Run 6 Inclusive Jet Cross Section (Tai Sakuma)
Inclusive Jet Cross Sections in Proton-proton collisions at √s = 200 GeV
Tai Sakuma
Preliminary Results
Introduction
We measured the inclusive jet cross section in proton-proton collisions at 200 GeV using data collected with the STAR detector during RHIC Run-6. The jet cross section is an essential quantity to test the predictive power of Quantum Chromodynamics (QCD). We have made several improvements since the previous measurement from STAR [PRL 97 (2006) 252001]; the data size increased from 0.3 pb-1 to 5.4 pb-1; while the previous measurement used the Time Projection Chamber (TPC) and only the west side of the Barrel Electromagnetic Calorimeter (BEMC), which corresponds to the acceptance of 0 ≤ η ≤ 1, this measurement used the TPC and both sides of the BEMC (-1 ≤ η ≤ 1).
Jet Definition
Jets are sprays of particles which are moving approximately in the same direction from the collision point. We used the mid-point cone jet-finding algorithm with the cone radius 0.7 to define jets. Jets can be defined at three different levels: the parton level, the hadron level, and the detector level. The parton-level jets are outgoing partons of the hard interactions. The hadron-level jets are composed of products of hadronization and particle decay of the outgoing partons. They are predominantly hadrons, but may contain leptons and photons as well. The detector-level jets are detector responses to the hadron-level jets. They are made of energy deposited in BEMC towers and charged tracks reconstructed in the TPC.
Hadron-level Jet Yields
We estimated the hadron-level jet yields from the detector-level jet yields by inverting the response of the detector using a MC simulation. Consequently, the results have a tendency to be biased toward the predictions of the MC simulation. To minimize this bias, we used MC events which desciribe the data well.
Results
The results are in agreement with next-to-leading-order (NLO) perturbative QCD predictions which include corrections for non-perturbative effects. This agreement is evidence that the measured inclusive jet ALL [PRL 97 (2006) 252001] [PRL 100 (2008) 232003] can be interpreted in the framework of the QCD factorization. Furthermore, having a theoretical model that well describes the inclusive jet production is a crucial step toward dijet measurements.
Poster
There is a poster about the preliminary results.
A full size pdf file can be found at (pdf).
Analysis Detail
Please, visit this site for the detail: http://people.physics.tamu.edu/sakuma/star/jets/c100826_inclusive_jets/s0000_index_001/prelim.php
MC production for the di-jet cross section measurements in pp collisions at 200 GeV
Introduction
Originally, the MC samples generated for the inclusive jet analyses were used for the di-jet analyses. However it turns out that these samples were not sufficient for the di-jet analyses especially for unfolding the cross sections for the 2005 di-jets. To generate sufficient MC samples with available computing resources, MC generations were designed to generate events only in the region of the phase space where the di-jet events in the STAR acceptance come from.
Original MC sample
These are the distributions of pseudorapidity and scattering angle for the original MC samples. The left plots of each image is for all the generated events and the right plots are for the dijet events.
Significant portion of the dijet events come from only the regions inside the red boxes.
New MC sample
The new MC samples were generated only in those regions of the phase space from which most dijet events come.
How to run the patched PYTHIA 6 in starsim
The most of the MC production jobs that the spin PWG requested for the di-jet analysis didn't finish successfully
Patch for a bug in PYTHIA6
This page explains how to run the patched PYHIA 6 as the event generator for starsim. The starsim has a mechanism where a user can choose a specific version of Pythia to use at run time.This feature will be used.
Install shared objects for the patched PYTHIA for starsim
This tar ball contains the source files for the patched PYTHIA 6.205 and 6.4.10 in the form that fits to starsim.
