Q.Find 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: De Broglie Wavelength — but here it’s the inverse: X-rays are produced when fast electrons are suddenly stopped. The maximum photon energy equals the kinetic energy of the electron.
-
The kinetic energy of an electron accelerated through 30 kV is
K=eV=30 keV.
-
The maximum X-ray photon energy is the same:
Emax=hfmax=eV.
-
(a) Maximum frequency:
fmax=heV=6.63×10−341.6×10−19×30×103
=7.24×1018 Hz.
-
(b) Minimum wavelength:
λmin=fmaxc=7.24×10183×108
=4.14×10−11 m=0.0414 nm.
The maximum frequency is 7.24×1018 Hz and the minimum wavelength is 0.0414 nm.
The maximum frequency of X-rays comes from an electron converting all its kinetic energy into a single photon, giving fmax=7.24×1018 Hz. The minimum wavelength follows from c=fλ, giving λmin=0.0414 nm.
This is a classic problem that connects two beautiful ideas: the kinetic energy gained by an electron accelerated through a potential difference, and the quantum nature of light. When an electron slams into a metal target in an X-ray tube, it can lose energy in one dramatic step — emitting a single photon. The most energetic photon possible corresponds to the electron giving up all its kinetic energy at once. That sets the upper limit on frequency and the lower limit on wavelength.
The key relationship is the de Broglie–Einstein relation for photons: E=hf, where h is Planck’s constant. For the electron, the kinetic energy gained is K=eV, where e is the electron charge and V is the accelerating voltage. Setting K=hfmax gives us the maximum frequency. Then λmin=c/fmax gives the minimum wavelength.
Let’s work through it step by step.
- Find the kinetic energy of the electron. An electron accelerated through a potential difference V=30 kV=30×103 V gains kinetic energy
K=eV=(1.602×10−19 C)(30×103 V)=4.806×10−15 J.
This is the maximum energy available to produce a single X-ray photon.
- Set this equal to the photon energy for maximum frequency. The photon energy is E=hf. For the most energetic photon,
hfmax=eV.
So
fmax=heV.
Using h=6.626×10−34 J⋅s,
fmax=6.626×10−344.806×10−15=7.25×1018 Hz.
(Rounding to three significant figures gives 7.24×1018 Hz if we use h=6.63×10−34 — both are acceptable in exams.)
A common mistake is to forget that V is in kilovolts. Always convert to volts first: 30 kV=30000 V, not 30 V.
- Now find the minimum wavelength. For any electromagnetic wave, c=fλ. The minimum wavelength corresponds to the maximum frequency:
λmin=fmaxc.
Using c=3.00×108 m/s,
λmin=7.25×10183.00×108=4.14×10−11 m.
That’s 0.0414 nm (since 1 nm=10−9 m).
There’s a handy shortcut formula for the minimum wavelength in X-ray tubes:
λmin(in nm)=V(in kV)1.24.
Here, 1.24/30=0.0413 nm — nearly identical. This comes from combining eV=hc/λ and plugging in constants. Memorise it for speed in exams.
- Check the numbers with the shortcut. From eV=hc/λmin, we get
λmin=eVhc.
With hc=1240 eV⋅nm (a very useful constant),
λmin=30000 eV1240 eV⋅nm=0.0413 nm.
This confirms our calculation.
The maximum frequency is 7.24×1018 Hz and the minimum wavelength is 0.0414 nm.
Method: De Broglie–Duane–Hunt Relation (Inverse Photoelectric Effect)
This problem uses the fact that when an electron is stopped completely in a target, its entire kinetic energy converts into a single X-ray photon. That photon has the maximum possible frequency and the minimum possible wavelength for that accelerating voltage.
Step 1 – Write the energy conversion
The kinetic energy gained by an electron accelerated through a potential difference V is:
K=eV
where e=1.6×10−19 C and V=30 kV=30×103 V.
When this electron is brought to rest in one collision, the photon produced has energy:
Ephoton=hfmax=eV
Step 2 – Find maximum frequency
From the equation above:
fmax=heV
Use h=6.63×10−34 J⋅s.
fmax=6.63×10−34(1.6×10−19)(30×103)
fmax=6.63×10−344.8×10−15≈7.24×1018 Hz
fmax=heV
Step 3 – Find minimum wavelength
Use the wave relation c=fλ:
λmin=fmaxc=eVhc
where c=3×108 m/s.
