Dark matter
Lecture Notes in Physics, ISSN: 1616-6361, Vol: 975, Page: 9-48
2020
- 3Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Metrics Details
- Captures3
- Readers3
Book Chapter Description
We discuss the phenomenology of dark matter at cosmological and galactic scales. Direct detection experiments like Xenon-1T have ruled out a large swathe of the mass vs. DM-nucleon cross-section parameter space challenging the conventional WIMP paradigm of the ∼100 GeV weakly interacting dark matter. New mechanisms for relic density like the freeze-in production of dark matter or the 3 → 2 annihilation process can give the correct relic density. These dark matter particles have very small couplings to standard model particles and lower (∼ MeV) mass therefore they can evade the stringent constraints from direct detection experiments. Dark matter can be self interacting thereby solving some problems with cold dark matter at galactic scales. Dark matter may be very light with mass 10 eV or they may be inelastic.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85092515409&origin=inward; http://dx.doi.org/10.1007/978-3-030-56201-4_2; http://link.springer.com/10.1007/978-3-030-56201-4_2; http://link.springer.com/content/pdf/10.1007/978-3-030-56201-4_2; https://dx.doi.org/10.1007/978-3-030-56201-4_2; https://link.springer.com/chapter/10.1007/978-3-030-56201-4_2
Springer Science and Business Media LLC
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