Diffraction, Dark Energy, and Higgs Bosons
K. GoulianosThe Rockefeller University
Seminar @ NESTOR Institute, PYLOS, GREECE, 20 Aug 07
QCD , Strings,
or OTHER?
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 2
ContentsIntroductionDiffractionDark EnergyHiggs Bosons
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 3
INTRODUCTION
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 4
The big bang
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Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 5
Blow-hole at Grand Cayman
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 6
Black Hole Eats Star!
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 7
What is Dark Energy?
* * ** * *
H He
E
M
* * ** * *
H He
E
M
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 8
Elementary Particles
Aristotle
450 BC
earthwaterairfire
atom
Demokritos
1869
periodictable
Mendeleyev
1897
electronThomson
1910
nucleusRutherford
1962
quarksGell-Mann
α-particlesSource
Rutherford Experiment
Large angle scattering atoms have nuclei
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 9
SU3: Law and Order in the Particle Zoo
Σ+
(1193)
n
Σ−
p
Ξ- Ξ0(1318)
Σο,ΛοΣ− Σο Σ+
(1384)
Ξ0(1533)Ξ-
Ω-
Δ+ Δ++Δ-Δo
1210
211 ++−−
3
2
1
0
−
−
−
Strangeness: SIsotopic spin:I3=Q-(B+S)/2
uud ddu
uus
QED – Quantum Electro-Dynamics
μ = 1.00115965219 ± 0.00000000003
μ = 1.00115965219 ± 0.00000000001
α
α
γe
e
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 11
Mγ, g = 0 MW, Z~100 Mp Mtop~Mgold
The Standard Model
Higgs field generates Mass !
Glashow, Salam, and Weinberg
Unification of forcesαs
αs
gq
q
STRONG ~ 1
α
α
γe
eELECTROMAGNETIC ~ 10-2 WEAK ~ 10-14
d
e-
W-
u
νe
charged current
νe+n -> p+e-
d
νZo
d
ν
neutral current
νe+p -> νe +p
αW
αW
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 13
Leon Lederman & the SM
A good theory shouldfit on a T-shirt!
( )
( )conjugatehermitian RLGRLG
V2
B2YW
21
RB2YR
LB2YW
21L
BB41WW
41
21 ++−
−⎥⎦
⎥⎢⎣
⎢⎟⎠⎞
⎜⎝⎛ ′−.−∂+
⎟⎠⎞
⎜⎝⎛ ′−∂+
⎟⎠⎞
⎜⎝⎛ ′−.−∂+
−−=
c
ggi
gi
ggi
L
φφ
φφτ
γ
τγ
μμμ
μμμ
μμμμ
μνμν
μνμν
But what aboutinteractions?
AND WHAT ABOUTGRAVITY?
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 14
String Theory, then?Particles correspond to the vibration modes of a string in 10 dimensions
Gravity is included!
Pythagoras applied it to music
in 400 BC:1+2+3+4=10
http://www.aboutscotland.com/harmony/prop.html
It surely makes an interesting T-shirt!
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 15
DIFFRACTION
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 16
p-p InteractionsDiffractive:Colorless exchange withvacuum quantum numbers
Non-diffractive:Color-exchange
Incident hadrons retain their quantum numbersremaining colorless
Incident hadrons acquire colorand break apart P
OMERON
rapidity gap
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 17
Elastic Scattering
DIFFRACTION PATTERN
PROTON BEAM
TARGETPROTON
PROTON-PROTON ELASTIC SCATTERING
p p' dtdσ
2
π
)(p4
R
cGeV13b
m1R
e~bte~dtdσ 2
2
−
−
⎟⎠⎞
⎜⎝⎛≈⇒=
θ
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 18
Diffraction DissociationRT
RL
M
P0
P0
Δ PT Δ PL,
m p
sM
PΔPξ
2
L
L ==
025.02
2
−=tdMdt
d σ
Momentum loss fraction
COHERENCE CONDITION 1.0
mm
p
≈< πξξ< 0.1
d
?M1~
dMdσWhy 22
Tevatron M 0.6 TeVLHC 4.4 TeV
KG, Phys. Rep. 101, 169 (1983)
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 19
Diffraction Kinematics
ξp
MX
η
dN/dηξ,t
pMX
p p’
p’rapgap
Δη=-lnξ
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 20
Rapidity Gaps and QCD
ξ1~
dξdσ
M
1~dM
dσconstantΔηddσ
220t
⇒⇒≈⎟⎟⎠
⎞⎜⎜⎝
⎛
=
p pX p
ξp
Particle production Rapidity gap
η
φ
-ln ξln MX2
ln s
X
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 21
PHENOMENOLOGY
Aristotle
450 BC
earthwaterairfire
atom
Demokritos
1869
periodictable
MendeleyevPlato (427-347 B.C)
platoniclove
2007
?
