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: …
- AP EAPCET 2025Set eng-2025-05-21-FN1 markMCQQ.If an electron in the excited state falls to ground state, a photon of energy 5 eV is emitted, then the wavelength of the photon is nearly (A) 748 nm (B) 598 nm (C) 398 nm (D) 248 nm
›Reveal solutionSolution
Tests the photon energy–wavelength relation for a hydrogen-atom-like transition; the emitted photon has λ≈248 nm.
Concept and Intuition
When an electron falls from an excited state to the ground state, the energy difference is carried away as a single photon, E=hν=λhc. It is convenient to remember the handy constant hc≈1240 eV⋅nm, so that E(eV)λ(nm)=1240.
Step-by-Step Solution
- Given photon energy E=5 eV.
- Using λ=E(eV)1240 nm: λ=51240=248 nm …
- AP EAPCET 2024Set eng-2024-05-23-FN1 markMCQQ.Energy levels A, B and C of a certain atom corresponding to increasing values of energy i.e., EA<EB<EC. If λ1,λ2 & λ3 are the wavelengths of a photon corresponding to the transitions shown, then [FIGURE] (an energy-level diagram with levels EC labelled C at the top, EB labelled B in the middle, and EA labelled A at the bottom; a downward transition arrow λ1 goes from C to B, a downward transition arrow λ2 goes from B to A, and a downward transition arrow λ3 goes directly from C to A) (A) λ3=λ1+λ2 (B) λ3=λ1λ2(λ1+λ2) (C) λ32=λ12+λ22 (D) λ3=(λ1+λ2)λ1λ2
›Reveal solutionSolution
Since the energy released in going directly from C to A must equal the energy released going C→B→A, the photon energies (not wavelengths) add, giving λ3=λ1λ2/(λ1+λ2).
Concept and Intuition
Energy levels obey conservation of energy: the total energy dropped going from level C to level A is a fixed number, EC−EA, regardless of the path taken. Whether the atom emits one photon directly (C→A) or two photons via an intermediate level (C→B then B→A), the energies released must add up to the same total. Photon energy is E=hc/λ, so it is the reciprocals of the wavelengths that add, not the wavelengths themselves.
Step-by-Step Solution
- Energy released in transition C→B: E1=λ1hc.
- Energy released in transition B→A: E2=λ2hc.
- Energy released in the direct transition C→A: E3=λ3hc.
- Conservation of energy: E3=E1+E2, since EC−EA=(EC−EB)+(EB−EA).
- So λ3hc=λ1hc+λ2hc⇒λ31=λ11+λ21=λ1λ2λ1+λ2.
- Invert: λ3=λ1+λ2λ1λ2.
Common Mistakes …
- AP EAPCET 2023Set eng-2023-05-17-AN1 markMCQQ.The particle having zero mass is (A) proton (B) neutron (C) photon (D) electron
›Reveal solutionSolution
The photon is the only listed particle with zero rest mass; protons, neutrons, and electrons are all massive particles.
Concept and Intuition
Particles are classified by whether they have rest mass. Matter particles like the proton, neutron, and electron all have well-defined nonzero rest masses (measured precisely in atomic mass units / MeV). The photon, the quantum of the electromagnetic field, has zero rest mass — it can never be brought to rest and always moves at speed c in vacuum; its total energy is purely kinetic in the relativistic sense, given by E=pc (the massless limit of E2=(pc)2+(mc2)2).
Step-by-Step Solution …
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