有限温度QCD: 相転移、トポロジー、axion
青木保道 素粒子物理学の進展2018 @ 基研
- Aug. 9, 2018
QCD: axion - - PowerPoint PPT Presentation
QCD: axion 2018 @ Aug. 9, 2018 GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV- DW OV index on DW ensemble OV-OV OV
青木保道 素粒子物理学の進展2018 @ 基研
GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV- DW OV index on DW ensemble OV-OV OV index on OV ensemble
5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV
4]
GL-DW GL-OV OV-DW OV-OV
32
3x12, β=4.3
GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV- DW OV index on DW ensemble OV-OV OV index on OV ensemble
5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV
4]
GL-DW GL-OV OV-DW OV-OV
32
3x12, β=4.3
GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV- DW OV index on DW ensemble OV-OV OV index on OV ensemble
5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV
4]
GL-DW GL-OV OV-DW OV-OV
32
3x12, β=4.3
physical ud
GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV- DW OV index on DW ensemble OV-OV OV index on OV ensemble
5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV
4]
GL-DW GL-OV OV-DW OV-OV
32
3x12, β=4.3
physical ud
Sinya Aoki YA Guido Cossu Hidenori Fukaya Shoji Hashimoto Takashi Kaneko Kei Suzuki …
クロスオーバー 一次転移 二次転移
[original Columbia plot: Brown et al 1990]
physical pt. [original Columbia plot: Brown et al 1990]
Fodor, Katz, Szabo: Nature 2006)
アプローチでは未踏
physical pt.
mud ms ∞ ∞
physical pt.
➡U(1)A 回復を示唆[JLQCD16] ➡一次転移の可能性 → χt(m)に飛び? [Pisarski&Wilczek]
physical pt.
physical pt.
external parameter → phase boundary → point of interest
➡ detour the demanding region
physical pt.
1st order 1st order crossover
0.05 0.1 0.15 0.2 0.25
(am u,d)2/5
(µ/T)
2
first order second order B region region
Bonati et al
external parameter → phase boundary → point of interest
➡ detour the demanding region
physical pt.
1st order 1st order crossover
0.05 0.1 0.15 0.2 0.25
(am u,d)2/5
(µ/T)
2
first order second order B region region
Bonati et al
external parameter → phase boundary → point of interest
➡ detour the demanding region
physical pt.
1st order 1st order crossover
physical pt.
1st order 1st order crossover
Nf=2+1 or 3
with both staggered and Wilson
“Surprises in the Columbia plot” (Lapland talk 2018)
physical pt.
1st order 1st order crossover
Nf=2+1 or 3
with both staggered and Wilson
“Surprises in the Columbia plot” (Lapland talk 2018)
現状良く行われる改良
U(1)B SU(Nf)V SU(Nf)A simulation cost Wilson ✓ ✓ × moderate staggered ✓ × U(1) cheep domain wall ✓ ✓ almost exact expensive
✓ ✓ ✓ almost impossible
ψ(n + ψ(n) Uµ(n) a
ψ(n + ˆ µ) ψ(n) Uµ(n) a
O|LQCD = O|QCD + ac1O1 + a2c2O2 . . .
0.01 0.02 0.03 0.04
mf a
1 1.2 1.4 1.6
t0 a
2
~30% difference in a
2
β=3.8 β=3.7
0.02 0.04 0.06 mf 0.1 0.2 Mπ
2
π5 π05 πi5 πi0 πij π0 πi πI 0.02 0.04 0.06 mf 0.1 0.2 0.3 Mπ
2
ξI ξi ξ4 ξiξj ξiξ4 ξ4ξ5 ξiξ5 ξ5
Nf=4, β=3.7
HISQ
0.05 0.1 0.15 0.2 0.25 0.3 Mπ
2 t0
0.0001 0.0002 0.0003 χtop t0
2
β=3.7 β=3.8
does not vanish in Mπ→0 ? better chiral behavior, and better a-scaling
0.05 0.1 0.15 0.2 0.25 0.3 MπI
2 t0
0.0001 0.0002 0.0003 χtop t0
2
β=3.7 β=3.8
(a la sChPT: see Billeter, DeTar, Osborn, PRD2004)
[JLQCD: S.Aoki et al 2017, Nf=2+1 DWF]
2x108 4x108 6x108 8x108 1x109 10 20 30 40 50 χt(MeV4) mMSbar
ud (MeV)
β=4.17, ms=0.04 β=4.17, ms=0.03 β=4.17, ms=0.04 (L=48) β=4.35, ms=0.025 β=4.35, ms=0.018 β=4.47, ms=0.015 ChPT fit (β=4.17) ChPT fit (β>=4.35)
➡ χt ~ O(m4) Cohen ➡ χt |m=0 = 0 & dnχt / dmn|m=0 = 0 Aoki-Fukaya-Tanigchi ➡ χt = 0 for 0 ≤ m < mc → 実現? →
mud ms ∞ ∞
physical pt.
