Q.The work function of caesium metal is 2.14 eV. When light of frequency 6×1014 Hz is incident on the metal surface, photoemission of electrons occurs. What is the
Concept understanding — Photon Energy
Photon Energy: The Energy Carried by Light
Light does not carry its energy in a continuous stream. It comes in discrete packets — like individual drops instead of a steady hose. Each packet is called a photon: the smallest possible unit of light of a given frequency. You cannot have half a photon; it is all or nothing.
The Intuition: Colour Determines Energy
Red light and blue light are both light, but they behave differently — blue light causes sunburn and drives chemical reactions more readily than red. The reason is that the colour (frequency) of light directly fixes how much energy each photon carries, and blue photons carry more energy than red photons.
The Planck–Einstein Relation
The energy E of a single photon is directly proportional to its frequency f, and inversely proportional to its wavelength λ:
E=hf=λhc
Where:
- E = energy of one photon (joules, J)
- f = frequency (hertz, Hz)
- λ = wavelength (metres, m)
- c = speed of light in vacuum (3.00×108 m/s)
- h = Planck's constant (6.626×10−34 J·s)
Planck's constant h is extremely tiny, so an individual photon carries a very small amount of energy — which is why we never feel single photons striking our skin.
What This Tells You
- Higher frequency = higher energy. Gamma rays have extremely energetic photons; radio waves have very low-energy photons.
- Shorter wavelength = higher energy. Ultraviolet photons are more energetic than visible-light photons; infrared photons are less.
- Energy is quantised. Light energy comes in fixed packets — you can have 1, 2, or 1000 photons, but never 0.5. This was Max Planck's revolutionary idea of 1900.
This is why UV light causes sunburn (UV photons carry enough energy to damage DNA, while visible photons do not), why X-ray photons are energetic enough to pass through soft tissue but get absorbed by bone, and why a photon needs enough energy to actually break a bond or drive a photochemical/biological reaction, rather than merely wavelength-dependent intensity.
A Concrete Example
Question: Which has more energy — a photon of red light (λ=700 nm) or a photon of blue light (λ=450 nm)?
Since E=λhc, energy is inversely proportional to wavelength, so the shorter-wavelength blue photon carries more energy:
- Red: Ered=700×10−9(6.626×10−34)(3.00×108)≈2.84×10−19 J
- Blue: Eblue=450×10−9(6.626×10−34)(3.00×108)≈4.42×10−19 J
The blue photon carries about 1.5 times the energy of the red photon.
A common mistake is to think brighter light means more energetic photons. Brightness is the number of photons per second, not the energy per photon. A bright red light has many low-energy photons; a dim blue light has fewer but higher-energy ones.
The Big Picture
Photon energy is the bridge between the wave nature of light (frequency, wavelength) and its particle nature (energy packets) — one of the foundational ideas of quantum mechanics: at the smallest scales, energy is not continuous but comes in discrete, indivisible units.
Photon energy, given by the Planck-Einstein relation E = hf, is one of the most fundamental formulas in the NCERT Class 12 Physics Dual Nature of Radiation and Matter chapter, and "photon energy formula and calculation" is a heavily searched query among students preparing for CBSE boards, JEE Main, and NEET. Because this idea links directly to the photoelectric effect and atomic spectra, it also anchors several "modern physics important questions" compiled for competitive-exam revision.
Why this formula?
Why Photon Energy is E=hf — The Reasoning Behind the Formula
The formula E=hf is not something you memorise and plug numbers into. It comes from a deep shift in how physicists understood light.
The problem that forced the formula
By the late 1800s, classical physics said light was a wave — continuous, carrying energy in proportion to its intensity (brightness). But blackbody radiation and the photoelectric effect showed something bizarre: when you shine light on a metal, electrons are ejected only if the light's frequency is above a certain threshold, no matter how bright the light is. Below that frequency, even the brightest lamp won't kick out a single electron. Classically this made no sense — a wave's energy depends on amplitude, not frequency.
Einstein's radical idea (1905)
Einstein proposed that light comes in discrete packets — photons — each carrying a fixed energy that depends only on its frequency, with Planck's constant h as the proportionality:
A single photon's energy is E=hf, where f is the frequency of the light.
