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Transcript of Craig Roberts Physics Division
Dyson-Schwinger Equations & Continuum QCD
Adnan BASHIR (U Michoacan);Stan BRODSKY (SLAC);Lei CHANG (ANL & PKU); Huan CHEN (BIHEP);Ian CLOËT (UW);Bruno EL-BENNICH (Sao Paulo);Xiomara GUTIERREZ-GUERRERO (U Michoacan);Roy HOLT (ANL);Mikhail IVANOV (Dubna);Yu-xin LIU (PKU);Trang NGUYEN (KSU);Si-xue QIN (PKU);Hannes ROBERTS (ANL, FZJ, UBerkeley);Robert SHROCK (Stony Brook);Peter TANDY (KSU);David WILSON (ANL)
Craig Roberts
Physics Division
StudentsEarly-career scientists
Published collaborations in 2010/2011
QCD’s Challenges
Dynamical Chiral Symmetry Breaking Very unnatural pattern of bound state masses;
e.g., Lagrangian (pQCD) quark mass is small but . . . no degeneracy between JP=+ and JP=− (parity partners)
Neither of these phenomena is apparent in QCD’s Lagrangian Yet they are the dominant determining characteristics
of real-world QCD.
QCD – Complex behaviour arises from apparently simple rules.Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Quark and Gluon ConfinementNo matter how hard one strikes the proton, one cannot liberate an individual quark or gluon
Understand emergent phenomena
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Universal Truths
Hadron spectrum, and 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 (almost) irrelevant to light-quarks. Running of quark mass entails that calculations at even modest Q2 require a
Poincaré-covariant approach. Covariance + M(p2) require existence of quark orbital angular momentum in
hadron's rest-frame wave function. Confinement is expressed through a violent change of the propagators for
coloured particles & can almost be read from a plot of a states’ dressed-propagator.
It is intimately connected with DCSB.
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Strong-interaction: QCD
Asymptotically free– Perturbation theory is valid
and accurate tool at large-Q2
– Hence chiral limit is defined Essentially nonperturbative
for Q2 < 2 GeV2
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Nature’s only example of truly nonperturbative, fundamental theory A-priori, no idea as to what such a theory can produce
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
Confinement
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Confinement
Quark and Gluon Confinement– No matter how hard one strikes the proton, or any other
hadron, one cannot liberate an individual quark or gluon Empirical fact. However
– There is no agreed, theoretical definition of light-quark confinement
– Static-quark confinement is irrelevant to real-world QCD• There are no long-lived, very-massive quarks
Confinement entails quark-hadron duality; i.e., that all observable consequences of QCD can, in principle, be computed using an hadronic basis.
X
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Confinement
Infinitely heavy-quarks plus 2 flavours with mass = ms – Lattice spacing = 0.083fm– String collapses
within one lattice time-stepR = 1.24 … 1.32 fm
– Energy stored in string at collapse Ec
sb = 2 ms – (mpg made via
linear interpolation) No flux tube between
light-quarks
G. Bali et al., PoS LAT2005 (2006) 308
Bs anti-Bs
“Note that the time is not a linear function of the distance but dilated within the string breaking region. On a linear time scale string breaking takes place rather rapidly. […] light pair creation seems to occur non-localized and instantaneously.”
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Confinement Confinement is expressed through a violent change in
the analytic structure of propagators for coloured particles & can almost be read from a plot of a states’ dressed-propagator– Gribov (1978); Munczek (1983); Stingl (1984); Cahill (1989);
Krein, Roberts & Williams (1992); Tandy (1994); …
complex-P2 complex-P2
o Real-axis mass-pole splits, moving into pair(s) of complex conjugate poles or branch pointso Spectral density no longer positive semidefinite & hence state cannot exist in observable spectrum
Normal particle Confined particle
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timelike axis: P2<0
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Dressed-gluon propagator
Gluon propagator satisfies a Dyson-Schwinger Equation
Plausible possibilities for the solution
DSE and lattice-QCDagree on the result– Confined gluon– IR-massive but UV-massless– mG ≈ 2-4 ΛQCD
perturbative, massless gluon
massive , unconfined gluon
IR-massive but UV-massless, confined gluon
A.C. Aguilar et al., Phys.Rev. D80 (2009) 085018
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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: Dyson-Schwinger Equations and Continuum QCD.
