Symmetries and dynamics in Particle Physics: the legacy of Yoichiro Nambu
O s a k a C i t y U n i v . 1 3 / 1 2 / 2 0 1 8
K . K o n i s h i ( U n i v . P i s a / I N F N , P i s a )
N a m b u S y m p o s i u m
Symmetries and dynamics in Particle Physics: the legacy of Yoichiro - - PowerPoint PPT Presentation
N a m b u S y m p o s i u m O s a k a C i t y U n i v . 1 3 / 1 2 / 2 0 1 8 Symmetries and dynamics in Particle Physics: the legacy of Yoichiro Nambu K . K o n i s h i ( U n i v . P i s a / I N F N , P i s a ) Achievements by Y. Nambu
O s a k a C i t y U n i v . 1 3 / 1 2 / 2 0 1 8
K . K o n i s h i ( U n i v . P i s a / I N F N , P i s a )
N a m b u S y m p o s i u m
🔶
Chiral symmetry breaking and physics of massless pions /current algebra
🔶
Quark model to Quantum Chromodynamics
🔶
Nambu-Goto action: birth of string theory
🔶
🔶
“Yoichiro Nambu: remembering an unusual physicist, a mentor, and a friend" Giovanni Jona-Lasinio, Prog. Theor. Exp. Phys. 2016 , 07B102
🔶
“BCS, Nambu-Jona-Lasinio, and Han-Nambu - A sketch of Nambu’s works in 1960-1965 ” Kazuo Fujikawa, arXiv:1602.08193
🔶
“Nambu at Work" Peter G. Freund, arXiv:1511.06955
🔶
“Professor Nambu, String Theory and Moonshine Phenomenon" Tohru Eguchi, arXiv:1608.06036
🔶
“Birth of String Theory" Hiroshi Itoyama arXiv:1604.03701
🔶
“Yoichiro Nambu" Holger B Nielsen, Int. J. Mod. Pays. A (2016)
Nambu’s lecture at the “Highlights in Particle Physics”
🔶
Nambu-Goldstone modes (pions), PCAC, soft-pion theorems
🔶
Englert-Brout-Higgs mechanism; Weinberg-Salam electroweak theory
🔶
🔶
Ettore Majorana Erice Summer School, 1972
“ … I am convinced that the strong interactions are also described by some sort of color gauge theory. ”
S u m m e r 1 9 7 2 Need of anomaly cancellation
🔶
🔶
🔶
J.C. Taylor P . Freund
Let’s start where Nambu has left out…
“The basic principle underlying the model is the idea that field theory may admit, as a result of dynamical instability, extraordinary (nontrivial) solutions that have less symmetries than are built into the Lagrangian. “
Massless Nambu-Goldstone bosons (pions) of broken
SUA(Nf)
Want a deeper understanding of
Nambu, Mandelstam, ’t Hooft, ~‘80
Confinement vs XSB
Monopoles weak coupled
SU(3) → SU(2) × U(1) → 1
Π
1
( S U ( 2 ) × U ( 1 ) ) = Z
‘80~’18
k s
ψ
L
D S U
A
( N
f
) π
2
( S U ( 3 ) / U ( 1 )
2
) = π
1
( U ( 1 )
2
) = ×
Seiberg-Witten
A r g y r e s , S e i b e r g , G a i
t
T a c h i k a w a … …
High density QCD / cold atoms
Pisa, Titech,
Minnesota, Cambridge, Keio
🔶
SW curves: all pert/nonpertive effects encoded
🔶
Exact low-energy dual Abelian or nonAbelian Leff
🔶
Analytic demonstration of confinement
🔶
Confinement vs XSB
🔶
Argyres-Douglas vacua
A b e l i a n a n d n
A b e l i a n d u a l M e i s s n e r p i c t u r e
c
fi n e m e n t O K ; B u t N O T s i m i l a r t
C D
🔶
Argyres-Seiberg S duality, Gaiotto and SCFT
🔶
Confining vacuum near strongly coupled SCFT
M
t i n t e r e s t i n g b u t d i f fi c u l t : s
e a n a l
y t
C D ? ’94 -
’09
’06
red curves= deformations by some relevant operators
N=2 SCFT
N=0 SCFT
aUV = 11NfNc 360 + 31 180(N 2
c − 1)
− aIR = N 2
f − 1
360 .
