Q.Consider a beam of electrons (each electron with energy E0) incident on a metal surface kept in an evacuated chamber. Then
Concept understanding — Photoelectric Effect
The Photoelectric Effect: When Light Knocks Electrons Loose
Imagine you're throwing tennis balls at a wall covered in loose pebbles. If you throw hard enough, a pebble might get knocked off. That's the basic picture — but the photoelectric effect is the quantum version of this, and it completely shattered classical physics.
The Intuition
Light is made of tiny packets of energy called photons. Each photon carries a specific amount of energy, determined by its colour (frequency). When a photon hits a metal surface, it can transfer its energy to an electron inside the metal. If that energy is enough, the electron breaks free and flies out.
Think of electrons in a metal like people in a room with a high window. To escape, they need enough energy to reach the window sill. A photon is like a boost — but only if it gives enough energy in one shot. No amount of weak boosts (dim light) will work if each individual boost is too small.
The Precise Statement
Ephoton=hf=ϕ+Kmax
Where:
- Ephoton=hf is the energy of a photon (Planck's constant h=6.63×10−34 J⋅s, f is frequency)
- ϕ is the work function — the minimum energy needed to remove an electron from that metal
- Kmax is the maximum kinetic energy of the ejected electron
What Classical Physics Got Wrong
Before Einstein (1905), physicists thought light was a continuous wave. They expected:
- Brighter light → more energy per electron → faster electrons
- Any colour would eventually eject electrons if you waited long enough
But experiments showed the opposite:
| Observation | Classical Prediction | Actual Result |
|---|---|---|
| Effect of intensity | Brighter light → faster electrons | Brighter light → more electrons, same speed |
| Threshold frequency | None — any light works eventually | Below a certain frequency, no electrons no matter how bright |
| Time delay | Electrons need time to absorb energy | Electrons appear instantly (within 10−9 s) |
The Key Insight
Einstein said: light behaves like a stream of particles (photons), each with energy hf. One photon interacts with one electron. If hf<ϕ, the electron cannot escape — period. If hf>ϕ, the excess energy becomes kinetic energy:
Kmax=hf−ϕ
This is why:
- Increasing intensity (more photons) ejects more electrons, but each electron still gets the same energy per photon — so their speed doesn't change.
- Below threshold frequency, even a trillion photons per second can't help — each one is too weak individually.
The photoelectric effect proved that light is quantized — it comes in discrete packets. This was the birth of quantum mechanics. Einstein won the 1921 Nobel Prize for this, not for relativity.
A Worked Example
Problem: A metal has work function ϕ=2.0 eV. Light of frequency f=6.0×1014 Hz shines on it. Find the maximum kinetic energy of ejected electrons. (h=4.14×10−15 eV⋅s)
Step 1: Photon energy
E=hf=(4.14×10−15)(6.0×1014)=2.48 eV
Step 2: Subtract work function
Kmax=2.48−2.0=0.48 eV
Step 3: Convert to joules if needed
0.48 eV×1.6×10−19=7.68×10−20 J
The electron escapes with this much kinetic energy.
Common Mistake to Avoid
Students often think "more intense light means more energy per electron." Wrong. Intensity = number of photons per second. Each photon still has the same hf. More photons = more electrons, but each electron gets the same energy kick.
The Big Picture
The photoelectric effect is your first encounter with wave-particle duality. Light, which we model as a wave for interference and diffraction, behaves as a particle when transferring energy to matter. This duality is central to all of quantum mechanics.
Final takeaway: Light ejects electrons only if each photon carries enough energy individually. The colour (frequency) determines whether ejection happens; the brightness (intensity) determines how many electrons get ejected.
"Photoelectric effect formula and Einstein equation" is among the most-searched Class 12 physics topics, and it is a core result of the Dual Nature of Radiation and Matter chapter in the NCERT/CBSE Class 12 Physics curriculum. Work function and threshold frequency questions built on this concept appear in nearly every JEE Main and NEET physics paper.
Why this formula?
Photoelectric Effect: Why the Key Formulas Hold
The photoelectric effect is a cornerstone of quantum physics. It showed that light behaves as particles (photons) , not just waves. Let's build the reasoning step-by-step.
1. The Core Idea: Energy Conservation
When a photon hits a metal surface, it transfers all its energy to a single electron inside the metal.
- The photon's energy is E=hf, where h is Planck's constant and f is the frequency of light.
- The electron needs a minimum energy to escape the metal — this is called the work function, ϕ.
Why only one electron?
Einstein proposed that light is quantized into discrete packets (photons). A single photon cannot split its energy among multiple electrons — it interacts with one electron at a time.
2. The Photoelectric Equation
If the photon's energy is greater than the work function, the excess energy becomes the electron's kinetic energy after escape:
hf=ϕ+Kmax
Where:
- hf = energy of incident photon
- ϕ = work function (minimum energy to remove electron)
- Kmax = maximum kinetic energy of ejected electron
Why "maximum" kinetic energy?
- Electrons inside the metal have different binding energies.
- Some electrons are near the surface (loosely bound) → get maximum K.
- Others are deeper → lose energy in collisions before escaping → lower K.
3. The Stopping Potential Connection
We measure Kmax using a stopping potential Vs:
Kmax=eVs
Where e is the electron charge. This is because:
- An electric field opposing the electron's motion does work eVs to stop it.
