Last updated: August 9, 1996 by BL.
diffVM is a Monte Carlo generator for diffractive processes in ep collisions based on the VDM. The main author is Benno List.
There is also an overview over banks produced by and used to steer diffVM.
This overview is not exhaustive. Files with 1993 running conditions have been left out, since they are generally not available on the dice, and also the first round of 1994 Monte Carlos is not described, because new (and, of course, better) files are now available.
Generated: May 19, 1995 by B.L.
Version 1.05/01
1994 running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: E>8GeV, theta<175deg
Kinematic cuts: Q^2>4GeV^2, W>20GeV
W-dependence of the differential cross section: W^0.8
(epsilon_pom = 0.2) for the elastic case,
W^0.48 (epsilon_pom = 0.12) for the proton dissociation case
Slope parameter b is constant
Q^2 dependence: standard VDM propagator, R limited to 2
Remarks:
epsilon_pom was chosen differently for the elastic and proton dissociation
files to partially compensate the t_min effect.
The t_min effect leads for the proton dissociation case to a steeper rise
of the cross section with W than for the elastic case, because the phase
space for proton dissociation grows fast with W.
This is a result of the one-pomeron-exchange approximation, which is known
to lead to a too fast rise of the cross section with W for proton dissocyiation
(compare Tevatron results).
Known problems:
The Q^2-dependence is a bit too shallow
(tail to higher Q^2 values is a bit too large),
because VDM does not correctly describe the Q^2 behavior.
Recommendation:
reweight events with factor ((m^2+4GeV^2)/(m^2+Q^2))^0.5,
where m is the mass of the respective vector meson.
20000 events,
cross section estimate 940pb,
integrated luminosity 21.2pb^-1
b=5.5GeV^-2
/acs/mc/diffvm10/RHOELAS1.DIS.A00
/acs/mc/diffvm10/RHOELAS1.DIS.S30609.A00 - A01
RHOELAS1.DIS.S30609.R60017.A00 - A04 (removed from ACS!) /acs/mc/diffvm10/RHOELAS1.DIS.S30609.R60017.DST.A00
2000 events,
cross section estimate 96pb,
integrated luminosity 20.7pb^-1
b=5.5GeV^-2
/acs/mc/diffvm10/OMGELAS1.DIS.A00
/acs/mc/diffvm10/OMGELAS1.DIS.S30609.A00
OMGELAS1.DIS.S30609.R60017.A00 (removed from ACS!) /acs/mc/diffvm10/OMGELAS1.DIS.S30609.R60017.DST.A00
3000 events,
cross section estimate 154pb,
integrated luminosity 19.5pb^-1
b=4.5GeV^-2
/acs/mc/diffvm10/PHIELAS1.DIS.A00
/acs/mc/diffvm10/PHIELAS1.DIS.S30609.A00
PHIELAS1.DIS.S30609.R60017.A00 (removed from ACS!) /acs/mc/diffvm10/PHIELAS1.DIS.S30609.R60017.DST.A00
20000 events,
cross section estimate 360pb,
integrated luminosity 56pb^-1
b=3.5GeV^-2
/acs/mc/diffvm10/RHOPDIS1.DIS.A00
/acs/mc/diffvm10/RHOPDIS1.DIS.S30609.A00 - A04
RHOPDIS1.DIS.S30609.R60017.A00 - A06 (removed from ACS!) /acs/mc/diffvm10/RHOPDIS1.DIS.S30609.R60017.DST.A00
2000 events,
cross section estimate 39pb,
integrated luminosity 51pb^-1
b=3.5GeV^-2
/acs/mc/diffvm10/OMGPDIS1.DIS.A00
/acs/mc/diffvm10/OMGPDIS1.DIS.S30609.A00
OMGPDIS1.DIS.S30609.R60017.A00 (removed from ACS!) /acs/mc/diffvm10/OMGPDIS1.DIS.S30609.R60017.DST.A00
3000 events,
cross section estimate 65pb,
integrated luminosity 46pb^-1
b=2.5GeV^-2
/acs/mc/diffvm10/PHIPDIS1.DIS.A00
/acs/mc/diffvm10/PHIPDIS1.DIS.S30609.A00
PHIPDIS1.DIS.S30609.R60017.A00 - A01 (removed from ACS!) /acs/mc/diffvm10/PHIPDIS1.DIS.S30609.R60017.DST.A00
Generated: August 28, 1995 by B.L.
Version 1.06/00
1994 running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: E>8GeV, theta<175deg
Kinematic cuts: Q^2>6GeV^2, W>20GeV
W-dependence of the differential cross section:
W^0.68 (epsilon_pom = 0.17) for the proton dissociation case
Slope parameter b is constant
Q^2 dependence: standard VDM propagator, R limited to 3.5
Remarks:
epsilon_pom was chosen in a way to partially compensate the t_min effect.
The t_min effect leads for the proton dissociation case to a steeper rise
of the cross section with W than for the elastic case, because the phase
space for proton dissociation grows fast with W.
