Mathematics – Logic
Scientific paper
Mar 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aas...21115801g&link_type=abstract
American Astronomical Society, AAS Meeting #211, #158.01
Mathematics
Logic
Scientific paper
We perform three-dimensional smoothed particle hydrodynamics simulations in a realistic cosmological setting to investigate the expansion, feedback, and chemical enrichment properties of a 200 Msun pair-instability supernova in the high-redshift universe. We find that the SN remnant propagates for a Hubble time at z 20 to a final mass-weighted mean shock radius of 2.5 kpc (proper), roughly half the size of the HII region, and in this process sweeps up a total gas mass of 2.5*105 Msun. The morphology of the shock becomes highly anisotropic once it leaves the host halo and encounters filaments and neighboring minihalos, while the bulk of the shock propagates into the voids of the IGM. The SN entirely disrupts the host halo and terminates further star formation for at least 200 Myr, while in our specific case it exerts positive mechanical feedback on neighboring minihalos by shock-compressing their cores. In contrast, we do not observe secondary star formation in the dense shell via gravitational fragmentation, due to the previous photoheating by the progenitor star. We find that cooling by metal lines is unimportant for the entire evolution of the SN remnant, while the metal-enriched, interior bubble expands adiabatically into the cavities created by the shock, and ultimately into the voids with a maximum extent similar to the final mass-weighted mean shock radius. Finally, we conclude that dark matter halos of at least Mvir > 108 Msun must be assembled to recollect all components of the swept-up gas.
Bromm Volker
Greif Thomas
Johnson Jarrett L.
Klessen Ralf S.
No associations
LandOfFree
The First Supernova Explosions 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 First Supernova Explosions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The First Supernova Explosions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1035503