- At the stopping potential, the electron's kinetic energy is exactly balanced by the electric potential energy.
Combining:
hf=ϕ+eVs
This is the Einstein photoelectric equation in its most testable form.
4. Why the Threshold Frequency Exists
From the equation:
hf=ϕ+eVs
If f is too low, hf<ϕ. Then:
- The photon cannot supply enough energy to overcome the work function.
- No electron is ejected, regardless of light intensity.
The threshold frequency f0 is when Kmax=0:
hf0=ϕ⇒f0=hϕ
Why intensity doesn't matter for ejection?
- Intensity = number of photons per second.
- Each photon still has energy hf. If hf<ϕ, even a billion photons won't eject an electron — each photon is individually too weak.
5. Why Kinetic Energy Depends on Frequency, Not Intensity
From Kmax=hf−ϕ:
- Frequency f directly determines Kmax.
- Intensity only affects the number of electrons ejected (more photons → more electrons), not their individual energy.
This was the key experimental contradiction with classical wave theory:
- Classical: Higher intensity = bigger wave amplitude = more energy to electrons.
- Reality: Higher frequency = more energy per electron; intensity only changes current.
6. Summary of Key Relationships
| Quantity | Formula | Why it holds |
|---|---|---|
| Photon energy | E=hf | Light is quantized (Planck-Einstein) |
| Work function | ϕ=hf0 | Minimum energy to escape at threshold |
| Max kinetic energy | Kmax=hf−ϕ | Energy conservation per photon-electron |
| Stopping potential | eVs=hf−ϕ | Electric work balances kinetic energy |
| Threshold frequency | f0=ϕ/h | Below this, no ejection possible |
7. The Deeper "Why" — Particle Nature of Light
The photoelectric effect cannot be explained by classical wave theory because:
- Waves spread energy over the whole wavefront — an electron would take time to absorb enough energy.
- But experiments show instantaneous ejection (within 10−9 s).
- Wave theory predicts kinetic energy should increase with intensity — it doesn't.
Einstein's photon model resolves all three:
- Instantaneous — one photon, one interaction.
- Frequency-dependent — photon energy is hf.
- Intensity-independent — more photons = more electrons, not more energy per electron.
Key takeaway: The photoelectric effect is a direct consequence of energy quantization — both light and electron binding energy are quantized. The formulas are simply conservation laws applied to this quantum world.
Concept: Photoelectric effect vs. electron-impact (secondary) emission.
A photon is not the only particle that can eject a bound electron. An incident electron of kinetic energy E0 can also knock electrons out of the metal by collision (secondary emission). In such a collision the incident electron may hand over any fraction of its energy, from almost none up to nearly all of E0. The freed electron must still spend the work function ϕ to leave the surface, so the largest kinetic energy it can carry away is E0−ϕ.
Hence electrons are emitted with a range of energies, up to a maximum of E0−ϕ.
The correct option is (C): electrons can be emitted with any energy, with a maximum of E0−ϕ.
An incident electron beam ejects electrons by collision (secondary emission); the freed electrons come out with a spread of energies whose maximum is E0−ϕ — option (C).
Setting up the physics
The photoelectric effect is the ejection of electrons by photons, but this question is different: the metal is bombarded by a beam of electrons, each of energy E0. Electrons are charged particles and interact with the metal's electrons through the Coulomb force, so an incident electron can transfer energy to a bound electron in a collision and knock it out. This is secondary electron emission — a real, well-known process (it is exactly what multiplies the signal on the dynodes of a photomultiplier).
How much energy can an ejected electron have?
- Energy available. The incident electron brings kinetic energy E0.
- Energy that must be paid. To escape the metal, the freed electron must spend at least the work function ϕ.
- The transfer is not fixed. In a collision the incident electron can give up any fraction of its energy — a glancing hit transfers little, a head-on hit transfers a lot. So the freed electron can emerge with kinetic energy anywhere from 0 up to a maximum.
- The maximum. The most the ejected electron can retain is the incident energy minus the escape cost:
Kmax=E0−ϕ.
So the emitted electrons are not mono-energetic; they form a continuous distribution up to E0−ϕ.
Why the other options fail
- (A) "No electrons emitted" is wrong: an energetic electron beam does eject electrons by collision.
- (B) "All with energy E0" is wrong: the incident electron loses part of its energy in the collision, and the escaping electron also pays ϕ.
- (D) "Maximum of E0" ignores the work function that must be spent to leave the surface.
The correct option is (C): electrons can be emitted with any energy, with a maximum of E0−ϕ.
Method: Distinguishing Emission Mechanisms — Photon Absorption vs Particle-Impact Collision
Use this reasoning pattern whenever a question describes electrons being knocked out of a metal by something other than a beam of light, and asks you to compare it with the ordinary photoelectric effect.
Steps
Step 1: Check what is actually incident on the metal
The photoelectric equation Ephoton=hf=ϕ+Kmax applies strictly to photon absorption — one photon, one electron, all-or-nothing. If the question instead describes a beam of charged particles (electrons, in this case) hitting the surface, that equation does not apply as written; you're dealing with a collision process instead.
Step 2: Recognise that a particle collision can transfer any fraction of energy
Unlike a photon (which either transfers all its energy or none), an incident particle interacting via a real physical collision can hand over anywhere from a small fraction to nearly all of its kinetic energy, depending on the geometry of the collision (glancing vs head-on). This means the freed electrons will not be mono-energetic — they emerge with a spread of energies.
