Structure Functions and Low-x Working Group Summary Convenors A. - - PowerPoint PPT Presentation

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Structure Functions and Low-x Working Group Summary Convenors A. - - PowerPoint PPT Presentation

Structure Functions and Low-x Working Group Summary Convenors A. Glazov S. Moch K. Nagano Sven-Olaf.Moch@desy.de DESY Zeuthen


slide-1
SLIDE 1

Structure Functions and Low-x

Working Group Summary

Convenors

  • A. Glazov
  • S. Moch
  • K. Nagano

Sven-Olaf.Moch@desy.de

DESY Zeuthen ————————————————————————————————————–

– XV International Workshop on Deep-Inelastic Scattering and Related Subjects, Munich, Apr 20, 2007 –

  • S. Moch

Structure Functions and Low-x – p.1

slide-2
SLIDE 2

Plan

Longitudinal structure function FL measurement of high-y cross sections, low energy run of HERA News on Parton density functions updates of global fits structure functions measurements (HERA) hard scattering cross sections (Tevatron) Forward jets and low-x HERA measurements and theory models Theory outlook

  • S. Moch

Structure Functions and Low-x – p.2

slide-3
SLIDE 3

Structure function FL

  • S. Moch

Structure Functions and Low-x – p.3

slide-4
SLIDE 4

vargas

DIS 2007, München Andrea Vargas Treviño

Cross Section

Data fill the transition region at Q² ~1 GeV² Combined preliminary H1 data in agreement with ZEUS

Vargas

H1 low-Q2 analysis final measurement for HERA-I at low Q2 (long time effort) improved precision for extraction of FL

  • S. Moch

Structure Functions and Low-x – p.4

slide-5
SLIDE 5

raicevic

  • Experimentalchallengesofthisanalysisaresimilartotheonesforanalysisof

lowenergyrun.

r 4 2 2 2

σ x Q Y 2π dxdQ σ d

+

= α

2

y) (1 1 Y − + =

+

) Q (x, F Y y ) Q (x, F σ

2 L 2 2 2 r +

− =

2 L

F F ≤ ≤ FL givessizablecontributiononlyathighy

/2) (θ sin E E 1 y

e 2 e ' e

− =

Thisanalysis:highy,lowandmediumQ2 aslowaspossiblelowE’e required

/sy Q x

2

=

xg(x)~FL(atlowx)

From

xg(x)– gluondensityfunction

x Q2 / GeV2

y = 1 y = 0.6 H1 HERA-I H1 HERA-II high y NMC BCDMS

1 10 10 2 10 3 10 4 10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

1

Raicevic

direct measurement of FL in high-y region (very difficult)

  • S. Moch

Structure Functions and Low-x – p.5

slide-6
SLIDE 6

raicevic

  • /
  • Epz =(E– pz)HFS +(E– pz)e’ =2P(measuredbeamenergy)

10 20 30 4 6 8 10

Ee /GeV 103 events Data HERA-II MC+BG BG (data)

5 10 15 20 150 155 160 165 170

Θe /deg 103 events

H1 Preliminary

5 10 15 20

  • 40
  • 20

20 40

Zv /cm 103 events

10 20 20 40 60 80

Total E-pz /GeV 103 events

Raicevic

large backgrounds photo-production low-Q2 electron (wrong charge lepton) initial state radiation large QED bkgd (cut beam energy)

  • S. Moch

Structure Functions and Low-x – p.6

slide-7
SLIDE 7

shimizu

9

6m tagged sample

Not perfect, but reasonable description of distribution shape by PHP MC.

Energy in 6mT xpos on 6mT CAL energy

  • f misidentified

electron e Normalized by Nevents

6m tagger located downstream of electron beam. Direct detection of PHP events with good acceptance.

e+ e+ + data – PHP MC

Shimizu

ZEUS: background control by e−-tagging at low Q2 different technologies as H1 (cross check)

  • S. Moch

Structure Functions and Low-x – p.7

slide-8
SLIDE 8

shimizu

14

Reduced cross section

Measured reduced cross sections are compared to SM predictions with – CTEQ5D – ZEUS-Jets PDF They are well described by the predictions. ZEUS

σ ~ y

1 2

2

= 27 GeV

2

Q

1 2

2

= 70 GeV

2

Q

1 2

2

= 200 GeV

2

Q

0.5 1 1 2

2

= 650 GeV

2

Q

2

= 35 GeV

2

Q

2

= 90 GeV

2

Q

2

= 250 GeV

2

Q 0.5 1

2

= 800 GeV

2

Q

2

= 45 GeV

2

Q

2

= 120 GeV

2

Q

2

= 350 GeV

2

Q 0.5 1

2

= 1200 GeV

2

Q

2

= 60 GeV

2

Q

2

= 150 GeV

2

Q

2

= 450 GeV

2

Q

ZEUS (prel.) )

  • 1

06e+p (29pb CTEQ5d ZEUS-Jets

Systematics

  • Electron energy scale

2%

  • PHP norm. factor

10%

  • Electron finding inefficiency 10%
  • E-pz threshold

2GeV

Shimizu

  • S. Moch

Structure Functions and Low-x – p.8

slide-9
SLIDE 9

raicevic

  • '

()*+,-. 01!! 23&4

  • Theprecisionofthenewmeasurementsisaboutfactorof2betterthaninthe

publishedresultsbasedonHERAIdata.

