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Transcript of Singularity Theory for Non-twist Tori · PDF fileIntroduction Introduction Alex Haro (UB)...
Singularity Theory for Non-twist Tori
A. González A. Haro R. de la Llave
Universitat de Barcelona & University of Texas at Austin
Hamiltonian Intensive Seminar IIFacultat de Matemàtiques i Estadística, UPC
December 3, 2010
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 1 / 48
Index
1 Introduction
2 Motivating examples
3 Methodology
4 Some applications
5 Interactions with Symplectic Geometry
6 Conclusions
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 2 / 48
Introduction
Introduction
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 3 / 48
Introduction
KAM TheoryExistence and persistence of quasi-periodic motions in Hamiltonian systems
Under twist conditions (' diffeomorphic frequency map):
Persistence of quasi-periodic motions (Kolmogorov, Arnold,Moser...)
A posteriori results of existence of invariant tori with fixedfrequency, based on reducibility (de la Llave, González,Jorba, Villanueva)
Existence of Cantor families of tori under weaker conditions:Unfoldings of quasi-periodic tori (Broer, Huitema, Moser,Pöschel, Sevryuk, Takens, ...)
Persistence of invariant tori under Rüssmann condition(Sevryuk, Rüssmann, Xu, You, Zhang, ...)
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 4 / 48
Introduction
Non-twist tori with fixed frequencyPrevious results
Numerical results in non-twist area preserving maps:del Castillo-Negrete, Greene, Morrison (1996, 1997):periodic orbits and transition to chaos (Apte, Wurm, Petrisor,Shinohara, Aizawa, ...)
Haro (2002): computation of non-twist tori and normal forms.
Rigorous results:Simó (1998): existence of meandering curves in areapreserving non-twist maps (but the curves are twist!).
Delshams, de la Llave (2002): existence and persistence ofnon-twist curves in 2-parameter families of apm.
Dullin, Ivanov, Meiss (2006): normal forms for the fold andcusp singularities for 4D maps.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 5 / 48
Introduction
Non-twist tori with fixed frequencyThis talk
Singularity Theory for non-twist tori(arbitrary dimension and any finite-determined singularity)
Bifurcations of invariant tori, with fixed frequency.At the bifurcation points, the invariant tori are non-twist.
Classification of the possible degeneracies of invariant tori.
Unfolding Hamiltonian systems around non-twist tori.
Persistence of non-twist invariant tori.
Efficient numerical methods to study bifurcations.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 6 / 48
Motivating examples
Motivating examples
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 7 / 48
Motivating examples
Motivation 1: Integrable systemsFrequency map of an integrable symplectomorphism
Consider the integrable system f0 : Tn × Rn → Tn × Rn,
f0(x , y) =
(x +∇W (y)
y
),
where W : Rn → R.
For p ∈ Rn, the torus Kp(θ) =
(θp
)is invariant for f0 with
frequency ω(p) = ∇W (p):
f0(Kp(θ)) = Kp(θ + ω(p)) .
Kp is twist if the torsion T (p) = Dω(p) = Hess W (p) is non-degenerate.
Observation: non-twist tori (with fixed frequency) can bedestroyed, even with integrable perturbations.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 8 / 48
Motivating examples
Motivation 1: Integrable systemsInvariant tori with frequency ω
Goal: Look for invariant tori with frequency ω.
Define the modified family
fλ(x , y) = f0(x , y) +
(λ0
).
A torus K (θ) is fλ-invariant with frequency ω if and only if:
fλ(K (θ)) = K (θ + ω) .
For p ∈ Rn, the couple (λ(p),Kp(θ)) with counterterm
λ(p) = ω −∇W (p)
satisfies the invariance equation.Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 9 / 48
Motivating examples
Motivation 1: Integrable systemsInvariant tori as critical points of the potential A
Define the potential A(p) = W (p)− p>ω.Hence:
λ(p) = −∇pA(p).T (p) = Hess A(p).
