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Structure of the Vacuum in Light-Front Dynamics

Structure of the Vacuum in Light-Front Dynamics

and Emergent Holographic QCD

Guy F. de Teramond

Universidad de Costa Rica

Ferrara International School

Niccolo Cabeo 2014

Vacuum and Symmetry Breaking:

From the Quantum to the Cosmos

Ferrara, May 19-23, 2014

Image credit: ic-msquare

In collaboration with Stan Brodsky (SLAC) and Hans G. Dosch (Heidelberg)

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 1

Structure of the Vacuum in Light-Front Dynamics

∆ηµoκριτoσ460 - 370 BC

νoµω ψυχρoν, νoµω θερµoν, ετεη δε ατoµα και κενoν

(By convention cold, by convention hot, in reality atoms and the void)

Democritus 460 - 370 BC

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 2

Structure of the Vacuum in Light-Front Dynamics

Contents

1 Introduction 4

2 Dirac Forms of Relativistic Dynamics 6

3 Light-Front Dynamics and Light-Front Vacuum 8

4 Light-Front Quantization of QCD 12

5 Semiclassical Approximation to QCD in the Light Front 15

6 Effective Confinement from Underlying Conformal Invariance 19

7 Gravity in AdS and Light Front Holographic Mapping 26

8 Higher Integer-Spin Wave Equations in AdS Space 27

9 Meson Spectrum 30

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 3

Structure of the Vacuum in Light-Front Dynamics

10 Higher Half-Integer Spin Wave Equations in AdS Space 34

11 Baryon Spectrum 36

12 Conclusions 38

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 4

Structure of the Vacuum in Light-Front Dynamics

1 Introduction

• SLAC and DESY 70’s: elementary interactions of quarks and gluons at short distances remarkably

well described by QCD

• No understanding of large distance strong dynamics of QCD: how quarks and gluons are confined and

how hadrons emerge as asymptotic states

• Euclidean lattice important first-principles numerical simulation of nonperturbative QCD: excitation

spectrum of hadrons requires enormous computational complexity beyond ground-state configurations

• Only known analytically tractable treatment in relativistic QFTh is perturbation theory: description of

confinement from perturbation theory is not possible (Kinoshita-Lee-Nauenberg Theorem)

• Important theoretical goal: find initial analytic approximation to strongly coupled QCD, like Schrodinger

or Dirac Eqs in atomic physics, corrected for quantum fluctuations

• Convenient frame-independent Hamiltonian framework for treating bound-states in relativistic theories

is light-front (LF) quantization

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Structure of the Vacuum in Light-Front Dynamics

• Definition of invariant LF vacuum within causal horizon P 2|0〉 = 0

• Simple structure of vacuum allows definition of partonic content of hadron in terms of wavefunctions:

quantum-mechanical probabilistic interpretation of hadronic states

• Calculation of matrix elements 〈P + q|J |P 〉 requires boosting the hadronic bound state from |P 〉 to

|P + q〉: no change in particle number from boost in LF (kinematical problem)

• To a first semiclassical approximation one can reduce the strongly correlated multi-parton LF dynamics

to an effective one-dim QFTh, which encodes the conformal symmetry of the classical QCD Lagrangian

• Uniqueness of the form of confining interaction from one dim conformal QFTh: extension of conformal

quantum mechanics to LF bound-state dynamics

• Invariant Hamiltonian equation for bound states similar structure of AdS equations of motion: direct

connection of QCD and AdS/CFT possible

• Description of strongly coupled gauge theory in physical space-time using a dual gravity description in

a higher dimensional space (holographic)

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 6

Structure of the Vacuum in Light-Front Dynamics

2 Dirac Forms of Relativistic Dynamics[Dirac (1949)]

• The Poincare group is the full symmetry group of any form of relativistic dynamics

[Pµ, P ν ] = 0,

[Mµν , P ρ] = i (gµρP ν − gνρPµ) ,

[Mµν ,Mρσ] = i (gµρMνσ − gµσMνρ + gνσMµρ − gνρMµσ) ,

• Poincare generators separated into kinematical and dynamical

• Kinematical generators act along the initial hypersurface where initial conditions are imposed and

contain no interactions (leave invariant initial surface)

