atlas week feb 2000 j. huston michigan state university understanding higgs production and...
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ATLAS week Feb 2000J. Huston
J. Huston
Michigan State University
Understanding Higgs Production and Backgrounds at the LHC Using Tevatron Data
For more details on Higgs production studies see:
•Proceedings of the Les Houches workshop on Physics at TeV Colliders, currently at http://www.pa.msu.edu/~huston/leshouches/
•C. Balazs, J. Huston, I. Puljak, Higgs Production: A Comparison of Monte Carlo and Resummation, hep-ph/0002032
Work on Higgs production withC. Balazs and I. Puljak; work on Higgs backgrounds withS. Murgia and B. Blair
ATLAS week Feb 2000J. Huston
Modelling the effects of initial state gluon radiation
(see also C. Balazs, J. Huston, I. Puljak, hep-ph/0002032
+ Workshop on Physics at TeV Colliders; http://www.pa.msu.edu/~huston/leshouches/)
J. Huston
Michigan State University
ATLAS week Feb 2000J. Huston
Reducible background for inclusive H->Comparison with Tevatron data
J. Huston
Michigan State University
Work done with Simona Murgiaand Bob Blair
ATLAS week Feb 2000J. Huston
Higgs-> and Backgrounds One of the most useful search modes for
the discovery of the Higgs in the 100-150 GeV mass range at the LHC is in the two photon mode
Unless the Higgs boson is non-standard, with an enhanced coupling to the two photon mode, there is no discovery potential at the Tevatron for a decay into two photons
Nonetheless searches are going on at the Tevatron in the Run 1 data (Simona Murgia thesis, Michigan State U. 2000; D0 paper) and will continue until the LHC turns on
Even if no discovery takes place, these exercises will be useful experience for the LHC, especially in understanding the backgrounds to Higgs searches, both and o and oo
S. Mrenna and J. Wells, hep-ph/0001226
enhanced2 BR
ATLAS week Feb 2000J. Huston
Diphoton Production at the Tevatron
QCD diphoton production is an interesting process in its own right new physics can show up in the two photon channel (extra dimensions,
SUSY, …) the final state kT can be measured very precisely; thus diphoton production is
a great place to test resummation formalisms
The backgrounds to diphoton production come from o and oo production
both backgrounds are much larger than the signal, unless an isolation cut is made
an isolation cut discriminates greatly against jets fragmenting into leading o’s at CDF (in Run 1B), require that additional energy in a cone of radius 0.4
about photon direction is < 1 GeV saturated by minimum bias energy
no explicit isolation cut in ATLAS, but an implicit one
ATLAS week Feb 2000J. Huston
Photon Measurements
The photon fraction of a sample can be determined on a statistical basis using CES and CPR weights
look for photon conversions in CPR (probability is greater for o)
look at shower width in CES (wider for o)
ATLAS week Feb 2000J. Huston
Photon Fractions for Single Photon Production
Photon fraction from Run 1A agrees roughly with leading order prediction
Photon fraction from Run 1B consistent with 1Abut may be flattening out(?)
fragmentation z values > 0.99
CDF Preliminary
ATLAS week Feb 2000J. Huston
Diphoton Fractions Background subtraction more
complicated for diphoton case both photons can fail CES/CPR test, both
can pass, or one can pass and one fail; end up with 4X4 matrix to invert with
output number of , go, o, oo pairs
•As expected diphoton events are more isolated than background
•consistent with min bias energy
CDF Preliminary
ATLAS week Feb 2000J. Huston
Diphoton Fractions as Function of Isolation
For these studies, a diphoton ntuple was used in which the leading photon was required to have > 22 GeV; no requirement on the 2nd photon
Trigger level isolation energy cuts kick in at about 4 GeV in a cone of radius 0.4; examine photon, background fractions up to that point
Diphoton fraction decreases as isolation cut energy is raised
oo is dominant background;is this reasonable?
