Q.A difference of 2.3 eV separates two energy levels in an atom. What is the frequency of radiation emitted when the atom makes a transition from the upper level to the lower level?
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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): …
The key idea is that the energy of the emitted photon equals the energy difference between the two levels, given by E=hf.
Step 1: Write the relation between energy and frequency:
E=hf
where h=4.135667696×10−15 eV⋅s (Planck's constant in eV·s).
Step 2: The energy difference is E=2.3 eV. Solve for f:
f=hE=4.135667696×10−152.3 …
The energy difference between two atomic levels is directly proportional to the frequency of the emitted photon via E=hν. For ΔE=2.3 eV, the frequency is ν=5.56×1014 Hz.
When an electron in an atom jumps from a higher energy level to a lower one, the atom loses energy. That energy doesn't vanish — it leaves the atom as a single packet of light, a photon. The photon’s energy is exactly equal to the difference between the two atomic energy levels.
This is the core idea behind atomic spectra: each spectral line corresponds to a specific transition, and the photon’s frequency is locked to the energy gap by Planck’s constant h.
Ephoton=hν=ΔE
Here h=6.626×10−34 J⋅s is Planck’s constant, and ν is the frequency in hertz. The problem gives ΔE=2.3 eV, but h is in joules — so we must convert the energy to joules first.
- Convert the energy from eV to joules. The conversion factor is 1 eV=1.602×10−19 J. So:
ΔE=2.3×1.602×10−19=3.6846×10−19 J
- Apply the photon energy relation. From E=hν, we solve for frequency:
ν=hΔE
- Plug in the numbers.
ν=6.626×10−343.6846×10−19
Divide:
ν=5.56×1014 Hz …
Method: Energy–Frequency Relation for a Photon (Planck–Einstein Relation)
This is a direct application of the Planck–Einstein equation, which connects the energy of a photon to its frequency. When an electron drops from a higher energy level to a lower one, the energy lost is emitted as a single photon. The photon’s energy equals the difference between the two atomic energy levels.
Step 1 – Write the Planck–Einstein relation
The energy E of a photon is proportional to its frequency ν:
E=hν
where h is Planck’s constant. In SI units, h=6.626×10−34 J⋅s. But here the energy is given in electronvolts (eV), so we need the value of h in eV·s:
h=4.135667696×10−15 eV⋅s
(You may use 4.14×10−15 eV⋅s in exams unless more precision is specified.)
Step 2 – Identify the photon energy
The energy difference between the two levels is given as ΔE=2.3 eV. This entire amount is carried away by the emitted photon:
Ephoton=ΔE=2.3 eV
Step 3 – Solve for frequency
Rearrange E=hν to get:
ν=hE
Substitute the numbers: …
Students often handle this question well because it is a direct application of the formula E=hν. But a few predictable mistakes trip people up. Here are the most common ones and how to avoid each.
1. Forgetting to convert electron-volts to joules
The energy difference is given in eV, but Planck’s constant h is usually taken in SI units (6.63×10−34 J⋅s). If you plug 2.3 eV directly into E=hν, you get a completely wrong frequency.
How to avoid: Always convert eV to joules before using h in J·s.
1 eV=1.6×10−19 J, so
E=2.3×1.6×10−19=3.68×10−19 J.
A common shortcut is to use h=4.14×10−15 eV⋅s — then you can work directly in eV. But if you do, make sure you use that value of h, not the SI one. Mixing units is the fastest way to lose marks.
2. Using the wrong formula (confusing frequency with wavelength)
Some students reach for E=λhc instead of E=hν. The question asks for frequency, not wavelength. Using the wrong formula wastes time and often leads to an incorrect unit (metres instead of Hz).
How to avoid: Read the question carefully. If it says “frequency”, think ν=hE. If it says “wavelength”, think λ=Ehc. There is no shortcut — you must match the formula to the quantity asked.
3. Arithmetic errors with powers of ten
When you divide 3.68×10−19 by 6.63×10−34, the exponents are (−19)−(−34)=+15. Students sometimes subtract incorrectly and get 10−53 or 1053.
How to avoid: Write the division step clearly: …
- 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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