• Dynamical generators are responsible for evolution of the system and depend on the interactions

(map initial surface into another surface)

• Each form has its Hamiltonian and evolve with different time, but results computed in any form should

be identical (different parameterizations of space-time)

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 7

Structure of the Vacuum in Light-Front Dynamics

ct(a) (b) (c)

y

z

ct

y

z

ct

y

z

8-20138811A4

• Instant-form: initial surface defined by x0 = 0

P 0, K dynamical, P, J kinematical

• Front-form: initial surface tangent to the light cone x+ = x0 + x3 = 0 ( P± = P 0 ± P 3)

P−, Jx, Jy dynamical, P+, P⊥, J3, K kinematical

• Point-form: initial surface is the hyperboloid x2 = κ2 > 0, x0 > 0

Pµ dynamical, Mµν kinematical

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 8

Structure of the Vacuum in Light-Front Dynamics

3 Light-Front Dynamics and Light-Front Vacuum

• Hadron with 4-momentum P = (P+, P−,P⊥), P± = P 0 ± P 3, mass-shell relation

P 2 = M2 leads to dispersion relation for LF Hamiltonian P−

P− =P2⊥ +M2

P+, P+ > 0

• n-particle bound state with p2i = m2

i , pi =(p+i , p

−i ,p⊥i

), for each constituent i

p−i =p2⊥i +m2

i

p+i

, p+i > 0

• Longitudinal momentum P+ is kinematical: sum of single particle constituents p+i of bound state

P+ =∑i

p+i , p+

i > 0

• LF Hamiltonian P− is dynamical: bound-state is arbitrarly off the LF energy shell

P− −n∑i

p−i < 0

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 9

Structure of the Vacuum in Light-Front Dynamics

• LF evolution given by relativistic Schrodinger-like equation (x+ = x0 + x3 LF time)

i∂

∂x+|ψ(P )〉 = P−|ψ(P )〉

where

P−|ψ(P )〉 =P2⊥ +M2

P+|ψ(P )〉

• Construct LF invariant Hamiltonian P 2 = PµPµ = P−P+ −P2

P 2|ψ(P )〉 = M2|ψ(P )〉

• Since P+ and P⊥ are kinematical, linear QM evolution in LF Hamiltonian P− is maintained

• State |ψ(P )〉 is expanded in multi-particle Fock states |n〉 of the free LF Hamiltonian

|ψ〉 =∑n

ψn|n〉, |n〉 = |uud〉, |uudg〉, |uudqq〉, · · ·

with p2i = m2

i , pi = (p+i , p

−i ,p⊥i), for each constituent i in state n

• Fock component ψn is the light-front wave function (LFWF)

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 10

Structure of the Vacuum in Light-Front Dynamics

Vaccum in the Front-Form of Dynamics

• P+ =∑

i p+i , p

+i > 0: LF vacuum is the state with P+ = 0 and contains no particles: all other

states have P+ > 0 (usual vacuum bubbles are kinematically forbidden in the front form !)

• Frame independent definition of the vacuum within the causal horizon

P 2|0〉 = 0

(LF vacuum also has zero quantum numbers and P+ = 0)

• LF vacuum is defined at fixed LF time x+ = x0 + x3

over all x− = x0 − x3 and x⊥, the expanse of space

that can be observed within the speed of light

• Causality is maintained since LF vacuum only

requires information within the causal horizon

• The front form is a natural basis for cosmology:

universe observed along the front of a light wave

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 11

Structure of the Vacuum in Light-Front Dynamics

Vacuum in the Instant-Form of Dynamics

• Unsolved problems concerning the instant vacuum structure of QCD, confinement and chiral symmetry

breaking

• In Lattice QCD the structure of the instant-form vacuum is sampled in the Euclidean region

• If monopoles or vortices are removed from the vacuum confinement and chiral symmetry breaking

disappear

• Instantons provide a mechanism for symmetry breaking through the Banks-Casher relation

〈0|ψψ|0〉 = −πρ(0),

where ρ(0) is the density or Dirac-zero modes /Dψλ = λψλ, but do not lead to confinement

