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arXiv · 2405.19087

Impacts of ALP on the Constraints of Dark Photon

Chuan-Ren Chen·Yuan-Feng Hsieh·Chrisna Setyo Nugroho
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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.

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Chuan-Ren Chen, Yuan-Feng Hsieh, Chrisna Setyo Nugroho. 2024-05-29. Impacts of ALP on the Constraints of Dark Photon. https://doi.org/10.1093/ptep/ptaf181

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