5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV
4]
GL-DW GL-OV OV-DW OV-OV
32
3x12, β=4.3
r e fi n e d
due to vanishing / suppressed topological susceptivility
➡ χt = 0 for small non-zero m OR ➡ exponential decay for T>Tc
➡ axion window can possibly be closed
Kitano-Yamada JHEP [1506.00370]
χt(T) ∼
QCD,
T < Tc, m2
qΛ2 QCDe−2c(mq)T 2/T 2
c , T > Tc,
h c(mq) → ∞ as mq → 0,
s χt = m2
af2 a.
topological susceptibility, U(1)A:
に重要。 それらを順に見ていく。 得に断りの無いものは JLQCD による仕事 (最新結果はpreliminary)
GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV-DW OV index on DW ensemble OV-OV OV index on OV ensemble
GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV-DW OV index on DW ensemble OV-OV OV index on OV ensemble
5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV
4]
GL-DW GL-OV OV-DW OV-OV
32
3x12, β=4.3
comparing 1/a=1.7 GeV and 1/a=2.6 GeV; ( (3.6fm)3 and (2.4fm)3 )
➡ (consistent with OV-OV with large error of OV-OV)
5 10 15 20 25 30 m [MeV] 0.0 5.0×10
7
1.0×10
8
1.5×10
8
2.0×10
8
χt [MeV
4]
β=4.1 GL-DW β=4.3 GL-DW β=4.1 OV-OV β=4.3 OV-OV
compare Nt=8(β=4.1) and 12(4.3) at simlar temperature (217 and 220 MeV)
5 10 15 m [MeV] 0.0 2.0×10
7
4.0×10
7
χt [MeV
4]
β=4.1 GL-DW β=4.3 GL-DW β=4.1 OV-OV β=4.3 OV-OV
compare Nt=8(β=4.1) and 12(4.3) at simlar temperature (217 and 220 MeV)
continuum scaling in 1st region
( V=(3.6fm)3 and (2.4fm)3 )
0.005 0.01 0.015
a
2 [fm 2] 1e+07 2e+07 3e+07 4e+07 5e+07
χt [MeV
4] GL-DW OV-OV
m=6.6MeV
1/a=2.6 GeV
suggesting 2 regions 1: χt is very small (may vanish in a→0): 0 ≤ m ≲ 10 MeV (→ consistent w/ Aoki-Fukaya-Tanigchi for U(1)A symm.) 2: sudden growth of χt : 10 MeV ≲ m
physical ud
5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV
4]
GL-DW OV-OV
32
3x12, β=4.3
5 10 15 mf [MeV] 2e+07 4e+07 χ [MeV
4]
GL-DW OV-OV
32
3x12, β=4.3
GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV-DW OV index on DW ensemble OV-OV OV index on OV ensemble
1/a=2.6 GeV
suggesting 2 regions 1: χt is very small (may vanish in a→0): 0 ≤ m ≲ 10 MeV (→ consistent w/ Aoki-Fukaya-Tanigchi for U(1)A symm.) 2: sudden growth of χt : 10 MeV ≲ m
physical ud
5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV
4]
GL-DW OV-OV
32
3x12, β=4.3
5 10 15 mf [MeV] 2e+07 4e+07 χ [MeV
4]
GL-DW OV-OV
32
3x12, β=4.3
GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV-DW OV index on DW ensemble OV-OV OV index on OV ensemble
1/a=2.6 GeV
suggesting 2 regions 1: χt is very small (may vanish in a→0): 0 ≤ m ≲ 10 MeV (→ consistent w/ Aoki-Fukaya-Tanigchi for U(1)A symm.) 2: sudden growth of χt : 10 MeV ≲ m
