KPinn signal and Kpi2 background

This study was performed in the process of preparation of CKM proposal for PAC review in March 2001. The goal was to study kinematical suppression of Kpi2 background and acceptance of the signal. In proposal we would like to have 2 events out of 1M kpi2 to sneak into the signal region, and we wanted to verify that using Geant Monte-Carlo. This job was repeated several times, because different bugs/features were uncovered. Below is the summary of the studies.

try# date ckmgeant
version
Code
adjustments
Improvements samples
try1 Feb 23 v3_2 none First version with complete CKM geometry. BIVS has lead/scint structure. The DMS and RICH analysis codes are installed. Update geometry of UMS with larger chambers. 100k kpinn
535k kpi2
try2 Mar 3 v3_3 none Update KRICH so that it cuts off lower wavelengths. This improves angular resolution. Now have capability to use matrix elements in decays. Available decay matrix elements now include: K->e nu gamma K->mu nu gamma. Can now stop showering of particles in vetoes with SWIT 4 1 option. UMS analysis code is installed. 100k kpinn
1M kpi2
try3 Mar 10 v3_4 none KEAT's taken out of the vacuum and put at 2.6m separation. Vertex finding routine installed. KEAT's included in UMS pattern recognition and track fitting. Available decay matrix elements now include: K->pi nu nubar K->pi gamma gamma 100k kpinn
100k kpi2
100k kmu2
try4 Mar 12 v3_4 none 100k kpi2
try5 Mar 16 v3_5 Available decay matrix elements now include: K->pi e+ e-, K->pi mu+ mu- Tag initial kaon so that it can have hadronic interactions and still be forced to decay within specified region. Dead beam region added to DMS chambers. Mylar entrance window for vacuum chamber. 100k kpinn
100k kpi2
try6 Mar 16 v3_5a 100k kpinn
1M kpi2
try7 Mar 20 v3_5a 100k kpinn
1M kpi2
try8 Mar 23 v3_5a gukine.F , guout.F , gustep.F speedup by taking out calls to BIVS and VVS
CKM_read_user.F , keatana.F Kaon track calculated using 2 KEAT stations
bivs_geom.kumac Changed the tracking medium from air to vacuum for inside the BIVS.
ckmgeom.F Changed liquid helium into gaseous helium (affected only KEAT)
keat_geom.F , pwc_08_120_lrg.config Changed KEAT chamber separation to 320 cm
100k kpinn
1M kpi2
try9 Mar 27 v3_6 gukine.F , guout.F , gustep.F speedup by taking out calls to BIVS and VVS
ums_geom.F UMS helium bags geomerty fixed (were 0 thikness tubes)
BIVS now has vacuum in the interior. DMS straw tubes made of 'gaseous kapton'. KEAT stations separated to 3.2 m Kaon angle now calculated only from KEAT hits. 100k kpinn
1M kpi2
try10 Apr 29 v3_7 gukine.F , guout.F , gustep.F speedup by taking out calls to BIVS and VVS Go back to original DMS straw construction. Set fixed 10 micron precision for step size calculation in GEANT. GEANT now calculates tracking parameters automatically. Various geometry fixes, mostly to magnetic fields, allow this. Add 4 body decay modes:
pi+ pi- e+ nu (ubuf(1)=7)
pi+ pi- mu+ nu (ubuf(1)=8)
pi0 pi0 e+ nu (ubuf(1)=9)
pi0 pi0 mu+ nu (ubuf(1)=10)
pi0 mu+ nu gamma (ubuf(1)=11)
pi0 e+ nu gamma (ubuf(1)=12) w/o matrix element
Wire pitch in UMS fixed. Magnetic field kick correctly set to 99.8 MeV. Optimize VVS code.
100k kpinn
1M kpi2


Alexander Kushnirenko
Last modified: Thu May 3 01:49:45 CDT 2001