The binding of cosmological structures by massless topological defects

ABSTRACT Assuming spherical symmetry and weak field, it is shown that if one solves the Poisson equation or the Einstein field equations sourced by a topological defect, i.e. a singularity of a very specific form, the result is a localized gravitational field capable of driving flat rotation (i.e. K...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2024-06, Vol.531 (1), p.1630-1636
1. Verfasser: Lieu, Richard
Format: Artikel
Sprache:eng
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Zusammenfassung:ABSTRACT Assuming spherical symmetry and weak field, it is shown that if one solves the Poisson equation or the Einstein field equations sourced by a topological defect, i.e. a singularity of a very specific form, the result is a localized gravitational field capable of driving flat rotation (i.e. Keplerian circular orbits at a constant speed for all radii) of test masses on a thin spherical shell without any underlying mass. Moreover, a large-scale structure which exploits this solution by assembling concentrically a number of such topological defects can establish a flat stellar or galactic rotation curve, and can also deflect light in the same manner as an equipotential (isothermal) sphere. Thus, the need for dark matter or modified gravity theory is mitigated, at least in part.
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stae1258