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T(r)opical Dyson Schwinger Equations Craig D. Roberts Physics Division Argonne National Laboratory & School of Physics Peking University & Department of Physics Transition Region

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T(r) opical Dyson Schwinger Equations. Craig D. Roberts Physics Division Argonne National Laboratory & School of Physics Peking University & Department of Physics. Transition Region. Universal Truths. - PowerPoint PPT Presentation

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Page 1: T(r) opical  Dyson Schwinger Equations

T(r)opical Dyson Schwinger EquationsCraig D. Roberts

Physics DivisionArgonne National Laboratory

&School of PhysicsPeking University

&Department of Physics

Transition Region

Page 2: T(r) opical  Dyson Schwinger Equations

Universal Truths

Spectrum of hadrons (ground, excited and exotic states), and hadron elastic and transition form factors provide unique information about long-range interaction between light-quarks and distribution of hadron's characterising properties amongst its QCD constituents.

Craig Roberts, Physics Division, Argonne National Laboratory

2

Page 3: T(r) opical  Dyson Schwinger Equations

Universal Truths

Spectrum of hadrons (ground, excited and exotic states), and hadron elastic and transition form factors provide unique information about long-range interaction between light-quarks and distribution of hadron's characterising properties amongst its QCD constituents.

Dynamical Chiral Symmetry Breaking (DCSB) is most important mass generating mechanism for visible matter in the Universe.

Craig Roberts, Physics Division, Argonne National Laboratory

3

Page 4: T(r) opical  Dyson Schwinger Equations

Universal Truths

Spectrum of hadrons (ground, excited and exotic states), and hadron elastic and transition form factors provide unique information about long-range interaction between light-quarks and distribution of hadron's characterising properties amongst its QCD constituents.

Dynamical Chiral Symmetry Breaking (DCSB) is most important mass generating mechanism for visible matter in the Universe.

Higgs mechanism is irrelevant to light-quarks.

Craig Roberts, Physics Division, Argonne National Laboratory

4

Page 5: T(r) opical  Dyson Schwinger Equations

Universal Truths

Spectrum of hadrons (ground, excited and exotic states), and hadron elastic and transition form factors provide unique information about long-range interaction between light-quarks and distribution of hadron's characterising properties amongst its QCD constituents.

Dynamical Chiral Symmetry Breaking (DCSB) is most important mass generating mechanism for visible matter in the Universe.

Higgs mechanism is irrelevant to light-quarks. Dynamical Chiral Symmetry Breaking (DCSB) is most important mass generating

mechanism for visible matter in the Universe.

Craig Roberts, Physics Division, Argonne National Laboratory

5

Page 6: T(r) opical  Dyson Schwinger Equations

Universal Truths

Spectrum of hadrons (ground, excited and exotic states), and hadron elastic and transition form factors provide unique information about long-range interaction between light-quarks and distribution of hadron's characterising properties amongst its QCD constituents.

Dynamical Chiral Symmetry Breaking (DCSB) is most important mass generating mechanism for visible matter in the Universe.

Higgs mechanism is irrelevant to light-quarks. Dynamical Chiral Symmetry Breaking (DCSB) is most important mass generating

mechanism for visible matter in the Universe. Covariance requires existence of quark orbital angular momentum in hadron's rest-frame wave function.

Craig Roberts, Physics Division, Argonne National Laboratory

6

Page 7: T(r) opical  Dyson Schwinger Equations

Universal Truths

Spectrum of hadrons (ground, excited and exotic states), and hadron elastic and transition form factors provide unique information about long-range interaction between light-quarks and distribution of hadron's characterising properties amongst its QCD constituents.

Dynamical Chiral Symmetry Breaking (DCSB) is most important mass generating mechanism for visible matter in the Universe.

Higgs mechanism is irrelevant to light-quarks. Dynamical Chiral Symmetry Breaking (DCSB) is most important mass generating

mechanism for visible matter in the Universe. Covariance requires existence of quark orbital angular momentum in hadron's rest-frame wave function.

Confinement is expressed through a violation of reflection positivity; and can almost be read-off from a plot of a states’ dressed-propagator. It is intimately connected with DCSB.

Craig Roberts, Physics Division, Argonne National Laboratory

7

Page 8: T(r) opical  Dyson Schwinger Equations

Universal Truths

Challenge: understand relationship between parton properties on the light-front and rest frame structure of hadrons.

Craig Roberts, Physics Division, Argonne National Laboratory

8

Page 9: T(r) opical  Dyson Schwinger Equations

In-Hadron Condensates

Challenge: understand relationship between parton properties on the light-front and rest frame structure of hadrons.

One problem: DCSB - an established keystone of low-energy QCD and the origin of constituent-quark masses - has not yet been realised in the light-front formulation.

Craig Roberts, Physics Division, Argonne National Laboratory

9

Page 10: T(r) opical  Dyson Schwinger Equations

In-Hadron Condensates

Challenge: understand relationship between parton properties on the light-front and rest frame structure of hadrons.

One problem: DCSB - an established keystone of low-energy QCD and the origin of constituent-quark masses - has not yet been realised in the light-front formulation.

Resolution– Whereas it might sometimes be convenient in computational truncation

schemes to imagine otherwise, “condensates” do not exist as spacetime-independent mass-scales that fill all spacetime.

– So-called vacuum condensates can be understood as a property of hadrons themselves, which is expressed, for example, in their Bethe-Salpeter or light-front wavefunctions.

Craig Roberts, Physics Division, Argonne National Laboratory

10

Page 11: T(r) opical  Dyson Schwinger Equations

In-Hadron Condensates

B Resolution

– Whereas it might sometimes be convenient in computational truncation schemes to imagine otherwise, “condensates” do not exist as spacetime-independent mass-scales that fill all spacetime.

– So-called vacuum condensates can be understood as a property of hadrons themselves, which is expressed, for example, in their Bethe-Salpeter or light-front wavefunctions.

