Q.Monochromatic light of frequency 6.0×1014 Hz is produced by a laser. The power emitted is 2.0×10−3 W.
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 — each photon carries a discrete quantum of energy E=hν, where h is Planck’s constant and ν is the frequency.
(a) Energy of one photon:
E=hν=(6.63×10−34)(6.0×1014)=3.978×10−19 J
(b) Power P is energy per second. If n photons are emitted each second, total energy per second is nE=P. Hence:
n=EP=3.978×10−192.0×10−3≈5.03×1015
- The energy of a photon is 3.98×10−19 J;
- the number of photons emitted per second is 5.0×1015.
The energy of a single photon is found using E=hν, giving 3.98×10−19 J. The number of photons emitted per second is the total power divided by the photon energy, yielding 5.0×1015 photons/s.
Why Photon Energy Matters Here
Light is not a continuous stream of energy — it comes in discrete packets called photons. Each photon carries a specific energy that depends only on the frequency (or wavelength) of the light, not on the intensity. The laser's power tells us how much total energy is delivered per second. To find how many photons leave the laser each second, we simply divide the total energy per second (power) by the energy carried by one photon.
This is a clean, two-step problem: first find the energy of one photon, then count how many such photons make up the total power.
Step-by-Step Solution
1. Energy of a single photon
The energy E of one photon is given by the Planck-Einstein relation:
E=hν
where
h=6.626×10−34 J⋅s (Planck's constant)
ν=6.0×1014 Hz (frequency)
Substitute:
E=(6.626×10−34)×(6.0×1014)
E=3.9756×10−19 J
Rounding to two significant figures (matching the given data):
E≈3.98×10−19 J
Ephoton=hν
If you ever forget the value of h, remember it's roughly 6.63×10−34 J⋅s. For quick mental checks: light of frequency 5×1014 Hz (yellow-green) has photon energy about 3.3×10−19 J.
2. Number of photons emitted per second
Power P is energy per unit time. If each photon carries energy E, then the number of photons emitted per second n satisfies:
P=n×E
So:
n=EP
Given P=2.0×10−3 W (which is 2.0×10−3 J/s):
n=3.9756×10−192.0×10−3
n=5.03×1015 photons/s
Rounding to two significant figures:
n≈5.0×1015 photons/s
A common mistake is to forget that power is already in joules per second — no extra conversion is needed. Also, be careful with exponents: 10−3 divided by 10−19 gives 1016, not 10−22.
The energy of a photon is 3.98×10−19 J and the number of photons emitted per second is 5.0×1015 photons/s.
Method: Photon Energy Approach (using Planck's relation)
This problem uses the fundamental idea that light energy comes in discrete packets called photons. The energy of each photon depends only on the frequency of the light, not on the power. Power tells us how much total energy is delivered per second, so dividing that by the energy per photon gives the number of photons per second.
(a) Energy of a single photon
Step 1: Recall Planck's relation — the energy of one photon is directly proportional to its frequency:
E=hf
where h=6.63×10−34 J⋅s (Planck's constant) and f is the frequency in hertz.
Step 2: Substitute the given frequency:
E=(6.63×10−34)(6.0×1014)
Step 3: Multiply the numbers and the powers of ten separately:
6.63×6.0=39.78
10−34×1014=10−20
So E=39.78×10−20 J=3.978×10−19 J
Always check the exponent: 10−34×1014=10−20, not 10−48 — a common slip.
Step 4: Round to two significant figures (since the given frequency has two significant figures):
E=4.0×10−19 J
(b) Number of photons emitted per second
Step 1: Understand what power means. Power P=2.0×10−3 W means the source delivers 2.0×10−3 joules of energy each second.
Step 2: If each photon carries E joules, then the number of photons emitted per second, n, is:
n=energy per photontotal energy per second=EP
Step 3: Substitute the values:
n=4.0×10−192.0×10−3
Step 4: Divide the coefficients and subtract the exponents:
4.02.0=0.5
10−1910−3=1016
So n=0.5×1016=5.0×1015
Dividing powers of ten: 10−3÷10−19=10−3−(−19)=1016. The minus of a minus becomes plus.
n=5.0×1015 photons per second
Final answers:
- Energy of one photon = 4.0×10−19 J
- Number of photons emitted per second = 5.0×1015
Common Mistakes & How to Avoid Them
Mistake 1: Using the wrong formula for photon energy
Students often confuse E=hf with E=λhc. Both are correct, but the first is direct when frequency is given. The second requires an extra step (converting frequency to wavelength) and introduces more places for error — like using the wrong value for c or forgetting to convert units.
How to avoid: When frequency is given, use E=hf directly. Only switch to E=hc/λ when wavelength is provided. Memorise both forms but pick the one that matches the data.
If the problem gives frequency, your first instinct should be E=hf. No conversions needed.
Mistake 2: Forgetting the value of Planck's constant or using the wrong one
Planck's constant h is 6.63×10−34 J⋅s. Some students use 6.6×10−34 (acceptable in some boards, but risky) or accidentally use h=4.14×10−15 eV⋅s when the answer is expected in joules.