SU(N), NF =2N-1
aUV = 7N 2 − N − 5 24
aN=2SCF T = 7N(N − 1) 24
aIR = (2N − 1)2 − 1 48
cUV = 4N 2 − N − 2 12
cN=2SCF T = N(N − 1) 3
cIR = (2N − 1)2 − 1 24
20NfNc + N 2
c 1
10 ;
cIR = N 2
f 1
120 ;
Nf < 11 2 Nc
Bolognesi, Giacomelli, KK ‘16 in adjoint repr of GF
♦
♦
♦
♦
🔶
NonAbelian vortex = ANO vortex embedded in CF locked vacuum
🔶
Non-Abelian monopoles are the endpoints of the nonAbelian vortices
🔶
Internal orientational zeromodes ~ Fluctuations: CPN-1 sigma model in 2D vortex world sheet
🔶
Notorious problems avoided
Auzzi et. al, Hanany-Tong ’03- Shifman-Yung, Nitta-Ohashi-Sakai …
🔶
Quantum physics of CPN-1 sigma model on finite-width vortex world sheet ; Unbroken isometry SU(N)
Bolognesi, Gudnason, Ohashi, KK ’16-‘18
Standard CPN-1 model at L
Vainshtein’ nov 18
SU(N + 1)color ⊗ SU(N)flavor
v1
− → (SU(N) × U(1))color ⊗ SU(N)flavor
v2
− → SU(N)C+F Monopole Vortex
C i p r i a n i , D
i g
i , G u d n a s
, K . K . M i c h e l i n i , 2 1 1 C h a t t e r j e e , K . K . 2 1 4
Vortices with fluctuating
H a n n a h , T
g , ’ 3 , A u z z i , B
n e s i , E v s l i n , K K , Y u n g ’ 3 S h i f m a n , Y u n g , ’ 3 A u z z i , B
n e s i , E v s l i n , K . K . , ’ 4
🔶
Quantum behavior of Abelian and nonAbelian monopoles in the IR fairly well (in N=2, N=1, susy gauge theories) understood;
🔶
The topological soliton monopoles and vortices (many applications): origin of the nonAbelian monopoles
🔶
Understanding of confinement /chiral symmetry breaking in the real-world (non supersymmetric) strong-interaction theory however remains a holy grail
🔶
Some new ideas ?
🔶
From 0-form symmetries (acting on local operators) to k-form symmetries (acting on line, surface, etc operators) e.g. the center symmetry in SU(N) YM (k=1)
S e i b e r g , K a p u s t i n , A h a r
y , G a i
t
T a c h i k a w a , W i l l e t , K
a r g
s k i , . . P
p i t z , K i k u c h i , T a n i z a k i , S a k a i , S h i m i z u , Y
e k u r a ,
’05-‘18
ei
H
γ A → ΩN ei
H
γ A ,
ΩN = e2πi/N ∈
N
W i l s
l
P
y a k
l
Criteria for different phases
Phases / symmetry realization of the system not described by the vacuum expectation values
hφ(x)i , h ¯ ψ(x)ψ(x)i
Nambu-Jona Lasinio L a n d a u
i n z b u r g
: a germ for change of PARADIGM (growing out of Nambu’s teaching…)
H a l d a n e ’ 8 3 W e n , ‘ 8 9
♦
♦
net effect:
🔶
Gauging the (k=1) discrete ∈
N center symmetry
♦
identify configurations related by ∈
N
♦
must eliminate the redundancies
♦
done by coupling the ordinary YM gauge theory to a BF theory
♦
modify the sum over gauge field configurations (path integral)
gets modified to
1 8π2 Z F ^ F = 1 8π2 Z d4x Fµν ˜ F µν 2 1 8π2 Z ( ˜ F B(2)) ^ ( ˜ F B(2)) 2 N , NB(2) = dB(1)
🔶
♦
CP (T) inv of SU(N) YM broken at
♦
Periodicity in θ
♦
Can be understood as a mixed discrete CP -
θ ⇠ θ + 2π ! θ ⇠ θ + 2Nπ θ = π
♦
In the infrared, if the system is confined, with mass gap
∈
N
’t Hooft anomaly
’t Hooft anomaly !
’t Hooft anomaly matching requires a double vacuum degeneracy !!
♦
In IR no gauge degrees of freedom: the above result must hold whether or not the “gauging” of
∈
N
Obstruction to gauging a symmetry
♦
A powerful theoretical reasoning!! is actually done
S e i b e r g , K a p u s t i n , G a i
t
W i l l e t , K
a r g
s k i , . . ‘ 1 7
θ ⇠ θ + 2π ! ⇠ ∆S
Y M
= θ 8π
2
Z F ^ F = π
(Galileo) They must fall at the same velocity
🔶
♦
Adjoint QCD: SU(N) with NF Weyl fermions Nonanomalous discrete
becomes anomalous after 1-form gauging
♦
QCD: SU(N) with NF quarks, NF =N, or gcd(NF , N)= k
⭐ standard center symmetry is absent
λ
i∆S = 2πi Nc
⭐ color-flavor locked
1-form symmetry is present
N.B. k-form symmetries Abelian except k=0
⭐ “gauging”
QCD: SU(N) with NF quarks, arbitrary NF
♦
2NF Nc ;
λ ! e2πi/2NF Ncλ
Anber, Poppits ‘18 Kikuchi, Tanizaki, Misui, Sakai, Shimizu, Yonekura, Kitano,Suyama, Yamada, ’18
Tanizaki ’18
Shimizu, Yonekura ‘18
k ⇢ Nc ⇥ Nf , Nf ⇢ UV (Nf)
k Axial 2NF
broken by mixed anomaly
Nc
Tdec Tchiral
⭐ flavor Nf 1-form symmetry ⭐ “gauging” ⭐ baryon number
UB(1)
Axial 2NF UB(1) 1 Nf mixed anomaly
Skyrmion needed ! S t e r n p h a s e N
Dumitrescu, Cordoba, ‘18
Chatterjee, Nitta, Yasui ’18
🔶
e.g., SU(N) theory with Weyl fermions standard ’t Hooft anomaly matching constraints for
ψ{ij} , ηB
i ,
B = 1, 2, . . . , N + 4
+ (N + 4) ¯
♦ ⭐
do not tell between
B[AB] = ψijηA
i ηB j ,
A, B = 1, 2, . . . , N + 4
⭐
hψijηB
i i = C δjB ,
j, B = 1, 2, . . . N ,
with some massless baryons and 8 N + 1 Nambu-Goldstone bosons
Uψη(1), SU(N + 4),
ψ, η,
♦
A p p e l q u i s t , D u a n , S a n n i n
B
n e s i , K K , S h i f m a n ‘ 1 8
SU(N + 4) × Uψη(1) → SU(N)cf × U(1)0
Gauging the color-flavor locked
1-form symmetry
N
Bolognesi, KK, Tanizaki ‘19
Z he Uψη(1), Zψ = ZN+2, t
both suffer mixed anomalies dynamical possibility A excluded; B OK
Y a m a g u c h i , n
‘ 1 8
🔶
Many exciting applications of these ideas being explored
🔶
But understanding of confinement /chiral symmetry breaking in the real-world (non supersymmetric) strong-interaction theory still remains a holy grail
🔶
Should we despair ?