– No qualitative difference between fπ and ρπ

Craig Roberts, Physics Division, Argonne National Laboratory

11

Brodsky, Roberts, Shrock, Tandy, Phys. Rev. C82 (Rapid Comm.) (2010) 022201

Page 12: T(r) opical  Dyson Schwinger Equations

In-Hadron Condensates

B Resolution

– Whereas it might sometimes be convenient in computational truncation schemes to imagine otherwise, “condensates” do not exist as spacetime-independent mass-scales that fill all spacetime.

– So-called vacuum condensates can be understood as a property of hadrons themselves, which is expressed, for example, in their Bethe-Salpeter or light-front wavefunctions.

– No qualitative difference between fπ and ρπ

– And

Craig Roberts, Physics Division, Argonne National Laboratory

12

Brodsky, Roberts, Shrock, Tandy, Phys. Rev. C82 (Rapid Comm.) (2010) 022201

Page 13: T(r) opical  Dyson Schwinger Equations

In-Hadron Condensates

B Resolution

– Whereas it might sometimes be convenient in computational truncation schemes to imagine otherwise, “condensates” do not exist as spacetime-independent mass-scales that fill all spacetime.

– So-called vacuum condensates can be understood as a property of hadrons themselves, which is expressed, for example, in their Bethe-Salpeter or light-front wavefunctions.

– Conjecture: Light-Front DCSB obtained via coherent contribution from countable infinity of higher Fock-state components in LF-wavefunction.

Craig Roberts, Physics Division, Argonne National Laboratory

13

Brodsky, Roberts, Shrock, Tandy, Phys. Rev. C82 (Rapid Comm.) (2010) 022201

Page 14: T(r) opical  Dyson Schwinger Equations

In-Hadron Condensates

“EMPTY space may really be empty. Though quantum theory suggests that a vacuum should be fizzing with particle activity, it turns out that this paradoxical picture of nothingness may not be needed. A calmer view of the vacuum would also help resolve a nagging inconsistency with dark energy, the elusive force thought to be speeding up the expansion of the universe.”

Cosmological Constant: – Putting QCD condensates back into hadrons reduces the mismatch

between experiment and theory by a factor of 1045

– Possibly by far more, if technicolour-like theories are the correct paradigm for extending the Standard Model

Craig Roberts, Physics Division, Argonne National Laboratory

14

“Void that is truly empty solves dark energy puzzle”Rachel Courtland, New Scientist 1st Sept. 2010

Page 15: T(r) opical  Dyson Schwinger Equations

Charting the interaction between light-quarks

Confinement can be related to the analytic properties of QCD's Schwinger functions.

Craig Roberts, Physics Division, Argonne National Laboratory

15

Page 16: T(r) opical  Dyson Schwinger Equations

Charting the interaction between light-quarks

Confinement can be related to the analytic properties of QCD's Schwinger functions.

Question of light-quark confinement can be translated into the challenge of charting the infrared behavior of QCD's universal β-function– This function may depend on the scheme chosen to renormalise the

quantum field theory but it is unique within a given scheme.

Of course, the behaviour of the β-function on the perturbative domain is well known.

Craig Roberts, Physics Division, Argonne National Laboratory

16

Page 17: T(r) opical  Dyson Schwinger Equations

Charting the interaction between light-quarks

Confinement can be related to the analytic properties of QCD's Schwinger functions.

Question of light-quark confinement can be translated into the challenge of charting the infrared behavior of QCD's universal β-function– This function may depend on the scheme chosen to renormalise the

quantum field theory but it is unique within a given scheme.Of course, the behaviour of the β-function on the perturbative domain is well known.

This is a well-posed problem whose solution is an elemental goal of modern hadron physics.

Craig Roberts, Physics Division, Argonne National Laboratory

17

Page 18: T(r) opical  Dyson Schwinger Equations

Charting the interaction between light-quarks

Through QCD's Dyson-Schwinger equations (DSEs) the pointwise behaviour of the β-function determines pattern of chiral symmetry breaking.

Craig Roberts, Physics Division, Argonne National Laboratory

18

Page 19: T(r) opical  Dyson Schwinger Equations

Charting the interaction between light-quarks

Through QCD's Dyson-Schwinger equations (DSEs) the pointwise behaviour of the β-function determines pattern of chiral symmetry breaking.

DSEs connect β-function to experimental observables. Hence, comparison between computations and observations ofo Hadron mass spectrumo Elastic and transition form factorscan be used to chart β-function’s long-range behaviour.

Craig Roberts, Physics Division, Argonne National Laboratory

19

Page 20: T(r) opical  Dyson Schwinger Equations

Charting the interaction between light-quarks

Through QCD's Dyson-Schwinger equations (DSEs) the pointwise behaviour of the β-function determines pattern of chiral symmetry breaking.

DSEs connect β-function to experimental observables. Hence, comparison between computations and observations ofo Hadron mass spectrumo Elastic and transition form factorscan be used to chart β-function’s long-range behaviour.

Extant studies of mesons show that the properties of hadron excited states are a great deal more sensitive to the long-range behaviour of the β-function than those of the ground states.

Craig Roberts, Physics Division, Argonne National Laboratory

20

Page 21: T(r) opical  Dyson Schwinger Equations

Charting the interaction between light-quarks

Through QCD's Dyson-Schwinger equations (DSEs) the pointwise behaviour of the β-function determines pattern of chiral symmetry breaking.

DSEs connect β-function to experimental observables. Hence, comparison between computations and observations can be used to chart β-function’s long-range behaviour.

To realise this goal, a nonperturbative symmetry-preserving DSE truncation is necessary:o Steady quantitative progress is being made with a scheme that is

systematically improvable (Bender, Roberts, von Smekal – nucl-th/9602012)

Craig Roberts, Physics Division, Argonne National Laboratory

21

Page 22: T(r) opical  Dyson Schwinger Equations

Charting the interaction between light-quarks

Through QCD's Dyson-Schwinger equations (DSEs) the pointwise behaviour of the β-function determines pattern of chiral symmetry breaking.

DSEs connect β-function to experimental observables. Hence, comparison between computations and observations can be used to chart β-function’s long-range behaviour.

To realise this goal, a nonperturbative symmetry-preserving DSE truncation is necessary:o On the other hand, at significant qualitative advances are possible with

symmetry-preserving kernel Ansätze that express important additional nonperturbative effects – M(p2) – difficult/impossible to capture in any finite sum of contributions.

