Newtonian Gravity and Galaxy Rotation Curves: An Axisymmetric Green's Function Perspective

Fuente: arXiv
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Autore principale: Govaerts, Jan
Natura: Preprint
Pubblicazione: 2024
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author Govaerts, Jan
author_facet Govaerts, Jan
contents The standard proposal within the context of General relativity and its weak field Newtonian limit for the nature of dark matter is that it consists of dark matter particles of unknown type. In the present work and specifically for spiral galaxy rotation curves, an alternative possibility is explored, in the form of an axially symmetric vortex mass distribution of finite extent threading the centre of the galaxy and perpendicular to its disk. Some general considerations are developed and characteristic properties are identified, pointing to the potential interest of such an alternative to be studied in earnest.
format Preprint
id arxiv_https___arxiv_org_abs_2408_09977
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Newtonian Gravity and Galaxy Rotation Curves: An Axisymmetric Green's Function Perspective
Govaerts, Jan
General Relativity and Quantum Cosmology
High Energy Physics - Theory
The standard proposal within the context of General relativity and its weak field Newtonian limit for the nature of dark matter is that it consists of dark matter particles of unknown type. In the present work and specifically for spiral galaxy rotation curves, an alternative possibility is explored, in the form of an axially symmetric vortex mass distribution of finite extent threading the centre of the galaxy and perpendicular to its disk. Some general considerations are developed and characteristic properties are identified, pointing to the potential interest of such an alternative to be studied in earnest.
title Newtonian Gravity and Galaxy Rotation Curves: An Axisymmetric Green's Function Perspective
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2408.09977