Random Geometry meets Lilliputian strings Yuri Makeenko (ITEP, - - PowerPoint PPT Presentation

random geometry meets lilliputian strings
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Random Geometry meets Lilliputian strings Yuri Makeenko (ITEP, - - PowerPoint PPT Presentation

Random Geometry meets Lilliputian strings Yuri Makeenko (ITEP, Moscow) Based on: J. Ambjrn, Y. M. Phys. Lett. B 756, 142 (2016) [ arXiv:1601.00540 ] J. Ambjrn, Y. M. Phys. Rev. D 93, 066007 (2016) [ arXiv:1510.03390 ] Talk at the 2nd


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Random Geometry meets Lilliputian strings

Yuri Makeenko (ITEP, Moscow)

Based on:

  • J. Ambjørn, Y. M. Phys. Lett. B 756, 142 (2016) [arXiv:1601.00540]
  • J. Ambjørn, Y. M. Phys. Rev. D 93, 066007 (2016) [arXiv:1510.03390]

Talk at the 2nd French-Russian Conference “Random Geometry and Physics” Paris, October 17–21, 2016

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Content of the talk

———————————–

  • effective string philosophy

– (off-shell) Nambu-Goto versus Polyakov string – invariant cutoff Λ2√g

  • approximate solution of proper-time regularized bosonic string

(mean field that becomes exact at large d) – the Alvarez-Arvis spectrum – the Lilliputian scaling limit

  • accounting for semiclassical fluctuations about the saddle-point

– Schwinger-Dyson equations versus path integral (d → d − 2) – 1/d correction via the path integral

  • living in the Lilliputian world
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  • 1. Introduction
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Problems of string theory

———————————– inherited from 1980’s

  • Path integral reproduces canonical quantization only

in critical dimension (d=26) and on-shell

  • Otherwise a non-linear problem emerges because the world-sheet

cutoff is Λ2√g where Λ is invariant cutoff (e.g. proper time) and g = det gab (of metric tensor)

Polyakov (1981)

  • It can be solved for the (closed) Polyakov string

Knizhnik-Polyakov-Zamolodchikov (1988), David (1988), Distler-Kawai (1989)

giving the string susceptibility index which is not real for 1 < d < 25 γ = d − 1 −

  • (d − 1)(d − 25)

12

  • Lattice regularization (by dynamical triangulation) scale to

a continuum string for d ≤ 1 but does not for d > 1 (same for hypercubic latticization of Nambu-Goto string in d > 2)

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Effective-string philosophy

———————————– String is formed by more fundamental constituents Effective or induced or emergent string makes sense when it is long Examples: – Abrikosov vertices in supercondactor – Nielsen-Olesen string in the Higgs model – Confining string in QCD In particular no tachyon for L > Ltachyon Pretty much like the view on Quantum Electrodynamics

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  • 2. Saddle-point solution to

bosonic string

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Nambu-Goto string via Lagrange multiplier

———————————– Lagrange multiplier λab for independent metric tensor ρab K0

  • d2ω
  • det ∂aX · ∂bX = K0
  • d2ω √ρ+K0

2

  • d2ω λab (∂aX · ∂bX − ρab)

World-sheet parameters ω1, ω2 ∈ ωL × ωβ rectangle Closed bosonic string winding once around compactified dimension of length β, propagating (Euclidean) time L. No tachyon if β is large enough Classical solution X1

cl = L

ωL ω1, X2

cl = β

ωβ ω2, X⊥

cl = 0,

[ρab]cl = diag

 L2

ω2

L

, β2 ω2

β

 

λab

cl = diag

  • βωL

Lωβ , Lωβ βωL

  • = ρab

cl

√ρcl minimizes the Nambu-Goto action (a classical vacuum)

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SLIDE 8

Effective action

———————————– Gaussian path integral over Xµ

q by splitting Xµ = Xµ cl + Xµ q:

Seff = K0

  • d2ω √ρ + K0

2

  • d2ω λab (∂aXcl · ∂bXcl − ρab)

+d − 2 2 tr log O, O = − 1 √ρ∂aλab∂b. in the static gauge modulo the ghost determinant Proper-time regularization of the trace tr log O = −

a2

dτ τ tr e−τO, a2 ≡ 1 4πΛ2 with −O being the 2d Laplacian for λab = ρab√ρ The effective action governs λab and ρab which do not fluctuate at large d (exact mean field) like 2d O(N) sigma-model at large N. Then ghosts can be ignored Saddle-point values ¯ λab and ¯ ρab minimize the effective action

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Effective action (cont.)

