Electroweak Symmetry Breaking with Holomorphic Supersymmetric Nambu–Jona-Lasinio Model
— Talk at PHENO 2010 OTTO C. W. KONG
— Nat’l Central U, Taiwan
Electroweak Symmetry Breaking with Holomorphic Supersymmetric - - PowerPoint PPT Presentation
Electroweak Symmetry Breaking with Holomorphic Supersymmetric NambuJona-Lasinio Model Talk at PHENO 2010 OTTO C. W. KONG Natl Central U, Taiwan 1 NambuJona-Lasinio Model :- Otto Kong (NCU) 09ntnu-1 dynamical symmetry
— Talk at PHENO 2010 OTTO C. W. KONG
— Nat’l Central U, Taiwan
Otto Kong (NCU) — 09ntnu-1
1
Lψ = i ¯ ψ+σµ∂µψ+ + i ¯ ψ−σµ∂µψ− + g2 ¯ ψ+ ¯ ψ−ψ+ψ− − → Lψ − (µφ† + gψ+ψ−)(µφ + g ¯ ψ+ ¯ ψ−) = i ¯ ψ+σµ∂µψ++i ¯ ψ−σµ∂µψ−−µ2φ†φ−µg(φ† ¯ ψ+ ¯ ψ−+φψ+ψ−)
(no kinetic term)
φ = −g/µ ¯ ψ+ ¯ ψ−
⇒ symmetry breaking and fermion mass
Otto Kong (NCU) — 09ntnu-2a
2
φ = 0 solution for g2Λ2
8π2 > 1
g2 ¯ ψ+ ¯ ψ−ψ+ψ− = ⇒ g2 ¯ ψ+ ¯ ψ−
fermion-loop propagator with Yukawa vertices (m ≪ Λ) Z = N
cµ2g2
16π2
M2 + O(1)
Otto Kong (NCU) — 09ntnu-2b
3
ψ+σµ∂µψ+ + i ¯ ψ−σµ∂µψ− + ∂µφ†∂µφ −˜ µ2φ∗φ −
˜ λ 2 (φ†φ)2 − ˜
yφψ+ψ− + h.c. — ˜ y =
µg √ Z = 4π √N
c
1
√
ln (Λ2/M2)
— ˜ µ2 =
N
cg2 − (Λ2 − M 2)
ln (Λ2/M2)
— ˜ λ =
32π2 N
cln (Λ2/M2)
ψ+σµ∂µψ+ − →
Φ+Φ+
ψ+ ¯ ψ−ψ+ψ− − →
Φ+ ¯ Φ−Φ+Φ−
− →
− →
µ 2 ΦΦ
BUT :-
ψ+ ¯ ψ− implies µ2φ∗φ = −µg φψ+ψ− = g2 ¯ ψ+ ¯ ψ−ψ+ψ− (no SUSY !)
ψ+σµ∂µψ+ − →
Φ+Φ+ (1 − m2θ2¯ θ2)
ψ+ ¯ ψ−ψ+ψ− − →
Φ+ ¯ Φ−Φ+Φ−
− →
− →
Φ1Φ1 BUT :-
implies
Φ1Φ1 =
Φ+ ¯ Φ−Φ+Φ−
Φ1 = 0
ψ+σµ∂µψ+ − →
Φ+Φ+ (1 − m2θ2¯ θ2)
− →
− →
µ 2 Φ0Φ0
= ⇒ L =
Φ+Φ+ + ¯ Φ−Φ−)(1 − m2θ2¯ θ2)
µ
2 Φ2 0 + √µGΦ0Φ+Φ−
W = G
2 Φ+Φ−Φ+Φ−
− → W − 1
2(√µΦ0 +
√ GΦ+Φ−)(√µΦ0 + √ GΦ+Φ−)
Otto Kong (NCU) — 09ntnu-6
7
2 Φ+Φ−Φ+Φ− contains no g2 ¯
ψ+ ¯ ψ−ψ+ψ−
implies
µ 2 Φ2 0 = −
√
µG 2
Φ0Φ+Φ− = G
2 Φ+Φ−Φ+Φ−
= ⇒
G 2 Φ+Φ− Φ+Φ−
Dirac mass for Φ+–Φ−
through Φ+–Φ− loop with Yukawa vertices
Otto Kong (NCU) — 09ntnu-7
8
Φ0 e2VΦ Φ0
θ2 where Z0 = N
cµG
16π2
M2 + O(1)
˜ m2
0 = −(2m2 + A2), tachyonic soft mass (cf. radiative EWSB)
— ˜ y = √
µG √Z0 = 4π √N
c
1
√
ln (Λ2/M2)
— ˜ µ =
µ Z0 = 16π2 N
cG
1 ln (Λ2/M2)
2 Φ2 term =
⇒ Φ in real representation of symmetry
Otto Kong (NCU) — 09ntnu-8
9
ψ+ ¯ ψ−
− → −µg φ ψ+ψ− — symmetry breaking with bi-fermion condensate φ
Φ+ ¯ Φ−
− → −g
1
1 = −µA2
− → √µG A0 [A+F− + A−F+ − ψ+ψ−] + √µG F0 A+A− — A0 = −
Otto Kong (NCU) — 09ntnu-9
10
Otto Kong (NCU) — 09ntnu-10
