toward the unknown: first physics from atlas
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Toward the Unknown: First Physics from Atlas. Outline. Introduction Why the LHC? Atlas Experiment Won’t discuss CMS, LHCB, … 1 st results Summary. Thanks to my Atlas colleagues…. Introduction. The Standard Model (SM) provides an excellent description of experiments and is predictive . - PowerPoint PPT PresentationTRANSCRIPT
Toward the Unknown: First Physics from Atlas
J. Hobbs, SBU Colloquium 2
Outline
• Introduction• Why the LHC?• Atlas Experiment
– Won’t discuss CMS, LHCB, …• 1st results• Summary
Oct. 5, 2010
Thanks to my Atlas colleagues….
J. Hobbs, SBU Colloquium 3
IntroductionThe Standard Model (SM) provides an
excellent description of experiments and is predictive
Oct. 5, 2010|c| contributions to fits assuming SM
a prio
ri “SM
”
predic
tions
J. Hobbs, SBU Colloquium 4
But there are still issues…• Some pieces of SM to work on
– Electroweak symmetry breaking unproven
– Precision flavor studies– Stability: fine tuning issues?
• SM doesn’t answer some big questions– Fermion mass spectrum?– Dark matter?– Matter/antimatter asymmetry?
Including D0 results described 2 weeks ago– Ultimately EW + strong unification
Oct. 5, 2010
J. Hobbs, SBU Colloquium 5
EW Symmetry Breaking• Simplest form of (Local) gauge
invariance requires massless force carriers– Photon (and gluon), m=0. OK…– MW = 80 and MZ = 91 GeV
• SM and the Higgs mechanism– Permits non-zero boson mass & gauge
invariance together– Requires a Higgs boson (thus “the Higgs
search”)
Oct. 5, 2010
Is this correct? We don’t know…
J. Hobbs, SBU Colloquium 6
EWSB: Current state
Oct. 5, 2010
Indirect constraints on Higgs from SM consistency…
… mW and mt precision are current limiting factors
J. Hobbs, SBU Colloquium 7
Fine Tuning / Dark Matter• SM has far too little dark matter (n’s).• Fine tuning: SM values must be within a
part in 1032 for stability. May be unnerving?Supersymmetry (e.g,) is a possible solution to both:
Includes a dark matter candidate. Removes fine-tuning by cancellation and leads to mH < 135 GeV? Predicts new particles whose multiplicity is determined by SM particle content
But no direct experimental evidence, only bounds if it exists M > 100 – 300 GeV Is it right?
Oct. 5, 2010
J. Hobbs, SBU Colloquium 8
LHC Motivation• Tests of posited solutions to SM
shortcomings have led to lower mass bounds for new physics, but no direct observation– The space of new physics possibilities is
large. Won’t discuss specifics further…• How to proceed?
– Indirect tests (ala Higgs constraints and CP violation of 2 weeks ago and others)
– Direct searches for higher mass.
Oct. 5, 2010
High mass means higher energy, thus the LHC
Large Hadron Collider (LHC)• In general, rate for
reaction X is – NX = sX* L
• LHC: pp collider design– Ecm = 14 TeV (7x FNAL)– L = 1034/cm2/s (30x FNAL)– Beam
Stored energy 360 MJ (!)
Current 0.58 AOct. 5, 2010 J. Hobbs, SBU Colloquium 9
Most significant increase in Ecm since 1981 (ISR -> SppS)
acceleratornature, ECM
J. Hobbs, SBU Colloquium 10
Jet rate vs. jet ET
Tevatron
This is background! unknown
LHC
Oct. 5, 2010
Other processes, s(LHC)/s(TeV) W ttbar gg(400 GeV) Z’(1 TeV) 10x 100x 20000x 300x (but mass dependent)
~~
Large Hadron ColliderRate vs. Ecm
Z
H (500)H (150)
Jet E T>100
b quark
t quark
Jet ET > ECM/4
J. Hobbs, SBU Colloquium 11
LHC: Is 14 TeV enough?• For WW scattering to remain bounded
– Requires *something* with M<1 TeV• MH (including SUSY)…
– In SM *something* = Higgs, so MH<O(1 TeV)
– In “SUSY”, MH < 135 GeV, and more particles
• Alternatives must leave WW OK.