• No convincing proof that continuum QCD is confining in the infrared

• Confinement in continuum QCD is a fundamental unsolved problem in theoretical physics

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 12

Structure of the Vacuum in Light-Front Dynamics

4 Light-Front Quantization of QCD

• Start with SU(3)C QCD Lagrangian

LQCD = ψ (iγµDµ −m)ψ − 14G

aµνG

aµν

• Express the hadron four-momentum generator P = (P+, P−,P⊥) in terms of dynamical fields

ψ+ = Λ±ψ and A⊥(Λ± = γ0γ±

)quantized in null plane x+ = x0 + x3 = 0

P− = 12

∫dx−d2x⊥ψ+ γ

+ (i∇⊥)2 +m2

i∂+ψ+ + interactions

P+ =∫dx−d2x⊥ψ+γ

+i∂+ψ+

P⊥ = 12

∫dx−d2x⊥ψ+γ

+i∇⊥ψ+

where the integrals are over initial surface x+ = 0, where commutation relation for fields are defined

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 13

Structure of the Vacuum in Light-Front Dynamics

• Dirac field ψ+ expanded in terms of ladder operators b(q)|0〉 = d(q)|0〉 = 0

ψ+(x−,x⊥)α =∑λ

∫q+>0

dq+√2q+

d2q⊥(2π)3

[bλ(q)uα(q, λ)e−iq·x + dλ(q)†vα(q, λ)eiq·x

]with

b(q), b†(q′)

=d(q), d†(q′)

= (2π)3 δ(q+ − q′+) δ(2)

(q⊥ − q′⊥

)

P− =∑λ

∫dq+d2q⊥

(2π)3(q2⊥ +m2

q+

)b†λ(q)bλ(q) + interactions

P+ =∑λ

∫dq+d2q⊥

(2π)3q+ b†λ(q)bλ(q)

P⊥ =∑λ

∫dq+d2q⊥

(2π)3q⊥ b

†λ(q)bλ(q)

where q− = q2⊥+m2

q+

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 14

Structure of the Vacuum in Light-Front Dynamics

• Relative partonic coordinates: k+i = xiP

+, p⊥i = xiP⊥i + k⊥in∑i=1

xi = 1,n∑i=1

k⊥i = 0

• Fock component ψn(xi,k⊥i, λzi ) depends only on relative coordinates: longitudinal momentum

fraction xi = k+i /P

+, transverse momentum k⊥i and spin λzi

• LFWF ψn is frame independent

• Momentum conservation: P+ =∑n

i=1 k+i , k+

i > 0, but LFWF represents a bound-state which is

off the LF energy shell, P− −∑n

i k−i < 0

• Express off-shell dependence of bound-state in terms of invariant variable

(invariant mass of constituents)

M2n = (k1 + k2 + · · ·+ kn)2 =

( n∑i=1

kµi

)2=∑i

k2⊥i +m2

i

xi

• M2−M2n is the measure of the off-energy shell: key variable which controls the bound state

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 15

Structure of the Vacuum in Light-Front Dynamics

5 Semiclassical Approximation to QCD in the Light Front[GdT and S. J. Brodsky, PRL 102, 081601 (2009)]

• Effective reduction of strongly coupled LF multiparticle dynamics to a 1-dim QFT with no particle cre-

ation and absorption: LF quantum mechanics !

• Central problem is derivation of effective interaction which acts only on the valence sector:

express higher Fock states as functionals of the lower ones

• Advantage: Fock space not truncated and symmetries of the Lagrangian preserved[H. C. Pauli, EPJ, C7, 289 (1999)

• Compute M2 from hadronic matrix element 〈ψ(P ′)|PµPµ|ψ(P )〉=M2〈ψ(P ′)|ψ(P )〉

• Find

M2 =∑n

∫ [dxi][d2k⊥i

]∑q

(k2⊥q +m2

q

xq

)|ψn(xi,k⊥i)|2 + interactions

with phase space normalization∑n

∫ [dxi] [d2k⊥i

]|ψn(xi,k⊥i)|2 = 1

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 16

Structure of the Vacuum in Light-Front Dynamics

• In terms of n−1 independent transverse impact coordinates b⊥j , j = 1, 2, . . . , n−1,

M2 =∑n

n−1∏j=1

∫dxjd

2b⊥jψ∗n(xi,b⊥i)∑q

(−∇2

b⊥q+m2

q

xq

)ψn(xi,b⊥i) + interactions

with normalization ∑n

n−1∏j=1

∫dxjd

2b⊥j |ψn(xj ,b⊥j)|2 = 1.