Step 3: Find the maximum by subtracting the fixed escape cost once
Whatever the mechanism of energy transfer, an electron still has to pay the same fixed price — the work function ϕ — to leave the metal surface. So the maximum possible kinetic energy of an emitted electron is always
Kmax=(energy available to the electron)−ϕ
Here the energy available is the full incident energy E0 of the electron doing the knocking, so Kmax=E0−ϕ.
Step 4: Rule out options that violate either principle
Check every option against the two principles above: an option claiming "no emission" ignores that particle collisions do transfer energy; an option claiming a single fixed energy ignores that collisions transfer a variable amount; an option that forgets to subtract ϕ ignores that escape always has a cost.
Showing the 12 most recent of 16 on this concept.
- TG EAPCET 2026Set eng-2026-05-11-AN1 markMCQQ.A potentiometer wire of length 10 m and resistance 9 Ω is connected to a cell of emf E and internal resistance 1 Ω. If V is the maximum potential difference that can be measured using the potentiometer, then the condition for the potentiometer to work is (A) E=V (B) 9E≥10V (C) E<V (D) 9V=10E
›Reveal solutionSolution
The key idea is that a potentiometer works only when the voltage across its entire wire (the maximum measurable voltage) is slightly greater than the voltage to be measured. Here, the maximum potential difference across the wire is 109E, so the condition for it to measure a voltage V is 9E≥10V, which corresponds to option (B).
Why this approach works
A potentiometer is a device for measuring an unknown potential difference without drawing current from the source being measured. It works by balancing the unknown voltage against a known potential difference taken from a uniform wire. For the potentiometer to function, the unknown voltage V must be less than or equal to the maximum potential difference that can be obtained across the entire length of the wire. If V exceeds that maximum, the balance point cannot be reached — the slider would have to go beyond the wire.
So the problem reduces to: What is the maximum voltage across the potentiometer wire? That depends on the driving cell's emf E, its internal resistance, and the wire's resistance.
Step-by-step reasoning
- Find the current in the main circuit The potentiometer wire (resistance 9Ω) is connected in series with the driving cell (emf E, internal resistance 1Ω). The total resistance in the circuit is
Rtotal=9+1=10Ω.
Hence the current supplied by the cell is
I=10E.
- Find the potential difference across the whole wire The wire has resistance 9Ω, so the voltage drop from one end to the other is
Vwire=I×9=10E×9=109E.
This is the maximum voltage that can be tapped from the wire (by using its full length).
- Condition for the potentiometer to work The potentiometer can measure any voltage V that is less than or equal to this maximum. If V is larger, no balance point exists on the wire. Therefore we require
V≤109E.
Rearranging:
9E≥10V.
- Match with the options The inequality 9E≥10V is exactly option (B).
Watch outA common mistake is to forget the internal resistance of the driving cell. If you treat the cell as ideal (zero internal resistance), the current would be E/9 and the wire voltage would be E, leading to the wrong condition E≥V (option A). But the internal resistance is given as 1Ω and must be included.
TipNotice that the wire length (10 m) is not needed for the calculation — it only tells us the wire is uniform. The maximum measurable voltage depends only on the resistances and the driving emf.
✓Final answerThe correct option is (B).
ANSWER: B
- TG EAPCET 2026Set ap-2026-05-05-FN1 markMCQQ.A potentiometer wire of length 4 m and resistance 20 Ω is connected in series to a resistor of resistance 28 Ω. If the emf of the cell is 5 V and its internal resistance is 2 Ω, then the maximum potential difference that the potentiometer can measure is (A) 4 V (B) 3 V (C) 2 V (D) 5 V
›Reveal solutionSolution
The maximum potential difference a potentiometer can measure is the potential drop across its entire wire. By calculating the total current in the primary circuit and then the potential drop across the potentiometer wire, we find this maximum measurable potential difference to be 2 V.
A potentiometer is a device used to measure an unknown electromotive force (EMF) or potential difference accurately. Its core principle relies on the concept of a uniform potential gradient along a wire.
The primary circuit of a potentiometer consists of a cell (driver cell), a rheostat (or a fixed series resistor), and the potentiometer wire itself, all connected in series. A constant current flows through this primary circuit, establishing a potential drop across the potentiometer wire. This potential drop is distributed uniformly along the length of the wire, meaning there's a constant potential difference per unit length, known as the potential gradient.
The maximum potential difference that a potentiometer can measure is limited by the total potential drop across its entire wire. If you try to measure a potential difference greater than this, you won't be able to find a null point on the wire. Therefore, to find the maximum measurable potential difference, we need to calculate the potential difference across the potentiometer wire when the primary circuit is operational.
Here's how to calculate it:
- Calculate the total resistance of the primary circuit. The primary circuit consists of the potentiometer wire, the external series resistor, and the internal resistance of the driving cell, all connected in series. Let Rp be the resistance of the potentiometer wire, Rext be the external series resistor, and r be the internal resistance of the cell. The total resistance Rtotal is:
Rtotal=Rp+Rext+r
Given $R_p = 20~\Omega$, $R_{ext} = 28~\Omega$, and $r = 2~\Omega$.Rtotal=20 Ω+28 Ω+2 Ω=50 Ω
- Calculate the current flowing through the primary circuit. The current I in the primary circuit is determined by the EMF of the driving cell (E) and the total resistance of the circuit. Using Ohm's Law:
I=RtotalE
Given $\mathcal{E} = 5~\mathrm{V}$.I=50 Ω5 V=0.1 A
- Calculate the potential difference across the potentiometer wire. The potential difference Vp across the potentiometer wire is the product of the current flowing through it and its resistance.