’94
W = (Aµ, λ), Φ = (φ, ψ)
Vacuum moduli (degeneracy): hφi = ✓ a a ◆ , u = Trhφ2i
Leff = Im[ Z d4θ ¯ A∂F(A) ∂A + Z d2θ∂2F(A) ∂A2 W αWα]
F(A)= prepotential holomorphic
✓ AD A ◆ → ✓ a b c d ◆ ✓ AD A ◆ ✓δL/δF +
µν
F +
µν
◆ → ✓ a b c d ◆ ✓δL/δF +
µν
F +
µν
◆
SU(2)/U(1): monopoles
massless monopoles at u= ± Λ2
AD = ∂ F / ∂ A
= AD
τ = F
00(A) = dAD
dA = θeff 2π + 4πi g2
eff
F(A) !
SUR(2)
FµνF µν + i ¯ λ γµDµλ + iFµν ˜ F µν + ...
y2 = (x − u)(x − Λ2)(x + Λ2)
dAD du = I
α
dx y , dA du = I
β
dx y ,
Im H
α dx y
H
β dx y
> 0
➞ F(A)
Seiberg-Witten curve
Leff(AD, F µν
D , ...) +
Z d4θ ¯ MeVDM + (M → ˜ M) + √ 2 Z d2θ MAD ˜ M
Magnetic monopole coupled minimally to the dual gauge field
Mnm,ne = |nmAD + neA|, AD = I
α
λ, A = I
β
λ,
Seiberg-Witten curves for general gauge groups
y2 =
N
Y
i=1
(x − φi)2 − Λ2N−NF
NF
Y
a=1
(x + ma) y2 = x
[N/2]
Y
i=1
(x − φ2
i )2 − 4Λ2(N−NF −NF )x2+✏ NF
Y
a=1
(x + m2
a)
B a c k t
. 1 2
Leff(AD, F µν
D , ...) +
Z d4θ ¯ MeVDM + (M → ˜ M) + √ 2 Z d2θ MAD ˜ M
+ Z d2θ µ U(AD)
AD = 0, hMi = r µ ∂U ∂AD = p µΛ
Seiberg-Witten ’94
monopole condensation
Yung-Vainshtein ’01
Dϕ ➞ 0; |ϕ|2 ➞ v2
Abrikosov ’56 Nielsen-Olesen ‘73
(Landau-Ginzburg model)
L = 1 4g2
N
(F a
µν)2 +
1 4e2( ˜ Fµν)2 + |Dµq|2 e2 2 | q† q c 1 |2 1 2 g2
N | q† taq |2,
(D1 + iD2) q = 0,
F (0)
12 + e2
2
= 0; F (a)
12 + g2 N
2 q†
i ta qi = 0.
Nonabelian vortex Bogomolnyi equations
(HT, ABEKY ‘03)
Benchmark H= SU(N)xU(1) model with NF = N
Broken to U(N-1) by the soliton vortex (“Nambu-Goldstone modes”)
Vortex moduli = SU(N)/ U(N-1) = CPN-1 (= CP1 ~ S2 for U(2) )
q = ⇤ ˜ q†⌅ = v2 = v2 ⌥ ↵ ↵ ↵ 1 1 ... 1
2
Auzzi, Bolognesi,Evslin,Konishi, Yung ’03 Hanany,Tong, Shifman-Yung
q = U ⇧ ⌥ eiφ φ(r) . . . χ(r) . . . . . . χ(r) . . . ... ⌃ ⌦ ⌦ ⌦ ⌦
U ⇧ ⌥ . . . w . . . ... . . . w ⌃ ⌦ ⌦ ⌦ U †
r=0
Color-flavor locked vacuum
(orientational zero modes)
S(1+1)
σ
= β
2 (∂ na)2 , Fluctuations: SO(3) sigma model
B a c k t
. 1 4
classification (’t Hooft)
Phases of SU(N) YM
N
, Z(E)
N ) classification (’t Hooft):
If field with x = (a, b) condense, particles X = (A, B) with ⟨x, X⟩ ≡ a B − b A ̸= 0 (mod N) are confined. (e.g. ⟨φ(0,1)⟩ ̸= 0 → Higgs phase.) ⟨χ
0)⟩ ̸= 0 → Confinement: What is χ ?