Then:
Kp∗ is an f0-invariant torus with frequency ω if and only if p∗is a critical point of the potential A(p).
Kp∗ is a twist f0-invariant torus with frequency ω if and onlyp∗ is a non-degenerate critical point of the potential A(p).
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 10 / 48
Motivating examples
Motivation 1: Integrable systemsThe simplest degenerate example
Assume A(p) =p3
3ω(y) = ω + y2.
p = 0 is a degenerate critical point of A(p).
The torus K0(θ) is non-twist.
Unfolding: A(p;µ) = µp +p3
3ω(y ;µ) = ω + µ+ y2.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 11 / 48
Motivating examples
Motivation 2: A collision of invariant toriA family of quadratic standard maps
Consider the quadratic standard family of symplectomorphismsfκ : T× R→ T× R, defined by:
x = 0.375 + x + y2 ,
y = y − κ
2πsin(2πx) .
Problem: Look for invariant tori with frequency ω = 3−√
52 , with
respect to parameter κ.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 12 / 48
Motivating examples
Motivation 2: A collision of invariant toriNumerical observations
-0.2
-0.15
-0.1
-0.05
0
0.05
0.1
0.15
0.2
0 0.2 0.4 0.6 0.8 1
y
x
K= 0.000000
-0.2
-0.15
-0.1
-0.05
0
0.05
0.1
0.15
0.2
0 0.2 0.4 0.6 0.8 1
y
x
K= 1.000000
-0.2
-0.15
-0.1
-0.05
0
0.05
0.1
0.15
0.2
0 0.2 0.4 0.6 0.8 1
y
x
K= 1.361408
-0.2
-0.15
-0.1
-0.05
0
0.05
0.1
0.15
0.2
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
y
x
K= 1.500000
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 13 / 48
Motivating examples
Questions(and partial answers)
In non-integrable cases, can we define an action whosecritical points correspond to invariant tori of a fixed ω?We construct a family of translated tori, so that the invariant toricorrespond to translated tori whose translation is zero. The translationis Moser’s counterterm.
Is there a general theory of bifurcations of KAM tori?The counterterm is a gradient function, i.e. with a potential. Hence, weuse Singularity Theory for analyzing the critical points of the potential.
Can we obtain results of persistence of non-twist tori (offixed frequency) under perturbations?Singularity Theory suggests that “finitely determined” non-twist tori arepersistent in families of a high enough number of parameters.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 14 / 48
Methodology
Methodology
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 15 / 48
Methodology
MethodologySetting
Let fκ : Tn × Rn → Tn × Rn be a smooth family of exactsymplectomorphisms, with κ ∈ P ⊂ Rm:
Dfκ(x , y)>J Dfκ(x , y) = J, where J =
(On −InIn On
);
There exists a primitive function Sκ : Tn × Rn → R, such thatdSκ = f ∗κ (y dx)− y dx .
Let ω ∈ Rn be fixed and Diophantine (ω ∈ Dn(γ, τ)):∣∣`>ω −m∣∣ ≥ γ |`|− τ1 , ∀` ∈ Zn \ 0, m ∈ Z.
Goal: Finding fκ-invariant tori, with frequency ω.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 16 / 48
Methodology
MethodologyModified family and parameter-torus deformations
1) Consider the modified family
f(κ,λ)(x , y) = fκ(x , y) +
(λ0
),
where −λ ∈ Rn is the counterterm.
2) Use KAM techniques to find a family of parameter-torus
K : D× P×Tn −→ Λ×Tn×Rn
(p, κ, θ) −→ (λ(p;κ),K(p;κ)(θ)),
such that:f(κ,λ(p;κ)) K(p;κ)(θ) = K(p;κ)(θ + ω) ,⟨
K(p;κ)(θ)− Kp(θ)⟩
= 0 .
