Dark photon limits: a cookbook

Alexander Millar
Fri December 10th 2021, 3:30pm
U Stockholm
Zoom and Varian 355

The dark photon is a massive hypothetical particle that interacts with the Standard Model by kinetically mixing with the visible photon.  Due to the similarities with the electromagnetic signals generated by axions, several bounds on dark photon signals are simply reinterpretations of historical bounds set by axion haloscopes. However, the dark photon has a property that the axion does not: an intrinsic polarisation. We show that if one does account for the dark photon polarisation, and the rotation of the Earth, an experiment's discovery reach can be enhanced by over an order of magnitude. We detail the strategies that would need to be taken to properly optimise a dark photon search. We also point out that several well-known searches for axions employ techniques for testing signals that preclude their ability to set exclusion limits on dark photons.