Search for dark matter WIMPs using upward through-going muons in Super-Kamiokande
By 井上 邦雄. 2004
149 citations recorded by the source corpus.
View Paper: https://www.semanticscholar.org/paper/5ba1a85bf3f7b3b0743d72e08bc12cf207fb1200
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Citations in the corpus
- A review of indirect searches for particle dark matter (2016, background): “Groundbased imaging atmospheric Cherenkov telescopes (IACTs) detect the Cherenkov light produced by particle showers induced by a gamma ray or cosmic ray interacting in the Earth’s atmosphere.”
- Dark Matter Candidates from Particle Physics and Methods of Detection (2010, background): “The prospects for Super-Kamiokande may therefore be compared to direct detection rates (73; 87; 88; 89).”
- Dark Matter: A Primer (2010, background): “Super-K looks in the direction of the Sun, earth, and galactic center, and, like AMANDA, has not detected any excess of muon rates above the expected background [84].”
- Extended gamma-ray emission from Coy Dark Matter (2014, background): “[101] Super-Kamiokande Collaboration, S. Desai et al., Phys.”