Important: The nondegeneracy condition is very mild.Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 17 / 48
Methodology
MethodologyPotential and countertem
3) Define the potential
A(p;κ) = −p>λ(p;κ)−⟨
Sκ K(p;κ)
(θ)⟩,
where Sκ is the primitive function of fκ.
The following holds:
λ(p;κ) = −∇pA(p;κ)
Hence, fixed κ = κ∗:
K(p∗;κ∗)
is fκ∗-invariant with frequency ω if and only if p∗ is acritical point of the potential A(p;κ∗).
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 18 / 48
Methodology
MethodologyPotential and torsion
4) The torsion of K(p;κ)
is the n × n symmetric matrix
T (p;κ) =⟨
N(p;κ)
(θ + ω)> J Dzf(κ,λ(p;κ))(K(p;κ)(θ)) N
(p;κ)(θ)⟩,
where N(p;κ)
(θ) = J DθK(p;κ)(θ)(
DθK(p;κ)(θ)>DθK(p;κ)
(θ))−1
.
There exist n × n matrices W1(p;κ) and W2(p;κ) such that:
T (p;κ) W1(p;κ) = W2(p;κ) HessA(p;κ) .
Hence, if W1(p∗;κ∗) and W2(p∗;κ∗) are invertible:
The co-rank of p∗ as a critical point of A(p;κ∗) equals theco-rank of the torsion T (p∗;κ∗).
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 19 / 48
Some applications
Some applications
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 20 / 48
Some applications
Example 1: A persistence resultHypotheses
Theorem (Persistence theorem of non-twist tori)Given:
ω ∈ Rn, a Diophantine frequency vector.f0, a real-analytic integrable simplectic map with frequencymap ω(y) = ω +∇A(y), s.t. y∗ = 0 is a finitely determinedsingularity of A(y).fµ, a µ-family of real-analytic integrable simplectic map withfrequency map ωµ(y) = ω +∇Aµ(y), s.t. Aµ(y) is a stableunfolding of the singularity at zero.fµ,ε, a perturbed family of exact symplectomorphims:
fµ,ε(x , y) =
(x + ω +∇Aµ(y)
y
)+ εg(x , y , ε).
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 21 / 48
Some applications
Example 1: A persistence resultTheses
Theorem (Theses)Then:
(KAM) For (µ, ε) sufficiently small, there exists a potentialAµ,ε(p) defined around 0 ∈ Rn and an n-dimensional torusKp,µ,ε : Tn → Tn × Rn, depending smoothly on (p, µ, ε), suchthat:
fµ,ε Kp,µ,ε(θ) = Kp,µ,ε(θ + ω) +
(∇pAµ,ε(p)
0
).
(ST) For ε sufficiently small, there exist µ(ε) and p(ε) suchthat Aµ(ε),ε has a singularity at p(ε) that is of the same type(in the sense of Singularity Theory) of the singularity of A0
at zero.Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 22 / 48
Some applications
Example 1: A persistence resultSketch of proof
f (x , y) =
(x + ω +∇A(y)
y
)Unfold the singularity
yfµ(x , y) =
(x + ω +∇Aµ(y)
y
)Perturb
yfµ,ε(x , y) =
(x + ω +∇Aµ(y)
y
)+ εg(x , y , ε).
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 23 / 48
Some applications
Example 1: A persistence resultSketch of proof
1 For each p, Kp,µ,0 = Kp is an approximate translated torusfor fµ,ε with translation −λµ(p) = ∇Aµ(p):
fµ,ε(Kp(θ)) = Kp(θ + ω)−(λµ(p)
0
)+ εg(Kp(θ), ε).
2 Apply the methodology to construct a family of couples
(λµ,ε(p),Kp,µ,ε), invariant under fµ,ε +
(λ0
), parameterized by
the moment:⟨K y
p,µ,ε⟩
= p.3 Use symplectic geometry to define the potential Aµ,ε(p).4 Apply Singularity Theory to obtain perturbed degenerate
tori.Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 24 / 48
Some applications
Example 2: A collision of toriApplying the methodology
Modified family:
f(κ,λ)(x , y) =
(0.375 + x +
(y − κ
2π sin(2πx))2
+ λy − κ
2π sin(2πx)
).
