Conference Summary ICHEP 2004, Beijing John Ellis CERN.
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Transcript of Conference Summary ICHEP 2004, Beijing John Ellis CERN.
Conference Summary
ICHEP 2004, BeijingJohn Ellis
CERN
The Basis of Particle Physics
String theory
Cosmology
Future accelerators
Barbieri
@ HERA
Klein
CrucialFor LHC
QCD Works!
@ Tevatron
b production
Lucchesi
World Summary of αS(MZ) – July 2004
world average (MSbar, NNLO)
αS(MZ) = 0.1182 0.0027
cf. (2002) 0.1183 0.0027
Bethke , hep-ex/0407021
Stirling
NNLO pQCDCalculations
Parton splitting functions
W, Z cross sections
+ 7 pages! Moch, Vermaseren & Vogt
jetson
way
Stirling
QCD Calculations in String Approach
• Maximal helicity-violating (MHV) amplitudes as effective vertices in a new scalar graph approach
• use them with scalar propagators to calculate
– tree-level non-MHV amplitudes
– with both quarks and gluons
– … and loop diagrams!
• dramatic simplification: compact output in terms of familiar spinor products
• phenomenology? multijet cross sections at LHC, etc. underway
Cachazo, Svrcek & Witten
Stirling
QCD phase diagram
Hadron gas
Dunlop
Particle Production Ratios
Well described by simple thermodynamic model, T ~ lattice …
… but could these just be phase space and statistics?
Dunlop
Elliptic Flow: the Shape of the Interaction Region at RHIC
Anisotropic Flow
x
yz
Peripheral Collisions
Reproduced well by hydrodynamic model
Shape parameter v2
but hydrodynamic model failsto reproduce HBT source size
Dunlop
Hadron Elliptic Flows Scale with Quark Number
)3/p( v3 ~)p( vand )2/p( v2 ~)p( vpions,Except T2,qTB2,T2,qTM2,
Dunlop
Jet Quenching @ RHIC …
… due to parton energy loss in QGP?
Dunlop
The State of Heavy-Ion Theory
• A patchwork, with model parameters adjusted independently for different observables.
• Statistical equilibriation or phase space?• Hydrodynamical model: EOS vs realistic quark-gluon
calculations?• Source size as measured by HBT?• Parton energy loss: promising development!• Watch out for J/ψ suppression!• For compelling QGP claim, need quantitative
estimates of theoretical uncertainties
Dunlop
Questions on Hadron Spectroscopy
• Do (which) pentaquarks exist?• Do other exotic hadrons exist?• What are the quark descriptions of the
DsJ(2317) and DsJ(2460)?• Does the DsJ(2632) exist (SELEX)?• What is the quark description of the X(3872)?• Interpretation of threshold reported states?• Fate of 12% rule in ψ’ decay (BES)?
Some Sightings of the Θ+(1530) …
… but many negative searches
Jin
Summary of Positive Results
(LEPS)
nK
Inconsistencies in Mθ and Γθ?
0SpK
Also width of θ+(1540)
- Two “positive” experiments:
HERMES: Γθ = 17 9 2 MeV
ZEUS: Γθ = 8 4 MeV
K+N PWA indicates Γθ < 1 MeV
Jin
M(nK+)≠ M(pKs)?
Summary of Negative Results
How Significant are Negative Results?
• Compare with production of other baryons resonances
• Λ(1520) may not be most reliable guide
• Most positive results at lower energies
• Different production mechanisms for exotic baryons?
Jin
Interpretations of θ+(1530) – if it exists
• Naïve non-relativistic quark model would need epicycles:
di/triquarks, P-wave ground state• Predicted in chiral soliton model:
fits data, predicts other exotic states• Existence requires confirmation:
a high-statistics, -significance experiment• If it exists, θ+ spin & parity distinguish models
The stakes are high: the θ+(Ξ , θc) may take us beyond the naïve quark model
← Based on idea thatquarks weigh << ΛQCD
Close
X(3872 ): Charmonium or D0D*0 “Molecular State”?
’J/
X(3872) 10σeffect
Belle, also CDF, D0
MeV
MeVM
3.2
5.06.00.3872at 90% C.L.
