Dark matter as a weakly coupled dark baryon

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作者
Andrea Mitridate
Michele Redi
Juri Smirnov
Alessandro Strumia
机构
[1] Scuola Normale Superiore (SNS),INFN and Department of Physics and Astronomy
[2] Istituto Nazionale di Fisica Nucleare (INFN) — Sezione di Pisa,Dipartimento di Fisica “E. Fermi”
[3] University of Florence,undefined
[4] Università di Pisa,undefined
[5] CERN,undefined
[6] Theory Division,undefined
关键词
Cosmology of Theories beyond the SM; Beyond Standard Model; Gauge Symmetry;
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摘要
Dark Matter might be an accidentally stable baryon of a new confining gauge interaction. We extend previous studies exploring the possibility that the DM is made of dark quarks heavier than the dark confinement scale. The resulting phenomenology contains new unusual elements: a two-stage DM cosmology (freeze-out followed by dark condensation), a large DM annihilation cross section through recombination of dark quarks (allowing to fit the positron excess). Light dark glue-balls are relatively long lived and give extra cosmological effects; DM itself can remain radioactive.
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