Stationary BECDM core and vortex solutions around a black hole exist across self-interaction strengths, with stable branches identified via the enthalpy turning-point criterion.
Scalar field dark mat- ter: Nonspherical collapse and late-time behavior
2 Pith papers cite this work, alongside 81 external citations. Polarity classification is still indexing.
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Self-interaction changes the energy-mass scaling of BECDM core mergers from E proportional to minus M cubed to milder forms, altering mass retention, while an ideal gas only modifies the gravitational background without changing the bosonic scaling.
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Equilibrium Core and Vortex Solutions of Bose Einstein Condensate Dark Matter around a Black Hole
Stationary BECDM core and vortex solutions around a black hole exist across self-interaction strengths, with stable branches identified via the enthalpy turning-point criterion.
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Effects of Self-Interaction and of an Ideal Gas in Binary Mergers of Bosonic Dark Matter Cores
Self-interaction changes the energy-mass scaling of BECDM core mergers from E proportional to minus M cubed to milder forms, altering mass retention, while an ideal gas only modifies the gravitational background without changing the bosonic scaling.