candidatessuperimposed
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 22
Diffraction at CDF
η
φ
Elastic scattering Total cross section
SD DD DPE SDD=SD+DD
σT=Im fel (t=0)
OPTICALTHEOREM
η
φGAP
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 23
CDF Run 1 (1992-1995)
DIPOLE MAGNETS
ROMAN POTS at 57 m
p- CDF
Scintillator fiber xy-tracker 270 pitch, 2 m lever armx<0.97
x=1
μ
Acceptance: 0 < |t| < 1, 0.03< < 0.1ξ
Run-IC Run-IA,B
HADRON
END PLUG EM
CENTRAL EMCES
EM
Forward(Not-To-Scale)
CPR
CENTRAL MUON
CENTRAL MUON UPGRADE
STEEL ABSORBER
η = 0
Silicon Vertex Detector
Central Muon Extension
Z
Vertex Tracking Chamber
CHAMBERTRAKCING
INTERACTION POINT
DetectorCDF
η = 4.2
η = 2.4
η = 0.9
PLUG
ENDHADRONCENTRAL
BBC
WALL
CENTRAL
SOLENOID
HADRON
END
HADRON
Forward DetectorsBBC 3.2<η<5.9FCAL 2.4<η<4.2
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 24
CDF forward detectorsROMAN POT DETECTORS
BEAM SHOWER COUNTERS:Used to reject ND events
MINIPLUG CALORIMETER
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Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 25
The MiniPlugs @ CDF
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 26
MiniPlug Construction
About 1500 wavelength shifting fibers of 1 mm dia. are ‘strung’ through holesdrilled in 36x¼” lead plates sandwiched between reflective Al sheets and guided
into bunches to be viewed individually by multi-channel photomultipliers.
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 27
SOFT DIFFRACTION
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 28
Diffraction and Unitarity
Unitarity problem:Using factorization and std pomeron fluxσSD exceeds σT at
Renormalization:Normalize Pomeron flux to unity to eliminate overlapping gaps
)(sσξ)(t,fdtdξσd
pIPIP/pSD
2
ξ−⋅=
KG, PLB 358 (1995) 379
TeV.2s ≈
1dtdξξ)(t,f0.1
ξIP/p
0
tmin
=∫ ∫−∞=
εσ
2~ sSD
εs
εs
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 29
A Scaling Law in Diffraction
14 GeV (0.01 < ξ < 0.03)
20 GeV (0.01 < ξ < 0.03)
546 GeV (0.005 < ξ < 0.03)
1800 GeV (0.003 < ξ < 0.03)
1____
(M2)1+Δ.....
←_____ 546 GeV std.flux prediction
← 1800 GeV std.flux prediction
Δ = 0.05 ________→
Δ = 0.15 _________→
renorm. fluxprediction
_________→
std. and renorm.flux fits
|↑
KG&JM, PRD 59 (1999) 114017
ε≡Δ
Factorization breaks down so as to ensure M2-scaling!
ε
εσ+∝ 12
2
2 )(Ms
dMd
renormalization
1
Independent of S over 6 orders of magnitude in M2 !
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 30
The QCD Connection
(see E. Levin, An Introduction to Pomerons,Preprint DESY 98-120)
εε σσσ ses oy
oT == ′Δ)(y
φ sy ln=′Δ
Emission spacing controlled by α-strongσΤ : power law rise with energy
∼1/αs
α’ reflects the size of the emitted cluster, which is controlled by 1 /αs and thereby is related to ε
( ) ytel etsf Δ′+∝ αε),(Im
yφ sy ln=Δ
Forward elastic scattering amplitude
assume linear t-dependence
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 31
Gap probability MUST be normalized to unity!
Single Diffraction in QCD
y′ΔyΔ
yt Δ,2 independent variables:
t
colorfactor 17.0
)0()(
≈=−−
−−
ppIP
IPIPIP tgβ
κ
( ){ } { }yo
ytp eetFC
yddtd ′ΔΔ′+ ⋅⋅⋅⋅=
Δεαε σκσ 22
2
)(gap probability sub-energy x-section
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 32
Multigap Diffraction
1y′Δ 2y′Δ1yΔ 2yΔ
1y′ 2y
(KG, hep-ph/0205141)
φ
y
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 33
Multigap Cross Sections
ssty ln/2~,ε
Δ∫Same suppressionas for single gap!