  • Systematiccrosssectionuncertainty23%.

1 1.1 1.2 1.3 1.4 10 15 20 25 Q2 /GeV2 σred

Y=0.825

H1 1997 (W=273 GeV) H1 HERA-II prelim. (W=289 GeV)

H1 Preliminary

Raicevic

cross section at high y (preliminary)

  • S. Moch

Structure Functions and Low-x – p.9

slide-10
SLIDE 10

shimizu

17

Low Energy Running

HERA has finished ‘usual’ operation on 21/Mar/2007 Since then, HERA started to deliver luminosity with lowered proton beam energy (LER) successfully. Congratulations to HERA! 26/Mar 2/Jul: 3 months of LER operation. Main issue in LER: FL Cross sections with same (x,Q2) but different y, i.e. Different centre

  • f mass energy

Direct separation of FL from F2 . w/o theory assumption FL at low-x : legacy of HERA ) , ( ) , ( ~

2 2 2 2

Q x F Y y Q x F

L

  • Shimizu

direct FL at HERA: unique measurement

  • S. Moch

Structure Functions and Low-x – p.10

slide-11
SLIDE 11

klein

Max Klein low energy run 17.4.2007 DIS07

Luminosity collected by April 16th

enlarged satelites

increase of L and with t

Klein

  • S. Moch

Structure Functions and Low-x – p.11

slide-12
SLIDE 12

Perturbative corrections for FL

S.M., Vermaseren, Vogt ‘05

large higher order corrections

b α (n)

a,i (N)

(4 π) = c(n−1)

a,i

(N) 2 c(n)

a,i (N) 0.2 0.4 0.6 0.8 10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

1

x(cL,q qS) ⊗

LO NLO NNLO

x x(cL,g g) ⊗

αS = 0.2, nf = 4

1 2 3 4 10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

1 0.2 0.4 0.6 0.8 1 5 10 15

α

∧ 2,ns(N) NLO N2LO N3LO

N

α

∧ L,ns(N) NLO N2LO

Nf = 4

0.1 0.2 0.3 0.4 5 10 15

  • S. Moch

Structure Functions and Low-x – p.12

slide-13
SLIDE 13

News on global fits

  • S. Moch

Structure Functions and Low-x – p.13

slide-14
SLIDE 14

thorne

0.5 1 1.5 10

  • 4

10

  • 3

10

  • 2

10

  • 1

xu(x,Q2=20)

Obtain NNLO partons with uncertainties due to experimental errors for the first time. Reported last year. Same procedure as before – 15 eigenvector sets of partons and ∆χ2 = 50 for 90% confidence limit. First time we have full NNLO with no major approximations. (Heavy flavours a major issue.) In general size of uncertainties similar (perhaps a little smaller) to at NLO. Change from NLO to NNLO greater than uncertainty in each. NNLO fit consistently better than NLO.

DIS07 MRST(MSTW) 3

Thorne

partons go NNLO with errors NNLO resolves more features of theory e.g.

qs, qv, q− all evolve with different kernels

  • S. Moch

Structure Functions and Low-x – p.14

slide-15
SLIDE 15

tung

  • $-" ="

#-*%-#"- = ?'#(*-"-!"-4 #"-" @8 A>

Tung

heavy flavor scheme with general mass implemented (charm) changes in PDF updates larger than previous error estimates

  • S. Moch

Structure Functions and Low-x – p.15

slide-16
SLIDE 16

robson

17/22 Aidan Robson Glasgow University

CDF kT

Measured in 5 bins of y jet Forward jet - asymmetric interaction DonÕt expect new physics in high y jet region

Robson

High-x gluon from inclusive jets

  • S. Moch

Structure Functions and Low-x – p.16

slide-17
SLIDE 17

toole

April 17, 2007 DIS 2007 6

Z Rapidity

* Curves made with code from Anastasiou, et. al., PRD69, 094008 (2004).