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This is a well-posed problem whose solution is an elemental goal of modern hadron physics.The answer provides QCD’s running coupling.
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Charting the interaction between light-quarks
Through QCD's Dyson-Schwinger equations (DSEs) the pointwise behaviour of the β-function determines the 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 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: Dyson-Schwinger Equations and Continuum QCD.
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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DSE Studies – Phenomenology of gluon
Wide-ranging study of π & ρ properties Effective coupling
– Agrees with pQCD in ultraviolet – Saturates in infrared
• α(0)/π = 3.2 • α(1 GeV2)/π = 0.35
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Maris & Tandy, Phys.Rev. C60 (1999) 055214
Running gluon mass– Gluon is massless in ultraviolet
in agreement with pQCD– Massive in infrared
• mG(0) = 0.76 GeV• mG(1 GeV2) = 0.46 GeV
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Dynamical Chiral Symmetry Breaking
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Dynamical Chiral Symmetry Breaking
Strong-interaction: QCD Confinement
– Empirical feature– Modern theory and lattice-QCD support conjecture
• that light-quark confinement is a fact• associated with violation of reflection positivity; i.e., novel analytic
structure for propagators and vertices– Still circumstantial, no proof yet of confinement
On the other hand, DCSB is a fact in QCD– It is the most important mass generating mechanism for visible
matter in the Universe. Responsible for approximately 98% of the proton’s
mass.Higgs mechanism is (almost) irrelevant to light-quarks.
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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.
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C.D. Roberts, Prog. Part. Nucl. Phys. 61 (2008) 50M. Bhagwat & P.C. Tandy, AIP Conf.Proc. 842 (2006) 225-227
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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.
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DSE prediction of DCSB confirmed
Mass from nothing!
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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.
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Hint of lattice-QCD support for DSE prediction of violation of reflection positivity
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
12GeVThe Future of JLab
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.
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Jlab 12GeV: Scanned by 2<Q2<9 GeV2 elastic & transition form factors.
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Dynamical Chiral Symmetry Breaking
Condensates?LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
Dichotomy of the pion
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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How does one make an almost massless particle from two massive constituent-quarks?
Naturally, one could always tune a potential in quantum mechanics so that the ground-state is massless – but some are still making this mistake
However: current-algebra (1968) This is impossible in quantum mechanics, for which one
always finds:
mm 2
tconstituenstatebound mm
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Gell-Mann – Oakes – RennerRelation
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This paper derives a relation between mπ
2 and the expectation-value < π|u0|π>,
where uo is an operator that is linear in the putative Hamiltonian’s explicit chiral-symmetry breaking term NB. QCD’s current-quarks were not yet invented, so u0 was not
expressed in terms of current-quark fields PCAC-hypothesis (partial conservation of axial current) is used in
the derivation Subsequently, the concepts of soft-pion theory
Operator expectation values do not change as t=mπ2 → t=0
to take < π|u0|π> → < 0|u0|0> … in-pion → in-vacuum
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Behavior of current divergences under SU(3) x SU(3).Murray Gell-Mann, R.J. Oakes , B. Renner Phys.Rev. 175 (1968) 2195-2199
Gell-Mann – Oakes – RennerRelation
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PCAC hypothesis; viz., pion field dominates the divergence of the axial-vector current
Soft-pion theorem
In QCD, this is and one therefore has
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Behavior of current divergences under SU(3) x SU(3).Murray Gell-Mann, R.J. Oakes , B. Renner Phys.Rev. 175 (1968) 2195-2199
Commutator is chiral rotationTherefore, isolates explicit chiral-symmetry breaking term in the putative Hamiltonian
qqm
Zhou Guangzhao 周光召Born 1929 Changsha, Hunan province
Gell-Mann – Oakes – RennerRelation
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Theoretical physics at its best. But no one is thinking about how properly to consider or
define what will come to be called the vacuum quark condensate
So long as the condensate is just a mass-dimensioned constant, which approximates another well-defined transition matrix element, there is no problem.
Problem arises if one over-interprets this number, which textbooks have been doing for a VERY LONG TIME.
