Chiral Effective Field Theory Inspired by Tony€¦ · Chiral Effective Field TheoryInspired by...
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Chiral Effective Field TheoryInspired by Tony
Derek Leinweber
Key Contributors
Ian Cloet, Ding Lu, Tony Thomas, Kazuo Tsushima,
Ping Wang, Stewart Wright, Ross Young
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Overview
1. “Baryon masses from lattice QCD: Beyond the perturbativechiral regime”D. B. Leinweber, A. W. Thomas, K. Tsushima and S. V. WrightPhys. Rev. D 61, 074502 (2000) [arXiv:hep-lat/9906027]102 Citations
2. “Nucleon magnetic moments beyond the perturbative chiralregime”D. B. Leinweber, D. H. Lu and A. W. ThomasPhys. Rev. D 60, 034014 (1999) [arXiv:hep-lat/9810005]89 Citations
3. “Physical nucleon properties from lattice QCD”D. B. Leinweber, A. W. Thomas and R. D. YoungPhys. Rev. Lett. 92, 242002 (2004) [arXiv:hep-lat/0302020]86 Citations
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Overview
4. “Chiral analysis of quenched baryon masses”R. D. Young, D. B. Leinweber, A. W. Thomas and S. V. WrightPhys. Rev. D 66, 094507 (2002) [arXiv:hep-lat/0205017]83 Citations
5. “Precise determination of the strangeness magnetic moment ofthe nucleon”D.B. Leinweber, S. Boinepalli, I.C. Cloet, A.W. Thomas, A.G.Williams, R.D. Young, J.M. Zanotti, J.B. Zhang,Phys. Rev. Lett. 94, 212001 (2005) [arXiv:hep-lat/0406002]73 Citations
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OverviewEarly Ideas – The Cloudy Bag Model and the Padé
Both small and large mπ limits are important!
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OverviewEarly Ideas – The Cloudy Bag Model and the Padé
Both small and large mπ limits are important!
Finite-Range Regularised Chiral Effective Field TheoryLoop integrals should become small for large mπ.
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OverviewEarly Ideas – The Cloudy Bag Model and the Padé
Both small and large mπ limits are important!
Finite-Range Regularised Chiral Effective Field TheoryLoop integrals should become small for large mπ.
Quenched Chiral Perturbation TheoryModification of meson-baryon verticesIncorporation of light η′ mesonCorrecting the Quenched Approximation
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OverviewEarly Ideas – The Cloudy Bag Model and the Padé
Both small and large mπ limits are important!
Finite-Range Regularised Chiral Effective Field TheoryLoop integrals should become small for large mπ.
Quenched Chiral Perturbation TheoryModification of meson-baryon verticesIncorporation of light η′ mesonCorrecting the Quenched Approximation
Fascinating aspects of baryon structure.
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Early Ideas – Proton Magnetic Moment
0.0 0.5 1.0 1.5 2.0mπ
2 (GeV
2)
0.5
1.0
1.5
2.0
2.5
3.0
µ p
LDWWDLCBMFitMIT
D.B. Leinweber, D.H. Lu, A.W. Thomas, Phys. Rev. D60, 034014 (1999)
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Early Ideas – The PadéSeries expansion of µp(n) in powers of mπ is not a usefulapproximation for mπ larger than the physical mass.
The simple Padé approximant:
µp(n) =µ0
1 − χ mπ/µ0 + β m2π
,
Builds in the Dirac moment at moderately large m2π
Has the correct LNA behavior of chiral perturbation theory
µ = µ0 + χmπ,
with χ a model independent constant, as m2π → 0.
Two-parameter fits to lattice results proceed byFixing χ at the value given by chiral perturbation theory,Optimizing µ0 and β.