/o ratio is < 1in this range; but might have expected closer ratio
o fraction seems to increase with increasing isolation
o is poorly determined at very low isolation (can end up with fit preferring a negative fraction)
black triangles: oo open circles: o
open triangles:
ATLAS week Feb 2000J. Huston
Number of Signal and Background Events
Look at signal fraction compared to background fraction as function of isolation
Increasing isolation energy increases number of events almost linearly, but little effect on signal
ATLAS week Feb 2000J. Huston
Diphoton Backgrounds in ATLAS Again, for a H-> search at the
LHC, face irreducible backgrounds
from QCD and reducible
backgrounds from o and oo
in range from 70 to 170 GeV
jet-jet cross section is estimated
to be a factor of 2E6 times the cross section and -jet a factor
of 8E2 larger Need rejection factors of 2E7 and
8E3 respectively PYTHIA results seem to indicate
that reducible backgrounds are
comfortably less than reducible
ones …but how to normalize PYTHIA
predictions for very high z fragmentation of jets; fragmentation not known well at high z and certainly not for gluon jets
ATLAS week Feb 2000J. Huston
/o ratio at the LHC Use same leading order program as was used
at the Tevatron to look at the /o ratio as a function of the isolation cut
Inclusive /o ratio is extremely small but the imposition of a reasonable isolation cut brings the ratio to the order of 1 or larger in the range of interest
expect /o to be of same order as oo
Picking out the tail of the isolation energy distribution
• /o as a function of isolation energy;uses a collinear approximation to fragmentation•no explicit isolation cut in ATLAS; would be veryinteresting to study effective isolation cut
inclusive
<1 GeV
<2 GeV<3 GeV
<5 GeV
isolation energy for o’s with ET>25 GeV
ATLAS week Feb 2000J. Huston
Study in Progress
Generate -jet, events in PYTHIA, pass them through CDF fast detector simulation program QFL, and trigger/reconstruct as data
qqbar-> ISUB=18 gg-> ISUB=114 qqbar->g ISUB=14 qg->q ISUB-29 gg->g ISUB=115
Compare PYTHIA predictions for background/signal to what is observed in CDF
Job started in Oct ‘99; 18.5 million events so far (~15.7 pb-1)
Just doing -o background for now given large number of events needed (and we haven’t tried to be clever)
o
in the data o is equalto at an isolation cut of 3 GeV
ATLAS week Feb 2000J. Huston
Pythia Study
only o backgrounds being considered
ATLAS week Feb 2000J. Huston
Isolation Energy in Pythia
ATLAS week Feb 2000J. Huston
Isolation Energy in Pythia
ATLAS week Feb 2000J. Huston
Isolation in Data and PythiaPythia Data
ATLAS week Feb 2000J. Huston
Isolation in Data and PythiaPythia Data
ATLAS week Feb 2000J. Huston
Isolation in Data and Pythia
Pythia Data
ATLAS week Feb 2000J. Huston
Comparison of o Isolation Energy Distributions from Pythia and Data
Data o-oPythia -o
ATLAS week Feb 2000J. Huston
QCD/EW at the Tevatron
The Tevatron Collider serves as arena for precision tests of QCD and EW with photons,electrons, W/Z’s, jets
Highest Q2 scales currently achievable (searches for new physics at small distance scales)
Sensitivity to parton distributions over wide kinematic range
2 scale problems: test effects of soft gluon resummation
Diffractive production of W/Z, jets, heavy flavor
Data compared to NLO, resummed, leading log Monte Carlo, fixed order calculations
Overall, the data from CDF and D0 agree well with NLO QCD
Some puzzles resolved: W + jet(s): R10
Some puzzles remain: Jet excess at high ET/mass??
Gluon/d quark distribution at large x?
630 GeV jet cross section and xT scaling
Some theory work needs to be done: Inclusive photon cross section
Some searches still continue: BFKL effects (D0 looks forET
decorrelation in dijet events as rapidity separation of jets increases)
No effects not “observed in Herwig”
ATLAS week Feb 2000J. Huston
Theoretical Predictions
There are a variety of programs available for comparison of data to theory and/or predictions. Tree level Leading log Monte Carlo
NnLO
Resummed
Important to know strengths/weaknesses of each.
In general, agree quite well…but before you appeal to new physics, check theME.
