Strong constraints from COSINE-100 on the DAMA dark matter results
Por um escritor misterioso
Last updated 20 junho 2024
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://www.science.org/cms/10.1126/sciadv.abk2699/asset/9073fb0c-6575-4c33-bf59-195b445dc239/assets/images/large/sciadv.abk2699-f1.jpg)
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://media.springernature.com/m685/springer-static/image/art%3A10.1038%2Fs41598-023-31688-4/MediaObjects/41598_2023_31688_Fig4_HTML.png)
An induced annual modulation signature in COSINE-100 data by DAMA/LIBRA's analysis method
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://www.researchgate.net/publication/329672043/figure/fig2/AS:731591139680256@1551436328016/Typical-waveforms-from-the-COSINE-100-PMTs-for-2-6-keV-signals-a-The-b-and-g.jpg)
Typical waveforms from the COSINE-100 PMTs for 2–6-keV signals a, The β
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://mcdonaldinstitute.ca/wp-content/uploads/2021/11/%E1%84%89%E1%85%B3%E1%84%8F%E1%85%B3%E1%84%85%E1%85%B5%E1%86%AB%E1%84%89%E1%85%A3%E1%86%BA-2018-12-07-%E1%84%8B%E1%85%A9%E1%84%92%E1%85%AE-5.06.48-1005x1024-1-707x720.jpg.webp)
New analysis from COSINE-100 Arthur B. McDonald Institute
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://www.frontiersin.org/files/Articles/1142765/fphy-11-1142765-HTML/image_m/fphy-11-1142765-g006.jpg)
Frontiers Performance of an ultra-pure NaI(Tl) detector produced by an indigenously-developed purification method and crystal growth for the COSINE-200 experiment
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://www.researchgate.net/publication/363554072/figure/fig2/AS:11431281084494757@1663215489319/Measured-modulation-amplitude-as-a-function-of-energy-in-1-keV-bins-for-the-COSINE-100.png)
Measured modulation amplitude as a function of energy in 1 keV bins for
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://www.researchgate.net/publication/369451823/figure/fig3/AS:11431281129430398@1679544453647/Low-energy-spectra-of-a-NaITl-crystal-in-the-COSINE-100-experiment-Energy-spectra-of_Q320.jpg)
PDF) An induced annual modulation signature in COSINE-100 data by DAMA/LIBRA's analysis method
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://i1.rgstatic.net/ii/profile.image/891658119954435-1589599270389_Q64/G-Adhikari-2.jpg)
PDF) Strong constraints from COSINE-100 on the DAMA dark matter results using the same sodium iodide target
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://d3i71xaburhd42.cloudfront.net/b4e54cee382383fbf39cb6fe694e87683ad06e5d/5-Figure7-1.png)
PDF] Depth profile study of 210Pb in the surface of an NaI(Tl) crystal
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://europepmc.org/articles/PMC10033922/bin/41598_2023_31688_Fig4_HTML.jpg)
An induced annual modulation signature in COSINE-100 data by DAMA/LIBRA's analysis method. - Abstract - Europe PMC
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://www.researchgate.net/publication/362619248/figure/fig2/AS:11431281078691796@1660187554486/Results-of-1-000-simulated-experiments-for-the-DAMA-LIBRA-experiment-We-generate-1-000_Q320.jpg)
PDF) An induced annual modulation signature in COSINE-100 data by DAMA/LIBRA's analysis method
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://typeset.io/figures/figure-5-the-3s-allowed-regions-of-wimp-mass-vs-wimp-nucleon-1cse9ded.webp)
PDF) Comparison between DAMA/LIBRA and COSINE-100 in the light of Quenching Factors (2019), Y. J. Ko
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://upload.wikimedia.org/wikipedia/commons/9/9a/Direct_Detection_Constraints.png)
Weakly interacting massive particle - Wikipedia
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://typeset.io/figures/figure-1-the-nuclear-recoil-quenching-factors-of-na-a-and-i-2z4q1nit.webp)
PDF) Comparison between DAMA/LIBRA and COSINE-100 in the light of Quenching Factors (2019), Y. J. Ko
![Strong constraints from COSINE-100 on the DAMA dark matter results](https://upload.wikimedia.org/wikipedia/commons/thumb/7/7f/CDMS_parameter_space_2004.png/350px-CDMS_parameter_space_2004.png)
Weakly interacting massive particle - Wikipedia
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