by the DAMA/LIBRA experiment with an array of 106 kg of low-background NaI(Tl) crystals at the Yangyang underground laboratory (Y2L) in South Korea [36,37]. Physics data have been collected since September 2016, and used to produce a series of first results and bounds on various dark matter models [38][39][40][41]. The first measurement of an annual event rate modulation was reported in 2019 [39] even though its sensitivity was not sufficient to probe the DAMA/LIBRA signal.…”

Section: Introductionmentioning

confidence: 99%

Measurement of the cosmic muon annual and diurnal flux variation with the COSINE-100 detector

Prihtiadi

Adhikari

Souza

et al. 2021

J. Cosmol. Astropart. Phys.

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We report measurements of annual and diurnal modulations of the cosmic-ray muon rate in the Yangyang underground laboratory (Y2L) using 952 days of COSINE-100 data acquired between September 2016 and July 2019. A correlation of the muon rate with the atmospheric temperature is observed and its amplitude on the muon rate is determined. The effective atmospheric temperature and muon rate variations are positively correlated with a measured effective temperature coefficient of α T = 0.80 ± 0.11. This result is consistent with a model of meson production in the atmosphere. We also searched for a diurnal modulation in the underground muon rate by comparing one-hour intervals. No significant diurnal modulation of the muon rate was observed.

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A search for solar axion induced signals with COSINE-100

Cited by 8 publications

References 47 publications

The Role of Small Scale Experiments in the Direct Detection of Dark Matter

The Role of Small Scale Experiments in the Direct Detection of Dark Matter

CUORE Opens the Door to Tonne-scale Cryogenics Experiments

Measurement of the cosmic muon annual and diurnal flux variation with the COSINE-100 detector

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