(’t Hooft) (1981)
W = (Aµ, λ), Φ = (φ, ψ)
1 2 3 4 5 6
0.5 1.0
Konishi ’96 Evans, Hsu, Schwetz ’96
B a c k t
. 1 2
Di Vecchia, Veneziano ’80
Seiberg-Witten, ... ... ...
SU(2) with NF = 0, 1,2,3 monopole condensation ⇒ confinement & dyn symm. breaking
SU(N) 𝒪 =2 SYM : SU(N) ⇒ U(1)N-1 SU(N) ⇒ SU(r) x U(1) x U(1) x ....
A r g y r e s , P l e s s e r , S e i b e r g , ’ 9 6 H a n a n y
z , ’ 9 6 Carlino-Konishi-Murayama ‘00
Beautiful, but don’t look like QCD
Beautiful, but don’t look like QCD
r vacua are local, IR free theories SCFT of highest criticality, EHIY points
Beautiful and interesting
Argyres,Plesser,Seiberg,Witten, Eguchi-Hori-Ito-Yang, ’96
SU(N), NF quarks
r ≤ NF /2
Shifman-Yung ’10-’13
Argyres-Seiberg, Gaiotto-Seiberg-Tahcikawa ’07, ’11 Giacomelli, Bolognesi, -Konishi ’12, - 17
Dynamical Abelianization
CONFINEMENT 13
r=1 r = nf /2
Non Abelian monopoles Abelian monopoles (Non-baryonic) Higgs Branches Baryonic Higgs Branch Coulomb Branch Dual Quarks
QMS of N=2 SQCD (SU(n) with nf quarks)
r=0 <Q> 0
< > 0
N=1 Confining vacua (with 2 perturbation) N=1 vacua (with 2 perturbation) in free magnetic phas
SCFT
Φ ≠
Di Pietro, Giacomelli ’11
CONFINEMENT 14
Non Abelian monopoles Higgs Branches Special Higgs Branch Coulomb Branch Dual Quarks
QMS of N=2 USp(2n) Theory with nf Quarks
<Q> 0 < > 0 N=1 Confining vacua (with 2 perturbation) N=1 vacua (with 2 perturbation) in free magnetic phas SCFT
Carlino-Konishi-Murayama ‘00
Φ
Φ Φ
m ≠ 0
previous slide (m = 0) (Universality)
≠
≠
(r ≤ Nf / 2 )
S e i b e r g
i t t e n ’ 9 4 A r g y r e s , P l e s s e r , S e i b e r g , ’ 9 6 H a n a n y
z , ’ 9 6 Carlino-Konishi-Murayama ‘00
μΦ2 perturbation
S h i f m a n
u n g ’ 1
1 3
SU(r) U(1)0 U(1)1 . . . U(1)N−r−1 U(1)B nf × M r 1 . . . M1 1 1 . . . . . . . . . . . . . . . ... . . . . . . MN−r−1 1 . . . 1
NonAbelian monopoles
Giacomelli-Konishi ’12
2 m· e ∈ Z
cfr.
(Dirac)
S1 = 1 √ 2α2(Eα + E−α); S2 = − i √ 2α2(Eα − E−α); S3 = α∗ · T,
φ̸=0
Ai(r) = Aa
i (r, h · α) Sa;
φ(r) = χa(r, h · α) Sa + [ h − (h · α) α∗] · T,
α∗ ≡ α α · α.
H generated by
H H
U(N) U(N)
SU(N) SU(N)/Z SO(2N) SO(2N) SO(2N+1) USp(2N) ∼
N
Fij = ⌅ijk rk r3(⇥ · T), 2 ⇥ · ∈ Z
Goddard-Nuyts-Olive, E.Weinberg, Lee,Yi, Bais, Schroer, .... ‘77-80
root vectors
e.g., SU(3) ➝ SU(2)×U(1) ⇒ ∄ monopoles ∼ (2, 1 )
“No colored dyons exist”
② Non-normalizable gauge zero modes:
No multiplets of H The real issue: how do they transform under H ? GNO
cfr. Jackiw-Rebbi Flavor Q.N. of monopoles via fermion zeromodes
N.B. : H and H relatively nonlocal
∼
Φ = diag(v,v,-2v)
Weinberg, ’82,’96 Dorey... ’96
Coleman, ... ’81
How do they do that ???
