3D Vortices and rotating solitons in ultralight dark matter
Ph. Brax, P. Valageas

TL;DR
This paper investigates vortex line formation and dynamics in rotating ultralight scalar dark matter halos, revealing stable rotating solitons with vortex lattices that emerge naturally in simulations, with implications for cosmic structure.
Contribution
It demonstrates the formation of stable, rotating solitons with vortex lattices in ultralight dark matter halos, combining analytical and numerical approaches.
Findings
Vortex lines form regular lattices aligned with total spin.
Rotating solitons exhibit oblate density profiles and solid-body rotation.
Vortex networks emerge dynamically within a few dynamical times.
Abstract
We study the formation and the dynamics of vortex lines in rotating scalar dark matter halos, focusing on models with quartic repulsive self-interactions. In the nonrelativistic regime, vortex lines and their lattices arise from the Gross-Pitaevskii equation of motion, as for superfluids and Bose-Einstein condensates studied in laboratory experiments. Indeed, in such systems vorticity is supported by the singularities of the phase of the scalar field, which leads to a discrete set of quantized vortices amid a curl-free velocity background. In the continuum limit where the number of vortex lines becomes very large, we find that the equilibrium solution is a rotating soliton that obeys a solid-body rotation, with an oblate density profile aligned with the direction of the total spin. This configuration is dynamically stable provided the rotational energy is smaller than the…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Advanced Thermodynamics and Statistical Mechanics