Submitted to PRD

Main contributions to syst's: eff's, backgrounds. At high y: eff's, PDFs Theory and data in good agreement Measurement is currently statistics limited

Toole

  • S. Moch

Structure Functions and Low-x – p.17

slide-18
SLIDE 18

toole

April 17, 2007 DIS 2007 9

W Charge Asymmetry with muons

Curves produced with Resbos-A Main systematic uncertainty is from efficiencies ε± Measurement currently statistics limited

∫Ldt = 230 pb-1

Toole

constrain u/d ratio

  • S. Moch

Structure Functions and Low-x – p.18

slide-19
SLIDE 19

bhadra

Sampa Bhadra, DIS2007 17

  • Combine e (L+R) to extract

“unpolarised” e- p cross section

  • Use HERA II “unpolarised” e- p

data with HERA I e+p data: * Reduced cross section difference e- p > e+ p (see effect of sign) Measure xF3 from this

) ~ ~ ( 2

3 p e NC p e NC

Y Y F x

  • ZEUS

0.2 0.4 0.6 0.8 1 1.2

2

= 200 GeV

2

Q 0.2 0.4 0.6 0.8 1 1.2

2

= 650 GeV

2

Q 0.2 0.4 0.6 0.8 1 1.2

2

= 2000 GeV

2

Q

  • 2

10

  • 1

10

0.2 0.4 0.6 0.8 1 1.2

2

= 12000 GeV

2

Q

2

= 250 GeV

2

Q

2

= 800 GeV

2

Q

2

= 3000 GeV

2

Q

  • 2

10

  • 1

10

2

= 20000 GeV

2

Q

2

= 350 GeV

2

Q

2

= 1200 GeV

2

Q

2

= 5000 GeV

2

Q

  • 2

10

  • 1

10

2

= 30000 GeV

2

Q

x

2

= 450 GeV

2

Q

2

= 1500 GeV

2

Q

2

= 8000 GeV

2

Q

ZEUS NC (prel.) = 0)

e

, P

  • 1

p (177 pb

  • e

SM (ZEUS-JETS) ZEUS NC = 0)

e

, P

  • 1

p (63.2 pb

+

e SM (ZEUS-JETS)

σ ~

2 2 2 4

1 2 ~ dxdQ d Y xQ

p e NC NC

  • Bhadra

full e− sample from HERA II 10-fold increased stats. compared to HERA I

  • S. Moch

Structure Functions and Low-x – p.19

slide-20
SLIDE 20

bhadra

Sampa Bhadra, DIS2007 18

Most precise measurement of xF3 from ep NC DIS at high Q2

  • Sensitivity to valence quark

distribution in a region where there were no previous DIS measurements with pure proton target

ZEUS

3

xF

  • 0.1

0.1 0.2

2

= 3000 GeV

2

Q

  • 1

10 1

  • 0.1

0.1 0.2

2

= 12000 GeV

2

Q

2

= 5000 GeV

2

Q

  • 1

10 1

2

= 20000 GeV

2

Q

2

= 8000 GeV

2

Q

  • 1

10 1

2

= 30000 GeV

2

Q

ZEUS NC (prel.) )

  • 1

p (240 pb

±

e SM (ZEUS-JETS)

x Extract xF3 for each bin

  • can extract xF3

z

Bhadra

valence quarks in high

Q2-region

(lowering x-range)

  • S. Moch

Structure Functions and Low-x – p.20

slide-21
SLIDE 21

thorne

CCFR/NuTeV dimuon cross-sections and strange quarks dσ dxdy(νµ(¯ νµ)N → µ+µ−X) = BcN A dσ dxdy(νµs(¯ νµ¯ s) → cµ−(¯ cµ+)X), Bc = semileptonic branching fraction N = nuclear correction A = acceptance correction. νµ and ¯ νµ cross-sections probe s and ¯ s (small mixing with d and ¯ d). Have previously indirectly used CCFR data to parameterise strange according to s(x, Q2

0) = ¯

s(x, Q2

0) = κ

2[¯ u(x, Q2

0) + ¯

d(x, Q2

0)]

κ ≈ 0.5 Now fit strange directly rather than assuming same shape as average of ¯ u + ¯ d at input and some fixed fraction. Also allow possibility of s(x, Q2

0) = ¯

s(x, Q2

0).

DIS07 MRST(MSTW) 8

Thorne

strange density from ν − N DIS data

  • S. Moch

Structure Functions and Low-x – p.21

slide-22
SLIDE 22

tung

  • Current global analysis does not

require a non-zero s-(x).

  • It can be non-zero. The range of its

magnitude as determined by current experimental constraints: —the same as in the 2003 study.

  • A range on its shape is found

Results on Strange Asymmetry

s-(x) x s-(x)

( )

Tung

asymmetric strange sea for NuTev anomaly (second moment s−)

  • S. Moch

Structure Functions and Low-x – p.22

slide-23
SLIDE 23

rogal

NuTeV experiment - Paschos-Wolfenstein relation

Exact relation for massless quarks and isospin zero target

Paschos,Wolfenstein’73, Llewelin Smith’83

R− = σ(νµN → νµX) − σ(¯ νµN → ¯ νµX) σ(νµN → µ−X) − σ(¯ νµN → µ+X) = 1 2 − sin2 θW

measurement of sin2 θW NuTeV ’01 with large deviations from Standard model expectations QCD corrections to the Paschos-Wolfenstein relation second moments of valence PDFs q− =