Build the shared objects with the following commands.
tai@rcas6007% stardev
tai@rcas6007% tar xvfz patched_pythia_for_starsim.1.0.0.tar.gz
tai@rcas6007% consTwo shared objects should be built in the directory $MINE_LIB.
pythia_6410t.so
These are loadable modules for starsim which contain the patched PYTHIA 6.205 and 6.4.10, respectively.
run starsim
This is a smple kumac file load the shared object pythia_6410t.so and generated one hundred events.
tai@rcas6007% starsim
******************************************************
* Starting starsim NwGEANT= 20000000 NwPAW= 2000000 *
**********************pid= 22383**********************
******************************************************
* *
* W E L C O M E to starsim *
* *
* Version INITIAL 16 November 2006 *
* *
******************************************************
Workstation type (?=HELP) <CR>=1 : 0
Version 1.29/04 of HIGZ started
1***** GEANT Version 3.21/08 Released on 230697
0***** Correction Cradle Version 0.0800
***** RZMAKE. OLD RZ format selected for RZDOC
starsim > exec sample.kumacYou should be able to find the output my_pythia_file.fz if the MC production is successful.
If you have a question or comment, send email to sakuma@bnl.gov or add comment to this page.
Patch for a bug in PYTHIA6
This patch is included in PYTHIA from PYTHIA 6.412. You don't need to apply this patch if you are using PYTHIA 6.412 or newer.
Download Patch
If you need the patch for a different version of PYTHIA, email sakuma@bnl.gov.
Introduction
At the end of the year 2006, The spin PWG requested the MC productions with uncommon kinematical cuts for the measurement of
the 2005 di-jet cross sections in pp collisions.
The most of the MC production jobs didn't finish successfully.
The failure is due to a bug in PYTHIA 6. This page provides a patch for the bug.
If you want to run the patched PYTHIA as the event generator for starsim, the instruction can be found at "How to run the patched PYTHIA 6 in starsim."
Bug description
PYTHIA 6 has options to generate events only a specific region of the phase space. You can specify the region in terms of various variables such as pT, y, cos(theta), s, t, u, x1, x2, and other kinematical variables. With some sets of the values for the cuts, PYTHIA 6 behaves improperly especially when cuts are applied on both pT and cos(theta) simultaneously. This is a main program that can reproduce the improper behavior.
This main.f should be able to reproduce the bug for any version of PYTHIA between 6.2 and 6.4.11. From the version 6.4.12, this patch is included in PYTHIA.
You can compile and run for yourself with the following commands.
f77 main.f pythia-6.4.11.f
./a.outPYTHIA 6 can be found at the following websites.
With the main.f, PYTHIA will try to generate one thousand events of the pp collisions at 200 GeV in the following region of the phase space.
-0.2 < y < 1.2
-0.6 < cos(theta) < -0.3
With the main.f, the cross section does not converge and sometime
becomes negative.
And you will also constantly get the warning like
Warning: negative cross-section fraction -2.262E+01 in event 140
ISUB = 28; Point of violation:
tau = 2.930E-02, y* = 3.735E-01, cthe = -0.5988706, tau' = 0.000E+00and
Advisory warning: maximum violated by 1.505E+01 in event 243
XSEC(68,1) increased to 1.631E-01Then, PYTHIA will gradually slow down in generating events and won't make
it to generate one thousand events within an hour on an average PC.
Patch for the bug
These are the patches for the bug for PYHIA 6.4.11 and 6.205.
You can apply these patches, for example, in this way.
patch pythia-6.4.11.f < pythia-6.4.11-t.diffComments from the author of PYTHIA
I reported the bug and sent my patch to Torbjörn Sjöstrand, the author of PYTHIA. He responded "Thanks a lot for your input. Yes, you are right, this is a
possibility we missed so far. Will try to have your fix inserted for the next subversion. ... In retrospect the number of kinematics options grew to a level
where not all possible combinations were sufficiently tested".
In another email, I asked him if my patch is safe to use for serious physics study. Torbjörn Sjöstrand said
"So far as I can see the patch should be safe and not have any
undesirable consequences, but I could not give any 100%
guarantees".
The patch that I actually sent to the author is simpler than ones in the previous section.
In the patches in the previous section, I also modified the title logo such that it indicates that the program is modified.
Verification of the patch
I compared the cross sections computed with the original PYTHIA and the patched PYTHIA. I got a consistent result. I'll write the detail later.
How to implement the patch to Starsim
I figured out how to implement this patch in starsim.
How to run the patched PYTHIA 6 in starsim