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Main Authors: Bianchi, Gabriele, Re, Federico, Piattella, Oliver Fabio
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2510.21470
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author Bianchi, Gabriele
Re, Federico
Piattella, Oliver Fabio
author_facet Bianchi, Gabriele
Re, Federico
Piattella, Oliver Fabio
contents We argue that the standard post-Newtonian expansion scheme used in General Relativity leaves room for time-space components $g_{ti}$ of the metric to be of the same order of the usual gravitational potential. We explore this possibility and find that such leading order contributions to $g_{ti}$ are related to the Coriolis field of Newton-Cartan gravity. We investigate the possibility that Coriolis fields mimic dark matter effects in disk galaxies. We find solutions from their field equations that sustain the velocity rotation curves in the bulge region and beyond it, notably describing flattish velocity profiles. We dub such solutions Dark Coriolis Fields.
format Preprint
id arxiv_https___arxiv_org_abs_2510_21470
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Dark Coriolis Fields
Bianchi, Gabriele
Re, Federico
Piattella, Oliver Fabio
General Relativity and Quantum Cosmology
We argue that the standard post-Newtonian expansion scheme used in General Relativity leaves room for time-space components $g_{ti}$ of the metric to be of the same order of the usual gravitational potential. We explore this possibility and find that such leading order contributions to $g_{ti}$ are related to the Coriolis field of Newton-Cartan gravity. We investigate the possibility that Coriolis fields mimic dark matter effects in disk galaxies. We find solutions from their field equations that sustain the velocity rotation curves in the bulge region and beyond it, notably describing flattish velocity profiles. We dub such solutions Dark Coriolis Fields.
title Dark Coriolis Fields
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2510.21470