Mixed Symbolic/Numerical Methods for Perturbation Theory - Differential Equations


In the previous tutorial, Mixed Symbolic/Numerical Methods for Perturbation Theory - Algebraic Equations, we discussed how to solve algebraic equations using Symbolics.jl. Here, our goal is to extend the method to differential equations. First, we import the following helper functions that were introduced in Mixed Symbolic/Numerical Methods for Perturbation Theory - Algebraic Equations.

using Symbolics, SymbolicUtils

def_taylor(x, ps) = sum([a*x^i for (i,a) in enumerate(ps)])
def_taylor(x, ps, p₀) = p₀ + def_taylor(x, ps)

function collect_powers(eq, x, ns; max_power=100)
    eq = substitute(expand(eq), Dict(x^j => 0 for j=last(ns)+1:max_power))

    eqs = []
    for i in ns
        powers = Dict(x^j => (i==j ? 1 : 0) for j=1:last(ns))
        push!(eqs, substitute(eq, powers))

function solve_coef(eqs, ps)
    vals = Dict()

    for i = 1:length(ps)
        eq = substitute(eqs[i], vals)
        vals[ps[i]] = Symbolics.solve_for(eq ~ 0, ps[i])
solve_coef (generic function with 1 method)

The Trajectory of a Ball!

In the first two examples, we applied the perturbation method to algebraic problems. However, the main power of the perturbation method is to solve differential equations (usually ODEs, but also occasionally PDEs). Surprisingly, the main procedure developed to solve algebraic problems works well for differential equations. In fact, we will use the same two helper functions, collect_powers and solve_coef. The main difference is in the way we expand the dependent variables. For algebraic problems, the coefficients of $\epsilon$ are constants; whereas, for differential equations, they are functions of the dependent variable (usually time).

As the first ODE example, we have chosen a simple and well-behaved problem, which is a variation of a standard first-year physics problem: what is the trajectory of an object (say, a ball or a rocket) thrown vertically at velocity $v$ from the surface of a planet? Assuming a constant acceleration of gravity, $g$, every burgeoning physicist knows the answer: $x(t) = x(0) + vt - \frac{1}{2}gt^2$. However, what happens if $g$ is not constant? Specifically, $g$ is inversely proportional to the distant from the center of the planet. If $v$ is large and the projectile travels a large fraction of the radius of the planet, the assumption of constant gravity does not hold anymore. However, unless $v$ is large compared to the escape velocity, the correction is usually small. After simplifications and change of variables to dimensionless, the problem becomes


\ddot{x}(t) = -\frac{1}{(1 + \epsilon x(t))^2} \,, $

with the initial conditions $x(0) = 0$, and $\dot{x}(0) = 1$. Note that for $\epsilon = 0$, this equation transforms back to the standard one. Let's start with defining the variables

n = 2
@variables ϵ t y[0:n](t) ∂∂y[0:n]
4-element Vector{Any}:
  Symbolics.Num[y₀(t), y₁(t), y₂(t)]
  Symbolics.Num[∂∂y₀, ∂∂y₁, ∂∂y₂]

Next, we define $x$.

x = def_taylor(ϵ, y[2:end], y[1])
y₀(t) + ϵ*y₁(t) + y₂(t)*(ϵ^2)

We need the second derivative of x. It may seem that we can do this using Differential(t); however, this operation needs to wait for a few steps because we need to manipulate the differentials as separate variables. Instead, we define dummy variables ∂∂y as the placeholder for the second derivatives and define

∂∂x = def_taylor(ϵ, ∂∂y[2:end], ∂∂y[1])
∂∂y₀ + ϵ*∂∂y₁ + ∂∂y₂*(ϵ^2)

as the second derivative of x. After rearrangement, our governing equation is $\ddot{x}(t)(1 + \epsilon x(t))^{-2} + 1 = 0$, or

eq = ∂∂x * (1 + ϵ*x)^2 + 1
1 + (∂∂y₀ + ϵ*∂∂y₁ + ∂∂y₂*(ϵ^2))*((1 + ϵ*(y₀(t) + ϵ*y₁(t) + y₂(t)*(ϵ^2)))^2