Craig Roberts, Physics Division, Argonne National Laboratory

22

Can’t walk beyond the rainbow, but must leap!

Page 23: T(r) opical  Dyson Schwinger Equations

Frontiers of Nuclear Science:Theoretical Advances

In QCD a quark's effective mass depends on its momentum. The function describing this can be calculated and is depicted here. Numerical simulations of lattice QCD (data, at two different bare masses) have confirmed model predictions (solid curves) that the vast bulk of the constituent mass of a light quark comes from a cloud of gluons that are dragged along by the quark as it propagates. In this way, a quark that appears to be absolutely massless at high energies (m =0, red curve) acquires a large constituent mass at low energies.

Craig Roberts, Physics Division, Argonne National Laboratory

23

Page 24: T(r) opical  Dyson Schwinger Equations

Frontiers of Nuclear Science:Theoretical Advances

In QCD a quark's effective mass depends on its momentum. The function describing this can be calculated and is depicted here. Numerical simulations of lattice QCD (data, at two different bare masses) have confirmed model predictions (solid curves) that the vast bulk of the constituent mass of a light quark comes from a cloud of gluons that are dragged along by the quark as it propagates. In this way, a quark that appears to be absolutely massless at high energies (m =0, red curve) acquires a large constituent mass at low energies.

Craig Roberts, Physics Division, Argonne National Laboratory

24

DSE prediction of DCSB confirmed

Page 25: T(r) opical  Dyson Schwinger Equations

Frontiers of Nuclear Science:Theoretical Advances

In QCD a quark's effective mass depends on its momentum. The function describing this can be calculated and is depicted here. Numerical simulations of lattice QCD (data, at two different bare masses) have confirmed model predictions (solid curves) that the vast bulk of the constituent mass of a light quark comes from a cloud of gluons that are dragged along by the quark as it propagates. In this way, a quark that appears to be absolutely massless at high energies (m =0, red curve) acquires a large constituent mass at low energies.

Craig Roberts, Physics Division, Argonne National Laboratory

25

Hint of lattice-QCD supportfor DSE prediction of violation of reflection positivity

Page 26: T(r) opical  Dyson Schwinger Equations

Frontiers of Nuclear Science:Theoretical Advances

In QCD a quark's effective mass depends on its momentum. The function describing this can be calculated and is depicted here. Numerical simulations of lattice QCD (data, at two different bare masses) have confirmed model predictions (solid curves) that the vast bulk of the constituent mass of a light quark comes from a cloud of gluons that are dragged along by the quark as it propagates. In this way, a quark that appears to be absolutely massless at high energies (m =0, red curve) acquires a large constituent mass at low energies.

Craig Roberts, Physics Division, Argonne National Laboratory

26

Jlab 12GeV: Scanned by 2<Q2<9 GeV2 elastic & transition form factors.

Page 27: T(r) opical  Dyson Schwinger Equations

Gap EquationGeneral Form

Craig Roberts, Physics Division, Argonne National Laboratory

27

Page 28: T(r) opical  Dyson Schwinger Equations

Gap EquationGeneral Form

Dμν(k) – dressed-gluon propagator Γν(q,p) – dressed-quark-gluon vertex

Craig Roberts, Physics Division, Argonne National Laboratory

28

Page 29: T(r) opical  Dyson Schwinger Equations

Gap EquationGeneral Form

Dμν(k) – dressed-gluon propagator Γν(q,p) – dressed-quark-gluon vertex Suppose one has in hand – from anywhere – the exact

form of the dressed-quark-gluon vertex

What is the associated symmetry-preserving Bethe-Salpeter kernel?!

Craig Roberts, Physics Division, Argonne National Laboratory

29

Page 30: T(r) opical  Dyson Schwinger Equations

Bethe-Salpeter EquationBound-State DSE

K(q,k;P) – fully amputated, two-particle irreducible, quark-antiquark scattering kernel

Textbook material. Compact. Visually appealing. Correct

Craig Roberts, Physics Division, Argonne National Laboratory

30

Page 31: T(r) opical  Dyson Schwinger Equations

Bethe-Salpeter EquationBound-State DSE

K(q,k;P) – fully amputated, two-particle irreducible, quark-antiquark scattering kernel

Textbook material. Compact. Visually appealing. Correct

Blocked progress for more than 60 years.

Craig Roberts, Physics Division, Argonne National Laboratory

31

Page 32: T(r) opical  Dyson Schwinger Equations

Bethe-Salpeter EquationGeneral Form

Equivalent exact bound-state equation but in this form K(q,k;P) → Λ(q,k;P)

which is completely determined by dressed-quark self-energy Enables derivation of a Ward-Takahashi identity for Λ(q,k;P)

Craig Roberts, Physics Division, Argonne National Laboratory

32

Lei Chang and C.D. Roberts0903.5461 [nucl-th]Phys. Rev. Lett. 103 (2009) 081601

Page 33: T(r) opical  Dyson Schwinger Equations

Ward-Takahashi IdentityBethe-Salpeter Kernel

Now, for first time, it’s possible to formulate an Ansatz for Bethe-Salpeter kernel given any form for the dressed-quark-gluon vertex by using this identity

Craig Roberts, Physics Division, Argonne National Laboratory

33

Lei Chang and C.D. Roberts0903.5461 [nucl-th]Phys. Rev. Lett. 103 (2009) 081601

iγ5 iγ5

Page 34: T(r) opical  Dyson Schwinger Equations

Ward-Takahashi IdentityBethe-Salpeter Kernel

Now, for first time, it’s possible to formulate an Ansatz for Bethe-Salpeter kernel given any form for the dressed-quark-gluon vertex by using this identity

This enables the identification and elucidation of a wide range of novel consequences of DCSB

Craig Roberts, Physics Division, Argonne National Laboratory

34

Lei Chang and C.D. Roberts0903.5461 [nucl-th]Phys. Rev. Lett. 103 (2009) 081601

iγ5 iγ5

Page 35: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Schwinger’s result for QED:

Craig Roberts, Physics Division, Argonne National Laboratory

35

Page 36: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Schwinger’s result for QED: pQCD: two diagrams

o (a) is QED-likeo (b) is only possible in QCD – involves 3-gluon vertex

Craig Roberts, Physics Division, Argonne National Laboratory

36

Page 37: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Schwinger’s result for QED: pQCD: two diagrams

o (a) is QED-likeo (b) is only possible in QCD – involves 3-gluon vertex

Analyse (a) and (b)o (b) vanishes identically: the 3-gluon vertex does not contribute to

a quark’s anomalous chromomag. moment at leading-ordero (a) Produces a finite result: “ – ⅙ αs/2π ”

~ (– ⅙) QED-result

Craig Roberts, Physics Division, Argonne National Laboratory

37

Page 38: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Schwinger’s result for QED: pQCD: two diagrams

o (a) is QED-likeo (b) is only possible in QCD – involves 3-gluon vertex

Analyse (a) and (b)o (b) vanishes identically: the 3-gluon vertex does not contribute to

a quark’s anomalous chromomag. moment at leading-ordero (a) Produces a finite result: “ – ⅙ αs/2π ”

~ (– ⅙) QED-result But, in QED and QCD, the anomalous chromo- and electro-

magnetic moments vanish identically in the chiral limit!Craig Roberts, Physics Division, Argonne National Laboratory

38

Page 39: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Interaction term that describes magnetic-moment coupling to gauge fieldo Straightforward to show that it mixes left ↔ righto Thus, explicitly violates chiral symmetry

Craig Roberts, Physics Division, Argonne National Laboratory

39

Page 40: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Interaction term that describes magnetic-moment coupling to gauge fieldo Straightforward to show that it mixes left ↔ righto Thus, explicitly violates chiral symmetry

Follows that in fermion’s e.m. current γμF1 does cannot mix with σμνqνF2

No Gordon Identityo Hence massless fermions cannot not possess a measurable

chromo- or electro-magnetic moment

Craig Roberts, Physics Division, Argonne National Laboratory

40

Page 41: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Interaction term that describes magnetic-moment coupling to gauge fieldo Straightforward to show that it mixes left ↔ righto Thus, explicitly violates chiral symmetry

Follows that in fermion’s e.m. current γμF1 does cannot mix with σμνqνF2

No Gordon Identityo Hence massless fermions cannot not possess a measurable

chromo- or electro-magnetic moment But what if the chiral symmetry is dynamically

broken, strongly, as it is in QCD?Craig Roberts, Physics Division, Argonne National Laboratory

41

Page 42: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Three strongly-dressed and essentially-

nonperturbative contributions to dressed-quark-gluon vertex:

Craig Roberts, Physics Division, Argonne National Laboratory

42

DCSB

Lei Chang, Yu-Xin Liu and Craig D. RobertsarXiv:1009.3458 [nucl-th]

Page 43: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Three strongly-dressed and essentially-

nonperturbative contributions to dressed-quark-gluon vertex:

Craig Roberts, Physics Division, Argonne National Laboratory

43

DCSB

Ball-Chiu term•Vanishes if no DCSB•Appearance driven by STI

Lei Chang, Yu-Xin Liu and Craig D. RobertsarXiv:1009.3458 [nucl-th]

Page 44: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Three strongly-dressed and essentially-

nonperturbative contributions to dressed-quark-gluon vertex:

Craig Roberts, Physics Division, Argonne National Laboratory

44

DCSB

Ball-Chiu term•Vanishes if no DCSB•Appearance driven by STI

Anom. chrom. mag. mom.contribution to vertex•Similar properties to BC term•Strength commensurate with lattice-QCD

Skullerud, Bowman, Kizilersu et al.hep-ph/0303176

Lei Chang, Yu-Xin Liu and Craig D. RobertsarXiv:1009.3458 [nucl-th]

Page 45: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Three strongly-dressed and essentially-

nonperturbative contributions to dressed-quark-gluon vertex:

Craig Roberts, Physics Division, Argonne National Laboratory

45

DCSB

Ball-Chiu term•Vanishes if no DCSB•Appearance driven by STI

Anom. chrom. mag. mom.contribution to vertex•Similar properties to BC term•Strength commensurate with lattice-QCD

Skullerud, Bowman, Kizilersu et al.hep-ph/0303176

Role and importance isNovel discovery•Essential to recover pQCD•Constructive interference with Γ5

Lei Chang, Yu-Xin Liu and Craig D. RobertsarXiv:1009.3458 [nucl-th]

Page 46: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Craig Roberts, Physics Division, Argonne National Laboratory

46

Formulated and solved general Bethe-Salpeter equation Obtained dressed electromagnetic vertex Confined quarks don’t have a mass-shello Can’t unambiguously define

magnetic momentso But can define

magnetic moment distribution

Lei Chang, Yu-Xin Liu and Craig D. RobertsarXiv:1009.3458 [nucl-th]

Page 47: T(r) opical  Dyson Schwinger Equations

Dressed-quark anomalousmagnetic moments

Craig Roberts, Physics Division, Argonne National Laboratory

47

Formulated and solved general Bethe-Salpeter equation Obtained dressed electromagnetic vertex Confined quarks don’t have a mass-shello Can’t unambiguously define

magnetic momentso But can define

magnetic moment distribution

Lei Chang, Yu-Xin Liu and Craig D. RobertsarXiv:1009.3458 [nucl-th]

ME κACM κAEM

Full vertex 0.44 -0.22 0.45

Rainbow-ladder 0.35 0 0.048

AEM is opposite in sign but of roughly equal magnitude as ACMo Potentially important for transition form factors, etc.o Muon g-2 ?