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Proton Magnetic Moment
0.0 0.5 1.0 1.5 2.0mπ
2 (GeV
2)
0.5
1.0
1.5
2.0
2.5
3.0
µ p
LDWWDLCBMFitMIT
D.B. Leinweber, D.H. Lu, A.W. Thomas, Phys. Rev. D60, 034014 (1999)
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Neutron Magnetic Moment
0.0 0.5 1.0 1.5 2.0mπ
2 (GeV
2)
−2.0
−1.5
−1.0
−0.5
0.0
µ n
LDWWDLCBMFitMIT
D.B. Leinweber, D.H. Lu, A.W. Thomas, Phys. Rev. D60, 034014 (1999)
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Chiral Effective Field Theory
General low-energy expansion about chiral limit (mq = 0)
MN = {Terms Analytic in mq} + {Chiral loop corrections}
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Chiral Effective Field Theory
General low-energy expansion about chiral limit (mq = 0)
MN = {Terms Analytic in mq} + {Chiral loop corrections}
Analytic termsCoefficients are not constrained by chiral symmetryTo be determined via analysis of Lattice QCD resultsRelated to the Low Energy Constants of χPT
Chiral loopsPredict nonanalytic behaviour in the quark massCoefficients are known and are model independent
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Chiral Effective Field Theory
General low-energy expansion about chiral limit (mq = 0)
Common to formulate the expansion in terms of m2π ∼ mq
MN = {a0 + a2m2π + a4m
4π + a6m
6π + · · · }
+{χπ Iπ(mπ) + χπ∆ Iπ∆(mπ) + · · · }
Iπ =
Iπ∆ =
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Regularisation of Loop Integrals
Consider the self-energy of the nucleon in heavy-baryon χPT
χπIπ(mπ) = −3 g2
A
32 π f2π
2
π
∫
∞
0
dkk4
k2 + m2
with gA = 1.26 and fπ = 0.093 GeV.
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Regularisation of Loop Integrals
Consider the self-energy of the nucleon in heavy-baryon χPT
χπIπ(mπ) = −3 g2
A
32 π f2π
2
π
∫
∞
0
dkk4
k2 + m2
Standard approach: dimensional regularisation, ǫ → 0
Iπ → ∞ + ∞m2π + m3
π
a0 and a2 undergo an infinite renormalisation
MN = {a0 + a2m2π + a4m
4π + a6m
6π + · · · }
+{χπIπ(mπ) + χπ∆Iπ∆(mπ) + · · · }
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Regularisation of Loop Integrals
Consider the self-energy of the nucleon in heavy-baryon χPT
χπIπ(mπ) = −3 g2
A
32 π f2π
2
π
∫
∞
0
dkk4
k2 + m2
Standard approach: dimensional regularisation, ǫ → 0
Iπ → ∞ + ∞m2π + m3
π
Nucleon expansion −→
MN = c0 + c2m2π + χπm3
π + c4m4π + · · ·
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Lattice QCD and Dim RegχPT
CP-PACS collaboration results Phys. Rev. D65 (2002) 054505
0.2 0.4 0.6 0.8 1mΠ
2 HGeV2L
1
1.2
1.4
1.6
1.8
2m
NHG
eVL
A: c0 + c2m2π
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Lattice QCD and Dim RegχPT
CP-PACS collaboration results Phys. Rev. D65 (2002) 054505
0.2 0.4 0.6 0.8 1mΠ
2 HGeV2L
1
1.2
1.4
1.6
1.8
2m
NHG
eVL
B: c0 + c2m2π + χπ m3
π
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Lattice QCD and Dim RegχPT
CP-PACS collaboration results Phys. Rev. D65 (2002) 054505
0.2 0.4 0.6 0.8 1mΠ
2 HGeV2L
1
1.2
1.4
1.6
1.8
2m
NHG
eVL
C: c0 + c2m2π + χπ m3
π + c4m4π
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Slow RATE of Convergence
Origin lies in regularisation prescription
DR: Large contributions to integral from k → ∞ portion of integral
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Slow RATE of Convergence
Origin lies in regularisation prescription
DR: Large contributions to integral from k → ∞ portion of integral
Short distance physics is highly overestimated!