physical ud
5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV
4]
GL-DW OV-OV
32
3x12, β=4.3
5 10 15 mf [MeV] 2e+07 4e+07 χ [MeV
4]
GL-DW OV-OV
32
3x12, β=4.3
GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV-DW OV index on DW ensemble OV-OV OV index on OV ensemble
1/a=2.6 GeV
suggesting 2 regions 1: χt is very small (may vanish in a→0): 0 ≤ m ≲ 10 MeV (→ consistent w/ Aoki-Fukaya-Tanigchi for U(1)A symm.) 2: sudden growth of χt : 10 MeV ≲ m
physical ud
5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV
4]
GL-DW OV-OV
32
3x12, β=4.3
5 10 15 mf [MeV] 2e+07 4e+07 χ [MeV
4]
GL-DW OV-OV
32
3x12, β=4.3
GL-DW gluonic charge on DW ensemble GL-OV gluonic charge on OV ensemble OV-DW OV index on DW ensemble OV-OV OV index on OV ensemble
1 2 3 Qt 1 10 100 1000 histogram OV-DW OV-OV
OV index
32
3x12, β=4.3, m=0.0015000 10000 15000 20000 25000 trajectory
1 2 Qt GL-DW OV-DW
β=4.3, 32
3x12, mf=0.0011 2 3 Qt 1 10 100 1000 histogram GL-DW OV-DW
32
3x12, β=4.3, m=0.0051 2 3 Qt 1 10 100 1000 histogram GL-DW GL-OV
gluonic
32
3x12, β=4.3, m=0.001 5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV 4] GL-DW OV-OV 32 3x12, β=4.3null measurement of topological excitation after reweighting
(this case <Q2>=4(4) x10-6 ↔ 6(3) x10-3 @m=13MeV)
Effective number of statistics
1 2 3 Qt 1 10 100 1000 histogram OV-DW OV-OV
OV index
32
3x12, β=4.3, m=0.001 5 10 15 20 25 30 mf [MeV] 5e+07 1e+08 1.5e+08 2e+08 χ [MeV 4] GL-DW OV-OV 32 3x12, β=4.3~30k, 30k, 10k
5 10 15 20 25 m [MeV] 0.0 5.0×10
7
1.0×10
8
1.5×10
8
χt [MeV
4]
24
3
32
3
48
3
OV-OV
5 10 15 20 25 m [MeV] 0.0 5.0×10
7
1.0×10
8
1.5×10
8
χt [MeV
4]
24
3
32
3
48
3
OV-OV
5 10 15 20 25 m [MeV] 0.0 5.0×10
7
1.0×10
8
1.5×10
8
χt [MeV
4]
24
3
32
3
48
3
GL-DW
Statistics in trajectory ~30k, 30k, 10k
5 10 15 20 25 m [MeV] 0.0 5.0×10
7
1.0×10
8
1.5×10
8
χt [MeV
4]
24
3
32
3
48
3
OV-OV
5 10 15 20 25 m [MeV] 0.0 5.0×10
7
1.0×10
8
1.5×10
8
χt [MeV
4]
24
3
32
3
48
3
GL-DW
Statistics in trajectory ~30k, 30k, 10k
1 2 3 Qt 1 10 100 1000 histogram GL-DW GL-OV
gluonic
32
3x12, β=4.3, m=0.003751 2 3 Qt 1 10 100 1000 histogram OV-DW OV-OV
OV index
32
3x12, β=4.3, m=0.003751 2 3 Qt 1 10 100 1000 histogram GL-DW GL-OV
gluonic
24
3x12, β=4.3, m=0.003751 2 3 Qt 1 10 100 1000 histogram GL-DW GL-OV
gluonic
48
3x12, β=4.3, m=0.003751 2 3 Qt 1 10 100 1000 histogram OV-DW OV-OV
OV index
24
3x12, β=4.3, m=0.003751 2 3 Qt 1 10 100 1000 histogram OV-DW OV-OV
OV index
48
3x12, β=4.3, m=0.00375m=10 MeV
low stat. low stat.
