Cosmological Simulations of the Formation of Primordial Gas Clouds

Details Cosmological Simulations of the Formation of Primordial Gas Clouds Cosmological Simulations of the Formation of Primordial Gas Clouds

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..666..147y&link_type=abstract

THE EMERGENCE OF COSMIC STRUCTURE: Thirteenth Astrophysics Conference. AIP Conference Proceedings, Volume 666, pp. 147-150 (200

Astronomy and Astrophysics

Astrophysics

Dark Matter, Origin And Formation Of The Universe

Scientific paper

We study the formation of primordial star-forming clouds in a ΛCDM universe using large N-body/SPH simulations. The simulations include non-equilibrium 9 species (e-, H, H+, He, He+, He++, H2, H2+, H-) chemistry and hydrogen molecular cooling. We determine that the critical halo mass to form primordial star-forming clouds is 5 × 105h-1Msolar, with a weak dependence on redshift in a range z > 16.

Affiliated with

Also associated with

No associations

Rating

Cosmological Simulations of the Formation of Primordial Gas Clouds 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 Cosmological Simulations of the Formation of Primordial Gas Clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmological Simulations of the Formation of Primordial Gas Clouds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1370598