Vp=I×Rp
Using the values calculated:Vp=0.1 A×20 Ω=2 V
- Determine the maximum measurable potential difference. The potential difference across the entire length of the potentiometer wire is the maximum potential difference that the potentiometer can measure. Any unknown potential difference greater than this value cannot be balanced on the wire. Therefore, the maximum potential difference the potentiometer can measure is Vp=2 V.
Watch outDo not confuse the EMF of the driving cell with the maximum potential difference the potentiometer can measure. The EMF of the driving cell is 5 V, but due to the voltage drops across the external series resistor and the internal resistance of the cell, the potential drop available across the potentiometer wire itself is less than the cell's EMF.
✓Final answerThe maximum potential difference that the potentiometer can measure is 2 V.
- TG EAPCET 2026Set ap-2026-05-05-FN1 markMCQQ.When monochromatic photons incident on a photosensitive material of cut-off wavelength 496 nm, photoelectrons are emitted with a maximum velocity of 8×105 ms−1. Then the energy of the incident photons is nearly (Mass of the electron =9×10−31 kg and charge of the electron =1.6×10−19 C) (A) 6.1 eV (B) 3.7 eV (C) 4.3 eV (D) 5.2 eV
›Reveal solutionSolution
Use the photoelectric equation: the incident photon energy equals the work function plus the maximum kinetic energy of the emitted electron. The work function is found from the cut-off wavelength. The result is about 4.3 eV, option (C).
The photoelectric effect is a clean example of energy conservation at the quantum level. A single photon gives all its energy to one electron. Part of that energy is used to overcome the binding force that holds the electron in the metal — that's the work function. The rest appears as the electron's kinetic energy. The cut-off wavelength tells you the minimum photon energy needed to just barely eject an electron (with zero kinetic energy), so it directly gives the work function.
Here, you're given the cut-off wavelength (496 nm) and the maximum speed of the emitted electrons (8×105 m/s). The mass of the electron is also provided. The plan is straightforward: find the work function from the cut-off wavelength, find the maximum kinetic energy from the speed, and add them to get the incident photon energy. Then convert everything to electronvolts (eV) to match the options.
- Find the work function from the cut-off wavelength. The cut-off wavelength λ0=496 nm is the longest wavelength that can still cause emission. At this wavelength, the photon energy exactly equals the work function ϕ (since the electron gets zero kinetic energy).
ϕ=λ0hc
Use hc=1240 eV·nm (a very handy constant for such problems).
ϕ=496 nm1240 eV⋅nm=2.5 eV
- Find the maximum kinetic energy of the photoelectrons. The maximum speed v=8×105 m/s. The kinetic energy is
Kmax=21mv2
with m=9×10−31 kg.
Kmax=21×(9×10−31)×(8×105)2
First compute v2=64×1010=6.4×1011 m²/s².
Then
Kmax=21×9×10−31×6.4×1011=21×57.6×10−20=28.8×10−20 J
Convert to eV using 1 eV=1.6×10−19 J:
Kmax=1.6×10−1928.8×10−20=1628.8=1.8 eV
- Add to get the incident photon energy. Einstein's photoelectric equation:
Ephoton=ϕ+Kmax
So
Ephoton=2.5 eV+1.8 eV=4.3 eV
Watch outA common slip is to forget converting the kinetic energy from joules to eV. Always check the units — the work function came out in eV directly from the hc shortcut, so the kinetic energy must also be in eV before adding.
TipMemorising hc=1240 eV·nm saves time and reduces errors. For any wavelength in nanometres, dividing 1240 by that wavelength gives the photon energy in eV instantly.
✓Final answerThe energy of the incident photons is nearly 4.3 eV, which corresponds to option (C).
- TG EAPCET 2025Set eng-2025-05-02-FN1 markMCQQ.As shown in the figure, a dielectric of constant K is placed between the plates of a parallel plate capacitor and is charged to a potential V using a battery. If the dielectric is pulled out after disconnecting the battery from the capacitor, the final potential difference across the plates of the capacitor is (A) (1+K1)2V (B) 2KV (C) (1+K1)2V (D) 2V(1+K1)
›Reveal solutionSolution
Charge is conserved once the battery is disconnected. With the dielectric slab shown occupying half the plate separation, the initial capacitance is a series combination of a dielectric-filled half-gap and a vacuum half-gap; once the dielectric is pulled out and the full gap is vacuum, working through Q=CiV=CfVf gives Vf=1+K12V, option (C).
Concept and intuition
The key idea is charge conservation after the battery is disconnected: the charge Q on the plates stays fixed no matter what happens to the dielectric afterward. Because the figure shows the dielectric slab filling only half the plate separation (not the whole gap), the capacitor must be modeled as two capacitors in series while it is being charged — one half-gap with the dielectric, one half-gap with vacuum. Once the dielectric is removed, the whole gap becomes vacuum and the capacitance drops to that of a plain parallel-plate capacitor of separation d; since Q is unchanged, V must rise to compensate for the smaller C.