The next two steps are the same as the ones for algebraic equations (note that we pass 0:n to collect_powers because the zeroth order term is needed here)

eqs = collect_powers(eq, ϵ, 0:n)
3-element Vector{Any}:
                                                     1 + ∂∂y₀
                                1 + ∂∂y₀ + ∂∂y₁ + 2∂∂y₀*y₀(t)
 1 + ∂∂y₀ + ∂∂y₂ + ∂∂y₀*(y₀(t)^2) + 2∂∂y₀*y₁(t) + 2∂∂y₁*y₀(t)


vals = solve_coef(eqs, ∂∂y)
Dict{Any, Any} with 3 entries:
  ∂∂y₁ => 2.0y₀(t)
  ∂∂y₂ => 2.0y₁(t) - (3.0(y₀(t)^2))
  ∂∂y₀ => -1.0

Our system of ODEs is forming. Now is the time to convert ∂∂s to the correct Symbolics.jl form by substitution:

D = Differential(t)
subs = Dict(∂∂y[i] => D(D(y[i])) for i in eachindex(y))
eqs = [substitute(first(v), subs) ~ substitute(last(v), subs) for v in vals]
3-element Vector{Symbolics.Equation}:
 Differential(t)(Differential(t)(y₁(t))) ~ 2.0y₀(t)
 Differential(t)(Differential(t)(y₂(t))) ~ 2.0y₁(t) - (3.0(y₀(t)^2))
 Differential(t)(Differential(t)(y₀(t))) ~ -1.0

We are nearly there! From this point on, the rest is standard ODE solving procedures. Potentially we can use a symbolic ODE solver to find a closed form solution to this problem. However, Symbolics.jl currently does not support this functionality. Instead, we solve the problem numerically. We form an ODESystem, lower the order (convert second derivatives to first), generate an ODEProblem (after passing the correct initial conditions), and, finally, solve it.

using ModelingToolkit, DifferentialEquations

sys = ODESystem(eqs, t)
sys = ode_order_lowering(sys)
6-element Vector{Any}:
# the initial conditions
# everything is zero except the initial velocity
u0 = zeros(2n+2)
u0[3] = 1.0   # y₀ˍt