Always require large analytic terms at next orderno sign of convergence
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Overcoming This Problem
KEEP low-energy (infrared) structure of χPT
REMOVE the incorrect short-distance contributions associatedwith ultraviolet behaviour of loop integrals
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Overcoming This Problem
KEEP low-energy (infrared) structure of χPT
REMOVE the incorrect short-distance contributions associatedwith ultraviolet behaviour of loop integrals
INTRODUCE “separation-scale” to identify short- andlong-distance physics
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Overcoming This Problem
KEEP low-energy (infrared) structure of χPT
REMOVE the incorrect short-distance contributions associatedwith ultraviolet behaviour of loop integrals
INTRODUCE “separation-scale” to identify short- andlong-distance physics
Natural scale to be associated is the physical size of the pionsource
Axial-vector form factor of the nucleon
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Regularisation: Revisited
Use a Finite-Range Regulator (FRR)
MN = {aΛ0 + aΛ
2 m2π + aΛ
4 m4π + aΛ
6 m6π + · · · }
+{χπ Iπ(mπ, Λ) + χπ∆ Iπ∆(mπ, Λ) + · · · }
Loop integral is cutoff in momentum space at mass scale Λ
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Regularisation: Revisited
Use a Finite-Range Regulator (FRR)
MN = {aΛ0 + aΛ
2 m2π + aΛ
4 m4π + aΛ
6 m6π + · · · }
+{χπ Iπ(mπ, Λ) + χπ∆ Iπ∆(mπ, Λ) + · · · }
Loop integral is cutoff in momentum space at mass scale Λ
Different from standard QFTΛ remains finite for EFTUltraviolet suppression for loop momenta k > Λ
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Finite-Range Regularisation
Consider the self-energy of the nucleon in heavy-baryon χPT
Iπ(mπ) =2
π
∫
∞
0
dkk4 u2(k)
k2 + m2
with a dipole regulator (on each NNπ vertex)
u(k) =
(
Λ2
Λ2 + k2
)2
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Finite-Range Regularisation
Consider the self-energy of the nucleon in heavy-baryon χPT
Iπ(mπ) =2
π
∫
∞
0
dkk4 u2(k)
k2 + m2
with a dipole regulator (on each NNπ vertex)
u(k) =
(
Λ2
Λ2 + k2
)2
Iπ =1
16
Λ5(m2π + 4mπΛ + Λ2)
(mπ + Λ)4
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Model-Independent Nonanalytic Behavior
Taylor expand
Iπ =1
16
Λ5(m2π + 4mπΛ + Λ2)
(mπ + Λ)4
about mπ = 0
Iπ →Λ3
16−
5Λ
16m2
π + m3π −
35
16Λm4
π +4
Λ2m5
π + . . .
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Model-Independent Nonanalytic Behavior
Taylor expand
Iπ =1
16
Λ5(m2π + 4mπΛ + Λ2)
(mπ + Λ)4
about mπ = 0
Iπ →Λ3
16−
5Λ
16m2
π + m3π −
35
16Λm4
π +4
Λ2m5
π + . . .
Iπ contains a resummation of the chiral expansion such that
Iπ → 0 as mπ becomes large.
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Model-Independent Nonanalytic Behavior
Taylor expand
Iπ =1
16
Λ5(m2π + 4mπΛ + Λ2)
(mπ + Λ)4
about mπ = 0
Iπ →Λ3
16−
5Λ
16m2
π + m3π −
35
16Λm4
π +4
Λ2m5
π + . . .
Iπ contains a resummation of the chiral expansion such that
Iπ → 0 as mπ becomes large.
In accord with the lattice simulation results.
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Renormalised Expansion Coefficients
Combine the analytic terms of
MLNAN = a0 + a2m
2π + χπIπ(mπ) + a4m
4π
andIDIPπ →
Λ3
16−
5Λ
16m2
π + m3π −
35
16Λm4
π + . . .
