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⚡ Class XII · Physics · Chapter 11

NCERT Solutions for Class 12 Physics Chapter 11: Dual Nature of Radiation and Matter

All 11 exercise questions of the latest NCERT textbook (2026–27 reprint) solved like a topper’s answer-sheet — X-ray limits, Einstein’s photoelectric equation, work function, stopping potential, photons, Planck’s constant and de Broglie wavelengths — with graphs linked to the exact NCERT pages, comparison tables, complete revision notes and exam tips.

11 questions3 diagrams10 tablesFull revision notes

Chapter at a glance — complete revision notes

11.1 Introduction

  • Maxwell’s equations and Hertz’s experiments (1887) strongly established the wave nature of light. At the same time, studies of electric discharge through gases at low pressure (~0.001 mm of Hg) gave the cathode rays (discovered by William Crookes, 1870, who suggested in 1879 that they are streams of fast-moving negatively charged particles) — X-rays were discovered by Roentgen in 1895 and the electron by J. J. Thomson in 1897. Thomson applied mutually perpendicular electric and magnetic fields and determined the speed (0.1–0.2 c) and specific charge e/m = 1.76 × 10¹¹ C kg⁻¹ — independent of the cathode material and the gas (universality); he named them electrons (Nobel Prize 1906). In 1913 Millikan’s oil-drop experiment showed that the charge on an oil drop is always an integral multiple of e = 1.602 × 10⁻¹⁹ C (charge is quantised), from which the electron mass could be found. Metals irradiated by ultraviolet light (1887) and heated metals emit particles with the same e/m: electrons.

11.2 Electron emission

  • Free electrons cannot normally escape from a metal: the surface acquires a positive charge and pulls the electron back. The minimum energy required for an electron to escape is the work function φ₀ (unit eV: 1 eV = 1.602 × 10⁻¹⁹ J, the energy gained by an electron accelerated through 1 V); it depends on the metal and the nature of its surface.
  • Three ways to supply the energy: thermionic emission (heating), field emission (strong field ~10⁸ V m⁻¹, as in a spark plug), and photoelectric emission (light of suitable frequency); the electrons emitted by the last are called photoelectrons.

11.3 Photoelectric effect

  • 11.3.1 Hertz’s observations: in 1887 Hertz found that the sparks across the detector loop were enhanced when the emitter plate was illuminated by ultraviolet light from an arc lamp — light helped the escape of charged particles (electrons) from the surface.
  • 11.3.2 Hallwachs’ and Lenard’s observations (1886–1902): Lenard found a current flowing in an evacuated tube when UV light fell on the emitter plate, and it stopped when the light was stopped (Fig. 11.1). Hallwachs (1888): a negatively charged zinc plate connected to an electroscope lost its charge when illuminated by UV; an uncharged zinc plate became positively charged and a positively charged plate became more positive. Below a threshold frequency (characteristic of the material) no electrons are emitted. Zinc, cadmium and magnesium respond only to UV; alkali metals (Li, Na, K, Cs, Rb) are sensitive even to visible light.

11.4 Experimental study of the photoelectric effect

  • Apparatus (Fig. 11.1): an evacuated glass/quartz tube with a photosensitive emitter plate C and a collector plate A; monochromatic light from the source S passes through the quartz window W; the battery and a commutator vary the potential and polarity of A relative to C; a voltmeter and a microammeter measure the p.d. and the photocurrent. Intensity is varied by changing the distance of the source; frequency by filters.
  • 11.4.1 Intensity: for fixed frequency and potential the photocurrent is directly proportional to the intensity (Fig. 11.2) — the number of photoelectrons per second ∝ intensity.
  • 11.4.2 Potential (Fig. 11.3): photocurrent rises with the positive potential of A until it saturates (all the emitted electrons collected: saturation current); with a negative potential on A (retarding) the current decreases and falls to zero at the stopping potential (cut-off potential) V₀, at which even the most energetic electrons are repelled: K_max = eV₀. For higher intensity the saturation current is larger but V₀ is the same — K_max is independent of intensity.
  • 11.4.3 Frequency (Figs 11.4, 11.5): the stopping potential rises with the frequency (V₀₃ > V₀₂ > V₀₁ for ν₃ > ν₂ > ν₁) while the saturation current is the same; V₀ varies linearly with ν and there exists a threshold (cut-off) frequency ν₀ below which no emission occurs however intense the light; the emission is instantaneous (~10⁻⁹ s or less) even for very dim light.
  • Summary of observations: (i) I ∝ intensity (above ν₀); (ii) saturation current ∝ intensity, V₀ independent of intensity; (iii) threshold frequency; K_max rises linearly with ν, independent of intensity; (iv) instantaneous emission.

11.5 Photoelectric effect and wave theory of light

  • The wave theory (continuous absorption of energy by electrons; larger intensity ⇒ larger amplitude ⇒ more energy per electron) predicts that K_max should increase with intensity, that no threshold frequency should exist (a sufficiently intense beam over a long enough time would suffice), and that the emission would take hours for the energy to build up — contradicting observations (i)–(iv). It cannot explain the basic features of the photoelectric effect.