How to avoid: Write down h=6.63×10−34 J⋅s at the top of your working. If the question asks for energy in joules (which it usually does unless specified), stick to this value. If you must use the eV version, convert at the end — don't mix units mid-calculation.
Mistake 3: Incorrect exponent handling in part (a)
The calculation is:
E=(6.63×10−34)(6.0×1014)
Students often add exponents incorrectly: 10−34×1014=10−20, not 10−48 or 10−20 with a sign error. Also, they sometimes forget to multiply the coefficients: 6.63×6.0≈39.78, not 3.978.
How to avoid: Separate the calculation into two parts:
- Multiply the coefficients: 6.63×6.0=39.78
- Add the exponents: −34+14=−20
- Combine: 39.78×10−20=3.978×10−19
Then round to appropriate significant figures (here, two significant figures from the given data gives 4.0×10−19 J).
10−34×1014=10−20, not 10−48 (that's multiplying exponents instead of adding them). This is the single most common exponent error.
Mistake 4: Confusing power with energy in part (b)
Power P=2.0×10−3 W means 2.0×10−3 J of energy is emitted per second. Some students treat power as the total energy or forget that it's already a rate.
How to avoid: Write down what power means: P=tEtotal. For t=1 s, Etotal=P×1=P. So the number of photons per second is:
n=energy per photontotal energy per second=EP
Mistake 5: Dividing in the wrong order
Students sometimes compute E/P instead of P/E, getting a tiny fraction instead of a large number.
How to avoid: Check the units. You want photons per second, which has units of s−1. P has units J/s, E has units J. So P/E gives JJ/s=s−1, which is correct. E/P gives seconds — a time, not a rate.
Unit check: JW=JJ/s=s−1. Always verify your formula by checking what units it produces.
Mistake 6: Arithmetic errors in part (b)
n=4.0×10−192.0×10−3=0.5×1016=5.0×1015
Common errors: dividing coefficients as 2.0/4.0=0.5 but then writing 0.5×10−16 (sign error on exponent), or forgetting that 10−3/10−19=1016.
How to avoid: Again, separate coefficient and exponent:
- Coefficients: 2.0/4.0=0.5
- Exponents: −3−(−19)=−3+19=16
- Combine: 0.5×1016=5.0×1015
Final Answers
(a) E=hf=4.0×10−19 J
(b) n=EP=5.0×1015 photons per second
- GSEB Higher Secondary Certificate (HSC) Examination 2026Set ANNUAL1 markMCQQ.Monochromatic light of frequency 6.0 x 10^14 Hz is produced by a laser. The power emitted is 2.0 x 10^-3 W. How many photons per second on an average, are emitted by the source?(a) 0.5 x 10^15(b) 0.5 x 10^17(c) 5 x 10^17(d) 5 x 10^15
›Reveal solutionSolution
The number of photons emitted per second is the total power divided by the energy carried by a single photon, E = h nu.
Given: nu = 6.0 x 10^14 Hz, P = 2.0 x 10^-3 W, h = 6.63 x 10^-34 J s.
Energy per photon: E = h nu = 6.63 x 10^-34 x 6.0 x 10^14 = 3.98 x 10^-19 J
Photons per second: n = P/E = (2.0 x 10^-3)/(3.98 x 10^-19) = 5.0 x 10^15 photons/s.
✓Final answer(d) 5 x 10^15.
- GSEB Higher Secondary Certificate (HSC) Examination 2025Set ANNUAL1 markMCQQ.Monochromatic light of frequency 6 x 10^14 Hz is produced by a laser. The power emitted is 2 x 10^-3 W. How many photons per second on an average are emitted by the source? [h = 6.63 x 10^-34 Js](a) 3.98 x 10^19(b) 1.99 x 10^15(c) 3 x 10^15(d) 5 x 10^15
›Reveal solutionSolution
Each photon carries energy E = hν; dividing the total power by this per-photon energy gives the photon emission rate.
E = hν = (6.63 × 10⁻³⁴)(6 × 10¹⁴) = 3.978 × 10⁻¹⁹ J.
n = P/E = (2 × 10⁻³)/(3.978 × 10⁻¹⁹) ≈ 5.03 × 10¹⁵ ≈ 5 × 10¹⁵ photons/s.
✓Final answer(d) 5 × 10¹⁵ photons/s.
- GSEB Higher Secondary Certificate (HSC) Examination 2025Set ANNUAL1 markMCQQ.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? [h = 6.63 x 10^-34 Js](a) 1.2 x 10^14 Hz(b) 5.6 x 10^14 Hz(c) 3.8 x 10^14 Hz(d) 1.6 x 10^6 Hz
›Reveal solutionSolution
The frequency of emitted radiation during an atomic transition follows Bohr's frequency condition: hν = ΔE.
ΔE = 2.3 eV = 2.3 × 1.6 × 10⁻¹⁹ = 3.68 × 10⁻¹⁹ J.
