ConceptComplete

ODEs in Physics - Core Definitions

Ordinary differential equations govern the time evolution of physical systems, from classical mechanics to quantum dynamics, providing mathematical models for deterministic processes.

Classification of ODEs

DefinitionOrder and Linearity

An ODE of order nn involves derivatives up to the nn-th order:

F(t,y,yβ€²,yβ€²β€²,…,y(n))=0F\left(t, y, y', y'', \ldots, y^{(n)}\right) = 0

A linear ODE has the form:

an(t)y(n)+anβˆ’1(t)y(nβˆ’1)+β‹―+a1(t)yβ€²+a0(t)y=f(t)a_n(t)y^{(n)} + a_{n-1}(t)y^{(n-1)} + \cdots + a_1(t)y' + a_0(t)y = f(t)

where f(t)f(t) is the forcing term. If f(t)=0f(t) = 0, the equation is homogeneous; otherwise it's inhomogeneous.

Physical laws are predominantly linear or linearizable, making linear ODE theory central to mathematical physics.

ExampleSimple Harmonic Oscillator

The undamped oscillator equation:

md2xdt2+kx=0m\frac{d^2x}{dt^2} + kx = 0

is second-order, linear, and homogeneous with constant coefficients. The general solution is:

x(t)=Acos⁑(Ο‰0t)+Bsin⁑(Ο‰0t)=Ccos⁑(Ο‰0t+Ο•)x(t) = A\cos(\omega_0 t) + B\sin(\omega_0 t) = C\cos(\omega_0 t + \phi)

where Ο‰0=k/m\omega_0 = \sqrt{k/m} is the natural frequency, and A,BA, B (or C,Ο•C, \phi) are determined by initial conditions x(0)x(0) and xΛ™(0)\dot{x}(0).

Existence and Uniqueness

TheoremPicard-LindelΓΆf Theorem

For the initial value problem:

dydt=f(t,y),y(t0)=y0\frac{dy}{dt} = f(t, y), \quad y(t_0) = y_0

if f(t,y)f(t,y) and βˆ‚f/βˆ‚y\partial f/\partial y are continuous in a region containing (t0,y0)(t_0, y_0), then there exists a unique solution in some interval ∣tβˆ’t0∣<Ξ΄|t - t_0| < \delta.

This theorem guarantees that physical systems described by ODEs have well-defined evolution given initial conditions, fundamental to deterministic physics.

ExampleExponential Growth

The equation dy/dt=Ξ»ydy/dt = \lambda y with y(0)=y0y(0) = y_0 has unique solution:

y(t)=y0eΞ»ty(t) = y_0 e^{\lambda t}

This models radioactive decay (Ξ»<0\lambda < 0), population growth (Ξ»>0\lambda > 0), and RC circuit discharge.

Systems of ODEs and Phase Space

DefinitionPhase Space Formulation

An nn-th order ODE can be rewritten as a system of nn first-order ODEs. For Newton's equation x¨=F(x,x˙,t)/m\ddot{x} = F(x,\dot{x},t)/m, define:

z=(xv),dzdt=(vF(x,v,t)/m)\mathbf{z} = \begin{pmatrix}x \\ v\end{pmatrix}, \quad \frac{d\mathbf{z}}{dt} = \begin{pmatrix}v \\ F(x,v,t)/m\end{pmatrix}

The space of (x,v)(\mathbf{x}, \mathbf{v}) is phase space, where trajectories represent system evolution.

ExampleDamped Harmonic Oscillator

The equation x¨+2γx˙+ω02x=0\ddot{x} + 2\gamma\dot{x} + \omega_0^2 x = 0 becomes:

ddt(xv)=(01βˆ’Ο‰02βˆ’2Ξ³)(xv)\frac{d}{dt}\begin{pmatrix}x \\ v\end{pmatrix} = \begin{pmatrix}0 & 1 \\ -\omega_0^2 & -2\gamma\end{pmatrix}\begin{pmatrix}x \\ v\end{pmatrix}

Eigenvalues Ξ»=βˆ’Ξ³Β±Ξ³2βˆ’Ο‰02\lambda = -\gamma \pm \sqrt{\gamma^2 - \omega_0^2} determine the solution type:

  • Underdamped (Ξ³<Ο‰0\gamma < \omega_0): Oscillatory decay
  • Critically damped (Ξ³=Ο‰0\gamma = \omega_0): Fastest return to equilibrium
  • Overdamped (Ξ³>Ο‰0\gamma > \omega_0): Exponential decay without oscillation

Green's Functions for ODEs

DefinitionGreen's Function

For the linear operator Ly=yβ€²β€²+p(t)yβ€²+q(t)y\mathcal{L}y = y'' + p(t)y' + q(t)y, the Green's function G(t,tβ€²)G(t,t') satisfies:

LG(t,tβ€²)=Ξ΄(tβˆ’tβ€²)\mathcal{L}G(t,t') = \delta(t - t')

with appropriate boundary conditions. The solution to Ly=f(t)\mathcal{L}y = f(t) is:

y(t)=∫G(t,tβ€²)f(tβ€²)dtβ€²y(t) = \int G(t,t')f(t')dt'

ExampleDriven Oscillator

For x¨+ω02x=F(t)/m\ddot{x} + \omega_0^2 x = F(t)/m with zero initial conditions, the Green's function is:

G(t,tβ€²)=sin⁑[Ο‰0(tβˆ’tβ€²)]mΟ‰0ΞΈ(tβˆ’tβ€²)G(t,t') = \frac{\sin[\omega_0(t-t')]}{m\omega_0}\theta(t-t')

The solution is:

x(t)=1mΟ‰0∫0tF(tβ€²)sin⁑[Ο‰0(tβˆ’tβ€²)]dtβ€²x(t) = \frac{1}{m\omega_0}\int_0^t F(t')\sin[\omega_0(t-t')]dt'

This is the convolution of the forcing with the impulse response, fundamental to linear response theory.

RemarkIntegrating Factors

For first-order linear equations yβ€²+p(t)y=q(t)y' + p(t)y = q(t), the integrating factor:

μ(t)=e∫p(t)dt\mu(t) = e^{\int p(t)dt}

transforms the equation to:

ddt[ΞΌ(t)y]=ΞΌ(t)q(t)\frac{d}{dt}[\mu(t)y] = \mu(t)q(t)

giving:

y(t)=1μ(t)[y0μ(t0)+∫t0tμ(s)q(s)ds]y(t) = \frac{1}{\mu(t)}\left[y_0\mu(t_0) + \int_{t_0}^t \mu(s)q(s)ds\right]

These foundational concepts enable systematic solution of ODEs governing time-dependent phenomena in physics, from orbital mechanics to quantum state evolution.