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Instability Stability Open Questions TTF & QP Fully Nonlinear
Revisiting Scalar Collapse in AdSNew Frontiers in Dynamical Gravity
DAMTP, Cambridge
Steve LieblingWith:
Venkat Balasubramanian (Western) Alex Buchel (Western/PI)
Stephen Green (Guelph) Luis Lehner (Perimeter)
Long Island UniversityNew York, USA
March 24, 2014
Steven L. Liebling Revisiting Scalar Collapse in AdS 1 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Instability of Scalar Field in spher. symm. aAdS
Evolution of a Scalar field in sph. symm., asympt. AdS (aAdS)[Bizon -Rostworowski,2011]
Fully nonlinear:Consider Gaussian-type initial data w/ amplitude ε and width σChoptuik-type critical behaviorHowever, sub-critical eventually collapses as well
Perturbative about pure AdS:At linear order, uncoupled modes: oscillonResonance at O(ε3): jr = j1 + j2 − j3Single mode stable, multiple modes unstable
Conjecture:AdS generically unstable to collapse via weakly nonlinearturbulent cascade
Steven L. Liebling Revisiting Scalar Collapse in AdS 2 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Instability in light of AdS/CFT Correspondence
Holographic duality between(d + 1)-dimensional global AdS (the bulk)
andconformal field theory (CFT) on d − 1-dim. boundary (Sd−1 × R)
Dictionary translates between bulk quantities of aAdS spacetimeand quantum operators of CFT
Interpretation of instability:initial data generically thermalizes by BH formation
...but are there non-thermalizing initial configurations in the CFT?
Steven L. Liebling Revisiting Scalar Collapse in AdS 3 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Paths to Stability
Perturbative analysis showing stable solutions[Dias,Horowitz,Marolf,Santos,1208.5772]
Argue perturbatively for nonlinear stabilityGeons and boson stars, not necessarily spher. symm.
Excite all modes[Buchel,Lehner,SLL,1210.0890]
Perturbative argument for stability at O(ε3)
ωjr → ωjr + ε2∑{j1,j2,j3}
Aj1Aj2
Aj3
AjrCj1j2j3jr , where the triple sum
is over all the resonance channels ωj1 + ωj2 = ωjr + ωj3
Time-periodic solutions[Maliborski,Rostworowski,1303.3186]
Construct time-periodic solutionsArgue for nonlinear stability
Frustrated resonance[Buchel,SLL,Lehner,1304.4166]
Steven L. Liebling Revisiting Scalar Collapse in AdS 4 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Frustrated Resonance
[Buchel,SLL,Lehner,1304.4166]
Broadly distrib. energy perturbs AdS & introduces dispersionDispersion competes with nonlinear sharpeningBR data: increasing σ increases distribution of energyIssues with σ-parameterization:[Maliborski,Rostworowski,1307.2875]
Large-σ ceases to be broadly distributed (us and[Abajo-Arrastia,Silva,Lopez,Mas,Serantes,1403.2632])“window” in σ shrinks for higher dims but other ID stable
Steven L. Liebling Revisiting Scalar Collapse in AdS 5 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Perturbed Boson Star
4dmdr1.mpg Perturbed BS
Steven L. Liebling Revisiting Scalar Collapse in AdS 6 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Effect of Mass [Balasubramanian,Buchel,Green,Lehner,SLL,in prep]
Motivation: explore CFT operators of different weight...mass changes decay rate of SF at boundary
Introduce mass term −µ2|φ|2No dispersion at linear order
Mass changes location of transition σcrit
−2 −1 0 1 2 3 4
µ2
0.2
0.3
0.4
0.5
0.6
0.7
0.8
σcr
it
Steven L. Liebling Revisiting Scalar Collapse in AdS 7 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Open Questions
Among others, just two here:
What’s stable and what’s unstable?...in other words, can we identify whether initial data willcollapse for any amplitude a priori?
For ID that appears unstable, can we be sure whether itextends to ε→ 0?
...using “unstable” as ID that collapses for ε→ 0 but ε 6= 0
Steven L. Liebling Revisiting Scalar Collapse in AdS 8 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Two-Time Formalism (TTF)
Dynamics characterized by two time scales:fast time t–generally t < π where π is time for a bounce offboundaryslow time τ–scale over which energy transfers among oscillons,τ ≡ ε2t
Allow mode amplitudes Aj(t) to be functions of both timesAj(t, τ)
Enforce at O(ε3) the absence of secular terms in the scalarfieldAdvantages:
Goes beyond initial transfer of energy (...to time t > 1/ε2)Conserves energyBoth direct and inverse cascades
Solve coupled, cubic, ODEs in complex mode amplitudes Aj
Resembles FPUT paradox
Steven L. Liebling Revisiting Scalar Collapse in AdS 9 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
TTF and Fermi-Pasta-Ulam-Tsingou (FPUT, 1953)
Model 1D atoms in a crystal by masses linked by springs withnonlinear termAt linear order, Fourier modes decoupleNonlinear system may not not approach equipartition, aspredicted by classical stat. mech.
...apparently still debated more than 50 years later!
