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AP Physics 2: Algebra Notes

7.6.3 Changes in Photon Energy, Frequency, and Wavelength

AP Syllabus focus: 'Energy transfer to an electron changes the photon’s energy, momentum, frequency, and wavelength after the interaction.'

When a photon transfers some of its energy to an electron, the photon that leaves the interaction is still light, but its measurable wave and particle properties are different.

Linked properties of a scattered photon

In this interaction, the incoming photon gives part of its energy to an electron. The outgoing photon is called the scattered photon.

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Schematic of Compton scattering: an incoming photon collides with an electron, producing a lower-energy scattered photon at a new angle and a recoiling electron. The geometry helps visualize why the photon’s momentum must change whenever energy is transferred to the electron. Source

Because it has lost some energy, it must also differ from the original photon in other linked quantities.

Scattered photon: The photon after it has interacted with an electron.

For AP Physics 2, the main idea is to see the connection: energy, frequency, wavelength, and momentum are related. If one changes, the others must change in a consistent way.

The most direct relationship is between photon energy and frequency.

E=hfE=hf

EE = photon energy, J

hh = Planck's constant, 6.63×1034 Js6.63\times10^{-34}\ J\cdot s

ff = photon frequency, Hz

Since hh is a constant, a decrease in photon energy means a decrease in photon frequency. So if the electron gains kinetic energy, the scattered photon must have a lower frequency than the incoming photon.

Frequency and wavelength change together

A photon’s frequency and wavelength are also linked. In vacuum, electromagnetic radiation travels at the speed of light, so frequency and wavelength must adjust together.

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Diagram of an electromagnetic wave showing electric and magnetic fields oscillating perpendicular to the direction of propagation, with wavelength marked peak-to-peak. This supports the relationship c=fλc=f\lambda by making wavelength a measurable spatial period while frequency is the corresponding time rate of oscillation. Source

c=fλc=f\lambda

cc = speed of light in vacuum, 3.00×108 m/s3.00\times10^8\ m/s

ff = frequency, Hz

λ\lambda = wavelength, m

Because cc stays constant in vacuum, a lower frequency means a longer wavelength. This gives the standard pattern for the scattered photon:

  • lower energy

  • lower frequency

  • longer wavelength

These are three ways of describing the same physical result. If an AP problem tells you only that the wavelength increased, you should immediately infer that the frequency and energy decreased.

It is also useful to combine the two relations mentally. Since energy is proportional to frequency and frequency is inversely related to wavelength, photon energy is inversely related to wavelength. A longer-wavelength photon carries less energy.

Momentum change follows the same pattern

Although this page centers on energy, frequency, and wavelength, the specification also notes that photon momentum changes. A photon with a longer wavelength has a smaller momentum.

p=hλp=\dfrac{h}{\lambda}

pp = photon momentum, kgm/skg\cdot m/s

hh = Planck's constant, 6.63×1034 Js6.63\times10^{-34}\ J\cdot s

λ\lambda = wavelength, m

This matters because the electron does not just receive energy; it also receives momentum. When the scattered photon leaves with a longer wavelength, that is evidence that its momentum is smaller than before the interaction.

Interpreting how much the photon changed

The amount of change is not always the same. Different interactions can transfer different amounts of energy to the electron.

  • If the electron gains only a little kinetic energy, the photon loses only a little energy.

  • A small energy loss means a small drop in frequency and a small increase in wavelength.

  • If the electron gains more kinetic energy, the photon’s energy decreases more, so the frequency decreases more and the wavelength increases more.

This means the final photon can leave with a range of possible energies, frequencies, and wavelengths, depending on how much energy was transferred during that specific interaction.

In problems, this is often described in whichever quantity is easiest to measure. A question may state that the outgoing photon has lower energy, or it may say that it has lower frequency, or it may say that it has longer wavelength. All three statements describe the same change in the scattered photon.

Recognizing equivalent descriptions in problems

AP Physics 2 questions often test whether you can translate between equivalent descriptions. The following statements all point to the same physical outcome:

  • the photon transferred energy to an electron

  • the photon’s energy decreased

  • the photon’s frequency decreased

  • the photon’s wavelength increased

  • the electron gained kinetic energy

You should practice moving quickly between these ideas. If one quantity changes, the others are not optional details; they are required by the photon relationships above.

A strong conceptual answer often uses words like proportional and inversely related:

  • from E=hfE=hf, energy is proportional to frequency

  • from c=fλc=f\lambda, wavelength is inversely related to frequency in vacuum

  • therefore, lower energy means lower frequency and longer wavelength

Common misunderstandings

One common mistake is to think that a lower-energy photon must travel more slowly. In vacuum, that is not correct. The photon still travels at speed cc; the change appears in frequency and wavelength.

Another mistake is to assume that the photon disappears completely whenever it gives energy to an electron. In this interaction, the photon usually continues after the event, but with reduced energy.

A third mistake is to treat the changes in energy, frequency, and wavelength as unrelated facts. They are not separate outcomes. They are linked descriptions of one process: energy transferred to the electron leaves the scattered photon with lower energy, lower frequency, and longer wavelength.

FAQ

The wavelength shift produced by scattering is very small in absolute size. For visible light, that change is tiny compared with the original wavelength, so it is difficult to measure clearly.

For X-rays, the original wavelengths are much shorter, so the same kind of shift is a much larger fraction of the starting wavelength and is easier to detect.

Photon energies at atomic and subatomic scales are extremely small in joules, so the numbers can be awkward to write and compare.

The electron-volt is a more convenient unit for these situations. One electron-volt is $1\ eV=1.60\times10^{-19}\ J$, so many photon energy changes can be written with simpler numbers.

If an instrument shows that the outgoing wavelength is longer, then the photon’s energy must be lower because $E=\dfrac{hc}{\lambda}$.

In practice, a spectrometer or diffraction setup can compare incoming and outgoing wavelengths. Even without measuring energy directly, the wavelength shift reveals the energy change.

Crystal atomic spacing is comparable to X-ray wavelengths, so crystals can diffract X-rays in a measurable way.

By observing the diffraction pattern or angle, physicists can determine the wavelength of the scattered photon. That makes crystals especially useful in experiments that track small wavelength changes.

At short wavelengths, energy changes rapidly with wavelength because $E=\dfrac{hc}{\lambda}$.

That means even a tiny absolute increase in $\lambda$ can represent a noticeable fractional decrease in energy. This is why small wavelength shifts can still indicate significant energy transfer for high-energy photons.

Practice Questions

A photon scatters from an electron, and the electron gains kinetic energy.

State how the scattered photon compares with the incident photon in: (a) frequency (b) wavelength

[2 marks]

  • 1 mark: frequency is lower / decreases

  • 1 mark: wavelength is longer / increases

An incident photon has energy EiE_i, frequency fif_i, and wavelength λi\lambda_i. After interacting with an electron, the scattered photon has energy 0.75Ei0.75E_i.

(a) Determine the scattered photon frequency in terms of fif_i. (b) Determine the scattered photon wavelength in terms of λi\lambda_i. (c) State what happened to the remaining energy.

[5 marks]


(a)

  • 1 mark: uses the idea that EE is proportional to ff

  • 1 mark: ff=0.75fif_f=0.75f_i

(b)

  • 1 mark: uses the idea that wavelength is inversely proportional to frequency

  • 1 mark: λf=10.75λi=43λi\lambda_f=\dfrac{1}{0.75}\lambda_i=\dfrac{4}{3}\lambda_i

(c)

  • 1 mark: remaining energy was transferred to the electron, typically as kinetic energy

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