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Hadron Phenomenology from QuenchedOverlap Fermions
D. Galletly1, M. Gürtler2, R. Horsley1, K. Koller3, P. Rakow4,G. Schierholz2, T. Streuer2
2NIC/DESY Zeuthen4University of Liverpool
1University of Edinburgh3University of Munich
Nicosia, Semptember 2005
Simulation DetailsGauge action: Tadpole-Improved Lüscher-Weisz
S = β∑
plaq
(1 − 13 re tr Uplaq) + βrect
∑
rect
(1 − 13 re tr Urect)
+βpar
∑
par
(1 − 13 re tr Upar)
Fermion action: Overlap Operator
D = ρ(1 + γ5sgn(HW (−ρ)))
Lattices:V β confs.
12324 7.60 15016332 8.00 30024348 8.45 200
Pion mass range: 300MeV..850MeV
Simulation DetailsTwo Point Function:
C2(t) = 12(1 + γ4)αβ〈Bα(t)Bβ(0)〉
Bα(t): Jacobi-smeared Proton OperatorThree Point Function:
CO3 (t , τ) = Γαβ〈Bα(t)O(τ)Bβ(0)〉
with Γ = 12(1 + γ4) (unpolarised) or 1
2(1 + γ4)γ5γ2 (polarised)For 0 � τ � t : C3(t ,τ)
C2(t)∝ 〈p|O|p〉
0 10 20 30 40
t
0
0.5
1
Lattice Spacing from fπβ = 7.6 β = 8.0 β = 8.45
0 0.2 0.4amq
0.1
0.2
af π
0 0.2amq
0.1
af π
0 0.2amq
0.1
af π
fπ = f + c · mq
β a(fm)
7.60 0.229(4)8.00 0.154(2)8.45 0.105(1)
Pion Mass
β = 7.6 β = 8.0 β = 8.45
0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 0.5 0.55amq
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
m2 π(G
eV
2)
0 0.02 0.04 0.06 0.08 0.1 0.12 0.14 0.16 0.18 0.2 0.22 0.24amq
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
m2 π(G
eV
2)
0 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1 0.11 0.12 0.13 0.14 0.15 0.16amq
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
m2 π(G
eV
2)
Quenched Chiral Log in mπ
0 0.02 0.04 0.06 0.08 0.1 0.12 0.14amq
1.4
1.5
1.6
1.7
1.8
am2 π/m
q
Quenched Chiral Perturbation Theory:
m2π = Amq
(
1 + δ logAmq
Λ2χ
)
+ bm2q + . . .
with
δ =m2
048π2f 2
Fit yields δ = 0.18(2), corresponding to
m0 = 850(45)MeV
Vector Meson Mass
Quenched Chiral Perturbation Theory:
mρ = cρ0 + cρ1mπ + cρ2m2π + · · ·
0 0.1 0.2 0.3 0.4 0.5amπ
0.4
0.5
0.6
amρ
Nucleon Mass
Quenched Chiral Perturbation Theory:
mN = cN0 + cN
1 mπ + cN2 m2
π + · · ·
0 0.1 0.2 0.3 0.4 0.5amπ
0.4
0.5
0.6
0.7
0.8
0.9
amN
Scaling ?
Vector meson Nucleon
0 200 400 600 800 1000
mπ(MeV)
600
800
1000
1200
mρ(M
eV)
β=7.6β=8.0β=8.45
0 200 400 600 800 1000
mπ(MeV)
600
800
1000
1200
mρ(M
eV)
β=7.6β=8.0β=8.45
→ Discretization errors small
Renormalisation - Axial Current
Ward Identity:
ZA〈∂4A4(t)P(0)〉 = 2m〈P(t)P(0)〉
0 0.05 0.1 0.15 0.2m
1.4
1.41
1.42
1.43
1.44
β ZA7.6 2.23(5)8.0 1.59(1)
8.45 1.42(1)
Renormalisation - Vector CurrentWard Identity:
ZV 〈N|V u−d4 |N〉 = 1
obtain ZV from ratio
Γαβ〈Bα(0)V u−d4 (τ)Bβ(t)〉
Γαβ〈Bα(0)Bβ(t)〉
0 0.05 0.1amq
1.35
1.4Z V
β ZV ZA7.6 2.00(12) 2.23(5)8.0 1.55(2) 1.59(1)
8.45 1.40(2) 1.41(1)
RenormalisationDivergent Operators: RI − MOM-Scheme (Martinelli,Sachrajda):Consider (non-singlet) quark propagator and quark Three-PointFunctions in Landau Gauge:
S(p) = 〈ψ(p)ψ(p)〉
GO(p) = 〈ψ(p)Oψ(p)〉
Renormalisation Condition:
ZψZO(µ)ΠO(ΓO(p)) = 1 at p2 = µ2
withΓO(p) = S−1(p)GO(p)S−1(p)
andΠO(ΓO(p)) =
112
tr(ΓO,Born(p)−1ΓO(p))
Renormalisation
Zψ determined from
ZψZAΠA(ΓA) = 1
Conversion to MS,2GeV:
Z RGIO = 1/Z RI−MOM,RGI
O (µ)Z RI−MOMO
Z MS(µ′) = Z MS,RGIO (µ′)Z RGI
O
ZS,RGIO (µ) =
(
2b1gS(µ)2)−
dO,12b1 e
R gS (µ)0 dξ
γSO(ξ)
βS(ξ)+
dO,1b1ξ
!