Recover the renormalized expansion coefficients ci
MLNAN =
(
a0 + χπ
Λ3
16
)
+
(
a2 − χπ
5Λ
16
)
m2π + χπm3
π
+
(
a4 − χπ
35
16Λ
)
m4π + · · ·
= c0 + c2m2π + χπm3
π + c4m4π
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Renormalised Expansion (FRR)
Any value of Λ is allowed!
MLNAN =
(
a0 + χπ
Λ3
16
)
+
(
a2 − χπ
5Λ
16
)
m2π + χπm3
π
+
(
a4 − χπ
35
16Λ
)
m4π + · · ·
= c0 + c2m2π + χπm3
π + c4m4π
To any finite order, FRR is mathematically equivalent toDimensional Regularisation.
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Renormalised Expansion (FRR)
Any value of Λ is allowed!
MLNAN =
(
a0 + χπ
Λ3
16
)
+
(
a2 − χπ
5Λ
16
)
m2π + χπm3
π
+
(
a4 − χπ
35
16Λ
)
m4π + · · ·
= c0 + c2m2π + χπm3
π + c4m4π
To any finite order, FRR is mathematically equivalent toDimensional Regularisation.
Within the power-counting regime of χPTFRR EFT is not a modelHigher-order terms are truly negligible.
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The Power Counting Regime
Renormalised coefficients c0, c2 and c4 are fixed.
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Application of FRR Result
Fit the resummed expression to lattice QCD results
MN = aΛ0 + aΛ
2 m2π + χπ Iπ(mπ, Λ) + aΛ
4 m4π
with
Iπ =1
16
Λ5(m2π + 4mπΛ + Λ2)
(mπ + Λ)4
andΛ = 0.8 GeV
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Lattice QCD and FRR EFT
Dipole Regularisation
0.2 0.4 0.6 0.8 1mΠ
2 HGeV2L
1
1.2
1.4
1.6
1.8
2m
NHG
eVL
A: a0 + a2m2π
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Lattice QCD and FRR EFT
Dipole Regularisation
0.2 0.4 0.6 0.8 1mΠ
2 HGeV2L
1
1.2
1.4
1.6
1.8
2m
NHG
eVL
B: a0 + a2m2π + χπIπ
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Lattice QCD and FRR EFT
Dipole Regularisation
0.2 0.4 0.6 0.8 1mΠ
2 HGeV2L
1
1.2
1.4
1.6
1.8
2m
NHG
eVL
C: a0 + a2m2π + χπIπ + a4m
4π
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Next Leading Order
MNLNAN = aΛ
0 + aΛ2 m2
π + χπIπ(mπ, Λ) + aΛ4 m4
π
+χπ∆Iπ∆(mπ, Λ) + χtadπ Itad
π (mπ, Λ) + aΛ6 m6
π
Iπ∆ = ∼ m4π lnmπ
Itadπ = ∼ m4
π lnmπ
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FRR Regulators
Alternatives:Sharp cut-off
θ(Λ − k)
Monopole(
Λ2
Λ2 + k2
)
Gaussian
exp(−k2
Λ2)
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MNLNAN Extrapolation
0.0 0.2 0.4 0.6 0.8 1.0mΠ
2 HGeV2L
0.8
1.0
1.2
1.4
1.6
1.8
MNHG
eVL
DIPOLE
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MNLNAN Extrapolation
0.0 0.2 0.4 0.6 0.8 1.0mΠ
2 HGeV2L
0.8
1.0
1.2
1.4
1.6
1.8
MNHG
eVL
SHARP CUTOFF
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MNLNAN Extrapolation
0.0 0.2 0.4 0.6 0.8 1.0mΠ
2 HGeV2L
0.8
1.0
1.2
1.4
1.6
1.8
MNHG
eVL
MONOPOLE
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MNLNAN Extrapolation
0.0 0.2 0.4 0.6 0.8 1.0mΠ
2 HGeV2L
0.8
1.0
1.2
1.4
1.6
1.8
MNHG
eVL
GAUSSIAN
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MNLNAN Extrapolation
0.0 0.2 0.4 0.6 0.8 1.0mΠ
2 HGeV2L
0.8
1.0
1.2
1.4
1.6
1.8
MNHG
eVL
DIMENSIONAL REGULARISATION
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Low Energy Coefficients
NLNA results are largely independent of the model!