———————————– The minimum is reached for diagonal and constant ¯ λab and ¯ ρab, when Seff = K0 2

 ¯

λ11L2 ω2

L

+ ¯ λ22β2 ω2

β

+ 2

  • ¯

ρ11¯ ρ22 − ¯ λ11¯ ρ11 − ¯ λ22¯ ρ22

  ωβωL

−d√¯ ρ11¯ ρ22 ωβωL 2 √¯ λ11¯ λ22 Λ2 − πd 6

  • ¯

λ22 ¯ λ11 ωL ωβ for L ≫ β The averaged induced metric ∂aX · ∂bX (that equals ¯ ρab at large d) depends on ω1 near the boundaries but this is not essential for L ≫ β

Ambjørn, Makeenko (2016)

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Side remark: a mathematical formula

———————————–

Ambjørn, Makeenko, Sedrakyan (2014)

Determinant for ω ∈ rectangle is given by the product over modes with the Dirichlet b.c. as the Dedekind η-function: det(−∆) =

  • m,n=1
  • πm2

ω2

T

+ πn2 ω2

R

  • =

1 √2ωR η

  • iωT

ωR

  • Alternatively for z ∈ upper half-plane L¨

uscher, Symanzik, Weisz (1980)

det(−∆) = 1 24π

  • d2z ∂a log
  • ∂ω(z)

∂z

  • ∂a log
  • ∂ω(z)

∂z

  • with the Schwarz–Christoffel map (0 < r < 1)

ω(z) =

z

r

ds

  • (1 − s)(s − r)s

, ωR ωT = K

√1 − r

  • K

√r

  • Gr¨
  • tzsch modulus

where K is the complete elliptic integral of the first kind. We have verified that indeed 1 2

  • K

√1 − r 1/2 η  i

K

√1 − r

  • K

√r

 =

1 25/6π1/2 [r(1 − r)]1/12

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Saddle-point solution

———————————–

Ambjørn, Makeenko (2016)

The minimum of the effective action (quantum vacuum) is given by ¯ ρ11 = L2 ω2

L

  • β2 − β2

2C

  • β2 − β2

C

  • C

2C − 1, ¯ ρ22 = 1 ω2

β

  • β2 − β2

2C

  • C

2C − 1, β2

0 = πd

3K0 ¯ λab = C¯ ρab ¯ ρ, C = 1 2 +

  • 1

4 − dΛ2 2K0 The conformal gauge ¯ ρ11 = ¯ ρ22 is realized for ωβ ωL = 1 L

  • β2 − β2

C same as classical for β ≫ β0 alternatively to fix ρ11 = ρ22 and minimize with respect to ωβ

ωL.

These generalize the classical solution, the WKB (perturbative or loop) expansion about which goes in 1/K0 ∼ , recovering one loop. C takes for K0 > 2dΛ2 values between 1 (classical) and 1/2 (quan- tum), which plays a crucial role for existence of the continuum limit

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Saddle-point solution (cont.)

———————————– Substituting the solution, we obtain the saddle-point value Seff = K0CL

  • β2 − β2

0/C

which is L times the ground state mass The average area of typical surfaces essential in the path integral Area =

  • d2ω
  • ¯

ρ11¯ ρ22 = L

  • β2 − β2

0/2C

  • β2 − β2

0/C

C (2C − 1). These results merely repeat Alvarez (1981) except he used the zeta- function regularization where formally our Λ = 0 and C = 1. We shall now see the scaling regime needs K0 → 2dΛ2 or C → 1/2

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  • 3. Two scaling regimes:

Gulliver’s vs. Lilliputian

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Lattice-like scaling limit (Gulliver’s)

