Numerical GPP-Euler simulations show BECDM vortex lines stay stable under baryonic collapse, seed gas condensation, and imprint ring-like features that could serve as observational tracers.
Imprint- ing vortices in a bose-einstein condensate using topolog- ical phases,
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Kinematic Imprints of vortex-lines of BEC Dark Matter on Baryonic Matter
Numerical GPP-Euler simulations show BECDM vortex lines stay stable under baryonic collapse, seed gas condensation, and imprint ring-like features that could serve as observational tracers.