prob = ODEProblem(sys, u0, (0, 3.0))
sol = solve(prob; dtmax=0.01)
retcode: Success
Interpolation: automatic order switching interpolation
t: 302-element Vector{Float64}:
u: 302-element Vector{Vector{Float64}}:
 [0.0, 0.0, 1.0, 0.0, 0.0, 0.0]
 [9.976696651635089e-7, -9.96091672587352e-10, 0.9990009994995016, 3.322518
3183212947e-10, -2.488196097577267e-13, 0.0009985014994983792]
 [0.00012031590433746151, -1.313675024660254e-6, 0.9890109944945178, 4.4112
24493041101e-7, -3.6163136458534604e-9, 0.010928626384482389]
 [0.00043745619814322776, -9.069307488622044e-6, 0.9790109944945178, 3.0659
81129291793e-6, -4.777432914805544e-8, 0.02076873632942756]
 [0.0009503986908478969, -2.891919290301644e-5, 0.9690109944945178, 9.84292
0408498354e-6, -2.253405719858556e-7, 0.030508846274372736]
 [0.0016571433824514696, -6.62992778592017e-5, 0.9590109944945178, 2.271996
227591275e-5, -6.846158733026939e-7, 0.04014895621931791]
 [0.0025556902729539453, -0.0001264323265297471, 0.9490109944945178, 4.3625
12872052407e-5, -1.6271927847283168e-6, 0.04968906616426308]
 [0.0036440393623553254, -0.0002143301206684335, 0.9390109944945177, 7.4466
44173132131e-5, -3.3058347541908906e-6, 0.05912917610920825]
 [0.004920190650655609, -0.0003347956596102526, 0.9290109944945177, 0.00011
713192329729352, -6.022377301729108e-6, 0.06846928605415342]
 [0.006382144137854795, -0.0004924253602714071, 0.9190109944945177, 0.00017
348959540742975, -1.0125651195304294e-5, 0.0777093959990986]
 [0.22471192394104525, 2.8247253103418704, -1.9209890055054843, 2.240961476
3951557, 1.8060647625748494, -1.3450993796364734]
 [0.1976175041144319, 2.814507114834879, -1.9309890055054844, 2.24307344453
3601, 1.8342621940922712, -1.3643592696915283]
 [0.17013688648671746, 2.8027476697776446, -1.9409890055054844, 2.244912539
151441, 1.8623497674202474, -1.3837191597465832]
 [0.14226807105790193, 2.789410746307444, -1.9509890055054844, 2.2464748882
70665, 1.8903118892738933, -1.403179049801638]
 [0.11400905782798529, 2.7744596885439723, -1.9609890055054844, 2.247756599
913262, 1.9181326019464422, -1.422738939856693]
 [0.08535784679696758, 2.757857411389343, -1.9709890055054844, 2.2487537621
01221, 1.94579557902807, -1.4423988299117478]
 [0.05631243796484875, 2.7395663983280887, -1.9809890055054844, 2.249462442
856531, 1.9732841211027194, -1.4621587199668027]
 [0.026870831331628833, 2.7195486992271602, -1.9909890055054844, 2.24987869
0201181, 2.000581151422923, -1.4820186100218575]
 [-6.521976042861373e-14, 2.6999999999999384, -2.0000000000000218, 2.249999
999999993, 2.024999999999945, -1.5000000000000422]

Finally, we calculate the solution to the problem as a function of ϵ by substituting the solution to the ODE system back into the defining equation for x. Note that 𝜀 is a number, compared to ϵ, which is a symbolic variable.

X = 𝜀 -> sum([𝜀^(i-1) * sol[y[i]] for i in eachindex(y)])
#16 (generic function with 1 method)

Using X, we can plot the trajectory for a range of $𝜀$s.

using Plots

plot(sol.t, hcat([X(𝜀) for 𝜀 = 0.0:0.1:0.5]...))

As expected, as 𝜀 becomes larger (meaning the gravity is less with altitude), the object goes higher and stays up for a longer duration. Of course, we could have solved the problem directly using as ODE solver. One of the benefits of the perturbation method is that we need to run the ODE solver only once and then can just calculate the answer for different values of 𝜀; whereas, if we had used the direct method, we would need to run the solver once for each value of 𝜀.

A Weakly Nonlinear Oscillator

For the next example, we have chosen a simple example from a very important class of problems, the nonlinear oscillators. As we will see, perturbation theory has difficulty providing a good solution to this problem, but the process is instructive. This example closely follows the chapter 7.6 of Nonlinear Dynamics and Chaos by Steven Strogatz.

The goal is to solve $\ddot{x} + 2\epsilon\dot{x} + x = 0$, where the dot signifies time-derivatives and the initial conditions are $x(0) = 0$ and $\dot{x}(0) = 1$. If $\epsilon = 0$, the problem reduces to the simple linear harmonic oscillator with the exact solution $x(t) = \sin(t)$. We follow the same steps as the previous example.

n = 2
@variables ϵ t y[0:n](t) ∂y[0:n] ∂∂y[0:n]
x = def_taylor(ϵ, y[2:end], y[1])
∂x = def_taylor(ϵ, ∂y[2:end], ∂y[1])
∂∂x = def_taylor(ϵ, ∂∂y[2:end], ∂∂y[1])
∂∂y₀ + ϵ*∂∂y₁ + ∂∂y₂*(ϵ^2)