( ){ } ( ){ }2122
2-1i1
2
51
5
)( yyo
ytp
ii
eetFCdV
dii ′Δ+′Δ
=
Δ′+
−=
××= ∏∏εαε σκσ
Gap probability Sub-energy cross section(for regions with particles)
1y ′Δ 2y ′Δ1yΔ 2yΔ
1y ′ 2y
1t 21 yyy Δ+Δ=Δ5 independent variables2t color
factor
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 34
p
p
IP
IPp p
η0ηp_ ηp
p
pIP
M1
M2
η
dNdη
ηη maxmin
ln M1 ln M22 2
ln s
ηη maxminp
0η
ln M1 ln M22 2
ln1/ξp ln s’ln s
p p
IP tpM1
IP tp
M2
Double Diffraction Dissociation
One central gap
Double Pomeron Exchange
Two forward gaps
SDD: Single+Double Diffraction
One forward gap+ one central gap
Central and Multigap Diffraction
Rate for second diffractive gap is not suppressed!
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 35
Central and Two-Gap Results
1
10
10 2
10 102
103
√s (GeV)
σ DD (m
b) fo
r Δη
> 3.
0
ReggeRenormalized gap
CDFUA5 (adjusted)
10-1
1
103
sub-energy √s--, (GeV)
gap
fract
ion
Δη >
3.0 CDF: one-gap/no-gap
CDF: two-gap/one-gapRegge predictionRenorm-gap prediction
2-gap
1-gap
210
0
0.1
0.2
0.3
0.4
0.5
103
√s⎯
(GeV)Fr
actio
n of
Eve
nts
with
ξp
< 0.
02
CDF Data: DPE/SD ratio (Preliminary)
Regge + Factorization
Gap Probability Renorm.
Pomeron Flux Renom.
One-gap cross sections are suppressedTwo-gap/one-gap ratios are 17.0=≈ κ
Agreement with renormalized Regge predictions
10
10 2
10 3
10 4
10 5
10-6
10-5
10-4
10-3
10-2
10-1
1ξp
X
MX2
Num
ber o
f Eve
nts
per Δ
logξ
= 0
.1
Data
DPE MC
SD MC
DPE+SD MC
√s⎯
= 1800 GeV
0.035 ≤ ξ- p ≤ 0.095
| t- p | ≤ 1.0 GeV2
( GeV 2 )1 10 10
210
310
410
510
6CDF Preliminary
10
10 2
10 3
10 4
10 5
0 1 2 3 4 5 6 7
√s=1800 GeV
DATADD + non-DD MCnon-DD MC
Δη0=ηmax-ηmin
even
ts
10 2
10 3
10 4
10 5
0 1 2 3 4 5 6 7Δη0
exp=ηmax-ηminev
ents
√s=1800 GeVDATASDD + SD MCSD MC
DD SDD DPE
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 36
DARK ENERGY?
P(Δy) is exponentially suppressed
dydN
ρ,ey)P( particlesΔyρ ==Δ −
Rapidity gaps are formed bymultiplicity fluctuations:
Non-diffractive interactions
Δy2εe~0ty)P( =Δ
2lnlnln Msy −=−≈Δ ξ
Rapidity gaps at t=0 grow with Δy:
Diffractive interactions
2ε: negative particle density!
Gravitational repulsion?
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 37
HARD DIFFRACTIONDiffractive fractionsDiffractive structure function
factorization breakdownRestoring factorizationQ2 dependencet dependenceHard diffraction in QCD
η
dN/dη
JJ, W, b, J/ψ
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 38
All ratios ~ 1% ~ uniform suppression~ FACTORIZATION !
Hard Diffraction Fractions
gap)( ++→ Xpp
1.45 (0.25)J/ψ
0.62 (0.25)b
0.75 (0.10)JJ
1.15 (0.55)W
Fraction(%)Fraction:SD/ND ratioat 1800 GeV
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 39
Diffractive non/Factorization
0.1 1
0.1
1
10
100
β
FD jj(β
)
from DPE/SD , 0.01 ≤ ξ ≤ 0.03
from SD/ND , 0.035 ≤ ξ ≤ 0.095
p
p
ND jetjet
0p
p
p
IP
SD jetjet
p
0
p
p
IP
IP
DPE jetjet
p p
η0ηp_ ηp
R(SD/ND)
R(DPE/SD)DSF from two/one gap:factorization restored!