A b
e l s a a d e t . a l . ‘ 8 3
Back to p.9
C
e m a n , N e l s
, ‘ 8 4
Back to p.14
hφi=v1
hqi=v2
SU(N + 1)color ⌦ SU(N)flavor
v1
v2
🔶
🔶 🔶
b(z,t)
endow the monopole with fluctuating CPN-1 modes
b(t)
e.g. G=SU(N), USp(2N): π1 = 1 ⇒ No Dirac monopoles (Wu-Yang)
G=SO(N) π1 =Z2 , Z2 monopoles; G=SU(N)/ZN : ZN monopoles;
Vortices end at regular monopoles
‘t Hooft SO(3)/U(1)
v1
v2
v1
v2
W = (Aµ, λ), Φ = (φ, ψ)
Konishi ’96 Evans, Hsu, Schwetz ’96
↔ ↔ −
2 4 6 8 10 0.2 0.4 0.6 0.8 1 2 4 6 8 10 0.2 0.4 0.6 0.8 1
qkA(x) =
ei k ϕφ2(r)
A3
i (x) = −εij
xj r2 ((n − k) − f3(r)) , A8
i (x) = −
√ 3 εij xj r2 ((n + k) − f8(r))
SU(N), SO(2N) USp(2N) models
Gudnason,Jiang,Konishi ’10
X = 1 + B†B , Y = 1N−1 + BB†
Reducing matrix
plex unit N-com nc = X− 1
2
BX− 1
2
! = √
A u z z i , B
n e s i , E v s l i n , K
i s h i , Y u n g ’ 3 H a n a n y , T
g , S h i f m a n
u n g ‘ 3
B = b1 b2 . . . bN−1
CPN-1 inhomogeneous coord
➯ orientational zeromodes (can fluctuate)
b(z,t)
〈Φ〉 ∿ m SU(N+1) SU(N) x U(1)
〈Q〉 ∿ √ m μ
1
endow the monopole with fluctuating CPN-1 modes
b(t)
⊃ SU(2)C ⊃ U(1)
monopole m
e
t e x c
p l e x
naive “nonAbelian monopole”
Monopole Moduli Vortex Moduli ~ CPN-1 SU(N) 1(H) 2(G/H)
Chatterjee, Konishi ’14
Cipriani, Gudnason, ... ’11
Bolognesi,Konishi,Ohashi, ’16 Betti, Bolognesi,Konishi,Ohashi, ’18 Bolognesi,Gudnason, Konishi, Ohashi ‘18
t h e n
m a l i z a b l e 3 D g a u g e z e r
e s
t h e m
e , w h e n d r e s s e d b y fl a v
c h a r g e s , t u r n i n t
m a l i z a b l e 2 D m
e s
t h e v
t e x w
l d s h e e t .
🔶
Boundary conditions:
Separating and integrating over ni , (i=2,3,.. N) (Large N approximation)
Seff = Z d2x
Generalized gap equations
E = N X
n
ωn + Z L
x + λ(x)
n fn(x) ,
∂2
xσ(x) λ(x)σ(x) = 0 .
N 2 X
n
fn(x)2 ωn + σ(x)2 r = 0 .
D-D : n1
2
L
2
ni
2
L
2
i > 1 . N-N : @xni
2
L
2
∀i.
x ∈ [−L 2 , L 2 ]
Bolognesi, KK.,Ohashi, ’16 Betti, Bolognesi, KK.,Ohashi, ‘17 Bolognesi, Gudnason, KK ,Ohashi, ’18
λ x 5 10 15 20 25 −6 −4 −2 2 4 6 σ2 x 0.1 0.2 0.3 0.4 0.5 0.6 0.7 −6 −4 −2 2 4 6
Figure 1: The functions λ(x) (left) and σ2(x) (right) which are solutions to the gap equa- tion, Eq. (2.6), for various values of L ranging L = 1 ∼ 12. Λ = 1 in this figure. The innermost (outermost) curve corresponds to L = 1 (L = 12).
A new random-walk method Back to p.14
✓ n1 L
2
L
2
= ✓ 1 ◆ √r✏ ; ✓ n1
2
2
= ✓ ei cos α ei sin α −e−i sin α e−i cos α ◆ ✓ √r✏ ◆ ∼ ✓ cos α sin α ◆ √r✏ ;
The most general Dirichlet conditions
N 2 X
n
fn(x)2 ωn e−✏!n + σ1(x)2 + σ2(x)2 − r✏ = 0 , ∂2
xσ1(x) − λ(x)σ1(x) = 0 ,
∂2
xσ2(x) − λ(x)σ2(x) = 0 ,
The gap equations
λ x Λ2 = 1 5 10 15 20 25 −2 −1.5 −1 −0.5 0.5 1 1.5 2 α = 0 α = π λ x Λ2 = 1 0.8 1 1.2 1.4 1.6 1.8 2 −2 −1.5 −1 −0.5 0.5 1 1.5 2
(∂E / ∂α) / N α
−0.002 0.002 0.004 0.006 0.008 0.01 0.012 0.014 0.016 0.018 π/8 π/4 π/2 3π/4 π 3π/8 5π/8 7π/8
∂E ∂α = +2 sin α W > 0 ,
Bolognesi,Gudnason, Konishi, Ohashi ‘18
🔶 A recent observation: the most singular (“Argyres-Douglas”) SCFT,
🔶 Further relevant deformations (shift of bare mass parameters)
G i a c
e l l i , ’ 1 5 , B
n e s i , G i a c
e l l i , K K ‘ 1 5
🔶 N=2 SCFT is a complicated, nonlocal theory of strongly interacting
🔶 N=1 SCFT is a theory of weak-coupled local theory of mesons M 🔶 In the nearby N=1 confining vacuum, M ~ NG bosons of symmetry
🔶 Analogy with the real-world QCD? * **
Giacomelli, ’15, Bolognesi,Giacomelli, KK ‘15
🔶 Seiberg-Witten curves for N=2 gauge theories
☞ SCFT by appropriate tuning of Gc , Gf , Ui (VEVs), g’s and m’s
🔶 Trace anomalies (any theory)
hT µ
µ i =
1 16π2 c (R2
µνρσ 2R2 µν + R2
3 ) a (R2
µνρσ 4R2 µν + R2)
Euler density
🔶 For any N=1 susy theory
a = 3 32(3Tr R3 Tr R) ; c = 1 32(9Tr R3 5Tr R) ,
Tr= sum over Weyl fermions
( R= UR (1) charge )
Anselmi, Freedman, Grisaru, Johansen (’98)
🔶 For N=2 susy fields
N
N
Tr R3
N =2 = Tr RN =2 = 48(a c) ;
Tr RN =2IaIb = δab(4a 2c) .