Page 48: T(r) opical  Dyson Schwinger Equations

Dressed Vertex & Meson Spectrum

Splitting known experimentally for more than 35 years Hitherto, no explanation

Craig Roberts, Physics Division, Argonne National Laboratory

48

Experiment Rainbow-ladder

One-loop corrected

Ball-Chiu Full vertex

a1 1230

ρ 770

Mass splitting 455

Page 49: T(r) opical  Dyson Schwinger Equations

Dressed Vertex & Meson Spectrum

Splitting known experimentally for more than 35 years Hitherto, no explanation Systematic symmetry-preserving, Poincaré-covariant DSE

truncation scheme of nucl-th/9602012.o Never better than ⅟₄ of splitting∼

Constructing kernel skeleton-diagram-by-diagram, DCSB cannot be faithfully expressed:

Full impact of M(p2) cannot be realised!Craig Roberts, Physics Division, Argonne National Laboratory

49

Experiment Rainbow-ladder

One-loop corrected

Ball-Chiu Full vertex

a1 1230 759 885

ρ 770 644 764

Mass splitting 455 115 121

Page 50: T(r) opical  Dyson Schwinger Equations

Dressed Vertex & Meson Spectrum

Fully consistent treatment of Ball-Chiu vertexo Retain λ3 – term but ignore Γ4 & Γ5

o Some effects of DCSB built into vertex & Bethe-Salpeter kernel Big impact on σ – π complex But, clearly, not the complete answer.

Craig Roberts, Physics Division, Argonne National Laboratory

50

Experiment Rainbow-ladder

One-loop corrected

Ball-Chiu Full vertex

a1 1230 759 885 1066

ρ 770 644 764 924

Mass splitting 455 115 121 142

Page 51: T(r) opical  Dyson Schwinger Equations

Dressed Vertex & Meson Spectrum

Fully consistent treatment of Ball-Chiu vertexo Retain λ3 – term but ignore Γ4 & Γ5

o Some effects of DCSB built into vertex & Bethe-Salpeter kernel Big impact on σ – π complex But, clearly, not the complete answer.

Fully-consistent treatment of complete vertex Ansatz

Craig Roberts, Physics Division, Argonne National Laboratory

51

Experiment Rainbow-ladder

One-loop corrected

Ball-Chiu Full vertex

a1 1230 759 885 1066 1230

ρ 770 644 764 924 745

Mass splitting 455 115 121 142 485

Page 52: T(r) opical  Dyson Schwinger Equations

Dressed Vertex & Meson Spectrum

Fully-consistent treatment of complete vertex Ansatz Subtle interplay between competing effects, which can only

now be explicated Promise of first reliable prediction of light-quark hadron

spectrum, including the so-called hybrid and exotic states.

Craig Roberts, Physics Division, Argonne National Laboratory

52

Experiment Rainbow-ladder

One-loop corrected

Ball-Chiu Full vertex

a1 1230 759 885 1066 1230

ρ 770 644 764 924 745

Mass splitting 455 115 121 142 485

Page 53: T(r) opical  Dyson Schwinger Equations

Pion’s Golderberger-Treiman relation

Craig Roberts, Physics Division, Argonne National Laboratory

53

Maris, Roberts and Tandynucl-th/9707003

Pion’s Bethe-Salpeter amplitude

Dressed-quark propagator

Page 54: T(r) opical  Dyson Schwinger Equations

Pion’s Golderberger-Treiman relation

Craig Roberts, Physics Division, Argonne National Laboratory

54

Maris, Roberts and Tandynucl-th/9707003

Pion’s Bethe-Salpeter amplitude

Dressed-quark propagator

Axial-vector Ward-Takahashi identity entails

Exact inChiral QCD

Page 55: T(r) opical  Dyson Schwinger Equations

Pion’s Golderberger-Treiman relation

Craig Roberts, Physics Division, Argonne National Laboratory

55

Maris, Roberts and Tandynucl-th/9707003

Pion’s Bethe-Salpeter amplitude

Dressed-quark propagator

Axial-vector Ward-Takahashi identity entails

Pseudovector componentsnecessarily nonzero.

Cannot be ignored!

Exact inChiral QCD

Page 56: T(r) opical  Dyson Schwinger Equations

Pion’s GT relationImplications for observables?

Craig Roberts, Physics Division, Argonne National Laboratory

56

Maris and Robertsnucl-th/9804062

Page 57: T(r) opical  Dyson Schwinger Equations

Pion’s GT relationImplications for observables?

Craig Roberts, Physics Division, Argonne National Laboratory

57

Maris and Robertsnucl-th/9804062

Pseudovector componentsdominate in ultraviolet:(Q/2)2 = 2 GeV2

pQCD point for M(p2)→ pQCD at Q2 = 8GeV2

Page 58: T(r) opical  Dyson Schwinger Equations

Pion’s GT relationImplications for observables?

Craig Roberts, Physics Division, Argonne National Laboratory

58

Maris and Robertsnucl-th/9804062

Pseudovector componentsdominate in ultraviolet:(Q/2)2 = 2 GeV2

pQCD point for M(p2)→ pQCD at Q2 = 8GeV2

Page 59: T(r) opical  Dyson Schwinger Equations

Pion’s GT relation

Craig Roberts, Physics Division, Argonne National Laboratory

59

Guttierez, Bashir, Cloët, RobertsarXiv:1002.1968 [nucl-th]

Pion’s Bethe-Salpeter amplitude

Dressed-quark propagator

Page 60: T(r) opical  Dyson Schwinger Equations

Pion’s GT relationContact interaction

Craig Roberts, Physics Division, Argonne National Laboratory

60

Guttierez, Bashir, Cloët, RobertsarXiv:1002.1968 [nucl-th]

Pion’s Bethe-Salpeter amplitude

Dressed-quark propagator

Bethe-Salpeter amplitude can’t depend on relative momentum; propagator can’t be momentum-dependent

1 MQ

Page 61: T(r) opical  Dyson Schwinger Equations

Pion’s GT relationContact interaction

Craig Roberts, Physics Division, Argonne National Laboratory

61

Guttierez, Bashir, Cloët, RobertsarXiv:1002.1968 [nucl-th]

Pion’s Bethe-Salpeter amplitude

Dressed-quark propagator

Bethe-Salpeter amplitude can’t depend on relative momentum; propagator can’t be momentum-dependent

Solved gap and Bethe-Salpeter equationsP2=0: MQ=0.4GeV, Eπ=0.098, Fπ=0.5MQ

1 MQ

Page 62: T(r) opical  Dyson Schwinger Equations

Pion’s GT relationContact interaction

Craig Roberts, Physics Division, Argonne National Laboratory

62

Guttierez, Bashir, Cloët, RobertsarXiv:1002.1968 [nucl-th]

