Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf..497l&link_type=abstract
ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,
Astronomy and Astrophysics
Astronomy
Scientific paper
Ultra-relativistic nucleus-nucleus collisions create a state of matter of high temperature and small baryo-chemical potential, which is similar to the thermodynamical conditions in the primordial universe. Recent analyses of Au+Au collisions at RHIC revealed the temperature, size and density of the system. Thus, a comparison to the primordial universe can be attempted. In particular, two observables shall be investigated, namely (1) the temperature at baryon freeze-out (t≃10 fm/c in the Au+Au collision) and (2) the matter density at the partonic stage (t≤1 fm/c).
No associations
LandOfFree
a Comparison Between AN Ultra-Relativistic AU+AU Collision and the Primordial Universe 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 a Comparison Between AN Ultra-Relativistic AU+AU Collision and the Primordial Universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and a Comparison Between AN Ultra-Relativistic AU+AU Collision and the Primordial Universe will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1466839