Q.A 100 watt bulb emits monochromatic light of wavelength 400 nm. Calculate the number of photons emitted per second by the bulb.
Concept understanding — Photon Energy Calculation
Photon Energy Calculation
The Intuition First
Imagine you're holding a rope tied to a wall. If you flick your wrist once, a single pulse travels down the rope. If you flick faster — more frequently — each pulse carries more energy; the rope vibrates more violently. Light behaves the same way. A photon is the smallest possible "flick" of the electromagnetic field — a single, indivisible packet of light energy.
What determines how much energy that one photon carries? Two things: how fast the wave is oscillating (its frequency), and a universal constant that connects the wave world to the particle world.
The Precise Statement
The energy E of a single photon is directly proportional to its frequency f (or inversely proportional to its wavelength λ). The proportionality constant is Planck's constant h, one of the most fundamental numbers in physics.
E=hf=λhc
Where:
- E = energy of one photon (in joules, J)
- h = Planck's constant = 6.626×10−34 J⋅s
- f = frequency of the electromagnetic wave (in hertz, Hz)
- c = speed of light = 3.00×108 m/s
- λ = wavelength of the light (in metres, m)
Why Two Forms?
The first form E=hf is the most direct: higher frequency means higher energy. The second form E=hc/λ is often more practical because wavelength is easier to measure than frequency. Since c=fλ, you can always swap between them.
What This Tells You
- Blue light (short wavelength, high frequency) has more energy per photon than red light (long wavelength, low frequency).
- Gamma rays have enormous photon energies; radio waves have tiny photon energies.
- The energy is quantised — you cannot have half a photon. Either the full energy hf is absorbed/emitted, or none at all.
A Worked Example
Question: Calculate the energy of a single photon of violet light with wavelength 400 nm.
Step 1: Convert wavelength to metres.
400 nm=400×10−9 m=4.00×10−7 m
Step 2: Use E=hc/λ.
E=4.00×10−7(6.626×10−34)(3.00×108)
Step 3: Compute.
E=4.00×10−71.9878×10−25=4.97×10−19 J
This is an incredibly tiny amount of energy — about 5×10−19 joules. That's why we often use electronvolts (eV) for photon energies in atomic physics. 1 eV=1.602×10−19 J, so this photon has about 3.1 eV.
Common Mistake to Avoid
Do not confuse the energy of one photon with the total energy of a light beam. A dim red laser and a bright red laser both emit photons of the same energy (same f, same λ). The bright laser just emits more photons per second. Total beam power = (energy per photon) × (number of photons per second).
Why This Matters
Photon energy calculation is the foundation of:
- The photoelectric effect (Einstein's Nobel-winning insight)
- Atomic spectra (why each element emits specific colours)
- Solar cell design (matching photon energy to semiconductor band gaps)
- Medical imaging (X-ray photon energies determine tissue penetration)
The key takeaway: frequency is energy. When you see light, you're seeing packets of energy whose size depends only on colour — not on brightness. That's the quantum world in a nutshell.
Photon energy calculation using E = hf = hc/lambda is one of the most frequently asked numerical formats in the NCERT Class 12 Physics Dual Nature of Radiation and Matter chapter, and "photon energy calculation important questions" is a common search for CBSE board and JEE Main/NEET revision. This same calculation reappears across atomic-spectra and photoelectric-effect problems, making it a high-value formula to master for competitive physics papers.
Concept: Photon Energy Calculation
The power of the bulb tells us the total energy emitted per second. Each photon carries energy E=λhc, so the number of photons emitted per second is simply the total energy per second divided by the energy per photon.
Step 1: Energy of one photon at λ=400 nm=400×10−9 m:
Ephoton=λhc=400×10−9(6.63×10−34)(3×108)=400×10−919.89×10−26=4.97×10−19 J
Step 2: Power P=100 W means 100 J of energy is emitted every second. The number of photons per second is:
n=EphotonP=4.97×10−19100≈2.01×1020 photons/s
The bulb emits 2.012×1020 photons per second.
Each photon carries energy E=λhc; dividing the bulb's power by the energy per photon gives the photon emission rate of 2.01×1020 photons per second.
