Pion Interferometry of $\sqrt{s_{NN}} = 130$ GeV Au+Au Collisions at RHIC

Details Pion Interferometry of $\sqrt{s_{NN}} = 130$ GeV Au+Au Collisions at RHIC Pion Interferometry of $\sqrt{s_{NN}} = 130$ GeV Au+Au Collisions at RHIC

2001-07-11

arxiv.org/abs/nucl-ex/0107008v1

Phys.Rev.Lett.87:082301,2001

Physics

Nuclear Physics

Nuclear Experiment

6 pages, 3 figures; accepted to Phys Rev Lett; data tables available at STAR web site http://www.star.bnl.gov/ Click on "Publi

Scientific paper

10.1103/PhysRevLett.87.082301

Two-pion correlation functions in Au+Au collisions at $\sqrt{s_{NN}} = 130$ GeV have been measured by the STAR (Solenoidal Tracker at RHIC) detector. The source size extracted by fitting the correlations grows with event multiplicity and decreases with transverse momentum. Anomalously large sizes or emission durations, which have been suggested as signals of quark-gluon plasma formation and rehadronization, are not observed. The HBT parameters display a weak energy dependence over a broad range in $\sqrt{s_{NN}}$.

Affiliated with

Also associated with

No associations

Rating

Pion Interferometry of $\sqrt{s_{NN}} = 130$ GeV Au+Au Collisions at RHIC 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 Pion Interferometry of $\sqrt{s_{NN}} = 130$ GeV Au+Au Collisions at RHIC, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Pion Interferometry of $\sqrt{s_{NN}} = 130$ GeV Au+Au Collisions at RHIC will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-192600