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The search for dark matter is of fundamental importance to our understandingof the universe. Weakly-Interacting Slim Particles (WISPs) such as axions andhidden sector photons (HSPs) are well motivated candidates for the dark matter.Some of the most sensitive and mature experiments to detect WISPs rely onmicrowave cavities, and the detection of weak photon signals. It is oftensuggested to power combine multiple cavities, which creates a host of technicalconcerns. We outline a scheme based on cross-correlation for effectively powercombining cavities and increasing the signal-to-noise ratio of a candidate WISPsignal.

Cross-correlation measurement techniques for cavity-based axion and weakly interacting slim particle searches