No D0D0 → unnatural spin-parity
Jin
M()
BK X(3872)
Belle
Also reported in ωJ/ψ:mixed isospin would
→ mixing with D0D*0 molecule Close
M=1859 MeV/c2
< 30 MeV/c2 (90% CL)
J/pp
M(pp)-2mp (GeV)
0 0.1 0.2 0.3
3-body phase space acceptance
2/dof=56/56
acceptance weighted BW +3 +5
10 25
BES IIalso pΛ,pΛc, KΛ,
ππ,πΚ
Hadronic Threshold States
Quark description inadequate: need hadronic description? molecules, …?
Jin
Electroweak Physics
APV, E158compatible
with expectedrunning of α(Q2)
NuTeV:EW corrections - 1σ?
Strange sea - 1σ?ubar ≠ dbar - 1σ?
(NOMAD)
Teubert
Low Energy vs High Energy
Top-Quark Mass: Run 1 Revisited
D0: improved Run 1 value
) GeV 5.1 174.3 m (previous t
t tM M 2.4 %
t
m 178.0 2.7(stat) 3.3
New world average (Run 1 on
(syst) GeV
178.0 4.3 GeV
ly):
new
Implications for fit to Higgs mass …
Denisov
FutureTevatronProspects
The Blue Band PlotGlobal electroweak fit – high Q2 data
Since Aachen EPS Summer 2003:
new top mass increases mH
by ~20 GeV
new 2-loop terms etc. increase mH by ~6 GeV
t
S Z
+ 69H - 4
2
5
H
m = 178.2 3.9 GeV
(M ) = 0.1186 0.0027
m = 114
= 15.8/13 df (prob = 2
GeV
m < 260 GeV (
6
95 )
%)
% cl
(5)had Z Hfor (M ) = 0.02749 0.00012 m 129 GeV
2W H
from uncertainties of 2 (& leading 3)
loops for M & sin (main ef
'bl
fec
ueb
t f
and'
or m )eff
new
Teubert
BES et al
Pulls on Global Fit
Direct search limit
Higgs mass from individual measurements
How Good is the Global Electroweak Fit?
Heavy flavours ≠ leptons, mW
Teubert
Denisov, Barr //
fb-1
1 year @1033
1 month @1033
1 year @1034
LHC: ATLAS
Values for single experiment
h → requiresexcellent low-pT lepton + tau jet trigger
tim
e
Looking for Standard-Model Higgs
Flavour Physics: Some Questions
• Are the data on quark mixing described by the CKM model?
• Are there signatures of physics beyond the SM?
• If not, why is new physics flavour-blind?• Why is neutrino mixing so different from
quark mixing?• Can they be related?
Sakai, Ali, Giorgi, Ligeti, Patera, Shipsey, Langacker, McGrew, Wang
New Determinations of Vus
CKM unitarity ‘crisis’ has disappeared
Vu
s x f
+(0
)
•PDG02
Patera
Global CKM FitSakai,Ali,
Giorgi,Ligeti
Matrix elements from lattice: Hashimoto
φK0 has moved towards SM
η’ Ks at 2.6 from sin2[cc]
<s-penguins> at 3.5 from sin2[cc]
BUT: expect corrections to sin2[cc] for many modes
Compare sin2 & s-Penguin Results
Sakai,Ali,
Giorgi,Ligeti
Measuring α with B→ ππ, ρπ and ρρ Decays
Excellent agreement with global CKM fit
100
+ 12- 10
CP Violation in B0 → K+ π-
Discrepancy withACP(K+π0 ) = 0.04 0.05 0.02 ?Electroweak penguins? NP? Final-state interactions?
First evidence for direct CPV in B decays
Sakai,Ali,
Giorgi,Ligeti
Putting all the Information Together
Is there room for NP?
Sakai, Ali, Giorgi, Ligeti
Still Room for Future ProgressLigeti
Rare KDecays
KL→0e+e-
KL→0+-
KS→0e+e-
KS→0+-
KL→0
Im t = A23
)0,1()0,0(
),(
The connection of the KL0e+e-() decays to t
needs work on ancillary modes
More handles on triangle
Results & prospectsfor K+ → π+νν
Bounds & prospectsfor KL
→ π0νν
KS → π0l +l-, π0γγimportant forKL → π0l +l-
Patera
Neutrino Masses & Oscillations• First confirmed physics beyond SM• LSND? Waiting for MiniBooNE• (Near) bimaximal mixing ≠ quarks:
Is there a relation: θν+θc = π/4? Reactors for θ13? • Dirac or Majorana masses: seesaw?
Normal or inverted hierarchy? ββ0ν?
