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Diffraction, Dark Energy, and Higgs Bosons K. Goulianos The Rockefeller University Seminar @ NESTOR Institute, PYLOS, GREECE, 20 Aug 07 QCD , Strings, or OTHER?
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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

NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07

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

NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07

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

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

NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07

Diffraction, Dark Energy, and Higgs Bosons K. Goulianos 42

ET distributions

120 GeV

NESTOR Institute SeminarPYLOS, GREECE, 20 Aug 07

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?


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