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We present a method to search for scalar field ultralight dark matter directly interacting with gravitational-wave interferometers via a modulation of the fine structure constant and the electron mass.
1903
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G. Heinzel, C. Braxmaier, K. Danzmann, P. Gath, J. Hough, O. Jennrich, U. Johann, A. Rudiger, M. Sallusti, and H. Schulte, LISA interferometry: Recent developments, Class. Quant. Grav. 23
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G. Hütsi, M. Raidal, V. Vaskonen, and H. Veermäe, Two populations of LIGO-Virgo black holes, JCAP 03
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S. Morisaki and T. Suyama, Detectability of ultralight scalar field dark matter with gravitational-wave detectors, Phys. Rev. D 100
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N. Bode et al. , Advanced LIGO Laser Systems for O3 and Future Observation Runs, Galaxies 8
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C. O’Hare, cajohare/AxionLimits: AxionLimits , https://cajohare.github.io/AxionLimits/ (2020)
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D. A. Palken, Enhancing the scan rate for axion dark matter: Quantum noise evasion and maximally informative analysis , Ph.D. thesis , University of Colorado, Boulder (2020)
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N. Aghanim et al. (Planck), Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641
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