5 10 15 20 25 m [MeV] 0.0 5.0×10 7 1.0×10 8 1.5×10 8 χt [MeV 4] 24 3 32 3 48 35 10 15 20 25 m [MeV] 0.0 5.0×10
7
1.0×10
8
1.5×10
8
χt [MeV
4]
24
3
32
3
48
3
KY scenario from ∆π−δ (m=3MeV) AFT scenario
OV-OV
5 10 15 20 25 m [MeV] 0.0 5.0×10
7
1.0×10
8
1.5×10
8
χt [MeV
4]
24
3
32
3
48
3
KY scenario from ∆π−δ (m=3MeV) AFT scenario
GL-DW
Kanazawa-Yamamoto
up to contact terms
➡ the symmetry effectively recovers ๏ here Nf=2 (including Nf=2+1 with “2” driven to chiral limit)
∂µJµ
5 = Nf
32π2 F ˜ F
h∂µJµ
5 (x) · O(0)i = Nf
32π2 hF ˜ F(x) · O(0)i
scalar
➡ 0 for U(1)A restoration
Δπ−δ ¼ Z d4x½hπaðxÞπað0Þi − hδaðxÞδað0Þi;
π δ
τ 2
: qγ5 q : q τ
2 q
: q : qγ5 σ η
L R
SU(2) x SU(2) SU(2) x SU(2)
L R
U(1)A U(1)A
q q
5,con
200 10 20 30 40 50 ∆MP S [MeV] mud [MeV] T = TC linear chiral extrapolation T = 0 physical point T = 0 chiral limit
Brandt et al JHEP [1608.06882]
very roughly speaking
hqqi = lim
m→0
Z ∞ dλρ(λ) 2m λ2 + m2 = πρ(0)
[JLQCD 2016 Tomiya et al]
Lowest bin→0 consistent with SUA(2) restoration
[JLQCD 2016 Tomiya et al]
range of JLQCD
Dick et al PRD [1502.06190]
¯ Δov
π−δ ≡ Δov π−δ − 2N0
Vm2 : ð
ð Þ
50 100 150 200 250 130 140 150 160 170 180 190 200 T [MeV] (χMS
π - χMS σ )/T2
mπ=135 MeV mπ=200 MeV 50 100 150 200 250 130 140 150 160 170 180 190 200 T [MeV] (χMS
π - χMS δ )/T2
mπ=135 MeV mπ=200 MeV
0.0 0.2 0.4 0.6 0.8 1.0
χπ − χσ χη− χδ χπ − χδ χσ− χη
[figures from Ding Lattice 2016]
π δ
τ 2
: qγ5 q : q τ
2 q
: q : qγ5 σ η
L R
SU(2) x SU(2) SU(2) x SU(2)
L R
U(1)A U(1)A
q q
5,con
ð Þ
10000 20000 30000 40000 V3 0.1 0.2 0.3 ∆subt m=12 MeV m= 9 MeV m= 2 MeV
Nt=8, T=217 MeV
100 200 300 m
2 [MeV 2]
0.1 0.2 0.3 16
3x8
32
3x8
Nt=8, T=217 MeV
[JLQCD 2016 Tomiya et al]
10000 20000 30000 40000 V3 0.1 0.2 0.3 ∆subt m=12 MeV m= 9 MeV m= 2 MeV
Nt=8, T=217 MeV
100 200 300 m
2 [MeV 2]
0.1 0.2 0.3 16
3x8
32
3x8
Nt=8, T=217 MeV
[JLQCD 2016 Tomiya et al]
A
10000 20000 30000 40000 V3 0.1 0.2 0.3 ∆subt m=12 MeV m= 9 MeV m= 2 MeV
Nt=8, T=217 MeV
100 200 300 m
2 [MeV 2]
0.1 0.2 0.3 16
3x8
32
3x8
Nt=8, T=217 MeV
[JLQCD 2016 Tomiya et al]
A
x ) )
fix V: Δ→0 as m2 for m→0 even for U(1)A br. case fix m : Δ∝V
10000 20000 30000 40000 V3 0.1 0.2 0.3 ∆subt m=12 MeV m= 9 MeV m= 2 MeV
Nt=8, T=217 MeV
100 200 300 m
2 [MeV 2]
0.1 0.2 0.3 16
3x8
32
3x8
Nt=8, T=217 MeV
[JLQCD 2016 Tomiya et al]
A
x ) )
fix V: Δ→0 as m2 for m→0 even for U(1)A br. case fix m : Δ∝V
10000 20000 30000 40000 V3 0.1 0.2 0.3 ∆subt m=12 MeV m= 9 MeV m= 2 MeV
Nt=8, T=217 MeV
100 200 300 m
2 [MeV 2]
0.1 0.2 0.3 16
3x8
32
3x8
Nt=8, T=217 MeV
[JLQCD 2016 Tomiya et al]
A
Note
∆"#$ = ' () * ) 2,- ()- + ,-)-
1 2
∆"#$
34 ≡
1 7(1 − ,-)- 9 2,-(1 − )34
(:)-)-
)34
(:);
Δ >"#$
34
≡ ∆"#$
34
− 2?2 7,- New order parameter: we subtract zero mode
The factor of 1/); enhances zero-mode contribution?