SUR(2) × UR(1); RN =2 ≡ UR(1) charge, I3 ⊂ SUR(2)
Any N=2 theory has global R symmetries
Tachikawa: Lecture Notes In Physics ‘15
Gaiotto, ‘09
Chacaltana, Distler, ‘10
a and c
Argyres-Plesser-Seiberg-Witten ‘96 Eguchi-Hori-Ito-Yan ‘96 Argyres-Douglas ‘95 Argyres-Seiberg ‘07 Shapere-Tachikawa ‘08
Most singular (“Argyres-Douglas”) SCFT in SQCD
🔶
Flowing down from N=2 SCFT to N=1 SCFT
µΦ2|F = µ ψψ + . . .
Bonelli, Giacomelli, Maruyoshi, Tanzini (’13)
🔶 ☞ relations
Dijkgraaf, Vafa ’03 Cachazo-Seiberg-Witten ‘03
e.g., for SU(2), NF =1,
RN =1 = 5 6RN =2 + 1 3I3
🔶 Known of N=2 SCFT ⟹
for SU(N), NF =2N-1,
RN =1 = 2 3RN =2 + 2 3I3
{RN =2 , I3} ↔ RN =1 {RN =2 , I3} RN =1
🔶 Known Tr R3 , Tr R of the IR theory - > a, c of the IR theory 🔶 N=1 curves (N=2 SW curves + factorization condition)
e.g., for SU(2), NF =1,
a = 1 48 , c = 1 24 ,
for SU(2), NF =3,
a = 1 6 , c = 1 3 ,
This is 32 -1= 8 massless meson chiral fields !! Weff = µ T r M 3 + . . .
Giacomelli, ‘15
🔶 In all cases,
a c = 1 2
2 ≤ a c ≤ 3 2
“Conformal collider bounds”
H
m a n , M a l d a c e n a , ‘ 8 H
m a n , L i , M e l t z e r , R e j
a r r e r a , R ‘ 1 6
end up with the curve 8 > > > < > > > : v02 = z03 ; w2 = µ02z0 ; z0w = µ0v0 , Ω = dv0dwdz0 . is simply the SW curve of the AD theory Imposing now the constraint [8] D R-charges:
(note)
SU(N), NF =2N-1 AD vacuum:
y2 = PN(x)2 − 4Λ Y
i
✓ x + mi − Λ N ◆ . y2 = x2N−1; λSW = xdy y . setting mi = m∗ = Λ/N
⟹
− D(Uk) = 2k − 1 2 ; k = 2, . . . , N ,
δm = 1 2N − 1 X
i
mi − m∗, m∗ ≡ Λ N .
µΦ2|F = µ ψψ + . . .
8 < : y2 = x2N1(x 4Λ) ; w2 = µ2x(x 4Λ) . variables
z2 + x2N1 = 0 ; w02 + µ02x = 0 ; µ0z = w0xN1 , Ω = dw0dxdz z .
change of variables
RIR = 2 3(RN=2 + I3)
🔶 ’t Hooft anomaly matching conditions Tr R3 , Tr R , Tr R(GF )2
F r e e m a s s l e s s m e s
s i n t h e a d j
n t r e p r e s e n t a t i
S U ( N
F
) ! ! !
W(Ψ) = 1 2 X
i
˜ miΨi + δm Tr Ψ2 + µ0Tr Ψ3,
Ψ
deformation, ˜ mi = δm = 0,
deformation, δm 6= 0
r vacua
a,c at IR
(*)
chiral multiplets
N=2 SCFT
N=0 SCFT
aUV = 11NfNc 360 + 31 180(N 2
c − 1)
− aIR = N 2
f − 1
360 .
SU(N), NF =2N-1
aUV = 7N 2 − N − 5 24
aN=2SCF T = 7N(N − 1) 24
aIR = (2N − 1)2 − 1 48
cUV = 4N 2 − N − 2 12
cN=2SCF T = N(N − 1) 3
cIR = (2N − 1)2 − 1 24
20NfNc + N 2
c 1
10 ;
cIR = N 2
f 1
120 ;
Nf < 11 2 Nc
ψ{ij} , χ[ij] , ηA
i ,
(A = 1, 2, . . . , 8) ,
fermions
⇣ ⌘
¯
¯
Gf = SU(8) × U1(1) × U2(1) ×
N∗ .