• Semiclassical approximation

ψn(k1, k2, . . . , kn)→ φn(

(k1 + k2 + · · ·+ kn)2︸ ︷︷ ︸M2n=

Pi

k2⊥i+m

2i

xi

), mq → 0

• For a two-parton system in the mq → 0 M2qq = k2

⊥x(1−x)

• Conjugate invariant variable in transverse impact space is

ζ2 = x(1− x)b2⊥

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 17

Structure of the Vacuum in Light-Front Dynamics

• To first approximation LF dynamics depend only on the invariant variable ζ , and dynamical properties

are encoded in the hadronic mode φ(ζ)

ψ(x, ζ, ϕ) = eiLϕX(x)φ(ζ)√2πζ

,

where we factor out the longitudinal X(x) and orbital kinematical dependence from LFWF ψ

• Ultra relativistic limit mq → 0 longitudinal modes X(x) decouple (L = Lz)

M2 =∫dζ φ∗(ζ)

√ζ

(− d2

dζ2− 1ζ

d

dζ+L2

ζ2

)φ(ζ)√ζ

+∫dζ φ∗(ζ)U(ζ)φ(ζ),

where effective potential U includes all interaction terms upon integration of the higher Fock states

• LF eigenvalue equation PµPµ|φ〉 = M2|φ〉 is a LF wave equation for φ(

− d2

dζ2− 1− 4L2

4ζ2︸ ︷︷ ︸kinetic energy of partons

+ U(ζ)︸ ︷︷ ︸confinement

)φ(ζ) = M2φ(ζ)

• Relativistic and frame-independent LF Schrodinger equation: U is instantaneous in LF time

• Critical valueL = 0 corresponds to lowest possible stable solution, the ground state of the LF invariant

Hamiltonian P 2

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 18

Structure of the Vacuum in Light-Front Dynamics

• Compare invariant mass in the instant-form in the hadron center-of-mass system P = 0,

M2qq = 4m2

q + 4p2

with the invariant mass in the front-form in the constituent rest frame, kq + kq = 0

M2qq =

k2⊥ +m2

q

x(1− x)

obtain

U = V 2 + 2√

p2 +m2q V + 2V

√p2 +m2

q

where p2⊥ = k2

⊥4x(1−x) , p3 = mq(x−1/2)√

x(1−x), and V is the effective potential in the instant-form

• For small quark masses a linear instant-form potential V implies a harmonic front-form potential U

and thus linear Regge trajectories

[A. P. Trawinski, S. D. Glazek, S. J. Brodsky, GdT, H. G. Dosch, arXiv: 1403.5651]

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 19

Structure of the Vacuum in Light-Front Dynamics

6 Effective Confinement from Underlying Conformal Invariance[S. J. Brodsky, GdT and H.G. Dosch, PLB 729, 3 (2014)]

• Incorporate in a 1-dim QFT – as an effective theory, the fundamental conformal symmetry of the 4-dim

classical QCD Lagrangian in the limit of massless quarks

• Invariance properties of 1-dim field theory under the full conformal group from dAFF action

[V. de Alfaro, S. Fubini and G. Furlan, Nuovo Cim. A 34, 569 (1976)]

S = 12

∫dt(Q2 − g

Q2

)where g is a dimensionless number (Casimir operator which depends on the representation)