11.6 Einstein’s photoelectric equation: energy quantum of radiation

  • Einstein (1905): radiation energy is built of discrete quanta (photons), each of energy hν (h = Planck’s constant = 6.63 × 10⁻³⁴ J s). An electron absorbs one quantum; if hν exceeds the work function the electron is emitted with the maximum kinetic energy K_max = hν − φ₀ (more tightly bound electrons emerge with less). In terms of the threshold frequency: K_max = h(ν − ν₀), ν₀ = φ₀/h; eV₀ = hν − φ₀, so V₀ = (h/e)ν − φ₀/e: a straight line of slope h/e (Fig. 11.5), from which Millikan’s measurements obtained an accurate value of h and confirmed the equation.
  • Explanation of the observations: K_max depends linearly on ν and is independent of intensity (a single photon is absorbed by a single electron); threshold frequency ν₀ = φ₀/h (below ν₀ no emission however intense or long the exposure); for ν > ν₀ the number of photons (intensity) fixes the number of electrons: current ∝ intensity; the absorption of a quantum is instantaneous. Einstein’s equation is the law of conservation of energy for the absorption of a photon by an electron. Nobel Prizes: Einstein (1921), Millikan (1923).

11.7 Particle nature of light: the photon

  • Einstein showed that the light quantum also carries momentum p = hν/c = h/λ — a strong sign of a particle (the photon); the particle-like behaviour was further confirmed by A. H. Compton’s experiment on the scattering of X-rays from electrons (1924). Photon picture: (i) radiation interacts with matter as particles (photons); (ii) each photon has E = hν and p = hν/c, and moves at the speed of light c; (iii) all photons of a given frequency have the same energy and momentum irrespective of the intensity — increasing the intensity only increases the number of photons per second crossing unit area; (iv) photons are electrically neutral and are not deflected by electric or magnetic fields; (v) in a photon–particle collision total energy and momentum are conserved, but the number of photons need not be (absorption or creation).
  • Example 11.1: 2.0 × 10⁻³ W of 6.0 × 10¹⁴ Hz light: E = hν = 3.98 × 10⁻¹⁹ J, N = P/E = 5.0 × 10¹⁵ photons per second. Example 11.2: caesium (φ₀ = 2.14 eV): threshold frequency ν₀ = φ₀/h = 5.16 × 10¹⁴ Hz, and the wavelength for a stopping potential of 0.60 V follows from hc/λ = φ₀ + eV₀.
  • Dual nature of radiation: wave nature in interference, diffraction and polarisation; particle nature (photons) in the photoelectric and Compton effects; the choice of description depends on the experiment (e.g. seeing: the eye-lens focuses light by the wave picture; absorption by the rods and cones needs the photon picture).

11.8 Wave nature of matter

  • Since radiation has a dual nature, Louis de Broglie (1924) hypothesised that moving particles of matter display wave-like properties: the wavelength associated with a particle of momentum p is λ = h/p = h/(mv) (de Broglie relation) — wave attribute λ on the left, particle attribute p on the right. For a photon λ = h/p equals the wavelength of the electromagnetic radiation. λ is smaller for heavier or faster particles; for a ball of 0.12 kg at 20 m s⁻¹ λ ~ 10⁻³⁴ m — unmeasurable, which is why macroscopic objects show no wave-like properties, whereas in the sub-atomic domain the wave character is significant and measurable. Example 11.3: electron at 5.4 × 10⁶ m s⁻¹: λ = 0.135 nm (comparable to X-ray wavelengths); ball of 150 g at 30 m s⁻¹: λ ≈ 1.5 × 10⁻³⁴ m (about 10⁻¹⁹ times the size of a proton).

Summary & key points (NCERT)

  • Work function; electron emission by heating, strong field and light; photoelectric effect — I ∝ intensity, V₀ depends on frequency and material (not on intensity), K_max = eV₀, threshold frequency, instantaneous; wave theory fails; Einstein’s equation ½mv²_max = hν − φ₀ and ν₀ = φ₀/h; photons E = hν, p = h/λ; Millikan’s measurements confirmed the equation and gave h; dual nature; de Broglie λ = h/p independent of the charge and nature of the particle.
Q1

Find the (a) maximum frequency, and (b) minimum wavelength of X-rays produced by 30 kV electrons.

Answer

Concept and context. X-rays are produced when fast electrons are suddenly stopped on striking a metal target: the kinetic energy of the electrons is converted into radiation (bremsstrahlung). This is the inverse of the photoelectric effect — an electron of kinetic energy K can create a photon of energy hν at most equal to K. An electron accelerated through a potential difference V acquires a kinetic energy eV. In the most energetic conversion all the kinetic energy of the electron is transferred to a single photon, giving the maximum frequency (the Duane–Hunt limit): hν_max = eV and, correspondingly, the minimum wavelength λ_min = c/ν_max = hc/(eV).