Step-by-step solution
- Initial capacitance (dielectric fills half the gap, thickness d/2) Two capacitors in series, each with the full plate area A but half the separation:
C1=d/2Kε0A=d2Kε0A,C2=d/2ε0A=d2ε0A
Ci1=C11+C21=2ε0Ad(K1+1)⇒Ci=d2ε0A⋅K+1K
- Charge stored while connected to the battery
Q=CiV=d2ε0A⋅K+1K⋅V
- After disconnecting the battery and removing the dielectric The gap is now entirely vacuum, so
Cf=dε0A
Charge is unchanged (no battery connected), so Q=CfVf:
d2ε0A⋅K+1K⋅V=dε0A⋅Vf⇒Vf=K+12KV
- Match to the options
Vf=K+12KV=1+K12V
This is exactly option (C).
Watch outIf the dielectric filled the entire gap, removing it would simply give Vf=KV — but that value isn't among the options, which is the clue that the dielectric only fills half the separation (as shown in the figure), making the series-capacitor treatment necessary.
TipWhenever a dielectric only partially fills the gap between the plates, split the capacitor into a series (partial thickness) or parallel (partial area) combination before applying Q=CV — don't treat it as a single capacitor with an effective dielectric constant unless it fills the whole gap.
✓Final answerThe correct option is (C).
ANSWER: C
- TG EAPCET 2025Set eng-2025-05-02-FN1 markMCQQ.Photons of energy 4.5 eV are incident on a photosensitive material of work function 3 eV. The de Broglie wavelength associated with the photoelectrons emitted with maximum kinetic energy is nearly (A) 10 A˚ (B) 5 A˚ (C) 20 A˚ (D) 15 A˚
›Reveal solutionSolution
Use the photoelectric equation to find the maximum kinetic energy of the emitted electrons, then convert that energy to momentum and apply de Broglie’s relation to get the wavelength. The result is about 8.7 Å, so the closest option is 10 Å — option (A).
The problem combines two classic ideas: the photoelectric effect and the de Broglie wavelength of a particle.
The key insight: the maximum kinetic energy of the photoelectrons comes from the photon energy minus the work function. Once we know that kinetic energy, we can find the electron’s momentum, and then the de Broglie wavelength is simply λ=h/p.
- Find the maximum kinetic energy of the photoelectrons The photoelectric equation:
Kmax=hν−ϕ
Here hν=4.5 eV and ϕ=3 eV.
So
Kmax=4.5−3=1.5 eV.
- Convert kinetic energy to joules Since 1 eV=1.602×10−19 J,
Kmax=1.5×1.602×10−19=2.403×10−19 J.
- Find the momentum of the electron For a non‑relativistic electron (1.5 eV is tiny compared to its rest energy 511 keV),
p=2meKmax.
Electron mass me=9.109×10−31 kg.
p=2×9.109×10−31×2.403×10−19.
First compute the product inside:
2×9.109×10−31×2.403×10−19=4.378×10−49.
Then
p=4.378×10−49=6.617×10−25 kg⋅m/s.
- Apply de Broglie’s relation
λ=ph,
with Planck’s constant h=6.626×10−34 J⋅s.
λ=6.617×10−256.626×10−34=1.001×10−9 m.
- Convert to angstroms 1 A˚=10−10 m, so
λ≈10.01 A˚.
This is very close to 10 Å.
TipA handy shortcut: for an electron with kinetic energy K in eV, the de Broglie wavelength in Å is approximately
λ(A˚)≈K(eV)12.26.
Here 1.5≈1.225, so λ≈12.26/1.225≈10.0 A˚. This avoids all the unit conversions.
Watch outA common mistake is to use the photon’s energy (4.5 eV) directly in the de Broglie formula. But de Broglie wavelength applies to particles with mass, not to photons in this context. Always use the electron’s kinetic energy, not the photon’s.
✓Final answerThe correct option is (A).
ANSWER: A
- TG EAPCET 2024Set ap-2024-05-08-FN1 markMCQQ.If the wavelength of the incident radiation on a photosensitive metal surface is decreased from 3100 A˚ to 1550 A˚, the maximum kinetic energy of the emitted photoelectrons is tripled. The work function of the metal surface is (A) 3 eV (B) 4 eV (C) 2 eV (D) 6 eV
›Reveal solutionSolution
When the wavelength of incident light decreases, the photon energy increases, leading to higher kinetic energy of emitted photoelectrons. By applying Einstein's photoelectric equation for two different wavelengths and using the given relationship between kinetic energies, we find the work function of the metal. The work function is 2 eV.
The problem describes a scenario involving the photoelectric effect, where light incident on a metal surface causes electrons to be ejected. The core concept here is Einstein's photoelectric equation, which relates the energy of the incident photon, the work function of the metal, and the maximum kinetic energy of the emitted photoelectrons.
Concept and Intuition
When light shines on a metal surface, if the photons have sufficient energy, they can eject electrons from the metal. This phenomenon is called the photoelectric effect.
- Photon Energy (E): Light consists of discrete packets of energy called photons. The energy of a single photon is directly proportional to its frequency (ν) and inversely proportional to its wavelength (λ).
E=hν=λhc
where h is Planck's constant and c is the speed of light.