  • dx x(q − ¯

q)

expansion in isoscalar combination u− + d−

Davidson, Forte, Gambino, Rius, Strumia ’01; Dobrescu, Ellis ‘03; Moch, McFarland ‘03 R− = 1 2 − sin2 θW + » 1 − 7 3 sin2 θW + 8αs 9π ˘ 1 + αs1.689 + α2

s(3.661 ± 0.002)

¯ „ 1 2 − sin2 θW «– × „u− − d− u− + d− − s− u− + d− + c− u− + d− «

main uncertainties in s−

Martin, Roberts, Stirling, Thorne ‘04; Lai, Nadolsky, Pumplin, Stump, Tung, Yuan ‘07

QCD corrections under control Moch, M. R., Vogt ‘07

Charged Current Deep Inelastic scattering at three loops – p.15

Rogal

  • S. Moch

Structure Functions and Low-x – p.23

slide-24
SLIDE 24

radescu

NuTeV Differential Cross Section:

0.5 1 1.5 2

(E=150 GeV) Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y

0.5 1 1.5 2

(E=150 GeV) Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y

0.5 1 1.5 2

(E=150 GeV) Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y

0.5 1 1.5 2

(E=150 GeV) Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y

0.5 1 1.5

(E=150 GeV) Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y

0.5 1 1.5

(E=150 GeV) Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y

0.2 0.4

(E=150 GeV) Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y

0.1 0.2 0.3 0.2 0.4 0.6 0.8 1

(E=150 GeV) Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y (E=150 GeV)

x=0.015

Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y (E=150 GeV)

x=0.045

Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y (E=150 GeV)

x=0.125

Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y (E=150 GeV)

x=0.175

Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y (E=150 GeV)

x=0.275

Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y (E=150 GeV)

x=0.35

Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y (E=150 GeV)

x=0.55

Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y

0.2 0.4 0.6 0.8 1

(E=150 GeV)

x=0.65

Neutrino Anti-Neutrino Y 1/E d2σ/dxdy (x 10-38 cm2/GeV) Y

LABEL: filled circles - NuTeV :: open squares - CCFR :: crosses - CDHSW :: line - NuTeV model

plots show extracted ν(ν) − Fe Cross-Sections as function of y for different x bins at Eν = 65 GeV and 150 GeV NuTeV has comparable statistics to other ν experiments: CDHSW [Z. Phys C49 187, 1991] - crosses

CCFR [U. K. Yang PhD. Thesis] - open squares

Better control of largest systematic uncertainties: data Eµ scale Ehad range CDHSW 2% 2.5% 20-200 GeV CCFR 1% 1% 30-300 GeV NuTeV 0.7% 0.43% 30-350 GeV

DIS 07, Munich Voica A. Radescu voica@mail.desy.de April 17, 2007 – p.7/25

Radescu

  • S. Moch

Structure Functions and Low-x – p.24

slide-25
SLIDE 25

radescu

Neutrino Data Comparison:

NuTeV compared to other ν − F e experiments (CCFR and CDHSW): good agreement at moderate x with CCFR over the full Eν and y range (level and shape), and with CDHSW (level) at x > 0.4 CCFR is consistently below NuTeV:

0.7 0.75 0.8 0.85 0.9 0.95 1 1.05 0.1 0.2 0.3 0.4 0.5 0.6 0.7

Ratio x

Neutrino Anti-neutrino

CCFR and NuTeV similar in design and analysis method; largest single contribution is due to miscalibration of the magnetic field map of the toroid in CCFR: accounts for ∼ +6% of the 18% difference at x = 0.65. model difference (fit to NuTeV data): accounts for ∼ +3% difference at x = 0.65. improved muon and hadron energy smearing models: accounts for ∼ +2% difference at x = 0.65. Other differences between CCFR and NuTeV experiments: NuTeV had separate neutrino and antineutrino runs (SSB): NuTeV always set to focus the “right-sign” muon: better acceptance CCFR had simultaneous neutrino and antineutrino runs CCFR had toroid polarity∼ 50% set to focus on µ+ and∼ 50% set on µ−

DIS 07, Munich Voica A. Radescu voica@mail.desy.de April 17, 2007 – p.8/25

Radescu

NuTev data not completely consistent with CCFR (nuclear corrections at high-x?)

  • S. Moch

Structure Functions and Low-x – p.25

slide-26
SLIDE 26

thorne

MSTW 2007 NLO PDFs (preliminary)

x

  • 4

10

  • 3

10

  • 2

10

  • 1

10

  • 0.2
  • 0.15
  • 0.1
  • 0.05

0.05 0.1 0.15 0.2

)

2

GeV

4

= 10

2

(x, Q u Fractional uncertainty on x

x

  • 4

10

  • 3

10

  • 2

10

  • 1

10

  • 0.2
  • 0.15
  • 0.1
  • 0.05

0.05 0.1 0.15 0.2

)

2

GeV

4

= 10

2

(x, Q d Fractional uncertainty on x

x

  • 4

10

  • 3

10

  • 2

10

  • 1

10

  • 0.2
  • 0.15
  • 0.1
  • 0.05

0.05 0.1 0.15 0.2

)

2

GeV

4

= 10

2

Fractional uncertainty on xs(x, Q

Fitting to strange from NUTEV dimuon data affects uncertainties on partons

  • ther than strange.