Electrons accelerated through V = 30 kV→Kinetic energy eV = 30 keV = 4.8 × 10⁻¹⁵ J→Strike a target and are stopped→All the energy goes to one photon: hν_max = eV→ν_max = eV/h ; λ_min = c/ν_max

Given: V = 30 kV = 3.0 × 10⁴ V; e = 1.6 × 10⁻¹⁹ C; h = 6.63 × 10⁻³⁴ J s; c = 3.0 × 10⁸ m s⁻¹.

(a) Maximum frequency

  1. Energy of the electrons: K = eV = 1.6 × 10⁻¹⁹ × 3.0 × 10⁴ = 4.8 × 10⁻¹⁵ J (= 30 keV).
  2. hν_max = eV ⇒ ν_max = eV/h = (4.8 × 10⁻¹⁵)/(6.63 × 10⁻³⁴) = 7.24 × 10¹⁸ Hz.

(b) Minimum wavelength

  1. λ_min = c/ν_max = (3.0 × 10⁸)/(7.24 × 10¹⁸) = 4.14 × 10⁻¹¹ m.
  2. λ_min = 4.1 × 10⁻¹¹ m = 0.041 nm (= 0.41 Å). (Handy formula: λ_min (nm) = 1.24/V(kV) = 1.24/30 = 0.0413 nm.)

ν_max = eV/h = 7.2 × 10¹⁸ Hz ; λ_min = hc/eV = 4.1 × 10⁻¹¹ m

QuantityValue
Electron energy eV30 keV = 4.8 × 10⁻¹⁵ J
ν_max7.24 × 10¹⁸ Hz
λ_min4.14 × 10⁻¹¹ m (0.041 nm)
Photon energy at the limit30 keV
  • Interpretation: the X-ray spectrum from such a tube is continuous but has a sharp cut-off at λ_min, which depends only on the applied voltage (not on the target material); raising the voltage shortens λ_min (higher penetrating power).
  • Region of the spectrum: 0.041 nm lies in the X-ray (and the beginning of the γ-ray) region — NCERT lists X-rays from about 10 nm to 10⁻⁴ nm.
Exam tip: Write hν_max = eV (all the kinetic energy to one photon) and quote λ_min = hc/eV. Keep the unit conversion 30 kV → 3.0 × 10⁴ V.

Conclusion: the maximum frequency of the X-rays is 7.2 × 10¹⁸ Hz and the minimum wavelength is 4.1 × 10⁻¹¹ m (0.041 nm).

Q2

The work function of caesium metal is 2.14 eV. When light of frequency 6 × 10¹⁴ Hz is incident on the metal surface, photoemission of electrons occurs. What is the (a) maximum kinetic energy of the emitted electrons, (b) Stopping potential, and (c) maximum speed of the emitted photoelectrons?

Answer

Concept and context. In Einstein’s photoelectric equation (NCERT Section 11.6) a single photon of energy hν gives all its energy to a single electron; part of it (the work function φ₀) is used to free the electron from the metal and the remainder appears as the electron’s kinetic energy: K_max = hν − φ₀ (more tightly bound electrons emerge with smaller energies). The stopping potential V₀ is the retarding potential at which even the fastest photoelectrons are stopped: eV₀ = K_max (NCERT Fig. 11.3, 11.5). Photoemission is possible only if hν > φ₀, i.e. ν > ν₀ = φ₀/h.

Stopping potential versus frequency for caesium: a straight line of slope h/e starting at the threshold frequency 5.17 x 10^14 Hz; at 6 x 10^14 Hz the stopping potential is 0.35 Vν (10¹⁴ Hz) →V₀ (volt)0123456789100123ν₀ = 5.17ν = 6.0 × 10¹⁴ Hz: V₀ ≈ 0.35 Vcaesium (φ₀ = 2.14 eV): stopping potential versus frequencystraight line of slope h/e = 4.14 × 10⁻¹⁵ V s, intercept ν₀ = 5.17 × 10¹⁴ Hz© iBioKaare
Fig. — stopping potential V₀ versus frequency ν for caesium: a straight line of slope h/e and intercept ν₀ (compare NCERT Fig. 11.5) (original iBioKaare schematic). Compare with NCERT textbook — Fig. 11.5, page 6 ↗

Given: φ₀ = 2.14 eV; ν = 6 × 10¹⁴ Hz; h = 6.63 × 10⁻³⁴ J s; 1 eV = 1.6 × 10⁻¹⁹ J; m = 9.11 × 10⁻³¹ kg.

(a) Maximum kinetic energy

  1. Photon energy: hν = (6.63 × 10⁻³⁴)(6 × 10¹⁴) = 3.98 × 10⁻¹⁹ J = 3.98 × 10⁻¹⁹/1.6 × 10⁻¹⁹ = 2.49 eV.
  2. K_max = hν − φ₀ = 2.49 − 2.14 = 0.35 eV (= 5.5 × 10⁻²⁰ J).

