Mathematics – Logic
Scientific paper
Sep 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phdt.......112f&link_type=abstract
ProQuest Dissertations And Theses; Thesis (Ph.D.)--The University of Western Ontario (Canada), 2001.; Publication Number: AATNQ6
Mathematics
Logic
Scientific paper
The chemical rate network responsible for the formation of molecular hydrogen was incorporated into an N-body hydrodynamic code, in order to study the formation of the first cosmological objects at redshifts between 10 and 50. The implementation of the chemical and cooling processes was tested by comparing top hat simulations with theoretical predictions from a semi-analytic model and was in good agreement. One objective was to determine the minimum mass (MSG(z)) of perturbations that could become self-gravitating (a prerequisite for star formation), and the redshift at which this occurred. Cosmological simulations with realistic initial conditions produced primordial objects that became self-gravitating at redshifts in agreement with the MSG( z) results from the top hat simulations. The rotation of the core gas was directly related to its mass, indicating that greater mass was required to reach the self-gravitating state in the presence of rotational support. The universal fraction of self-gravitating gas increased from 10-4 at z = 23 to 5 x 10-3 at z = 10, and provides an upper constraint on the efficiency of early star formation. Simulations have been performed of supernovae explosions in spherically symmetric test objects, and in realistic primordial objects. These simulations indicated that even one supernova can remove a substantial amount of the gas from the parent object. The removal of this gas caused a drop in the depth of the gravitational potential well, which subsequently produced a drop in the kinetic energy and the density profile of the dark matter halo, but it did remain intact. Supernovae were found to have little kinetic effect on neighbouring objects. The photoionizing radiation produced by a supernova and its progenitor star created conditions ideal for rapid H2 formation after the photoionization ceased. This caused neighbouring objects to form self-gravitating cores somewhat sooner than they otherwise would have. A method for incorporating radiative transfer into smoothed particle hydrodynamics was developed and tested under some simple conditions.
No associations
LandOfFree
Simulation of primordial objects 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 Simulation of primordial objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Simulation of primordial objects will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1162361