Blast-Wave fit to spectra and HBT in AuAu @ 19.6 GeV
1. Blast Wave fit to spectra and HBT from AuAu@19GeV.
Here, I present results of BW fit to spectra (from Daniel Cebra) and HBT radii from the most central [0-10%] Au+Au@19.6 GeV. I used Fabrice's code to do the fit.
Figure 1: Light particle spectra
Figure 2: HBT radii vs kT
Chi2/(number of data points) | ||
π+ spectra | 60.0394 / 31 | |
π- spectra | 50.8827 / 31 | |
K+ spectra | 43.3543 / 20 | |
K- spectra | 32.4811 / 19 | |
p spectra | 47.1665 / 28 | |
pbar spectra | 28.2348 / 28 | |
π Rout | 3.91632 / 4 | |
π Rside | 1.59221 / 4 | |
π Rlong | 0.832901 / 4 | |
Total |
268.5/164 | |
T (MeV) |
106 ± 2 | |
Rho0 | 0.83 ± 0.02 | |
Rho2 | 0.058 | fixed |
Rho4 | 0 | fixed |
Rx (fm) | 11.1 ± 0.5 | |
Ry (fm) | 11.1 | fixed |
As | 0 | fixed |
Tau (fm/c) | 7.3 ± 0.7 | 6.8 ± 0.3 -value obtained from the fit to Rlong - see Fig. 4 and Fig. 5 |
Deltat (fm/c) | 1.7 ± 0.7 |
Table 1: Fit results
In case someone wants to compare those results to BW fit results to RHIC data at 130 GeV presented in Retiere, Lisa, Phys.Rev.C70:044907,2004 I put a copy of the table from this paper here.
2. Comparision of BW fit results from AuAu@200 GeV and AuAu@19 GeV.
Figure 3: BW fit results to AuAu@200 GeV (empty points) and AuAu@19GeV (full points)
3. System evolution time (tau).
Figure 4: Fit to mT dep of Rlong from the most central AuAu@19GeV. Rlong=tau * sqrt{T/mT2(mT/T)/K1(mT/T)} K
Figure 5: System evolution time vs multiplicity. Data from AuAu@200GeV taken from Phys. Rev. C 71 (2005) 044906.
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