This directly explains the photoelectric effect: an electron needs a minimum energy (the work function ϕ) to escape. If a photon's energy hf<ϕ, no electron is ejected — regardless of how many photons you send, because each photon interacts with one electron individually.
E=hf is not derived from deeper principles — it is a postulate justified by the experiments it explains, and it unified optics with quantum mechanics.
The equivalent forms
Since c=fλ for light in vacuum, the same idea in terms of wavelength is:
E=λhc
Use this when you're given λ instead of f. A photon also carries momentum (despite having no mass):
p=cE=λh
This follows from special relativity: E2=(pc)2+(mc2)2, and for a photon m=0, so E=pc, hence p=h/λ.
- h=6.626×10−34 J⋅s (Planck's constant)
- c=3.0×108 m/s (speed of light)
- For atomic-scale problems use electronvolts: 1 eV=1.602×10−19 J
A common exam trap
E=hf means higher frequency = more energy per photon — true. But a brighter light does not mean higher photon energy. Intensity is the number of photons per second per area; each photon still carries hf.
Do not confuse intensity (number of photons) with frequency (energy per photon). They are independent.
Final answer: E=hf
Concept: Photon Energy — The energy of an incident photon is E=hν. Part of it goes into overcoming the work function ϕ, and the remainder appears as the maximum kinetic energy Kmax of the photoelectron.
Step 1: Photon energy
E=hν=(6.63×10−34)(6×1014)=3.978×10−19 J
Convert to eV: E=1.6×10−193.978×10−19=2.486 eV
Step 2: Maximum kinetic energy
Kmax=E−ϕ=2.486−2.14=0.346 eV
In joules: Kmax=0.346×1.6×10−19=5.536×10−20 J
Step 3: Stopping potential
V0=eKmax=0.346 V
Step 4: Maximum speed
Kmax=21mvmax2⟹vmax=m2Kmax
vmax=9.1×10−312×5.536×10−20=3.49×105 m/s
- Kmax=0.346 eV,
- V0=0.346 V,
- vmax=3.49×105 m/s
Using Einstein’s photoelectric equation, the maximum kinetic energy is found from the difference between the incident photon energy and the work function. The stopping potential is that kinetic energy divided by the electron charge, and the maximum speed comes from the kinetic energy formula. The answers are: (a) 0.345 eV,
(b) 0.345 V,
(c) 3.48×105 m/s.
The Core Idea: Photon Energy and the Photoelectric Effect
When light hits a metal surface, it behaves as a stream of particles — photons. Each photon carries a quantum of energy given by E=hf, where h is Planck’s constant and f is the frequency. For an electron to be ejected, the photon must supply enough energy to overcome the work function ϕ — the minimum energy needed to free an electron from the metal surface.
Any extra energy beyond ϕ appears as the maximum kinetic energy of the emitted electron. This is Einstein’s photoelectric equation:
Kmax=hf−ϕ
The stopping potential V0 is the voltage that just stops the most energetic electrons — it’s directly related to Kmax by eV0=Kmax. And once we know Kmax in joules, the maximum speed follows from Kmax=21mvmax2.
Let’s apply this step by step.
Step 1: Find the photon energy
The incident light has frequency f=6×1014 Hz. Planck’s constant is h=6.63×10−34 J⋅s.
Photon energy in joules:
E=hf=(6.63×10−34)(6×1014)=3.978×10−19 J
We’ll need this in electronvolts too. Since 1 eV=1.6×10−19 J:
E=1.6×10−193.978×10−19=2.486 eV
A quick check: the product hf in eV can be found using h=4.14×10−15 eV⋅s. Then E=(4.14×10−15)(6×1014)=2.484 eV — essentially the same.
Step 2: Maximum kinetic energy (part a)
Work function ϕ=2.14 eV. Using Einstein’s equation:
Kmax=hf−ϕ=2.486 eV−2.14 eV=0.346 eV
Rounding to three significant figures (matching the given data):
Kmax=0.345 eV
A common mistake is to forget that hf and ϕ must be in the same units. Here both are in eV, so subtraction is straightforward. If you work in joules, convert ϕ first: ϕ=2.14×1.6×10−19=3.424×10−19 J, then Kmax=(3.978−3.424)×10−19=0.554×10−19 J, which equals 0.346 eV — same result.
