Photon Properties and Energy-Momentum Relations
Photons are massless particles of light characterized by their energy, frequency, momentum, and charge neutrality, and their interactions obey conservation laws.
Why this shows up in the exam
NEET often asks you to relate photon energy and momentum to frequency and wavelength, and to apply conservation laws in photon-matter interactions.
How NEET tests this
Learn the idea
Photons are mass‑less quanta whose energy E = hν = hc/λ and momentum p = h/λ (or p = E/c); they always travel at speed c in vacuum. The unlocking insight is that a single constant h ties frequency, wavelength, energy and momentum together.
🧠 Memory hook: Think of a photon as a light‑bulb ticket: h is the ticket number that tells you both the price (energy = h·ν) and the size (momentum = h/λ), and the ticket always rides at speed c.
Get this one clearly and it pays off every single time it shows up in the paper. 🎯
Formulas & facts to keep ready
- Photon energy E = hν where ν = c/λ
- Photon momentum p = h/λ = E/c
- h ≈ 6.6×10⁻³⁴ J·s (NCERT value)
- Photons are charge‑neutral, massless and move with speed c in free space
- Power P = energy per second, so number of photons per second N = P/E_photon
- Wavelength must be expressed in metres when using the formulas
How to approach it
- 1Write the photon energy using E = hc/λ (or E = hν)
- 2Convert every length unit to metres and frequency to s⁻¹
- 3If the question asks for a count, use N = P/E_photon (or N = Energy supplied / energy of one photon)
- 4For momentum‑related queries replace E by pc or use p = h/λ
Worked example — watch it click
The number of photons per second on an average emitted by the source of monochromatic light of wavelength 600 nm, when it delivers the power of 3.3 × 10⁻³ watt will be (h = 6.6 × 10⁻³⁴ J s)
- A)10¹⁵
- B)10¹⁸
- C)10¹⁷
- ✅10¹⁶
The concept behind this problem
The worked example forces you to compute the energy of a single photon from its wavelength, then relate power to photon count – a direct application of E = hc/λ and N = P/E.
Step by step
- 1Energy of one photon: E = (hc)/(λ). h = 6.6×10⁻³⁴ J s, c = 3×10⁸ m/s, λ = 600 nm=6×10⁻⁷ m.
- 2E = 6.6×10⁻³⁴×3×10⁸6×10⁻⁷ = 1.98×10⁻²⁵6×10⁻⁷ = 3.3×10⁻¹⁹ J per photon.
- 3Number of photons emitted per second N = PowerE = 3.3×10⁻³ J/s3.3×10⁻¹⁹ J = 10¹⁶.
- 4A value of 10¹⁵ would result from using a larger photon energy (e.g., taking λ as 600 Å), while 10¹⁷ or 10¹⁸ would come from under-estimating the photon energy.
- 5So the correct answer is 10¹⁶.
Watch out
Students often forget to change 600 nm to 6×10⁻⁷ m, which makes the photon energy off by a factor of 10⁹ and gives the wrong photon‑per‑second count.
Common slip-ups that cost marks
- •Forgetting to convert nm (or Å) to metres – a common 10⁹ error
- •Mixing up ν and λ in the formula (using ν where λ is required)
- •Assuming a photon can have a speed different from c in vacuum
🌟 That's the whole idea — you've got this. Try the practice set below; every question you attempt makes it stick a little harder.
Practise it
These are real questions from past NEET papers that test this exact idea.
The number of photons per second on an average emitted by the source of monochromatic light of wavelength 600 nm, when it delivers the power of 3.3 × 10⁻³ watt will be (h = 6.6 × 10⁻³⁴ J s)
Push further
More challenging5 harder questions built from the past papers above — a step up in difficulty, with distractors designed so you can't get there by elimination. Written and checked by our reviewers, not from a real paper.
An X-ray photon with a wavelength of 0.1 nm undergoes Compton scattering with a stationary electron. Which of the following statements is true regarding the scattered photon?
More from Dual Nature of Matter and Radiation
Photoelectric Effect
The photoelectric effect describes the emission of electrons from a material when it is exposed to light of sufficient frequency, governed by concepts such as threshold frequency, work function, stopping potential, and the Einstein photoelectric equation.
de Broglie Wavelength and Matter Waves
All matter exhibits wave-like properties, with the de Broglie wavelength inversely proportional to momentum and dependent on factors like velocity, temperature, and particle type.
Photon Energy and Momentum
For a photon in vacuum, energy is proportional to frequency and momentum is energy divided by c. Frequency and wavelength obey c = nu lambda, so shorter-wavelength photons have larger energy and momentum.
Photon Rate, Power, and Energy Density
For monochromatic radiation, total energy is the number of photons times h nu. Power is energy per unit time, so the photon emission rate equals power divided by single-photon energy.
Radiation Pressure and Photon Momentum Transfer
Radiation force is the rate of photon momentum transfer. For normal incidence on an ideal absorber the pressure is intensity divided by c; for an ideal reflector it is twice that value.
Photoelectric Effect Observations
For a fixed emitter, emission occurs only when incident frequency reaches the threshold frequency. Above threshold, maximum kinetic energy depends on frequency, while saturation current is primarily proportional to intensity.