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- (0.25GeV)3
Note of Warning
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Chiral Magnetism (or Magnetohadrochironics)A. Casher and L. Susskind, Phys. Rev. D9 (1974) 436
These authors argue that dynamical chiral-symmetry breaking can be realised as aproperty of hadrons, instead of via a nontrivial vacuum exterior to the measurable degrees of freedom
The essential ingredient required for a spontaneous symmetry breakdown in a composite system is the existence of a divergent number of constituents – DIS provided evidence for divergent sea of low-momentum partons – parton model.
QCD Sum Rules
Introduction of the gluon vacuum condensate
and development of “sum rules” relating properties of low-lying hadronic states to vacuum condensates
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QCD and Resonance Physics. Sum Rules.M.A. Shifman, A.I. Vainshtein, and V.I. Zakharov Nucl.Phys. B147 (1979) 385-447; citations: 3713
QCD Sum Rules
Introduction of the gluon vacuum condensate
and development of “sum rules” relating properties of low-lying hadronic states to vacuum condensates
At this point (1979), the cat was out of the bag: a physical reality was seriously attributed to a plethora of vacuum condensates
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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QCD and Resonance Physics. Sum Rules.M.A. Shifman, A.I. Vainshtein, and V.I. Zakharov Nucl.Phys. B147 (1979) 385-447; citations: 3781
“quark condensate”1960-1980
Instantons in non-perturbative QCD vacuum, MA Shifman, AI Vainshtein… - Nuclear Physics B, 1980
Instanton density in a theory with massless quarks, MA Shifman, AI Vainshtein… - Nuclear Physics B, 1980
Exotic new quarks and dynamical symmetry breaking, WJ Marciano - Physical Review D, 1980
The pion in QCDJ Finger, JE Mandula… - Physics Letters B, 1980
No references to this phrase before 1980Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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6550+ REFERENCES TO THIS PHRASE SINCE 1980
Universal Conventions
Wikipedia: (http://en.wikipedia.org/wiki/QCD_vacuum)“The QCD vacuum is the vacuum state of quantum chromodynamics (QCD). It is an example of a non-perturbative vacuum state, characterized by many non-vanishing condensates such as the gluon condensate or the quark condensate. These condensates characterize the normal phase or the confined phase of quark matter.”
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Universal Misapprehensions
Since 1979, DCSB has commonly been associated literally with a spacetime-independent mass-dimension-three “vacuum condensate.”
Under this assumption, “condensates” couple directly to gravity in general relativity and make an enormous contribution to the cosmological constant
Experimentally, the answer is
Ωcosm. const. = 0.76 This mismatch is a bit of a problem.
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Resolution?
Quantum Healing Central: “KSU physics professor [Peter Tandy] publishes groundbreaking
research on inconsistency in Einstein theory.” Paranormal Psychic Forums:
“Now Stanley Brodsky of the SLAC National Accelerator Laboratory in Menlo Park, California, and colleagues have found a wayto get rid of the discrepancy. “People have just been taking it on faith that this quark condensate is present throughout the vacuum,” says Brodsky.
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Paradigm shift:In-Hadron Condensates
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.
– GMOR cf.
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QCD
Brodsky, Roberts, Shrock, Tandy, Phys. Rev. C82 (Rapid Comm.) (2010) 022201Brodsky and Shrock, PNAS 108, 45 (2011)M. Burkardt, Phys.Rev. D58 (1998) 096015
Paradigm shift:In-Hadron Condensates
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
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Brodsky, Roberts, Shrock, Tandy, Phys. Rev. C82 (Rapid Comm.) (2010) 022201Brodsky and Shrock, PNAS 108, 45 (2011)
Paradigm shift:In-Hadron Condensates
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
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0);0( qq
Chiral limit
Brodsky, Roberts, Shrock, Tandy, Phys. Rev. C82 (Rapid Comm.) (2010) 022201Brodsky and Shrock, PNAS 108, 45 (2011)
“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.”
