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interesting dark-matter candidate
I'm now at a cosmology conference:
https://indico.cern.ch/event/736594/overview One reason to go to a conference is to hear about interesting things one might have missed. For me, probably the most interesting talk was the penultimate one, an update on these publications concerning a novel dark-matter candidate: https://arxiv.org/abs/1202.0560 https://arxiv.org/abs/1311.1627 http://iopscience.iop.org/article/10...6/496/1/012023 https://arxiv.org/abs/1801.04206 There are many connections between particle physics and astronomy, but this is closer than most, is a really novel idea, makes clear predictions, explains very many (otherwise not closely related) things with a simple idea, and has already had some predictions confirmed. While I've been to other conferences which covered a wide range of topics, at this one there were intentionally no sessions on specific topics, but, say, a talk on observational astronomy could be followed by one on theoretical particle physics. I can't write a summary here, of course, but one general theme is that while large-scale cosmology is more or less solved, it is becoming even more clear that many things about galaxies, particularly dwarf galaxies, are not understood, and it is unclear which of many options is the way forward. One aspect of this is dark matter, and both the lack of direct (or indirect) detections as well as the discovery of a light Higgs seems to be swinging the pendulum away from WIMPs as dark matter to other ideas. Also, it might turn out that more than one of the alternatives to WIMPs is correct. |
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