Electroweak Physics at HERAjmeyer/talks.and.pubs/ringberg2005.talk.pdf · ∆χ2=1 (M H=120GeV)...

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Electroweak Physics at HERA Joachim Meyer DESY

Transcript of Electroweak Physics at HERAjmeyer/talks.and.pubs/ringberg2005.talk.pdf · ∆χ2=1 (M H=120GeV)...

Page 1: Electroweak Physics at HERAjmeyer/talks.and.pubs/ringberg2005.talk.pdf · ∆χ2=1 (M H=120GeV) ∆χ2=1 (M H=300GeV) m t world average M W world average H1 m t (GeV) M W (GeV) 80

Electroweak Physics at HERA

Joachim MeyerDESY

Page 2: Electroweak Physics at HERAjmeyer/talks.and.pubs/ringberg2005.talk.pdf · ∆χ2=1 (M H=120GeV) ∆χ2=1 (M H=300GeV) m t world average M W world average H1 m t (GeV) M W (GeV) 80

The conference logo really fits this talk …….

Joachim Meyer Ringberg 2005 2

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OutlineTest of electroweak SM at high spacelike momentum transfers

HERA I : • Electroweak Unification• Electroweak DIS cross section fits • Propagator mass• NC quark couplingsHERA II :• Polarized CC cross sections• Polarized NC cross sections

Outlook

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Inclusive Neutral Current (NC) &Charged Current (CC) Cross Sections

Structure Functions (SFs) Electroweak Parameters Polarization Pe

(HERA-II only)

Parton Distribution Functions(PDFs)

This talk

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1993 :Very first electroweak result at HERA from 0.3 pb-1

HERA total CC cross section converted to equivalent neutrino cross section

Fixed targetNeutrino experiments

HERA

0

50

100

150

0 50 100 150 200

this expt.σ (p

⊥>

25 G

eV)

pb

GeV

Mprop

H�

−310 −210 −110 010 110 2100.01

0.1

1

10

100

1000

�tot

�N

pb

nucleon

H�

TeV

E�

First evidence of W-Propagator effect in Charged Current DIS

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Joachim Meyer Ringberg 2005 6

Measured NC and CC cross sections

NC

CC

Suppressed due to large mass of W boson compared to NC DIS

Electro-Weak unification at high Q2

High Q2 results statistics limited !

HERA I Data 1994 – 2000 (100 pb-1 per experiment)

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Kinematics :

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CC Cross Section

s)](dy)(1cu[)QM

M(x 4π

GdxdQ

p)(eσd 2222

W

2W

2F

2

CC2

+−+++

=+

e+p

)]sd(y)(1c[u)QM

M(x 4π

GdxdQ

p)(eσd 2222

W

2W

2F

2

CC2

+−+++

=−

e-p

Joachim Meyer Ringberg 2005 8

10-7

10-6

10-5

10-4

10-3

10-2

10-1

1

103

104

HERA Charged Current

H1 e+p 94-00

ZEUS e+p 99-00

SM e+p (CTEQ6D)

H1 e-p

ZEUS e-p 98-99

SM e-p (CTEQ6D)

y < 0.9

Q2 (GeV2)

dσ/

dQ

2 (p

b/G

eV2 )

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HERA-I Results : Combined EW+PDF Fit (H1)

The low Q2 precision cross section data +the high Q2 NC e+p & e-p data +the high Q2 CC e+p & e-p data

gluon, up-type quark, down-type quark & their anti-quarks

constrain 5 sets of PDFs:

• NC data at high Q2 also sensitive to quark couplings to the Z boson

• CC data also sensitive to G, W propagator mass [model independent]MW, mt [within the SM framework]

)PDFs()MQ(

Mx2

GQdxd

)pe(d2W

2 2

4W

2F

2CC

+π=σ ±

aq, vq (q=u, d)

Joachim Meyer Ringberg 2005 10

W

GF

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Combined EW+PDF Analysis Strategies

Model independent fits:1) Fit au-vu-ad-vd-PDF

to extract light quark couplings to the Z boson

2) Fit G-Mprop-PDFto determine the normalization factor G and W propagator mass Mprop

3) Fit Mprop-PDF [fix G to GF]to determine the W propagator mass Mprop

Fits within the SM framework:

4) Fit MW-PDF [fix mt to 178GeV, MH to 120GeV]to determine the SM W mass MW

5) Fit mt-PDF [fix MW to 80.425GeV, MH to 120GeV]to determine the top quark mass mt

r11

M2G

2Z

2W

MM

1W2

2F ∆−

πα=⎟⎟⎠

⎞⎜⎜⎝

⎛−

∆r contains - quadratic dependence on mt- logarithmic dependence on MH

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First Results on Light Quark Couplings to Z at HERA

H1

68% CL

vu-au-vd-ad-PDF

Standard ModelCDF

LEP EWWG preliminary (Feb. 05)

au

v u

-1

-0.5

0

0.5

1

-1 -0.5 0 0.5 1

H1

68% CL

vu-au-vd-ad-PDF

Standard Model

CDFLEP EWWG preliminary (Feb. 05)

adv d

-1

-0.5

0

0.5

1

-1 -0.5 0 0.5 1

SM :

Tevatron: qq ee Drell-Yan, AFB: CDF Collab., Phys. Rev. D71(2005)052002, hep-ex/0411059LEP: ee qq(γ) [a2

q+v2q]: http://lepewwg.web.cern.ch/LEPEWWG/plots/winter2005/

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With GF from PDG :

MProp= 82.9 +- 1.9 GeV

W Propagator Mass and Coupling

0.115

0.12

0.125

x 10-4

75 80 85 90

68% CL

G-Mprop-PDF

Mprop-PDF (G=GF)