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“Void that is truly empty solves dark energy puzzle”Rachel Courtland, New Scientist 4th Sept. 2010
Cosmological Constant: Putting QCD condensates back into hadrons reduces the mismatch between experiment and theory by a factor of 1046
Possibly by far more, if technicolour-like theories are the correct paradigm for extending the Standard Model
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Paradigm shift:In-Hadron Condensates
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Dynamical Chiral Symmetry Breaking
Importance of being well-dressed for quarks
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Strong-interaction: QCD
Gluons and quarks acquire momentum-dependent masses– characterised by an infrared mass-scale m ≈ 2-4 ΛQCD
Significant body of work, stretching back to 1980, which shows that, in the presence of DCSB, the dressed-fermion-photon vertex is materially altered from the bare form: γμ.– Obvious, because with
A(p2) ≠ 1 and B(p2) ≠ constant, the bare vertex cannot satisfy the Ward-Takahashi identity; viz.,
Number of contributors is too numerous to list completely (300 citations to 1st J.S. Ball paper), but prominent contributions by:J.S. Ball, C.J. Burden, C.Roberts, R. Delbourgo, A.G. Williams, H.J. Munczek, M.R. Pennington, A. Bashir, A. Kizilersu, P.Tandy, L. Chang, Y.-X. Liu …
Dressed-quark-gluon vertex
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Dressed-quark-gluon vertex
Single most important feature– Perturbative vertex is helicity-conserving:
• Cannot cause spin-flip transitions– However, DCSB introduces nonperturbatively generated
structures that very strongly break helicity conservation– These contributions
• Are large when the dressed-quark mass-function is large– Therefore vanish in the ultraviolet;
i.e., on the perturbative domain– Exact form of the contributions is still the subject of debate
but their existence is model-independent - a fact.
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Gap EquationGeneral Form
Dμν(k) – dressed-gluon propagator Γν(q,p) – dressed-quark-gluon vertex Until 2009, all studies of other hadron phenomena used the
leading-order term in a symmetry-preserving truncation scheme; viz., – Dμν(k) = dressed, as described previously– Γν(q,p) = γμ
• … plainly, key nonperturbative effects are missed and cannot be recovered through any step-by-step improvement procedure
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Bender, Roberts & von SmekalPhys.Lett. B380 (1996) 7-12
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Gap EquationGeneral Form
Dμν(k) – dressed-gluon propagator good deal of information available
Γν(q,p) – dressed-quark-gluon vertex Information accumulating
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?!
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If kernels of Bethe-Salpeter and gap equations don’t match,one won’t even get right charge for the pion.
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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.
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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)
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Lei Chang and C.D. Roberts0903.5461 [nucl-th]Phys. Rev. Lett. 103 (2009) 081601
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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
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Lei Chang and C.D. Roberts0903.5461 [nucl-th]Phys. Rev. Lett. 103 (2009) 081601
iγ5 iγ5
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Relativistic quantum mechanics
Dirac equation (1928):Pointlike, massive fermion interacting with electromagnetic field
Spin Operator
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Massive point-fermion Anomalous magnetic moment
Dirac’s prediction held true for the electron until improvements in experimental techniques enabled the discovery of a small deviation: H. M. Foley and P. Kusch, Phys. Rev. 73, 412 (1948).– Moment increased by a multiplicative factor: 1.001 19 ± 0.000 05.
This correction was explained by the first systematic computation using renormalized quantum electrodynamics (QED): J.S. Schwinger, Phys. Rev. 73, 416 (1948), – vertex correction
The agreement with experiment established quantum electrodynamics as a valid tool.
e e
0.001 16
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Fermion electromagnetic current – General structure
with k = pf - pi F1(k2) – Dirac form factor; and F2(k2) – Pauli form factor
– Dirac equation: • F1(k2) = 1 • F2(k2) = 0
– Schwinger: • F1(k2) = 1• F2(k2=0) = α /[2 π]
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Plainly, can’t simply take the limit m → 0. Standard QED interaction, generated by minimal substitution:
Magnetic moment is described by interaction term:
– Invariant under local U(1) gauge transformations – but is not generated by minimal substitution in the action for a free
Dirac field. Transformation properties under chiral rotations?
– Ψ(x) → exp(iθγ5) Ψ(x)
Magnetic moment of a massless fermion?