Why this approach works
Power tells us energy per unit time. A 100 W bulb delivers 100 joules every second. If the bulb emits monochromatic light, every photon carries the same energy determined by its wavelength. The number of photons emitted per second is simply the total energy per second divided by the energy carried by one photon.
The energy of a single photon depends on its frequency (or equivalently, its wavelength) through Planck's relation:
Ephoton=hν=λhc
where h is Planck's constant, c is the speed of light, and λ is the wavelength.
Step-by-step calculation
1. Identify the given quantities
The bulb's power is P=100 W=100 J/s, meaning it emits 100 joules of energy every second. The wavelength of the emitted light is λ=400 nm=400×10−9 m.
2. Calculate the energy of one photon
Using the photon energy formula:
Ephoton=λhc
Substitute the constants:
- Planck's constant: h=6.626×10−34 J⋅s
- Speed of light: c=3×108 m/s
- Wavelength: λ=400×10−9 m
Ephoton=400×10−9(6.626×10−34)(3×108)
Ephoton=400×10−919.878×10−26=4×10−719.878×10−26
Ephoton=4.9695×10−19 J
Rounding appropriately, Ephoton≈4.97×10−19 J.
3. Find the number of photons emitted per second
The number of photons N emitted per second is the total energy emitted per second divided by the energy per photon:
N=EphotonP=4.97×10−19100
N=2.012×1020 photons/s
For quick estimates, remember that visible light photons (400–700 nm) carry energies on the order of 10−19 J. A 1 W source emits roughly 1018 to 1019 photons per second.
This calculation assumes all the bulb's electrical power is converted to light. Real incandescent bulbs are inefficient (most energy becomes heat), so the actual number of photons would be much smaller. The problem implicitly asks for the idealized case where 100 W of optical power is emitted.
The bulb emits 2.01×1020 photons per second.
Showing the 12 most recent of 28 on this concept.
- AP EAPCET 2026Set eng-2026-05-14-FN1 markMCQQ.The work function of Mg, Cu, Ag, Li are 3.7, 4.8, 4.3, 2.5 eV respectively. A wavelength of 300 nm light is shined on them. The metals which undergo photoelectric effect are (A) Mg, Cu (B) Cu, Ag (C) Ag, Li (D) Mg, Li
›Reveal solutionSolution
Compare each metal's work function to the incident photon energy (~4.13 eV at 300 nm); photoemission occurs only if ϕ<Ephoton. That's true for Mg and Li only.
Concept and Intuition
Photoelectric emission from a metal happens only if each incoming photon carries at least as much energy as the metal's work function — below that threshold, no number of low-energy photons can eject an electron (this is the key experimental fact that classical wave theory couldn't explain, and which Einstein's photon picture resolved).
Step-by-Step Solution
- Photon energy at λ=300 nm: E=3001240≈4.13 eV.
- Compare to work functions: Mg =3.7 eV <4.13 eV → emission occurs.
- Cu =4.8 eV >4.13 eV → no emission.
- Ag =4.3 eV >4.13 eV → no emission (photon energy falls just short).
- Li =2.5 eV <4.13 eV → emission occurs.
- So photoelectric effect occurs only for Mg and Li.
Common Mistakes
- Missing that Ag's work function (4.3 eV), though close, is still above the photon energy (4.13 eV), so no emission happens there.
- Assuming higher work function metals are "easier" to ionize — it's the opposite; lower work function metals emit more easily.
✓Final answerThe correct option is (D) — Mg, Li.
ANSWER: D
- AP EAPCET 2026Set eng-2026-05-14-AN1 markMCQQ.In a photoelectric effect, the kinetic energy of electrons is 1.3×10−19 J. If work function of the metal is 2.27 eV, then the frequency (in Hz) of the incident radiation is (h=6.6×10−34 Js, 1 eV=1.6×10−19 J) (A) 7.47×1015 (B) 7.47×1014 (C) 6.47×1015 (D) 3.47×1014
›Reveal solutionSolution
A direct application of Einstein's photoelectric equation to find the frequency of incident radiation from the given kinetic energy and work function.
