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Stable vortex in Bose-Einstein condensate dark matter

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arxiv 2103.07856 v1 pith:RB3C7SFH submitted 2021-03-14 nlin.PS cond-mat.quant-gasgr-qc

Stable vortex in Bose-Einstein condensate dark matter

classification nlin.PS cond-mat.quant-gasgr-qc
keywords vortexmatterangularbeenbose-einsteincondensatedarkincluding
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The nature of dark matter (DM) is one of the most fascinating unresolved challenges of modern physics. One of the perspective hypotheses suggests that DM consists of ultralight bosonic particles in the state of Bose-Einstein condensate (BEC). The superfluid nature of BEC must dramatically affect the properties of DM matter including quantization of the angular momentum. Angular momentum quantum in the form of a vortex line is expected to produce a considerable impact on the luminous matter in galaxies including density distribution and rotation curves. We investigate the evolution of spinning DM cloud with typical galactic halo mass and radius. Analytically and numerically stationary vortex soliton states with different topological charges have been analyzed. It has been shown that while all multi-charged vortex states are unstable, a single-charged vortex soliton is extremely robust and survives during the lifetime of the Universe.

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Cited by 1 Pith paper

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  1. Vortex State of Ultralight Dark Matter and the Fornax Timing Problem

    astro-ph.GA 2026-07 conditional novelty 5.0

    A vortex state of ultralight dark matter suppresses dynamical friction for co-rotating globular clusters, potentially resolving the Fornax timing problem.