Previously for us (and everyone else) strange a fixed proportion of total sea in global fit. Genuine larger uncertainty on s(x)– feeds into that on ¯ u and ¯ d quarks. Low x data on F2(x, Q2) constrains sum 4/9(u + ¯ u) + 1/9(d + ¯ d + s + ¯ s). Changes in fraction of s + ¯ s affects size

  • f ¯

u and ¯ d at input. The size of the uncertainty on the small x anti-quarks roughly doubles – ∼ 1.5% →∼ 3%. (Remember uncertainties quoted as 90% confidence limits.)

DIS07 MRST(MSTW) 14

Thorne

PDF errors will get larger (relaxing previous constraints)

  • S. Moch

Structure Functions and Low-x – p.26

slide-27
SLIDE 27

thorne

  • 40
  • 20

20 40 10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

1

x percentage uncertainty Q2=5GeV2

MRST uncertainty blows up for very small x, whereas Alekhin (and ZEUS and H1) gets slowly bigger, and CTEQ saturates (or even decreases). Related to input forms and scales. (Neck in MRST gluon cured in MSTW).

DIS07 MRST(MSTW) 27

Thorne

Error on gluon density at x = 10−5 largely due to parametrization bias (no data available)

  • S. Moch

Structure Functions and Low-x – p.27

slide-28
SLIDE 28

coopersarkar

MRST PDF

NNLO corrections small ~ few% NNLO residual scale dependence < 1% PDF Set ZEUS-S CTEQ6.1 MRST01

  • l

W W B

  • l

W W B

  • ll

Z Z B

  • 41

. 07 . 12

  • (nb)

(nb) (nb)

30 . 76 . 8

  • 06

. 89 . 1

  • 56

. 66 . 11

  • 43

. 58 . 8

  • 08

. 92 . 1

  • 23

. 72 . 11

  • 16

. 72 . 8

  • 03

. 96 . 1

  • W/Z production have been considered

as good standard candle processes with small theoretical uncertainty.

PDF uncertainty has been considered as a dominant contribution and most PDF groups quote uncertainties <~5% BUT the central values differ by more than some of the uncertainty estimates. AND the situation just got dramatically worse. The new CTEQ6.5 estimate is 8% higher

Not so well known Not such a good bet for a precise luminosity monitor What do we think is well known: W/Z cross-sections?

Cooper-Sarkar

Uncertainty estimates for LHC cross sections (e.g. large shifts CTEQ6.1 vs. CTEQ6.5)

  • S. Moch

Structure Functions and Low-x – p.28

slide-29
SLIDE 29

thorne

Drell-Yan Cross-section at Tevatron for 80 GeV with Different Orders 0.5 1 0.25 0.5 0.75 1 1.25 1.5 1.75 2 2.25 2.5

y ratio NLOP-NLOM NLOP-LOM LOP-LOM

M=80GeV

Look at W production at Tevatron. Indeed see that nearer to truth with LO matrix element and NLO parton than LO matrix element and LO

  • parton. Shape good – too small.

LO parton and LO matrix element wrong shape and worse at central rapidity but indeed better at high rapidity.

DIS07 Monte Carlo 4

Thorne

LO PDFs vs. NLO PDFs vs. NNLO PDFs largely depended on

  • bservable (K-factor

philosophy) There is no free lunch.

  • S. Moch

Structure Functions and Low-x – p.29

slide-30
SLIDE 30

yuan

  • Better determine PDFs
  • Better determine, for example,

the mass of W boson MW

  • ,

,

e e e T T

y p m

W

e

e

  • New Task of Global Analysis:

Include Transverse Momentum pT distributions

Measuring MW

1 S

  • QCD

Resummation

Yuan

global fit with pt-resummation (large logarithms in pt)

  • S. Moch

Structure Functions and Low-x – p.30

slide-31
SLIDE 31

white

Global Fit - Results

Reduced Cross-Section

0.2 0.4 0.6 0.8 1 10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

1

σ

~(x,Q2)

Q2=2 GeV2

H1 data H1 prelim 0.25 0.5 0.75 1 10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

Q2=3.5 GeV2

0.5 1 10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

1

x σ

~(x,Q2)

Q2=6.5 GeV2

0.5 1 10

  • 5

10

  • 4

10

  • 3

10

  • 2

10

  • 1

x Q2=8.5 GeV2

◮ Turnover required by data

at low x (high y) - NLO fails.

◮ Resummation helps!

Interesting to compare with NNLO.

