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Our Understanding of Sea Quarks in the Nucleon Wen-Chen Chang 章章章 Institute of Physics, Academia Sinica Weekly Journal Club for Medium Energy Physics at IPAS 2011/1/10

Our Understanding of Sea Quarks in the Nucleon

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Weekly Journal Club for Medium Energy Physics at IPAS 2011/1/10. Our Understanding of Sea Quarks in the Nucleon. Wen-Chen Chang 章文箴 Institute of Physics, Academia Sinica. Inelastic Electron Scattering. Q 2 : Four-momentum transfer x : Bjorken variable (=Q 2 /2 M n ) - PowerPoint PPT Presentation

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Page 1: Our Understanding of  Sea Quarks in the Nucleon

Our Understanding of Sea Quarks in the Nucleon

Wen-Chen Chang 章文箴Institute of Physics, Academia Sinica

Weekly Journal Club for Medium Energy Physics at IPAS 2011/1/10

Page 2: Our Understanding of  Sea Quarks in the Nucleon

2

Q2 :Four-momentum transferx : Bjorken variable (=Q2/2M) : Energy transferM : Nucleon massW : Final state hadronic mass

Inelastic Electron Scattering

Page 3: Our Understanding of  Sea Quarks in the Nucleon

Structure Function F2(Q2,x)

3

Page 4: Our Understanding of  Sea Quarks in the Nucleon

J. G. Contreras CTEQ School 2005

4

Describing F2 behavior with partons

Lots of partons at small x!

Page 5: Our Understanding of  Sea Quarks in the Nucleon

5

Unpolarized Parton Distributions (CTEQ6)

u valence

sea (x 0.05)

gluon (x 0.05)

d

Page 6: Our Understanding of  Sea Quarks in the Nucleon

What is Origin of Sea Quarks?

• Extrinsic: the sea quarks solely originate from the splitting of gluons, emitted by valence quarks.

6

Page 7: Our Understanding of  Sea Quarks in the Nucleon

7

Is in the proton?

Gottfried Sum Rule Gottfried Sum Rule 1

2 20

1

0

[( ( ) ( )) / ]

1 2( ( ) ( ))

3 3

( )1

3 p p

p nG

p p

S F x F x x dx

u x d

i

x dx

f u d

=

du

Page 8: Our Understanding of  Sea Quarks in the Nucleon

8

Experimental Measurement of Gottfried Sum

New Muon Collaboration (NMC), Phys. Rev. D50 (1994) R1

SG = 0.235 ± 0.026

( Significantly lower than 1/3 ! )

Page 9: Our Understanding of  Sea Quarks in the Nucleon

9

Explanations for the NMC result

• Uncertain extrapolation for 0.0 < x < 0.004

• Charge symmetry violation

• in the proton

• Uncertain extrapolation for 0.0 < x < 0.004

• Charge symmetry violation

• in the proton

,( )n p n pu d d u ( ) ( )u x d x

1

0( ( ) ( )) 0.148 0.04d x u x dx

Need independent methods to check the

asymmetry, and to measure its x-dependence !

Need independent methods to check the

asymmetry, and to measure its x-dependence !

d u

Page 10: Our Understanding of  Sea Quarks in the Nucleon

10

xtarget xbeam

Detector acceptance chooses xtarget and xbeam.

Fixed target high xF = xbeam – xtarget

Beam nucleon: valence quarks at high-x. Target nucleon: sea quarks at low/intermediate-x. Measure ratio of DY process from hydrogen and deuterium:

Drell-Yan process: A laboratory for sea quarks

)2(

)2(1

2

1

)2(

)2(1

)2(

)2()1(4)1(

1

)1(4)1(

1

2

1|

221

xu

xd

xu

xd

xu

xdxuxd

xuxd

xxpp

pd

Page 11: Our Understanding of  Sea Quarks in the Nucleon

11

Light Antiquark Flavor Asymmetry: Brief History Naïve Assumption:

NA51 (Drell-Yan, 1994)

NMC (Gottfried Sum Rule)

NA 51 Drell-Yan confirms

d(x) > u(x)

NA 51 Drell-Yan confirms

d(x) > u(x)

Page 12: Our Understanding of  Sea Quarks in the Nucleon

12

Light Antiquark Flavor Asymmetry: Brief History Naïve Assumption:

NA51 (Drell-Yan, 1994)

E866/NuSea (Drell-Yan, 1998)

NMC (Gottfried Sum Rule)

Page 13: Our Understanding of  Sea Quarks in the Nucleon

13

Advantages of 120 GeV Main InjectorThe (very successful) past:

Fermilab E866/NuSeaFermilab E866/NuSea Data in 1996-1997 1H, 2H, and nuclear targets 800 GeV proton beam

The future:

Fermilab E906Fermilab E906 Data taking planned in 2010 1H, 2H, and nuclear targets 120 GeV proton Beam

Cross section scales as 1/s – 7x that of 800 GeV beam

Backgrounds, primarily from J/ decays scale as s– 7x Luminosity for same detector

rate as 800 GeV beam

50x statistics!!50x statistics!!