For N →∞ (nonlinear string) and small energies, system issimilarly resonant
[D. Campbell’s APS 2010 talk]
Steven L. Liebling Revisiting Scalar Collapse in AdS 10 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
TTF and Fully Nonlinear...two-mode ID
Similar “evolutions”...both direct and inverse cascades
TTF convergent with increasing jmax
In ε→ 0 and jmax →∞ limits, TTF & NL should converge
Steven L. Liebling Revisiting Scalar Collapse in AdS 11 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
TTF and Quasi-Periodic (QP) Solutions
Specify Aqpj (τ) = αje
−iβjτ
Solutions branching from dominant mode jr ...two branches forjr > 0One-parameter generalizations of MR time-periodic solutionsSuch solutions balance direct and inverse transfers...no energytransfer among modes Ej = 0Approximated by exponential spectrum Ej = e−µj
Steven L. Liebling Revisiting Scalar Collapse in AdS 12 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
(Approximate) QP Solution Evolved Fully Nonlinearly
0 5 10 15 20 25 30 35 40ε2t
1.45
1.50
1.55
1.60
1.65
1.70
1.75
Log
10|Π
2(x,0
)/ε2|
lnasqj qp.mpg QP NL
Steven L. Liebling Revisiting Scalar Collapse in AdS 13 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Engineered Initial Data (ID)
Form of ID for fully nonlinear evolutions
Specify amplitudes cj of oscillons present in ID:
Π(x , 0) = 0
φ(x , 0) = Σj (cjej(x))
Examples:
Equal energy 2-mode ID: cj = δij/(3 + 2i) + δkj /(3 + 2k)
Exponential amplitude ID: cj = e−αj
Exponential energy ID: cj = e−αj/(3 + 2j)
Steven L. Liebling Revisiting Scalar Collapse in AdS 14 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Two-mode Stable SolutionsEqual-Energy Two-Mode Initial Data: Modes 0 and 1: cj = e0/3 + e1/5
0 2 4 6 8 10 12ε2t
1
2
3
4
5
6
7
8
9
10L
og10|Π
2(x,0
)/ε2|
Steven L. Liebling Revisiting Scalar Collapse in AdS 15 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Two-mode Stable SolutionsEqual-Energy Two-Mode Initial Data: Modes 0 and 1: cj = e0/3 + e1/5
0 2 4 6 8 10 12ε2t
1
2
3
4
5
6
7
8
9
10L
og10|Π
2(x,0
)/ε2|
BH FormationF
rustratedR
esonance
Steven L. Liebling Revisiting Scalar Collapse in AdS 16 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Two-mode Stable SolutionsEqual-Energy Two-Mode Initial Data: Modes 0 and 1: cj = e0/3 + e1/5
Left from: Benettin,Carati,Galgani,Giorgilli, 2008]
Steven L. Liebling Revisiting Scalar Collapse in AdS 17 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Other stable solutionsThree-Mode Initial Data: Modes 1, 3, and 8: cj = e1/10 + e3 + e8/10
0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5ε2t
4.2
4.4
4.6
4.8
5.0
5.2
5.4
Log
10|Π
2(x,0
)/ε2|
Steven L. Liebling Revisiting Scalar Collapse in AdS 18 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Other stable solutionsThree-Mode Initial Data: Modes 1, 3, and 8: cj = e1/10 + e3 + e8/10
0.0 0.1 0.2 0.3 0.4 0.5ε2t
4.2
4.4
4.6
4.8
5.0
5.2
5.4
Log
10|Π
2(x,0
)/ε2|
Steven L. Liebling Revisiting Scalar Collapse in AdS 19 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Other (possibly) stable solutionsThree-Mode Initial Data: Modes 1, 3, and 8: cj = e1 + e3 + e8
not one-mode dominant
0.00 0.05 0.10 0.15 0.20ε2t
5
6
7
8
9
10
11
12
Log
10|Π
2(x,0
)/ε2|
0.00 0.01 0.02 0.03 0.04 0.05ε2t
5
6
7
8
9
10
11
12
Log
10|Π
2(x,0
)/ε2|
Steven L. Liebling Revisiting Scalar Collapse in AdS 20 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Other (possibly) stable solutionsExponential Amplitude: cj = e−αj for α = 0.575
0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4ε2t
3
4
5
6
7
8
9
10
Log
10|Π
2(x,0
)/ε2|
Steven L. Liebling Revisiting Scalar Collapse in AdS 21 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Take-home Points
TTF formalism most useful, perturbative approach
System demonstrates both direct- and indirect cascades
Similarity to FPUT system...identical structure of equationsas TTF; resonant and nonresonant regimes
Stability regionsExistence of stable, quasi-periodic solutionsID w/ broadly distributed energy immune frustratedresonance...(regardless of deficiencies in large-σparameterization)Frustrated resonance continues to higher dimensionsFrustrated resonance extends to massive case (qualitativelysimilar)Other, not just one-mode dominant solutions...equal energy,two-mode IDPoses questions about thermalization/equilibration in CFT
Steven L. Liebling Revisiting Scalar Collapse in AdS 22 / 23
Instability Stability Open Questions TTF & QP Fully Nonlinear
Uncanny resemblance!FPUT and 2-Mode 0-1 Equal Energy FNL
Plot of energy in each mode Ej(t)
Steven L. Liebling Revisiting Scalar Collapse in AdS 23 / 23