This is a result of the one-pomeron-exchange approximation, which is known
to lead to a too fast rise of the cross section with W for proton dissocyiation
(compare Tevatron results).
After integration over t and M_X the gamma-p cross section rises
approximately as W^1.0.
Modelling of proton dissociation
This file is produced in a special mode of diffVM.
For masses M_X of the dissociating proton system below 2.0GeV the
dissociating proton is treated as N* resonance, as usual.
Above 2.0GeV, however, it is assumed that the proton decays to a nucleon (p or n),
and a number of charged and neutral pions, following the KNO scaling
law (see K. GOULIANOS: Diffractive interactions of hadrons at
high energies. Phys. Rep. 101 (1983) 169-219.).
These particles are then distributed isotropically in phase space,
using the phase space generator RAMBO (R. KLEISS, W.J. STIRLING & S.D. ELLIS:
A new Monte Carlo treatment of multiparticle phase space at high energies.
Comp. Phys. Commun. 40 (1986) 359-373.).
This is an extreme model which is not expected to describe the data,
particularily the p_T spectrum of the pions originating from the
phase space decay is too hard. Therefore results obtained with this
Monte Carlo should only be taken as cross check of the robustness of
the acceptance of forward detectors against extreme dissociation
models.
Known problems:
The Q^2-dependence is a bit too shallow
(tail to higher Q^2 values is a bit too large),
because VDM does not correctly describe the Q^2 behavior.
Recommendation:
reweight events with factor ((m^2+4GeV^2)/(m^2+Q^2))^0.5,
where m is the mass of the respective vector meson.
20000 events,
cross section estimate 500pb,
integrated luminosity 40pb^-1
b=3.5GeV^-2
/acs/mc/diffvm10/RHOPDIS1.DIS.ISO.A00
/acs/mc/diffvm10/RHOPDIS1.DIS.ISO.S30622.A00 - A05
RHOPDIS1.DIS.ISO.S30622.R60021.A00 - A04 (removed from ACS!) /acs/mc/diffvm10/RHOPDIS1.DIS.ISO.S30622.R60021.CDST.A00
Generated: November 1, 1995 by B.L.
Version 1.06/01
1994 running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: E>8GeV, theta<175deg
Kinematic cuts: Q^2>6.5GeV^2, W>10GeV
W-dependence of the differential cross section: W^0.5
(epsilon_pom = 0.125) for the elastic case,
Slope parameter b is constant
Q^2 dependence: Modified VDM propagator: (1+Q^2/m^2)^-3,
R limited to 3
Known problems:
The W-dependence is a bit too shallow, W^0.8 would be closer
to the truth. The cross section estimate is valid in the region
around W=80GeV.
Recommendation:
reweight events with factor (W/80GeV)^0.3.
30000 events,
cross section estimate 560pb,
integrated luminosity 53.6pb^-1
b=5.5GeV^-2
/acs/mc/diffvm10/RHOELAS2.DIS.A00
/acs/mc/diffvm10/RHOELAS2.DIS.S30627.A00 - A01
RHOELAS2.DIS.S30627.R60107.A00 - A07 (removed from ACS!) /acs/mc/diffvm10/RHOELAS2.DIS.S30627.R60107.DST.A00
Generated: May 11-19, 1995 by B.L.
Version 1.05/01
1994 shifted vertex running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: theta<177deg
Kinematic cuts: Q^2>1GeV^2, W>20GeV
W-dependence of the differential cross section: W^0.8
(epsilon_pom = 0.2) for the elastic case,
W^0.48 (epsilon_pom = 0.12) for the proton dissociation case
Slope parameter b is constant
Q^2 dependence: MODIFIED VDM propagator: (1+Q^2/m^2)^-3,
R=0.2*Q^2/m^2
Remarks:
epsilon_pom was chosen differently for the elastic and proton dissociation
files to partially compensate the t_min effect.
The t_min effect leads for the proton dissociation case to a steeper rise
of the cross section with W than for the elastic case, because the phase
space for proton dissociation grows fast with W.
This is a result of the one-pomeron-exchange approximation, which is known
to lead to a too fast rise of the cross section with W for proton dissocyiation
(compare Tevatron results).
The VDM propagator was modified to give a better description of the Q^2
dependence of the cross section.