This time we also need the first derivative terms. Continuing,

eq = ∂∂x + 2*ϵ*∂x + x
eqs = collect_powers(eq, ϵ, 0:n)
vals = solve_coef(eqs, ∂∂y)
Dict{Any, Any} with 3 entries:
  ∂∂y₁ => -2.0∂y₀ - y₁(t)
  ∂∂y₂ => -2.0∂y₁ - y₂(t)
  ∂∂y₀ => -y₀(t)

Next, we need to replace s and ∂∂s with their Symbolics.jl counterparts:

D = Differential(t)
subs1 = Dict(∂y[i] => D(y[i]) for i in eachindex(y))
subs2 = Dict(∂∂y[i] => D(D(y[i])) for i in eachindex(y))
subs = subs1 ∪ subs2
eqs = [substitute(first(v), subs) ~ substitute(last(v), subs) for v in vals]
3-element Vector{Symbolics.Equation}:
 Differential(t)(Differential(t)(y₁(t))) ~ -y₁(t) - (2.0Differential(t)(y₀(
 Differential(t)(Differential(t)(y₂(t))) ~ -y₂(t) - (2.0Differential(t)(y₁(
 Differential(t)(Differential(t)(y₀(t))) ~ -y₀(t)

We continue with converting 'eqs' to an ODEProblem, solving it, and finally plot the results against the exact solution to the original problem, which is $x(t, \epsilon) = (1 - \epsilon)^{-1/2} e^{-\epsilon t} \sin((1- \epsilon^2)^{1/2}t)$,

sys = ODESystem(eqs, t)
sys = ode_order_lowering(sys)
Model ##ODESystem#8559 with 6 equations
States (6):
Parameters (0):
# the initial conditions
u0 = zeros(2n+2)
u0[3] = 1.0   # y₀ˍt

prob = ODEProblem(sys, u0, (0, 50.0))
sol = solve(prob; dtmax=0.01)

X = 𝜀 -> sum([𝜀^(i-1) * sol[y[i]] for i in eachindex(y)])
T = sol.t
Y = 𝜀 -> exp.(-𝜀*T) .* sin.(sqrt(1 - 𝜀^2)*T) / sqrt(1 - 𝜀^2)    # exact solution

plot(sol.t, [Y(0.1), X(0.1)])

The figure is similar to Figure 7.6.2 in Nonlinear Dynamics and Chaos. The two curves fit well for the first couple of cycles, but then the perturbation method curve diverges from the true solution. The main reason is that the problem has two or more time-scales that introduce secular terms in the solution. One solution is to explicitly account for the two time scales and use an analytic method called two-timing.


These tutorials are a part of the SciMLTutorials.jl repository, found at: https://github.com/SciML/SciMLTutorials.jl. For more information on high-performance scientific machine learning, check out the SciML Open Source Software Organization https://sciml.ai.

To locally run this tutorial, do the following commands:

using SciMLTutorials

Computer Information:

Julia Version 1.6.2
Commit 1b93d53fc4 (2021-07-14 15:36 UTC)
Platform Info:
  OS: Linux (x86_64-pc-linux-gnu)
  CPU: AMD EPYC 7502 32-Core Processor
  LIBM: libopenlibm
  LLVM: libLLVM-11.0.1 (ORCJIT, znver2)
  JULIA_DEPOT_PATH = /root/.cache/julia-buildkite-plugin/depots/a6029d3a-f78b-41ea-bc97-28aa57c6c6ea

Package Information:

      Status `/var/lib/buildkite-agent/builds/2-amdci4-julia-csail-mit-edu/julialang/scimltutorials-dot-jl/tutorials/perturbation/Project.toml`
  [0c46a032] DifferentialEquations v6.17.1
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  [91a5bcdd] Plots v1.15.2
  [30cb0354] SciMLTutorials v0.9.0
  [d1185830] SymbolicUtils v0.11.2
  [0c5d862f] Symbolics v0.1.25

