Einstein Equation Masterclass · Vidya720
Physics · Class 12 Dual Nature of Radiation and Matter · NEET

One packet, one electron: Einstein's equation, from a mela coconut stall to a NEET numerical

A full lesson: a cartoon movie to start, then why the wave picture fails, Einstein's energy packets, how K_max = hν − φ₀ explains every observation, Millikan's straight line with slope h/e, a numerical calculator, NEET shortcuts, problems to solve yourself, and 12 MCQs.

NCERT Class 12 Physics Part II · Ch 11 Dual Nature of Radiation and Matter · §11.5 Photoelectric effect and wave theory of light, §11.6 Einstein's photoelectric equation · pp. 281–283 · about 60 min

Voice
About 6 minutes. The animations start by themselves as the teacher explains them. Each stage's Listen button uses the same language.

A thousand peas cannot knock the coconut down, one cricket ball can. Light behaves the same way: what matters is the energy in one packet, hν, not how many packets arrive. Energy left after paying the work function becomes kinetic energy.

Stage 1 · The hook (5 min)

The coconut stall at the mela

Level

At the village mela, the shopkeeper's challenge is simple: knock a coconut off its stand and take it home. Arjun empties a whole bag of dried peas at it, hundreds of hits, and the coconut only wobbles. Meera throws one cricket ball. The coconut flies off. One strong hit beats any number of weak ones, because the energies of separate hits do not add up on the coconut.

In Lesson 2 you saw light behave exactly like this: very bright red light frees no electrons, while dim ultraviolet frees them at once. In 1905 Einstein explained it: light energy comes in packets (quanta) of hν, and one electron absorbs one whole packet. That one idea gives the equation K_max = hν − φ₀, which NEET uses in almost every paper.

Teacher says

"The coconut is the electron, the stand's grip is the work function, the cricket ball is a high-frequency photon, and the peas are low-frequency photons. More peas, brighter light, still no coconut."

Pause and predict

"If Meera throws the ball harder than needed, where does the extra energy go?"

Answer (this is the equation)

Into the coconut's flight: it flies off faster. For the electron, energy left over after paying the work function becomes its kinetic energy: K_max = hν − φ₀.

Stage 2 · The concept (10 min)

Why the wave picture fails

Level

In the wave picture, light energy is spread smoothly over the wavefront and every electron soaks up a little of it. That makes three predictions. Pick a test, move the sliders, and compare what wave theory says with what the experiment shows. The metal is sodium (φ₀ = 2.75 eV).

TestWave theory predictsExperiment shows
Brighterfaster electrons: K_max grows with intensityK_max does not depend on intensity
Low νany frequency works if bright enough or long enoughno emission below ν₀, whatever the intensity
Dima wait of hours or more while energy builds upinstantaneous (≲ 10⁻⁹ s)
Teacher says

"NCERT's line: the wave picture is unable to explain the most basic features of photoelectric emission. Three predictions, three failures. The problem is not the experiment; it is the idea that energy is spread out smoothly."

Stage 3 · The law (10 min)

Einstein's packets: K_max = hν − φ₀

Level

Light of frequency ν is a stream of quanta, each of energy E = hν. One electron absorbs one whole quantum in a single event. It spends at least φ₀ to escape; the rest is kinetic energy. Drag the top of the photon arrow (or use the slider) to change hν, and watch electrons from different depths.

  1. Energy of one quantum

    E = hν = hc/λ, E (eV) = 1240 / λ (nm)

    h = 6.63 × 10⁻³⁴ J s. A 400 nm photon carries 3.1 eV.

  2. Energy balance for one electron

    hν = φ₀ + K_max

    The least tightly bound electrons pay only φ₀ and leave with the most energy.

  3. Einstein's photoelectric equation

    K_max = ½ m v²_max = hν − φ₀

    Electrons bound more firmly lose more energy on the way out, so they leave with less than K_max.

Teacher says

"One photon, one electron, one event. Never add the energies of two photons for one electron. This is the cricket ball, not the bag of peas."

Stage 4 · Maths (10 min)

The equation explains every fact

Level

Photons rain on a sodium plate. Change the number of photons per second (intensity) and the energy of each (frequency). The graph on the right plots K_max against ν: watch which slider moves the point.

  1. K_max is set by ν only

    K_max = hν − φ₀

    Intensity does not appear in the equation. Brighter light means more photons, not bigger ones.

  2. Threshold

    K_max ≥ 0 ⇒ ν ≥ ν₀ = φ₀ / h

    Write the equation as K_max = h(ν − ν₀). Equivalently, λ₀ = hc/φ₀.