Perhaps biggest effort…include NLO MEcorrections in Monte Carlo programs…correct normalizations.
Resummed description describes soft gluoneffects (better than MC’s)…has correct normalization (but need HO to get it); resummed predictions include non-perturbative effects correctly…may have to be put in by hand in MC’sthreshold kT
W,Z, Higgsdijet, direct
b space
qt space
ATLAS week Feb 2000J. Huston
Theoretical Predictions
Determination of the Higgs signal requires an understanding of the Higgs pT distribution
for example, for gg->HX->X, the shape of the signal pT distribution is harder than that of the background; this can be used to advantage
To reliably predict the Higgs pT distribution, especially for low to medium pT region, have to include effects of soft gluon radiation
can either use parton showering a la Herwig, Pythia, ISAJET or kT resummation a la ResBos
parton showering resums primarily the (universal) leading logs while an analytic kT resummation can resum all logs with Q2/pT
2 in their arguments; but expect predictions to be similar and Monte Carlos offer a more useful format
Where possible it’s best to compare pT predictions to a similar data set to insure correctness of formalism; if data is not available, compare MC’s to a resummed calculation
Note the large difference between PYTHIA versions5.7 and 6.1
ATLAS week Feb 2000J. Huston
Change in PYTHIA Older version of PYTHIA has more events at
moderate pT
Two changes from 5.7 to 6.1 A cut has been placed on the combination of z
and Q2 values in a branching: u=Q2-s(1-z)<0 where s refers to the subsystem of hard scattering plus shower partons
corner of emissions that do not respect this requirement occurs when Q2 value of space-like emitting parton is little changed and z value of branching is close to unity
necessary if matrix element corrections are to be made to process
net result is substantial reduction in amount of gluon radiation
In principle affects all processes; in practice only gg initial states
Parameter for minimum gluon energy emitted in space-like showers is modified by extra factor corresponding to 1/ factor for boost to hard subprocess frame
result is increase in gluon radiation
The above are choices, not bugs; which version is more correct?
->Compare to ResBos
S. Mrenna80 GeV Higgs generated at the Tevatron with Pythia
ATLAS week Feb 2000J. Huston
Diphoton production at the Tevatron and LHC
gg
resummation at 14 TeV
gg scattering is an important process for diphoton production at both the Tevatronand the LHC. May be able to constrain resummation formalism for gg processes.
ATLAS week Feb 2000J. Huston
Comparison of CDF Z pT to Resbos and Pythia
Use high statistics precision Z data at the Tevatron to compare PYTHIA and ResBos predictions
from Willis Sakumoto
Note agreement with data
and Pythia at high pT due to
matrix element matching
ATLAS week Feb 2000J. Huston
Low pT region and kT
A blowup of the low pT region shows that an additional “intrinsic” kT (of about 2 GeV) is needed for agreement with
data and ResBos; implemented by a
Gaussian smearing at the start of
the parton shower ResBos needs no additional kT
The 2 GeV needed by PYTHIA
does not mean that the intrinsic
kT inside of a proton is 2 GeV,
just that this amount is needed
to compensate for the cutoff
imposed in the parton shower;
this amount of non-
perturbative kT is automatically
generated by ResBos given the
non-perturbative parameters
determined by fits to fixed target data
(and the evolution to Tevatron
kinematics)
ATLAS week Feb 2000J. Huston
Need gg initial state
Z production primarily from qqbar initial state; would like to have to similar gg process to test resummation/Monte Carlo formalism
A little less than half of Tevatron diphoton cross section (with a pT cut of 12 GeV) is due to gg scattering
ATLAS week Feb 2000J. Huston
Compare PYTHIA and ResBos diphoton predictions
ResBos is larger than PYTHIA at high pT for qqbar scattering
ResBos switches to the appropriate Y piece (exact matrix element) at high pT; Monte Carlo matrix element matching not yet available for Higgs production