The diffractive structure function measured on the proton side in events with a leading antiproton is NOT suppressed relative to predictions based on DDIS
β=momentum fractionof parton in Pomeron
β=xBj/ξ
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 40
Diffractive Structure Function
)(xF)(xF
)(xRate)(xRate
)R(x
BjNDjj
BjSDjj
BjNDjj
BjSDjj
Bj
⇒
≡
Systematic uncertainties due to energy scale and resolutioncancel out in the ratio
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 41
Dijet Properties
SD boosted opposite to pbar
p
p
jet
jet
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Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 42
ET distributions
120 GeV
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Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 43
Diffractive Structure Function:Q2 dependence
ETjet ~ 100 GeV !
Small Q2 dependence in region 100 < Q2 < 10,000 GeV2
Pomeron evolves as the proton!
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 44
Diffractive Structure Function:t- dependence
No diffraction dipsNo Q2 dependence in slopefrom inclusive to Q2~104 GeV2
Fit dσ/dt to a double exponential:
Same slope over entire region of0 < Q2 < 4,500 GeV2
across soft and hard diffraction!
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 45
valence quarks
antiproton
x=ξ
Hard Diffraction in QCD
proton
deep sea
Derive diffractivefrom inclusive PDFsand color factors
antiproton
valence quarks
p
p
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 46
HIGGS BOSONS
22H )'pp'p(pM −−+= ΔM~(1-2) GeV Determine spin of H
gap gap
b
b -jet
-jet
ηp p
H
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 47
Exclusive dijets and Higgs bosons
H
Measure exclusive jj & γγ Calibrate predictions for H production rates @ LHC
Bialas, Landshoff,Phys.Lett. B 256,540 (1991)Khoze, Martin, Ryskin,Eur. Phys. J. C23, 311 (2002); C25,391 (2002);C26,229 (2002)C. Royon, hep-ph/0308283B. Cox, A. Pilkington,PRD 72, 094024 (2005)OTHER…………………………
Search for exclusive dijets:Measure dijet mass fraction
Look for signal as Rjj 1
( )rscalorimeteallMM
RX
jjjj =
KMR: σH(LHC) ~ 3 fbS/B ~ 1 if ΔM ~ 1 GeV
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 48
Exclusive Dijet Signal
b-tagged dijet fractionDijet fraction – all jets
Exclusive b-jets are suppressedby JZ= 0 selection rule
Excess over MC predictions at large dijet mass fraction
DIJETS
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 49
RJJ(excl): Data vs MC
Shape of excess of events at high Rjjis well described by both models
ExHuME (KMR): gg gg processuses LO pQCD
Exclusive DPE (DPEMC)non-pQCD based on Regge theory
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 50
jjexcl: Exclusive Dijet SignalCOMPARISON
ofInclusive data vs MC @ b/c-jet data vs inclusive
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 51
JJexcl : x-section vs ET(min)Comparison with hadron level predictions
ExHuME (red)Exclusive DPE in DPEMC (blue)
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 52
JJexcl : cross section predictionsExHuME Hadron-Level Differential Exclusive Dijet Cross Section vs Dijet Mass (dotted/red): Default ExHuME prediction(points): Derived from CDF Run II Preliminary excl. dijet cross sections
Statistical and systematic errors are propagated from measured cross section uncertainties using ExHuME Mjj distribution shapes.
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 53
Looking forward @ LHC
TOTEM/CMS ATLAS
FP420 project: http://www.fp420.com/Measure protons at 420 m from the IP during normal high luminosity running to be used in conjunction with CMS and ATLASFeasibility study and R&D for Roman Pot detector development
Physics aim :pp → p+ X + p (Higgs, New physics, QCD studies)Status: Project funded by the UK
NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07
Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 54
SummaryCDF - what we have learnt
M2 – scaling dσ/M2 not a function of smultigap diffraction restoration of factorization!flavor independence of diffractive fractions small Q2 dependence of SD/ND xBJ-distributionst-distributions independent of Q2exclusive dijet cross sections favor the
perturbative QCD over the DPE approachLHC - what to do
Elastic and total cross sections & ρ-valueHigh mass ( 4 TeV) and multi-gap diffraction Exclusive production (FP420 project)
darkenergy?