A useful shortcut: hc≈1240 eV⋅nm (or 1.24×10−6 eV⋅m). Here:
λmin=30×103 eV1240 eV⋅nm≈0.0413 nm
In metres:
λmin=4.13×10−11 m
λmin=eVhc
Final Answer
- Maximum frequency: 7.24×1018 Hz
- Minimum wavelength: 4.13×10−11 m (or 0.0413 nm)
Tip
For quick calculation, remember hc=1240 eV⋅nm. Then λmin in nm is simply V (in volts)1240.
Watch outDo not confuse this with the de Broglie wavelength of the electron itself. The de Broglie wavelength of a 30 keV electron is about 7×10−12 m — noticeably smaller than the X-ray photon's minimum wavelength here. They are different physical quantities.
Common Mistakes on the De Broglie / X-Ray Wavelength Problem
This question is from the X-ray production chapter, not directly from the De Broglie wavelength topic — and that itself is the first trap. Students often mix up the two concepts. Let me walk through the mistakes one by one.
Mistake 1: Using the De Broglie wavelength formula instead of the Duane–Hunt relation
The most common error: a student sees "wavelength" and "electrons" and immediately writes
λ=ph=2meVh
This gives the De Broglie wavelength of the electron, not the X-ray wavelength. The question asks for the X-rays produced when electrons strike a target. The minimum wavelength of X-rays comes from the entire kinetic energy of the electron converting into a single photon:
λmin=eVhc
De Broglie wavelength is for a moving particle. X-ray wavelength is for a photon. They are different physical quantities — never use λ=h/p for photon wavelength in this context.
How to avoid: Read the question carefully. If it says "X-rays produced by electrons," you are in the X-ray production chapter. The relevant formula is eV=hfmax (or eV=hc/λmin). The De Broglie formula belongs to a different chapter.
Mistake 2: Forgetting to convert kV to V
The voltage is given as 30 kV. That is 30×103=3.0×104 V. Students sometimes plug in 30 directly, which gives an answer off by a factor of 1000.
How to avoid: Always write the conversion explicitly: V=30 kV=30×103 V=3.0×104 V. Do it on paper before substituting.
Mistake 3: Using the wrong value of Planck's constant or speed of light
Two common sub-mistakes here:
- Using h=6.63×10−34 J s but forgetting that eV is in joules. The energy eV must be in joules: E=(1.6×10−19)(3.0×104)=4.8×10−15 J.
- Using c=3×108 m/s but then getting the wavelength in metres — which is fine, but then you must convert to ångströms or picometres as the problem expects.
How to avoid: Keep a consistent unit system. Use SI units throughout, then convert at the end. A useful shortcut: for X-ray problems, use the formula in eV and ångströms:
λmin(in A˚)=V(in volts)12400
This comes from hc=12400 eV⋅A˚. For V=30 kV=30000 V:
λmin=3000012400=0.413 A˚
Memorise hc=12400 eV⋅A˚. It saves time and avoids unit errors in X-ray problems.
Mistake 4: Confusing maximum frequency with minimum wavelength
Students sometimes calculate the frequency correctly but then write λmin=c/fmax and get the right answer — but they mix up which is maximum and which is minimum. The relationship is:
fmax=heV,λmin=fmaxc=eVhc
Since f and λ are inversely related, the maximum frequency corresponds to the minimum wavelength. There is no "maximum wavelength" in this context — the continuous X-ray spectrum has a sharp cut-off at the short-wavelength end.
How to avoid: Write the two relations side by side:
- eV=hfmax → solve for fmax
- eV=λminhc → solve for λmin
Then check: does a larger V give a larger fmax? Yes. Does it give a smaller λmin? Yes. That consistency check catches errors.
Mistake 5: Not showing the final answer with correct units and significant figures
Examiners expect:
- Frequency in Hz (or s−1)
- Wavelength in metres or ångströms (often ångströms are preferred for X-rays)
For V=3.0×104 V:
fmax=heV=6.63×10−34(1.6×10−19)(3.0×104)=7.24×1018 Hz
λmin=eVhc=(1.6×10−19)(3.0×104)(6.63×10−34)(3×108)=4.14×10−11 m=0.414 A˚
How to avoid: After calculation, ask: "Does this wavelength make sense for X-rays?" X-ray wavelengths are of the order of 10−10 to 10−11 m (0.1–1 Å). If you get 10−8 m (UV range) or 10−12 m (gamma rays), you've made an error.
Summary of the correct approach
fmax=heV,λmin=eVhc
- Convert kV to V.
- Use eV in joules (or use the 12400 eV⋅A˚ shortcut).
- Do not use the De Broglie formula.
- Check that your final wavelength is in the X-ray range (~0.1–1 Å).
The correct answers:
- (a) fmax≈7.24×1018 Hz
- (b) λmin≈4.14×10−11 m (or 0.414 A˚)
- 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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