Searching for dark matter with a spin-based interferometer

Daniel Gavilan-Martin; Grzegorz Łukasiewicz; Mikhail Padniuk; Emmanuel Klinger; Magdalena Smolis; Nataniel L. Figueroa; Derek F. Jackson Kimball; Alexander O. Sushkov; Szymon Pustelny; Dmitry Budker; Arne Wickenbrock

doi:10.1038/s41467-025-60178-6

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Searching for dark matter with a spin-based interferometer

Daniel Gavilan-Martin et al.

2025Nature Communications 16, 4953CC BY 4.0LCP000030

Fig. 8, panel (1)

Histogram of the normalized signal estimator, counts against $S(\omega)/\mathrm{fit}(\omega)$ on a logarithmic count axis, with the fitted non-central $\chi^2$ distribution (orange) and the 95% global-significance threshold (red dashed line).

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Data: data.csv
Overlay (Non-central $\chi^2$): overlay.csv

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This panel was recovered from the published vector figure. The plot shown here is re-rendered for interactive viewing and analysis. See the paper for the original figure and full scientific context.

License: CC BY 4.0.

Nat. Commun. 16, 4953 (2025) · DOI: 10.1038/s41467-025-60178-6 · arXiv: 2408.02668

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