  3. Current and time

    electrons/s ∝ photons/s

    Above threshold, each absorbed photon can free one electron, so current ∝ intensity. One absorption is a single quick event: no build-up, no time lag.

Teacher says

"Weak light reduces how many electrons come out, not how soon. That one sentence answers the time-lag question every time."

Stage 5 · The big idea (10 min)

Millikan's straight line

Level

Put K_max = eV₀ into the equation: V₀ = (h/e) ν − φ₀/e. A graph of V₀ against ν must be a straight line of slope h/e, the same for every metal. Millikan worked from 1906 to 1916 hoping to prove Einstein wrong. Be Millikan: drag the two handles to fit a line through his kind of data (sodium) and read off h.

Slope

slope (V₀–ν) = h/e

Millikan's slope gave h ≈ 6.6 × 10⁻³⁴ J s, agreeing with Planck. For a K_max–ν graph (in joule) the slope is h itself.

Intercepts

ν-axis: ν₀ · V₀-axis: −φ₀/e

Extend the line backwards: it cuts the V₀-axis at −φ₀/e. In eV the intercept is simply −φ₀.

The verdict (1916)

photons accepted

The data supported Einstein. Einstein got the 1921 Nobel prize for the photoelectric law; Millikan got his in 1923.

Teacher says

"A scientist who tried hard to disprove a theory, and ended up proving it. That is how good physics is done. And for you: slope h by e, never just h, on a V₀–ν graph."

Stage 6 · Real life (5 min)

The photoelectric calculator

Level

Pick a real light source and a metal. The calculator does every step the way you should write it in the exam: photon energy, compare with φ₀, K_max, stopping potential and maximum speed.

Photocells and light meters

caesium, potassium

Low work function: visible light is above threshold, so ordinary light gives a current.

Germicidal lamps

254 nm → 4.9 eV

Enough to free electrons even from copper. The same high photon energy damages the DNA of germs.

Sodium lamps

589 nm → 2.11 eV

Below sodium's own 2.75 eV and just below caesium's 2.14 eV: a street lamp frees electrons from neither. Check the numbers, never guess.

Stage 7 · NEET level (10 min)

Shortcuts and tricks

Level

The 1240 rule

E (eV) = 1240 / λ (nm)

300 nm → 4.13 eV, 400 nm → 3.1 eV, 620 nm → 2.0 eV. Saves the whole hc/λ calculation.

Stopping potential in one line

V₀ (volt) = 1240/λ(nm) − φ₀(eV)

300 nm on 2.5 eV: V₀ = 4.13 − 2.5 = 1.63 V.

Threshold wavelength

λ₀ (nm) = 1240 / φ₀ (eV)

φ₀ = 2.0 eV → λ₀ = 620 nm. Emission needs λ < λ₀ (or ν > ν₀).

Ratio trick

K_max = h(ν − ν₀)

ν = 2ν₀ and 3ν₀ → K_max ratio 1 : 2 (not 2 : 3).

Two wavelengths, unknown φ₀

e(V₁ − V₂) = hc(1/λ₁ − 1/λ₂)

Subtract the two equations: φ₀ cancels. Use it to find h or V₂.

Graph slopes

V₀–ν: h/e · K_max–ν: h

Both straight lines, parallel for all metals. ν-intercept ν₀; V-intercept −φ₀/e.

Teacher says

"Every numerical here has the same three lines: photon energy with the 1240 rule, subtract the work function, then convert to whatever is asked: volts, joules or speed."

Stage 8 · Solve it yourself

Five worked problems

Level

Cover the solution, write the formula, and solve on paper. Open the hint only if you are stuck for more than a minute. Use hc = 1240 eV nm, e = 1.6 × 10⁻¹⁹ C, m = 9.1 × 10⁻³¹ kg.

Problem 1 · The standard numerical

Ultraviolet light of wavelength 250 nm falls on sodium (φ₀ = 2.75 eV). Find the maximum kinetic energy, the stopping potential and the maximum speed of the photoelectrons.

Hint

E = 1240/λ, then K_max = E − φ₀, V₀ = K_max/e.

Full solution
E = 1240 / 250 = 4.96 eV
K_max = 4.96 − 2.75 = 2.21 eV ⇒ V₀ = 2.21 V
v = √(2 × 2.21 × 1.6 × 10⁻¹⁹ / 9.1 × 10⁻³¹) = 8.8 × 10⁵ m/s
2.21 eV, 2.21 V, 8.8 × 10⁵ m/s
Problem 2 · Threshold

The work function of caesium is 2.14 eV. Find its threshold frequency and threshold wavelength. Will red light of 650 nm free electrons from it?

Hint

ν₀ = φ₀/h, λ₀ = 1240/φ₀.