Using perturbative (3-Loop) γ-Function (Gracey, Chetyrkin)
Renormalisation: Scalar Density
Z RI−MOMS Z RGI
S
0 10 20
p2(GeV2)
0.8
1
1.2
1.4
1.6
0 10 20
p2(GeV2)
0.8
1
1.2
1.4
1.6
β Z MSS (2GeV)
7.6 1.82(4)8.0 1.48(2)
8.45 1.29(1)
Renormalisation: Tensor Current
Z RI−MOMT Z RGI
T
0 10 20
p2
1.4
1.6
1.8
2
2.2
2.4
2.6
2.8
3
3.2
3.4
0 10 20
p21.5
1.6
1.7
1.8
1.9
2
2.1
2.2
β Z MST (2GeV)
7.6 2.36(4)8.0 1.73(1)
8.45 1.54(1)
Renormalisation: v2
Z RI−MOMv2
Z RGIv2
0 10 20
p21
2
3
4
5
0 10 20
p21
1.5
2
2.5
3
3.5
4
4.5
5
β Z MSv2
(2GeV)
7.6 2.65(5)8.0 2.11(3)
8.45 1.90(2)
Renormalisation: a1
Z RI−MOMa1
Z RGIa1
0 10 20
p21
2
3
4
5
0 10 20
p21
1.5
2
2.5
3
3.5
4
4.5
5
β Z MSa1
(2GeV)
7.6 2.95(4)8.0 2.21(2)
8.45 1.98(1)
Renormalisation
Comparison to Tadpole-Improved Perturbation Theory(Perlt et al.)β = 8.45, MS(2GeV):
Matrix Element Z MS TI PT Z MS NPgA 1.30 1.42h1 1.33 1.54v2 1.40 1.90a1 1.41 1.98
Large Difference for Operators with Derivative!
Nucleon Structure
Nucleon described by structure functions:I F1, F2 UnpolarisedI g1, g2 PolarisedI h1 Transversity
Operator Product Expansion:
2∫
dxF1(x ,q2)xn−1 = cn(q2)vn + O(1/q2) (n even)
and similar for other structure functions.cn(q2): Wilson Coefficient (perturbative)vn defined by
〈p|γ{µ1↔
Dµ2 . . .↔
Dµn} −Traces|p〉 = 2vn(p{µ1 . . . pµn} − Traces)
Nucleon Structure
Matrix Element OperatorgA ψγ5γ2ψh1 ψγ5σ24ψv2 O44 −
13 (O11 + O22 + O33)
a1 O524
with
Oµν = ψγ{µ↔
Dν} ψ
O5µν = ψγ5γ{µ
↔
Dν} ψ
Axial Charge gA
gA defined by〈p|Au−d
µ |p〉 = gAupγµγ5un
0 0.2 0.4 0.6 0.8 1
m2π(GeV)2
1
1.1
1.2
1.3
1.4
1.5
1.6
β=7.6β=8.0β=8.45
β gA7.6 1.21(7)8.0 1.37(5)
8.45 1.14(5)
Tensor Charge
〈p|ψσµνγ5ψ|p〉 =2
mph1sµpµ
0 0.2 0.4 0.6 0.8 1
m2π(GeV)2
0.9
1
1.1
1.2
1.3
1.4
1.5
1.6
1.7
1.8
1.9
2
2.1
2.2
β=7.6β=8.0β=8.45
β h17.6 1.33(8)8.0 1.35(4)
8.45 1.18(5)
v2
〈p|ψγ{µ↔
Dν} ψ|p〉 = 2v2p{µpν}
0 0.2 0.4 0.6 0.8 1
m2π(GeV)2
0
0.1
0.2
0.3
0.4
0.5
β=7.6β=8.0β=8.45
β v27.6 0.23(3)8.0 0.28(2)
8.45 0.26(2)
a1
〈p|ψγ5γ{µ
↔
Dν} ψ|p〉 = 2a1s{µpν}
0 0.2 0.4 0.6 0.8 1
m2π(GeV)2
0
0.1
0.2
0.3
0.4
0.5
β=7.6β=8.0β=8.45
β a17.6 0.56(7)8.0 0.58(4)
8.45 0.62(4)