Step 3: Stopping potential (part b)
The stopping potential V0 satisfies eV0=Kmax. Since Kmax is in eV, the numerical value of V0 in volts is the same:
V0=eKmax=0.345 V
Step 4: Maximum speed (part c)
First convert Kmax to joules:
Kmax=0.345 eV×1.6×10−19 J/eV=5.52×10−20 J
Electron mass m=9.1×10−31 kg. From Kmax=21mvmax2:
vmax=m2Kmax=9.1×10−312×5.52×10−20
Calculate inside the square root:
9.1×10−311.104×10−19=1.213×1011
Taking square root:
vmax=1.213×1011=3.48×105 m/s
This speed is about 0.1% of the speed of light — non-relativistic, so the classical kinetic energy formula is perfectly valid.
(a) Maximum kinetic energy is 0.345 eV, (b) stopping potential is 0.345 V, and (c) maximum speed is 3.48×105 m/s.
Method: Einstein's Photoelectric Equation
This problem is solved using Einstein's photoelectric equation, which states that the incident photon energy is used partly to overcome the work function and the remainder appears as the maximum kinetic energy of the emitted electron.
Step 1: Write down the given data
| Quantity | Value |
|---|---|
| Work function ϕ | 2.14 eV |
| Frequency of incident light f | 6×1014 Hz |
| Planck's constant h | 6.63×10−34 J⋅s |
| 1 eV | 1.6×10−19 J |
| Mass of electron me | 9.1×10−31 kg |
Step 2: Calculate the incident photon energy
Photon energy E=hf
E=(6.63×10−34)(6×1014)=3.978×10−19 J
Convert to eV:
E=1.6×10−193.978×10−19=2.486 eV
Always check whether the photon energy exceeds the work function — only then will photoemission occur. Here 2.486 eV>2.14 eV, so emission is possible.
Step 3: Find maximum kinetic energy (part a)
Einstein's photoelectric equation:
Kmax=hf−ϕ
Kmax=2.486−2.14=0.346 eV
In joules:
Kmax=0.346×1.6×10−19=5.536×10−20 J
Kmax=hf−ϕ
Step 4: Find stopping potential (part b)
The stopping potential V0 is related to Kmax by:
Kmax=eV0
V0=eKmax=e0.346 eV=0.346 V
When Kmax is in eV, the stopping potential in volts is numerically equal to Kmax in eV. So V0=0.346 V directly.
Step 5: Find maximum speed (part c)
Use kinetic energy in joules:
Kmax=21mevmax2
vmax=me2Kmax
vmax=9.1×10−312×5.536×10−20
vmax=1.216×1011=3.487×105 m/s
Final Answers
(a) Maximum kinetic energy: 0.346 eV (or 5.54×10−20 J)
(b) Stopping potential: 0.346 V
(c) Maximum speed: 3.49×105 m/s
Common Mistakes Students Make on This Photon Energy Problem
Mistake 1: Forgetting to convert units before using formulas
The work function is given in eV, but the Planck constant h is usually taken in J·s (6.63×10−34 J⋅s). Students often plug 2.14 eV directly into Kmax=hf−ϕ without converting everything to joules first.
How to avoid: Always check unit consistency. Convert the work function from eV to joules using 1 eV=1.6×10−19 J:
ϕ=2.14×1.6×10−19=3.424×10−19 J
Now compute hf in joules:
hf=(6.63×10−34)(6×1014)=3.978×10−19 J
Then Kmax=3.978×10−19−3.424×10−19=5.54×10−20 J.
If you keep ϕ in eV and hf in joules, you'll get a meaningless number. Always work in a single unit system — joules is safest for kinetic energy and speed calculations.
Mistake 2: Confusing stopping potential with maximum kinetic energy
Students sometimes write V0=Kmax directly, forgetting that stopping potential is related by eV0=Kmax.
How to avoid: Remember the definition: stopping potential is the voltage that just stops the most energetic electrons. The work done by the electric field (eV0) equals the maximum kinetic energy lost. So:
V0=eKmax
Using Kmax=5.54×10−20 J:
V0=1.6×10−195.54×10−20=0.346 V
If you already have Kmax in eV, then V0 in volts is numerically equal to Kmax in eV. Here Kmax=0.346 eV, so V0=0.346 V — a handy shortcut.