ν = ΔE/h = 3.68 × 10⁻¹⁹ / 6.63 × 10⁻³⁴ ≈ 5.55 × 10¹⁴ Hz ≈ 5.6 × 10¹⁴ Hz.
✓Final answer(b) 5.6 × 10¹⁴ Hz.
- GSEB Higher Secondary Certificate (HSC) Examination 2024Set ANNUAL1 markMCQQ.The momentum of a photon of light of frequency f is ___.(a) hc/f(b) h/cf(c) hf/c(d) hcf
›Reveal solutionSolution
A photon of energy E = hf carries momentum p = E/c.
p = E/c = hf/c.
✓Final answer(c) hf/c.
- GSEB Higher Secondary Certificate (HSC) Examination 2023Set ANNUAL1 markMCQQ.Monochromatic light of frequency 6 x 10^14 Hz is produced by laser. The power emitted is 2 x 10^-3 W. The energy of the photon in this light beam is ___ eV. [h = 6.63 x 10^-34 Js, 1 eV = 1.6 x 10^-19 J](a) 3.0(b) 3.5(c) 4.0(d) 2.5
›Reveal solutionSolution
Photon energy E = h*nu = 3.98 x 10^-19 J; dividing by 1.6 x 10^-19 J/eV gives about 2.5 eV.
Energy of a photon: E = h*nu = (6.63 x 10^-34)(6 x 10^14) = 3.978 x 10^-19 J.
Convert to eV: E = (3.978 x 10^-19)/(1.6 x 10^-19) = 2.49 eV approximately 2.5 eV.
(The beam power 2 x 10^-3 W is extra data - it fixes the number of photons per second, not the energy of one photon.)
✓Final answer(d) 2.5 eV.
- GUJCET 2022Set 171 markMCQQ.A difference of 5.4 eV separates two energy levels in an atom. What is the frequency of radiation emitted when the atom make a transition from the upper level to the lower level? [1 eV = 1.6×10−19 J, h=6.625×10−34 J.s.] (A) 1.304×1015 Hz (B) 5.6×1015 Hz (C) 5.6×1014 Hz (D) 1.304×1014 Hz
›Reveal solutionSolution
Photon frequency f=ΔE/h.
Steps.
- ΔE=5.4 eV=5.4×1.6×10−19=8.64×10−19 J.
- f=6.625×10−348.64×10−19=1.304×1015 Hz.
✓Final answer(A) 1.304×1015 Hz
ANSWER: (A)
- GUJCET 2022Set 171 markMCQQ.What is the shortest wavelength present in the Paschen series of spectral lines? (A) 320 nm (B) 720 nm (C) 840 nm (D) 820 nm
›Reveal solutionSolution
Shortest wavelength = series limit, 1/λ=RH/9.
Concept. The shortest wavelength of a hydrogen series comes from the transition n=∞→nf. For Paschen, nf=3.
Steps.
- λ1=RH(321−0)=91.097×107=1.219×106 m−1.
- λ=8.2×10−7 m=820 nm.
✓Final answer(D) 820 nm
ANSWER: (D)
- GSEB Higher Secondary Certificate (HSC) Examination 2020Set ANNUAL1 markMCQQ.Monochromatic light of frequency 6x10^14 Hz is produced by laser. Each photon has an energy = ____ J.(a) 6x10^14(b) 4x10^-19(c) 4x10^-20(d) 6x10^-14
›Reveal solutionSolution
Photon energy E = hf; substituting f = 6×10¹⁴ Hz gives about 4×10⁻¹⁹ J.
E=hf=(6.63×10−34)×(6×1014)=3.978×10−19 J≈4×10−19 J.
✓Final answer(b) 4×10^-19 J.
- GSEB Higher Secondary Certificate (HSC) Examination 2019Set ANNUAL1 markMCQQ.Which of the following physical quantity has the dimension of planck constant (h)?(a) Angular momentum(b) Force(c) Energy(d) Power
›Reveal solutionSolution
Planck's constant has dimensions of Energy × Time =[ML2T−2][T]=[ML2T−1], which is also the dimension of angular momentum.
Angular momentum =mvr has dimension [M][LT−1][L]=[ML2T−1], matching h. Force, energy, and power all have different dimensions ([MLT−2], [ML2T−2], [ML2T−3] respectively).
✓Final answer(a) Angular momentum.
- GSEB Higher Secondary Certificate (HSC) Examination 2018Set ANNUAL1 markMCQQ.Energy of photon is E = hf and its momentum is P = h/lambda, where lambda is the wavelength of photon. With this assumption speed of light wave is ___.(a) P/E(b) E/P(c) EP(d) (E/P)^2
›Reveal solutionSolution
Speed of light = f x lambda; using f = E/h and lambda = h/P gives speed = E/P.
The speed of a light wave is v = f lambda.
From E = h f: f = E/h.
From P = h/lambda: lambda = h/P.
Therefore v = f lambda = (E/h)(h/P) = E/P.
(This is the familiar relation E = P c for a photon, since v = c.)
✓Final answer(b) E/P.
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