• The equation of motion

Q− g

Q3= 0

and the generator of evolution in t, the Hamiltonian

H = 12

(Q2 +

g

Q2

)follow from the dAFF action

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 20

Structure of the Vacuum in Light-Front Dynamics

• Absence of dimensional constants implies that the action

S = 12

∫dt(Q2 − g

Q2

)is invariant under a larger group of transformations, the general conformal group

t′ =αt+ β

γt+ δ, Q′(t′) =

Q(t)γt+ δ

with αδ − βγ = 1

• Applying Noether’s theorem one obtains 3 conserved operators

I. Translations in t: H = 12

(Q2 + g

Q2

),

II. Dilatations: D = 12

(Q2 + g

Q2

)t− 1

4

(QQ+QQ

),

III. Special conformal transformations: K = 12

(Q2 + g

Q2

)t2 − 1

2

(QQ+QQ

)t+ 1

2Q2,

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 21

Structure of the Vacuum in Light-Front Dynamics

• Using canonical commutation relations [Q(t), Q(t)] = i find

[H,D] = iH, [H,K] = 2iD, [K,D] = −iK,

the algebra of the generators of the conformal group Conf(R1)

• Introduce the linear combinations

J12 =12

(1aK + aH

), J01 =

12

(1aK − aH

), J02 = D,

where a has dimension t since H and K have different dimensions

• Generators J have commutation relations

[J12, J01] = iJ02, [J12, J02] = −iJ01, [J01, J02] = −iJ12,

the algebra of SO(2, 1)

• J0i, i = 1, 2, boost in space direction i and J12 rotation in the (1,2) plane

• J12 is compact and has thus discrete spectrum with normalizable eigenfunctions and a ground state

• The relation between the generators of conformal group and generators of SO(2, 1) suggests that

the scale a may play a fundamental role

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 22

Structure of the Vacuum in Light-Front Dynamics

• dAFF construct a new generator as a superposition of the 3 constants of motion

G = uH + vD + wK

and introduce new time variable τ and field operator q(τ)

dτ =dt

u+ vt+ wt2, q(τ) =

Q(t)

[u+ vt+ wt2]12

• Find usual quantum mechanical evolution for time τ

G|ψ(τ)〉 = id

dτ|ψ(τ)〉

i [G, q(τ)] =dq(τ)dτ

and usual equal-time quantization [q(t), q(t)] = i

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 23

Structure of the Vacuum in Light-Front Dynamics

• In terms of τ and q(τ)

S = 12

∫dt(Q2 − g

Q2

)= 1

2

∫dτ(q2 − g

q2− 4uω − v2

4q2)

+ surface term

Action is conformal invariant invariant up to a surface term !

• The corresponding Hamiltonian

G = 12

(q2 +

g

q2+

4uω − v2

4q2)

is a compact operator for4uω − v2

4> 0

• Scale appears in the Hamiltonian without affecting the conformal invariance of the action !

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 24

Structure of the Vacuum in Light-Front Dynamics

• Evolution in τ in terms of original field operator Q(t) at t = 0

G(Q, Q) =12u

(Q2 +

g

Q2

)− 1

4v(QQ+ QQ

)+

12wQ2

= uH + vD + wK,

• The Schrodinger picture follows from the representation of Q and P = Q

Q→ x, Q→ −i ddx

• dAFF Conformal Quantum Mechanics !

• Schrodinger wave equation determines evolution of bound states in terms of the variable τ

i∂

∂τψ(x, τ) = Hτ

(x,−i d

dx

)ψ(x, τ)

• dAFF Hamiltonian G

G =12u

(− d2

dx2+

g

x2

)+i

4v

(xd

dx+

d

dxx

)+

12wx2

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 25

Structure of the Vacuum in Light-Front Dynamics

• Compare dAFF Hamiltonian

G =12u

(− d2

dx2+

g

x2

)+i

4v

(xd

dx+

d

dxx

)+

12wx2

with LF Hamiltonian for u = 2, v = 0,

P 2 = − d2

dζ2− 1− 4L2

4ζ2+ U(ζ)

• x is identified with the LF variable ζ : x = ζ

• Casimir g with the LF orbital angular momentum L: g = L2 − 14

• w = 2λ2 ∼ 1a2 fixes effective LF confining interaction to quadratic λ2 ζ2 dependence

U ∼ λ2ζ2

• Also, dAFF evolution variable τ is identified with LF time τ = x+/P+

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 26

Structure of the Vacuum in Light-Front Dynamics

7 Gravity in AdS and Light Front Holographic Mapping

RNKLM = −1

R2(gNLgKM − gNMgKL)

• Why is AdS space important?