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Standard QED interaction, generated by minimal substitution:
– Unchanged under chiral rotation– Follows that QED without a fermion mass term is helicity conserving
Magnetic moment interaction is described by interaction term:
– NOT invariant– picks up a phase-factor exp(2iθγ5)
Magnetic moment interaction is forbidden in a theory with manifest chiral symmetry
Magnetic moment of a massless fermion?
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One-loop calculation:
Plainly, one obtains Schwinger’s result for me2 ≠ 0
However,
F2(k2) = 0 when me2 = 0
There is no Gordon identity:
Results are unchanged at every order in perturbation theory … owing to symmetry … magnetic moment interaction is forbidden in a theory with manifest chiral symmetry
Schwinger’s result?
e e
m=0 So, no mixingγμ ↔ σμν
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QCD and dressed-quark anomalous magnetic 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: Dyson-Schwinger Equations and Continuum QCD.
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Dressed-quark anomalousmagnetic moments
Three strongly-dressed and essentially-
nonperturbative contributions to dressed-quark-gluon vertex:
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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
L. Chang, Y. –X. Liu and C.D. RobertsarXiv:1009.3458 [nucl-th]Phys. Rev. Lett. 106 (2011) 072001
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Dressed-quark anomalous chromomagnetic moment
Lattice-QCD– m = 115 MeV
Nonperturbative result is two orders-of-magnitude larger than the perturbative computation– This level of
magnification istypical of DCSB
– cf.
Skullerud, Kizilersu et al.JHEP 0304 (2003) 047
Prediction from perturbative QCD
Quenched lattice-QCD
Quark mass function:M(p2=0)= 400MeVM(p2=10GeV2)=4 MeV
LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
Dressed-quark anomalousmagnetic moments
Three strongly-dressed and essentially-
nonperturbative contributions to dressed-quark-gluon vertex:
52
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
L. Chang, Y. –X. Liu and C.D. RobertsarXiv:1009.3458 [nucl-th]Phys. Rev. Lett. 106 (2011) 072001
LightCone 2011, SMU 23-27 May - 77pgs
Dressed-quark anomalousmagnetic moments
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
53
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
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 ACM
L. Chang, Y. –X. Liu and C.D. RobertsarXiv:1009.3458 [nucl-th]Phys. Rev. Lett. 106 (2011) 072001
Factor of 10 magnification
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Dressed-quark anomalousmagnetic moments
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
54
Potentially important for elastic and transition form factors, etc. Significantly, also quite possibly for muon g-2 – via Box diagram,
which is not constrained by extant data. (I.C. Cloët et al.)
L. Chang, Y. –X. Liu and C.D. RobertsarXiv:1009.3458 [nucl-th]Phys. Rev. Lett. 106 (2011) 072001
Factor of 10 magnification
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
Contemporary theoretical estimates:1 – 10 x 10-10
Largest value reduces discrepancy expt.↔theory from 3.3σ to below 2σ.
LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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:
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Experiment Rainbow-ladder
One-loop corrected
Ball-Chiu Full vertex
a1 1230
ρ 770
Mass splitting 455
Full impact of M(p2) cannot be realised!
Experiment Rainbow-ladder
One-loop corrected
Ball-Chiu Full vertex
a1 1230 759 885
ρ 770 644 764
Mass splitting 455 115 121
Location of zeromarks –m2
meson
LightCone 2011, SMU 23-27 May - 77pgs
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 Promise of 1st reliable prediction
of light-quark hadron spectrumCraig Roberts: Dyson-Schwinger Equations and Continuum QCD.
56
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
Experiment Rainbow-ladder
One-loop corrected
Ball-Chiu Full vertex
a1 1230 759 885 1128 1270
ρ 770 644 764 919 790
Mass splitting 455 115 121 209 480
BC: zero moves deeper for both ρ & a1 Both masses grow
Full vertex: zero moves deeper for a1 but shallower for ρProblem solved
LightCone 2011, SMU 23-27 May - 77pgs
Lei Chang & C.D. Roberts, arXiv:1104.4821 [nucl-th]Tracing massess of ground-state light-quark mesons
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Grand Unification
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
Unification of Meson & Baryon Properties
Correlate the masses of meson and baryon ground- and excited-states within a single, symmetry-preserving framework Symmetry-preserving means:
Poincaré-covariant & satisfy relevant Ward-Takahashi identities Constituent-quark model has hitherto been the most widely applied
spectroscopic tool; whilst its weaknesses are emphasized by critics and acknowledged by proponents, it is of continuing value because there is nothing better that is yet providing a bigger picture.