Fixed Target

Beam lines

Tevatron 800 GeV

Main Injector

120 GeV

Page 14: Our Understanding of  Sea Quarks in the Nucleon

14

Extracting d-bar/-ubar From Drell-Yan ScatteringRatio of Drell-Yan cross sections

(in leading order—E866 data analysis confirmed in NLO)

Global NLO PDF fits which include E866 cross section ratios agree with E866 results

Fermilab E906/Drell-Yan will extend these measurements and reduce statistical uncertainty.

E906 expects systematic uncertainty to remain at approx. 1% in cross section ratio.

Page 15: Our Understanding of  Sea Quarks in the Nucleon

Deep-Inelastic Neutrino Scattering

15

)]()()()([2)(2 xcxsxuxdxxF p

)]()()()([2)(2 xcxsxdxuxxF n

Page 16: Our Understanding of  Sea Quarks in the Nucleon

Adler Sum Rule

16

2)]()([2)],(),([1

0

1

0

22

22 dxxdxu

x

dxQxFQxF VV

pn

Page 17: Our Understanding of  Sea Quarks in the Nucleon

Strange Quark and Anti-quark in the Nucleon

17CCFR, Z. Phys. C 65, 189 (1995)CCFR, Z. Phys. C 65, 189 (1995)

scXcN ;

)(*5.0)( duss

)()( xsxs

Page 18: Our Understanding of  Sea Quarks in the Nucleon

Strange Quark and Antiquark in the Nucleon

18NuTeV, PRL 99, 192001 (2007)NuTeV, PRL 99, 192001 (2007)

Page 19: Our Understanding of  Sea Quarks in the Nucleon

19

Semi-inclusive DIS

Page 20: Our Understanding of  Sea Quarks in the Nucleon

Strange Quarks from Charged-Kaon DIS Production

20HERMES, Phys. Lett. B 666, 446 (2008)HERMES, Phys. Lett. B 666, 446 (2008)

Page 21: Our Understanding of  Sea Quarks in the Nucleon

Asymmetry of W Production and Flavor Asymmetry of Nucleon Sea

21

Yang, Peng, and Groe-Perdekam,Phys. Lett. B 680, 231 (2009)Yang, Peng, and Groe-Perdekam,Phys. Lett. B 680, 231 (2009)

p+p at sqrt(s)=14 TeVp+p at sqrt(s)=14 TeV

Page 22: Our Understanding of  Sea Quarks in the Nucleon

CMS Measurement of W Asymmetry at sqrt(s)=7 TeV

22CMS, arXiv:1012.2466 CMS, arXiv:1012.2466

Measured W-asymmetry is consistent with the prediction from the PDF with a flavor asymmetry of sea quarks.Measured W-asymmetry is consistent with the prediction from the PDF with a flavor asymmetry of sea quarks.

Page 23: Our Understanding of  Sea Quarks in the Nucleon

Origin of u(x)d(x): Valence quark effect?

• Pauli blocking

– guu is more suppressed than gdd in the proton since p=uud (Field and Feynman 1977)

– pQCD calculation (Ross Sachrajda)

– Bag model calculation (Signal, Thomas, Schreiber)

• Chiral quark-soliton model (Diakonov, Pobylitsa, Polyakov)

• Instanton model (Dorokhov, Kochelev)

• Statistical model (Bourrely, Buccella, Soffer; Bhalerao)

• Balance model (Zhang, Ma)

23

The valence quarks affect the Dirac vacuum and the quark-antiquark sea.The valence quarks affect the Dirac vacuum and the quark-antiquark sea.

Page 24: Our Understanding of  Sea Quarks in the Nucleon

24

Balance Model

A physical hadron state is expanded by a complete set of quark-gluon Fock states

The parton numbers of quarks and gluons in the proton are

•Splitting and recombination

qqg gqqbar

Page 25: Our Understanding of  Sea Quarks in the Nucleon

Balance Model (Phys. Lett. B 523 (2001) 260-264)

25

More u valence quark in the proton leads to more recombination and thus less ubar.Inclusion of gqqbar does not affect the result of flavor asymmetry.

More u valence quark in the proton leads to more recombination and thus less ubar.Inclusion of gqqbar does not affect the result of flavor asymmetry.

Page 26: Our Understanding of  Sea Quarks in the Nucleon

Origin of u(x)d(x): Non-perturbative effect?

• Meson cloud in the nucleons (Thomas, Kumano): Sullivan process in DIS.

• Chiral quark model (Eichten, Hinchliffe, Quigg; Wakamatsu): Goldstone bosons couple to valence quarks.

26

The pion cloud is a source of antiquarks in the protons and it lead to d>u.The pion cloud is a source of antiquarks in the protons and it lead to d>u.

Page 27: Our Understanding of  Sea Quarks in the Nucleon

27

Meson Cloud Model

Virtual is emitted by the proton and the intermediate state is + baryons.

