Q.The work function of caesium is 2.14 eV. Find
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🔒 Start your 14-day free trial to unlock the full solution →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 …
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): …
Einstein's photoelectric equation: hν=ϕ+eV0.
(a) Threshold frequency: at threshold Kmax=0, so ν0=ϕ/h=4.1357×10−15 eV⋅s2.14 eV≈5.17×1014 Hz. …
The threshold frequency is ν0=ϕ/h≈5.17×1014 Hz, and the wavelength corresponding to a 0.60 V stopping potential is λ≈453 nm.
Why this approach works
The photoelectric effect is governed by Einstein's equation: a photon of energy hν must first supply the work function ϕ (the minimum energy to free an electron); anything left over becomes the electron's kinetic energy. At the threshold frequency, the photon has just enough energy to free the electron with zero leftover kinetic energy. When a stopping potential V0 is applied, it is just enough to stop even the fastest-ejected electrons, so their maximum kinetic energy equals eV0.
hν=ϕ+Kmax=ϕ+eV0
(a) Threshold frequency
At threshold, Kmax=0, so
hν0=ϕ⟹ν0=hϕ.
Using ϕ=2.14 eV and h=4.1357×10−15 eV⋅s (working directly in eV avoids converting ϕ to joules):
ν0=4.1357×10−152.14≈5.17×1014 Hz.
Keeping h in eV·s (≈4.14×10−15 eV⋅s) is a handy shortcut that saves a unit conversion whenever the work function is already given in eV.
(b) Wavelength for stopping potential V0=0.60 V
The photon's energy must supply both the work function and the stopping energy:
hν=ϕ+eV0=2.14+0.60=2.74 eV.
Convert to wavelength using hc≈1240 eV⋅nm:
λ=hνhc=2.741240≈452.6 nm≈453 nm.
Consistency check …
Method: Photoelectric Effect Equations
This problem uses Einstein's photoelectric equation, which connects the energy of incident photons to the work function of the metal and the kinetic energy of emitted electrons.
Step 1 — Recall the key relations
The photoelectric equation is:
hf=ϕ+Kmax
where:
- h is Planck's constant (6.63×10−34 J⋅s)
- f is the frequency of incident light
- ϕ is the work function of the metal
- Kmax is the maximum kinetic energy of emitted electrons
The stopping potential V0 is related to Kmax by:
Kmax=eV0
where e=1.6×10−19 C is the electronic charge.
At the threshold frequency f0, the kinetic energy is zero, so:
hf0=ϕ
Step 2 — Find the threshold frequency (part a)
Given ϕ=2.14 eV. Convert to joules:
ϕ=2.14×1.6×10−19=3.424×10−19 J
From hf0=ϕ:
f0=hϕ=6.63×10−343.424×10−19
f0=5.16×1014 Hz
You can also work entirely in eV·s for h: h=4.14×10−15 eV⋅s. Then f0=2.14/(4.14×10−15)=5.17×1014 Hz — the slight difference is due to rounding.
Step 3 — Find the wavelength for the given stopping potential (part b)
Given V0=0.60 V, so:
Kmax=eV0=0.60 eV
The incident photon energy is:
hf=ϕ+Kmax=2.14+0.60=2.74 eV
Convert to joules: …
Common Mistakes on Photon Energy & Photoelectric Effect Questions
Students lose marks on this exact type of problem in predictable ways. Here are the most frequent errors and how to fix them.
Mistake 1: Forgetting to convert electron-volts to joules
The work function is given as 2.14 eV, but the formula hf0=ϕ requires h in J⋅s and ϕ in joules. Many students plug 2.14 directly into f0=ϕ/h and get a nonsense answer.
How to avoid: Always convert eV to joules using 1 eV=1.6×10−19 J. So ϕ=2.14×1.6×10−19=3.424×10−19 J. Only then divide by h=6.63×10−34 J⋅s.
If you keep ϕ in eV and use h in J·s, your units won't cancel. The threshold frequency will be off by a factor of 1.6×10−19.
Mistake 2: Confusing threshold frequency with threshold wavelength
Part (a) asks for threshold frequency f0, not wavelength. Some students compute λ0=hc/ϕ instead. That's the threshold wavelength — a different quantity.
How to avoid: Read the question carefully. Threshold frequency comes from f0=ϕ/h. Threshold wavelength comes from λ0=hc/ϕ. They are not interchangeable.
Mistake 3: Using the wrong equation for part (b)
For the stopping potential part, students sometimes write eV0=hf alone, forgetting that the work function must be subtracted. The correct relation is:
eV0=hf−ϕ
or equivalently
hf=ϕ+eV0
How to avoid: Remember the photoelectric equation: kinetic energy of the fastest electron equals photon energy minus work function. Stopping potential just measures that maximum kinetic energy: Kmax=eV0.
Mistake 4: Mixing up units of stopping potential
The stopping potential is 0.60 V. When you compute eV0, you get 0.60 eV — that's already in electron-volts. But if you then add it to ϕ (which is also in eV), you must keep everything consistent. Some students convert eV0 to joules but leave ϕ in eV, or vice versa.
How to avoid: Work entirely in eV for the addition step, then convert to joules only when you need to use h or c. Here's the cleanest path:
- Total photon energy in eV: E=ϕ+eV0=2.14+0.60=2.74 eV
- Convert to joules: E=2.74×1.6×10−19=4.384×10−19 J
- Then λ=hc/E
Mistake 5: Using c=3×108 but forgetting to check units
When computing λ=hc/E, if E is in joules and h in J·s, c in m/s gives λ in metres. Students sometimes leave E in eV and get a wavelength off by 10−19.
How to avoid: Write out the units explicitly before calculating. If E is in joules, hc/E gives metres. If you prefer to keep E in eV, use the shortcut: …
- 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 …
- 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. …
- 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 …
- 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 …
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