Oct. 5, 2010
Encouraging… (some say “guaranteed”)
J. Hobbs, SBU Colloquium 12
LHC: What’s the situation now?• Restart in Sept. 2009 after year delay for
magnet connection induced problems• ECM = 7 TeV.
– A safety factor for magnet connections– (Also lower energies during start up)
• Beyond ECM, performing very well– Already at design protons/bunch– Long beam lifetimes, good emittance– Stored energy, 5 MJ – 10 MJ (FNAL, 2 MJ)
Oct. 5, 2010
J. Hobbs, SBU Colloquium 13
LHC Performance
Oct. 5, 2010
For past two weeks, injecting more bunches While writing this talk, the record instantaneous luminosity increased 4x with possibly another >2x coming this month…
Bunch trainscommissioned !!
4/pb/day: 400,000 W/day 400 top pairs/day
J. Hobbs, SBU Colloquium 14
Atlas Experiment• Higher energies means more particles
and particles with more energy. – Drives experimental design: energy
containment, particle density
Oct. 5, 2010
“jet”
Charged particle trajectories EM energy
Hadronic energy
m
Beam perp to screen
g
e
p
n
J. Hobbs, SBU Colloquium 15
Atlas Experiment
Oct. 5, 2010
O(107) read out channels operating efficiency 98%
J. Hobbs, SBU Colloquium 16Oct. 5, 2010
Dijet Event: MJJ = 2.55 TeV ET
J1 = 420 GeV ET
J2 = 320 GeV
(plus others…)
J. Hobbs, SBU Colloquium 17Oct. 5, 2010
J. Hobbs, SBU Colloquium 18Oct. 5, 2010
J. Hobbs, SBU Colloquium 1920% of the Atlas collaborators
Can you find Caputo, McCarthy or Hobbs?
Atlas Experimeters
Oct. 5, 2010
SBU Atlas @ SBUSBU Atlas @ CERN + a few missing
J. Hobbs, SBU Colloquium 20
1st Science• Can we see the things we expect?
– Reconstruct charged particles– p0, hadronic jets, J/y– W*, Z bosons– Top quark?– Aggregations: multiplicities, W+jets*
• Or the unexpected? Early (proto)searches– q* high rate, low S/B– W’ lower rate, excellent S/B– Early SUSY*, LQ*
Oct. 5, 2010
Every measurement at the LHC is new territory…
*SBU involved
J. Hobbs, SBU Colloquium 21
Low Masses: p0->gg
Oct. 5, 2010
Azimuthal angle
Pseudorapidity, h (polar angle) Diphoton mass
Mass vs. h
Are the material and calorimeter understood for the inner “1/2” of the detector?
OK at O(1%)…
ECM = 900 GeV
J. Hobbs, SBU Colloquium 22
Dijet Production
Oct. 5, 2010
High-rate process
Differential cross section (pT) for |y| < 2.8
Measures shape, but not absolute rate.
NLOJET++ 4.1.2, CTEQ6.6
J. Hobbs, SBU Colloquium 23Oct. 5, 2010
Low Masses: J/y -> mm
Somewhat different samples and selections
Do we understand the material in the outer detector?
J. Hobbs, SBU Colloquium 24
High Mass: Z and W Bosons
Oct. 5, 2010
Reconstruct Z->ll (l=e,m), This is a critical standard candle. But low rate…
Low mass resonances indicated OK understanding of material, but here resolution mismatch indicates better stats for (probably) alignment and channel-to-channel calibration
J. Hobbs, SBU Colloquium 25
W->ln
Oct. 5, 2010
Loose Selection
Final Selection primarily adds MET requirement
Tests understanding of hadronic calib
SBU involvement…
MT= √2pTlpT
v(1-cosdf)
J. Hobbs, SBU Colloquium 26
W Cross Section
Oct. 5, 2010
W cross section
Why is W+ different than W-
J. Hobbs, SBU Colloquium 27
Correlations: W and Z with jets
• Intrinsically interesting because– Hard to calculate rates with precision.– Dominant background to many new
physics scenariosOct. 5, 2010
SBU works on this
More gluons give more jets. (Each gluon is one more factor of as)
J. Hobbs, SBU Colloquium 28
W+Jets
Oct. 5, 2010
Jet multiplicity distribution
jet pT distribution
Stony Brook group working on this topic. Cross sections in internal review now…
J. Hobbs, SBU Colloquium 29
Top Quarks? Well, maybeExpect a few top pairs in summer data
sample
Oct. 5, 2010
Analyses ready, and and a few events…
J. Hobbs, SBU Colloquium 30
Charged particle multiplicities in pp Collisions at ECM = 900 GeV (Phys Lett B 68, Issue 1, 21-42)And updated for 7 TeV data
1st Physics Publications
Oct. 5, 2010
Early bread & butter science which requires low Linst
J. Hobbs, SBU Colloquium 31
Excited quark search• Highest rate visible process is pp ->
jet+jet. Can be enhanced by direct production of new
particles or indirect effects (high mass states)
Oct. 5, 2010
Signal e.g. excited quarks,Excluded over region
0.3 TeV < mq* < 1.26 TeV
(Prev. excl. mq*<0.76 TeV)
Accepted by Phys. Rev. Lett.
