Vector Dark Matter from Inflationary Fluctuations
Peter W. Graham, Jeremy Mardon, and Surjeet Rajendran

TL;DR
This paper proposes a new mechanism for vector dark matter production during inflation via quantum fluctuations, resulting in a distinctive peaked power spectrum that links dark matter properties to the inflationary scale.
Contribution
It introduces a novel inflationary production process for vector dark matter with a unique peaked spectrum, differing from scalar and tensor cases, and connects dark matter abundance to inflation parameters.
Findings
Vector dark matter can be produced with a peaked power spectrum during inflation.
The predicted dark matter mass is around 10^-5 eV for high-scale inflation.
Detection of such dark matter could reveal the inflationary scale and history.
Abstract
We calculate the production of a massive vector boson by quantum fluctuations during inflation. This gives a novel dark-matter production mechanism quite distinct from misalignment or thermal production. While scalars and tensors are typically produced with a nearly scale-invariant spectrum, surprisingly the vector is produced with a power spectrum peaked at intermediate wavelengths. Thus dangerous, long-wavelength, isocurvature perturbations are suppressed. Further, at long wavelengths the vector inherits the usual adiabatic, nearly scale-invariant perturbations of the inflaton, allowing it to be a good dark matter candidate. The final abundance can be calculated precisely from the mass and the Hubble scale of inflation, H_I. Saturating the dark matter abundance we find a prediction for the mass m = 10^-5 eV (10^14 GeV/H_I)^4. High-scale inflation, potentially observable in the CMB,…
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