SLIDE 26 A (semi) relativistic effective theory NR Green’s functions
b b H(E)
SR = M3 + eQ0 b
' + (3 + i2) b π2 2M − i2 M (S · b π)2 + e 2M2 (1 + 1) × iC(0) h b E · b π − SiSj b Ej b πi i − 2C(2)
1 (r · b
E) + 2C(2)
3
r · b E − 1 2(SiSj + SjSi)ri b Ej
2M2 (1 − 1) h b π · b E − SiSj b πj b Ei i + O ✓ 1 M4 , F 2 ◆ .(35)
G i d dt ⌥ b H(±)
NR(b
π, b x3)
λ,λ0(x, t; x0, t0) = iδ3(x x0)δ(t t0)δλ,λ
for ±(t t0) > 0, a
Relativistic Green’s functions
dt
b HSR h i d
dt b
HSR i GSR(x, t; x0, t0) = iδ(x x0)δ(t t0) c Hamiltonian
A NR effective theory
b b H(±)
NR = M I3⇥3 ± eQ0ϕ I3⇥3 + b
π2 2M I3⇥3 ⌥ e(µ1 Q0) 2M2 S · ( b E ⇥ b π) ± ie(µ1 Q0) 4M2 S · (r ⇥ b E) ⌥hr2iE 6 r · b E I3⇥3 ⌥ Q2 4 SiSj + SjSi 2 3S2δij
Ej + O ✓ 1 M3 , F 2 ◆ . (84)
Lattice QCD correlation functions
Cαβ(x, τ; x0, τ 0) = h0|[Oψ(x, τ)]α[Oψ†(x0, τ 0)]β|0iAµ
Transformed correlation functions
1 ) M AT C H I N G T O C O R R E L AT I O N F U N C T I O N S
b C(±)
MS,M0
S(x, τ; x0, τ 0) = P(±) ⌦ T(MS) U(x; b
p)C(x, τ; x0, τ 0)U1(x0; b p0) P(±) ⌦ T T
(MS)