Fig. 2: Constraints on the coupling parameters Λγ and Λe as a function of the mass of the field mϕ, for scalar field dark matter as in the basic scalar scenario. | Nature

Fig. 2: Constraints on the coupling parameters Λγ and Λe as a function of the mass of the field mϕ, for scalar field dark matter as in the basic scalar scenario.

From: Direct limits for scalar field dark matter from a gravitational-wave detector

Fig. 2

Dashed lines represent constraints on the electron coupling Λe and dotted lines represent constraints on the photon coupling Λγ, at the 95% confidence level. The green region denotes the parameter space excluded in the current study through the spectral analysis of data from the GEO600 gravitational-wave detector. Other coloured regions indicate parameter spaces excluded through previous direct experimental searches: Hees et al.6 (blue), Van Tilburg et al.5 (yellow), Kennedy et al.45 (brown), Aharony et al.38 (magenta), Branca et al.40 (purple), Savalle et al.8 (cyan) and Antypas et al.39 (red). The black curves and grey regions correspond to previous constraints from ‘fifth-force’ searches/tests of the equivalence principle; to our knowledge, the most stringent such constraints for this dark matter scenario are from the MICROSCOPE experiment7,43 (lower curves at low mass) and the Cu/Pb torsion pendulum experiment performed by the Eöt-Wash group26,37,41 (at higher masses).

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