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2015

Freeze-In Dark Matter with Displaced Signatures at Colliders

Co, Raymond T., D'Eramo, Francesco, Hall, Lawrence J. et al.

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Dark matter, $X$, may be generated by new physics at the TeV scale during an early matter-dominated (MD) era that ends at temperature $T_R \ll {\rm TeV}$.

Compared to the conventional radiation-dominated (RD) results, yields from both Freeze-Out and Freeze-In processes are greatly suppressed by dilution from entropy production, making Freeze-Out less plausible while allowing successful Freeze-In with a much larger coupling strength.
Freeze-In is typically dominated by the decay of a particle $B$ of the thermal bath, $B \rightarrow X$.
For a large fraction of the relevant cosmological parameter space, the decay rate required to produce the observed dark matter abundance leads to displaced signals at LHC and future colliders, for any $m_X$ in the range ${\rm keV} < m_X < m_B$ and for values of $m_B$ accessible to these colliders.

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