Known problems:
None so far
5000 events,
cross section estimate 11.3nb,
integrated luminosity 440nb^-1
b=5.5GeV^-2
/acs/mc/diffvm10/RHOELAS4.SHVTX.A00
/acs/mc/diffvm10/RHOELAS4.SHVTX.S30609.A00
RHOELAS4.SHVTX.S30609.R60017.A00 - A01 (removed from ACS!) /acs/mc/diffvm10/RHOELAS4.SHVTX.S30609.R60017.DST.A00
1000 events,
cross section estimate 1.67nb,
integrated luminosity 600nb^-1
b=5.5GeV^-2
/acs/mc/diffvm10/OMGELAS4.SHVTX.A00
/acs/mc/diffvm10/OMGELAS4.SHVTX.S30609.A00
OMGELAS4.SHVTX.S30609.R60017.A00 (removed from ACS!) /acs/mc/diffvm10/OMGELAS4.SHVTX.S30609.R60017.DST.A00
1500 events,
cross section estimate 2.7nb,
integrated luminosity 560nb^-1
b=4.5GeV^-2
/acs/mc/diffvm10/PHIELAS4.SHVTX.A00
/acs/mc/diffvm10/PHIELAS4.SHVTX.S30609.A00
PHIELAS4.SHVTX.S30609.R60017.A00 (removed from ACS!) /acs/mc/diffvm10/PHIELAS4.SHVTX.S30609.R60017.DST.A00
5000 events,
cross section estimate 5.1nb,
integrated luminosity 990nb^-1
b=3.0GeV^-2
/acs/mc/diffvm10/RHOPDIS4.SHVTX.A00
/acs/mc/diffvm10/RHOPDIS4.SHVTX.S30609.A00 - A01
RHOPDIS4.SHVTX.S30609.R60017.A00 - A02 (removed from ACS!) /acs/mc/diffvm10/RHOPDIS4.SHVTX.S30609.R60017.DST.A00
1000 events,
cross section estimate 1.73nb,
integrated luminosity 1340nb^-1
b=3.0GeV^-2
/acs/mc/diffvm10/OMGPDIS4.SHVTX.A00
/acs/mc/diffvm10/OMGPDIS4.SHVTX.S30609.A00
OMGPDIS4.SHVTX.S30609.R60017.A00 (removed from ACS!) /acs/mc/diffvm10/OMGPDIS4.SHVTX.S30609.R60017.DST.A00
1500 events,
cross section estimate 1.23nb,
integrated luminosity 1220pb^-1
b=2.5GeV^-2
/acs/mc/diffvm10/PHIPDIS4.SHVTX.A00
/acs/mc/diffvm10/PHIPDIS4.SHVTX.S30609.A00
PHIPDIS4.SHVTX.S30609.R60017.A00 (removed from ACS!) /acs/mc/diffvm10/PHIPDIS4.SHVTX.S30609.R60017.DST.A00
Generated: July 22, 1996 by B.L.
Version 1.07/01
1995 running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: E>12GeV, theta<178deg
Kinematic cuts: Q^2>1.0GeV^2, W>20GeV
W-dependence of the differential cross section: W^0.5
(epsilon_pom = 0.125) for the elastic case,
Slope parameter b is constant
Q^2 dependence: Modified VDM propagator: (1+Q^2/m^2)^-2.5,
R limited to 3, grows as 0.33*Q^2/m^2
Known problems:
None so far.
50000 events,
cross section estimate 9800pb,
integrated luminosity 5.1pb^-1
b=6.0GeV^-2
/acs/mc/diffvm10/RHOELAS3.DIS.A00
/acs/mc/diffvm10/95/RHOELAS3.DIS.S30645.A00-A05 (not yet imported...)
/acs/mc/diffvm10/---
50000 events,
cross section estimate 1420pb,
integrated luminosity 35pb^-1
b=4.5GeV^-2
/acs/mc/diffvm10/PHIELAS3.DIS.A00
/acs/mc/diffvm10/95/PHIELAS3.DIS.S30645.A00-A03
/acs/mc/diffvm10/95/PHIELAS3.DIS.S30645.R71700.DST.A00-A01
50000 events,
cross section estimate 9500pb,
integrated luminosity 6.0pb^-1
b=3.0GeV^-2
/acs/mc/diffvm10/RHOPDIS4.DIS.A00
/acs/mc/diffvm10/95/RHOPDIS4.DIS.S30645.A00-A09
/acs/mc/diffvm10/95/RHOPDIS4.DIS.S30645.R71700.DST.A00-A01
50000 events,
cross section estimate 1230pb,
integrated luminosity 40pb^-1
b=2.5GeV^-2
/acs/mc/diffvm10/PHIPDIS3.DIS.A00
/acs/mc/diffvm10/95/PHIPDIS3.DIS.S?????.A??
/acs/mc/diffvm10/95/PHIPDIS3.DIS.S?????.R?????.DST.A??
Generated: January 18-February 5, 1996 by B.L.
Version 1.06/01 (updated)
1995 running conditions, 27.55GeV positrons on 820GeV protons.
Kinematic cuts: W>20GeV
W-dependence of the differential cross section: W^0.3232
(epsilon_pom = 0.0808) for the elastic case
Slope parameter b varies with W, alpha' = 0.25GeV^-2
Q^2 dependence: Modified VDM propagator: (1+Q^2/m^2)^-2.5,
R limited to 3, rises as 0.67 Q^2/m^2 for low Q^2
Files with additional cuts:
particles from decay of vector meson have to be within
4 degree < theta < 176 degree, p_T > 100 MeV (if the decay is to a three
particle final state, then the 2 charged particles have to fulfill the cut).
Known problems:
None so far.
