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.
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.
Publication: The analysis is under preparation for publication, with the same author list.
Presenters
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Felipe J. J Llanes-Estrada
Univ Complutense
Authors
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Adriana Bariego Quintana
Univ. Complutense de Madrid and Univ. Autónoma de Madrid
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Felipe J. J Llanes-Estrada
Univ Complutense
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Oliver Manzanilla Carretero
Univ. Complutense de Madrid