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Dark Matter-Induced Baryonic Feedback in Galaxies

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arxiv 2309.08661 v2 pith:BFYTCS52 submitted 2023-09-15 hep-ph astro-ph.COastro-ph.GA

Javier F. Acevedo , Haipeng An , Yilda Boukhtouchen , Joseph Bramante , Mark Richardson , Lucy Sansom This is my paper · ORCID
classification hep-phastro-ph.COastro-ph.GA
keywords darkfeedbackbaryonicgalaxiesmatterdemonstratematter-inducedaffect
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We demonstrate that non-gravitational interactions between dark matter and baryonic matter can affect structural properties of galaxies. Detailed galaxy simulations and analytic estimates demonstrate that dark matter which collects inside white dwarf stars and ignites Type Ia supernovae can substantially alter star formation, stellar feedback, and the halo density profile through a dark matter-induced baryonic feedback process, distinct from usual supernova feedback in galaxies.

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Cited by 1 Pith paper

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  1. Dark-matter-induced transients over cosmic time: The role of star formation history profiles

    astro-ph.GA 2025-05 conditional novelty 5.0 of 10

    A closed-form formula for star formation histories in galactocentric radial shells is derived from empirical galaxy scaling relations and two star formation history models.

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