11
g2 ¯ Q¯ tcQtc
φ = −g/µ( ¯ Q¯ tc)
— gives top quark mass at to infared quasi-fixed point
(Λ ∼ 1019 GeV )
Bardeen, Hill, Lindner 90
mt ∼ 214 − 202 GeV (Λ ∼ 1015 − 1019 GeV )
Marciano 89,90
mt ∼ 253 GeV
Miransky, Tanabashi, Yamawaki 89; King & Mannan 90,91
Otto Kong (NCU) — 09ntnu-11
12
scalar field is somewhat sick
e.g. OK 96
scalar content — only part arbitrary (cf. gauge symmetry)
scalar as (part of) chiral superfield (constrained as fermions) Vs Georgi’s survival hypothesis
— and avoid fine-tuning of four-quark coupling(s)
Otto Kong (NCU) — 09ntnu-12
13
αβ ˆ
Qα ˆ U c ˆ Q′β ˆ Dc (1 + Bθ2) W − → W − µ ( ˆ Hd − λu ˆ Q ˆ U c)( ˆ Hu − λd ˆ Q′ ˆ Dc)(1 + Bθ2) = (−µ ˆ Hd ˆ Hu + yu ˆ Q ˆ Hu ˆ U c + yd ˆ Hd ˆ Q′ ˆ Dc)(1 + Bθ2)
— ˆ Hu = yd
µ ˆ
Q′ ˆ Dc and ˆ Hd = yu
µ
ˆ Q ˆ U c
Hu and ˆ Hd
µ
= G
— expect hu > ∼ hd (Vs UBB in D-flat)
Otto Kong (NCU) — 09ntnu-13
14
(vs At ≃ 0)
H d ≃ −(m2 Q + m2 b + |Ab|2)
plus (vs only) m2
H u ≃ −(m2 Q + m2 t + |At|2)
j QkDc h(1 + Aθ2) + Ge ij Q
3U c 3 LiEc
j(1 + Aθ2)]
— non-holomorphic case needs similar holomorphic terms for Yukawa couplings of down-type quarks and charged leptons
(vs top condensate and stop condensates for ui and di + ℓi masses)
Otto Kong (NCU) — 09ntnu-14
15
(without background model)
Froggatt et.al 93
mt = 184.3 ± 6.8 GeV, mh = 121.8 ± 4.3 GeV
Carena et.al 92
— high Λ and large tanβ lower mt
SNJL – yt blows up at Λ HSNJL – yt and yb blows up at ∼ Λ
Otto Kong (NCU) — 09ntnu-14p
16
35 40 45 50 55 60 65 70 75 104 106 108 1010 1012 1014 1016 tanβ Λ [GeV] Ms = 10 TeV Ms = 1 TeV Ms = 200 GeV
Otto Kong (NCU) — 09ntnu-14r
17
0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 103 104 105 106 107 108 109 1010 1011 yt, yb µ [GeV] Ms = 1 TeV tanβ = 57.8 Λb = 104 GeV tanβ = 42.8 Λb = 1010 GeV yb yt
Otto Kong (NCU) — 09ntnu-14h
18
90 95 100 105 110 115 120 125 130 103 104 mh [GeV] Ms [GeV] 200
mA ≥ 100 GeV mA = 140 GeV mA = 130 GeV mA = 120 GeV mA = 110 GeV mA = 100 GeV
Otto Kong (NCU) — 09ntnu-15
19
— SUSY : scalar → chiral superfield — problematic MSSM superfield spectrum — vectorlike Higgs superfields, turn up as composites — four-superfield (G) term from integrated out heavy Higgs superfields ? — more natural B (and A) term, and all Yukawa coupling
Otto Kong (NCU) — end
20
well done Otto !