An experiment to search for dark-matter interactions using sodium iodide detectors

@article{AdhikariAdhikarideSouzaCarlinChoiDjamalEzer20,
  title={An experiment to search for dark-matter interactions using sodium iodide detectors},
  author={Govinda Pushparaj Estella Barbosa Nelson Seonho Mitra Anth Adhikari Adhikari de Souza Carlin Choi Djamal Ezer and Govinda Adhikari and Pushparaj Adhikari and Estella Barbosa de Souza and Nelson Carlin and Seonho Choi and Mitra Djamal and Anthony C. Ezeribe and Chang Hyon Ha and Insik Hahn and Antonia Hubbard and Eun Ju Jeon and Jay Hyun Jo and Hanwool Joo and Woon Gu Kang and W S Kang and Matthew Kauer and Bonghee Kim and Hongjoo Kim and Hyounggyu Kim and Kyungwon Kim and Nam Young Kim and Sun Kee Kim and Yeongduk Kim and Yong-Hamb Kim and Young Ju Ko and V. A. Kudryavtsev and Hyun Su Lee and Jaison Lee and Jooyoung Lee and Moo Hyun Lee and Douglas S. Leonard and Warren A. Lynch and Reina Maruyama and Fr'ed'eric Mouton and Stephen Lars Olsen and Byung Do Park and Hyang-Kyu Park and Hyeonseo Park and Jungsic Park and Kang Soon Park and W. Pettus and Hafizh Prihtiadi and Sejin Ra and Carsten Rott and Andrew Scarff and Keon Ah Shin and N. J. C. Spooner and William G Thompson and Liang Yang and Seok Hyun Yong},
  journal={Nature},
  year={2018},
  volume={564},
  pages={83 - 86}
}
Observations of galaxies and primordial radiation suggest that the Universe is made mostly of non-luminous dark matter1,2. Several new types of fundamental particle have been proposed as candidates for dark matter3, such as weakly interacting massive particles (WIMPs)4,5. These particles would be expected to interact with nuclei in suitable detector materials on Earth, for example, causing them to recoil. However, no definitive signal from such dark-matter interactions has been detected despite… 
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References

SHOWING 1-10 OF 35 REFERENCES
Detecting cold dark-matter candidates.
The growing synergy between astrophysics, particle physics, and low background experiments strengthens the possibility of detecting astrophysical non-baryonic matter. The idea of direct detection is
Signal modulation in cold-dark-matter detection.
TLDR
The seasonal modulation of the signal can be used to detect WIMP's even at low-signal-to-background levels and thus without the necessity of going to very-low-energy thresholds, suggesting the prospects for detecting a variety of cold-dark-matter candidates may be closer at hand than previously thought.
Compatibility of DAMA/LIBRA dark matter detection with other searches
The DAMA/NaI and DAMA/LIBRA annual modulation data, which may be interpreted as a signal for the existence of weakly interacting dark matter (WIMPs) in our galactic halo, are examined in light of
First search for a dark matter annual modulation signal with NaI(Tl) in the Southern Hemisphere by DM-Ice17
The first search for a dark matter annual modulation signal with NaI(Tl) target material in the Southern Hemisphere conducted with the DM-Ice17 experiment is presented. DM-Ice17 consists of 17 kg of
Muon detector for the COSINE-100 experiment
The COSINE-100 dark matter search experiment has started taking physics data with the goal of performing an independent measurement of the annual modulation signal observed by DAMA/LIBRA. A muon
DAMA/LIBRA-phase2 in WIMP effective models
The DAMA/LIBRA collaboration has recently released updated results from their search for the annual modulation signal expected from Dark Matter (DM) scattering in their NaI detectors. We have fitted
...
...