30 August 2026 to 4 September 2026
Asia/Tokyo timezone

Broadband Axion Dark Matter Search via Heterodyne Atom Interferometry

Not scheduled
20m
Oral Dark matter searches (both direct and indirect)

Speaker

Dr Paul Robert (University of Florence)

Description

Ultralight \textit{axion-like particles} (ALPs) are among the most theoretically motivated dark matter candidates, yet their detection remains challenging across a wide range of masses. We present a novel \textbf{heterodyne atom interferometry scheme} that dramatically extends the sensitivity of quantum sensors to ALP dark matter, covering up to \textit{six orders of magnitude} in axion mass beyond conventional configurations.

The method exploits the coupling of the ALP field to nuclear spins, $\Delta E \propto g_{aNN}\,\nabla a \cdot \mathbf{s}$, and overcomes the fundamental limitation of standard axion searches at low frequencies: the dominance of $1/f$ noise from seismic and gravity-gradient backgrounds. By applying a rotating magnetic field that induces coherent spin precession at a tunable frequency $\Omega$, the axion-induced signal is upconverted from near-DC to a well-controlled carrier, where synchronous detection suppresses environmental noise by orders of magnitude. This shifts the accessible axion mass window from the sub-Hz regime to frequencies up to $\sim\!100$\,kHz, probing a largely unexplored region of parameter space.

We implement this scheme using \textbf{fermionic $^{87}$Sr} in a Ramsey interferometry configuration, which provides direct sensitivity to internal-state energy shifts and offers superior broadband response compared to Mach--Zehnder geometries. The sensitivity of the scheme scales with interrogation time and atom number, making it complementary to existing haloscope and spin-precession experiments such as CASPEr and ABRACADABRA in the ultralight mass range ($m_a \lesssim 10^{-10}$\,eV).

To distinguish genuine ALP signals from magnetic backgrounds, we propose a \textbf{differential double atom interferometer} configuration combined with \textbf{sidereal modulation} as a direction-sensitive discriminator. This provides a robust veto against local systematic effects and constitutes a key signature of a dark matter origin. Together, these features make atom interferometry a powerful and scalable platform for next-generation ALP searches, with a clear path toward probing axion--nucleon couplings at or below the level predicted for QCD axion models.

Primary author

Dr Paul Robert (University of Florence)

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