U1(1) : ψ ! ei
α N+2ψ ;
η ! e−i α
8 η ;
U2(1) : ψ ! ei
β N+2ψ ;
χ ! e−i
β N−2χ
N∗ ,
N ∗ = GCD{N + 2, N 2, 8}
🔶 Asymptotically free 🔶 No gauge invariant bifermion condensates (four-fermion condensates?)
Bolognesi, Konishi, Shifman ‘18
🔶 Planar equivalence to SYM at large N ?
Armoni, Shifman ‘12
🔶 How is Gf realized at low energies?
] Stuart Raby, Savas Dimopoulos, and Leonard Susskind, Tumbling Gauge Theo- ries, Nucl. Phys. B169, 373 (1980). ] T. Appelquist, A. G. Cohen, M. Schmaltz and R. Shrock, New constraints on chiral gauge theories, Phys. Lett. B 459, 235 (1999) [hep-th/9904172]; T. Ap- pelquist, Z. y. Duan and F. Sannino, Phases of chiral gauge theories, Phys.
F chi- ral gauge theories, Phys. Rev. D 92,105032 (2015) [arXiv:1510.07663 [hep-th]];
tive Behavior of Chiral Gauge Theories with Fermions in Higher-Dimensional Representations, Phys. Rev. D 92, 125009 (2015) [arXiv:1509.08501 [hep-th]]. 4] E. Poppitz and Y. Shang, Chiral Lattice Gauge Theories Via Mirror-Fermion Decoupling: A Mission (im)Possible?, Int. J. Mod. Phys. A 25, 2761 (2010) [arXiv:1003.5896 [hep-lat]].
hφiAi ⇠ hψijηA
j i ,
A = 1, 2, . . . , 8 , h˜ φi
ji = hψikχkji ,
(bifundamental in color and in SU(8))
(adjoint of color SU(N))
🔶 Partial color-flavor locking and dynamical Abelianization
hφiAi = Λ3 B B @ c18 0N−8,8 1 C C A , h˜ φi
ji = Λ3
B B B B B @ a 18 d1 ... dN−12 b 14 1 C C C C C A ,
SU(N)c ⇥ SU(8)f ⇥ U(1)2 ! SU(8)cf ⇥ U(1)N−11 ⇥ SU(4)c .
B a r y
s
B{AB} = ψ{ij}ηA
j ηB i
i
contribute 8+4=12 contribute N-12
˜ BA
j = ψikχkjηA i ⇠ h˜
φi
jiηA i
The sum = N = SU(8)3 |UV
⇥ U(1)2 ⇥ SU(8)f
broken by the adjoint condensate
🔶 Split color-flavor locked SU(8)
h
ji
SU(N)c ⇥ SU(8)f ⇥ U(1)2 ! Y
i
SU(Ai)cf ⇥ Y U(1)cf ⇥ U(1)N−11 ⇥ SU(4)c .
’t Hooft OK
🔶 Full Abelianization
SU(N)c ⇥ SU(8)f ⇥ U(1)2 ! U(1)N−1 ⇥ SU(8)f .
weakly coupled and saturate ’t Hooft trivially
Partial color-flavor locking and partial dynamical Abelianization
Full dynamical Abelianization
🔶 No planar equivalence to SYM 🔶 Dynamical Abelianization (ubiquitous in N=2 theories) 🔶 MAC criterion supports
hφiAi ⇠ hψijηA
j i ,
A = 1, 2, . . . , 8 ,
h˜ φi
ji = hψikχkji ,
🔶 Four-fermion condensates less likely
superconductor picture;
naïvely expected, e.g. with a larger degrees of freedom;
U(1)2 or SU(2) x U(1) #d.f < #d.f
Abelian monopoles strongly-coupled nonAbelian monopoles
Strongly-coupled nonAbelian monopoles and IR fixed point
exp ige
Ai dxi → exp ige
(H = ∇gm r ). 2 ge gm = n, n ∈ Z, Π1(U(1)) = Z
⟨φ⟩̸=0
− → H : similar → monopoles with nonabelian charges if Π2(G/H) ̸= ∅
Dirac ~1930 Regular monopoles F i b e r b u n d l e
B a c k t
. 4
Back to p.18
SU(N) SW curve (pure YM) y2 = PN(x)2 − Λ2N = x2N − X
k
Uk xN−k − Λ2N λ = 1 2πi ∂P(x) ∂x xdx y SW differential aDi = I
αi
λ; ai = I
βi
λ; SU(3) pure YM: a (1,0) monopole, a (1,1) dyon and the (0,1) quark Mnm,i,ne,i = √ 2 |nm,iaDi + ne,iai|
Argyrers, Douglas ’95
massless simultaneously at
M1 M2 M3 M4 A1 A3 A4 A5 A2 A6 M6 M5
Figure 3: Zero loci of the discriminant of the curve of N = 2, SU(3), nf = 4 theory at small m.
