0000000000628587

AUTHOR

Daekyoung Kang

showing 2 related works from this author

Production of dark-matter bound states in the early universe by three-body recombination

2018

The small-scale structure problems of the universe can be solved by self-interacting dark matter that becomes strongly interacting at low energy. A particularly predictive model for the self-interactions is resonant short-range interactions with an S-wave scattering length that is much larger than the range. The velocity dependence of the cross section in such a model provides an excellent fit to self-interaction cross sections inferred from dark-matter halos of galaxies and clusters of galaxies if the dark-matter mass is about 19 GeV and the scattering length is about 17 fm. Such a model makes definite predictions for the few-body physics of weakly bound clusters of the dark-matter particl…

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Nuclear Theorymedia_common.quotation_subjectPhysics beyond the Standard ModelDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBound stateEffective field theoryCluster (physics)lcsh:Nuclear and particle physics. Atomic energy. RadioactivityNuclear Experiment (nucl-ex)010306 general physicsNuclear Experimentmedia_commonPhysics010308 nuclear & particles physicsScattering lengthCosmology of Theories beyond the SMUniverseGalaxyHigh Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798Astrophysics - Cosmology and Nongalactic Astrophysics
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Dark Matter Bound States from Three-Body Recombination

2020

The small-scale structure problems of the universe can be solved by self-interacting dark matter that becomes strongly interacting at low energies. A particularly predictive model is resonant short-range self-interactions, with a dark-matter mass of about 19 GeV and a large S-wave scattering length of about 17 fm. Such a model makes definite predictions for the few-body physics of weakly bound clusters of the dark-matter particles. We calculate the production of two-body bound clusters by three-body recombination in the early universe under the assumption that the dark matter particles are identical bosons, which is the most favorable case for forming larger clusters. The fraction of dark m…

PhysicsOrders of magnitude (time)media_common.quotation_subjectBound stateBinding energyDark matterScattering lengthAtomic physicsUniverseRecombinationmedia_commonBoson
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