橋本幸士
大阪大学素粒子論研究室 H726室
理化学研究所
橋本数理物理学研究室
[Oka, Aoki, PRL 95 (2005) 137601]
Supersymmetric QCD 1d Mo8 insulator
[Oka, KH 1307.7423]
Condensed ma8er
“QCD-‐ma8er”
What resides inside neutron stars?
Supernova remnant RCW103
[D.Page]
[Fukushima, Hatsuda 1005.4814]
``QCD ma4er” : fron8er in quark physics
Phase diagram of QCD
L = 1
2E2 − 1 8π2
! ∞
0
ds s3
"
eEs cot(eEs)− 1 + 1
3(eEs)2
#
Im L =
$∞ n=1
e2E2 4π3
1
n2 exp
"
−nπm2 eE
#
L = TD72π2R2
!
dr r3
%
1 − (2πα"E)2 R4
((2πα"m)2 + r2)2 z = R2/r
dz = −R2dr/r2
dzz−5 = (r5/R10)(−R2)dr/r2 = −r3dr/R8 critical electric field
Ecr = 2πα"m2 R2 =
√2πm2
√λ
Im L = Nc
25πe2E2
&
1 + 25/2 m2
√λeE log m2
√λeE + higher '
Im L = 1
24πe2E2
&
1 + 6 π
m2
eE log m2
eE + higher '
LQCD = −1
4Fµνa Faµν + ¯ψi(iγµDµ − mi) ψi
1
[藤森研講義録]
Mee8ng point for … observa8on and theory
EquaJon of state for nuclear ma8er
[Hebeler et.al (2010 PRL)]
Theory
(QCD)
Obs.
Superstringy mathemaJcs resolves mysteries in strongly correlated systems
1. Is superstring useful?
2. Duality connecting theories 3. Challenge to neutron stars
Road map 7 pages
7 pages 5 pages
1
2
3
Superstring gets useful in these 7 years
1997
2013 My publicaJon With units
Without units (hep-‐th)
hep-‐ph astro-‐ph
nucl-‐th hep-‐lat
cond-‐mat
1
-1Quarks and gluons
Nucleons and hadrons
Atomic nuclei, neutron stars Nuclear physics
LaZce QCD Superstring Isola8on between par8cle and nuclear physics
1
-2QCD is strongly coupled, hard to calculate
L = 1
2E2 − 1 8π2
! ∞
0
ds s3
"
eEs cot(eEs) − 1 + 1
3(eEs)2
#
Im L =
$∞ n=1
e2E2 4π3
1
n2 exp
"
−nπm2 eE
#
L = TD72π2R2
!
dr r3
%
1 − (2πα"E)2 R4
((2πα"m)2 + r2)2 z = R2/r
dz = −R2dr/r2
dzz−5 = (r5/R10)(−R2)dr/r2 = −r3dr/R8 critical electric field
Ecr = 2πα"m2
R2 =
√2πm2
√λ
Im L = Nc
25πe2E2
&
1 + 25/2 m2
√λeE log m2
√λeE + higher '
Im L = 1
24πe2E2
&
1 + 6 π
m2
eE log m2
eE + higher '
LQCD = −1
4Fµνa Faµν + ¯ψi (iγµDµ − mi) ψi
1
QCD acJon for quarks and gluons: simple but highly nonlinear j = 0
j = (2πα!E)3/2/R
δE = TD7π2(2πα!E)2R4
!
−
" 1 0
dy y3
#1 − y2 −
$
−
" ∞
0
dy y3
%
1 − y2 1 − y3
&'
y ≡ 2πα!Ez2/R2
= c
8π2 NcE2
(c ≈ 0.856)
Γ ∼ exp
!
−
√2π2m2
√λeE '
" ∞
−∞
dx e−mx2 =
( π m
" ∞
−∞
dx e−mx2−gx4 = ?
" ∞
−∞
dx e−mx2−gx4 =
" ∞
−∞
dx e−mx2 )
1 − gx4 + 1
2g2x8 + · · ·
*
=
( π m
)
1 − 3
4m2g + 105
32m4 g2 + · · ·
*
3
Strong nonlinearity (strong coupling), perturbaJon impossible j = 0
j = (2πα!E)3/2/R
δE = TD7π2(2πα!E)2R4
!
−
" 1 0
dy y3
#1 − y2 −
$
−
" ∞
0
dy y3
%1 − y2 1 − y3
&'
y ≡ 2πα!Ez2/R2
= c
8π2 NcE2
(c ≈ 0.856)
Γ ∼ exp
!
−
√2π2m2
√λeE '
" ∞
−∞
dx e−mx2 =
( π m
" ∞
−∞
dx e−mx2−gx4 = ?
