Abstract

The vector $U$-bosons, or so called 'dark photons', are one of the possible candidates for the dark matter mediators. They are supposed to interact with the standard matter via a 'vector portal' due to the $U(1)-U(1)^\prime$ symmetry group mixing which might make them visible in particle and heavy-ion experiments. While there is no confirmed observation of dark photons, the detailed analysis of different experimental data allows to estimate the upper limit for the kinetic mixing parameter $\epsilon^2$ depending on the mass $M_U$ of $U$-bosons which is also unknown. In this study we present theoretical constraints on the upper limit of $\epsilon^2(M_U)$ in the mass range $M_U \le 0.6$ GeV from the comparison of the calculated dilepton spectra with the experimental data from the HADES Collaboration at SIS18 energies where the dark photons are not observed. Our analysis is based on the microscopic Parton-Hadron-String Dynamics (PHSD) transport approach which reproduces well the measured dilepton spectra in $p+p$, $p+A$ and $A+A$ collisions. Additionally to the different dilepton channels originating from interactions and decays of ordinary matter particles (mesons and baryons), we incorporate the decay of hypothetical $U$-bosons to dileptons, $U\to e^+e^-$, where the $U$-bosons themselves are produced by the Dalitz decay of pions $\pi^0\to \gamma U$, $\eta$-mesons $\eta \to \gamma U$ and Delta resonances $\Delta \to N U$. Our analysis can help to estimate the requested accuracy for future experimental searches of 'light' dark photons by dilepton experiments.

Highlights

  • An understanding of the structure of our Universe is one of the intriguing topics of modern physics

  • In order to explore the theoretical uncertainties in setting the upper limit we present in Fig. 4 the Parton-Hadron-String Dynamics (PHSD) results for the differential cross section dσ=dM for eþe− production in p þ p reactions at 3.5 GeV beam energy calculated for different ε2 scenarios in comparison to the experimental measurements by the HADES collaboration [62]: (i) CU corresponding to 0.1% and 10% (10% as in Fig. 1) allowed surplus of total Standard Model (SM) yield; (ii) constant ε2 1⁄4 10−5 and ε2 1⁄4 10−6

  • In this study we presented the first microscopic transport calculations, based on the PHSD approach, for the dilepton yield from the decay of hypothetical dark photons, U → eþe−, from p þ p, p þ A and heavy-ion collisions at SIS18 energies

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Summary

Introduction

An understanding of the structure of our Universe is one of the intriguing topics of modern physics. According to the present knowledge, the standard matter represents less than 5% of our Universe, while about 27% of it consists of socalled “dark matter” (DM) and about 68% is the “dark energy” [1]. The dark matter is supposed to be a relic from the big bang, which makes itself noticeable by its gravitational action on the large-scale cosmic structures. It was advocated that the dark matter mediators can interact with the Standard Model (SM) particles by four possible “portals”—vector, Higgs, neutrino and axion (cf the reviews [2,3,4] and references therein)

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