Concept and Intuition
Einstein's photoelectric equation states that the energy of an incident photon is split between overcoming the work function (the minimum energy needed to free an electron from the metal) and giving the emitted electron kinetic energy: hν=KEmax+ϕ. Since KE is given in joules and ϕ in eV, we must convert everything to the same unit (joules) before adding.
Step-by-Step Solution
- Convert work function to joules: ϕ=2.27eV×1.6×10−19J/eV=3.632×10−19 J.
- Total photon energy: hν=KE+ϕ=1.3×10−19+3.632×10−19=4.932×10−19 J.
- Frequency: ν=hhν=6.6×10−344.932×10−19≈0.7473×1015=7.47×1014 Hz.
Common Mistakes
- Forgetting to convert the work function from eV to joules before adding to KE (which is already given in joules).
- Misplacing the power of ten when dividing (giving 1015 instead of the correct 1014).
✓Final answerThe correct option is (B) — 7.47×1014 Hz.
ANSWER: B
- AP EAPCET 2026Set eng-2026-05-15-FN1 markMCQQ.The threshold frequency of a metal is 1.15×1015 Hz. If electrons with kinetic energy of 0.20 eV are ejected when this metal surface is irradiated with photons of frequency 'v', the value of v is (h = 6.60×10−34 Js, 1 eV = 1.6×10−19 J) (A) 1.20×1014 Hz (B) 1.20×1015 Hz (C) 1.98×1014 Hz (D) 1.98×1015 Hz
›Reveal solutionSolution
Einstein's photoelectric equation, solved for the incident frequency given the threshold frequency and the photoelectron kinetic energy, gives ν≈1.20×1015 Hz. Answer: (B).
Concept and Intuition
The photoelectric equation KEmax=hν−hν0 says the photon's energy above the threshold (work-function) energy directly becomes the electron's kinetic energy. Converting the given kinetic energy from eV to joules and dividing by h gives the extra frequency needed above threshold.
Step-by-Step Solution
- Convert KE=0.20 eV to joules: KE=0.20×1.6×10−19=3.2×10−20 J.
- Photoelectric equation: hν=hν0+KE⇒ν=ν0+hKE.
- Compute hKE=6.60×10−343.2×10−20=0.4848×1014=4.848×1013 Hz.
- Add to threshold: ν=1.15×1015+0.04848×1015=1.1985×1015≈1.20×1015 Hz.
Common Mistakes
- Forgetting to convert eV to joules before dividing by h (which is in SI units), leading to an answer off by a factor of 1.6×10−19.
- Misplacing a decimal/power-of-ten when adding the small correction term (∼1013) to the threshold term (∼1015).
✓Final answerThe correct option is (B) — 1.20×1015 Hz.
ANSWER: B
- AP EAPCET 2026Set eng-2026-05-18-FN1 markMCQQ.Threshold frequencies of the metals A, B respectively are 4×1014 Hz and 6×1014 Hz. If both are irradiated with light of frequency 1015 Hz, what is the ratio of the kinetic energy of electrons emitted from A and B? (A) 2:3 (B) 3:2 (C) 4:9 (D) 9:4
›Reveal solutionSolution
Einstein's photoelectric equation gives KE=hν−hν0; computing this for both metals gives a ratio of 3:2.
Concept and Intuition
Each metal has its own threshold frequency ν0 — the minimum frequency needed to just eject an electron with zero kinetic energy. Any extra energy in the incident photon beyond hν0 appears entirely as the photoelectron's kinetic energy: KE=hν−hν0. A metal with a lower threshold frequency "uses up" less energy freeing the electron, so more energy is left over as kinetic energy.
Step-by-Step Solution
- Given ν0A=4×1014 Hz, ν0B=6×1014 Hz, incident ν=1015 Hz =10×1014 Hz.
- KEA=h(ν−ν0A)=h(10−4)×1014=6×1014h.
- KEB=h(ν−ν0B)=h(10−6)×1014=4×1014h.
- Ratio KEA:KEB=6:4=3:2.
Common Mistakes
- Taking the ratio of threshold frequencies instead of the ratio of the differences (ν−ν0).
- Inverting the ratio (computing KEB:KEA instead of KEA:KEB).
✓Final answerThe correct option is (B) — 3:2.