- Work Function (ϕ): This is the minimum energy required to remove an electron from the surface of a particular metal. It's a characteristic property of the metal. Electrons deeper inside the metal require more energy to escape, but the work function refers to the minimum energy for the most loosely bound electrons at the surface.
- Maximum Kinetic Energy (Kmax): When a photon strikes an electron, it transfers its energy. If this energy is greater than the work function, the electron is ejected. Any excess energy beyond the work function is converted into the kinetic energy of the emitted electron. Since the work function is the minimum energy to escape, the maximum kinetic energy is achieved by electrons that require only this minimum energy to escape.
Einstein's photoelectric equation elegantly combines these ideas:
Kmax=E−ϕ=λhc−ϕ
This equation tells us that the maximum kinetic energy of the emitted photoelectron is the energy of the incident photon minus the work function of the metal. If the photon energy is less than the work function, no photoemission occurs, regardless of the intensity of the light.
In this problem, we are given two different wavelengths of incident radiation and the corresponding relationship between the maximum kinetic energies. We can set up two equations based on Einstein's photoelectric equation and then solve them simultaneously to find the unknown work function.
Step-by-step Solution
-
Identify the given information and constants:
- Initial wavelength, λ1=3100 A˚
- Final wavelength, λ2=1550 A˚
- Relationship between maximum kinetic energies: Kmax,2=3Kmax,1
- We need to find the work function, ϕ.
- For calculations involving photon energy, it's convenient to use the product hc. Since the wavelengths are in Angstroms and the options for work function are in electron volts (eV), we use the value hc≈12400 eV⋅A˚.
-
Apply Einstein's photoelectric equation for the first case:
When the wavelength is λ1=3100 A˚, let the maximum kinetic energy be Kmax,1.
The photon energy is E1=λ1hc.
Using Einstein's equation:
Kmax,1=λ1hc−ϕ
Kmax,1=3100 A˚12400 eV⋅A˚−ϕ
Kmax,1=4 eV−ϕ(Equation 1)
-
Apply Einstein's photoelectric equation for the second case:
When the wavelength is λ2=1550 A˚, let the maximum kinetic energy be Kmax,2.
The photon energy is E2=λ2hc.
Using Einstein's equation:
Kmax,2=λ2hc−ϕ
Kmax,2=1550 A˚12400 eV⋅A˚−ϕ
Kmax,2=8 eV−ϕ(Equation 2)
TipNotice that λ2=λ1/2. This means E2=2E1. Halving the wavelength doubles the photon energy. This is a common relationship to quickly calculate photon energies.
-
Use the given relationship between kinetic energies:
We are given that the maximum kinetic energy is tripled when the wavelength is decreased:
Kmax,2=3Kmax,1
-
Substitute Equation 1 and Equation 2 into the relationship from Step 4:
(8 eV−ϕ)=3(4 eV−ϕ)
Now, solve for ϕ:
8 eV−ϕ=12 eV−3ϕ
Rearrange the terms to isolate ϕ:
3ϕ−ϕ=12 eV−8 eV
2ϕ=4 eV
ϕ=24 eV
ϕ=2 eV
The work function of the metal surface is 2 eV.
✓Final answerThe work function of the metal surface is 2 eV.
- Photon Energy (E): Light consists of discrete packets of energy called photons. The energy of a single photon is directly proportional to its frequency (ν) and inversely proportional to its wavelength (λ).
- TG EAPCET 2024Set ap-2024-05-07-FN1 markMCQQ.Two photons of energies 2.5eV and 5.5eV incident on a metal surface of work function 1.5eV. The ratio of the maximum speeds of the photoelectrons emitted from the metal surface is (A) 1:4 (B) 1:2 (C) 1:1 (D) 5:11
›Reveal solutionSolution
The maximum kinetic energy of a photoelectron is the photon energy minus the work function; since kinetic energy scales with speed squared, the ratio of maximum speeds is the square root of the ratio of the excess energies, giving 1:2.
The key concept here is the photoelectric effect: a photon’s energy is used first to overcome the work function (the minimum energy needed to free an electron), and any leftover energy becomes the electron’s kinetic energy. The maximum speed corresponds to the case where no energy is lost to internal collisions, so all excess energy goes into kinetic energy: Kmax=hf−ϕ. Since kinetic energy is 21mv2, the speed is proportional to the square root of the excess energy.
Let’s work through it step by step.
- Write the photoelectric equation For a photon of energy E, the maximum kinetic energy of an emitted electron is
Kmax=E−ϕ,
where ϕ=1.5eV is the work function.
- Compute the excess energies
- For the 2.5eV photon:
K1=2.5−1.5=1.0eV.
- For the 5.5eV photon:
K2=5.5−1.5=4.0eV.
- Relate kinetic energy to speed Since K=21mv2, we have v=m2K. The mass m of the electron is the same for both, so the ratio of maximum speeds is
v2v1=K2K1.
- Plug in the numbers
v2v1=4.01.0=41=21.
Thus the ratio v1:v2=1:2.
Watch outA common mistake is to take the ratio of the photon energies directly (2.5:5.5=5:11) or the ratio of the kinetic energies (1:4) and forget that speed goes as the square root of kinetic energy. Always remember: v∝K.
TipSince the work function is the same for both, the ratio of speeds depends only on the excess energies. You don’t need to convert eV to joules — the units cancel in the ratio.