• Holy Grail: CP violation via phase δ?Indirect relation to cosmology via
baryogenesis?
• Search for violation of charged lepton numbers
Langacker
L/E Significance
The dips in the data cannot be explained by other models
Δχ2 (neutrino decay – oscillation) =11.4 3.4 σ
Δχ2 (neutrino decoherence – osc’n)
=14.6 3.8 σ
Evidence for Neutrino Oscillation Patternfrom Super-Kamiokande & KamLAND
Oscillation
Decay
Decoherence
Wang
KamLAND
SK/SNO
sin2 is determined by SK/SNO
KamLAND consistent with SK/SNO
Wang
K2K confirms Super-Kamiokande
K2K Rate suppression and
spectral distortion …
… agree with SK azimuthal distributionsand
L/E analysis
McGrew, Wang
Physics beyond the SM
• The most pressing issue is breaking EW symmetry
• Must be solved below 1 TeV energy• Would be a revolution in fundamental physics• Basis for any further theoretical speculations• Hints of grand unification: gauge couplings,
neutrino masses, but wait and see• String unification is still the dream
Barbieri
Breaking Electroweak Symmetry• Calculability principle:
EW scale should be calculable in terms of other mass scale
• No quadratic divergences: supersymmetry ?
or Higgs as pseudo-Goldstone boson ?
• Supersymmetry: also gauge unification and dark matter
• LEP data: some fine-tuning needed
Barbieri
Alternatives to Supersymmetry
• Interpretation of EW data?consistency of measurements? Discard some?
• Higgs + higher-dimensional operators?corridors to higher Higgs masses?
• Little Higgs modelsextra `Top’, gauge bosons, `Higgses’
• Higgsless modelsstrong WW scattering, extra D?
Barbieri
Little Higgs Models
• Embed SM in larger gauge group• Higgs as pseudo-Goldstone boson• Cancel top loop
with new heavy T quark
• New gauge bosons, Higgses• Higgs light, other new
physics heavyNot as complete as susy: more physics > 10 TeV
MT < 2 TeV (mh / 200 GeV)2
MW’ < 6 TeV (mh / 200 GeV)2
MH++ < 10 TeV
zoomzoom
gμ - 2: e+e- Data vs τ Data
KLOE agrees with CMD-2: discard τ dataWhy the 10%
τ - e+e- discrepancy above ρ peak?
Largest contributions, errors from low energies
Teubert
Updated Results for gμ - 2(693.4 ± 5.3 ± 3.5) 10 –10=
(11 659 182.8 ± 6.3had ± 3.5LBL ± 0.3QED+EW) 10 –10=a SM
[e+e– ]
ahad [e+e– ]
Weak contribution : aweak = + (15.4 ± 0.3) 10 –10
Hadronic contribution from higher order : ahad [( /)3] = – (10.0 ± 0.6) 10 –10
Hadronic contribution from LBL scattering: ahad [LBL] = + (12.0 ± 3.5) 10 –10
2.7 standard deviations
=(25.2 ± 9.2) 10 –10a
exp – a SM
not yet published
not yet published
preliminary
BNL E821 (2004):aexp = (11 659 208.0 5.8) 1010
Teubert
Squark & Gluino Searches @ FNAL
GeneralSquarks
& gluinos
Specificsearch
for lightsbottom
Heinemann
Sparticle mass measurements @ LHC
• Mass measurements from exclusive cascade decays
• Mass differences well measured– Typically limited by
detector performance• Of order 1%
• Error in overall mass scale– Unknown missing energy
• Of order 10%
ATLASSquark – neutralino1mass difference5 fb-1
q
qR
~
qR
~q
p p
Barr //
l+
l- parton-level
-> Measure spin-1/2 nature of neutralino-2-> Also can measure scalar nature of slepton-> Success at several distinct points in parameter space
detector-level
Lepton+jet invariant massC
har
ge a
sym
met
ry
spin-0
Eve
nts
Measuring Sparticle Spin @ LHC
0* 1*
ATLAS
ATLAS
Barr //
NLO QCD Calculations Needed for Extracting BSM signals
Stirling
Road Map for EWSB Physics
Barbieri
A Few Remarks on String Theory
• A very powerful tool, e.g., for QCD• Already solved many problems in Q. Gravity• Is it relevant to particle physics?• Can string theory explain the origin of the
Universe?• Could it replace inflation by a scalar field?• What is the landscape of string vacua?• Distinctive experimental signature: extra D?