18 / 19

White

improved global fit through small-x resummation (NLL accuracy)

  • S. Moch

Structure Functions and Low-x – p.31

slide-32
SLIDE 32

alekhin

Kinematics of the inclusive DIS data

1 10 10 2 10

  • 4

10

  • 3

10

  • 2

10

  • 1

x Q2 (GeV2) BCDMS SLAC E665 H1/ZEUS NMC W=4 1.8

Regular practice it to cut the low-Q (low-W) data in order to avoid potentially dangerous re- gions, however in this case a lot

  • f precise data is lost.

3

Alekhin

Use precision data at low Q2 extract higher twist

F exp

2

(x, Q2) = F twist−2

2

(x, Q2) 1 + CHT(x, Q2) Q2[GeV2] !

  • S. Moch

Structure Functions and Low-x – p.32

slide-33
SLIDE 33

yang

Un-ki Yang, University of Manchester

7

UniÞed approach

! NNLO pQCD +TM describes the DIS and resonance data very well

" Theoretically, breaks down at low Q2 " Practically, no way for MC

! A phenomenological HT from the NLO analysis is close to the NNLO pQCD term ! Can we use an effective LO PDFs with a modified scaling variable to absorb TM, HT, missing higher orders?

P=M q

mf=M*

!W = (Q

2 + mf 2 " mi 2)+ (Q 2 + mf 2 " mi 2) 2 + 4Q 2(mi 2 + P t 2)

2M#[1+ (1+Q

2 /# 2)]

!W = Q

2 + B

{M"[1+ (1+Q

2 /" 2)] + A}

Q

2

Q

2 + C

F

2(!w ,Q 2)[LO]

Yang

unfied approach to e/ν − N cross sections useful for MINOS, MiniBooNE, K2K, ...

  • S. Moch

Structure Functions and Low-x – p.33

slide-34
SLIDE 34

gabbert Fit Result and Data

6 GeV 2 < Q2 < 90 GeV 2

10

  • 1

1 10 10 2

W2 σtot • c (barn)

6.8E+00 1.636 8.3E+00 1.635 1.2E+01 1.634 1.6E+01 1.633 2.2E+01 1.632 3.1E+01 1.631 4.3E+01 1.630 6.1E+01 1.629 8.5E+01 1.628

↑ ↑ , GeV 2 10 102 103 104 105

, GeV

Q2 c

Gabbert

updating ALLM parametrization with new data

  • S. Moch

Structure Functions and Low-x – p.34

slide-35
SLIDE 35

rojo

Introduction Methodological issues The nonsinglet case Status of the singlet case Conclusions and outlook

Comparison to other approaches

  • 1. Underestimated uncertainties in existing fits (both global and NS fits)
  • 2. Larger uncertainties both in data and in extrapolation region: absence of

functional form bias.

  • 3. Clear effect of error increase in extrapolation region.

Juan Rojo-Chac´

  • n

LPTHE - Universit´ e Paris VI et Paris VII Progress in neural parton distributions

Rojo

– neural network analysis without parametrization bias – more data input needed for constraints on uncertainties – first neural PDF set announced for summer 2008

  • S. Moch

Structure Functions and Low-x – p.35

slide-36
SLIDE 36

liuti

Liuti

PDF fits with self-organizing maps (proof of principle) LO central values of fit (no smoothness criterium)

  • S. Moch

Structure Functions and Low-x – p.36

slide-37
SLIDE 37

pisano

Curvature of F2

  • At x = 10−4 most measurements lie along a straight (dotted) line, if plotted versus

q = log10 „ 1 + Q2 0.5 GeV2 «

  • D. Haidt, EPJ C35, 519 (2004)

0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2 1.4

q F2

p

NNLO 0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2 1.4

q F2

p

NLO-MS 0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2 1.4

q F2

p

NLO-DIS 0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2 1.4

q F2

p

MRST01 0.5 1 1.5 2 0.2 0.4 0.6 0.8 1 1.2 1.4

q F2

p

  • MRST01 fit (NLO-MS): sizable curvature for F2, incompatible with the data, mainly

caused by the valence–like input gluon distribution at Q2

0 = 1 GeV2

. – p.7/11

Pisano

tests of pQCD (global fit to F2)

  • S. Moch

Structure Functions and Low-x – p.37

slide-38
SLIDE 38

detmold

Example: axial charge

¥ simplest twist-two op.

0.2 0.4 0.6 0.8

m!

2 (GeV 2)

0.2 0.4 0.6 0.8 1 1.2 1.4

gA

LHPC/MILC LHPC/SESAM RBCK QCDSF/UKQCD Experiment

L H P C , P R L 6

Unquenched data

gA = x0∆u−∆d

W Detmold Hadron structure in lattice QCD DIS2007

Detmold

lattice: moments of PDFs at low scales

  • S. Moch

Structure Functions and Low-x – p.38

slide-39
SLIDE 39

gousset

Inclusive photons at y = 0

Motivations Inclusive photons Prompt photon Nuclear ratios y = 0 y = 3 Isolated photons Outlook

6 Gousset

nuclear modifications of gluon distribution (can be up to 30%) study prompt-photon production in p-A collisions

  • S. Moch

Structure Functions and Low-x – p.39

slide-40
SLIDE 40

zotov

Nikolai Zotov, DIS’07 Workshop Munich, April 18, 2004

Here the measurement is compared to the fit of the SF F2(x, Q2):

10

  • 1

1 10 1 10 10

2

10

3

Q2 (GeV2) F2

H1 EPJC 21 (2001) 33 H1 F2-fit CCFM F2-fit

The SF F2(x, Q2) as function of Q2 for different values of x. The shaded area shows the region which is not used in the fit.

