By the end of this chapter you'll be able to…

  • 1State the photoelectric observations and apply Einstein's equation and stopping potential
  • 2Compute photon energy and momentum and the de Broglie wavelength
  • 3Use the Bohr radius and energy-level formulas and the hydrogen spectral series
  • 4Relate mass defect to binding energy and read the binding-energy curve
  • 5Apply the radioactive decay law, half-life and the α/β/γ transformation rules
  • 6Explain fission and fusion and where nuclear energy comes from
  • 7Describe doping, the p–n junction, rectifiers and logic gates
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Why this chapter matters in NEET UG
Modern physics is a small syllabus with an outsized NEET yield — a reliable 4–5 questions from a compact, clean set of ideas: the dual nature of light and matter, quantised atomic energy levels, the nucleus and radioactivity, and semiconductor devices. Because the formulas are few and the concepts distinctive, it is one of the highest-return blocks in the paper. This chapter derives the key results (Einstein's equation, the Bohr energy levels, the decay law), explains why each experiment forced a new idea, and drills the standard problems so these become near-certain marks.

Modern Physics and Electronic Devices — NEET Physics

Modern physics is a small syllabus with an outsized NEET yield — a reliable 4–5 questions from a compact set of revolutionary ideas: light and matter are both particle and wave; atoms have quantised energy levels; nuclei store colossal energy; and semiconductors, engineered atom by atom, run all electronics. The formulas are few and clean, so this is one of the highest-return blocks in the paper. This chapter derives the key results, explains why each experiment forced a new idea, and drills the standard problems in full.


PART A — DUAL NATURE OF RADIATION AND MATTER

1. The photoelectric effect — the experiment

Shine light on a metal and electrons are ejected. Careful measurement gives five facts that no wave theory could explain:

  1. Emission is instantaneous (no build-up time), even for faint light.
  2. For each metal there is a threshold frequency below which no electrons come out, however intense the light.
  3. The maximum kinetic energy of the electrons depends on the frequency, not the intensity.
  4. The number of electrons (the photocurrent) depends on the intensity.
  5. The stopping potential (the reverse voltage that just halts the most energetic electron) rises with frequency.

2. Einstein's photoelectric equation

Einstein resolved this by quantising light into photons of energy . Each photon gives all its energy to one electron; part (, the work function) frees it, the rest becomes kinetic energy:

Since the stopping potential satisfies :

A graph of against is a straight line of slope — the same for every metal — and an intercept fixing the work function. This clinched the photon idea and won Einstein the 1921 Nobel Prize.

  • Intensity → number, frequency → energy. Doubling intensity doubles the current but leaves each electron's energy unchanged; raising frequency raises the energy.

Worked example 2.1. A metal has work function 2 eV. Light of energy 5 eV strikes it. Maximum KE of the photoelectrons? eV. The stopping potential is V.


3. Photon energy and momentum

A convenient shortcut in exam units: .

  • A 620 nm photon carries eV.
  • A photon has momentum despite being massless — the basis of radiation pressure and light sails.

4. Matter waves: de Broglie

If light waves behave as particles, particles should behave as waves. de Broglie proposed every moving particle has a wavelength:

For an electron accelerated through a potential difference , , giving the handy formula

  • Heavier or faster particles have shorter wavelengths — why an electron microscope (tiny ) resolves far finer detail than a light microscope. The Davisson–Germer experiment (electron diffraction off a crystal) confirmed matter waves directly.

PART B — ATOMS AND NUCLEI

5. The Bohr model — postulates and derivation

Rutherford's nuclear atom was unstable in classical physics (orbiting electrons should radiate and spiral in). Bohr fixed this with three postulates:

  1. Electrons orbit in stationary states without radiating.
  2. Angular momentum is quantised: ().
  3. Radiation is emitted/absorbed only when an electron jumps between levels: .

Balancing the Coulomb force against the centripetal requirement and applying quantisation gives, for a hydrogen-like atom (nuclear charge ):

For hydrogen ():

  • Ground state eV; the ionisation energy is eV.
  • Radius grows as : the second orbit is the first ( Å).
  • Energy of a transition ; the jump releases eV.

Limitations: the model works only for one-electron atoms and cannot explain fine structure or intensities — but its energy-level picture is exactly what NEET tests.


6. The hydrogen spectrum

Transitions grouped by the final level form series, all captured by the Rydberg formula:

SeriesRegion
Lyman1Ultraviolet
Balmer2Visible
Paschen3Infrared
Brackett4Infrared

The Balmer series (jumps down to ) is the visible one you see as hydrogen's coloured lines.