Liu
Stirling
Particle Astrophysics and Cosmology
• What is the Dark Matter?• Is there Dark Energy?• Are there Ultra-High-Energy Cosmic
Rays beyond the GZK cutoff?• Was there inflation?• How did the Universe begin?
Binetruy
Composition of the Cosmos
WIMPs
WMAP best fit
Binetruy
Concordance Cosmological Model
WMAP+SN+HST
WMAP, Supernovae,Large-scale structures …
Barbiellini //, Ghirlanda et al
… and gamma-ray bursters?
Candidates for Cold Dark Matter
• Axion?• Lightest Supersymmetric Particle (LSP)?
neutralino? gravitino?accelerators vs non-accelerator expts?
• Lightest Kaluza-Klein Particle (LKP)?in models with universal extra
dimensions• Superheavy (metastable) Particle?
‘WIMPzilla’ produced at inflation?decays responsible for UHECRs??
Direct Search for Dark Matter
- Look for elastic scatteringon nuclei in low-backgroundexperiment
- DAMA modulation signaldifficult to reconcile withother experiments, such asCDMS2
- Good prospects forimprovement by factor ~ 20
- Starting to reach regionexpected in models
Binetruy
~2 degrees around the galactic center
EGRET data
Annihilation channel W+W-
Mχ =80.3 GeV
background model(Galprop)WIMP annihilation (DarkSusy)Total
Contribution
Gamma Rays from Neutralino Annihilations?
- Uncertainties incosmic-ray bkgrd- Also in signalnormalization
Morselli, Sander //
Neutralino Annihilations inside Sun?
Look forχχ→ν→μ
Future
Present
Questions on Future Accelerators
• What do we want?• How can we involve a diversity of regions?• How can we ensure diversity of facilities?• Can we work together to get them approved?• Can we build them?• Can we do experiments with them?• Will they answer all our questions?• How can we ensure access to them? Lüth
Brau
Yokoya
Dorfan
Miller
Barbieri
Motivations for Future Colliders
• Physics AND cosmology make us expect strong new signals at the scale of 1 TeV
• Physics case for LHC has been made and accepted:
It will look into the whole region where new physics should be
• Physics case for the TeV ILC has been made.• Physics cases for CLIC (and Larger HC?) will
follow results from LHC (and TeV ILC)
Miller
Tasks for the TeV ILC
• Measure mt to < 100 MeV
• If there is a light Higgs of any kind, pin it down:
Does it have standard model couplings? What is its precise mass?
• If there are extra light particles: Measure mass and
properties
• If LHC sees nothing new below ~ 500 GeV:
Look for indirect signatures
Miller
Examples of Possible Indirect Physics
- (e+e- f f )(direct)
ILC
Sensitivities to a Z’ Parameters of a WLWL Resonance
Imposing a1=1 (SM coupling) get blue bar from LHC, red from ILC.
LHC fit,100fb-1
LC 1 TeV 1 ab-1
Miller
The ITRP Recommendation• We recommend that the linear collider be based on superconducting rf
technology (from Exec. Summary)
– This recommendation is made with the understanding that we are recommending a technology, not a design. We expect the final design to be developed by a team drawn from the combined warm and cold linear collider communities, taking full advantage of the experience and expertise of both (from the Executive Summary).
– We submit the Executive Summary today to ILCSC & ICFA
– Details of the assessment will be presented in the body of the ITRP report to be published around mid September
– The superconducting technology has features that tipped the balance in its favor. They follow in part from the low rf frequency.
Dorfan
Beyond the TeV ILC
• We need 2 LCs:The TeV ILC, asap, then a multi- (~3?) TeV CLIC
The CLIC two-beam accelerator concept The third CLIC test facility
Plan to demonstrate R1, R2 BY 2009: Δt ~ 5y relative to ILCYokoya
Miller
Sparticles may not be very light
FullModel
samples
Detectable@ LHC
ProvideDark Matter
Dark MatterDetectable
Directly
Lightest visible sparticle →
← S
econd lightest visible sparticle
JE, Olive, Santoso, Spanos
Summary of the Summary
• QCD ever more quantitative• Electroweak theory suggests new physics @ TeV
scale: Higgs + ?• Flavour physics becoming quantitative• CKM looking better and better• Neutrinos really do oscillate!• Growing symbiosis with cosmology• LHC on its way• Good ideas for future accelerators• ITRP has done its work
Lets get back to our work!