✓Final answerThe correct option is (B).
ANSWER: B
- TG EAPCET 2024Set eng-2024-05-10-AN1 markMCQQ.The work function of a photosensitive metal surface is 1.1 eV. Two light beams of energies 1.5 eV and 2 eV incident on the metal surface. The ratio of the maximum velocities of the emitted photoelectrons is (A) 3:4 (B) 1:1 (C) 2:3 (D) 4:9
›Reveal solutionSolution
The maximum kinetic energy of a photoelectron is the photon energy minus the work function, and since kinetic energy scales with velocity squared, the ratio of velocities is the square root of the ratio of the excess energies. The correct ratio is 2:3, so option (C).
The key concept here is the photoelectric effect: a photon gives all its energy to an electron, but the electron must first overcome the binding energy (work function ϕ) to escape. The leftover energy becomes kinetic energy. Since kinetic energy K=21mv2, the velocity v is proportional to K. So the ratio of velocities is the square root of the ratio of the kinetic energies, not the photon energies themselves.
Let’s work it through:
- Find the kinetic energy for each photon. For the first beam: photon energy E1=1.5 eV, work function ϕ=1.1 eV. Maximum kinetic energy:
K1=E1−ϕ=1.5−1.1=0.4 eV.
For the second beam: E2=2.0 eV, so
K2=2.0−1.1=0.9 eV.
- Relate kinetic energy to velocity. Since K=21mv2, we have v∝K. Therefore,
v2v1=K2K1.
- Plug in the numbers.
v2v1=0.90.4=94=32.
So the ratio of maximum velocities is 2:3.
Watch outA common mistake is to take the ratio of the photon energies (1.5:2=3:4) or the ratio of the kinetic energies directly (0.4:0.9=4:9). Both ignore the square-root relationship between velocity and kinetic energy.
TipAlways subtract the work function first, then take the square root. The work function is a fixed “tax” — only the excess energy counts for motion.
✓Final answerThe correct option is (C).
ANSWER: C
- TG EAPCET 2023Set ap-2023-05-11-AN1 markMCQQ.An electric charge (q) moves along a metal tube with a variable cross-section as shown in the figure. It's velocity at the wider position A is Vo. Then the velocity of the charge when it approaches the neck of tube (position B) is (A) greater than Vo (B) equal to Vo (C) less than Vo (D) less than or equal to Vo
›Reveal solutionSolution
Inside a metallic tube the charge feels no force (a conductor screens the field), so it moves at constant speed — the velocity at the neck B equals Vo.
Concept: The tempting (wrong) analogy is fluid flow, where the equation of continuity (A1v1=A2v2) forces the speed to increase where the cross-section narrows. But a single charge is not an incompressible fluid; its motion is governed by Newton's laws, i.e. by the forces on it.
Reasoning:
- The tube is metal (a conductor). The electrostatic field inside the body of a conductor is zero, and a neutral conducting enclosure screens the interior.
- No electric or mechanical force acts on the charge as it drifts along the axis.
- With zero net force, the charge moves with constant velocity.
Therefore its speed at the neck B is the same as at the wide region A.
✓Final answerThe velocity at B equals Vo, option (B).
ANSWER: B
- TG EAPCET 2023Set eng-2023-05-14-FN1 markMCQQ.Metal detector works on the principle of (A) Ohm’s law (B) Coulomb’s law (C) Electromagnetic induction (D) Stefan’s law of radiation
›Reveal solutionSolution
A metal detector works by generating a changing magnetic field that induces currents in metal objects; this is the principle of electromagnetic induction, making option (C) correct.
The key concept here is electromagnetic induction — the production of an electric current in a conductor when it is exposed to a changing magnetic field. A metal detector doesn’t simply “sense” metal; it actively creates a magnetic field that changes over time. When this field encounters a metal object, it induces tiny electric currents (called eddy currents) in the metal. Those currents then create their own magnetic field, which the detector picks up. The other options are unrelated: Ohm’s law deals with voltage, current, and resistance in a circuit; Coulomb’s law describes electrostatic forces between charges; Stefan’s law is about thermal radiation.
Let’s break down why each option is or isn’t correct:
-
Ohm’s law (A) — This law states V=IR, relating voltage, current, and resistance. While a metal detector contains circuits that obey Ohm’s law, the operating principle of detection is not Ohm’s law. It doesn’t explain how the detector senses metal.
-
Coulomb’s law (B) — This law describes the force between stationary electric charges: F=kr2q1q2. Metal detectors do not rely on static electric charges; they rely on changing magnetic fields, so this is incorrect.
-
Electromagnetic induction (C) — This is the correct principle. A metal detector’s coil carries an alternating current, producing a rapidly changing magnetic field. When this field passes over a metal object, it induces eddy currents in the metal (Faraday’s law: E=−dtdΦB). Those eddy currents generate a secondary magnetic field, which induces a voltage in the detector’s receiver coil, triggering an alert.
-
Stefan’s law of radiation (D) — This law relates the power radiated by a blackbody to its temperature: P=σAT4. It has nothing to do with detecting metal objects.
Watch outA common mistake is to think metal detectors use “magnetism” in the static sense (like a magnet attracting iron). But they work with changing magnetic fields to detect all metals, not just ferrous ones. Static magnetism would only detect iron, not aluminum or gold.
