Search for dark photons at future e$^+$e$^-$ colliders
Mikael Berggren (1) ((1) DESY, Hamburg, Germany)

TL;DR
This paper explores the potential of future e$^+$e$^-$ colliders to detect dark photons via their decay into muon pairs, focusing on the dependency of detection limits on the mixing parameter and mass.
Contribution
It presents a study using fully simulated events to evaluate the sensitivity of future colliders for dark photon detection across various energies.
Findings
Future colliders can effectively search for dark photons with small mixing parameters.
Detection sensitivity depends on the dark photon mass and collider energy.
Low background and high resolution at colliders improve dark photon search prospects.
Abstract
In a class of theories, dark matter is explained by postulating the existence of a `dark sector', which interacts gravitationally with ordinary matter. If this dark sector contains a U(1) symmetry, and a corresponding `dark' photon () , it is natural to expect that this particle kineticly mix with the ordinary photon, and hence become a `portal' through which the dark sector can be studied. The strength of the mixing is given by a mixing parameter . This same parameter governs both the production and the decay of the back to SM particles, and for values of not already excluded, the signal would be a quite small, and quite narrow resonance: If is large enough to yield a detectable signal, its decay width will be smaller than the detector resolution, but so large that the decay back to SM particles is prompt. For masses of the dark photon…
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