(b) Stopping potential

eV₀ = K_max ⇒ V₀ = 0.35 eV/e = 0.35 V

(c) Maximum speed of the photoelectrons

  1. K_max = ½ m v²_max ⇒ v_max = √(2K_max/m).
  2. v_max = √[2 × 5.5 × 10⁻²⁰/(9.11 × 10⁻³¹)] = √(1.2 × 10¹¹) = 3.5 × 10⁵ m s⁻¹.
QuantityValue
Photon energy hν2.49 eV
Work function φ₀2.14 eV
K_max = hν − φ₀0.35 eV (5.5 × 10⁻²⁰ J)
V₀0.35 V
v_max3.5 × 10⁵ m s⁻¹
Threshold frequency ν₀ = φ₀/h5.16 × 10¹⁴ Hz (6.0 × 10¹⁴ Hz is above it ✓)
  • Check: ν = 6.0 × 10¹⁴ Hz is greater than ν₀ = 5.16 × 10¹⁴ Hz, so photoemission occurs; the corresponding wavelength is 500 nm (green light). The speed is a small fraction of c (10⁻³), so the non-relativistic formula is valid.
  • Intensity would only change the number of photoelectrons per second (the photocurrent), not K_max.
Exam tip: Convert hν to eV (divide by 1.6 × 10⁻¹⁹) before subtracting φ₀ in eV; use K in joules for the speed.

Conclusion: (a) K_max = 0.35 eV; (b) stopping potential = 0.35 V; (c) maximum speed = 3.5 × 10⁵ m s⁻¹.

Q3

The photoelectric cut-off voltage in a certain experiment is 1.5 V. What is the maximum kinetic energy of photoelectrons emitted?

Answer

Concept and context. In the photoelectric experiment (NCERT Fig. 11.1), when the collector plate A is made negative with respect to the emitter C, the electrons are decelerated. At the stopping (cut-off) potential V₀ the photocurrent just becomes zero: even the most energetic electrons (emitted with K_max) are brought to rest just before reaching the collector. The work done by the retarding field, eV₀, equals the maximum kinetic energy: K_max = eV₀. This gives a direct way of measuring the maximum energy of photoelectrons (and, by Einstein’s equation, h/e).

  • Given: V₀ = 1.5 V.
  • K_max = eV₀ = e × 1.5 V = 1.5 eV = 1.5 × 1.6 × 10⁻¹⁹ J = 2.4 × 10⁻¹⁹ J.

Kmax = eV₀ = 1.5 eV = 2.4 × 10⁻¹⁹ J

QuantityValue
Cut-off voltage V₀1.5 V
K_max in eV (numerically = V₀)1.5 eV
K_max in joule2.4 × 10⁻¹⁹ J
Maximum speed (extra)√(2K/m) = 7.3 × 10⁵ m s⁻¹
  • Remark: when the energy is measured in electron-volts it is numerically equal to the stopping potential in volts — the great convenience of the eV unit.
  • Independent of intensity: V₀ (hence K_max) does not change when the intensity of the light is increased; only the saturation current does (NCERT Fig. 11.3). It rises with the frequency (Fig. 11.4).
  • Possible follow-up: with Einstein’s equation hν = φ₀ + eV₀ the work function of the emitter can be found if the frequency is known (Exercise 11.9).
Exam tip: K_max = eV₀ — write the answer in both eV and J.

Conclusion: the maximum kinetic energy of the photoelectrons is 1.5 eV (2.4 × 10⁻¹⁹ J).

Q4

Monochromatic light of wavelength 632.8 nm is produced by a helium-neon laser. The power emitted is 9.42 mW. (a) Find the energy and momentum of each photon in the light beam, (b) How many photons per second, on the average, arrive at a target irradiated by this beam? (Assume the beam to have uniform cross-section which is less than the target area), and (c) How fast does a hydrogen atom have to travel in order to have the same momentum as that of the photon?

Answer

Concept and context. In the photon picture of light (NCERT Section 11.7) a beam of monochromatic light of wavelength λ (frequency ν = c/λ) consists of photons, each carrying energy E = hν = hc/λ and momentum p = h/λ = E/c, independent of the intensity of the beam. The intensity (power) of the beam is determined by the number of photons per second N: P = N E. Photons are electrically neutral and always move with the speed c.

Given: λ = 632.8 nm = 6.328 × 10⁻⁷ m; P = 9.42 mW = 9.42 × 10⁻³ W; h = 6.63 × 10⁻³⁴ J s; c = 3.0 × 10⁸ m s⁻¹; m_H = 1.67 × 10⁻²⁷ kg.

(a) Energy and momentum of each photon

  1. Energy: E = hc/λ = (6.63 × 10⁻³⁴ × 3.0 × 10⁸)/(6.328 × 10⁻⁷) = 3.14 × 10⁻¹⁹ J = 3.14 × 10⁻¹⁹/1.6 × 10⁻¹⁹ = 1.96 eV.
  2. Momentum: p = h/λ = (6.63 × 10⁻³⁴)/(6.328 × 10⁻⁷) = 1.05 × 10⁻²⁷ kg m s⁻¹ (= E/c ✓).