Jul. 23 (preliminary)
J. Hobbs, SBU Colloquium 32
But it’s already been updated…
Oct. 5, 2010 Preliminary, 9/26
Signal e.g. excited quarks,Excluded over region
0.5 TeV < mq* < 1.53 TeV
Sep. 26
J. Hobbs, SBU Colloquium 33
Near Term: W’ search
Oct. 5, 2010
Heavy vector bosons (W’, Z’) features of many new physics models
Clean channel, but yield falls quickly as a function of mass
Existing FNAL bounds roughly 1 TeV, so wait < 1 yr.
J. Hobbs, SBU Colloquium 34
And down the road, e.g. SUSY
Oct. 5, 2010
Start with a basic selection and then specific requirements. Early days…
J. Hobbs, SBU Colloquium 35
Future• Continue running at 7 TeV until end 2011
– Accumulate 1 fb-1 data (increase 100x)– Already significant room for discovery
Not Higgs, though…• LHC shutdown for 1 yr. Finish magnet
fixes, maybe modest Atlas changes• After restart, move to 14 TeV• Longer term
– Atlas upgrades (2 stages at least)– LHC luminosity growth to design
Oct. 5, 2010
J. Hobbs, SBU Colloquium 36
• After a long wait, the LHC/Atlas program is really underway– LHC & experiments working well– Established 1st signals and initial
calibrations– Early search results already new mass
range
• Will explore significant new territory with the current data. What’s there? – Dark Matter? EWSB explained? It really
is unknown territory Oct. 5, 2010
Summary
J. Hobbs, SBU Colloquium 37
Where to?
Oct. 5, 2010
J. Hobbs, SBU Colloquium 38Oct. 5, 2010
(Simulated) H->ZZ->eejj(Simulated )SUSY event
J. Hobbs, SBU Colloquium 39
BACKUP
Oct. 5, 2010
J. Hobbs, SBU Colloquium 40
Gauge Unification
Oct. 5, 201040
g3
g1
g2
g3
g1
g2SM SUSY
The SM couplings do not intersect at one point.
SUSY does…
J. Hobbs, SBU Colloquium 41
Composition of the Universe
Oct. 5, 2010
(0.4% stars)
J. Hobbs, SBU Colloquium 42Oct. 5, 2010
J. Hobbs, SBU Colloquium 43
Atlas good beam efficiency
Oct. 5, 2010
J. Hobbs, SBU Colloquium 44Oct. 5, 2010
Z cross section
J. Hobbs, SBU Colloquium 45Oct. 5, 2010
Trigger rates crossing at 40 MHz -> L1 then at 10 kHz -> L2 then at 1 kHz -> HLT (10 GB/s) then at 100 Hz -> tape (1 GB/s)
In a year at 50% duty cycle: 15 PB
J. Hobbs, SBU Colloquium 46
Magnet Problem
Oct. 5, 2010
During ramp tests, a solder joint in the cold region failed with 1 V at 9 kA. 1. current ramp (10 A/s) auto stopped 2. relief circuit automatically turned on to dump magnet current ==> All functioned correctly to this pt 3. An arc developed causing failure of He (1.9K) containment 4. He boiled catastrophically causing high pressure…
J. Hobbs, SBU Colloquium 47Oct. 5, 2010