In 7 → ∞ limit, we know zero- mode contribution is suppressed: Δ2#CDEF
34
= 2?2 7,- (∝ 1/ 7
24/Jul/2018 11
integrated up to λ0 subtracted zero mode
Lattice 2018
Note
∆"#$ = ' () * ) 2,- ()- + ,-)-
1 2
∆"#$
34 ∝ ,- ln Λ + ⋯
We assume valence quark mass dependence of ∆"#$ (for small m):
24/Jul/2018 12 Lattice 2018
∆"#$ (,) = : ,- + ; + <,- + =(,>) From 3 eqs. for ∆"#$(,?), ∆"#$(,-), ∆"#$ ,@ , : and < are eliminated ∆"#$~ ; + =(,>) (, that depends on sea quark mass) * ) ~)@ ~1/)> The term depends on cutoff Λ and valence quark mass , Zero-mode
(disappears in D → ∞)
,- ln Λ
(disappears in m → 0)
JLQCD, preliminary (2018)
32 24
Suzuki, Lattice 2018 physical ud
0.005 0.01 0.015 0.02 0.025 0.03 0.035 0.04 50 100 150 200 250 ρ(|λ|) [GeV3] Overlap Dirac eigenvalue |λ| [MeV] 323x12, β=4.3, T=220MeV, m=0.001(2.64MeV)
0.005 0.01 0.015 0.02 0.025 0.03 0.035 0.04 0.045 0.05 50 100 150 200 250 ρ(|λ|) [GeV3] Overlap Dirac eigenvalue |λ| [MeV] 323x12, β=4.3, T=220MeV, m=0.01(26.4MeV)
2+1 2+1 2+1 2+1
2 2 2 2 2 2
quantum chromodynamics”
10 20 30 100 200 500 1000 2000 5000 nf=3+1 nf=2+1+1 phys mud/mud
phys
T[MeV] staggered staggered fix Q
Z0
= exp Z mphys
s
mphys
ud
d log mud mudhψψudi1−0 ! · Z1 Z0
d log T = dβ d log ahSgiQ−0 + X
f
d log mf d log a mfhψψfiQ−0.
possible (our choice is given ion = −
−
O O O
Q Q
10-7 10-6 10-5 10-4 10-3 10-2 10-1 100 200 500 χ[fm-4] T[MeV] 1512.06746 1606.03145 χt 1606.03145 m2χdisc this work
10-7 10-6 10-5 10-4 10-3 10-2 10-1 100 200 500 χ[fm-4] T[MeV] 1512.06746 1606.03145 χt 1606.03145 m2χdisc this work
up to 3 GeV means that we do not have to rely on the dilute instanton gas approximation (DIGA). Note that a posteriori the exponent predicted by DIGA turned out to be compatible with
case. Though some of our simulations (see Supplementary Fig. 18) are already carried
large cut-off effects are a priori absent, it is an important task for the future to crosscheck these results with a calculation using chiral fermions only.
