Lyapunov Exponents
The Finite Time Lyapunov Spectrum (FTLS) for a 2D billiard system consists of a set of 4 numbers $\lambda_i \, , \{ i = 1, ...,4 \}$ that characterize how fast the separation of initially close initial conditions grows.
It can be shown theoretically that two of these exponents must be zero ($\lambda_2$ =$\lambda_3$ = 0) and the other two are paired in such a way that they sum up to zero, i.e. $\lambda_1 = -\lambda_4$).
The function provided to calculate the FTLS is
DynamicalBilliards.lyapunovspectrum
— Functionlyapunovspectrum([p::AbstractParticle,] bd::Billiard, t)
Returns the finite time lyapunov exponents (averaged over time t
) for a given particle in a billiard table using the method outlined in [1]. t
can be either Float
or Int
, meaning total time or total amount of collisions.
Returns zeros for pinned particles.
If a particle is not given, a random one is picked through randominside
. See parallelize
for a parallelized version.
[1] : Ch. Dellago et al, Phys. Rev. E 53 (1996)
Here its basic use is illustrated
using DynamicalBilliards
radius = 1.0
l = 2.0
bd = Billiard(billiard_polygon(6, l; setting = "periodic")..., Disk([0., 0.], radius))
par = randominside(bd)
t = 1000.0
exps = lyapunovspectrum(par, bd, t)
4-element Vector{Float64}:
0.64789569519552
0.0015805439766546864
-2.16017524882894e-5
-0.6494546374196865
In the following example we compute the change of $\lambda_1\$ versus the distance between the disks in a hexagonal periodic billiard.
using DynamicalBilliards, CairoMakie
t = 5000.0
radius = 1.0
spaces = 2.0:0.1:4.4 #Distances between adjacent disks
lyap_time = zero(spaces) #Array where the exponents will be stored
for (i, space) in enumerate(spaces)
bd = billiard_polygon(6, space/(sqrt(3)); setting = "periodic")
disc = Disk([0., 0.], radius)
billiard = Billiard(bd.obstacles..., disc)
p = randominside(billiard)
lyap_time[i] = lyapunovspectrum(p, billiard, t)[1]
end
fig = Figure(); ax = Axis(fig[1,1]; xlabel = L"w", ylabel = L"\lambda_1")
lines!(ax,spaces, lyap_time)
fig
The plot of the maximum exponent can be compared with the results reported by Gaspard et. al (see figure 7), showing that using just t = 5000.0
is already enough of a statistical averaging.
Perturbation Growth
To be able to inspect the dynamics of perturbation growth in more detail, we also provide the following function:
DynamicalBilliards.perturbationgrowth
— Functionperturbationgrowth([p,] bd, t) -> ts, Rs, is
Calculate the evolution of the perturbation vector Δ
along the trajectory of p
in bd
for total time t
. Δ
is initialised as [1,1,1,1]
.
If a particle is not given, a random one is picked through randominside
. Returns empty lists for pinned particles.
Description
This function safely computes the time evolution of a perturbation vector using the linearized dynamics of the system, as outlined by [1]. Because the dynamics are linear, we can safely re-normalize the perturbation vector after every collision (otherwise the perturbations grow to infinity).
Immediately before and after every collison, this function computes
- the current time.
- the element-wise ratio of Δ with its previous value
- the obstacle index of the current obstacle
and returns these in three vectors ts, Rs, is
.
To obtain the actual evolution of the perturbation vector you can use the function perturbationevolution(Rs)
which simply does
Δ = Vector{SVector{4,Float64}}(undef, length(R))
Δ[1] = R[1]
for i in 2:length(R)
Δ[i] = R[i] .* Δ[i-1]
end
[1] : Ch. Dellago et al, Phys. Rev. E 53 (1996)
For example, lets plot the evolution of the perturbation growth using different colors for collisions with walls and disks in the Sinai billiard:
using DynamicalBilliards, CairoMakie, LinearAlgebra
bd = billiard_sinai()
ts, Rs, is = perturbationgrowth(Particle(0.1, 0.1, 0.1), bd, 10.0)
Δ = perturbationevolution(Rs)
fig = Figure()
ax = Axis(fig[1,1]; xlabel = L"t", ylabel = L"\log(||\Delta ||)")
lines!(ts, log.(norm.(Δ)))
scatter!(ts, log.(norm.(Δ)); color = [j == 1 ? :black : :red for j in is])
fig