11

Zotov

F2 fits with unintegrated

gluon distribution (kt-dependence) CCFM evolution

  • S. Moch

Structure Functions and Low-x – p.40

slide-41
SLIDE 41

Forward jets

  • S. Moch

Structure Functions and Low-x – p.41

slide-42
SLIDE 42

danielson

QCD Dynamics in low-x DIS T. Danielson, U. Wisconsin DIS 2007, April 18, 2007 - 8

ZEUS Dijet pT Correlations vs. xBj ZEUS Dijet pT Correlations vs. xBj

|pT|/(2 ET

jet1) sensitive to parton evolution, gluon radiation

  • |pT|/(2 ET

jet1) = 1 without gluon radiation

NLOjet calculations at O(s

2) do not describe dijet data at low xBj

NLOjet calculations at O(s

3) describe data, even at low xBj

  • Higher order terms important at low xBj
  • Allows for more gluon emission

Danielson

study gluon dynamics

  • S. Moch

Structure Functions and Low-x – p.42

slide-43
SLIDE 43

danielson

QCD Dynamics in low-x DIS T. Danielson, U. Wisconsin DIS 2007, April 18, 2007 - 12

Summary: Low-xBj Dynamics at HERA Summary: Low-xBj Dynamics at HERA

Dijet, trijet correlations at ZEUS measured at small xBj (10-2 < xBj < 10-4)

  • Dijet, trijet pT and azimuthal correlations most senstive

to gluon radiation, parton evolution

  • Higher-order terms important at low Q2, xBj
  • Effects more pronounced for dijets
  • Higher-order calculations up to 10x larger at very small xBj
  • Correlations well-described by NLOjet calcs.
  • Cross sections in xBj, correlations in well-described by

NLOjet calcs.

  • Less sensitive to parton evolution scheme

Danielson

  • S. Moch

Structure Functions and Low-x – p.43

slide-44
SLIDE 44

nowak

Grayna Nowak DIS 2007, April 16-20, Munich 8

H1 preliminary H1 preliminary

Threejet Cross-section – Forward Jet Selection

LO O(s

2 ) (1 gluon rad.) NLOO(s 3) (2 gluons rad.)

1 forward + 2 central jets: good agreement

at low x description improves by a factor of 2; missing only 30% of events

2 forward + 1 central jets: large deficit

discrepancy at low x reduced: 10 3.5 but with still a large discrepancy remaining

d/dxBj

parton level parton level

subsample with forward jet:

jet > 1.73 , xjet=E*jet/Ep,beam> 0.035

largest disagreement at low x and large

Nowak

constrain jet data to low-x

  • S. Moch

Structure Functions and Low-x – p.44

slide-45
SLIDE 45

nowak

3-jet x-sections, Frwd Jet Selection, Comparison

d/dcos

,

, d/dcos

,

2 forward jet sample

cross sections are shape normalized to the data (NLOjet++ +32%, CDM -9%, RAPGAP +63 %)

NLOjet++ (parton level)

CDM, RAPGAP (hadron level)

angular topology for

H1 preliminary H1 preliminary H1 preliminary H1 preliminary

here: NLOjet++ better than CDM CDM better than RG d+r

Grayna Nowak DIS 2007, April 16-20, Munich 13 Nowak

effective description by CDM (color dipole model)

  • S. Moch

Structure Functions and Low-x – p.45

slide-46
SLIDE 46

khein

  • D

=< /(,& " " 5

#$ #$

Khein

perturbative higher orders large (NLOJET++ fails) test Ariadne Monte Carlo (modelling CDM) Cascade Monte Carlo to be improved

  • S. Moch

Structure Functions and Low-x – p.46

slide-47
SLIDE 47

avsar

Mueller’s Dipole Model

x x x y y y w w w z z z

x x x y y y x x x y y y z z z x x x y y y z z z w w w

Decay probability given by dP dY = ¯ α 2π (x x x − y y y)2 (x x x − z z z)2(z z z − y y y)2d2z z z, ¯ α = αsNc π , Y = ln1/x Reproduces LO BFKL evolution.

Emil Avsar, 2007, DESY – p.3/15

Avsar

Dipole phenomenology (Monte Carlo approach)

  • S. Moch

Structure Functions and Low-x – p.47

slide-48
SLIDE 48

shoshi

Shortcomings of “mean field equations”: Pomeron loops

[Iancu,Triantafyllopoulos 2005]

Two dipoles scattering off a target:

∂ ∂Y

  • “mean field equations”

graph missed!