Mistake 3: Using the wrong mass for the electron in the speed calculation
Students sometimes use the mass of a proton or forget to square the speed properly in K=21mv2.
How to avoid: The electron mass is me=9.1×10−31 kg. Rearranging:
vmax=me2Kmax=9.1×10−312×5.54×10−20
Compute step by step:
- 2Kmax=1.108×10−19
- Divide by me: 9.1×10−311.108×10−19=1.218×1011
- Take square root: vmax=3.49×105 m/s
| Quantity | Value | Unit |
|----------|-------|------|
| Kmax | 5.54×10−20 | J |
| V0 | 0.346 | V |
| vmax | 3.49×105 | m/s |
Mistake 4: Forgetting that photoemission requires hf≥ϕ
Some students attempt the problem even when the photon energy is below the work function, getting a negative kinetic energy.
How to avoid: First check if emission is possible. Here hf=3.978×10−19 J and ϕ=3.424×10−19 J, so hf>ϕ — emission occurs. If hf<ϕ, simply state "no photoemission" and stop.
Mistake 5: Rounding intermediate values too aggressively
Rounding Kmax to 5.5×10−20 J early can throw off the speed calculation significantly because of the square root.
How to avoid: Keep at least 3 significant figures throughout, and round only the final answer. Use h=6.63×10−34 consistently (not 6.6×10−34).
Final answers:
- (a) Kmax=5.54×10−20 J (or 0.346 eV)
- (b) V0=0.346 V
- (c) vmax=3.49×105 m/s
- KCET 2024Set D-21 markMCQQ.The ratio of area of first excited state to ground state of orbit of hydrogen atom is (A) 1:16 (B) 1:4 (C) 4:1 (D) 16:1
›Reveal solutionSolution
r∝n2⇒ area ∝n4; for n=2 vs n=1 that is 24:14=16:1.
Step 1 — Bohr's radius formula
For a hydrogen-like atom, Bohr's quantisation of angular momentum (mvr=nℏ) combined with the Coulomb-force–centripetal-force balance gives
rn=πme2Zn2h2ε0⟹rn∝n2 (for fixed Z)
For hydrogen (Z=1), rn=n2a0 with a0=0.529 A˚.
Step 2 — From radius to area
The orbit is a circle, so the area enclosed is
An=πrn2
Since rn∝n2,
An∝(n2)2=n4
This n4 (not n2) is the crux of the question — the squaring of an already-squared quantity.
Step 3 — Identify the two states
- Ground state: n=1.
- First excited state: the next level up, n=2. (Not n=3 — the "first excited" state is the first level above the ground state.)
Step 4 — Take the ratio
A1A2=πr12πr22=(12a0)2(22a0)2=(a0)2(4a0)2=a0216a02=16
The question asks for first excited : ground, i.e.
A2:A1=16:1
Step 5 — Guard against the traps
- 4:1 (option C) is the ratio of the radii, not the areas.
- 1:4 and 1:16 have the ratio inverted — the excited orbit is bigger, so the ratio must be greater than 1.
✓Final answerThe correct option is (D) — 16:1.
ANSWER: D
- COMEDK 2024Set 2024-M1 markMCQQ.The difference in energy levels of an electron at two excited levels is 13.75 eV. If it makes a transition from the higher energy level to the lower energy level then what will be the wave length of the emitted radiation? [given h=6.6×10−34 m2 kg s−1;c=3×108 ms−1;1 eV=1.6×10−19 J] (A) 900 nm (B) 90 A (C) 9000 nm (D) 900∘A
›Reveal solutionSolution
Using E=hc/λ, the 13.75 eV energy difference corresponds to a wavelength of 90 nm, i.e. 900 Å — matching option (D).
Step-by-step reasoning
- Convert the energy to joules.
E=13.75 eV×1.6×10−19 J/eV=2.2×10−18 J
- Solve for wavelength.
λ=Ehc=2.2×10−18(6.6×10−34)(3×108)=2.2×10−1819.8×10−26=9.0×10−8 m
- Convert to convenient units.
9.0×10−8 m=90 nm=900 A˚(since 1 nm=10 A˚)
This matches the option listing 900 Å.
Watch outDon't confuse nm and Å — 1 nm equals 10 Å, not 100 Å. Here 90 nm equals 900 Å.