(b) Number of photons per second

  1. P = N E ⇒ N = P/E = (9.42 × 10⁻³)/(3.14 × 10⁻¹⁹) = 3.0 × 10¹⁶ photons per second.

(c) Speed of a hydrogen atom with the same momentum

  1. p = m_H v ⇒ v = p/m_H = (1.05 × 10⁻²⁷)/(1.67 × 10⁻²⁷) = 0.63 m s⁻¹ (about 63 cm s⁻¹).
QuantityValue
Photon energy3.14 × 10⁻¹⁹ J = 1.96 eV
Photon momentum1.05 × 10⁻²⁷ kg m s⁻¹
Photons per second3.0 × 10¹⁶ s⁻¹
Speed of H atom with equal momentum0.63 m s⁻¹
  • Observation: although 3 × 10¹⁶ photons arrive per second, each carries a tiny momentum; a hydrogen atom moving at a leisurely 0.63 m s⁻¹ has as much momentum as a visible-light photon — which is why light exerts only a very small radiation pressure.
  • Colour: 632.8 nm is the red line of the He–Ne laser (photon energy 1.96 eV).
Exam tip: Use E = hc/λ, p = h/λ, N = P/E and v = p/m. Keep nm → m and mW → W conversions.

Conclusion: (a) each photon has energy 3.14 × 10⁻¹⁹ J (1.96 eV) and momentum 1.05 × 10⁻²⁷ kg m s⁻¹; (b) 3.0 × 10¹⁶ photons arrive per second; (c) a hydrogen atom needs a speed of 0.63 m s⁻¹ to have the same momentum.

Q5

In an experiment on photoelectric effect, the slope of the cut-off voltage versus frequency of incident light is found to be 4.12 × 10⁻¹⁵ V s. Calculate the value of Planck’s constant.

Answer

Concept and context. Einstein’s photoelectric equation gives K_max = hν − φ₀ and, since K_max = eV₀, V₀ = (h/e) ν − φ₀/e. Hence the graph of the cut-off (stopping) voltage V₀ against the frequency ν of the incident light is a straight line with slope h/e and an intercept on the frequency axis equal to the threshold frequency ν₀ = φ₀/h (NCERT Fig. 11.5). This was the basis of Millikan’s precise measurement of Planck’s constant and the proof of Einstein’s equation. Knowing e, the slope immediately yields h.

Cut-off voltage versus frequency: the slope of the line is h/e = 4.12 x 10^-15 V s, giving h = 6.6 x 10^-34 J sν (10¹⁴ Hz) →V₀ (volt)012345678910012345ν₀ = 3ΔV₀/Δν = 4.12 × 10⁻¹⁵ V scut-off voltage versus frequency: the slope of the straight line gives h/eh = e × slope = 1.6 × 10⁻¹⁹ × 4.12 × 10⁻¹⁵ = 6.59 × 10⁻³⁴ J s© iBioKaare
Fig. — cut-off voltage versus frequency of incident light: the slope of the straight line equals h/e (compare NCERT Fig. 11.5) (original iBioKaare schematic). Compare with NCERT textbook — Fig. 11.5, page 6 ↗

Given: slope = ΔV₀/Δν = h/e = 4.12 × 10⁻¹⁵ V s; e = 1.6 × 10⁻¹⁹ C.

  1. Relation: V₀ = (h/e)ν − φ₀/e, so slope = h/e.
  2. Planck’s constant: h = e × slope = (1.6 × 10⁻¹⁹ C) × (4.12 × 10⁻¹⁵ V s).
  3. h = 6.59 × 10⁻³⁴ C V s = 6.59 × 10⁻³⁴ J s (since C V = J).

h = e × (slope) ≈ 6.6 × 10⁻³⁴ J s

  • Check: the accepted value is 6.63 × 10⁻³⁴ J s (so the slope of the ideal line is 4.14 × 10⁻¹⁵ V s) — the experimental value agrees to within 1 %.
  • Significance: the slope is the same for every metal (universal constant h/e); only the intercept ν₀ differs from metal to metal (it depends on φ₀) — different metals give parallel lines.
Exam tip: State slope = h/e from V₀ = (h/e)ν − φ₀/e, then multiply by e. The units V s × C = J s.

Conclusion: Planck’s constant h = e × slope = 6.59 × 10⁻³⁴ J s (≈ 6.6 × 10⁻³⁴ J s).

Q6

The threshold frequency for a certain metal is 3.3 × 10¹⁴ Hz. If light of frequency 8.2 × 10¹⁴ Hz is incident on the metal, predict the cut-off voltage for the photoelectric emission.

Answer

Concept and context. The threshold frequency ν₀ is the minimum frequency of the incident radiation that can eject electrons from a metal: hν₀ = φ₀ (work function). For ν > ν₀ the emitted electrons have the maximum kinetic energy K_max = h(ν − ν₀) (Einstein’s equation), and the cut-off (stopping) voltage is the retarding potential that just stops them: eV₀ = K_max = h(ν − ν₀) (NCERT Fig. 11.5). Since 8.2 × 10¹⁴ Hz > 3.3 × 10¹⁴ Hz, photoemission occurs.