" ∞
−∞
dx e−mx2−gx4 =
" ∞
−∞
dx e−mx2 )
1−gx4+ g2x8
2 + · · ·
*
=
( π m
)
1− 3g
4m2 +105g2
32m4 +· · ·
*
3 Linear
Nonlinear
j = 0
j = (2πα!E)3/2/R
δE = TD7π2(2πα!E)2R4
!
−
" 1 0
dy y3
#1 − y2 −
$
−
" ∞
0
dy y3
%
1 − y2 1 − y3
&'
y ≡ 2πα!Ez2/R2
= c
8π2NcE2
(c ≈ 0.856)
Γ ∼ exp
!
−
√2π2m2
√λeE '
" ∞
−∞
dx e−mx2 =
( π m
" ∞
−∞
dx e−mx2−gx4 = ?
" ∞
−∞
dx e−mx2−gx4 =
" ∞
−∞
dx e−mx2 )
1−gx4+g2x8
2 + · · ·
*
=
( π m
)
1− 3g
4m2 +105g2
32m4 +· · ·
*
3 j = 0
j = (2πα!E)3/2/R
δE = TD7π2(2πα!E)2R4
!
−
" 1 0
dy y3
#1 − y2 −
$
−
" ∞
0
dy y3
%
1 − y2 1 − y3
&'
y ≡ 2πα!Ez2/R2
= c
8π2NcE2
(c ≈ 0.856)
Γ ∼ exp
!
−
√2π2m2
√λeE '
" ∞
−∞
dx e−mx2 =
( π m
" ∞
−∞
dx e−mx2−gx4 = ?
" ∞
−∞
dx e−mx2−gx4 =
" ∞
−∞
dx e−mx2 )
1−gx4+g2x8
2 + · · ·
*
=
( π m
)
1− 3g
4m2 +105g2
32m4 +· · ·
*
3
0.5 1.0 1.5 2.0
0.5 1.0
1.5 2.0 1.0
1.5 2.0 2.5 3.0
Numerical calculaJon?
+ + + …
PerturbaJon
1
-3QCD Hypothetical higher dim. gravity Graviton excitation
U(Nf) gauge theory Soliton
Glueball Meson Baryon
Deconfinement Finite temp
Quark density Plasma
Black hole
Hawking temp
Electric field in U(Nf)
Event horizon formation
Useful superstring as a math tool
Solve equivalent system via duality
Problems : Strong coupling, many body, solitons, …
Note: no need for theories to be really stringy.
Exciton Insulator
Conduction Phonon
electrons Heat bath
Impurity
Thermalize
1
-4[Brower,Mathur,Tan (03)]
LaZce
[Morningstar,Peardon (99)]
Superstring
Superstring: better than simulations?
1
-5Superstring Experiment
LaZce
[Sakai,Sugimoto,KH (0806.3122)]
(0.74 fm)2 0
0.54 fm 2.2 – 1.3
0.73 7.5 5.8 4.4 2.3 0.20 –1.9
(0.875 fm)2 – 0.116 fm2
0.674 fm 2.79 –1.91
1.27 13.2 4.2 – 6.5 3.7 – 7.5
– – –
4.99 2.49 0.06 –2.45 Radii of proton/neutron
Ex) Proton radius from superstring
1
-610 15 20 25 30
-0.004 -0.002 0.002 0.004 0.006 0.008 0.010
V (r)
r
(Inter-‐nucleon distance)3
S
1[Sakai,Sugimoto,KH (0901.4449)]
[Aoki,Ishii,Hatsuda (‘07)]
LaZce QCD simulaJons : Experiments:
[Stoks,Klomp,Terheggen,deSwart (‘94)]
Superstring: Nuclear forces
Ex) Nuclear force from superstring
1
-7Superstringy mathemaJcs resolves mysteries in strongly correlated systems
1. Is superstring useful?
2. Duality connecting theories 3. Challenge to neutron stars
Road map 7 pages
7 pages 5 pages
1
2
3
Duality
theory
A Theory
= B
Strongly coupled (correlated) Too nonlinear to solve
Too many DoF
Weakly coupled, solvable
2
-1Holographic equivalence
Describe mulJ vorJces.
A) Field theory of order parameter
S = dt
k
( ˙X(k)i (t))2 +
k1=k2
V (|X(k1)(t) X(k2)(t)|)
S = d3x | µ (x, y, t)|2 V (| |) B) ParJcle-‐like vorJces
For full equivalence?
Topological number fixed?
Near-‐vorJces?
VorJces on top of each other?
Low energy excitaJons only?