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  [e33a78d0] Hwloc_jll v2.4.1+0
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  [dd192d2f] LibVPX_jll v1.9.0+1
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  [7e76a0d4] Libglvnd_jll v1.3.0+3
  [7add5ba3] Libgpg_error_jll v1.42.0+0
  [94ce4f54] Libiconv_jll v1.16.1+0
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  [38a345b3] Libuuid_jll v2.36.0+0
  [e7412a2a] Ogg_jll v1.3.4+2
  [458c3c95] OpenSSL_jll v1.1.1+6
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  [ea2cea3b] Qt5Base_jll v5.15.2+0
  [f50d1b31] Rmath_jll v0.3.0+0
  [fb77eaff] Sundials_jll v5.2.0+1
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  [2381bf8a] Wayland_protocols_jll v1.18.0+4
  [02c8fc9c] XML2_jll v2.9.12+0
  [aed1982a] XSLT_jll v1.1.34+0
  [4f6342f7] Xorg_libX11_jll v1.6.9+4
  [0c0b7dd1] Xorg_libXau_jll v1.0.9+4
  [935fb764] Xorg_libXcursor_jll v1.2.0+4
  [a3789734] Xorg_libXdmcp_jll v1.1.3+4
  [1082639a] Xorg_libXext_jll v1.3.4+4
  [d091e8ba] Xorg_libXfixes_jll v5.0.3+4
  [a51aa0fd] Xorg_libXi_jll v1.7.10+4
  [d1454406] Xorg_libXinerama_jll v1.1.4+4
  [ec84b674] Xorg_libXrandr_jll v1.5.2+4
  [ea2f1a96] Xorg_libXrender_jll v0.9.10+4
  [14d82f49] Xorg_libpthread_stubs_jll v0.1.0+3
  [c7cfdc94] Xorg_libxcb_jll v1.13.0+3
  [cc61e674] Xorg_libxkbfile_jll v1.1.0+4
  [12413925] Xorg_xcb_util_image_jll v0.4.0+1
  [2def613f] Xorg_xcb_util_jll v0.4.0+1
  [975044d2] Xorg_xcb_util_keysyms_jll v0.4.0+1
  [0d47668e] Xorg_xcb_util_renderutil_jll v0.3.9+1
  [c22f9ab0] Xorg_xcb_util_wm_jll v0.4.1+1
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  [a9144af2] libsodium_jll v1.0.20+0
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  [0dad84c5] ArgTools
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  [2a0f44e3] Base64
  [ade2ca70] Dates
  [8bb1440f] DelimitedFiles
  [8ba89e20] Distributed
  [f43a241f] Downloads
  [7b1f6079] FileWatching
  [9fa8497b] Future
  [b77e0a4c] InteractiveUtils
  [b27032c2] LibCURL
  [76f85450] LibGit2
  [8f399da3] Libdl
  [37e2e46d] LinearAlgebra
  [56ddb016] Logging
  [d6f4376e] Markdown
  [a63ad114] Mmap
  [ca575930] NetworkOptions
  [44cfe95a] Pkg
  [de0858da] Printf
  [3fa0cd96] REPL
  [9a3f8284] Random
  [ea8e919c] SHA
  [9e88b42a] Serialization
  [1a1011a3] SharedArrays
  [6462fe0b] Sockets
  [2f01184e] SparseArrays
  [10745b16] Statistics
  [4607b0f0] SuiteSparse
  [fa267f1f] TOML
  [a4e569a6] Tar
  [8dfed614] Test
  [cf7118a7] UUIDs
  [4ec0a83e] Unicode
  [e66e0078] CompilerSupportLibraries_jll
  [deac9b47] LibCURL_jll
  [29816b5a] LibSSH2_jll
  [c8ffd9c3] MbedTLS_jll
  [14a3606d] MozillaCACerts_jll
  [4536629a] OpenBLAS_jll
  [bea87d4a] SuiteSparse_jll
  [83775a58] Zlib_jll
  [8e850ede] nghttp2_jll
  [3f19e933] p7zip_jll