90000 events,
cross section estimate 303nb,
integrated luminosity 297nb^-1
b=10.75 GeV^-2 at W = 55.00 GeV
/acs/mc/diffvm10/OMGELAS6.A00 /acs/mc/diffvm10/OMGELAS6.THCUT.A00
/acs/mc/diffvm10/---
/acs/mc/diffvm10/---
90000 events,
cross section estimate 189nb,
integrated luminosity 477npb^-1
b=6.80 GeV^-2 at W = 13.00 GeV
/acs/mc/diffvm10/PHIELAS7.A00 /acs/mc/diffvm10/PHIELAS7.THCUT.A00
/acs/mc/diffvm10/PHIELAS7.THCUT.S30627.A00-A03
/acs/mc/diffvm10/---
Generated: February 5, 1996 by B.L.
Version 1.06/01 (updated version)
1994 running conditions, 27.55GeV positrons on 820GeV protons.
The rho(1450) decays solely to rho0 pi+ pi-
Cuts on the scattered electron: E>10GeV, theta<175deg
Kinematic cuts: Q^2>4.0GeV^2, W>10GeV
W-dependence of the differential cross section: W^0.5
(epsilon_pom = 0.125) for the elastic case
Slope parameter b varies, alpha' = 0.25
Q^2 dependence: Modified VDM propagator: (1+Q^2/m^2)^-2.5,
R limited to 4, rises as 0.5 Q^2/m^2 for low Q^2
Known problems:
No angular correlations for the pions are included, i.e. the decay products
rho0 pi+ pi- are distributed according to phase space, the subsequent decay
rho -> pi+ pi- (gamma) is isotropic.
20000 events,
No cross section estimate!
b=5.5GeV^-2 at W=80 GeV
/acs/mc/diffvm10/RHO1450.ELAS1.DIS.A00
/acs/mc/diffvm10/---
/acs/mc/diffvm10/---
Generated: April 19, 1996 by B.L.
Version 1.07/00
1995 running conditions, 27.55GeV positrons on 820GeV protons.
The rho(1450) decays to rho0 pi+ pi-
Cuts on the scattered electron: none
Kinematic cuts: W>20GeV
W-dependence of the differential cross section: W^0.32
(epsilon_pom = 0.08)
Slope parameter b varies, alpha' = 0.25
Q^2 dependence: Modified VDM propagator: (1+Q^2/m^2)^-2.5,
Known problems:
None so far.
Status: Simulation & reconstruction requested (19.4.96)
20000 events,
No cross section estimate!
b=10.9GeV^-2 at W=55 GeV
/acs/mc/diffvm10/RHO1450.ELAS.A00
/acs/mc/diffvm10/RHO1450.ELAS.S30639.A00-A01
/acs/mc/diffvm10/95/RHO1450.ELAS.S30639.R71400.DST.A00
Generated: April 19, 1996 by B.L.
Version 1.07/00
1995 running conditions, 27.55GeV positrons on 820GeV protons.
The phi(1680) decays to K K*bar + c.c.
Cuts on the scattered electron: none
Kinematic cuts: W>20GeV
W-dependence of the differential cross section: W^0.32
(epsilon_pom = 0.08)
Slope parameter b varies, alpha' = 0.25
Q^2 dependence: Modified VDM propagator: (1+Q^2/m^2)^-2.5,
Known problems:
None so far.
Status: Simulation & reconstruction requested (19.4.96)
20000 events,
No cross section estimate!
b=6.8GeV^-2 at W=13 GeV
/acs/mc/diffvm10/PHI1680.ELAS.A00
/acs/mc/diffvm10/PHI1680.ELAS.S30639.A00-A01
/acs/mc/diffvm10/PHI1680.ELAS.S30639.R71301.DST.A00
Generated: May 19, 1995 by B.L.
Version 1.05/01
1994 e+ running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: E>5GeV, theta<175deg
Kinematic cuts: Q^2>4GeV^2, W>5GeV
W-dependence of the differential cross section: W^1.0
(epsilon_pom = 0.25)
Slope parameter b is constant
Q^2 dependence: MODIFIED VDM propagator: (1+Q^2/m^2)^-2.5,
R=1.0*Q^2/m^2
Remarks:
The VDM propagator was modified to give a better description of the Q^2
dependence of the cross section.
The files were simulated and reconstructed twice,
with H1SIM 3.06/09 (*.S30609.*) and H1SIM 3.06/14 (*.S30614.*).
This was due to a misunderstanding.
No special problems with either of the two simulations is known to me.
It is recommended to use the later version, though.
Known problems:
None so far.
5000 events,
cross section estimate 25.4pb,
integrated luminosity 197pb^-1
b=2.5GeV^-2
/acs/mc/diffvm10/JPSIELAS.EE.DIS.A00
/acs/mc/diffvm10/JPSIELAS.EE.DIS.S30609.A00 JPSIELAS.EE.DIS.S30614.A00 - A01 (removed from ACS!)