Full solution
ν₀ = 2.14 × 1.6 × 10⁻¹⁹ / 6.63 × 10⁻³⁴ = 5.2 × 10¹⁴ Hz
λ₀ = 1240 / 2.14 = 579 nm
650 nm > 579 nm, so ν < ν₀
ν₀ ≈ 5.2 × 10¹⁴ Hz, λ₀ ≈ 579 nm; red 650 nm gives no emission
Problem 3 · Finding h and φ₀

For a metal, V₀ = 0.20 V at ν = 6.0 × 10¹⁴ Hz and V₀ = 1.03 V at ν = 8.0 × 10¹⁴ Hz. Find Planck's constant and the work function.

Hint

Subtract: e(V₂ − V₁) = h(ν₂ − ν₁). Then φ₀ = hν₁ − eV₁.

Full solution
h = 1.6 × 10⁻¹⁹ × 0.83 / 2.0 × 10¹⁴ = 6.64 × 10⁻³⁴ J s
hν₁ = 6.64 × 10⁻³⁴ × 6.0 × 10¹⁴ = 3.98 × 10⁻¹⁹ J = 2.49 eV
φ₀ = 2.49 − 0.20 = 2.29 eV
h ≈ 6.6 × 10⁻³⁴ J s, φ₀ ≈ 2.3 eV
Problem 4 · Halve the wavelength

Light of 400 nm gives photoelectrons with K_max = 1.0 eV. What is K_max for 200 nm light on the same metal? Is it simply double?

Hint

Find φ₀ first; it does not change.

Full solution
E(400) = 3.1 eV ⇒ φ₀ = 3.1 − 1.0 = 2.1 eV
E(200) = 6.2 eV ⇒ K_max = 6.2 − 2.1 = 4.1 eV
4.1 eV: more than double, because φ₀ is subtracted only once
Problem 5 · Ratio without numbers

Light of frequency 1.5ν₀ (ν₀ = threshold) gives photoelectrons of maximum kinetic energy K. The frequency is raised to 2ν₀. Find the new K_max in terms of K.

Hint

K_max = h(ν − ν₀).

Full solution
K = h(1.5ν₀ − ν₀) = 0.5 hν₀
K' = h(2ν₀ − ν₀) = hν₀
K' = 2K
Stage 9 · Practice ladder

12 MCQs, from easy to NEET-level

Level

Use hc = 1240 eV nm, h = 6.6 × 10⁻³⁴ J s, e = 1.6 × 10⁻¹⁹ C. Write the energy balance first, then click.

Score: 0 / 12

Stage 10 · Exam corner

How NEET asks this

If the question says…Write this firstThe trap
"light of wavelength λ falls on a metal of work function φ₀"K_max = 1240/λ − φ₀ (eV)Forgetting to subtract φ₀, or mixing J and eV
"stopping potential"eV₀ = hν − φ₀Writing V₀ = hν/e
"threshold wavelength / frequency"λ₀ = hc/φ₀, ν₀ = φ₀/hTaking λ > λ₀ as "enough"
"wavelength halved"find φ₀, recomputeDoubling K_max
"slope of V₀–ν graph"h/eAnswering h (that is the K_max–ν slope)
"intercept on the V₀-axis"−φ₀/eAnswering ν₀ (that is the ν-axis intercept)
"two wavelengths, two stopping potentials"subtract: e(V₁ − V₂) = hc(1/λ₁ − 1/λ₂)Solving each one for φ₀ separately and rounding
"which prediction of wave theory fails"K_max with intensity, threshold, time lagChoosing interference or "light carries energy"

Mistakes to avoid

Where this connects next

Lesson 4 takes Einstein's packets seriously as particles: the photon, with energy hν and momentum h/λ. Then light behaves as a wave in interference and as a particle in the photoelectric effect: the dual nature of radiation.

Values used: h = 6.63 × 10⁻³⁴ J s = 4.14 × 10⁻¹⁵ eV s, c = 3 × 10⁸ m/s, hc ≈ 1240 eV nm, e = 1.602 × 10⁻¹⁹ C, m = 9.11 × 10⁻³¹ kg. Work functions from NCERT Table 11.1. The Millikan-style data points in Stage 5 are generated for sodium-like behaviour with small scatter, not his original readings.

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Well done. What next?

Follow the four steps: understand it, remember it, try it, then prove it with past papers.

Lesson 4: Photons ›✍️ Practise this lesson: Dual Nature Challenge Q8–13: Einstein's equationRemember it: 5-Minute Revise‹ Previous: Lesson 2: The photoelectric experiment‹ Back to chapter🏠 Physics Part 2 home