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2018

Parametric Resonance Production of Ultralight Vector Dark Matter

Dror, Jeff A., Harigaya, Keisuke, Narayan, Vijay

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Vector bosons heavier than $10^{-22}$ eV can be viable dark matter candidates with distinctive experimental signatures.

Ultralight dark matter generally requires a non-thermal origin to achieve the observed density, while still behaving like a pressureless fluid at late times.
We show that such a production mechanism naturally occurs for vectors whose mass originates from a dark Higgs.
If the dark Higgs has a large field value after inflation, the energy in the Higgs field can be efficiently transferred to vectors through parametric resonance.

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