JPSIELAS.EE.DIS.S30609.R60017.A00 - A01 (removed from ACS!) JPSIELAS.EE.DIS.S30614.R60019.A00 - A01 (removed from ACS!) /acs/mc/diffvm10/JPSIELAS.EE.DIS.S30609.R60017.DST.A00
5000 events,
cross section estimate 25.8pb,
integrated luminosity 194pb^-1
b=2.5GeV^-2
/acs/mc/diffvm10/JPSIELAS.MUMU.DIS.A00
/acs/mc/diffvm10/JPSIELAS.MUMU.DIS.S30609.A00 JPSIELAS.MUMU.DIS.S30614.A00 - A01 (removed from ACS!)
JPSIELAS.MUMU.DIS.S30609.R60017.A00 - A01 (removed from ACS!) JPSIELAS.MUMU.DIS.S30609.R60017.A00 - A01 (removed from ACS!) /acs/mc/diffvm10/JPSIELAS.MUMU.DIS.S30609.R60017.DST.A00
5000 events,
cross section estimate 15.9pb,
integrated luminosity 310pb^-1
b=2.5GeV^-2
/acs/mc/diffvm10/JPSIPDIS.EE.DIS.A00
/acs/mc/diffvm10/JPSIPDIS.EE.DIS.S30609.A00 JPSIPDIS.EE.DIS.S30614.A00 - A01 (removed from ACS!)
JPSIPDIS.EE.DIS.S30609.R60017.A00 - A02 (removed from ACS!) JPSIPDIS.EE.DIS.S30614.R60019.A00 - A02 (removed from ACS!) /acs/mc/diffvm10/JPSIPDIS.EE.DIS.S30609.R60017.DST.A00
5000 events,
cross section estimate 15.8pb,
integrated luminosity 320pb^-1
b=2.5GeV^-2
/acs/mc/diffvm10/JPSIPDIS.MUMU.DIS.A00
/acs/mc/diffvm10/JPSIPDIS.MUMU.DIS.S30609.A00 JPSIPDIS.MUMU.DIS.S30614.A00 - A01(removed from ACS!)
JPSIPDIS.MUMU.DIS.S30609.R60017.A00 - A02 (removed from ACS!) JPSIPDIS.MUMU.DIS.S30614.R60019.A00 - A02 (removed from ACS!) /acs/mc/diffvm10/JPSIPDIS.MUMU.DIS.S30609.R60017.DST.A00
Generated: May 22, 1995 (JPSI????2.*), November 17-22 (JPSI????3.*) by B.L.
Version 1.05/01 (JPSI????2.*), 1.06/00 (JPSI????3.*)
1994 e+ running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: none
Kinematic cuts: W>20GeV
W-dependence of the differential cross section: W^0.90
(epsilon_pom = 0.225)
Slope parameter b is constant
Q^2 dependence: MODIFIED VDM propagator: (1+Q^2/m^2)^-2.5,
R=1.0*Q^2/m^2
Remarks:
The VDM propagator was modified to give a better description of the Q^2
dependence of the cross section.
Known problems:
The H1SIM version 3.06/11 contained a collimator in the forward
region which is not as thick as in reality. This might effect the simulated
efficiencies of the forward detectors. To check this, the files were
simulated again with H1SIM 3.06/27, where this problem
has been fixed.
10000 events,
cross section estimate 640pb,
integrated luminosity 15.5pb^-1
b=4.0GeV^-2
/acs/mc/diffvm10/JPSIELAS2.EE.A00 /acs/mc/diffvm10/JPSIELAS3.EE.A00
/acs/mc/diffvm10/JPSIELAS2.EE.S30611.A00 /acs/mc/diffvm10/JPSIELAS3.EE.S30627.A00
JPSIELAS2.EE.S30611.R60017.A00 - A01 (removed from ACS!) /acs/mc/diffvm10/JPSIELAS2.EE.S30611.R60017.DST.A00
10000 events per file,
cross section estimate 660pb,
integrated luminosity 15.3pb^-1 per file
b=4.0GeV^-2
/acs/mc/diffvm10/JPSIELAS2.MUMU.A00 /acs/mc/diffvm10/JPSIELAS3.MUMU.A00
/acs/mc/diffvm10/JPSIELAS2.MUMU.S30611.A00 /acs/mc/diffvm10/JPSIELAS3.MUMU.S30627.A00
JPSIELAS2.MUMU.S30611.R60017.A00 - A01 (removed from ACS!) /acs/mc/diffvm10/JPSIELAS2.MUMU.S30611.R60017.DST.A00 /acs/mc/diffvm10/JPSIELAS3.MUMU.S30627.R60108.DST.A00
10000 events,
cross section estimate 940pb,
integrated luminosity 10.6pb^-1
b=2.0GeV^-2
/acs/mc/diffvm10/JPSIPDIS2.EE.A00 /acs/mc/diffvm10/JPSIPDIS3.EE.A00
/acs/mc/diffvm10/JPSIPDIS2.EE.S30611.A00 - A02 /acs/mc/diffvm10/JPSIPDIS3.EE.S30627.A00 - A01
JPSIPDIS2.EE.S30611.R60017.A00 - A04 (removed from ACS!) /acs/mc/diffvm10/JPSIPDIS2.EE.S30611.R60017.DST.A00 /acs/mc/diffvm10/JPSIPDIS3.EE.S30627.R60108.DST.A00
10000 events per file,
cross section estimate 930pb,
integrated luminosity 10.8pb^-1 per file
b=2.0GeV^-2
/acs/mc/diffvm10/JPSIPDIS2.MUMU.A00 /acs/mc/diffvm10/JPSIPDIS3.MUMU.A00
/acs/mc/diffvm10/JPSIPDIS2.MUMU.S30611.A00 - A02 /acs/mc/diffvm10/JPSIPDIS2.MUMU.S30627.A00 - A02 /acs/mc/diffvm10/JPSIPDIS3.MUMU.S30627.A00 - A02
JPSIPDIS2.MUMU.S30611.R60017.A00 - A04 (removed from ACS!) /acs/mc/diffvm10/JPSIPDIS2.MUMU.S30611.R60017.DST.A00 /acs/mc/diffvm10/JPSIPDIS2.MUMU.S30627.R60108.DST.A00 /acs/mc/diffvm10/JPSIPDIS3.MUMU.S30627.R60108.DST.A00
Modelling of proton dissociation
This file is produced in a special mode of diffVM.