The primitive function of fκ,λ is
Sκ(x , y) =κ
4 π2 cos(2πx) +23
(y − κ
2πsin(2πx)
)3.
The co-rank of the torsion of a torus is either 0 (twist) or 1(non-twist).
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 25 / 48
Some applications
A fold singularityA collision of invariant tori
-0.2
-0.15
-0.1
-0.05
0
0.05
0.1
0.15
0.2
0 0.2 0.4 0.6 0.8 1
y
x
K= 0.000000
T = 0.1669253T = −0.1669253
-0.005
0
0.005
0.01
-0.1 -0.05 0 0.05 0.1p
-0.0004
-0.0002
0
0.0002
0.0004
-0.1 -0.05 0 0.05 0.1
A
p
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 26 / 48
Some applications
A fold singularityA collision of invariant tori
-0.2
-0.15
-0.1
-0.05
0
0.05
0.1
0.15
0.2
0 0.2 0.4 0.6 0.8 1
y
x
K= 1.000000
T = 0.1123464T = −0.1123464
-0.005
0
0.005
0.01
-0.1 -0.05 0 0.05 0.1p
-0.0004
-0.0002
0
0.0002
0.0004
-0.1 -0.05 0 0.05 0.1
A
p
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 27 / 48
Some applications
A fold singularityA collision of invariant tori
-0.2
-0.15
-0.1
-0.05
0
0.05
0.1
0.15
0.2
0 0.2 0.4 0.6 0.8 1
y
x
K= 1.361408
T = 0.6558 · 10−8
T = −0.6558 · 10−8
-0.005
0
0.005
0.01
-0.1 -0.05 0 0.05 0.1p
-0.0004
-0.0002
0
0.0002
0.0004
-0.1 -0.05 0 0.05 0.1
A
p
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 28 / 48
Some applications
A fold singularityA collision of invariant tori
-0.2
-0.15
-0.1
-0.05
0
0.05
0.1
0.15
0.2
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
y
x
K= 1.500000
-0.005
0
0.005
0.01
-0.1 -0.05 0 0.05 0.1p
-0.0004
-0.0002
0
0.0002
0.0004
-0.1 -0.05 0 0.05 0.1
A
p
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 29 / 48
Some applications
Example 3: The birth of meandering toriAnother family of quadratic standard maps
Consider a quadratic standard family of symplectomorphismsfκ : T× R→ T× R, defined by:
x = x + (y + 0.1)(y − 0.2) ,
y = y − κ
2πsin(2πx) .
Problem: Look for invariant tori with frequency ω =√
5−132 , with
respect to parameter κ.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 30 / 48
Some applications
A fold singularityThe birth of meandering tori
-0.4
-0.3
-0.2
-0.1
0
0.1
0.2
0.3
0.4
0.5
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
y
x
K= 0.420000
-0.02
-0.01
0.00
0.01
0 0.02 0.04 0.06 0.08 0.1p
-0.0022
-0.0020
-0.0018
-0.0016
0 0.02 0.04 0.06 0.08 0.1
A
p
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 31 / 48
Some applications
A fold singularityThe birth of meandering tori
-0.4
-0.3
-0.2
-0.1
0
0.1
0.2
0.3
0.4
0.5
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
y
x
K= 0.430396
T = −1.6261 · 10−7
T = 1.6261 · 10−7
-0.02
-0.01
0.00
0.01
0 0.02 0.04 0.06 0.08 0.1p
-0.0022
-0.0020
-0.0018
-0.0016
0 0.02 0.04 0.06 0.08 0.1
A
p
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 32 / 48
Some applications
A fold singularityThe birth of meandering tori
-0.4
-0.3
-0.2
-0.1
0
0.1
0.2
0.3
0.4
0.5
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
y
x