Pion’s Bethe-Salpeter amplitude

Dressed-quark propagator

Bethe-Salpeter amplitude can’t depend on relative momentum; propagator can’t be momentum-dependent

Solved gap and Bethe-Salpeter equationsP2=0: MQ=0.4GeV, Eπ=0.098, Fπ=0.5MQ

1 MQ

Nonzero and significant

Page 63: T(r) opical  Dyson Schwinger Equations

Pion’s GT relationContact interaction

Craig Roberts, Physics Division, Argonne National Laboratory

63

Guttierez, Bashir, Cloët, RobertsarXiv:1002.1968 [nucl-th]

Pion’s Bethe-Salpeter amplitude

Dressed-quark propagator

Asymptotic form of Fπ(Q2)Eπ

2(P)→ Fπem(Q2) = MQ

2/Q2

1 MQ

For 20+ years it was imagined that contact-interaction produced a result that’s indistinguishable From pQCD counting rule

Page 64: T(r) opical  Dyson Schwinger Equations

Pion’s GT relationContact interaction

Craig Roberts, Physics Division, Argonne National Laboratory

64

Guttierez, Bashir, Cloët, RobertsarXiv:1002.1968 [nucl-th]

Pion’s Bethe-Salpeter amplitude

Dressed-quark propagator

Asymptotic form of Fπ(Q2)Eπ

2(P)→ Fπem(Q2) = MQ

2/Q2

Eπ(P) Fπ(P) – cross-term → Fπ

em(Q2) = (Q2/MQ2) * [Eπ(P)/Fπ(P)] * Eπ

2(P)-term = CONSTANT!

1 MQ

For 20+ years it was imagined that contact-interaction produced a result that’s indistinguishable From pQCD counting rule

Page 65: T(r) opical  Dyson Schwinger Equations

Pion’s ElectromagneticForm Factor

Craig Roberts, Physics Division, Argonne National Laboratory

65

Guttierez, Bashir, Cloët, RobertsarXiv:1002.1968 [nucl-th]

QCD-based DSE prediction: D(x-y) = produces M(p2)~1/p2

cf. contact-interaction: produces M(p2)=constant

)( 2

1

yx

)(~)( 4 yxyxD

Page 66: T(r) opical  Dyson Schwinger Equations

Pion’s ElectromagneticForm Factor

Craig Roberts, Physics Division, Argonne National Laboratory

66

Guttierez, Bashir, Cloët, RobertsarXiv:1002.1968 [nucl-th]

QCD-based DSE prediction: D(x-y) = produces M(p2)~1/p2

cf. contact-interaction: produces M(p2)=constant

)( 2

1

yx

)(~)( 4 yxyxD

Page 67: T(r) opical  Dyson Schwinger Equations

Pion’s ElectromagneticForm Factor

Craig Roberts, Physics Division, Argonne National Laboratory

67

Guttierez, Bashir, Cloët, RobertsarXiv:1002.1968 [nucl-th]

QCD-based DSE prediction: D(x-y) = produces M(p2)~1/p2

cf. contact-interaction: produces M(p2)=constant

)( 2

1

yx

)(~)( 4 yxyxD

Single mass parameter in both studies Same predictions for Q2=0 observables Disagreement >20% for Q2>MQ

2

Page 68: T(r) opical  Dyson Schwinger Equations

BaBar Anomalyγ* γ → π0

Craig Roberts, Physics Division, Argonne National Laboratory

68

H.L.L. Roberts, C.D. Roberts, Bashir, Guttierez, TandyarXiv:1009.0067 [nucl-th]

QCD-based DSE prediction: D(x-y) = produces M(p2)~1/p2

cf. contact-interaction: produces M(p2)=constant

)( 2

1

yx

)(~)( 4 yxyxD

Page 69: T(r) opical  Dyson Schwinger Equations

BaBar Anomalyγ* γ → π0

Craig Roberts, Physics Division, Argonne National Laboratory

69

H.L.L. Roberts, C.D. Roberts, Bashir, Guttierez, TandyarXiv:1009.0067 [nucl-th]

QCD-based DSE prediction: D(x-y) = produces M(p2)~1/p2

cf. contact-interaction: produces M(p2)=constant

)( 2

1

yx

)(~)( 4 yxyxD

pQCD

Page 70: T(r) opical  Dyson Schwinger Equations

BaBar Anomalyγ* γ → π0

Craig Roberts, Physics Division, Argonne National Laboratory

70

H.L.L. Roberts, C.D. Roberts, Bashir, Guttierez, TandyarXiv:1009.0067 [nucl-th]

QCD-based DSE prediction: D(x-y) = produces M(p2)~1/p2

cf. contact-interaction: produces M(p2)=constant

)( 2

1

yx

)(~)( 4 yxyxD

No fully-self-consistent treatment of the pion can reproduce the BaBar data. All produce monotonically- increasing concave functions. BaBar data not a true measure of γ* γ → π0

Likely source of error is misidentification of π0 π0

events where 2nd π0 isn’t seen.

pQCD

Page 71: T(r) opical  Dyson Schwinger Equations

Unifying Baryonsand Mesons

Craig Roberts, Physics Division, Argonne National Laboratory

71

M(p2) – effects have enormous impact on meson properties.Must be included in description and prediction of baryon

properties.

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Unifying Baryonsand Mesons

Craig Roberts, Physics Division, Argonne National Laboratory

72

M(p2) – effects have enormous impact on meson properties.Must be included in description and prediction of baryon

properties. M(p2) is essentially a quantum field theoretical effect. In quantum

field theory Meson appears as pole in four-point quark-antiquark Green function

→ Bethe-Salpeter Equation Nucleon appears as a pole in a six-point quark Green function

→ Faddeev Equation.