AdS5 is space of maximal symmetry, negative curvature and a four-dim boundary: Minkowski space

• Isomorphism of SO(4, 2) group of conformal transformations with generators Pµ,Mµν,Kµ, D with

the group of isometries of AdS5 Dim isometry group of AdSd+1: (d+1)(d+2)2

• AdS5 metric xM = (xµ, z):

ds2 =R2

z2(ηµνdxµdxν − dz2)

• Since the AdS metric is invariant under a dilatation of all coordinates xµ → λxµ, z → λz, the

variable z acts like a scaling variable in Minkowski space

• Short distances xµxµ → 0 map to UV conformal AdS5 boundary z → 0

• Large confinement dimensions xµxµ ∼ 1/Λ2

QCD map to IR region of AdS5, z ∼ 1/ΛQCD, thus

AdS geometry has to be modified at large z to include the scale of strong interactions

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 27

Structure of the Vacuum in Light-Front Dynamics

8 Higher Integer-Spin Wave Equations in AdS Space[GdT, H.G. Dosch and S. J. Brodsky, PRD 87, 075004 (2013)]

• Description of higher spin modes in AdS space (Frondsal, Fradkin and Vasiliev)

• Integer spin-J fields in AdS conveniently described by tensor field ΦN1···NJ with effective action

Seff =∫ddx dz

√|g| eϕ(z) gN1N ′1 · · · gNJN ′J

(gMM ′DMΦ∗N1...NJ

DM ′ΦN ′1...N′J

− µ2eff (z) Φ∗N1...NJ

ΦN ′1...N′J

)DM is the covariant derivative which includes affine connection and dilaton ϕ(z) breaks conformality

• Effective mass µeff (z) is determined by precise mapping to light-front physics

• Non-trivial geometry of pure AdS encodes the kinematics and the additional deformations of AdS

encode the dynamics, including confinement

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 28

Structure of the Vacuum in Light-Front Dynamics

• Physical hadron has plane-wave and polarization indices along 3+1 physical coordinates and a profile

wavefunction Φ(z) along holographic variable z

ΦP (x, z)µ1···µJ = eiP ·xΦ(z)µ1···µJ , Φzµ2···µJ = · · · = Φµ1µ2···z = 0

with four-momentum Pµ and invariant hadronic mass PµPµ=M2

• Further simplification by using a local Lorentz frame with tangent indices

• Variation of the action gives AdS wave equation for spin-J field Φ(z)ν1···νJ = ΦJ(z)εν1···νJ[−z

d−1−2J

eϕ(z)∂z

(eϕ(z)zd−1−2J

∂z

)+(mR

z

)2]

ΦJ = M2ΦJ

with

(mR)2 = (µeff (z)R)2 − Jz ϕ′(z) + J(d− J + 1)

and the kinematical constraints

ηµνPµ ενν2···νJ = 0, ηµν εµνν3···νJ = 0.

• Kinematical constrains in the LF imply that m must be a constant

[See also: T. Gutsche, V. E. Lyubovitskij, I. Schmidt and A. Vega, Phys. Rev. D 85, 076003 (2012)]

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 29

Structure of the Vacuum in Light-Front Dynamics

Light-Front Mapping

[GdT and S. J. Brodsky, PRL 102, 081601 (2009)]

• Upon substitution ΦJ(z) ∼ z(d−1)/2−Je−ϕ(z)/2 φJ(z) and z→ζ =√x(1− x)b in AdS WE[

−zd−1−2J

eϕ(z)∂z

(eϕ(z)

zd−1−2J∂z

)+(mR

z

)2]

ΦJ(z) = M2ΦJ(z)

we find LFWE (d = 4)(− d2

dζ2− 1− 4L2

4ζ2+ U(ζ)

)φJ(ζ) = M2φJ(ζ)

withU(ζ) = 1

2ϕ′′(ζ) +

14ϕ′(ζ)2 +

2J − 32z

ϕ′(ζ)

and (mR)2 = −(2− J)2 + L2

• Unmodified AdS equations correspond to the kinetic energy terms of the partons inside a hadron

