Classical Mechanics

Overview

The study of classical mechanics involves understanding the motion of bodies under the influence of forces. We assume no relativistic effects are at play and study simple systems using Newtonian, Lagrangian, and Hamiltonian frameworks.

Learning Path

Progress through Taylor’s Classical Mechanics.

Resources

Newton’s Laws of Motion

We first establish the Cartesian coordinate system with basis vectors (e1,e2,e3)(e_1, e_2, e_3) and position vector r=xe1+ye2+ze3\mathbf{r} = x e_1 + y e_2 + z e_3 which is written as (x,y,z)(x,y,z). We have all the standard vector operations for R3\mathbb{R}^3 such as dot product ab\mathbf{a} \cdot \mathbf{b} and cross product a×b\mathbf{a} \times \mathbf{b}.

For instance, consider a force F\mathbf{F} acting about the origin (like a stone). The torque Γ=r×F\mathbf{\Gamma} = r \times \mathbf{F} is defined as such.

We then have a vector valued function r(t)=(x(t),y(t),z(t))\mathbf{r}(t) = (x(t), y(t), z(t)) which can be differentiated and integrated with minimal issue. Most importantly, we note that r(t)=x(t)e1+y(t)e2+z(t)e3\mathbf{r}(t) = x(t) e_1 + y(t) e_2 + z(t) e_3, and so when we differentiate wrt time tt, each term is constant, and so you have three terms. This is special to the Cartesian coordinate system, and doesn’t hold for the Polar Coordinate system.

First and Second Law of Motion

The First Law of Motion states that an object with no forces acting on it will maintain constant velocity, i.e F=0    d2rdt2=0\mathbf{F} = 0 \implies \frac{d^2 \mathbf{r}}{dt^2} = 0.

And more generally, for an object with mass mm and force F\mathbf{F} acting on it, we have the Second Law of Motion:

F=md2rdt2=ma\mathbf{F} = m \frac{d^2 \mathbf{r}}{dt^2} = m \mathbf{a}

Recalling that momentum is defined as p=mv\mathbf{p} = m \mathbf{v}, we also have that F=dpdt\mathbf{F} = \frac{d \mathbf{p}}{dt}.

Inertial Frames

Note that the laws of motion only hold in inertial frames of reference, which are frames that are either at rest or moving with constant velocity. The easiest example of a non-inertial frame is an object moving inside a train that is accelerating. In such a frame, fictitious forces (like the Coriolis force) may appear to act on objects.

Third Law of Motion

For a pair of objects AA and BB, the force exerted by AA on BB is equal in magnitude and opposite in direction to the force exerted by BB on AA, i.e FAB=FBAF_{AB} = - F_{BA}.

Now consider a system of two objects AA and BB, we can write out their net forces as FAnet=FAB+FAextF_A^{net} = F_{AB} + F_{A}^{ext} and FBnet=FBA+FBextF_B^{net} = F_{BA} + F_{B}^{ext}. Adding these two equations, we have:

FAnet+FBnet=FAext+FBext=FextF_{A}^{net} + F_{B}^{net} = F_{A}^{ext} + F_{B}^{ext} = F_{ext}

If Fext=0F_{ext} = 0, then we have FAnet+FBnet=0F_{A}^{net} + F_{B}^{net} = 0, which implies that the total momentum of the system is conserved. Interestingly enough, the third law doesn’t even always hold up in classical mechanics, for instance, in electromagnetic interactions. Take two positive charges moving orthogonally to each other, the magnetic forces they exert on each other do not satisfy the third law by the Right Hand Rule.

Polar Newton

Recall r2=x2+y2r^2 = x^2 + y^2, x=rcos(θ)x = r \cos(\theta), y=rsin(θ)y = r \sin(\theta), and θ=tan1(y/x)\theta = \tan^{-1}(y/x). We have new unit vectors r^\hat{r} and θ^\hat{\theta} defined as:

r^=cos(θ)e1+sin(θ)e2,θ^=sin(θ)e1+cos(θ)e2\hat{r} = \cos(\theta) e_1 + \sin(\theta) e_2, \quad \hat{\theta} = -\sin(\theta) e_1 + \cos(\theta) e_2

This follows from r^=r(cos(θ),sin(θ))/r\hat{r} =r(cos(\theta), sin(\theta))/r and θ^\hat{\theta} being orthogonal to r^\hat{r} in the counter-clockwise direction. Trivially, swapping components and adding a negative sign achieves this.

Now that we have basis vectors that are not simple, we need to take care in differentiating. For a force F=Frr^+Fθθ^\mathbf{F} = F_r \hat{r} + F_\theta \hat{\theta} we want to determine what this is written as. Take a stone rotating around the origin on a string, FrF_r is the tension in the string and FθF_{\theta} is any air resistant perpendiular to the string.

To compute r¨\ddot{\mathbf{r}} so we can equate to Fr/mF_r/m, need to differentiate:

r˙=drdθdθdt=θθ˙\dot{\mathbf{r}} = \frac{d \mathbf{r}}{d \theta} \frac{d \theta}{d t} = \mathbf{\theta} \cdot \dot{\theta}

Then similarly compute θ˙=rθ˙\dot{\mathbf{\theta}} = - \mathbf{r} \dot{\theta}. We can differentiate again to obtain the acceleration.

Example: Skateboard on a Half Pipe

Consider a Skateboard with mass mm on a half pipe of radius RR. It’s dropped from rest at an angle θ\theta from the center of the half-pipe. As the radius is constant, we can simplify the acceleration formula by dropping out the r¨\ddot{r} terms yielding Fr=mRθ˙2F_r = - m R \dot{\theta}^2 and Fθ=mRθ¨F_{\theta} = m R \ddot{\theta}. The forces acting on the skateboard are Fr=mgcos(θ)NF_r =mg \cos(\theta) - N and Fθ=mgsin(θ)F_{\theta} = - mg \sin(\theta) where NN is the normal force from the half-pipe. Looking at the θ\theta equation, we have:

θ¨=gRsin(θ)\ddot{\theta} = - \frac{g}{R} \sin(\theta)

This is a nonlinear differential equation with no closed form solution. However, supposing that the skateboard is dropped near the center, we assume a small angle approximation sin(θ)θ\sin(\theta) \approx \theta, yielding θ¨=gRθ\ddot{\theta} = - \frac{g}{R} \theta. This is a simple harmonic oscillator with solution Let ω=gR\omega = \sqrt{\frac{g}{R}}, then we have:

θ(t)=θ0cos(ωt)\theta(t) = \theta_0 \cos(\omega t)