Page 73: T(r) opical  Dyson Schwinger Equations

Unifying Baryonsand Mesons

Craig Roberts, Physics Division, Argonne National Laboratory

73

M(p2) – effects have enormous impact on meson properties.Must be included in description and prediction of baryon

properties. M(p2) is essentially a quantum field theoretical effect. In quantum

field theory Meson appears as pole in four-point quark-antiquark Green function

→ Bethe-Salpeter Equation Nucleon appears as a pole in a six-point quark Green function

→ Faddeev Equation. Poincaré covariant Faddeev equation sums all possible exchanges

and interactions that can take place between three dressed-quarks Tractable equation is founded on observation that an interaction

which describes colour-singlet mesons also generates nonpointlike quark-quark (diquark) correlations in the colour-antitriplet channel

R.T. Cahill et al.,Austral. J. Phys. 42 (1989) 129-145

Page 74: T(r) opical  Dyson Schwinger Equations

Faddeev Equation

Craig Roberts, Physics Division, Argonne National Laboratory

74

Linear, Homogeneous Matrix equation

R.T. Cahill et al.,Austral. J. Phys. 42 (1989) 129-145

diquark

quark

Page 75: T(r) opical  Dyson Schwinger Equations

Faddeev Equation

Craig Roberts, Physics Division, Argonne National Laboratory

75

Linear, Homogeneous Matrix equationYields wave function (Poincaré Covariant Faddeev Amplitude)

that describes quark-diquark relative motion within the nucleon

R.T. Cahill et al.,Austral. J. Phys. 42 (1989) 129-145

diquark

quark

quark exchangeensures Pauli statistics

Page 76: T(r) opical  Dyson Schwinger Equations

Faddeev Equation

Craig Roberts, Physics Division, Argonne National Laboratory

76

Linear, Homogeneous Matrix equationYields wave function (Poincaré Covariant Faddeev Amplitude)

that describes quark-diquark relative motion within the nucleon Scalar and Axial-Vector Diquarks . . .

Both have “correct” parity and “right” masses In Nucleon’s Rest Frame Amplitude has

s−, p− & d−wave correlations

R.T. Cahill et al.,Austral. J. Phys. 42 (1989) 129-145

diquark

quark

quark exchangeensures Pauli statistics

Page 77: T(r) opical  Dyson Schwinger Equations

Spectrum of some known u- & d-quark baryons

Craig Roberts, Physics Division, Argonne National Laboratory

77

Mesons & Diquarks

H.L.L. Roberts, L. Chang and C.D. RobertsarXiv:1007.4318 [nucl-th]H.L.L. Roberts, L. Chang, I.C. Cloët and C.D. Roberts arXiv:1007.3566 [nucl-th]

m0+ m1+ m0- m1- mπ mρ mσ ma1

0.72 1.01 1.17 1.31 0.14 0.80 1.06 1.23

Page 78: T(r) opical  Dyson Schwinger Equations

Spectrum of some known u- & d-quark baryons

Craig Roberts, Physics Division, Argonne National Laboratory

78

Mesons & DiquarksCahill, Roberts, Praschifka: Phys.Rev. D36 (1987) 2804

Proof of mass ordering: diquark-mJ+ > meson-mJ-

H.L.L. Roberts, L. Chang and C.D. RobertsarXiv:1007.4318 [nucl-th]H.L.L. Roberts, L. Chang, I.C. Cloët and C.D. Roberts arXiv:1007.3566 [nucl-th]

m0+ m1+ m0- m1- mπ mρ mσ ma1

0.72 1.01 1.17 1.31 0.14 0.80 1.06 1.23

Page 79: T(r) opical  Dyson Schwinger Equations

Spectrum of some known u- & d-quark baryons

Craig Roberts, Physics Division, Argonne National Laboratory

79

Mesons & DiquarksCahill, Roberts, Praschifka: Phys.Rev. D36 (1987) 2804

Proof of mass ordering: diquark-mJ+ > meson-mJ-

H.L.L. Roberts, L. Chang and C.D. RobertsarXiv:1007.4318 [nucl-th]H.L.L. Roberts, L. Chang, I.C. Cloët and C.D. Roberts arXiv:1007.3566 [nucl-th]

m0+ m1+ m0- m1- mπ mρ mσ ma1

0.72 1.01 1.17 1.31 0.14 0.80 1.06 1.23

Baryons: ground-states and 1st radial exciationsmN mN* mN(⅟₂) mN*(⅟₂-) mΔ mΔ* mΔ(3⁄₂-) mΔ*(3⁄₂-)

DSE 1.05 1.73 1.86 2.09 1.33 1.85 1.98 2.16EBAC 1.76 1.80 1.39 1.98

Page 80: T(r) opical  Dyson Schwinger Equations

Spectrum of some known u- & d-quark baryons

Craig Roberts, Physics Division, Argonne National Laboratory

80

Mesons & DiquarksCahill, Roberts, Praschifka: Phys.Rev. D36 (1987) 2804

Proof of mass ordering: diquark-mJ+ > meson-mJ-

H.L.L. Roberts, L. Chang and C.D. RobertsarXiv:1007.4318 [nucl-th]H.L.L. Roberts, L. Chang, I.C. Cloët and C.D. Roberts arXiv:1007.3566 [nucl-th]

m0+ m1+ m0- m1- mπ mρ mσ ma1

0.72 1.01 1.17 1.31 0.14 0.80 1.06 1.23

Baryons: ground-states and 1st radial exciationsmN mN* mN(⅟₂) mN*(⅟₂-) mΔ mΔ* mΔ(3⁄₂-) mΔ*(3⁄₂-)

DSE 1.05 1.73 1.86 2.09 1.33 1.85 1.98 2.16EBAC 1.76 1.80 1.39 1.98

mean-|relative-error| = 2%-Agreement DSE dressed-quark-core masses cf. Excited Baryon Analysis Center (JLab) bare masses is significant ’cause no attempt was made to ensure this.