• Interaction terms in the QCD Lagrangian build the effective confining potential U(ζ) and correspond

to the truncation of AdS space in an effective dual gravity approximation

• AdS Breitenlohner-Freedman bound (mR)2 ≥ −4 equivalent to LF QM stability condition L2 ≥ 0

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 30

Structure of the Vacuum in Light-Front Dynamics

9 Meson Spectrum

• Dilaton profile in the dual gravity model determined from one-dim QFTh (dAFF)

ϕ(z) = λz2, λ2 = w/2

• Effective potential: U = λ2ζ2 + 2λ(J − 1)

• LFWE (− d2

dζ2− 1− 4L2

4ζ2+ λ2ζ2 + 2λ(J − 1)

)φJ(ζ) = M2φJ(ζ)

• Normalized eigenfunctions 〈φ|φ〉 =∫dζ φ2(z) = 1

φn,L(ζ) = |λ|(1+L)/2

√2n!

(n+L)!ζ1/2+Le−|λ|ζ

2/2LLn(|λ|ζ2)

• Eigenvalues for λ > 0 M2n,J,L = 4λ

(n+

J + L

2

)• λ < 0 incompatible with LF constituent interpretation

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 31

Structure of the Vacuum in Light-Front Dynamics

ζ

φ(ζ)

0 4 80

0.4

0.8

2-2012

8820A9 ζ

φ(ζ)

0 4 8

0

0.5

-0.5

2-2012

8820A10

LFWFs φn,L(ζ) in physical space-time: (L) orbital modes and (R) radial modes

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 32

Structure of the Vacuum in Light-Front Dynamics

• Results easily extended to light quarks masses (Ex: K-mesons)

[GdT, S. J. Brodsky and H. G.Dosch, arXiv:1405.2451 [hep-ph]]

• First order perturbation in the quark masses

∆M2 = 〈ψ|∑a

m2a/xa|ψ〉

• Holographic LFWF with quark masses

[S. J. Brodsky and GdT, arXiv:0802.0514 [hep-ph]

ψ(x, ζ) ∼√x(1− x) e−

12λ

(m2qx

+m2q

1−x

)e−

12λ ζ

2

• Ex: Description of diffractive vector meson production at HERA

[J. R. Forshaw and R. Sandapen, PRL 109, 081601 (2012)]

• For the K∗

M2n,L,S = M2

K± + 4λ(n+

J + L

2

)• Effective quark masses from reduction of higher Fock states as functionals of the valence state:

mu = md = 46 MeV, ms = 357 MeV

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 33

Structure of the Vacuum in Light-Front Dynamics

M2IGeV2MHaL n 3 n 2 n 1 n 0

ΡH1700L

ΡH1450L

ΡH770L

a2H1320L

Ρ3H1690L

a4H2040L

f2H1270L

f4H2050L

f2H2300L

f2H1950L

ΩH782L

ΩH1650L

ΩH1420L

Ω3H1670L

L0 1 2 3 4

0

1

2

3

4

5

6

L

M2IGeV2M n 2 n 1 n 0

K*H892L

K*H1410L

K*H1680L

K2*H1430L

K3*H1780L

K4*H2045L

HbL

0 1 2 3 40

1

2

3

4

5

6

Orbital and radial excitations for vector mesons for√λ = 0.54 GeV

• Linear Regge trajectories, a massless pion and relation between the ρ and a1 massMa1/Mρ =√

2usually obtained from Weinberg sum rules described by LF harmonic confinement model

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 34

Structure of the Vacuum in Light-Front Dynamics

10 Higher Half-Integer Spin Wave Equations in AdS Space

[J. Polchinski and M. J. Strassler, JHEP 0305, 012 (2003)]

[GdT and S. J. Brodsky, PRL 94, 201601 (2005)]

[GdT, H.G. Dosch and S. J. Brodsky, PRD 87, 075004 (2013)]

Image credit: N. Evans

• The gauge/gravity duality can give important insights into the strongly coupled dynamics of nucleons

using simple analytical methods: analytical exploration of systematics of light-baryon resonances

• Extension of holographic ideas to spin-12 (and higher half-integral J ) hadrons by considering wave

equations for Rarita-Schwinger spinor fields in AdS space and their mapping to light-front physics