U = Tr Φ2 ' 3m2 ; V = Tr Φ3 ' 2m3
Auzzi, Grena, K.K. ‘13
Matrix Charge M1, M4 (±1, 1, 0, 0)4 A2, A5 (±1, −1, ∓1, 0)4 M2, M5 (±2, 2, ∓1, 0) A3, A6 (±2, −2, ±1, 0) M3, M6 (0, 2, ±1, 0) A1, A4 (±4, −2, ∓1, 0)
back to p.11
Qi, ˜ Qi
=
SU(2) × SU(6) ⊂ E6
Flavor symmetry ~ SU(6) x U(1)
g = ∞ g = 0
Minahan-Nemeschansky ’96
α f(r)
A|M⇥ ,
monopole bckgrd gauge su(2) spin 3D normalizable zero mode
c = 1 120(NS + 6 NF + 12 NV ) ; a = 1 360(NS + 11 NF + 62 NV ) N a = 1 360(4 + 11) = 1 24 ; c = 1 120(4 + 6) = 1 12 . a = 1 360(2 + 11 + 62) = 5 24 ; c = 1 120(2 + 6 + 12) = 1 6 .
For N=2 hypermultiplet (pair of chiral multiplets Q and Q bar):
For N=2 vector multiplet:
Back to p.37 ☞
− cUV = 1 20NfNc + N 2
c − 1
10 ; aUV = 11NfNc 360 + 31 180(N 2
c − 1) ,
− cIR = N 2
f − 1
120 ; aIR = N 2
f − 1
360 .
For real-world QCD:
🔶 The result has been checked by following alternative RG paths
UV IR N = 2 IR N = 1 UV N = 1 µ ⌧ Λ2 µ Λ1 IR
Figure 1: RG flow for various values of µ.
N=1 Leff of SQCD
(M, B, q, …)
Seiberg, ‘94
Carlino, K.K. Murayama ‘00 Di Pietro, Giacomelli ’12
B
n e s i , G i a c
e l l i , K K ‘ 1 5
“Left RG route” ( )
µ ⌧ Λ2
discussed above; “Right RG route” ( ):
µ Λ2
the system first flows down to N=1 SQCD with
Weff = m TrM − 1 2µ ✓ Tr M 2 − 1 N (Tr M)2 ◆ + 1 Λ
3N−Nf Nf −N
1
(det M)
1 Nf −N ,
η∗ = m∗ p 2 = ωk 2N Nf N 2Nf/(4N−2Nf)Λ ,
M 2
ij − 2↵Mij + ↵2ij = 0 ;
↵ ≡ Nµm∗ 4N − 2Nf = Tr M Nf .
f M 2 = 0 , f M ≡ M − ↵I . (**)
A bonus: our mesons M ~ Meson M in the Seiberg’s N=1 duality SU(N), NF Q’s < —- > SU(NF - N), NF q’s, M; Result valid for any NF
N.B.
(*) = (**)
− p − − p − − As f → 1 the curve clearly degenerates to a genus one curve. Th ferential develops a pair of poles at infinity
: setting u = 0 th
With the redefinition x → −ix v ; y → 2y v; v → 2iv, we finally get y2 = x3 − v4; ∂λ ∂v = dx y ,
E6 Minahan-Nemeschansky theory
f → 1 τ → 0
means
g → ∞
SCFT at u=v=0
v=0 ➯
But this is SCFT SU(2), NF = 4 theory!
y2 = [(1 - √f) x3 - u x - v ] [(1 + √f) x3 - u x - v ] y2 = - v [ 2 x3 - v ] , ∂λ/∂v = dx /y
Back to p. 38
Vortex 2D dynamics in Higgs phase (U(2))
S(1+1)
σ
= β
2 (∂ na)2 ,
+ fermionic terms
N=(2,2) CP1 sigma model : 2 vacua ➞ kinks = (Abelian) monopole!
Global SU(2) unbroken (Coleman) ≡ Gauge dynamics in 4D in Coulomb phase
Dorey
dt dz
V a f a , H
i Shifman et. al.
xy2 ∼
n)
⇥2 − 4Λ4x2n = x2n(x − φ2
n − 2Λ2)(x − φ2 n + 2Λ2).
y2 ∿ x2n singular SCFT (EHIY point); strongly interacting, relatively non-local monopoles and dyons
Vacua in confinement phase surviving N=1, μ Φ2 perturbation)
⟹
✓Nf ◆ + ✓Nf 2 ◆ + . . . ✓Nf Nf ◆ = 2Nf−1
even r vacua, from one of the Chebyshev vacua
vacua
Carlino-Konishi-Murayama ‘00
✓Nf 1 ◆ + ✓Nf 3 ◆ + . . . ✓ Nf Nf 1 ◆ = 2Nf−1 .
Figs.
20 40
5 10 15
Jackiw-Rebbi flavor dressing color fields color flavor fields correlated UNCORRELATED
Qi, ˜ Qi
=
SU(2) × SU(6) ⊂ E6
Flavor symmetry ~ SU(6) x U(1)
g = ∞ g = 0
Minahan-Nemeschansky ’96
Gauge symmetry destroyed (inconsistency)
Abelian / nonAbelian anomalies
♦ ♦ Anomaly cancellation needed
OK in
(NOT an inconsistency)
♦
Back to p.4
(Nambu’s Erice lecture!)
Fukuda, Steinberger, Schwinger, Adler, Bell, Jackiw, Bardeen, …