arXiv:2601.15066·v2·High Energy Physics — Phenomenology
Combined constraints on dark photons from high-energy collisions, cosmology, and astrophysics
A. W. Romero Jorge🇩🇪 · L. Sagunski🇩🇪 · Guan-Wen Yuan🇮🇹 · T. Song🇩🇪 · E. Bratkovskaya🇩🇪
Abstract
We investigate a dark sector coupled to the Standard Model (SM) through a kinetically mixed dark photon associated with a new gauge symmetry. Kinetic mixing induces an effective coupling to the electromagnetic current, while interacts with stable dark matter (DM) via a dark gauge coupling . Our analysis is based on the parton-hadron-string dynamics (PHSD) transport approach, extended to include dark photon production and decay into dileptons (). In PHSD, dark photons are produced in high-energy collisions through Dalitz decays of light mesons (), Delta-resonances (), direct vector meson decays (), kaon decays, and annihilation. Building on previous PHSD benchmarks against dilepton data, we extract upper limits on in both the visible regime (), where dominates, and the invisible regime (), where is kinematically open. Cosmological and astrophysical constraints are incorporated in two complementary ways. First, we compute the velocity-dependent self-interaction cross section 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 , consistent with \textit{Planck} measurements of the cosmic microwave background. Combining PHSD limits on with relic density and self-interaction requirements, we exclude regions of the 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.
Comments: 19 pages, 9 figures