ANSWER: B
- AP EAPCET 2026Set ap-2026-05-19-FN1 markMCQQ.A photon of energy 12.09 eV is absorbed by a hydrogen atom in its first excited state, resulting in the ejection of an electron. The kinetic energy (in J) of the emitted photoelectron is (1 eV = 1.6×10−19 J, RH=13.6 eV) (A) 3.02×10−19 (B) 1.39×10−18 (C) 1.93×10−18 (D) 2.15×10−19
›Reveal solutionSolution
This is a photoelectric-effect-style calculation applied to a hydrogen atom: KE of the ejected electron equals photon energy minus the binding energy of the orbit it was ejected from.
Concept and Intuition
An electron in the n=2 state of hydrogen is bound with energy ∣E2∣=13.6/n2=13.6/4=3.4 eV — the minimum energy needed to just free it (ionize it) from that orbit. Any additional photon energy beyond this threshold appears as the electron's kinetic energy after ejection, exactly like Einstein's photoelectric equation but with the "work function" replaced by the orbit's binding energy.
Step-by-Step Solution
- Energy of hydrogen atom in n=2: E2=−2213.6=−3.4 eV, so the ionisation energy from this state is 3.4 eV.
- Photon energy supplied =12.09 eV.
- Kinetic energy of ejected electron =12.09−3.4=8.69 eV.
- Convert to joules: 8.69×1.6×10−19=1.390×10−18 J.
Common Mistakes
- Using the ground-state ionisation energy (13.6 eV) instead of the first-excited-state value (3.4 eV).
- Forgetting to convert eV to joules at the end.
✓Final answerThe correct option is (B) — 1.39×10−18 J.
ANSWER: B
- AP EAPCET 2025Set eng-2025-05-21-FN1 markMCQQ.When a metal surface is irradiated with light of frequency x Hz, the kinetic energy of emitted photoelectrons is z J. When the same metal is irradiated with light of frequency y Hz, the kinetic energy of emitted electrons is 3z J. What is the threshold frequency (in Hz) of metal? (A) 23(y−x) (B) (23y−x) (C) (32y−x) (D) 32(y−x)
›Reveal solutionSolution
Applying Einstein's photoelectric equation to two frequency/KE data pairs and eliminating the unknown z gives the threshold frequency ν0=23y−x.
Concept and Intuition
Einstein's photoelectric equation states that the kinetic energy of an emitted photoelectron equals the incident photon energy minus the work function: KE=hν−hν0, where ν0 is the threshold frequency. Given two experiments at frequencies x and y with corresponding kinetic energies z and z/3, we can eliminate z to solve directly for ν0.
Step-by-Step Solution
- At frequency x: z=h(x−ν0) … (i)
- At frequency y: 3z=h(y−ν0), i.e. z=3h(y−ν0) … (ii)
- Equating (i) and (ii): h(x−ν0)=3h(y−ν0)
- Divide by h: x−ν0=3y−3ν0
- Rearranging: 2ν0=3y−x
- So: ν0=23y−x
Common Mistakes
- Sign errors when moving ν0 terms across the equation.
- Forgetting that z/3 multiplied by 3 gives z again — mixing up which side the factor of 3 goes on.
✓Final answerThe correct option is (B) — (23y−x).
ANSWER: B
- AP EAPCET 2025Set eng-2025-05-24-FN1 markMCQQ.The work functions (in eV) of Mg, Cu, Ag, Na respectively are 3.7, 4.8, 4.3, 2.3. From how many metals, the electrons will be ejected if their surfaces are irradiated with an electromagnetic radiation of wavelength 300 nm? (h=6.6×10−34 Js, 1 eV=1.6×10−19 J) (A) 1 (B) 4 (C) 2 (D) 3
›Reveal solutionSolution
Tests the photoelectric threshold condition hf>ϕ0 across several metals; only Mg and Na (2 metals) qualify.
Concept and Intuition
Photoemission from a metal surface occurs only if the incident photon's energy exceeds that metal's work function. So the first step is finding the photon energy for the given radiation, then simply comparing it against each listed work function.
Step-by-Step Solution
- Photon energy: E=λhc=300×10−9(6.6×10−34)(3×108)=6.6×10−19 J.
