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    Effects of new forces on scalar dark matter solitons

    Alize Sucsuzer1,*, Mark P. Hertzberg1,†, and Michiru Uwabo-Niibo2,‡

    • 1Institute of Cosmology, Department of Physics and Astronomy Tufts University, Medford, Massachusetts 02155, USA
    • 2Cosmology, Gravity, and Astroparticle Physics Group, Center for Theoretical Physics of the Universe, Institute for Basic Science (IBS), Daejeon, Korea

    • *Contact author: alize.sucsuzer@tufts.edu
    • †Contact author: mark.hertzberg@tufts.edu
    • ‡Contact author: michiru@ibs.re.kr

    Phys. Rev. D 113, 063575 – Published 31 March, 2026

    DOI: https://doi.org/10.1103/qqzf-fv8h

    Abstract

    New long range forces acting on ordinary matter are highly constrained. However it is possible such forces act on dark matter, as it is less constrained observationally. In this work, we consider dark matter to be made of light bosons, such as axions. We introduce a mediator that communicates a new force between dark matter particles, in addition to gravity. The mediator is taken to be light, but not massless, so that it can affect small scale galactic behavior, but not current cosmological behavior. As a concrete application of this idea, we analyze the effects on scalar dark matter solitons bound by gravitation, i.e., boson stars, which have been claimed to potentially provide cores of galaxies. We numerically determine the soliton’s profiles in the presence of this new force. We also extend the analysis to multiple mediators. We show that this new force alters the relation between core density and core radius in a way that can provide improvement in fitting data to observed galactic cores, but for couplings of order the gravitational strength, the improvement is only modest.

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