———————————– The ground state energy E(β) = K0C

  • β2 − β2

0/C

does not scale generically because K0 > 2dΛ2 for C to be real (> 1/2). Let β2 > β2

min =

π 3dΛ2 for not to have a tachyon. Choosing the smallest possible value β = βmin, we find E(β) =

π

3 K0C Λ √ 2C − 1 which scales to m for C − 1 2 ∝ m2 Λ2 , K0 − 2dΛ2 ∝ m4 Λ2 This scaling does not exist for larger values of β and thus is particle-like similar to lattice regularizations of a string, where

  • nly the lowest mass scales to finite, excitations scale to infinity

Durhuus, Fr¨

  • hlich, Jonsson (1984), Ambjørn, Durhuus (1987)
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Lilliputian string-like scaling limit

———————————– Let us “renormalize” the units of length LR =

  • C

2C − 1 L, βR =

  • C

2C − 1 β, to obtain for the effective action Seff = KR LR

  • β2

R −

πd 3KR , KR = K0(2C − 1) The renormalized string tension KR scales if K0 → 2dΛ2 + K2

R

2dΛ2 reproducing the Alvarez-Arvis spectrum of continuum string The average area is also finite Area = LR

  • β2

R − πd 6KR

  • β2

R − πd 3KR

It is simply the minimal area for β2

R ≫ πd/(3KR) and diverges when

β2

R → πd/(3KR) like for the zeta-function regularization

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Lilliputian string-like scaling limit (cont. 1)

———————————– Everything is like for the zeta-function regularization, but length =

  • 2C − 1

C lengthR ∼ √2dKR lengthR Λ in target space which is of order of the cutoff (Lilliputian) Nevertheless, the cutoff (in parameter space) ∆ω = 1/(Λ 4 √g) fixes maximal number of modes in the mode expansion Xq =

  • m,n≥0
  • amn cos 2πmω2

ωβ +bmn sin 2πmω2 ωβ

  • sin πnω1

ωL , to be n(1)

max ∼ Λ 4

√gωL n(2)

max ∼ Λ 4

√gωβ Classically

4

√gωβ = β reproducing Brink-Nielsen (1973) Quantumly

4

√gωβ = β √2C − 1 = √ 2d Λβ √KR is much larger = ⇒ classical music can be played on the Lilliputian strings

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Lilliputian string-like scaling limit (cont. 2)

———————————– Why it was not observed before? The Lilliputian scaling in nonperturbative in : Semiclassically (recalling that 1/K0 ∼ ) C = 1 2 +

  • 1

4 − dΛ2 2K0 = 1 − dΛ2 2K0 + O(2) cannot approach 1/2 and thus the metric cannot become singular. The scaling regime of KR = K0(2C−1) cannot be seen semiclassically. We found a certain geometry (metric tensor) which self-consistently dominates the path integral over geometries and becomes singular as K0 → 2dΛ2 + K2

R

2dΛ2

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The Lilliputian world

———————————– Summary:

  • The Lilliputian world is of the size of the target-space cutoff
  • It is still a continuum because infinitely smaller distances can be

resolved (infinitely many stringy modes)

  • The Lilliputian scaling regime is perfectly recovered by results of

the zeta-function regularization

  • Linear Regge trajectories signalize about the Lilliputian world
  • Gulliver’s tools are too coarse to resolve the Lilliputian world

(this is why lattice string regularizations of 1980’s never reproduce canonical quantization)

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  • 4. Fluctuations about saddle point
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Schwinger-Dyson equations

———————————– Relativistic string can be quantized by the Schwinger-Dyson equations rather than a path integral Advantage: terms from ghosts and the gauge fixing mutually cancel Averages of non-invariant quantities may vanish, so we have to con- sider proper averages like

  • ρ(ω)
  • . These would coincide with those

computed with fixed gauge (e.g. conformal gauge). Invariance of the measure under a shift of ρab gives

  • λab(ω)
  • =
  • ρab(ω)
  • ρ(ω) −

d 2K0 ω| e−a2O|ω

  • + 2

K0

δ

  • ρ(ω)

δρab(ω)

  • Proper-time regularized variational derivative in the second term

δ δρab(ω) →

  • d2ω′ ω| e−a2O|ω′

δ δρab(ω′)

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Schwinger-Dyson equations (cont.)