7. The nucleus: size, mass defect and binding energy

  • Composition: protons and neutrons; is the mass number.
  • Size: with fm, so nuclear density is essentially constant ( kg/m³) — matter is mostly empty space with a fantastically dense core.
  • Mass defect: a nucleus is lighter than its separate nucleons; the missing mass is converted to the binding energy that holds it together, via (with MeV).

The binding energy per nucleon curve rises steeply, peaks at about 8.8 MeV near iron (), then falls slowly. This single curve explains nuclear energy: fusing light nuclei or fissioning heavy ones both move toward iron and release energy.

Worked example 7.1. If 0.02 u of mass is lost when a nucleus forms, its binding energy is MeV.


8. Radioactivity and the decay law

Unstable nuclei emit:

  • α — a helium nucleus (): , . Low penetration.
  • β⁻ — an electron from a neutron converting to a proton: , unchanged.
  • γ — a high-energy photon: , unchanged (the nucleus de-excites).

Decay is random but statistically exponential:

  • After half-lives, a fraction remains: after 2, after 3.
  • Activity (decays per second, in becquerel). Carbon-14 dating and medical tracers rely on these laws.

9. Fission and fusion

  • Fission: a heavy nucleus (U-235) absorbs a neutron and splits, releasing MeV and more neutrons — a controllable chain reaction (reactors) or an explosive one (bombs).
  • Fusion: light nuclei (hydrogen isotopes) merge into helium, releasing even more energy per nucleon — the power source of the Sun and stars, requiring enormous temperatures.

PART C — SEMICONDUCTOR ELECTRONICS

10. Energy bands and doping

Solids have a valence band (bound electrons) and a conduction band (free to move), separated by a band gap :

  • Conductors: bands overlap ().
  • Insulators: large gap ( eV).
  • Semiconductors: small gap (Si eV, Ge eV) — insulating when cold, conducting when warmed or doped.

Doping a pure (intrinsic) semiconductor tailors its conduction:

  • n-type: add a pentavalent donor (P, As, Sb) → spare electrons are the majority carriers.
  • p-type: add a trivalent acceptor (B, Al, Ga) → holes are the majority carriers.

The crystal stays electrically neutral overall; doping just decides which carrier dominates.


11. The p–n junction and diode

Join p- and n-type material and electrons/holes diffuse across, leaving a charged depletion region with a barrier potential (~0.7 V for Si, ~0.3 V for Ge).

  • Forward bias (p to +, n to −): the barrier is lowered, and the diode conducts freely above ~0.7 V.
  • Reverse bias (p to −, n to +): the barrier widens, and only a tiny leakage current flows — the diode blocks. A large enough reverse voltage causes breakdown.

A diode is thus a one-way valve for current.


12. Rectifiers and special diodes

  • Rectifier: converts AC to DC. A half-wave rectifier (one diode) passes only one half of each cycle; a full-wave bridge rectifier (four diodes) uses both halves, giving smoother DC.
  • Zener diode: operated in reverse breakdown at a fixed voltage — a voltage regulator.
  • LED: emits light on forward conduction (energy ).
  • Photodiode / solar cell: light generates a current — the basis of light sensors and solar panels.

13. Logic gates (basics)

Digital electronics is built from gates acting on binary inputs (0/1):

GateOutput is 1 when…
ORany input is 1
ANDall inputs are 1
NOTinput is 0 (inverts)
NANDNOT of AND (universal gate)
NORNOT of OR (universal gate)

14. Common traps NEET sets here

  • Intensity vs frequency in the photoelectric effect — intensity sets the number of electrons, frequency their energy; no emission below , however bright.
  • Sign of energy levels — bound states are negative; ionisation energy is the positive amount to reach zero.
  • Radius as , energy as — don't swap; and for hydrogen-like atoms include the factors.
  • Half-life fractions — after half-lives, remains, not .
  • α and β changes — α: ; β⁻: , same; γ: no change.
  • Binding energy peaks at iron — both fusion (light) and fission (heavy) release energy moving toward it.
  • n-type has electrons, p-type has holes — pentavalent vs trivalent doping; the crystal stays neutral.
  • Diode direction — conducts only in forward bias.

15. Memory aids

  • "Frequency = energy, intensity = number" — photoelectric rule.
  • "1240/λ(nm) = eV" — quick photon energy.
  • "−13.6 Z²/n² energy, 0.53 n²/Z radius" — the Bohr atom.
  • "Balmer is the visible series."
  • "Iron is most tightly bound."
  • "(½)ⁿ per n half-lives; τ = T/0.693."
  • "Penta → n-type electrons, tri → p-type holes."
  • "Forward conducts, reverse blocks; bridge = 4 diodes."