0:1:2:: , 0 Np

0

00

0000

00 |6

1|

3

1|

2

1|

3

2|

3

1|1| bnpapbap

Page 28: Our Understanding of  Sea Quarks in the Nucleon

28

Chiral Quark Model

Virtual is emitted by the constituent quark.

2:3:4:: , 0 qq

dua y probabilit splitting the:

Page 29: Our Understanding of  Sea Quarks in the Nucleon

24 February 2010

Paul E. Reimer, Physics Division, Argonne National Laboratory

29

Proton Structure: Remove perturbative sea There is a gluon splitting component

which is symmetric

– Symmetric sea via pair production from

gluons subtracts off– No Gluon contribution at 1st order in s

– Nonperturbative models are motivated by the observed difference

A proton with 3 valence quarks plus glue cannot be right at any scale!!

Greater deviation at large-x

Page 30: Our Understanding of  Sea Quarks in the Nucleon

Intrinsic Sea Quark?

• Brodsky et al. (1980) proposed an “intrinsic” (long time-scale) charm component in the proton (PLB 93,451; PRD 23, 2745).

• A decomposition of |uudccbar> Fock state for proton. The intrinsic charm component is distributed at relatively large x region and could explain the large cross-section for charm production at large xf in hadron collisions.

• Jen-Chieh and I are considering to extend this 5q model to describe the non-singlet distributions of (dbar-ubar) and (ubar+dbar-s-sbar), which are independent of the contributions from “extrinsic” sea quarks.

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Page 31: Our Understanding of  Sea Quarks in the Nucleon

Sea quarks in

31

cuudc|

5

1

22

2

5

151

)(

)1(),...,(

i i

ip

ii

xm

m

xNxxP

GeV 3/938.0

GeV 5.1

,

du

c

m

m

Page 32: Our Understanding of  Sea Quarks in the Nucleon

Sea quarks in

32

suuds|

GeV 3/938.0

GeV 5.0

,

du

s

m

m

Page 33: Our Understanding of  Sea Quarks in the Nucleon

Sea quarks in

33

uuudu|

GeV 3/938.0, dum

Page 34: Our Understanding of  Sea Quarks in the Nucleon

Sea quarks in

34

uuudu|

The light quark distribution in 5q configuration, which is assumed to be intrinsic,is consistent with the non-singlet distribution of (dbar-ubar). The light quark distribution in 5q configuration, which is assumed to be intrinsic,is consistent with the non-singlet distribution of (dbar-ubar).

GeV 3/938.0, dum

Page 35: Our Understanding of  Sea Quarks in the Nucleon

Sea quarks in

35

uuudu|

GeV 3/938.0, dum

Page 36: Our Understanding of  Sea Quarks in the Nucleon

W production at the LHC is sensitive to the gluon distribution function.

Tevatron: W production is dominated by a LO process with two valence quarks.

LHC: The LO contribution must involve a sea quark; and the NLO contribution from a gluon is significant.

Page 37: Our Understanding of  Sea Quarks in the Nucleon

?

Page 38: Our Understanding of  Sea Quarks in the Nucleon

Interesting Topics Missing in This Talk

• Transverse spin structure of sea quarks.

• Transverse momentum distribution of sea quarks.

• The correlation of these two properties.

• Flavor asymmetry of these two properties.

• Interpretations from the Lattice QCD.

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Page 39: Our Understanding of  Sea Quarks in the Nucleon

Conclusion• From DIS, DY and SIDIS processes, the structure of sea

quarks in the nucleon are explored.• A large asymmetry between dbar and ubar was found at

intermediate-x regions. The origin can be interpreted under the meson cloud model, chiral soliton model, intrinsic 5q model and etc. The intrinsic non-perturbative effect rather than extrinsic perturbative gluon-splitting seems more likely to be the cause.

• No large asymmetry was observed for s and sbar. • The E906/FNAL and LHC experiments are expected to extend

the measurement of sea quarks to the high-x regions where the existing uncertainties are large.

• Precise understanding of sea quark distribution is important for the search of BSM in LHC.

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Page 40: Our Understanding of  Sea Quarks in the Nucleon

References

• C. Grosso-Pilcher and M. J. Shochet, Annu. Rev. Nucl. Part. Sci. 36 (1986) 1.

• S. Kumano, Physics Reports 303 (1998) 183.• J.M. Conrad and M.H. Shaevitz, Rev. Mod. Phys. 70

(1998) 1341.• P.L. McGaughey, J.M. Moss and J.C. Peng, Annu. Rev.

Nucl. Part. Sci. 49 (1999) 217.• G.T. Garvey and J.C. Peng, Prog. in Part. And Nucl. Phys.

47 (2001) 203.• J.C. Peng, Eur. Phys. J. A 18 (2003) 395.• J.T. Londergan, J.C. Peng, and A.W. Thomas, Rev. Mod.

Phys. 82 (2010) 2009.

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