ResBos agrees with PYTHIA for gg initial state, even though ResBos has exact ME at high pT and PYTHIA does not
this shows the smallness of the Y piece for gg->g
ATLAS week Feb 2000J. Huston
Compare two versions of PYTHIA
pT distributions look similar between the two versions for both subprocesses
ATLAS week Feb 2000J. Huston
Comparison to CDF data
Diphoton statistics limited from Run 1 but in good agreement with resummed predictions from ResBos
kT distribution in disagreement with NLO predictions, indicating need for soft gluon resummation
More precise comparisons, out to higher pT, will be possible the >20 times the statistics in Run 2
ATLAS week Feb 2000J. Huston
Diphoton Production at the LHC…again, a large fraction of continuum diphoton production from gg scattering
…better agreement for gg subprocess than for qqbar for the same reasons as the Tevatron
ATLAS week Feb 2000J. Huston
Comparison of two versions of PYTHIA
Starting to see more differences for gg initial state due to larger phase space for gluon emission at the Tevatron
ATLAS week Feb 2000J. Huston
Comparison of PYTHIA and ResBos for Higgs Production at LHC
ResBos agrees much better with the more recent version of PYTHIA
Suppression of gluon radiation leading to a decrease in the average pT of the produced Higgs
Affects the ability of CMS to choose to the correct vertex to associate with the diphoton pair
Note that PYTHIA does not describe the high pT end well unless Qmax
2 is set to s (14 TeV)
Again, ResBos has the correct matrix element matching at high pT; setting Qmax
2=s allows enough additional gluon radiation to mimic the matrix element
ATLAS week Feb 2000J. Huston
Similar behavior at the Tevatron Differences between the two
versions are smaller, though (again less phase space for gluon radiation)
ATLAS week Feb 2000J. Huston
Comparisons with Herwig
HERWIG (v5.6) similar in shape in PYTHIA 6.1 (and perhaps even more similar in shape to ResBos)
Is there something similar to the uhat cut that regulates the HERWIG behavior?
ATLAS week Feb 2000J. Huston
“Intrinsic kT” for Higgs Production
How much intrinsic kT to use with PYTHIA for Higgs production at the LHC?
Amount of intrinsic or primordial kT chosen does not matter for Higgs production at LHC since most of kT is “radiated away” before hard collision
Note that peak is above 10 GeVcompared to 3 GeV for the Z atthe Tevatron; larger color factorfor gg state and more phase spacefor gluon emission
ATLAS week Feb 2000J. Huston
Intrinsic kT at the Tevatron
Similar effect (but smaller) for Higgs production at the Tevatron
ATLAS week Feb 2000J. Huston
Z Production at the LHC
Sensitivity to kT still present for Z production
ATLAS week Feb 2000J. Huston
Diphoton Measurements at CDF
2 aspects:•QCD measurements of •exotic searches with diphotons,e.g. Higgs->: looser cuts to maximizeefficiency
Require:•ET
1,2 > 12 GeV/c•Isolation energy in cone of 0.4 < 1 GeV/c
saturated by MB energy forN.B. backgrounds come from jets withzo (=Eo/Ejet) > Eo/(Eo+1)
•zmin~0.95 for ET=20 GeV/c
•fragmentation functions not welldetermined here, especially notwith gluons and especially notin Monte Carlos
Note that distributions that are functionsat LO are not well-described at NLO
->need resummed predictions
ATLAS week Feb 2000J. Huston
Jet Production and the Gluon Distribution
@LO, jet cross section is proportional to s
2g(x,Q)g(x’,Q) and s2g(x,Q)q(x’,Q)
•flexibility in gluon allows for increase intheoretical cross section at high ET
Note that if jet cross section increases by 20%, gluon distribution must double (fraction of gluon jets also almost doubles)
ATLAS week Feb 2000J. Huston
Conclusions
Preliminary conclusion: PYTHIA overestimates backgrounds in CDF->will be investigated in more detail
ATLAS note will be written
New version of PYTHIA in relatively good agreement with both HERWIG and ResBos for predictions of Higgs pT distribution at the LHC
Don’t rely totally on Monte Carlos and certainly not on one Monte Carlo alone
Verify, if possible, theoretical predictions/formalisms with data exisiting Run 1 data/Run 2 data “background” data to be taken at the LHC
If no data, then verify with more complete theoretical treatments