2.3.3 · D4Modern Physics

Exercises — Photon properties — E = hf, p = h - λ

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Figure — Photon properties — E = hf, p = h - λ

The picture above is the whole map: give me any one of and I can reach the other three by walking these arrows. Every problem below is just a walk on this map.


L1 — Recognition

You are handed one variable; return another by plugging into one formula. No tricks.

Recall Solution 1.1

WHAT we need: energy from frequency → use (the version that takes directly). WHY this form: we were given , so no need to detour through .

Recall Solution 1.2

WHAT we need: momentum from wavelength → the shortest route is . Convert first: .


L2 — Application

Two-step chains: convert or combine one relation with another.

Recall Solution 2.1

Step 1 — WHAT: given , want energy → use . Step 2 — WHY convert: joules this small are unreadable; divide by to get eV. A short wavelength ⇒ high energy — exactly why X-rays penetrate flesh.

Recall Solution 2.2

WHAT: we are handed and want → invert into . Is it visible? The visible band is roughly . is shorter, so it is ultraviolet, just outside what our eyes detect.

Recall Solution 2.3

Step 1 — energy per photon: Step 2 — WHY divide: power = (energy per photon)(photons per second), so .


L3 — Analysis

Compare, scale, or reason about ratios — not just single plug-ins.

Recall Solution 3.1

Reasoning: both and go as . So the ratio is just the inverse ratio of wavelengths. Photon B (shorter ) has the energy and 3× the momentum. Scaling both the same way is the fingerprint of .

Recall Solution 3.2

WHAT: ratio of energies of two photons → , so factor . The gamma photon is three trillion times more energetic — same equation, opposite ends of the spectrum.

Recall Solution 3.3

WHY this tool: the photon delivers all its energy in one lump; the electron spends escaping and keeps the rest as kinetic energy. This is Einstein's photoelectric equation — see Photoelectric Effect. If , no electron escapes at all — the lump simply isn't big enough, no matter how many lumps arrive.


L4 — Synthesis

Assemble several relations into one argument; watch limiting cases.

Recall Solution 4.1

Algebra (WHY): start from the parent's two definitions and eliminate . This is the same result the Relativistic Energy-Momentum Relation gives when you set rest mass . Numeric check (): , and . Then

Recall Solution 4.2

WHY momentum enters: force = rate of momentum delivered. Each photon carries . In one second the beam delivers energy , hence momentum per second. Tiny, but real — this is Radiation Pressure, the force that pushes solar sails. (A reflecting panel would double this to because momentum reverses.)

Recall Solution 4.3

Key insight: the de Broglie Wavelength relation is the same relation for the electron as for the photon — de Broglie ran the photon rule backwards for matter. Since both share the same , they share the same momentum: too. Their energies differ wildly (electron has rest mass, photon does not), but is fixed purely by .


L5 — Mastery

Multi-stage chains with a conceptual twist; every prior idea in play.

Recall Solution 5.1

(a) Photons per second. Energy per photon: (b) Force on the mirror. Power reaching mirror: . Reflection ⇒ momentum reverses ⇒ force . The distance is a decoy — it does not enter, because we were told the fraction of light caught directly.

Recall Solution 5.2

This is the Compton Effect: a photon behaving like a solid ball that loses energy to a recoiling electron. (a) Energy lost by photon = energy gained by electron. Compute both photon energies via . Electron's gain (b) The proof: the photon changed wavelength (hence momentum ). A pure wave bouncing off would keep its wavelength. A wavelength shift means the photon carried and traded momentum like a particle — momentum is the smoking gun.


Recall Self-test summary (fold and recite)

Give me , I get how? ::: . Give me , I get how? ::: . Force of an absorbed beam of power ? ::: . Force of a reflected beam of power ? ::: . Photons per second from power , wavelength ? ::: . Shorter wavelength means ___ energy and ___ momentum. ::: more; more (both ).


Connections