Stopping potential versus frequency for a metal with threshold frequency 3.3 x 10^14 Hz: V0 = 2.03 V at 8.2 x 10^14 Hzν (10¹⁴ Hz) →V₀ (volt)0123456789100123ν₀ = 3.3ν = 8.2 × 10¹⁴ Hz: V₀ = 2.03 Vmetal with threshold frequency 3.3 × 10¹⁴ Hz: stopping potential versus frequencyV₀ = h(ν − ν₀)/e = 4.14 × 10⁻¹⁵ × (8.2 − 3.3) × 10¹⁴ = 2.03 V© iBioKaare
Fig. — stopping potential versus frequency for the metal (threshold 3.3 × 10¹⁴ Hz): a straight line of slope h/e (compare NCERT Fig. 11.5) (original iBioKaare schematic). Compare with NCERT textbook — Fig. 11.5, page 6 ↗

Given: ν₀ = 3.3 × 10¹⁴ Hz; ν = 8.2 × 10¹⁴ Hz; h = 6.63 × 10⁻³⁴ J s; e = 1.6 × 10⁻¹⁹ C.

  1. Einstein’s equation: eV₀ = hν − hν₀ = h(ν − ν₀).
  2. ν − ν₀ = (8.2 − 3.3) × 10¹⁴ = 4.9 × 10¹⁴ Hz.
  3. V₀ = h(ν − ν₀)/e = (6.63 × 10⁻³⁴ × 4.9 × 10¹⁴)/(1.6 × 10⁻¹⁹) = (3.25 × 10⁻¹⁹)/(1.6 × 10⁻¹⁹) = 2.03 V.

V₀ = h(ν − ν₀)/e ≈ 2.0 V

QuantityValue
hν5.44 × 10⁻¹⁹ J = 3.40 eV
hν₀ = φ₀2.19 × 10⁻¹⁹ J = 1.37 eV
K_max = h(ν − ν₀)3.25 × 10⁻¹⁹ J = 2.03 eV
Cut-off voltage2.03 V
  • Check: (h/e)(ν − ν₀) = 4.14 × 10⁻¹⁵ V s × 4.9 × 10¹⁴ Hz = 2.03 V ✓.
  • Increasing the intensity would not change this cut-off voltage.
Exam tip: Use eV₀ = h(ν − ν₀); the slope h/e = 4.14 × 10⁻¹⁵ V s gives a quick check.

Conclusion: the cut-off voltage is ≈ 2.0 V (2.03 V).

Q7

The work function for a certain metal is 4.2 eV. Will this metal give photoelectric emission for incident radiation of wavelength 330 nm?

Answer

Concept and context. Photoelectric emission occurs only if the energy of a single incident photon, E = hν = hc/λ, is at least equal to the work function φ₀ of the metal: hν ≥ φ₀ (equivalently ν ≥ ν₀ or λ ≤ λ₀ = hc/φ₀, the threshold wavelength). If hν < φ₀ no electron can escape, however intense the light and however long it shines (NCERT Section 11.6) — an electron absorbs only one photon at a time. A convenient relation: E (eV) = 1240/λ (nm).

  1. Photon energy: E = hc/λ = (6.63 × 10⁻³⁴ × 3.0 × 10⁸)/(330 × 10⁻⁹) = 6.03 × 10⁻¹⁹ J = 6.03 × 10⁻¹⁹/1.6 × 10⁻¹⁹ = 3.77 eV (= 1240/330).
  2. Compare with the work function: E = 3.77 eV < φ₀ = 4.2 eV.
  3. Conclusion: the photon energy is insufficient to liberate an electron: no photoelectric emission takes place.
  4. Check by threshold wavelength: λ₀ = hc/φ₀ = 1240/4.2 = 295 nm; the incident wavelength 330 nm > λ₀ (≈ 295 nm), i.e. the frequency 9.1 × 10¹⁴ Hz < ν₀ = 1.01 × 10¹⁵ Hz.

E = 3.77 eV < φ₀ = 4.2 eV ⇒ no photoelectric emission

QuantityValue
Work function φ₀4.2 eV
Photon energy at 330 nm3.77 eV
Threshold wavelength λ₀ = hc/φ₀295 nm
Threshold frequency ν₀1.01 × 10¹⁵ Hz
Emission?No (λ = 330 nm > λ₀)
  • What would work? Ultraviolet light of wavelength shorter than 295 nm (e.g. 250 nm: E = 4.96 eV ⇒ K_max = 0.76 eV).
  • Why not a stronger beam? Increasing the intensity increases the number of photons but not the energy of each; with the wave picture one would expect emission eventually — but experiments show none (the failure of the wave theory, NCERT Section 11.5).
Exam tip: Compare hν (in eV = 1240/λ in nm) with φ₀ — a one-line decisive test. Mention the threshold wavelength 295 nm.

Conclusion: the photon energy (3.77 eV) is less than the work function (4.2 eV), so the metal will not give photoelectric emission for radiation of wavelength 330 nm.

Q8

Light of frequency 7.21 × 10¹⁴ Hz is incident on a metal surface. Electrons with a maximum speed of 6.0 × 10⁵ m/s are ejected from the surface. What is the threshold frequency for photoemission of electrons?