Explicit examples:
ADHM construcJon of instantons Nahm construcJon of monopoles
2
-2Stringy duality: Gauge/gravity duality
D-‐brane = vorJces in superstring theory
・ Characterized by mass and charges
・ Gauge theories on the D-‐branes Gauge/Gravity duality:
A) Gauge theory Strongly coupled, large N
B) Gravity Weakly coupled, curved higher dimensional space [Maldacena ‘98]
S = 1
16⇡GN
Z
d5x p
g (R + 2⇤) + · · ·
S = 1
2g2 Z
d4x tr Fµ⌫Fµ⌫ + · · ·
2
-3Quantizing strings defined in 10D spacetime
Open string Massless gauge field Closed string Massless graviton
D-branes = Object on which open strings can end
Open string theory on the Dp-brane is : SU(Nc) gauge theory in p+1 dimensions
Nc open strings
Nc parallel Dp-branes
2
D-‐brane giving the duality
2
-4Deform
Quantizing strings defined in 10D spacetime
Open string Massless gauge field Closed string Massless graviton
D-branes = Object on which open strings can end D-‐brane giving the duality
2
-4= Source of closed strings
= Source of gravity
= Extended blackhole “blackbrane” in 10D
Quantizing strings defined in 10D spacetime
Open string Massless gauge field Closed string Massless graviton
D-branes = Object on which open strings can end D-‐brane giving the duality
2
-4Black brane Nc D-branes
Propagation of SU(Nc) gauge theory
composite states
Propagation of graviton in near-horizon geometry
of black p-brane (Glueball)
Gluon
Large N
cLarge λ
Deriving the Gauge/gravity duality
2
-5Superstringy mathemaJcs resolves mysteries in strongly correlated systems
1. Is superstring useful?
2. Duality connecting theories 3. Challenge to neutron stars
Road map 7 pages
7 pages 5 pages
1
2
3
[D.Page]
[Fukushima, Hatsuda 1005.4814]
What resides inside the neutron stars?
Phase diagram of QCD
L = 1
2E2 − 1 8π2
! ∞
0
ds s3
"
eEs cot(eEs)− 1 + 1
3(eEs)2
#
Im L =
$∞ n=1
e2E2 4π3
1
n2 exp
"
−nπm2 eE
#
L = TD72π2R2
!
dr r3
%
1 − (2πα"E)2 R4
((2πα"m)2 + r2)2 z = R2/r
dz = −R2dr/r2
dzz−5 = (r5/R10)(−R2)dr/r2 = −r3dr/R8 critical electric field
Ecr = 2πα"m2 R2 =
√2πm2
√λ
Im L = Nc
25πe2E2
&
1 + 25/2 m2
√λeE log m2
√λeE + higher '
Im L = 1
24πe2E2
&
1 + 6 π
m2
eE log m2
eE + higher '
LQCD = −1
4Fµνa Faµν + ¯ψi(iγµDµ − mi) ψi
1
3
-1From hypothe8cal QCD to real QCD
Gauge theory with 4 supersymmetries (N=4 Super Yang-‐Mills)
Supersymmetric gauge theory + quarks (N=2 Super QCD)
Non-‐supersymmetric SU(N) gauge theory + quarks (Large N QCD)
Non-‐supersymmetric SU(3) gauge theory + quarks (QCD) (1)
(2)
(3)
(4)
3
-2Gauge theory with 4 supersymmetries (N=4 Super Yang-‐Mills)
The road to real QCD: (1)
(1)
Gluon sector: gluons + 4 gluinos + 6 scalars Quark sector: Not allowed
Temp
Baryon chemical potenJal Gluon plasma
Black hole in
higher dimensions
Closed string
3
-3(2)
Gluon sector: gluons + 2 gluinos + 2 scalars Quark sector: quarks + scalar quarks
Quark-‐gluon plasma
Gluon plasma + mesons
Unstable phase
[Ghoroku, Ishihara, Nakamura ‘07]
Closed string
Open string Temp
Baryon chemical potenJal
The road to real QCD: (2)
Supersymmetric gauge theory + quarks (N=2 Super QCD)
3
-4(3)
Gluon sector: gluons + heavy gluinos Quark sector: quarks
Quark gluon plasma
Hadron Instability?
Gluon plasma + meson
[Aharony, Sonnenschein, Yankielowicz ‘06]
Temp
Baryon chemical potenJal
The road to real QCD: (3)
Non-‐supersymmetric SU(N) gauge theory + quarks (Large N QCD)
3
-5(4)
Gluon sector: gluons Quark sector: quarks
? Challenge ?
Temp
Baryon chemical potenJal
The road to real QCD: (4)
Non-‐supersymmetric SU(3) gauge theory + quarks (QCD)
3
-6Various applica8ons to cond-‐mat
Holographic superconducJvity
Scalar condensaJon
[Hartnoll, Herzog, Horowitz ‘08]
Holographic viscosity
Gravity perturbaJon
[Kovtun, Son, Starinets ‘04]
3
-7Superstringy mathemaJcs resolves mysteries in strongly correlated systems
1. Is superstring useful?
2. Duality connecting theories 3. Challenge to neutron stars
Road map 7 pages
7 pages 5 pages