New directions in secluded dark matter searches
APA
(2026). New directions in secluded dark matter searches. SciVideos. https://videos.cern.ch/record/3025328
MLA
New directions in secluded dark matter searches. SciVideos, Apr. 14, 2026, https://videos.cern.ch/record/3025328
BibTex
@misc{ scivideos_oai:cds.cern.ch:3025328,
doi = {},
url = {https://videos.cern.ch/record/3025328},
author = {},
keywords = {},
language = {en},
title = {New directions in secluded dark matter searches},
publisher = {},
year = {2026},
month = {apr},
note = {oai:cds.cern.ch:3025328 see, \url{https://scivideos.org/cern-cds/3025328}}
}
Abstract
Less than 20% of the total matter content of the universe consists of known forms of matter. After decades of experimental efforts, the leading hypothesis for the missing part - namely a new type of weakly interacting massive particle - is starting to become seriously pressured. As a result, the true nature of dark matter is more elusive now than ever.
I will start with a pedagogic reminder of the most convincing pieces of evidence that we have for the existence of dark matter. I will then highlight new model building avenues that may explain why traditional searches have, so far, failed to see any signals. In fact, I will argue that it might well be generally impossible to directly detect or produce any dark matter particles in the laboratory - but that cosmological and astrophysical observations still have the potential to conclusively pinpoint some of their microscopic properties.
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