- Convert to eV: E=1.6×10−196.6×10−19=4.125 eV.
- Compare with each work function: Mg =3.7 eV <4.125 eV → ejected; Cu =4.8 eV >4.125 eV → not ejected; Ag =4.3 eV >4.125 eV → not ejected; Na =2.3 eV <4.125 eV → ejected.
- Count of metals from which electrons are ejected: Mg and Na → 2.
Common Mistakes
- Forgetting to convert the photon energy from joules to eV before comparing.
- Using the wrong speed of light or forgetting the 10−9 in the wavelength conversion.
✓Final answerThe correct option is (C) — 2.
ANSWER: C
- AP EAPCET 2025Set eng-2025-05-26-AN1 markMCQQ.a, b, c, d are electromagnetic radiations. Frequencies of a, b are 3×1015 Hz, 2×1014 Hz, respectively, whereas wavelength of c, d are 400 nm, 750 nm, respectively. The increasing order of their energies is (A) b, d, c, a (B) a, d, c, b (C) a, b, c, d (D) b, c, d, a
›Reveal solutionSolution
Photon energy is directly proportional to frequency (E=hf=hc/λ); converting all four radiations to a common frequency scale and ordering them gives b, d, c, a.
Concept and Intuition
All electromagnetic radiations obey E=hf=λhc — higher frequency (or shorter wavelength) always means higher photon energy. To compare radiations given in mixed units (some by frequency, some by wavelength), convert everything to the same quantity — here, frequency — using f=c/λ.
Step-by-Step Solution
- Given directly: fa=3×1015 Hz, fb=2×1014 Hz.
- Convert c's wavelength to frequency: fc=λcc=400×10−93×108=7.5×1014 Hz.
- Convert d's wavelength to frequency: fd=λdc=750×10−93×108=4×1014 Hz.
- Now order all four frequencies from smallest to largest: fb(2×1014)<fd(4×1014)<fc(7.5×1014)<fa(3×1015).
- Since energy increases with frequency, the increasing-energy order is the same: b, d, c, a.
Common Mistakes
- Ordering by wavelength directly without converting to a common basis (mixing wavelength and frequency comparisons leads to wrong order).
- Forgetting that larger wavelength means smaller frequency/energy (an inverse relationship), which could flip the order of c and d if handled carelessly.
✓Final answerThe correct option is (A) — b, d, c, a.
ANSWER: A
- AP EAPCET 2025Set eng-2025-05-26-FN1 markMCQQ.The work function of Cu is 7.68×10−19 J. If photons of wavelength 221 nm are made to strike the surface of the metal, the kinetic energy (in J) of the ejected electrons will be (h=6.63×10−34 Js) (A) 2.64×10−18 (B) 1.32×10−19 (C) 2.64×10−19 (D) 6.60×10−19
›Reveal solutionSolution
Einstein's photoelectric equation says the ejected electron's kinetic energy is the photon energy minus the metal's work function; computing hc/λ for 221 nm and subtracting ϕ=7.68×10−19 J gives 1.32×10−19 J.
Concept and Intuition
When light of energy greater than the work function strikes a metal, each absorbed photon can eject one electron. The work function ϕ is the minimum energy needed just to free an electron from the metal surface; any extra photon energy beyond that becomes the electron's kinetic energy. This is Einstein's photoelectric equation: KEmax=hν−ϕ=λhc−ϕ.
Step-by-Step Solution
- Compute photon energy: E=λhc=221×10−9(6.63×10−34)(3×108).
- Numerator: 6.63×10−34×3×108=1.989×10−25J⋅m.
- Divide: 2.21×10−71.989×10−25=9.00×10−19J.
- Apply Einstein's equation: KE=E−ϕ=9.00×10−19−7.68×10−19=1.32×10−19J.
Common Mistakes
- Using λ in nm directly instead of converting to metres, which throws off the exponent by a factor of 109.
- Adding ϕ instead of subtracting it, or subtracting in the wrong order.
✓Final answerThe correct option is (B) — 1.32×10−19.
