physics i+computing
DESCRIPTION
Physics I+Computing. John Huth. Transition from cosmic rays to collider physics. Cosmic ray reconstructed in both the muon spectrometer and inner detector. Use expertise in muon spectrometer to investigate early physics: W/Z production Z pt, distributions Lay groundwork for - PowerPoint PPT PresentationTRANSCRIPT
Physics I+Computing
John Huth
21-Aug-09 John Huth DOE Site Visit 2
Transition from cosmic rays to collider physics
Cosmic ray reconstructed in both themuon spectrometer and inner detectorUse expertise in
muon spectrometer toinvestigate early physics:
W/Z productionZ pt, distributions
Lay groundwork for higher energy+lum.discovery physics
21-Aug-09 John Huth DOE Site Visit 3
21-Aug-09 John Huth DOE Site Visit 4
Z’s in early data (Kashif, Black, Huth)
Calibration of spectrometer, inner detectorEarly physics –
Pt distribution helps understand PDF’sσ*Br*eff=150 pb at 7 TeV
Inv. Mass distribution withbckg. sim. from bbar
Pt distribution, withunfolding
21-Aug-09 John Huth DOE Site Visit 5
W-/W+ Ratio (Martinez, Belloni, Guimaraes)
Sensitive to PDF’sMain backgrounds:
W→τνTopZ →μμ
Can be done with low energy + modest Lum.→Extension of cosmic ray asym
→Can be done with a few days at 1029
21-Aug-09 John Huth DOE Site Visit 6
W-/W+ Ratio in Rapidity
21-Aug-09 John Huth DOE Site Visit 7
Z+jets (Kagan, Black, Huth, Moed)
QCD testsSensitive to new physics (technicolor, Higgs)Calibration of jet energy scales (from recoil system)
Predictions for Z+N jetcross sections for varying CM energies
At low luminosities,examine energy flowIn recoil system
Gain experience in jet systematics
21-Aug-09 John Huth DOE Site Visit 8
Δφ Z-Jet (Kagan, Black, Huth, Moed)
Z
Jet
Δφ
TeVs 10
21-Aug-09 John Huth DOE Site Visit 9
Back-to-back deviation from QCDradiation effects
Relatively insensitiveto jet energy scales= early measurement
Derive hadronicenergy scale
10TeV@100 pb-1
Δφ Z-Jet (Kagan, Black, Huth, Moed)
21-Aug-09 John Huth DOE Site Visit 10
Investigation of associated Higgs production (Kagan, Black, Huth,
+Gallichio, Schwartz)
From Butterworth et al arXiv:0810.0409v1 :
ZH final state had longbeen neglected at LHC
Backgrounds dominate
Recent studies have revived interest in thismode
Jet recombinationBoosted Higgs
21-Aug-09 John Huth DOE Site Visit 11
bckg
Higgs
Fuller treatment
Studies by Butterworth etal. had neglected b-quarkshowering and decay
New variables found show s/b rejection
21-Aug-09 John Huth DOE Site Visit 12
ΔR
Heavy flavor in VB Production (Martinez, Guimaraes)
B-jet merging in W/Z+bbar
Matrix element generation ofWbbar required to get fullkinematic distribution
21-Aug-09 John Huth DOE Site Visit 13
B-jet corrections (Moed)
Improving resolution of b-bar dijets→ Correct for energy loss andneutrinos in semi-leptonic decaysElectrons more difficult (insidejets)
21-Aug-09 John Huth DOE Site Visit 14
Technirho decays into Z+γ(Black)
Cleaner signature thanZ+2 jets, smaller branching fraction – viable with a few fb-1of data
Red=background from contiuumBlue=signal
TeVs 10 15 fb
21-Aug-09 John Huth DOE Site Visit 15
Involvement in analysis groups
• Early work in muon combined performance working group– Capitalize on experience with cosmic ray analysis– Reconstruction efficiency
• Work with SM Z/W (+jets) groups– Z pt distribution, cross section– Introduction of MadGraph to ATLAS– W+/W- asymmetry
• Top group (see also MF’s talk next)– b quark energy corrections– Jet merging– Heavy flavor studies
• Lepton+X convenor (K. Black)• Luminosity group (L. Kashif)• US ATLAS Analysis Forum Chair (K. Black)
21-Aug-09 John Huth DOE Site Visit 16
Physics I Summary
• Early physics – concentrate on SM measurements– Z cross section (Kashif)– W+/W- ratio (Martinez)– Z+jets (Kagan)
• Preparation for higher energy/luminosity– Understand b-jet response, jet merging
21-Aug-09 John Huth DOE Site Visit 17
Computing
• Relevant sites:– CERN
• Tier 0 – work on reconstruction• LxPlus – main development site• Local cluster shared with U. Michigan in Bldg. 188
– BNL• Tier 1 site, development, main data repository for US
– Harvard• Tier 2 – Odyssey cluster major engine for US ATLAS Production• Tier 3 – Odyssey cluster – main data repositories for Harvard
group
21-Aug-09 John Huth DOE Site Visit 18
MITHarvard
Networking in Boston
Harvard
BU
-> NYC -> BNL -> CERN
NoX metro ring: 128 fibers(only a few fibers are in use)
300 Bent St.
1 Summer St.
21-Aug-09 John Huth DOE Site Visit 19
Northeast Tier 2 Center
700 cores, 2.1 MSpecInt2K500 TB SANCisco 6509 + 10 Gbps dedicated fiber to NoXATLAS DEDICATED
6568 cores, 21.0 MSpecInt2K750 TB SAN2 x Cisco 6509 + 10 Gbps dedicated fiber to NoXLustre parallel file system + NFSShared access to FAS FACILITY
BU:
Harvard:500-700 dedicated
cores for ATLAS prod.
21-Aug-09 John Huth DOE Site Visit 20
ATLAS Computing@Harvard
1 FTE sys. admin from Harvard supports T2/T3
300-500 cores availablefor individual analyses
Disk space had been main bottleneck – usageapprox. 20 TB
30 TB donated from M.Seltzer(SEAS)
Production jobs on HU_T2
21-Aug-09 John Huth DOE Site Visit 21
79635 simulation12191 pile-up 5680 validation 3573 event generation 1546 merge 1420 reconstruction 941 test 4 digitization
Odyssey
Tier 1
20.1 Terabytes
9.1 Terabytes
104,990 successful PANDA jobs
500 cores 2.33 Ghz Intel Harpertown
NET2 storage500T GPFSBoston University
ATLAS work done on the Harvard Odyssey cluster Apr-15-2009 through Jul-15-2009
28,000 cpu-days delivered