Improved Dark Photon Sensitivity from the Dark SRF Experiment
Saarik Kalia, Zhen Liu, Bianca Giaccone, Oleksandr Melnychuk, Roman Pilipenko, Asher Berlin, Anson Hook, Sergey Belomestnykh, Crispin Contreras-Martinez, Daniil Frolov, Timergali Khabiboulline, Yuriy Pischalnikov, Sam Posen, Oleg Pronitchev, Vyacheslav Yakovlev, Anna Grassellino, Roni Harnik, Alexander Romanenko
TL;DR
This work reanalyzes the Dark SRF pathfinder data by incorporating a refined jittering model for high-$Q$ resonators, based on the Lorentzian jitter-spectrum framework of Ref. $\text{cui2025}$. By replacing a severe power-suppression assumption with a perturbative correction $\alpha$ that remains small ($\alpha\approx0.15$) and restricting the data window to mitigate slow drift, the authors achieve an approximate order-of-magnitude improvement in the dark-photon exclusion bound for masses below $6\,\mu\mathrm{eV}$, with an associated $\sim 4$-order-of-magnitude enhancement in the effective SNR. This refined Dark SRF bound translates into a world-leading laboratory limit on the SM photon mass, $m_\gamma<1.6\times10^{-15}\ \mathrm{eV}=2.9\times10^{-48}\ \mathrm{g}$, via the longitudinal-mode mapping of a kinetically mixed dark photon. The paper also outlines upgrade paths for a next-generation Dark SRF in a dilution refrigerator, including higher frequency operation, reduced cavity volume, active frequency stabilization, and potential Josephson-parametric amplification to further boost sensitivity.
Abstract
We report the refined dark-photon exclusion bound from Dark SRF's pathfinder run. Our new result is driven by improved theoretical modeling of frequency instability in high-quality resonant experiments. Our analysis leads to a constraint that is an order of magnitude stronger than previously reported (corresponding to a signal-to-noise ratio that is four orders of magnitude larger). This result represents the world-leading constraint on non-dark-matter dark photons over a wide range of masses below $6\,\rm μeV$ and translates to the best laboratory-based limit on the photon mass $m_γ<2.9\times 10^{-48}\,\rm g$.
