First results from Au+Au collisions at $\sqrt(s_{NN})$ = 9.2 GeV in STAR

Details First results from Au+Au collisions at $\sqrt(s_{NN})$ = 9.2 GeV in STAR First results from Au+Au collisions at $\sqrt(s_{NN})$ = 9.2 GeV in STAR

2008-12-22

arxiv.org/abs/0812.4099v1

J.Phys.G36:064066,2009

Physics

Nuclear Physics

Nuclear Experiment

six pages, eight figures, proceedings for the talk given at Strange Quark Matter 2008, Beijing, China, October 6 - 10, 2008

Scientific paper

10.1088/0954-3899/36/6/064066

One of the primary aims of heavy-ion collisions is to map the QCD phase diagram and search for different phases and phase boundaries. RHIC Energy Scan Program was launched to address this goal by studying heavy-ion collisions at different center of mass energies. The first test run with Au+Au collisions at $\sqrt{s_{NN}}$ = 9.2 GeV took place in early 2008. The large acceptance STAR detector has collected few thousands minimum bias collisions at this beam energy. We present the first results for identified particle yields and particle ratios. The results for the azimuthal anisotropy parameters $v_1$ and $v_2$ and those from pion interferometry measurements are also discussed in this paper. These results are compared to data from the SPS at similar beam energies.

Affiliated with

Also associated with

No associations

Rating

First results from Au+Au collisions at $\sqrt(s_{NN})$ = 9.2 GeV in STAR 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 First results from Au+Au collisions at $\sqrt(s_{NN})$ = 9.2 GeV in STAR, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and First results from Au+Au collisions at $\sqrt(s_{NN})$ = 9.2 GeV in STAR will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-538304