K= 0.440000
T = −0.0211805T = 0.0211805
-0.02
-0.01
0.00
0.01
0 0.02 0.04 0.06 0.08 0.1p
-0.0022
-0.0020
-0.0018
-0.0016
0 0.02 0.04 0.06 0.08 0.1
A
p
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 33 / 48
Some applications
A fold singularityThe birth of meandering tori
-0.4
-0.3
-0.2
-0.1
0
0.1
0.2
0.3
0.4
0.5
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
y
x
K= 0.450000
T = −0.0309003T = 0.0309003
-0.02
-0.01
0.00
0.01
0 0.02 0.04 0.06 0.08 0.1p
-0.0022
-0.0020
-0.0018
-0.0016
0 0.02 0.04 0.06 0.08 0.1
A
p
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 34 / 48
Interactions with Symplectic Geometry
Interactions withSymplectic Geometry
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 35 / 48
Interactions with Symplectic Geometry
Compatible triple in an annulusDefinition and matrix representation
A ⊂ Tn × Rn is an annulus, endowed with a compatible tiple
(ω = dα,J,g) .
The matrix representation of the compatible triple is
(Ω(z) = Da(z)> − Da(z), J(z),G(z)) ,
where a : A → Rn, that satisfy the relations
Ω> = −Ω, J2 = −I2n, G> = G,
Ω = J>ΩJ = GJ = −J>G, G = J>GJ = −ΩJ = J>Ω .
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 36 / 48
Interactions with Symplectic Geometry
Geometric properties ofinvariant Lagrangian toriAutomatic reducibility
Setting: A is an annulus with a compatible triple (ω= dα,J,g),and A0 ⊂ A is another annulus.
Lemma (Automatic reducibility)Let f : A0 → A be a (homotopic to the identity)symplectomorphism: f ∗ω = ω.Let K : Tn → A0 be a (homotopic to the zero-section) torus.Assume that K is f -invariant and that the dynamics is theergodic rotation Rω(θ) = θ + ω: f K = K Rω.Then, the following hold:
a) f is exact symplectic: f ∗α−α = dS.b) K is Lagrangian: K ∗ω = 0.
HermanAlex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 37 / 48
Interactions with Symplectic Geometry
Lemma (cont.)
c) Define LK ,NK : Tn → R2n×n and MK : Tn → R2n×2n by
MK (θ) = (DθK (θ)︸ ︷︷ ︸LK (θ)
J(K (θ)) DθK (θ) GK (θ)−1︸ ︷︷ ︸NK (θ)
) ,
where GK (θ) = LK (θ)>G(K (θ))LK (θ). Then, the vectorbundle morphism induced by MK :
MK : Tn × R2n −→ TKA0
(θ, ξ) −→ (K (θ),MK (θ)ξ)
is an isomorphism such that M∗Kω = ω0.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 38 / 48
Interactions with Symplectic Geometry
Lemma (cont.)d) The linearized dynamics Dz f K reduces to block-triangular:
MK (θ + ω)−1Dz f (K (θ))MK (θ) =
(In T
(f ,K )(θ)
On In
),
where T(f ,K )
is the symmetric n×n matrix defined by
T(f ,K )
(θ) = NK (θ + ω)> Ω(K (θ + ω)) Dz f (K (θ)) NK (θ) .
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 39 / 48
Interactions with Symplectic Geometry
Geometric properties ofinvariant fibered Lagrangian deformationsHamiltonian deformations
DefinitionLet Λ ⊂ Rs be open. A Hamiltonian deformation with base Λ is asmooth function g : Λ×A0 → A inducing a family of exactsymplectomorphisms:
g : Λ −→ Sympe(A0,A)λ −→ gλ.