Regulator c0 c2 c4
Dipole 0.922 2.49 18.9
Sharp cutoff 0.923 2.61 15.3
Monopole 0.923 2.45 20.5
Gaussian 0.923 2.48 18.3
Dim. reg. 0.875 3.14 7.2
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Series Truncation
Residual series coefficients
Regulator a4 (GeV−3) a6 (GeV−5)Dipole −0.49 0.09
Sharp cutoff −0.55 0.12
Monopole −0.49 0.09
Gaussian −0.50 0.10
Dim. reg. 8.9 0.38
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FRR Summary
To any finite order, FRR is mathematically equivalent toDimensional Regularisation.
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FRR Summary
To any finite order, FRR is mathematically equivalent toDimensional Regularisation.
Lattice QCD simulation results are generally smooth slowlyvarying functions of the quark mass.
Higher-order terms of the DR expansion must sumapproximately to zero.
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FRR Summary
To any finite order, FRR is mathematically equivalent toDimensional Regularisation.
Lattice QCD simulation results are generally smooth slowlyvarying functions of the quark mass.
Higher-order terms of the DR expansion must sumapproximately to zero.
Finite-range regularisation resums the chiral expansion of DR.Linear combinations of higher order DR terms appearalready in one-loop calculations.
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FRR Summary
To any finite order, FRR is mathematically equivalent toDimensional Regularisation.
Lattice QCD simulation results are generally smooth slowlyvarying functions of the quark mass.
Higher-order terms of the DR expansion must sumapproximately to zero.
Higher order DR terms obtained in FRR EFT sum such that loopcontributions vanish as the quark mass becomes large.
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FRR Summary
To any finite order, FRR is mathematically equivalent toDimensional Regularisation.
Lattice QCD simulation results are generally smooth slowlyvarying functions of the quark mass.
Higher-order terms of the DR expansion must sumapproximately to zero.
Higher order DR terms obtained in FRR EFT sum such that loopcontributions vanish as the quark mass becomes large.
Regulator parameter, Λ, shifts strength between FRR loopintegrals and the residual expansion of terms analytic in thequark mass.
Provides a new mechanism to optimize the convergenceproperties of the chiral expansion.
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Optimal Regularisation?
Regulator parameter Λ should be constrained by lattice QCDresults.
Several criteria were under investigation.
See Jonathan Hall’s poster tomorrow for the solution.
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Proton Moment in Quenched QCD
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Proton Radius in Quenched QCD
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Quenched Chiral Nonanalytic Behavior
“Disconnected” sea-quark loops are absent, modifying vertices.
(a) (b)
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Quenched Chiral Nonanalytic Behavior
“Disconnected” sea-quark loops are absent, modifying vertices.
(a) (b)
η′-meson mass remains degenerate with the pion and cancontribute new nonanalytic terms to the chiral expansion.
