Vector dark matter production from inflation with symmetry breaking
Borna Salehian, Mohammad Ali Gorji, Hassan Firouzjahi, Shinji, Mukohyama

TL;DR
This paper proposes a model where vector dark matter is produced from symmetry breaking at the end of inflation, with quantum fluctuations of the dark photon accounting for current dark matter density, and predicts cosmic string formation.
Contribution
It introduces a novel mechanism linking inflation, symmetry breaking, and vector dark matter production, including cosmic string formation and specific parameter ranges.
Findings
Dark photon fluctuations can account for dark matter density
Model predicts cosmic strings consistent with CMB bounds
Reheat temperature around 10^{12} GeV supports the scenario
Abstract
We present a scenario of vector dark matter production from symmetry breaking at the end of inflation. In this model, the accumulated energy density associated with the quantum fluctuations of the dark photon accounts for the present energy density of dark matter. The inflaton is a real scalar field while a heavy complex scalar field, such as the waterfall of hybrid inflation, is charged under the dark gauge field. After the heavy field becomes tachyonic at the end of inflation, rolling rapidly towards its global minimum, the dark photon acquires mass via the Higgs mechanism. To prevent the decay of the vector field energy density during inflation, we introduce couplings between the inflaton and the gauge field such that the energy is pumped to the dark sector. The setup can generate the observed dark matter abundance for a wide range of the dark photon's mass and with the reheat…
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