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Composite strongly interacting dark matter

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arxiv 1312.3325 v3 pith:JQYAJYQY submitted 2013-12-11 hep-ph astro-ph.CO

Composite strongly interacting dark matter

classification hep-ph astro-ph.CO
keywords darkmatterstronglybeencompositeconstraintsinteractingmodels
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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It has been suggested that cold dark matter (CDM) has difficulties in explaining tentative evidence for noncuspy halo profiles in small galaxies, and the low velocity dispersions observed in the largest Milky Way satellites ("too big to fail" problem). Strongly self-interacting dark matter has been noted as a robust solution to these problems. The elastic cross sections required are much larger than predicted by generic CDM models, but could naturally be of the right size if dark matter is composite. We explore in a general way the constraints on models where strongly interacting CDM is in the form of dark "atoms" or "molecules," or bound states of a confining gauge interaction ("hadrons"). These constraints include considerations of relic density, direct detection, big bang nucleosynthesis, the cosmic microwave background, and LHC data.

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Cited by 5 Pith papers

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