freezer runs

These are runs that Bernd and I are doing, from data generated by Hylander.
Go to: runs 2-10 (on another page)
runs 11-12 (on another page)
run 13 (on another page)
run 14 Bernd EOS #??
run 15 ''
run 16 ''
run 17 ''
run 18 ''
run 19 ''
run 20 ''
run 21 ''
run 22 ''
run 23 New data set
run 24 ''
run 25 ''
run 26 ''
run 27 ''
run 28 ''
run 29 ''
runs 30-up (on another page)
Last update: 12 feb98

RUN 014

19 December 97. A run using MC data sets from Bernd. Here are the inputs: singles pi+, pi-, K+, K-, and pairs pi+, pi-, K+, K-, and these were the input parameters. This run was with no systematic errors, and resulted in a bad chi**2. See the log file.


RUN 015

19 December 97. Same as run 14, but with added 10% systematic errors, see the input parameter file. See the log file. (note that the input files had an implicit efficiency of 90% in it.


RUN 016

6 Jan 1998. Same as run 15, but to compensate for the implicit efficiency, the input Z and A are reduced by a factor of 0.9.
See the input parameter file. See the log file. This run took a long time; normally, 15-20 iterations are done, but this one took 57 rounds. The chisq/dof overall is 24, not too good. If you look at the log file, you can see that this is completely dominated by the terrible fit to the pion BE data, also reflected in the huge R found.

 Here is the BEST point !
 **********************************************

 Total chi^2 =  59739.75630549779
 chi^2/d.o.f =  24.61465031128875
 Probability of perfect model =  .0

 Fixed parameters:
   aT =   -.9900000
 lamK =   1.0000000
normpi=   1.0000000
normK =   1.0000000

 Variable parameters:
    T =   98.8762643 +/-   3.2403190 MeV
 vT/c =     .8254691 +/-    .0197095
  et0 =    2.6069185 +/-    .0251666
muB/T =    3.9538487 +/-    .2574856
  tau =     .0153866 +/-    .0017893 fm/c
    R =   98.8611252 +/-   1.7384788 fm
  ycm =    -.0100097 +/-    .0110566
   fs =    1.3466445 +/-    .0991520
  lam =     .2105840 +/-    .0073149

 Calculated Quantities:
 vs/c =    -.0100094 +     .0110563    -.0110539
 vL/c =     .9891774 +     .0005285    -.0005555
  muB =  390.9417876 +   15.3943255  -16.3575785 MeV
   t1 =     .0015387 +     .0001779    -.0001782 fm/c
   t3 =     .1048669 +     .0140059    -.0136073 fm/c
t2-t1 =     .0138479 +     .0016007    -.0016036 fm/c
 dtau =     .0145181 +     .0017016    -.0016947 fm/c
   z3 =     .1037320 +     .0129497    -.0134400 fm
  muS =   32.0679171 +    3.2786466   -3.0755850 MeV
  muI =   -2.9707652 +     .3574922    -.3846667 MeV
 Bar# =   10.4388677 +    1.4051798   -1.2460073
Bproj =    -.0113163 +     .0125133    -.0126092
Btarg =   10.4501840 +    1.4091967   -1.2484270
brdn1 =    .00727418 +    .00164945   -.00143050 fm^-3
brdn2 =    .00726493 +    .00164859   -.00142927 fm^-3

---------------------------------------------------------

 chi^2/dof for each data set ...
 335 333.762315270936 365.2731403196502 1.09441097333932
 335 333.762315270936 527.0940649252853 1.57924978587654
 257 256.0504926108375 400.3445204002943 1.56353739576188
 213 212.2130541871921 870.4608626349222 4.10182524335705
 324 322.8029556650246 28304.91590757799 87.68481022506574
 324 322.8029556650246 28306.71355607188 87.69037909753838
 324 322.8029556650246 514.880639684714 1.59503074754684
 324 322.8029556650246 450.0736138830471 1.3942673261954
    chi^2 = 59739.75630549779        chi^2/dof = 24.61465031128875
chi^2_min =   59739.756305497789


RUN 017

7 Jan 1998. Same as run 16, but the input singles data are now restricted to rapidity -1>y>+1. This is done because this particular EOS leads to dn/dy distributions which have a central peak and pronounced shoulders. FREEZER has no shoulders, and therefore should have trouble with the large-y data.
The input Z and A are reduced by a factor of 0.9, as before.
Input files are: singles pi+, pi-, K+, K-, and pairs pi+, pi-, K+, K-
See the input parameter file. See the log file.

RUN 018

10 Jan 1998. Same as run 17, but with R=8.0 fm and fixed. This was because we saw in run 17 that the radius had run away.
See the input parameter file. See the log file.
The chisq/ndf went up, as expected, to 66, but T is now very large, compensated by a very low v. Apparently, what was found was just another point in the T-v valley of low chisq.

RUN 019

12 Jan 1998. Same as run 18, but only fitting to the singles.
See the input parameter file. See the log file.

RUN 020

13 Jan 1998. Same as run 19, but R is free and systematic errors set to 0 (note the individual point already have a 5% error on them).
See the input parameter file. See the log file.

RUN 021

14 Jan 1998. Same as run 20, but T is fixed at 140. Curent settings: (note the individual point already have a 5% error on them).
See the input parameter file. See the log file.

RUN 022

15 Jan 1998. Same as run 21, but add the kaon correlations (note the individual point already have a 5% error on them).
See the input parameter file. See the log file.






RUN 023

26 Jan 1998. A new data set: the 'efficiency' is now 100%, and there are more integration points in the pairs files. This set is limited to -1< y < +1.

Input files are: singles pi+, pi-, K+, K-, and pairs pi+, pi-, K+, K-
All parameters are free for this run. See the input parameter file. and the output log file.
aT runs away to +1, and the program stops.


RUN 024

****************** ignore everything below this line ******************* 15 Jan 1998. Same as run 23, but with aT fixed at +0.99, as per instruction from FREEZER. Terrible fit. R goes off to infinity, and tau goes to 0.

See the input parameter file. and the output log file.


RUN 025

20 Jan 1998. Same as

See the input parameter file. and the output log file.


RUN 026

2 feb 1998. T=140, aT=-1, tau=

See the input parameter file. and the output log file.


RUN 027

3 feb 1998. Singles only, T fixed at 140, aT fixed at -1.

See the input parameter file. and the output log file. OK run found reasonable v.


RUN 028

5 feb 1998. Singles only, let T loose, aT fixed at -1.

See the input parameter file. and the output log file.
T floated down from 140 to 116.


RUN 029

6 feb 1998. Singles only, everything free

See the input parameter file. and the output log file.
















Basically, it was clear we could not get a good fit to all the data sets. At a meeting on 11 feb 98, Ray suggested we should increase the number of integration points. This we did, and the results are on the next page.