16. Exam protocol

  1. Photoelectric: , ; no emission below ; intensity → number, frequency → energy.
  2. Photon eV; momentum .
  3. de Broglie ; electron through : Å.
  4. Bohr: eV, Å; transition energy = level difference; Balmer is visible.
  5. Nucleus: (constant density); BE , MeV; peak at iron.
  6. Decay: , ; α (), β⁻ (), γ (no change).
  7. Semiconductors: doping (penta → n, tri → p); diode conducts forward; bridge rectifier = 4 diodes; Zener regulates.

Key formulas & results

Everything to memorise for the exam hall, in one card. Screenshot this for revision.

Einstein's photoelectric equation
No emission below the threshold frequency f₀ = φ/h.
Photon energy & momentum
A massless photon still carries momentum.
de Broglie wavelength
Faster/heavier particles have shorter wavelengths.
Bohr atom
Energy scales as 1/n², radius as n².
Rydberg formula
Balmer (n₁=2) is the visible series.
Radioactive decay
After n half-lives, (1/2)ⁿ remains; activity A = λN.
Binding energy
Binding energy per nucleon peaks near iron (A ≈ 56).
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Traps NEET UG sets — and how to dodge them

These are the exact option-traps and misreads that cost marks under negative marking.

WATCH OUT
Thinking intensity changes the electrons' energy in the photoelectric effect.
Intensity sets the number of photoelectrons (the current); frequency sets their maximum kinetic energy. Below the threshold frequency there is no emission at all, no matter how intense the light.
WATCH OUT
Getting the sign of atomic energy levels wrong.
Bound-state energies are negative (E_n = −13.6/n² eV for hydrogen). The ionisation energy is the positive amount needed to raise the electron to E = 0, i.e. +13.6 eV from the ground state.
WATCH OUT
Swapping the n-dependence of radius and energy.
Radius grows as n² (r_n = 0.53 n²/Z Å) while energy grows as 1/n² (E_n = −13.6 Z²/n² eV). Higher orbits are larger and less tightly bound.
WATCH OUT
Using 1/n instead of (1/2)ⁿ for decay fractions.
After n half-lives the remaining fraction is (1/2)ⁿ — one-quarter after 2, one-eighth after 3 — not 1/n. The decay is exponential, not linear.
WATCH OUT
Mis-stating the α and β transformations.
Alpha decay reduces A by 4 and Z by 2; beta-minus decay raises Z by 1 with A unchanged (a neutron becomes a proton); gamma emission changes neither A nor Z. Track both numbers when balancing a decay.
WATCH OUT
Confusing n-type and p-type doping.
Pentavalent donors (P, As, Sb) give an n-type semiconductor with electrons as majority carriers; trivalent acceptors (B, Al, Ga) give p-type with holes as majority carriers. The crystal remains electrically neutral overall.

Exam-pattern practice

PYQ-style questions with full solutions. Work through them as a readiness check — mark yourself honestly and get your gap report at the end.

Readiness check

Are you exam-ready for Modern Physics and Electronic Devices?

15 problems from this chapter. Try each one, reveal the worked solution, mark yourself honestly — get your gap report at the end.

15 questions~11 min

5-minute revision

The whole chapter, distilled. Read this the night before the exam.

  • Photoelectric: KE_max = hf − φ = eV₀; no emission below f₀; intensity → number, frequency → energy
  • Photon E = hc/λ = 1240/λ(nm) eV; momentum p = h/λ
  • de Broglie λ = h/mv; electron through V: λ = 12.27/√V Å
  • Bohr: E_n = −13.6 Z²/n² eV, r_n = 0.53 n²/Z Å; ionisation energy of H = 13.6 eV
  • Rydberg 1/λ = R(1/n₁² − 1/n₂²); Balmer (n₁=2) visible
  • Nucleus R = R₀A^(1/3) (constant density); BE = Δmc², 1 u = 931.5 MeV; peak at iron
  • Decay N = N₀(1/2)^(t/T), T = 0.693/λ; α (A−4, Z−2), β⁻ (Z+1), γ (no change)
  • Doping: pentavalent → n-type (electrons), trivalent → p-type (holes)
  • Diode conducts forward, blocks reverse; bridge rectifier = 4 diodes; Zener regulates

NEET UG question blueprint

How this topic is asked, tier by tier — so you can prep to the pattern.

