Math 2.0

Dynamical systems and ergodic theory Hamiltonian dynamics Theorem

Nekhoroshev estimates

Builds on Hamiltonian systemAction-angle coordinatesIntegrable system

Statement

Let n≥2n \ge 2, let D⊆ℝnD \subseteq \R^n be a bounded open set and let 𝕋n=ℝn/2πℤn\mathbb{T}^n = \R^n / 2\pi \Z^n. Use action-angle coordinates (I,θ)(I, \theta) on D×𝕋nD \times \mathbb{T}^n. Consider the Hamiltonian system with Hamiltonian Hε(I,θ)=h(I)+εf(I,θ).H_\varepsilon(I, \theta) = h(I) + \varepsilon f(I, \theta). Assume that hh and ff are real-analytic on a complex neighbourhood of D‾×𝕋n\overline{D} \times \mathbb{T}^n. Assume that hh is steep, for example strictly convex. Then there are constants a,b,C,ε0>0a, b, C, \varepsilon_0 > 0 with the following property. Let 0<ε<ε00 < \varepsilon < \varepsilon_0, and take a solution with I(0)I(0) in DD, away from the boundary of DD. Then ∣I(t)−I(0)∣≤Cεbfor∣t∣≤Cexp⁡(ε−a).\abs{I(t) - I(0)} \le C \varepsilon^b \quad \text{for} \quad \abs{t} \le C \exp\left(\varepsilon^{-a}\right).

Remarks

The proof has two parts. The analytic part builds, near each resonance, a normal form in which the angle dependence that does not belong to the resonance is exponentially small in 1/ε1/\varepsilon. The geometric part uses steepness to show that an orbit cannot move far along the directions allowed by a resonance before it leaves the resonance zone.

For strictly convex hh one can take a=b=12na = b = \frac{1}{2n}.

Unlike the KAM theorem, the estimate holds for all initial conditions, not only for most of them, but only for a finite, exponentially long time. Together with the existence of Arnold diffusion, it shows that instability can occur in nearly integrable systems but only on exponentially long time scales.

Some steepness condition is needed. For n=2n = 2, h(I)=I12−I22h(I) = I_1^2 - I_2^2, which is not steep, and f=sin⁡(θ1+θ2)f = \sin(\theta_1 + \theta_2), the equations give (θ1+θ2)′=2(I1−I2)(\theta_1 + \theta_2)' = 2(I_1 - I_2) and I1′=I2′=−εcos⁡(θ1+θ2)I_1' = I_2' = -\varepsilon \cos(\theta_1 + \theta_2). The solution with I1(0)=I2(0)I_1(0) = I_2(0) and θ1(0)+θ2(0)=0\theta_1(0) + \theta_2(0) = 0 has I1(t)=I1(0)−εtI_1(t) = I_1(0) - \varepsilon t and I2(t)=I2(0)−εtI_2(t) = I_2(0) - \varepsilon t, so the actions drift by order one in time of order 1/ε1/\varepsilon.

Going deeper

For a student

The Nekhoroshev estimates complement KAM theory. KAM gives stability forever on a large set of invariant tori, but says nothing about the orbits between them. Nekhoroshev gives stability for all orbits, over times that are exponentially long in a power of 1/ε1/\varepsilon. They are used in celestial mechanics, for example to discuss the long-time stability of asteroids near the Lagrange points.

Reading path

To understand this page from the ground up, read these 4 pages in order. The foundations come first.

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Each page uses the pages above it. The colour of the bar on a box shows how strong the evidence is, and the box also gives it as text. The list has the same pages.
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  1. Action-angle coordinates concept
  2. Hamiltonian system concept
  3. Integrable system concept
  4. Nekhoroshev estimates statement

Further reading

  1. Web https://en.wikipedia.org/wiki/Nekhoroshev_estimates
About this page
TagPYEN6SFS9P
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Kindstatement, theorem
WritingW0 stub
MSC37J40, 70H08
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AboutIntegrable system
UsesHamiltonian system, Action-angle coordinates, Integrable system
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