• LF clustering decomposition of invariant variable ζ : same multiplicity of states for mesons and baryons

ζ =√

x1−x

∣∣∣∑n−1j=1 xjb⊥j

∣∣∣ (spectators vs active quark)

• But in contrast with mesons there is important degeneracy of states along a given Regge trajectory for

a given L: no spin-orbit coupling

[See also: T. Gutsche, V. E. Lyubovitskij, I. Schmidt and A. Vega, Phys. Rev. D 85, 076003 (2012)]

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 35

Structure of the Vacuum in Light-Front Dynamics

• Half-integer spin J = T + 12 conveniently represented by RS spinor [ΨN1···NT ]α with effective AdS

action

Seff = 12

∫ddx dz

√|g| gN1N ′1 · · · gNT N ′T[

ΨN1···NT

(iΓA eMA DM − µ− U(z)

)ΨN ′1···N ′T + h.c.

]where the covariant derivative DM includes the affine connection and the spin connection

• eAM is the vielbein and ΓA tangent space Dirac matrices

ΓA,ΓB

= ηAB

• LF mapping z → ζ find coupled LFWE

− d

dζψ− −

ν + 12

ζψ− − V (ζ)ψ− = Mψ+

d

dζψ+ −

ν + 12

ζψ+ − V (ζ)ψ+ = Mψ−

provided that |µR| = ν + 12 and

V (ζ) =R

ζU(ζ)

a J -independent potential – No spin-orbit coupling along a given trajectory !

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 36

Structure of the Vacuum in Light-Front Dynamics

11 Baryon Spectrum

• Choose linear potential V = λ ζ , λ > 0 to satisfy dAFF

• Eigenfunctions

ψ+(ζ) ∼ ζ12+νe−λζ

2/2Lνn(λζ2), ψ−(ζ) ∼ ζ32+νe−λζ

2/2Lν+1n (λζ2)

• Eigenvalues: M2 = 4λ(n+ν+1)

• Lowest possible state n = 0 and ν = 0: orbital excitations ν = 0, 1, 2 · · · = L

• L is the relative LF angular momentum between the active quark and spectator cluster

• ν depends on internal spin and parity

The assignment

S = 12 S = 3

2

P = + ν = L ν = L+ 12

P = - ν = L+ 12 ν = L+ 1

describes the full light baryon orbital and radial excitation spectrum

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 37

Structure of the Vacuum in Light-Front Dynamics

LL1-20148844A5

M2

(G

eV

2)

(c) (d)

n=2 n=1 n=0

n=2n=3 n=1 n=0

Δ(1950)

Δ(1920)

Δ(1700)

Δ(1620)

Δ(1910)

Δ(1905)

Δ(1232)

Δ(1600)

Δ(2420)

N(1875)

N(1535)

N(1520)

0 2 41

3

5

7

20 40

2

4

6

M2

(G

eV

2)

(a) (b)

n=2n=3 n=1 n=0

N(1710)

N(1700)

N(1720)

N(1680)

N(1675)

N(2250)

N(2600)

N(2190)

N(2220)

ν=L

ν=L+1

N(1650)

N(940)

N(1440)

N(940)

N(1900) N(2220)

N(1720)

N(1680)

0 2 40

2

4

6

0 2 4 60

4

8

Baryon orbital and radial excitations for√λ = 0.49 GeV (nucleons) and 0.51 GeV (Deltas)

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 38

Structure of the Vacuum in Light-Front Dynamics

12 Conclusions

We have described a threefold connection between

a one-dimensional QFT semiclassical approximation

to light-front QCD with gravity in a higher dimensional

AdS space, and the constraints imposed by the invariance

properties under the full conformal group in one dimension.

This provides a new insight into the physics underlying the

QCD vacuum, confinement, chiral invariance and the QCD

mass scale

4 – dim Light –

Front Dynamics

SO(2,1)

5 – dim

Classical Gravity

dAFF

1 – dim

Quantum Field Theory

AdS5

AdS2LFQM

Conf(R1)

LFD

1-20148840A1

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 39

Structure of the Vacuum in Light-Front Dynamics

Thank you !

Niccolo Cabeo 2014, Ferrara, May 20, 2012Page 40