For masses M_X of the dissociating proton system below 2.0GeV the
dissociating proton is treated as N* resonance, as usual.
Above 2.0GeV, however, it is assumed that the proton decays to a nucleon (p or n),
and a number of charged and neutral pions, following the KNO scaling
law (see K. GOULIANOS: Diffractive interactions of hadrons at
high energies. Phys. Rep. 101 (1983) 169-219.).
These particles are then distributed isotropically in phase space,
using the phase space generator RAMBO (R. KLEISS, W.J. STIRLING & S.D. ELLIS:
A new Monte Carlo treatment of multiparticle phase space at high energies.
Comp. Phys. Commun. 40 (1986) 359-373.).
This is an extreme model which is not expected to describe the data,
particularily the p_T spectrum of the pions originating from the
phase space decay is too hard. Therefore results obtained with this
Monte Carlo should only be taken as cross check of the robustness of
the acceptance of forward detectors against extreme dissociation
models.
10000 events,
cross section estimate 940pb,
integrated luminosity 10.6pb^-1
b=2.0GeV^-2
/acs/mc/diffvm10/JPSIPDIS3.ISO.EE.A00
/acs/mc/diffvm10/---
/acs/mc/diffvm10/---
10000 events per file,
cross section estimate 930pb,
integrated luminosity 10.8pb^-1 per file
b=2.0GeV^-2
/acs/mc/diffvm10/JPSIPDIS3.ISO.MUMU.A00
/acs/mc/diffvm10/---
/acs/mc/diffvm10/---
Generated: April 6-9, 1996 by B.L.
Version 1.06/02
1995 e+ running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: none
Kinematic cuts: W>5.04 GeV
W-dependence of the differential cross section: W^0.90
(epsilon_pom = 0.225);
effective rise of the cross section for p-dissociation is W^1.28.
Slope parameter b is constant
Q^2 dependence: MODIFIED VDM propagator: (1+Q^2/m^2)^-2.5,
R=1.0*Q^2/m^2
Remarks:
The VDM propagator was modified to give a better description of the Q^2
dependence of the cross section.
Apart from the removal of the kinematic cut on W and a changed
b-slope for the p-dissociation files, these files were generated the same
way as the files for 1994 running conditions, so that efficiencies are
directly comparable.
The cross section estimates are derived from fits to FTPS, H1, and
(for the elastic case) ZEUS data. The parametrizatiuon used describes
these data (E516, PRL 52:795; ZEUS, DESY 95-052; H1, DESY 96-037) very well,
and the estimated cross section is believed to be accurate within 10%
(elastic case) to 15% (p-dissociation).
Known problems:
None so far.
20000 events,
cross section estimate 816pb,
integrated luminosity 24.5pb^-1
b=4.0GeV^-2
/acs/mc/diffvm10/JPSIELAS4.EE.A00
/acs/mc/diffvm10/JPSIELAS4.EE.S30639.A00-A01
/acs/mc/diffvm10/JPSIELAS4.EE.S30639.R71301.DST.A00
20000 events per file,
cross section estimate 815pb,
integrated luminosity 24.5pb^-1
b=4.0GeV^-2
/acs/mc/diffvm10/JPSIELAS4.MUMU.A00
/acs/mc/diffvm10/JPSIELAS4.MUMU.S30639.A00-A01
/acs/mc/diffvm10/JPSIELAS4.MUMU.S30639.R71301.DST.A00
20000 events,
cross section estimate 800pb,
integrated luminosity 25.1pb^-1
b=1.6GeV^-2
Pomeron intercept for M_X-dependence: 1.0808
(i.e. d^2 sigma / [d t d M_X^2] = 1/M_X^2[1.0808] )
/acs/mc/diffvm10/JPSIPDIS4.EE.A00
/acs/mc/diffvm10/JPSIPDIS4.EE.S30639.A00-A03
/acs/mc/diffvm10/---
20000 events per file,
cross section estimate 790pb,
integrated luminosity 25.4pb^-1
b=1.6GeV^-2
/acs/mc/diffvm10/JPSIPDIS4.MUMU.A00
/acs/mc/diffvm10/---
/acs/mc/diffvm10/JPSIPDIS4.MUMU.S30641.R71301.DST.A00 /acs/mc/diffvm10/JPSIPDIS4.MUMU.S30642.R71400.DST.A00
Generated: April 5, 1995 by B.L.
