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Gravitational cooling of self-gravitating Bose-Condensates

3 Pith papers cite this work, alongside 202 external citations. Polarity classification is still indexing.

3 Pith papers citing it
202 external citations · Pith
abstract

Equilibrium configurations for a self-gravitating scalar field with self-interaction are constructed. The corresponding Schr\"odinger-Poisson (SP) system is solved using finite differences assuming spherical symmetry. It is shown that equilibrium configurations of the SP system are late-time attractor solutions for initially quite arbitrary density profiles, which relax and virialize through the emission of scalar field bursts; a process dubbed gravitational cooling. Among other potential applications, these results indicate that scalar field dark matter models (in its different flavors) tolerate the introduction of a self-interaction term in the SP equations. This study can be useful in exploring models in which dark matter in galaxies is not point-like.

representative citing papers

The three dynamical fates of Boson Stars

gr-qc · 2019-07-18 · unverdicted · novelty 3.0

Numerical classification of spherically symmetric boson star evolutions into stable, black-hole-forming, and exploding categories via constrained evolution of the Einstein-Klein-Gordon system.

Dynamical Boson Stars

gr-qc · 2012-02-27 · unverdicted · novelty 2.0

Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.

citing papers explorer

Showing 3 of 3 citing papers.

  • Vortex-reconnection energy bounds in Bose-Einstein-condensed and superfluid dark matter halos astro-ph.GA · 2026-07-08 · conditional · none · ref 243 · internal anchor

    Vortex reconnections in BEC/superfluid dark-matter cores can transfer at most 0.06–4.5% of the virial energy in 10 Gyr under fiducial assumptions, so they cannot appreciably restructure the core.

  • The three dynamical fates of Boson Stars gr-qc · 2019-07-18 · unverdicted · none · ref 1 · internal anchor

    Numerical classification of spherically symmetric boson star evolutions into stable, black-hole-forming, and exploding categories via constrained evolution of the Einstein-Klein-Gordon system.

  • Dynamical Boson Stars gr-qc · 2012-02-27 · unverdicted · none · ref 235 · internal anchor

    Boson stars are particle-like solutions in general relativity that model dark matter, black hole mimickers, and binary systems.