Nevertheless, no connection with quantum field theory & therefore not with QCD not symmetry-preserving & therefore cannot veraciously connect
meson and baryon properties
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
58LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
Baryons Dynamical chiral symmetry breaking (DCSB)
– has enormous impact on meson properties.Must be included in description and prediction of baryon properties.
DCSB 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 based on observation that an interaction which
describes colour-singlet mesons also generates nonpointlike quark-quark (diquark) correlations in the colour-antitriplet channel
59
R.T. Cahill et al.,Austral. J. Phys. 42 (1989) 129-145
rqq ≈ rπ
LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
Faddeev Equation
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 correlations60
R.T. Cahill et al.,Austral. J. Phys. 42 (1989) 129-145
diquark
quark
quark exchangeensures Pauli statistics
composed of strongly-dressed quarks bound by dressed-gluons
LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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“Spectrum” of nonpointlike quark-quark correlations
Observed in– DSE studies in QCD– 0+ & 1+ in Lattice-QCD
Scalar diquark form factor– r0+ ≈ rπ
Axial-vector diquarks– r1+ ≈ rρ
Diquarks in QCD
LightCone 2011, SMU 23-27 May - 77pgs
Zero relation with old notion of pointlike constituent-like diquarks
BOTH essential
H.L.L. Roberts et al., 1102.4376 [nucl-th]Phys. Rev. C in press
Masses of ground and excited-state hadronsHannes L.L. Roberts, Lei Chang, Ian C. Cloët and Craig D. Roberts, arXiv:1101.4244 [nucl-th] Few Body Systems (2011) pp. 1-25
Baryons & diquarks
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
62
Provided numerous insights into baryon structure; e.g., There is a causal connection between mΔ - mN & m1+- m0+
mΔ - mN
mN
mΔ
Physical splitting grows rapidly with increasing diquark mass difference
LightCone 2011, SMU 23-27 May - 77pgs
Masses of ground and excited-state hadronsHannes L.L. Roberts, Lei Chang, Ian C. Cloët and Craig D. Roberts, arXiv:1101.4244 [nucl-th] Few Body Systems (2011) pp. 1-25
Baryons & diquarks
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
63
Provided numerous insights into baryon structure; e.g., mN ≈ 3 M & mΔ ≈ M+m1+
LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Photon-nucleon current
Composite nucleon must interact with photon via nontrivial current constrained by Ward-Takahashi identities
DSE, BSE, Faddeev equation, current → nucleon form factors
Vertex contains dressed-quark anomalous magnetic moment
Oettel, Pichowsky, SmekalEur.Phys.J. A8 (2000) 251-281
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Nucleon Form Factors
LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
Survey of nucleon electromagnetic form factorsI.C. Cloët et al, arXiv:0812.0416 [nucl-th], Few Body Syst. 46 (2009) pp. 1-36
Unification of meson and nucleon form factors.
Very good description.
Quark’s momentum-dependent anomalous magnetic moment has observable impact & materially improves agreement in all cases.
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
66
I.C. Cloët, C.D. Roberts, et al.arXiv:0812.0416 [nucl-th]
)(
)(
2
2
QG
QG
pM
pEp
Highlights again the critical importance of DCSB in explanation of real-world observables.
DSE result Dec 08
DSE result – including the anomalous magnetic moment distribution
I.C. Cloët, C.D. Roberts, et al.In progress
LightCone 2011, SMU 23-27 May - 77pgs
67
Quark anomalous magnetic moment hasbig impact on proton ratio
But little impact on theneutron ratio
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
)(
)(2
2
QG
QGnM
nEn
I.C. Cloët, C.D. Roberts, et al.In progress
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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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
LightCone 2011, SMU 23-27 May - 77pgs
Phys.Rev.Lett. 105 (2010) 262302
Hadron Spectrum
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
69
Legend: Particle Data Group H.L.L. Roberts et al. EBAC Jülich
o Symmetry-preserving unification of the computation of meson & baryon masseso rms-rel.err./deg-of-freedom = 13%o PDG values (almost) uniformly overestimated in both cases - room for the pseudoscalar meson cloud?!