Version 1.04/00
Status: Simulation and reconstruction of the electron files not requested at the moment.
1994 e+ running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: none
Kinematic cuts: W>15GeV
W-dependence of the differential cross section: W^1.0
(epsilon_pom = 0.25)
Slope parameter b varies, alpha'_pom = 0.25GeV^-1
Q^2 dependence: standard VDM propagator,
R=1.0*Q^2/m^2
Remarks:
The Q^2-dependence may be a bit too flat
(i.e. too many events at high Q^2).
Known problems:
Extended GKI bank does not contain helicity information of the photon
(words IHELI, FTRANS, EPSIL)
The pipi mass spectrum in the decay psi'->J/psi pi+ pi- does not
correspond to the one which was measured in e+e- experiments.
The distribution of the three particles is simply accordng to phase space.
Cascade decays via chi states are not included.
10000 events,
cross section estimate 69pb,
integrated luminosity 145pb^-1
b=3.5GeV^-2 at W=14GeV
/acs/mc/diffvm10/PSI2ELAS.EE.A00
10000 events,
cross section estimate 69pb,
integrated luminosity 146pb^-1
b=3.5GeV^-2 at W=14GeV
/acs/mc/diffvm10/PSI2ELAS.MUMU.A00
/acs/mc/diffvm10/PSI2ELAS.MUMU.S30614.A00 - A03
PSI2ELAS.MUMU.S30614.R60019.A00 - A02 (removed from ACS!) /acs/mc/diffvm10/PSI2ELAS.MUMU.S30614.R60108.DST.A00
10000 events,
cross section estimate 102pb,
integrated luminosity 98pb^-1
b=2.50GeV^-2 at W=14.00 GeV and M_x=3.00 GeV
/acs/mc/diffvm10/PSI2PDIS.EE.A00
10000 events,
cross section estimate 108pb,
integrated luminosity 93pb^-1
b=2.50GeV^-2 at W=14.00 GeV and M_x=3.00 GeV
/acs/mc/diffvm10/PSI2PDIS.MUMU.A00
/acs/mc/diffvm10/PSI2PDIS.MUMU.S30614.A00 - A03
PSI2PDIS.MUMU.S30614.R60019.A00 - A04 (removed from ACS!) PSI2PDIS.MUMU.S30614.R60105.DST.A01 - A03 (removed from ACS!) /acs/mc/diffvm10/PSI2PDIS.MUMU.S30614.R60108.DST.A00
Generated: April 4 (mumu)/May 29 (ee), 1996 by B.L.
Version 1.06/02 (mumu), 1.07/00 (ee)
Status: files with decay to mu+mu- are finished for 94 and 95 running conditions, files with decay to e+e- have been simulated at RAL, but are not yet on ACS. (13.6.96)
1994 e+ running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: none
Kinematic cuts: none
W-dependence of the differential cross section: W^0.9
(epsilon_pom = 0.225),
effective rise for p-dissociation files is faster
Slope parameter b constant, alpha'_pom = 0GeV^-2
Q^2 dependence: MODIFIED VDM propagator: (1+Q^2/m^2)^-2.5,
R=1.0*Q^2/m^2
Remarks:
The cross section estimate is derived from the J/psi measurements, assuming
a ratio of 1:0.2 for J/psi:psi' (as measured), and is believed to be
accurate within 20%.
The pomeron intercept is assumed to be the same as for J/psi production,
as are the b slopes.
Known problems:
The pipi mass spectrum in the decay psi'->J/psi pi+ pi- does not
correspond to the one which was measured in e+e- experiments.
The distribution of the three particles is simply accordng to phase space.
Cascade decays via chi states are not included for the mumu files.