———————————– Computing the partial derivative by using the formula ∂√ρ ∂ρab = 1 2ρab√ρ we find

  • λab(ω)
  • =
  • ρab(ω)
  • ρ(ω) − (d − 2)

2K0 ω| e−a2O|ω

  • Proven Theorem: similarly to the saddle point at large d

λab w.s. = Cρab√ρ, C = 1 2 +

  • 1

4 − (d − 2)Λ2 2K0 It is valid for any d, accounting for the fluctuations

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Coleman-Weinberg potential

———————————– Integrating out Xµ

q we get

d − 2 2 tr ln

  • − 1

√ρ∂aλab∂b

  • =
  • n

1 n

✣✢ ✤✜

· · · · · · ··· resulting in the effective action Seff = K0

  • d2ω √ρ + K0

2

  • d2ω λab (∂aXcl · ∂bXcl − ρab)

−d − 2 2 Λ2

  • d2ω

√ρ

  • det λab + finite

Expanding λab = (¯ λ + δλ)δab, ρab = (¯ ρ + δρ)δab we find (in conformal gauge) to quadratic order Seff = Ss.p.

eff − K0(2C − 1)

C

  • d2ω δλδρ − d − 2

2C3 Λ2¯ ρ

  • d2ω δλ2 + . . .

with one positive and one negative eigenvalues = ⇒ stable fluctuations because δλ is imaginary and δρ is real (in particular justifying constant ¯ λ and ¯ ρ)

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Critical dimension

———————————– Polyakov string: 26 − 1 = 25 ghosts metric dc Nambu-Goto string: 26 − 1 + 1 = 26 ghosts metric Lagrange dc multiplier The signs are opposite because the metric and the Lagrange multiplier are real and imaginary, respectively

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(In)Stability of the Liouville action

———————————– For Polyakov’s string in conformal gauge ρab = eϕδab (−∆reg)−(d−26)/2 ∝ e

(d−26) 96π

  • d2ω
  • (∂ϕ)2+µ2 eϕ

if ϕ is smooth (curvature R ≪ Λ2 is not large). Higher derivatives become essential otherwise. The expansion goes in R/Λ2. So the det may be finite in spite of the Liouville action diverges. Let ϕ is constant along ω2 and has a discontinuity from 0 to ϕ0 > 0 at certain ω1. Since the integral then diverges (opposite to Brownian trajectories), one might think this leads to an instability for d > 26. But det(−∆) for such a discontinuous ϕ is larger than one for constant ϕ = ϕ0, because all eigenvalues are larger. It cannot be zero as Liouville says. The one for constant ϕ0 is as above with ¯ λab = δab. det(−∆) for such a discontinuous ϕ can be explicitly computed using the Gel’fand-Yaglom technique and shown to be finite.

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Conformal anomaly and beyond

———————————– Pauli-Villars regularization of the Polyakov string [det(−∆)]reg = det(−∂2) det(−∂2 + M2ρ) To quadratic order, we expand ρ = ¯ ρ + δρ that generates the propa- gator of the field Xµ

M and the triple vertex:

M(k)Xν M(−k)

  • =

δab k2 + M2¯ ρ

  • δρ(−p)Xµ

M(k + p)Xν M(−p)

  • truncated = −M2δµν.

The effective action to quadratic order −d 2

  • d2p

(2π)2 δρ(p)δρ(−p) 2

  • d2k

(2π)2 M4 (k2 + M2¯ ρ)[(k + p)2 + M2¯ ρ] = − d 96π¯ ρ2

  • d2p

(2π)2

  • (paδρ)2 + O(p4/M2)
  • which coincides to quadratic order in δρ with the conformal anomaly

− d 96π

  • d2ω (∂a log ρ)2
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Conclusion

———————————–

  • Path-integral quantization reproduces canonical quantization

in d > 2 only for the Lilliputian strings

  • Gulliver’s tools (inherited from QFT) are too coarse to deal with

this scaling regime

  • It does not exist for d < 2 or fermionic strings when the sign

changes

The world of: Lilliputian strings for d > 2 Gulliver’s strings for d < 2