A primitive function of g is a smooth function S : Λ×A0 → Asuch that g∗λα−α = Sλ.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 40 / 48
Interactions with Symplectic Geometry
Geometric properties ofinvariant fibered Lagrangian deformationsMoment map of a Hamiltonian deformation
The generator of g is G : Λ×A0 → R2n×s defined by
G(λ, z) = Dλg(λ,g−1λ (z)).
The moment map of g is G : Λ×A0 → Rs defined by
G(λ, z)> = a(z)>G(λ, z)− DλS(λ,g−1λ (z)).
The potential of g is V : Λ×A0 → R defined by
V (λ, z) = −G(λ, z)>λ− S(λ,g−1λ (z)).
Important: G(λ, z) = Ω(z)−1DzG(λ, z)>.Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 41 / 48
Interactions with Symplectic Geometry
Geometric properties ofinvariant fibered Lagrangian deformationsExistence of a potential
DefinitionLet D,Λ ⊂ Rs be open.
i) A fibered Lagrangian deformation (FLD) is a smooth map
K = (λ,K ) : D×Tn −→ Λ×A0
(p, θ) −→ (λ(p),Kp(θ)),
such that, for each p ∈ D, Kp ∈ Lag(Tn,A0).ii) The FLD K = (λ,K ) is g-invariant with frequency ω if for any
p ∈ D, gλ(p) Kp − Kp Rω = 0.iii) The FLD K = (λ,K ) is parameterized by the momentum
parameter p if G(p) := 〈G(λ(p),Kp(θ))〉 = p.Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 42 / 48
Interactions with Symplectic Geometry
Theorem (The potential of a FLD)Let g : Λ×A0 → A be a Hamiltonian deformation.Let K = (λ,K ) : D×Tn → Λ×A0 be a g-invariant FLD, withfrequency ω ∈ Dn(γ, τ), with momentum parameter p.Define V : D → R as V (p) = 〈V (λ(p),Kp(θ))〉.Then, the following holds:
λ(p) = −∇pV (p).
T (p) Dpc(p) = W (p) Hessp V (p),
where:T (p) =
⟨T(gλ(p),Kp)(θ)
⟩is the torsion of Kp w.r.t. gλ(p);
c(p) =⟨a(Kp(θ))>DθKp(θ)
⟩> is the averaged action of Kp;
W (p) = 〈DzG(λ(p),Kp(θ)) (Np(θ)− Lp(θ)RωTp(θ)) 〉>, withRωTp(θ)−RωTp(θ+ω) = Tp(θ)−〈Tp(θ)〉 and 〈RωTp(θ)〉 = 0.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 43 / 48
Conclusions
Conclusions
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 44 / 48
Conclusions
Conclusions
The infinite dimensional problem of finding invariant tori forHamiltonian systems is reduced to the finite dimensionalproblem of finding critical points of the potential.
Non-twist tori correspond to degenerate critical points of thepotential.
The Singularity Theory for invariant tori is provided by theSingularity Theory of the critical points of the potential.
There is an analogous theory for Hamiltonian vector fields.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 45 / 48
Conclusions
Conclusions
The method yields very efficient numerical algorithms tocompute invariant tori and its bifurcations.
The method is suitable to validate numerical computations.
We are able to study any finite-determined singularity of thefrequency map.
The method can be also applied for obtaining small twisttheorems.
Our method is designed for the cases on which numericalevidence of bifurcations is known but the system is notclose to integrable.
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 46 / 48
A road map
Symplectic deformations and moment maps Reducibility of invariant tori
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Approx. reducibility of approx. invariant tori
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Potential for invariant fibered Lagrangian deformations ?
Parametric KAM Theorem
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Existence of invariant fibered Lagrangian deformations
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Singularity Theory for invariant tori
??Persistence of invariant tori forclose-to-integrable systems
Non-twist tori forclose-to-integrable systems
Numerical methods forinvariant tori bifurcations
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Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 47 / 48
Thanks!
Alex Haro (UB) Singularity Theory for Non-twist Tori UPC 2010 48 / 48