Answer

Concept and context. Einstein’s equation relates the incident frequency, the threshold frequency and the maximum kinetic energy of the photoelectrons: hν = hν₀ + ½ m v²_max, i.e. K_max = ½ m v²_max = h(ν − ν₀). Given the incident frequency and the maximum speed of the emitted electrons we can find ν₀ (and hence the work function φ₀ = hν₀).

Given: ν = 7.21 × 10¹⁴ Hz; v_max = 6.0 × 10⁵ m s⁻¹; m = 9.11 × 10⁻³¹ kg; h = 6.63 × 10⁻³⁴ J s.

  1. Maximum kinetic energy: K_max = ½ m v²_max = ½ × 9.11 × 10⁻³¹ × (6.0 × 10⁵)² = ½ × 9.11 × 10⁻³¹ × 3.6 × 10¹¹ = 1.64 × 10⁻¹⁹ J (≈ 1.02 eV).
  2. Photon energy: hν = 6.63 × 10⁻³⁴ × 7.21 × 10¹⁴ = 4.78 × 10⁻¹⁹ J.
  3. Work function: φ₀ = hν − K_max = 4.78 × 10⁻¹⁹ − 1.64 × 10⁻¹⁹ = 3.14 × 10⁻¹⁹ J (≈ 1.96 eV).
  4. Threshold frequency: ν₀ = φ₀/h = (3.14 × 10⁻¹⁹)/(6.63 × 10⁻³⁴) = 4.74 × 10¹⁴ Hz (≈ 4.7 × 10¹⁴ Hz).

ν₀ = ν − m v²_max/(2h) ≈ 4.7 × 10¹⁴ Hz

QuantityValue
hν4.78 × 10⁻¹⁹ J (2.99 eV)
K_max1.64 × 10⁻¹⁹ J (1.02 eV)
φ₀ = hν₀3.14 × 10⁻¹⁹ J (1.96 eV)
ν₀4.74 × 10¹⁴ Hz
λ₀ = c/ν₀633 nm (red)
  • Check: ν = 7.21 × 10¹⁴ Hz > ν₀ = 4.74 × 10¹⁴ Hz ✓ (emission occurs); the metal responds to visible (red) light like the alkali metals.
  • The speed 6 × 10⁵ m s⁻¹ is non-relativistic (0.2 % of c).
Exam tip: Find K_max from the speed, subtract from hν to get φ₀, then ν₀ = φ₀/h (or ν₀ = ν − K_max/h).

Conclusion: the threshold frequency for photoemission is ≈ 4.7 × 10¹⁴ Hz (4.74 × 10¹⁴ Hz).

Q9

Light of wavelength 488 nm is produced by an argon laser which is used in the photoelectric effect. When light from this spectral line is incident on the emitter, the stopping (cut-off) potential of photoelectrons is 0.38 V. Find the work function of the material from which the emitter is made.

Answer

Concept and context. By Einstein’s photoelectric equation the photon energy hν = hc/λ is shared between the work function φ₀ and the maximum kinetic energy of the photoelectrons; the maximum kinetic energy is measured by the stopping potential: K_max = eV₀. Hence φ₀ = hc/λ − eV₀. Working in electron-volts: hc = 1240 eV nm, and eV₀ numerically equals V₀ in volts.

Given: λ = 488 nm; V₀ = 0.38 V; hc = 1240 eV nm (= 1.99 × 10⁻²⁵ J m).

  1. Photon energy: E = hc/λ = 1240/488 = 2.54 eV (= 4.07 × 10⁻¹⁹ J).
  2. Maximum kinetic energy: K_max = eV₀ = 0.38 eV.
  3. Work function: φ₀ = E − K_max = 2.54 − 0.38 = 2.16 eV (≈ 3.46 × 10⁻¹⁹ J).

φ₀ = hc/λ − eV₀ = 2.54 − 0.38 = 2.16 eV

QuantityValue
Photon energy hc/λ2.54 eV
eV₀0.38 eV
Work function φ₀2.16 eV
Threshold wavelength λ₀ = 1240/2.16574 nm (yellow-green)
  • Interpretation: φ₀ ≈ 2.2 eV is typical of alkali metals such as caesium (2.14 eV) or potassium (2.3 eV) which respond to visible light; the blue-green light of the argon laser has enough energy.
  • Check: the stopping potential for a green line of wavelength 546 nm for this metal would be 1240/546 − 2.16 = 0.11 V — decreasing with the wavelength as expected.
Exam tip: Use hc = 1240 eV nm: E = 1240/488 = 2.54 eV; φ₀ = E − eV₀ = 2.16 eV.

Conclusion: the work function of the emitter material is 2.16 eV.

Q10

What is the de Broglie wavelength of (a) a bullet of mass 0.040 kg travelling at the speed of 1.0 km/s, (b) a ball of mass 0.060 kg moving at a speed of 1.0 m/s, and (c) a dust particle of mass 1.0 × 10⁻⁹ kg drifting with a speed of 2.2 m/s?