  • Pomeron loops missed!

Shoshi

improvements of dipole model adding pomeron loops see also Nikolayev in HFL-WG on AKG unitarity cutting rules in QCD

  • S. Moch

Structure Functions and Low-x – p.48

slide-49
SLIDE 49

lublinsky

Multi gluon production in dilute limit

For the BFKL approximation:

Y Y Y Y Y Y

1 2 3 4 5

k k k k k

1 2 3 4 5

G G G G

BFKL BFKL BFKL BFKL

Very schematically: dσ dY1 dk2

1 . . . dYn dk2 n

∼ ΦT GBF KL

Yn−Y0 L(kn) . . . GBF KL Y1−Y2 L(k1) GBF KL Y −Y1

ΦP What if we have multiple rescatterings? many letters: GLR-BK-JIMWLK and BKP

Lublinsky

modelling multiple gluons at high energies

  • S. Moch

Structure Functions and Low-x – p.49

slide-50
SLIDE 50

royon

Mueller Navelet jets Same kind of processes at the Tevatron and the LHC

feff x2 h feff h x1 k1, y1 = ln(x1 √ S/k1) k2, y2 = − = ln(x2 √ S/k2) ∆η = ln(x1x2s/(k1k2))

  • Same kind of processes at the Tevatron and the LHC:

Mueller Navelet jets

  • Study the ∆Φ between jets dependence of the cross

section:

Royon

phenomenology of forward jets for hadron colliders (Tevatron, LHC)

  • S. Moch

Structure Functions and Low-x – p.50

slide-51
SLIDE 51

sabiovera

Y

C1 C0

2 3 4 5 6 .2 .4 .6 .8 1 1

Figure 2: cos φ = C1/C0 at a p¯ p collider with √s = 1.8 TeV for BFKL at LO (solid), NLO (dashed), and collinear resummation (dash–dotted).

Sabio-Vera

analysis of dijet angular correlations for Tevatron data effective small-x description of Mueller-Navalet jets

  • S. Moch

Structure Functions and Low-x – p.51

slide-52
SLIDE 52

Theory outlook

  • S. Moch

Structure Functions and Low-x – p.52

slide-53
SLIDE 53

basso

Symmetries of Anomalous Dimensions

Symmetries of anomalous dimensions reflect the symmetries of the theory

Conformal invariance

◮ Define the scaling function f as

γ(N) = f „ N + 1 2γ(N) « Conformal invariance is broken by the running of the coupling constant

◮ Nevertheless, the beta-function contribution can be incorporated in the

above consideration, within MS-like renormalization scheme. This leads to a slightly modified definition of the scaling function f γ(N) = f „ N + 1 2γ(N) − β(αs) 2αs «

BASSO Benjamin Anomalous Dimensions of High-Spin Operators Beyond the Leading Order

Basso

expolit underlying relation for DIS anomalous dimensions (splitting functions)

  • S. Moch

Structure Functions and Low-x – p.53

slide-54
SLIDE 54

lipatov

6 Maximal transcedentality

Most transcendental functions (K.,L. (2002)) γ(j) = ˆ aγ1(j)+ˆ a2γ2(j)+ˆ a3γ3(j)+... , γ1(j+2) = −4S1(j) Two-loop dimension (K.,L.,V. (2003)) γ2(j + 2) 8 = 2S1

  • S2 + S−2
  • − 2S−2,1 + S3 + S−3

Three-loop dimension (K.,L.,O.,V. (2004)) γ3(j + 2)/32 = −12 (S−3,1,1 + S−2,1,2 + S−2,2,1) +6 (S−4,1 + S−3,2 + S−2,3) − 3 S−5 − 2 S3 S−2 − S5 −2 S2

1 (3 S−3 + S3 − 2 S−2,1)−S2 (S−3 + S3 − 2 S−2,1)

+24 S−2,1,1,1 − S1

  • 8S−4 + S2

−2 + 4S2S−2 + 2S2 2

  • −S1 (3S4 − 12S−3,1 − 10S−2,2 + 16S−2,1,1) ,

Sa(j) =

j

  • m=1

1 ma , Sa,b,c,···(j) =

j

  • m=1

1 ma Sb,c,···(m) , S−a(j) =

j

  • m=1

(−1)m ma , S−a,b,···(j) =

j

  • m=1

(−1)m ma Sb,···(m), S−a,b,c···(j) = (−1)jS−a,b,...(j)+S−a,b,···(∞)

  • 1−(−1)j

Lipatov

review on N = 4 SYM new avenues from pomerons to gravitons opening up . . .

  • S. Moch

Structure Functions and Low-x – p.54

slide-55
SLIDE 55

Thanks

– to the organizers for this very nice workshop – to my co-convenors A. Glazov and K. Nagano

  • S. Moch

Structure Functions and Low-x – p.55