Page 81: T(r) opical  Dyson Schwinger Equations

Spectrum of some known u- & d-quark baryons

Craig Roberts, Physics Division, Argonne National Laboratory

81

Mesons & DiquarksCahill, Roberts, Praschifka: Phys.Rev. D36 (1987) 2804

Proof of mass ordering: diquark-mJ+ > meson-mJ-

H.L.L. Roberts, L. Chang and C.D. RobertsarXiv:1007.4318 [nucl-th]H.L.L. Roberts, L. Chang, I.C. Cloët and C.D. Roberts arXiv:1007.3566 [nucl-th]

m0+ m1+ m0- m1- mπ mρ mσ ma1

0.72 1.01 1.17 1.31 0.14 0.80 1.06 1.23

Baryons: ground-states and 1st radial exciationsmN mN* mN(⅟₂) mN*(⅟₂-) mΔ mΔ* mΔ(3⁄₂-) mΔ*(3⁄₂-)

DSE 1.05 1.73 1.86 2.09 1.33 1.85 1.98 2.16EBAC 1.76 1.80 1.39 1.98

mean-|relative-error| = 2%-Agreement DSE dressed-quark-core masses cf. Excited Baryon Analysis Center (JLab) bare masses is significant ’cause no attempt was made to ensure this.

1st radialExcitation ofN(1535)?

Page 82: T(r) opical  Dyson Schwinger Equations

Nucleon ElasticForm Factors

Craig Roberts, Physics Division, Argonne National Laboratory

82

Photon-baryon vertexOettel, Pichowsky and von Smekal, nucl-th/9909082

I.C. Cloët, C.D. Roberts, et al.arXiv:0812.0416 [nucl-th]

Page 83: T(r) opical  Dyson Schwinger Equations

Nucleon ElasticForm Factors

Craig Roberts, Physics Division, Argonne National Laboratory

83

Photon-baryon vertexOettel, Pichowsky and von Smekal, nucl-th/9909082

I.C. Cloët, C.D. Roberts, et al.arXiv:0812.0416 [nucl-th]

“Survey of nucleon electromagnetic form factors” – unification of meson and baryon observables; and prediction of nucleon elastic form factors to 15 GeV2

Page 84: T(r) opical  Dyson Schwinger Equations

Craig Roberts, Physics Division, Argonne National Laboratory

84

New JLab data: S. Riordan et al., arXiv:1008.1738 [nucl-ex]

I.C. Cloët, C.D. Roberts, et al.arXiv:0812.0416 [nucl-th]

)(

)(2

2

QG

QGnM

nEn

Page 85: T(r) opical  Dyson Schwinger Equations

Craig Roberts, Physics Division, Argonne National Laboratory

85

New JLab data: S. Riordan et al., arXiv:1008.1738 [nucl-ex]

DSE-prediction

I.C. Cloët, C.D. Roberts, et al.arXiv:0812.0416 [nucl-th]

)(

)(2

2

QG

QGnM

nEn

This evolution is very sensitive to momentum-dependence of dressed-quark propagator

Page 86: T(r) opical  Dyson Schwinger Equations

Craig Roberts, Physics Division, Argonne National Laboratory

86

New JLab data: S. Riordan et al., arXiv:1008.1738 [nucl-ex]

I.C. Cloët, C.D. Roberts, et al.arXiv:0812.0416 [nucl-th]

)(

)(2,

1

2,1

QF

QFup

dp

Page 87: T(r) opical  Dyson Schwinger Equations

Craig Roberts, Physics Division, Argonne National Laboratory

87

New JLab data: S. Riordan et al., arXiv:1008.1738 [nucl-ex]

I.C. Cloët, C.D. Roberts, et al.arXiv:0812.0416 [nucl-th]

)(

)(2,

1

2,1

QF

QFup

dp

Brooks, Bodek, Budd, Arrington fit to data: hep-ex/0602017

Page 88: T(r) opical  Dyson Schwinger Equations

Craig Roberts, Physics Division, Argonne National Laboratory

88

New JLab data: S. Riordan et al., arXiv:1008.1738 [nucl-ex]

DSE-prediction

I.C. Cloët, C.D. Roberts, et al.arXiv:0812.0416 [nucl-th]

)(

)(2,

1

2,1

QF

QFup

dp

Location of zero measures relative strength of scalar and axial-vector qq-correlations

Brooks, Bodek, Budd, Arrington fit to data: hep-ex/0602017

Page 89: T(r) opical  Dyson Schwinger Equations

Craig Roberts, Physics Division, Argonne National Laboratory

89

Neutron Structure Function at high x

SU(6) symmetry

pQCD

0+ qq only

Reviews: S. Brodsky et al.

NP B441 (1995)W. Melnitchouk & A.W.Thomas

PL B377 (1996) 11N. Isgur, PRD 59 (1999)R.J. Holt & C.D. Roberts

RMP (2010)DSE: 0+ & 1+ qq

I.C. Cloët, C.D. Roberts, et al.arXiv:0812.0416 [nucl-th]

Page 90: T(r) opical  Dyson Schwinger Equations

Craig Roberts, Physics Division, Argonne National Laboratory

90

Epilogue

Dynamical chiral symmetry breaking (DCSB) is a realityo Expressed in M(p2), with observable signals in experiment

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Craig Roberts, Physics Division, Argonne National Laboratory

91

Epilogue

Dynamical chiral symmetry breaking (DCSB) is a realityo Expressed in M(p2), with observable signals in experiment

Poincaré covarianceCrucial in description of contemporary data

Page 92: T(r) opical  Dyson Schwinger Equations

Craig Roberts, Physics Division, Argonne National Laboratory

92

Epilogue

Dynamical chiral symmetry breaking (DCSB) is a realityo Expressed in M(p2), with observable signals in experiment

Poincaré covarianceCrucial in description of contemporary data

Fully-self-consistent treatment of an interaction Essential if experimental data is truly to be understood.

Page 93: T(r) opical  Dyson Schwinger Equations

Craig Roberts, Physics Division, Argonne National Laboratory

93

Epilogue

Dynamical chiral symmetry breaking (DCSB) is a realityo Expressed in M(p2), with observable signals in experiment

Poincaré covarianceCrucial in description of contemporary data

Fully-self-consistent treatment of an interaction Essential if experimental data is truly to be understood.

Dyson-Schwinger equations: o single framework, with IR model-input turned to advantage,

“almost unique in providing unambiguous path from a defined interaction → Confinement & DCSB → Masses → radii → form factors → distribution functions → etc.” McLerran & Pisarski

arXiv:0706.2191 [hep-ph]