STAR has collected data from the following collision energies (in decreasing energy order) : STAR has collected data from the following collision energies (in decreasing energy order) : - 200, 130, 62.4, 39, 19.6, 11.5, 9, 7.7 GeV
This presentation aims to show the work-in-progress analysis of the 39 GeV data sample Spectra shapes and particle ratios help connect collected data to observables that are expected to change in such a phase transition
The TPC is a barrel shaped detector consisting of a gas-filled chamber, magnet providing a strong uniform magnetic field, and an electric field between the center and endplates The TPC is a barrel shaped detector consisting of a gas-filled chamber, magnet providing a strong uniform magnetic field, and an electric field between the center and endplates We use measurements of the ionization energy loss (dE/dx) and momentum to identify particles
From Min-Bias Trigger |Vz| < 30 cm |Vr| < 2 cm 10 M events pass cuts Track-Quality Cuts |Dca| < 3 cm NHitFits > 25 NHitFits/NHitPoss > 0.51
For overlap areas we rely on extrapolated centroid positions and yields This is done independently in each particle-centered histogram, and across different rapidity bins
Cannot make a physics conclusions without corrections, which include: Cannot make a physics conclusions without corrections, which include:
Our work-in-progress min-bias π+/π- ratio at 39 GeV is similar to results from 19 GeV & 200 GeV Our work-in-progress min-bias π+/π- ratio at 39 GeV is similar to results from 19 GeV & 200 GeV Plans for the future include: - Efficiency Corrections
- Proton Background
- Energy Loss Corrections
- Investigate Rapidity Dependence
- K/Pi, p/Pi
- Integrated Yields & Ratios
Dostları ilə paylaş: |