Typical weightage: 20

Question styleMarks eachTypical countWhat it tests
Photoelectric effect & dual nature~1–2 Q
Atoms & hydrogen spectrum~1 Q
Nuclei & radioactivity~1 Q
Semiconductors & devices~1–2 Q
Prep strategy
  • Master the photoelectric equation, stopping potential and the intensity/frequency distinction
  • Memorise the Bohr energy/radius formulas and the spectral series
  • Drill decay-law fractions and the α/β/γ transformation rules
  • Learn doping, diode biasing and rectifier circuits cold

Exam-hall strategy

Battle-tested tips from mentors and toppers for this topic under the sectional clock.

  1. Photoelectric: KE_max = hf − φ; no emission below f₀; intensity → number, frequency → energy.
  2. Photon E = 1240/λ(nm) eV, momentum h/λ; de Broglie λ = h/mv.
  3. Bohr: E_n = −13.6 Z²/n² eV, r_n = 0.53 n²/Z Å; transition energy = level difference.
  4. Binding energy peaks at iron; BE = Δmc², 1 u = 931.5 MeV.
  5. Decay N = N₀(1/2)^(t/T); α (A−4, Z−2), β⁻ (Z+1), γ (no change).
  6. Doping: pentavalent → n-type, trivalent → p-type.
  7. Diode conducts forward; bridge rectifier uses 4 diodes; Zener regulates voltage.

Beyond the exam

Where this skill shows up in the job you're competing for — and in life.

Medical imaging and therapy

X-rays, PET and radiotherapy use photon energy, radioactivity and decay laws directly in diagnosis and treatment.

Radioisotope dating and tracers

Carbon-14 dating and medical tracer studies rely on the exponential decay law and half-life.

All modern electronics

Diodes, transistors and logic gates — built on semiconductor physics — run every phone, computer and monitor.

Solar power and LEDs

Photodiodes and solar cells convert light to current; LEDs convert current to light — both p–n junction devices.

Where else this topic is tested

Prepare once, score in every exam that asks it.

JEE MainModern physics & semiconductors
JEE AdvancedPhotoelectric, nuclear & atomic detail
CUET (Science)Dual nature, atoms & electronics
State medical/engg CETsModern-physics MCQs

Questions aspirants ask

Pulled from the Q&A community and mentor sessions.

Wave theory predicts that brighter light (more energy) should eject more energetic electrons and that dim light should need time to build up. Experiment showed the opposite: the electrons' energy depends only on frequency, emission is instantaneous, and below a threshold frequency nothing happens however bright the light. Einstein explained this by treating light as photons of energy hf, each delivering its energy to one electron at once. Only frequency (photon energy) sets the electron's energy; intensity sets the number of photons and hence electrons.

The electron in an atom is bound, so its total energy is less than that of a free electron at rest (taken as zero). The negative value, E_n = −13.6/n² eV for hydrogen, measures how much energy you must supply to free it. The ground state (−13.6 eV) is the most tightly bound; higher levels are less negative (closer to zero) and less bound. Reaching E = 0 means ionisation, which is why hydrogen's ionisation energy is exactly 13.6 eV.

The binding energy per nucleon rises to a peak near iron (A ≈ 56) and falls off for lighter and heavier nuclei. Any process that moves nuclei toward that peak — fusing very light nuclei or splitting very heavy ones — increases the binding energy per nucleon, and the extra binding energy is released. The Sun fuses hydrogen into helium; reactors fission uranium. Both convert a tiny mass defect into large energy via E = mc².

Radioactive decay is exponential: N = N₀e^(−λt). The half-life T = 0.693/λ is the time for half the nuclei to decay, and it is constant regardless of how many remain. After each half-life the amount halves, so after n half-lives a fraction (1/2)ⁿ is left — one-quarter after two, one-eighth after three. This fixed, statistical clock is what makes carbon-14 dating and medical tracer timing possible.

Both start from a pure semiconductor like silicon. Doping with a pentavalent element (five valence electrons, e.g. phosphorus) leaves a spare electron per dopant atom, so electrons are the majority carriers — an n-type semiconductor. Doping with a trivalent element (three valence electrons, e.g. boron) leaves an electron vacancy, or hole, so holes are the majority carriers — p-type. In both cases the material stays electrically neutral; doping only decides which carrier dominates conduction.

At the junction, diffusing carriers create a depletion region with a barrier potential. In forward bias (p to +, n to −) the barrier is lowered and current flows freely; in reverse bias the barrier widens and only negligible leakage flows. So the diode conducts in only one direction. A rectifier exploits this to turn alternating current into direct current — a half-wave rectifier uses one diode to pass one half of each cycle, while a full-wave bridge uses four diodes to pass both halves in the same direction, giving smoother DC.
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