Impacts of ALP on the Constraints of Dark Photon

TL;DR

This paper explores how a spontaneously broken dark sector with an axion-like particle alters dark photon constraints, allowing it to explain the muon g-2 anomaly for masses above 10 GeV.

Contribution

It introduces a model where a dark sector axion-like particle modifies dark photon decay channels, relaxing experimental constraints and expanding the parameter space for muon g-2 explanation.

Findings

Dark photon can explain muon g-2 for masses >10 GeV.

Modified decay channels relax existing experimental constraints.

Dark sector interactions significantly impact dark photon phenomenology.

Abstract

Dark sector may exist and interact with Standard Model (SM) through the $U(1)$ kinetic mixing. Through this portal-type interaction, dark photon from dark sector couples to SM fermions, and may explain the discrepancy between experimental data and SM calculations on muon anomalous magnetic moment, muon $g-2$. However, current searches for dark photon impose stringent constraints on the mixing parameter $\varepsilon$ for various dark photon masses, excluding the favorite parameter space for muon $g-2$. In this paper, we study the case where a global $U(1)$ in dark sector is spontaneously broken, resulting a light pseudo-Goldstone, axion-like particle (ALP) $a$, which couples to dark photon and SM photon, $g_{a\gamma\gamma'}$. Through this interaction, dark photon may decay into photon and ALP when this channel is kinematically allowed. As a result, the experimental constraints on dark photon change significantly, and dark photon is able to explain the muon $g-2$ anomaly when its mass is heavier than $10$ GeV.