General Relativity

Einstein's Masterpiece: Gravity is the curvature of spacetime. Mass-energy tells spacetime how to curve, and spacetime tells mass-energy how to move.

Chapter 23: PP Waves

PP waves (plane-fronted parallel rays) are exact gravitational wave solutions representing waves with planar wave fronts. They're important in theoretical physics and provide exact solutions to Einstein's equations.

PP Wave Metric

\( ds^2 = 2du\,dv + H(u, x, y)du^2 + dx^2 + dy^2 \)

u, v are null coordinates, H is the profile function

Vacuum Condition

\( \nabla^2_{\perp} H = \frac{\partial^2 H}{\partial x^2} + \frac{\partial^2 H}{\partial y^2} = 0 \)

H is harmonic in transverse coordinates

Key Properties

Exact Solutions

Unlike linearized waves, pp waves are exact solutions to the full nonlinear Einstein equations.

Impulsive Waves

H(u) = δ(u)f(x,y) describes an impulsive gravitational wave — a sudden "shock" in spacetime.

Penrose Limit

Any spacetime, zoomed in near a null geodesic, becomes a pp wave. Universally important!