Dilaton-Induced Resonant Production of Ultralight Vector Dark Matter
Imtiaz Khan, G. Mustafa, Jehanzad Zafar, Farruh Atamurotov, Ahmadjon Abdujabbarov, and Chengxun Yuan

TL;DR
This paper investigates a resonant mechanism for producing ultralight vector dark matter via a dilaton coupling to a scalar field, deriving conditions for relic abundance, mass ranges, and theoretical consistency.
Contribution
It introduces a detailed analysis of dilaton-induced resonant production of ultralight vector dark matter, including polarization effects and UV consistency conditions.
Findings
Relic dark-photon mass scales as the inverse square of the initial fraction.
The mass range $10^{-20}$--$10^{-18}$ eV corresponds to specific initial conditions.
Derived polarization-resolved quadratic action and UV bounds for St"uckelberg and Higgs completions.
Abstract
We study the resonant production of ultralight vector dark matter from an oscillating spectator scalar coupled to a massive vector through a dilatonic kinetic function . The mechanism contains a narrow branch near . Assuming that the spectator remains subdominant until oscillations begin, we derive the onset fraction and show that, in the linear regime and for a background with constant equation-of-state parameter , the growth-to-Hubble ratio scales as . Combined with the tuned-branch abundance estimate, this implies for the relic dark-photon mass. In particular, the interval -- maps to --, corresponding to a radiation-dominated onset with a subdominant spectator, while for…
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