ANSWER: B
- AP EAPCET 2024Set ap-2024-05-16-FN1 markMCQQ.A spectral line in hydrogen spectrum is due to electron transition between energy levels whose sum and difference are respectively 5 and 3. The wavelength of it (in cm) is (R = Rydberg constant in cm−1) (A) 15R16 (B) 16R15 (C) 1516R (D) 1615R
›Reveal solutionSolution
The sum and difference of the two quantum numbers pin down the transition as n=4→n=1, giving wavelength λ=15R16 cm.
Concept and Intuition
Any hydrogen spectral line is characterised by the two principal quantum numbers of the levels involved. Given their sum and difference, the individual quantum numbers can be recovered by solving simultaneous equations, after which the Rydberg formula gives the wavelength directly.
Step-by-Step Solution
- Let the two levels be n1 (lower) and n2 (upper), with n1+n2=5 and n2−n1=3.
- Adding: 2n2=8⇒n2=4. Subtracting: 2n1=2⇒n1=1.
- So the transition is n=4→n=1 (a Lyman-series line).
- Rydberg formula: λ1=R(n121−n221)=R(1−161)=R⋅1615.
- Therefore λ=15R16 cm.
Common Mistakes
- Swapping which quantum number is n1 vs n2, which would invert the fraction inside the Rydberg formula.
- Arithmetic slip solving the sum/difference simultaneous equations.
✓Final answerThe correct option is (A) — 15R16.
ANSWER: A
- AP EAPCET 2024Set ap-2024-05-16-FN1 markMCQQ.A light of frequency x Hz when falls on a metal plate emits electrons that have double the kinetic energy compared to kinetic energy of emitted electrons when light of frequency y Hz falls on the same plate. The threshold frequency of the metal in Hz is (A) y−x (B) x−y (C) x−2y (D) 2y−x
›Reveal solutionSolution
Writing Einstein's photoelectric equation for both frequencies and using the given ratio of kinetic energies isolates the threshold frequency as ν0=2y−x.
Concept and Intuition
The maximum kinetic energy of a photoelectron is KE=h(ν−ν0), linear in the incident frequency ν, with the threshold frequency ν0 as the frequency-intercept. Given kinetic energies at two different frequencies (and their ratio), we get two linear equations that can be solved for ν0.
Step-by-Step Solution
- At frequency x: KEx=h(x−ν0).
- At frequency y: KEy=h(y−ν0).
- Given KEx=2KEy: h(x−ν0)=2h(y−ν0).
- Divide by h and expand: x−ν0=2y−2ν0.
- Rearranging: 2ν0−ν0=2y−x⇒ν0=2y−x.
Common Mistakes
- Losing track of which frequency (x or y) corresponds to the doubled kinetic energy when setting up the equation.
- Sign errors when moving ν0 terms across the equation.
✓Final answerThe correct option is (D) — 2y−x.
ANSWER: D
- AP EAPCET 2024Set eng-2024-05-21-AN1 markMCQQ.If λ0 and λ are respectively the threshold wavelength and wavelength of incident light, the velocity of photo electrons ejected from the metal surface is (A) m2h(λ0−λ) (B) m2hc(λλ0λ0−λ) (C) m2hc(λ0−λ) (D) m2h(λ01−λ1)
›Reveal solutionSolution
Combine Einstein's photoelectric equation with the kinetic-energy definition and solve algebraically for v. Answer: option (B).
Concept and Intuition
Einstein's photoelectric equation states the photon energy equals the work function plus the electron's maximum kinetic energy: λhc=λ0hc+21mv2 (since the work function W=hc/λ0). Solving for v requires combining the two reciprocal wavelength terms over a common denominator.
Step-by-Step Solution
- 21mv2=λhc−λ0hc=hc(λ1−λ01).
- Combine over a common denominator: λ1−λ01=λλ0λ0−λ.
- So 21mv2=hc⋅λλ0λ0−λ.
- v=m2hc(λλ0λ0−λ).
Common Mistakes
- Forgetting the factor of c when converting from 1/λ terms to energy (energy is hc/λ, not h/λ).
- Leaving the expression as separate 1/λ and 1/λ0 terms without combining them, which doesn't match the algebraically simplified answer choice.
✓Final answerThe correct option is (B) — m2hc(λλ0λ0−λ).
ANSWER: B
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