World Average

H1

Mprop (GeV)

G (

GeV

−2)

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Improved Precision on W Propagator Mass

H1 e+p 94-97

ZEUS e+p 99-00

H1 e-p 98-99

ZEUS e+p 94-97

ZEUS e-p 98-99

H1 94-00 (this analysis)

HERA measurement of W propagator mass

Mw (GeV)

76 78 80 82 84 86 88 90 92

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Fits Imposing the SM Constraints

22 22

2 2 2

d ( )d d 2

W

W

CC MM

G pdfsx Q Qπσ ±

±⎛ ⎞= ⋅ ⋅Φ⎜ ⎟+⎝ ⎠

( )

22 22

2 22 2 224

2

d 1 ( )d d 1

4 1

WCC

W

Z

WW

pdfsx Q Q

MM

MM

rM

πασ ±±⎛ ⎞

= ⋅ ⋅ ⋅Φ⎜ ⎟+− ∆⎛ ⎞ ⎝ ⎠−⎜ ⎟

⎝ ⎠

Introducing SM GF-MW relationin On-Mass-Shell (OMS) scheme

Quadratic dependence on mt Logarithmic dependence on MH

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∆χ2=1 (MH=120GeV)

∆χ2=1 (MH=300GeV)

mt world average

MW world average

H1

mt (GeV)

MW

(GeV

)

80

80.5

81

81.5

100 150 200

Determination of SM Parameters

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W mass value:MW=80.786 ± 0.205exp GeV

+ the world average MZindirect determination of

sin2θW=1−M2W/M2

Z=0.2151 ± 0.0040exp

Using MW (PDG) restrictstop quark mass

mt=104 ± 44exp GeVFirst determination in DIS at EW scale

178±4.3 GeV80.425±0.038 GeV

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HERA II

• Substantial increase in luminosity• Longitudinally polarized lepton beams

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Luminosity at HERA-IIHigh Luminosity → sensitivity in High-Q2 region

2005

2003-2004

1992-2000

Luminosity used for physics analysis per experiment :

HERA-I : 100pb-1(e+p), 20pb-1(e-p)

HERA-II : 40pb-1(e+p), 100pb-1(e-p)

By the end of the HERA-II in July 2007,

expect ~700pb-1

per experiment

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Data samples

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P < 0 (LH) P > 0 (RH)e+p data L = 21.7 pb–1

P = – 40.2 %L = 15.3 pb–1

P = + 33.0 %e–p data L = 17.8 pb–1

P = – 25.4 %

P < 0 (LH) P > 0 (RH)

e+p data L = 16.4 pb–1

P = – 40.2 %L = 14.1 pb–1

P = + 31.8 %

e–p data L = 35.3 pb–1

P = – 25.9 %L = 6.5 pb–1

P = + 29.2 %

e-p

e+pH1 data samples

ZEUS data samples

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Charged current physicsat HERA II

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CC Total Cross-Section (H1)Q2>400GeV2, y<0.9

e+p

Remind : CC is pure weak

Direct observation of chiralstructure of weak interaciton

A clear linear dependence is observed both e+ and e-

Data are in agreement with the SM prediction

0)(P)σP(1)(Pσ eCCeeCC =±= ±±±

pb pb

.)(94.0.)(04.180.13%)40(

.)(66.1.)(94.167.34%)33(syststatPsyststatP

eCC

eCC

±±=−=±±=+=

σσ

Joachim Meyer Ringberg 2005 21e-p pb .)(99.2.)(39.242.66%)25( syststatPeCC ±±=−=σ

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The polarization dependence of CC – DIS scattering has already been measured in 1979 at the CERN Neutrino beam. (Phys.Lett. B86 ; 222 (1979))

Neutrino Interaction inCDHS Detector

Measurement of muon longitudinalPolarization in CHARM detector

Result :

The longitudinal Polarisation of the positive muons is P = + 1.09 +- 0.22

(at an average momentum transfer 3.2 GeV2 !!!)

RighthandedAntineutrino

RighthandedPositive Muon

History:

!

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e+ e-

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Neutral current physicsAt HERA II

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NC & CC Cross Sections Dependence on Polarization Pe

For NC: emcontributiondominating at low Q2 isindependentof Pe. weak NC onlysignificant at high Q2

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Outlook HERA II is expected to deliver approx 700 pb-1 toeach experiment. There will be an equal share ofe+ and e-, left- and righthanded polarized.

More precise checks of electroweak SM possible : • Better MW determination (spacelike Propagatormass)• More precise Z0 couplings to light quarks

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HERA Physics workshop studies : W - Propagator Mass

H1 Result :

HERA I (100 pb-1 , unpol.) :

Mprop = 82.9 +- 1.9 GeV

MW = 80.8 +- 0.2 GeV

Precise check of EW theory when combined with Mtop from Tevatron (LHC)

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HERA Physics workshop studies : Light Quark Couplings to Z0

H1 RESULT :

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Conclusion• With approx. 200 pb-1 significant tests of the

SM electroweak sector at high spacelikemomentum transfers have been performed :-Electroweak unification, CC-Propagator mass,-Light quark Z0 couplings, CC-chiral structure,-NC polarisation dependences

• A factor 3 more luminosity still to come at HERA IIand the availibility of longitudinally polarized electrons and positrons will significantly enhancethe sensitivity of these SM tests.

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Despite ‘HERA is a QCD machine’ there are alsointeresting electroweak results which I hope justify the conference logo …

Many thanks foryour attention

Thanks to my colleagues from Zeus and H1 for supplying some of these slides

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