TipA neat way to remember: if a device uses a coil and a changing current to “see” hidden metal, it’s using electromagnetic induction — the same principle behind electric generators and transformers.
✓Final answerThe correct option is (C).
ANSWER: C
-
- TG EAPCET 2023Set eng-2023-05-14-FN1 markMCQQ.At very high frequencies, the current (i) in the given circuit is [FIGURE] (A) 4 A (B) 0.4 A (C) 44 A (D) 4.4 A
›Reveal solutionSolution
At ω→∞ capacitors short and inductors open. The ladder collapses to 1Ω+(4∥4)+2Ω=5Ω, giving i=220/5=44 A — option (C).
The concept first
A frightening-looking AC network becomes trivial once you use the two limiting behaviours of reactive elements:
XC=ωC1 ω→∞ 0(capacitor→short circuit)
XL=ωL ω→∞ ∞(inductor→open circuit)
Why? A capacitor opposes a change of voltage; at very high frequency the voltage barely has time to build up across it, so it offers almost no opposition — a wire. An inductor opposes a change of current; at very high frequency the back-emf is enormous, so essentially no current gets through — a break.
Once every capacitor is a wire and every inductor is a gap, all the reactances vanish, the impedance is purely resistive, and Ohm's law i=V/R finishes the job. (The values 6μF, 0.8μF, 0.5μF, 20 mH, 50 mH are deliberate red herrings — none of them matters in the limit.)
Step-by-step
1. Kill the inductors (open circuits).
- The upper row begins 8Ω→20mH→…. With the 20mH open, the 8Ω leads nowhere: it is a dead branch carrying zero current. Delete it.
- Similarly, near the right the 50mH opens, orphaning the last upper 8Ω (which only connects to the right terminal through that broken inductor). Delete it too.
2. Short every capacitor.
- The three 0.8μF capacitors in the lower row become wires, so the lower row reduces to just its resistors: 1Ω, then 4Ω, then 2Ω in series from the left terminal to the right terminal.
- The 6μF capacitor in the upper row becomes a wire, so the upper 4Ω is now directly connected between the two cross-link nodes.
- The two 0.5μF cross-links become wires, welding each upper node to the lower node beneath it.
3. Rename the surviving nodes. Call the left terminal L, the right terminal R, and let X and Y be the two (now merged, upper=lower) cross-link nodes. Then:
- L→X: the 1Ω resistor.
- X→Y: two paths in parallel — the lower 4Ω and the upper 4Ω.
- Y→R: the 2Ω resistor.
4. Combine.
4∥4=4+44×4=2Ω
Req=1+2+2=5Ω
5. Apply Ohm's law. With no net reactance, Z=Req=5Ω and the source is 220 V:
i=ZV=5220=44 A.
A useful habit: whenever an AC question says "at very high frequency" or "at very low frequency", do not compute a single reactance. Just redraw the circuit with caps/inductors replaced by wires or gaps (ω→0 flips it: capacitors open, inductors short) — the answer usually falls out in two lines.
✓Final answerThe current at very high frequency is 44 A, so the correct option is (C).
ANSWER: C
- TG EAPCET 2022Set ap-2022-07-31-FN1 markMCQQ.When the brakes are applied to two cars moving with initial velocities V and 2V and the cars stop at distances d1 and d2 respectively. Assuming the work done on the cars is the same, then the value of ratio d1d2 is (A) 1 (B) 2 (C) 0.5 (D) 4
›Reveal solutionSolution
The key idea is that the work done by the brakes equals the change in kinetic energy, and since the work is the same for both cars, the stopping distance is proportional to the square of the initial speed. The ratio d1d2 is 4, so the correct option is (D).
Concept and Intuition
When brakes are applied, the force of friction (assumed constant) does work to bring the car to rest. The work-energy theorem tells us that the net work done on an object equals its change in kinetic energy. Here, the work done by the brakes is the same for both cars, so the initial kinetic energy of each car is entirely dissipated by the same braking force over different distances. Since kinetic energy depends on the square of velocity, a car starting at twice the speed has four times the kinetic energy, and thus needs four times the stopping distance if the braking force is constant.
Step-by-step solution
-
Apply the work-energy theorem
For each car, the work done by the brakes (which is the net work, since other forces are balanced) equals the change in kinetic energy. The car starts with kinetic energy 21mv2 and ends at rest, so the work done is W=21mv2.
-
Express work in terms of force and distance
If the braking force F is constant (same for both cars, as the problem implies identical braking conditions), then the work done is also W=F⋅d, where d is the stopping distance. Thus:
Fd=21mv2
- Write equations for both cars For the first car (initial speed V, stopping distance d1):
Fd1=21mV2
For the second car (initial speed 2V, stopping distance d2):
Fd2=21m(2V)2=21m⋅4V2=2mV2
- Find the ratio Divide the second equation by the first:
Fd1Fd2=21mV22mV2
Simplify:
d1d2=212=4
TipA quick shortcut: Since d∝v2 for constant force and mass, doubling the speed quadruples the stopping distance. No need to write out the mass or force explicitly.
Watch outA common mistake is to think that because the work is the same, the distances are equal (option A), or that distance is proportional to speed (option B). But work depends on the square of speed, not the speed itself.
✓Final answerThe correct option is (D).
ANSWER: D
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