Answer

Concept and context. Louis de Broglie (1924) proposed that a moving particle of mass m and speed v has an associated matter wave of wavelength λ = h/p = h/(mv) (NCERT Eq. 11.5), where h = 6.63 × 10⁻³⁴ J s is Planck’s constant. The wavelength is smaller for a heavier or faster particle. For ordinary macroscopic objects, h is so small compared with their momentum that λ is far smaller than any measurable length, which is why no wave-like behaviour is noticed in everyday life (NCERT: the wave character is significant only in the sub-atomic domain).

Given: h = 6.63 × 10⁻³⁴ J s.

  1. (a) Bullet: m = 0.040 kg, v = 1.0 km s⁻¹ = 1000 m s⁻¹ ⇒ p = mv = 40 kg m s⁻¹; λ = h/p = 6.63 × 10⁻³⁴/40 = 1.7 × 10⁻³⁵ m.
  2. (b) Ball: m = 0.060 kg, v = 1.0 m s⁻¹ ⇒ p = 0.060 kg m s⁻¹; λ = 6.63 × 10⁻³⁴/0.060 = 1.1 × 10⁻³² m.
  3. (c) Dust particle: m = 1.0 × 10⁻⁹ kg, v = 2.2 m s⁻¹ ⇒ p = 2.2 × 10⁻⁹ kg m s⁻¹; λ = 6.63 × 10⁻³⁴/(2.2 × 10⁻⁹) = 3.0 × 10⁻²⁵ m.
ObjectMass (kg)Speed (m/s)Momentum (kg m/s)de Broglie wavelength
Bullet0.0401000401.7 × 10⁻³⁵ m
Ball0.0601.00.0601.1 × 10⁻³² m
Dust particle1.0 × 10⁻⁹2.22.2 × 10⁻⁹3.0 × 10⁻²⁵ m
Electron at 5.4 × 10⁶ m/s (NCERT Ex. 11.3)9.11 × 10⁻³¹5.4 × 10⁶4.9 × 10⁻²⁴1.35 × 10⁻¹⁰ m (X-ray scale)
  • Meaning: these wavelengths are 10²⁰–10¹⁰ times smaller than a proton (~10⁻¹⁵ m) or an atom (10⁻¹⁰ m) and are quite beyond measurement; no diffraction or interference of such objects can ever be observed, so classical mechanics is perfectly adequate for them. Compare the electron, whose wavelength 0.135 nm equals X-ray wavelengths and can be diffracted by crystals.
  • Rule: λ ∝ 1/(mv): smaller for heavier and faster objects; the bullet (fastest, heaviest) has the smallest wavelength here.
Exam tip: λ = h/mv with SI units: convert 1.0 km/s to 1000 m/s. Comment that these wavelengths are unobservably small.

Conclusion: the de Broglie wavelengths are (a) 1.7 × 10⁻³⁵ m, (b) 1.1 × 10⁻³² m, (c) 3.0 × 10⁻²⁵ m — all immeasurably small, so macroscopic objects show no wave-like behaviour.

Q11

Show that the wavelength of electromagnetic radiation is equal to the de Broglie wavelength of its quantum (photon).

Answer

Concept and context. The de Broglie relation λ = h/p was proposed for material particles; its validity can be tested only by experiment. However, it is interesting that it is also satisfied by a photon, the quantum of electromagnetic radiation: a photon of frequency ν and wavelength λ carries energy E = hν and momentum p = E/c = hν/c (NCERT Section 11.7: Einstein’s result that a light quantum has momentum hν/c). The de Broglie wavelength of the photon, defined as h/p, should therefore equal the wavelength of the electromagnetic wave.

Photon energy E = hν→Photon momentum p = E/c = hν/c→de Broglie wavelength λ_dB = h/p = h c/(hν)→λ_dB = c/ν→c/ν = λ of the electromagnetic radiation

Proof

  1. Wave relation: for electromagnetic radiation in vacuum c = νλ ⇒ λ = c/ν.
  2. Photon momentum: from special relativity (or Einstein’s photon concept) for a particle of zero rest mass E = pc ⇒ p = E/c = hν/c.
  3. de Broglie wavelength: λ_dB = h/p = h/(hν/c) = c/ν.
  4. Compare: λ_dB = c/ν = λ. Hence the de Broglie wavelength of a photon equals the wavelength of the electromagnetic radiation of which it is the quantum. Q.E.D.

λdB = h/p = h/(hν/c) = c/ν = λ

PropertyPhotonMatter particle
EnergyE = hν = hc/λE = p²/2m (non-relativistic)
Momentump = hν/c = h/λp = mv
Wavelengthλ = h/p (identical to the em wavelength)λ = h/p (de Broglie)
  • Example: for a photon of green light, λ = 500 nm, p = h/λ = 1.33 × 10⁻²⁷ kg m s⁻¹ and E = 2.5 eV: the “particle” attribute (momentum) and the “wave” attribute (λ) are connected by the same relation h = pλ.
  • Significance: the dual nature of radiation and matter is described by one relation λ = h/p, with Planck’s constant as the bridge.
Exam tip: Three lines: E = hν; p = E/c = hν/c; λ_dB = h/p = c/ν = λ.

Conclusion: with p = hν/c for a photon, the de Broglie wavelength λ = h/p = c/ν, which is exactly the wavelength of the electromagnetic radiation.

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