# Non-spherical dark matter structures detection

@article{Loizeau2022NonsphericalDM,
title={Non-spherical dark matter structures detection},
author={Nicolas Loizeau and Glennys R. Farrar},
journal={Journal of Cosmology and Astroparticle Physics},
year={2022},
volume={2022}
}
• Published 28 June 2021
• Physics
• Journal of Cosmology and Astroparticle Physics
A rotation curve inequality that holds for spherically symmetric mass distributions is derived, and tested against the SPARC galaxy rotation curves dataset. We identify several Galaxies, e.g. NGC7793 and UGC11557, which are candidates for hosting non-spherical dark matter structures that could be detected by more precise measurements.
1 Citations
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We use the galaxy rotation curves in the SPARC database to compare nine different dark matter (DM) and modified gravity models on an equal footing, paying special attention to the stellar

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