(a) (b)
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Quenched Quark Flow for Form Factors
Hadronic Level
Quark Flow Level
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Finite-Range Regularisation
Finite Range Regulator
µp = aΛ0 +µp χη Iη(mπ, Λ)+χπ Iπ(mπ, Λ)+χK IK(mK , Λ)+aΛ
2 m2π+· · ·
Kaon mass relation
m2K = m
(0) 2K +
1
2m2
π
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Finite-Range Regularisation
Finite Range Regulator
µp = aΛ0 +µp χη Iη(mπ, Λ)+χπ Iπ(mπ, Λ)+χK IK(mK , Λ)+aΛ
2 m2π+· · ·
Limit mπ → 0
µp = c0 + µp χη
[
l0 + log
(
m2π
Λ2
)]
+ χπ mπ + χK mK + c2 m2π + · · ·
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Finite-Range Regularisation
Finite Range Regulator
µp = aΛ0 +µp χη Iη(mπ, Λ)+χπ Iπ(mπ, Λ)+χK IK(mK , Λ)+aΛ
2 m2π+· · ·
Limit mπ → 0
µp = c0 + µp χη
[
l0 + log
(
m2π
Λ2
)]
+ χπ mπ + χK mK + c2 m2π + · · ·
Dimensional Regularisation
µp = c0+µp χη
[
logΛ2
Λ′2+ log
(
m2π
Λ2
)]
+χπ mπ+χK mK+c2 m2π+· · ·
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Direct Loop Contributions
(a) Full QCD = (b) + (c)
(b) Valence in Full & Quenched QCD
(c) Direct sea-quark loop
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Direct Loop Contributions
(a) Full QCD = (b) + (c)
(b) Valence in Full & Quenched QCD
(c) Direct sea-quark loop
Phys. Rev. D69 (2004) 014005[arXiv:hep-lat/0211017].
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Indirect Loop Contributions
(a) Full QCD = (b) + (c)
(b) Valence in Full & Quenched QCD
(c) Valence only in Full QCD
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Indirect Loop Contributions
(a) Full QCD = (b) + (c)
(b) Valence in Full & Quenched QCD
(c) Valence only in Full QCD
(c) Indirect sea-quark loop
(c) is removed upon quenching
Phys. Rev. D69 (2004) 014005[arXiv:hep-lat/0211017].
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Coefficientsχπχπχπ and χKχKχK (µNµNµN /GeV)
Quark Int. Total Direct Loop Valence Quenched
2 up Nπ −6.87 +4.12 −11.0 −3.33
ΛK −3.68 0 −3.68 0
ΣK −0.15 0 −0.15 0
dp Nπ +6.87 +4.12 +2.75 +3.33
ΣK −0.29 0 −0.29 0
sp ΛK +3.68 +3.68 0 0
ΣK +0.44 +0.44 0 0
2 uΣ+ Σπ −2.16 +2.16 −4.32 0
Λπ −1.67 +1.67 −3.33 0
NK 0 +0.29 −0.29 −0.29
ΞK −6.87 0 −6.87 −3.04
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Finite Volume ArtifactsDirectly incorporate finite-volume effects into the chiralexpansion.
General expansion for the small parameters mπ and 1/L
MN = {Terms Analytic in m2π and 1/L}
+{Volume-modified Chiral loop corrections}
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Finite Volume ArtifactsDirectly incorporate finite-volume effects into the chiralexpansion.
General expansion for the small parameters mπ and 1/L
MN = {Terms Analytic in m2π and 1/L}
+{Volume-modified Chiral loop corrections}
Performed with the constraint mπL ≫ 1.Corrections are perturbative in the pion cloud.Analytic terms in 1/L are small by constraint.
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Finite Volume ArtifactsDirectly incorporate finite-volume effects into the chiralexpansion.
General expansion for the small parameters mπ and 1/L
MN = {Terms Analytic in m2π and 1/L}
+{Volume-modified Chiral loop corrections}
Performed with the constraint mπL ≫ 1.Corrections are perturbative in the pion cloud.Analytic terms in 1/L are small by constraint.
The finite periodic volume of the lattice modifies integrals
∫
d3k →
(
2π
L3
)3∑
kx,ky,kz
.