20000 events,
cross section estimate 110pb,
integrated luminosity 170pb^-1
b=4.0GeV^-2
acs/mc/diffvm10/PSI2ELAS4.MUMU.A00
/acs/mc/diffvm10/PSI2ELAS4.MUMU.S30627.A00-A01 (1994 detector)/acs/mc/diffvm10/PSI2ELAS4.MUMU.S30639.A00-A01 (1995 detector)
/acs/mc/diffvm10/PSI2ELAS4.MUMU.S30627.R60108.DST.A00 (1994 detector)/acs/mc/diffvm10/PSI2ELAS4.MUMU.S30639.R71400.DST.A00 (1995 detector)
20000 events,
cross section estimate 120pb,
integrated luminosity 170pb^-1
b=4.0GeV^-2
Pomeron intercept for M_X-dependence: 1.0808
(i.e. d^2 sigma / [d t d M_X^2] = 1/M_X^2[1.0808] )
/acs/mc/diffvm10/PSI2ELAS4.EE.A00
20000 events,
cross section estimate 110pb,
integrated luminosity 180pb^-1
b=1.6GeV^-2
Pomeron intercept for M_X-dependence: 1.0808
(i.e. d^2 sigma / [d t d M_X^2] = 1/M_X^2[1.0808] )
/acs/mc/diffvm10/PSI2PDIS4.MUMU.A00
/acs/mc/diffvm10/PSI2PDIS4.MUMU.S30627.A00-A04 (1994 detector)/acs/mc/diffvm10/PSI2PDIS4.MUMU.S30639.A00-A04 (1995 detector)
/acs/mc/diffvm10/PSI2PDIS4.MUMU.S30627.R60108.DST.A00 (1994 detector)/acs/mc/diffvm10/PSI2PDIS4.MUMU.S30639.R71400.DST.A00 (1995 detector)
20000 events,
cross section estimate 110pb,
integrated luminosity 180pb^-1
b=2.0GeV^-2
Pomeron intercept for M_X-dependence: 1.0808
(i.e. d^2 sigma / [d t d M_X^2] = 1/M_X^2[1.0808] )
/acs/mc/diffvm10/PSI2PDIS4.EE.A00
Generated: May 24, 1995 by B.L.
Version 1.05/01
1994 e+ running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: none
Cuts on the decay leptons: both leptons 4deg < theta < 175 deg
Kinematic cuts: W>11.4GeV
W-dependence of the differential cross section: W^0.90
(epsilon_pom = 0.225)
Slope parameter b constant
Q^2 dependence: MODIFIED VDM propagator: (1+Q^2/m^2)^-2.5,
R=1.0*Q^2/m^2
Remarks: Cross section may be off by a factor of 10 or more!
Known problems:
None so far.
2500 events,
cross section estimate 0.3pb,
integrated luminosity 9000pb^-1
b=4.0GeV^-2
/acs/mc/diffvm10/UPSILONEL.EE.A00
/acs/mc/diffvm10/UPSILONEL.EE.S30614.A00
UPSILONEL.EE.S30614.R60019.A00 (removed from ACS!) /acs/mc/diffvm10/UPSILONEL.EE.S30614.R60108.DST.A00
2500 events,
cross section estimate 0.3pb,
integrated luminosity 9600pb^-1
b=4.0GeV^-2
/acs/mc/diffvm10/UPSILONEL.MUMU.A00
/acs/mc/diffvm10/UPSILONEL.MUMU.S30614.A00
UPSILONEL.MUMU.S30614.R60019.A00 (removed from ACS!) /acs/mc/diffvm10/UPSILONEL.MUMU.S30614.R60108.DST.A00
2500 events,
cross section estimate 0.3pb,
integrated luminosity 8100pb^-1
b=4.0GeV^-2
/acs/mc/diffvm10/UPSILONPD.EE.A00
/acs/mc/diffvm10/UPSILONPD.EE.S30614.A00
UPSILONPD.EE.S30614.R60019.A00 (removed from ACS!) /acs/mc/diffvm10/UPSILONPD.EE.S30614.R60108.DST.A00
2500 events,
cross section estimate 0.3pb,
integrated luminosity 8300pb^-1
b=4.0GeV^-2
/acs/mc/diffvm10/UPSILONPD.MUMU.A00
/acs/mc/diffvm10/UPSILONPD.MUMU.S30614.A00
UPSILONPD.MUMU.S30614.R60019.A00 (removed from ACS!) /acs/mc/diffvm10/UPSILONPD.MUMU.S30614.R60108.DST.A00
Generated: November 1, 1995 by B.L.
Version 1.06/01
1994 running conditions, 27.55GeV positrons on 820GeV protons.
Cuts on the scattered electron: E>8GeV, theta<175deg
Kinematic cuts: Q^2>6.5GeV^2, W>10GeV
W-dependence of the differential cross section: W^0.5
(epsilon_pom = 0.125),
Slope parameter b is constant
Q^2 dependence: Modified VDM propagator: (1+Q^2/m^2)^-3, m=0.77GeV,
R limited to 3
Remarks:
This is really a toy model for photon dissociation, where a mass
M_X is chosen at the photon-pomeron-vertex according to a 1/M_X distribution,
and the mass is assumed to decay to a q-qbar pair collinear with
the photon's flight direction. The q-qbar pair is then linked with
a Lund string and fragmented with JETSET.
The cross section estimate should not be taken too seriously.
10000 events,
cross section estimate 550pb,
integrated luminosity 19.0pb^-1
b=2.5GeV^-2
/acs/mc/diffvm10/RHODISS2.DIS.A00
/acs/mc/diffvm10/RHODISS2.DIS.S30627.A00 - A01
RHODISS2.DIS.S30627.R60107.A00 - A03 (removed from ACS!) /acs/mc/diffvm10/RHODISS2.DIS.S30627.R60107.DST.A00