TipQuick shortcut: E(eV)≈λ(nm)1240, so λ≈1240/13.75≈90.2 nm — confirming the result fast.
✓Final answerThe correct option is (D): 900 Å.
- KCET 2022Set B-31 markMCQQ.The radius of hydrogen atom in the ground state is 0.53 A∘. After collision with an electron, it is found to have a radius of 2.12 A∘, the principle quantum number 'n' of the final state of the atom is (A) n = 3 (B) n = 4 (C) n = 1 (D) n = 2
›Reveal solutionSolution
Bohr radii go as n2; the radius has grown by a factor of 4, so n2=4 and the atom is excited to n=2.
1. The Bohr radius law
Quantising the angular momentum (mvr=nh/2π) and balancing the Coulomb force against the centripetal requirement gives, for a hydrogen-like atom,
rn=πme2Zn2h2ε0=Zn2a0
where a0=0.53 A˚ is the Bohr radius. For hydrogen Z=1, so simply
rn=n2a0
The radius grows as the square of the principal quantum number — that quadratic dependence is the whole content of the problem.
2. Set up the ratio
Ground state: r1=0.53 A˚ (with n=1, consistent with the formula).
Final state after the collision: rn=2.12 A˚.
Taking the ratio kills a0 entirely:
r1rn=12a0n2a0=n2
3. Solve
n2=0.532.12=4
n=4=2
4. Physical reading
The collision with the electron transferred just enough energy to lift the atom from the ground state to the first excited state. Check consistency with the energy ladder: En=−13.6/n2 eV, so E2−E1=−3.4−(−13.6)=10.2 eV — precisely the well-known first excitation energy of hydrogen. Everything is self-consistent.
(Trap: option (C) n=1 would mean nothing happened, and n=3 or 4 would require the radius to be 9a0=4.77 A˚ or 16a0=8.48 A˚, not 2.12 A˚.)
✓Final answerThe correct option is (D) — n = 2.
ANSWER: D
- KCET 2019Set A-11 markMCQQ.Frequency of revolution of an electron revolving in nth orbit of H-atom is proportional to (A) n21 (B) n (C) n independent of n (D) n31
›Reveal solutionSolution
The frequency of revolution of an electron in the nth orbit of a hydrogen atom is proportional to n31, making option (D) correct.
The key here is to connect the frequency of revolution — how many times per second the electron circles the nucleus — to the orbital radius and velocity. In Bohr's model, the electron moves in a circular orbit under electrostatic attraction, and its angular momentum is quantized. Frequency is simply v/(2πr), so if we find how v and r depend on n, we can combine them.
Let's work through it step by step.
- Write the force balance for a stable orbit. The centripetal force is provided by the Coulomb attraction between the electron and the proton:
rmv2=r2ke2
where m is the electron mass, v its speed, r the orbit radius, k=1/(4πϵ0), and e the elementary charge.
- Apply Bohr's quantization condition. Angular momentum is an integer multiple of ℏ=h/(2π):
mvr=nℏ
- Solve for r in terms of n. From the quantization condition, v=nℏ/(mr). Substitute into the force equation:
rm(mrnℏ)2=r2ke2
Simplify:
mr3n2ℏ2=r2ke2
Multiply both sides by r3:
mn2ℏ2=ke2r
So:
r=mke2n2ℏ2
This shows r∝n2.
- Find v in terms of n. From mvr=nℏ, we have v=nℏ/(mr). Substitute r∝n2:
v∝n2n=n1
So v∝1/n.
- Now compute the frequency of revolution. Frequency f is the number of orbits per second:
f=2πrv
Substitute the proportionalities v∝1/n and r∝n2:
f∝n21/n=n31
Watch outA common mistake is to think frequency is proportional to 1/n2 because energy is proportional to 1/n2. But frequency here is mechanical revolution frequency, not the frequency of emitted radiation (which relates to energy differences). They are different quantities.
TipYou can also derive this directly from the known expressions: rn=n2a0 and vn=αc/n, where a0 is the Bohr radius and α the fine-structure constant. Then f=vn/(2πrn)∝(1/n)/(n2)=1/n3.
✓Final answerThe frequency of revolution is proportional to n31, so the correct option is (D).
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