LightCone 2011, SMU 23-27 May - 77pgs
Masses of ground and excited-state hadronsH.L.L. Roberts et al., arXiv:1101.4244 [nucl-th] Few Body Systems (2011) pp. 1-25
Baryon Spectrum
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
70
In connection with EBAC's analysis, dressed-quark Faddeev-equation predictions for bare-masses agree within rms-relative-error of 14%. Notably, EBAC finds a dressed-quark-core for the Roper resonance,
at a mass which agrees with Faddeev Eq. prediction.
LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
71
EBAC & the Roper resonance
EBAC examined the dynamical origins of the two poles associated with the Roper resonance are examined.
Both of them, together with the next higher resonance in the P11 partial wave were found to have the same originating bare state
Coupling to the meson-baryon continuum induces multiple observed resonances from the same bare state.
All PDG identified resonances consist of a core state and meson-baryon components.
N. Suzuki et al., Phys.Rev.Lett. 104 (2010) 042302
LightCone 2011, SMU 23-27 May - 77pgs
Hadron Spectrum
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
72
Legend: Particle Data Group H.L.L. Roberts et al. EBAC Jülich
Now and for the foreseeable future, QCD-based theory will provide only dressed-quark core masses;EBAC or EBAC-like tools necessary for mesons and baryons
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Baryon Spectrum
LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
73
Masses of ground and excited-state hadronsHannes L.L. Roberts, Lei Chang, Ian C. Cloët and Craig D. Roberts, arXiv:1101.4244 [nucl-th] Few Body Systems (2011) pp. 1-25
0+ 77%
1+ 23% 100% 100% 100%
0- 51% 43%
1- 49% 57% 100% 100%
diquark contentFascinating suggestion: nucleon’s first excited state = almost entirely axial-vector diquark, despite the dominance of scalar diquark in ground state
Owes fundamentally to close relationship between scalar diquark and pseudoscalar mesonAnd this follows from dynamical chiral symmetry breaking
74
Nucleon to Roper Transition Form Factors Extensive CLAS @ JLab Programme has produced the first
measurements of nucleon-to-resonance transition form factors
Theory challenge is toexplain the measurements
Notable result is zero in F2p→N*,
explanation of which is a realchallenge to theory.
DSE study connects appearanceof zero in F2
p→N* with axial-vector-diquark dominance in Roper resonance and structure of form factors of J=1 state
LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
I. Aznauryan et al., Results of the N* Program at JLabarXiv:1102.0597 [nucl-ex]
Preliminary
I.C. Cloët, C.D. Roberts, et al.In progress
75
Nucleon to Roper Transition Form Factors
Tiator and Vanderhaeghen – in progress– Empirically-inferred light-front-transverse
charge density– Positive core plus negative annulus
Readily explained by dominance of axial-vector diquark – Considering isospin and charge– Negative d-quark twice as likely to be
delocalised from always-positive core than positive u-quark
LightCone 2011, SMU 23-27 May - 77pgs
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
{uu}
d
2 {ud}
u
1+
76
Epilogue
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Epilogue
Dynamical chiral symmetry breaking (DCSB) – mass from nothing for 98% of visible matter – 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 Comprehensive treatment of vast body of observablesEssential 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.”
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
McLerran & PisarskiarXiv:0706.2191 [hep-ph]
Confinement is almost Certainly the origin of DCSB
e.g., BaBar anomaly
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Just in case …
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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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
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Craig Roberts: Dyson-Schwinger Equations and Continuum QCD.
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Neutron Structure Function at high x
SU(6) symmetry
pQCD, uncorrelated Ψ
0+ qq only
Deep inelastic scattering – the Nobel-prize winning quark-discovery experiments
Reviews: S. Brodsky et al.
NP B441 (1995) W. Melnitchouk & A.W.Thomas
PL B377 (1996) 11 N. 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]
Distribution of neutron’s momentum amongst quarks on the valence-quark domainLightCone 2011, SMU 23-27 May - 77pgs