LΛ - 名古屋大学素粒子宇宙起源研究機構（KMI）

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Nf=9, α*>αcr , broken phasem 0/ 0.70.8 L = 12L = 160.6 L = 20L = 25L = 300.5 0.70.40.60.3Raw data(Mock data)0.20.50 0.1 0.1 0.2 0.2 0.3 0.3 0.4 0.4 0.5 0.5 0.6m P/ m PLFinite size Hyperscaling test25201510 = 2.0L = 12L = 16L = 20L = 25L = 3050 5 10 15 20 25x
Nf=12, α*
Page 10 and 11: LatKMI collaboration• Y.Aoki, T.A
Page 13: m_pi0.90.80.70.60.50.40.30.20.1m_pi
Page 16 and 17: f π = 0 or = 0? as m f → 0f_pi v
Page 18 and 19: f π = F + Am α f0.20.18f_pi vs mf
Page 20 and 21: 0.2f_pi vs mfL^3x(4L/3)0.180.16f_pi
Page 24 and 25: LM H = F H (x),LF H = G F (x)x ≡
Page 26 and 27: 4Lf vs. X(=0.6)Nf=8, =3.8, L^3x(4L/
Page 28 and 29: P (γ) 20151052 4 6 8
Page 30 and 31: LM H = F H (x),LF H = G F (x)x ≡
Page 32 and 33: hyperscaling (m_pv vs x)(m_pv)=0.84
Page 35 and 36: γ(M π ) = γ(f π ) N f =4, 12
Page 37 and 38: N f =4=3.7, = 0.0=3.7, = 1.0=3.7,
Page 39 and 40: (Nf=11), α*~αcr , just below conf
Page 42: Summary (Preliminary)SU(3) gauge th
Page 45: m_pv vs mfL^3x(4L/3), Quadratic fit

LΛ - 名古屋大学 素粒子宇宙起源研究機構（KMI）

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LΛ - 名古屋大学素粒子宇宙起源研究機構（KMI）