Combined constraints on dark photons from high-energy collisions, cosmology, and astrophysics

TL;DR

This paper combines collider, cosmological, and astrophysical data to constrain dark photon models, exploring their production, decay, and dark matter interactions across multiple experimental and observational domains.

Contribution

It introduces a comprehensive analysis framework that integrates high-energy collision data with cosmological and astrophysical constraints to limit dark photon parameter space.

Findings

PHSD limits on kinetic mixing parameter $\

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Abstract

We investigate a dark sector coupled to the Standard Model (SM) through a kinetically mixed dark photon $U$ associated with a new $U(1)'$ gauge symmetry. Kinetic mixing $\varepsilon$ induces an effective coupling to the electromagnetic current, while $U$ interacts with stable dark matter (DM) $\chi$ via a dark gauge coupling $g_\chi$. Our analysis is based on the parton-hadron-string dynamics (PHSD) transport approach, extended to include dark photon production and decay into dileptons ($U\!\to e^+e^-$). In PHSD, dark photons are produced in high-energy collisions through Dalitz decays of light mesons ($\pi^0,\eta,\eta',\omega$), Delta-resonances ($\Delta\!\to N U$), direct vector meson decays ($\rho,\omega,\phi\!\to U$), kaon decays, and $q\bar q\!\to U$ annihilation. Building on previous PHSD benchmarks against dilepton data, we extract upper limits on $\varepsilon^2(m_U,m_\chi,\alpha_\chi)$ in both the visible regime ($m_U<2m_\chi$), where $U\!\to e^+e^-$ dominates, and the invisible regime ($m_U>2m_\chi$), where $U\!\to\chi\bar\chi$ is kinematically open. Cosmological and astrophysical constraints are incorporated in two complementary ways. First, we compute the velocity-dependent self-interaction cross section $\sigma/m_\chi$ for Yukawa-mediated SIDM and confront it with bounds from dwarf galaxies, galaxy groups, and clusters. Second, we determine thermal relic target curves by computing the relic abundance and requiring $\Omega_{\rm DM}h^2\simeq 0.12$, consistent with \textit{Planck} measurements of the cosmic microwave background. Combining PHSD limits on $\varepsilon^2$ with relic density and self-interaction requirements, we exclude regions of the $(m_\chi,m_U)$ plane for each DM realization (Dirac, Majorana, or complex scalar) and identify benchmark scenarios in which heavy-ion, cosmological, and astrophysical constraints are simultaneously satisfied.