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uuu quark in the Proton: Quenched QCD
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uuu quark in the Proton: Quenched QCD
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QuenchedFinite Volume Moments
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QuenchedFinite Volume Moments
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Correcting the Quenched Approximation
Studied a matched set of quenched QCD and full QCD gaugeconfigurations from the MILC Collaboration
Fit the nucleon mass in quenched QCD and in full QCDWith Finite-Range Regularised quenched EFT and full EFTRegulator Parameter Λ = 0.8
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Correcting the Quenched Approximation
Studied a matched set of quenched QCD and full QCD gaugeconfigurations from the MILC Collaboration
Fit the nucleon mass in quenched QCD and in full QCDWith Finite-Range Regularised quenched EFT and full EFTRegulator Parameter Λ = 0.8
Discovered the coefficients of analytic terms in quenched QCDand full QCD
Are the same within errors
MN = {aΛ0 + aΛ
2 m2π + aΛ
4 m4π + aΛ
6 m6π + · · · }
+{χπ Iπ(mπ, Λ) + χπ∆ Iπ∆(mπ, Λ) + · · · }
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Correcting the Quenched Approximation
Studied a matched set of quenched QCD and full QCD gaugeconfigurations from the MILC Collaboration
Fit the nucleon mass in quenched QCD and in full QCDWith Finite-Range Regularised quenched EFT and full EFTRegulator Parameter Λ = 0.8
Discovered the coefficients of analytic terms in quenched QCDand full QCD
Are the same within errors
Leads to the concept of separatingThe pion cloud
Affected by quenching and finite volumeThe core (the source of the pion cloud)
Invariant to quenching and finite volume artifacts.
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MILC Collaboration Simulations
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Coefficients of Analytic Terms
For case of Regulator Parameter Λ = 0.8
Nucleon
a0 a2 a4
N (Dynamical) 1.23(1) 1.13(8) −0.4(1)
N (Quenched) 1.20(1) 1.10(8) −0.4(1)
Units are in appropriate powers of GeV.
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Coefficients of Analytic Terms
For case of Regulator Parameter Λ = 0.8
Nucleon
a0 a2 a4
N (Dynamical) 1.23(1) 1.13(8) −0.4(1)
N (Quenched) 1.20(1) 1.10(8) −0.4(1)
Units are in appropriate powers of GeV.
Delta
a0 a2 a4
∆ (Dynamical) 1.40(3) 1.1(2) −0.6(3)
∆ (Quenched) 1.43(3) 0.8(2) −0.1(3)
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Nucleon and Delta Masses
0 0.2 0.4 0.6 0.8mΠ2 HGeV2
L
1
1.2
1.4
1.6
1.8
2m
BHG
eVL
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Quenched Baryon Masses
η ’ η ’
+
++
ππ
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NucleonQuenchedχPT Fit
0 0.2 0.4 0.6 0.8mΠ2 HGeV2
L
1
1.2
1.4
1.6
1.8
2m
BHG
eVL
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Delta QuenchedχPT Fit
0 0.2 0.4 0.6 0.8mΠ2 HGeV2
L
1
1.2
1.4
1.6
1.8
2m
BHG
eVL
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Correct Chiral Nonanalytic Behavior
+π π
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Correct the Quenched Approximation
0 0.2 0.4 0.6 0.8mΠ2 HGeV2
L
1
1.2
1.4
1.6
1.8
2m
BHG
eVL
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Correct Moments to Full QCD
Quenched QCD
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Correct Moments to Full QCD
Quenched QCD
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Correct Moments to Full QCD
Quenched QCD
Full QCD
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Indirect Loop Contributions
(a) Full QCD = (b) + (c)
(b) Valence in Full & Quenched QCD
(c) Valence only in Full QCD
(c) Indirect sea-quark loop
(c) is removed upon quenching
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Coefficientsχπχπχπ and χKχKχK (µNµNµN /GeV)
Quark Int. Total Direct Loop Valence Quenched
2 up Nπ −6.87 +4.12 −11.0 −3.33
ΛK −3.68 0 −3.68 0
ΣK −0.15 0 −0.15 0
dp Nπ +6.87 +4.12 +2.75 +3.33
ΣK −0.29 0 −0.29 0
sp ΛK +3.68 +3.68 0 0
ΣK +0.44 +0.44 0 0
2 uΣ+ Σπ −2.16 +2.16 −4.32 0
Λπ −1.67 +1.67 −3.33 0
NK 0 +0.29 −0.29 −0.29
ΞK −6.87 0 −6.87 −3.04
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uuu quark in the Proton: Quenched QCD
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Valenceuuu quark in the Proton: Full QCD
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Direct Loop Contributions
(a) Full QCD = (b) + (c)
(b) Valence in Full & Quenched QCD
(c) Direct sea-quark loop
