Scalar Field Dark Matter: head-on interaction between two structures
arXiv:astro-ph/0610682 · doi:10.1103/PhysRevD.74.103002
Abstract
In this manuscript we track the evolution of a system consisting of two self-gravitating virialized objects made of a scalar field in the newtonian limit. The Schrödinger-Poisson system contains a potential with self-interaction of the Gross-Pitaevskii type for Bose Condensates. Our results indicate that solitonic behavior is allowed in the scalar field dark matter model when the total energy of the system is positive, that is, the two blobs pass through each other as should happen for solitons; on the other hand, there is a true collision of the two blobs when the total energy is negative.
8 revtex pages, 11 eps figures. v2 matches the published version. v2=v1+ref+minor_changes
References in corpus (20)
- Cold and Fuzzy Dark Matter
- A New Cosmological Model of Quintessence and Dark Matter
- A Further Analysis of a Cosmological Model of Quintessence and Scalar Dark Matter
- Scalar Fields as Dark Matter in Spiral Galaxies
- Evolution of the Schrödinger--Newton system for a self--gravitating scalar field
- Gravitational cooling of self-gravitating Bose-Condensates
- Quintessence and Scalar Dark Matter in the Universe
- Galactic Halos of Fluid Dark Matter
- Quintessential Haloes around Galaxies
- Spherical Scalar Field Halo in Galaxies
- An alternative approach to the galactic dark matter problem
- Newtonian Collapse of Scalar Field Dark Matter
- Galactic Collapse of Scalar Field Dark Matter
- Accretion disk onto boson stars: a way to supplant black holes candidates
- Numerical studies of Phi^2-Oscillatons
- Cosmological constraints on quintessential halos
- Scalar Field Dark Matter: non-spherical collapse and late time behavior
- Modelling the rotational curves of spiral galaxies with a scalar field
- On the nature of dark matter
- Scalar dark matter in spiral galaxies
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- On the mass of ultra-light bosonic dark matter from galactic dynamics
- Interference of Dark Matter Solitons and Galactic Offsets
- Rotation curves of rotating galactic BEC dark matter halos
- Solitons in the dark: non-linear structure formation with fuzzy dark matter
- Collisional interactions between self-interacting non-relativistic boson stars: effective potential analysis and numerical simulations
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- Investigation of two colliding solitonic cores in Fuzzy Dark Matter models
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- Gravity- and temperature-driven phase transitions in a model for collapsed axionic condensates
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- A Newtonian Analysis of Multi-scalar Boson Stars with Large Self-couplings
- Stationary solutions of the Schrödinger-Poisson-Euler system and their stability
- Construction and evolution of equilibrium configurations of the Schrödinger-Poisson system in the Madelung frame
- Solving the Schrodinger Poisson System using the coordinate Adaptive Moving Mesh method
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- Tightly bound solitons and vortices in three-dimensional bosonic condensates with the electromagnetically-induced gravity
- Could primordial galactic Magnetic Fields be generated by Charged Ultra-Light Boson Dark Matter?
- Fundamental fields around compact objects: Massive spin-2 fields, Superradiant instabilities and Stars with dark matter cores
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- Integrating factor techniques applied to the Schrödinger-like equations. Comparison with Split-Step methods