10-7 10-6 10-5 10-4 10-3 10-2 10-1 100 200 500 χ[fm-4] T[MeV] 1512.06746 1606.03145 χt 1606.03145 m2χdisc this work
0.0005 0.001 0.0015 0.002 0.0025 0.003 0.0035
a
2 [fm 2]
10 20 30 40 50
χ
1/4[MeV]
Borsanyi et al. Bonati et al.
mres = 0.05(3) MeV (β=4.3, Ls=16)
mres = 0.05(3) MeV (β=4.3, Ls=16)
hOiov ¼ hORiDW hRiDW ;
mres = 0.05(3) MeV (β=4.3, Ls=16)
hOiov ¼ hORiDW hRiDW ;
R ≡ det½HovðmÞ2 det½H4D
DWðmÞ2 × det½H4D DWð1=4aÞ2
det½Hovð1=4aÞ2 :
mres = 0.05(3) MeV (β=4.3, Ls=16)
Dov = 1 2
(1 + γ5sgnλi) |λi⇤⇥λi|
+D4D
DW
|λi⇤⇥λi|
,
hOiov ¼ hORiDW hRiDW ;
R ≡ det½HovðmÞ2 det½H4D
DWðmÞ2 × det½H4D DWð1=4aÞ2
det½Hovð1=4aÞ2 :
mres = 0.05(3) MeV (β=4.3, Ls=16)
Dov = 1 2
(1 + γ5sgnλi) |λi⇤⇥λi|
+D4D
DW
|λi⇤⇥λi|
,
hOiov ¼ hORiDW hRiDW ;
R ≡ det½HovðmÞ2 det½H4D
DWðmÞ2 × det½H4D DWð1=4aÞ2
det½Hovð1=4aÞ2 :
HM ¼ γ5 αDW 2 þ DW ;
λ for
with ρ(0)→0 and ρ’(0)→0
with ρ(0)→0 and ρ’(0)≠ 0 non-analyticity at λ→0 required
sectors
Z(T, V3, M) = exp
T f(T, V3, M)
f(T, V3, M) = f0 − f2 tr M†M − fA(det M + det M†) + O(M4) ,
represents the effect of axial as det M → e4iθA det M
breaks U(1)A
all invariant under SU(2)LxR
M → e−2iθAVLMV †
R
via M → M eiθ/Nf
ZQ(T, V3, M) ≡ dθ 2π e−iQθ Z(T, V3, Meiθ/2). = e−V4[f0−f2(m2
u+m2 d)]
dθ 2π e−iQθ e2V4fAmumd cos θ = e−V4[f0−f2(m2
u+m2 d)] IQ(2V4fAmumd) ,
∆π−δ =
∞
X
Q=−∞
ZQ Z PQ PQ = 8fA
I′
Q(2V4fAm2)
IQ(2V4fAm2)
via M → M eiθ/Nf
ZQ(T, V3, M) ≡ dθ 2π e−iQθ Z(T, V3, Meiθ/2). = e−V4[f0−f2(m2
u+m2 d)]
dθ 2π e−iQθ e2V4fAmumd cos θ = e−V4[f0−f2(m2
u+m2 d)] IQ(2V4fAmumd) ,
∆π−δ =
∞
X
Q=−∞
ZQ Z PQ PQ = 8fA
I′
Q(2V4fAm2)
IQ(2V4fAm2)
relative contribution of modes
x ) )
∆|full
via M → M eiθ/Nf
ZQ(T, V3, M) ≡ dθ 2π e−iQθ Z(T, V3, Meiθ/2). = e−V4[f0−f2(m2
u+m2 d)]
dθ 2π e−iQθ e2V4fAmumd cos θ = e−V4[f0−f2(m2
u+m2 d)] IQ(2V4fAmumd) ,
∆π−δ =
∞
X
Q=−∞
ZQ Z PQ PQ = 8fA
I′
Q(2V4fAm2)
IQ(2V4fAm2)
relative contribution of modes
x ) )
∆|full
via M → M eiθ/Nf
ZQ(T, V3, M) ≡ dθ 2π e−iQθ Z(T, V3, Meiθ/2). = e−V4[f0−f2(m2
u+m2 d)]
dθ 2π e−iQθ e2V4fAmumd cos θ = e−V4[f0−f2(m2
u+m2 d)] IQ(2V4fAmumd) ,
∆π−δ =
∞
X
Q=−∞
ZQ Z PQ PQ = 8fA
I′
Q(2V4fAm2)
IQ(2V4fAm2)
relative contribution of modes
x ) )
∆|full