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Coefficientsχπχπχπ and χKχKχK (µNµNµN /GeV)
Quark Int. Total Direct Loop Valence Quenched
2 up Nπ −6.87 +4.12 −11.0 −3.33
ΛK −3.68 0 −3.68 0
ΣK −0.15 0 −0.15 0
dp Nπ +6.87 +4.12 +2.75 +3.33
ΣK −0.29 0 −0.29 0
sp ΛK +3.68 +3.68 0 0
ΣK +0.44 +0.44 0 0
2 uΣ+ Σπ −2.16 +2.16 −4.32 0
Λπ −1.67 +1.67 −3.33 0
NK 0 +0.29 −0.29 −0.29
ΞK −6.87 0 −6.87 −3.04
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uuu quark in the Proton: Full QCD
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uuu quark in Σ+Σ+Σ+
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uuu quark in ppp
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uuu quark in nnn
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uuu quark in Ξ0Ξ0Ξ0
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sss quark in Ξ0Ξ0Ξ0
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sss quark in ΛΛΛ
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uuu or ddd quark in ΛΛΛ
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Octet Baryon Magnetic Moments
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Octet Baryon Magnetic Moments
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uuu quark in ppp
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uuu quark in nnn
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Proton Charge Radius
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Neutron Charge Radius
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uuu quark in ppp
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uuu quark in Σ+Σ+Σ+
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uuu quark in nnn
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uuu quark in Ξ0Ξ0Ξ0
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sss quark in Ξ0Ξ0Ξ0
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sss quark in ΛΛΛ
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sss quark in ΣΣΣ
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uuu or ddd quark in ΛΛΛ
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Octet Baryon Charge Radii
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Proton Moment in Full QCD
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Power Counting: O(m1π)O(m1π)O(m1π)
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Power Counting: O(m2π)O(m2π)O(m2π)
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Power Counting: O(m3π)O(m3π)O(m3π)
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Power Counting: O(m4π)O(m4π)O(m4π)
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Power Counting: O(m5π)O(m5π)O(m5π)
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Power Counting: O(m6π)O(m6π)O(m6π)
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Power Counting: O(m8π)O(m8π)O(m8π)
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Power Counting: O(m10π )O(m10π )O(m10π )
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Power Counting: O(m20π )O(m20π )O(m20π )
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Power Counting: O(m40π )O(m40π )O(m40π )
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Power Counting: O(m80π )O(m80π )O(m80π )
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Power Counting: O(m160π )O(m160π )O(m160π )
Chiral Effective Field TheoryInspired by Tony – p.92/101
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∆++∆++∆++ Decay in Full QCD
Chiral Effective Field TheoryInspired by Tony – p.93/101
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QCD is Flavour Blind
Chiral Effective Field TheoryInspired by Tony – p.94/101
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But there is nouuuuuuuuu proton!
Chiral Effective Field TheoryInspired by Tony – p.95/101
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Quenched∆∆∆: Negative Metric Contribution
Chiral Effective Field TheoryInspired by Tony – p.96/101
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p and ∆+ Magnetic Moments
Chiral Effective Field TheoryInspired by Tony – p.97/101
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p/∆+ Magnetic Moment Ratio in QQCD
Chiral Effective Field TheoryInspired by Tony – p.98/101
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p/∆+ Magnetic Ratio in Full QCD
Chiral Effective Field TheoryInspired by Tony – p.99/101
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The Structure of the Nucleon
Chiral Effective Field TheoryInspired by Tony – p.100/101
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Chiral Effective Field TheoryInspired by Tony – p.101/101