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beginner · Physics · Waves, Light & Classical Background

Wave Basics: Wavelength and Period

Before quantum mechanics there were waves — and quantum mechanics turns out to be wave mechanics. Getting the vocabulary right now will pay off every time you encounter the Schrödinger equation, de Broglie wavelengths, or interference.

What a wave is

A travelling wave is a disturbance that moves through space at a definite speed without permanently transporting matter. The snapshot of the wave at any instant is periodic in space; the motion at any fixed point is periodic in time.

Two lengths fully characterise that periodicity:

| Symbol | Name | Definition | |--------|------|------------| | λ\lambda | wavelength | spatial distance between successive identical phases (e.g. crest to crest), in metres | | TT | period | time for one complete oscillation at a fixed point, in seconds |

The corresponding rates are the wave number k=2π/λk = 2\pi/\lambda (radians per metre) and the frequency f=1/Tf = 1/T (cycles per second, or hertz).

The fundamental wave relation

A crest travels one wavelength λ\lambda in exactly one period TT. Speed is distance divided by time, so

v=λT=λf.v = \frac{\lambda}{T} = \lambda f.

This is the single most useful equation in wave physics. For light in vacuum the speed is the universal constant c=2.998×108m/sc = 2.998 \times 10^8\,\text{m/s}, giving

c=λfλ=cf.c = \lambda f \quad \Longrightarrow \quad \lambda = \frac{c}{f}.

Angular frequency and wave number

Physicists often prefer the angular frequency ω=2πf\omega = 2\pi f (radians per second) and the wave number k=2π/λk = 2\pi/\lambda (radians per metre). In these variables the wave relation becomes simply ω=kv\omega = k v, and a sinusoidal wave travelling in the +x+x direction is written

y(x,t)=Acos(kxωt+ϕ0),y(x, t) = A\cos(kx - \omega t + \phi_0),

where AA is the amplitude and ϕ0\phi_0 is an initial phase.

Why this matters for quantum mechanics

De Broglie (1924) proposed that every particle with momentum pp has an associated wavelength

λ=hp,\lambda = \frac{h}{p},

where h=6.626×1034J sh = 6.626 \times 10^{-34}\,\text{J s} is Planck's constant. This one equation bridges the classical wave picture developed here and the quantum mechanical wave function developed in later modules. The smaller the wavelength (higher kk), the higher the momentum — a direct consequence of v=λfv = \lambda f applied to matter waves.

Try it

This is a numerical exercise — your code should return a number, not a circuit. Use the wave relation λ=c/f\lambda = c/f to find the wavelength of a 100 MHz radio wave in metres. Take c=3.0×108m/sc = 3.0 \times 10^8\,\text{m/s}.

Run your code to see the quantum state.

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