Computer Science
Scientific paper
Aug 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..421o&link_type=abstract
THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1
Computer Science
Dark Matter, Galaxies, Supernovae, Star Formation, Dark Matter, Galactic Halo, Supernovae, Star Formation
Scientific paper
``The Core-Cusp problem'' is one of the open questions on Cold Dark Matter (CDM) cosmology. It is a discrepancy about the mass-density distribution of a dark matter halo between theory and observation. We study about the dynamical response of a virialized system with a central cusp to a mass loss driven by supernova feedback from the galaxy center using collisionless N-body simulations. Our results show that the system expands and recovers a new equilibrium state as a loosely bound core, if a certain fraction of the initial mass is lost from the galactic center on a shorter timescale in comparison to the mean crossing time in the system. The dynamical evolution of the central density profile is determined not only by the amount of gas removal but also by its timescale. We furthermore discuss the relation among the feedback parameters, the star formation rate and the metal enrichment.
Mori Masao
Ogiya Go
No associations
LandOfFree
The core-cusp problem in CDM halos and supernova feedback does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The core-cusp problem in CDM halos and supernova feedback, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The core-cusp problem in CDM halos and supernova feedback will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1862738