Spiral galaxy rotation favors prolate dark matter haloes

POSTER

Abstract

The flattening rotation velocity v(r)→constant found by Rubin and collaborators, and very distinct in the SPARC galaxy rotation data coincides with Kepler's law in one less dimension.  Thus, it is naturally reproduced by filamentary sources of gravity, for example elongated dark matter distributions with the axis of prolateness perpendicular to the galactic plane as we here consider.

This theoretical understanding is borne out by the detailed fits to the rotation data that we report: for equal dark matter profile, elongated distributions provide smaller χ^2 than purely spherical ones.

This is of consequence for the estimated dark matter density near Earth.

*Supported by spanish grant MICINN: PID2019-108655GB-I00 (Spain), and Univ. Complutense de Madrid under research group 910309 and the IPARCOS institute.

Publication: The analysis is under preparation for publication, with the same author list.

Presenters

  • Felipe J. J Llanes-Estrada

    • Univ Complutense

Authors

  • Adriana Bariego Quintana

    • Univ. Complutense de Madrid and Univ. Autónoma de Madrid
  • Felipe J. J Llanes-Estrada

    • Univ Complutense
  • Oliver Manzanilla Carretero

    • Univ. Complutense de Madrid