Gravothermal collapse of isolated self-interacting dark matter haloes: N-body simulation versus the fluid model

Self-interacting dark matter (SIDM) is a collisional form of cold dark matter (CDM), originally proposed to solve problems that arose when the collisionless CDM theory of structure formation was compared with observations of galaxies on small scales. The quantitative impact of the proposed elastic c...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2011-08, Vol.415 (2), p.1125-1137
Hauptverfasser:	Koda, Jun, Shapiro, Paul R.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics Collapse Computer simulation cosmology: theory Dark matter Earth, ocean, space Elastic scattering Exact sciences and technology Fluid flow galaxies: haloes galaxies: kinematics and dynamics Halos Mathematical models methods: numerical Monte Carlo methods Monte Carlo simulation
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!