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Dual Nature of Radiation and Matter: NEET previous year questions

Every Dual Nature of Radiation and Matter question from the official NEET papers on this site, with the answer and a worked solution.

The questions come from NEET 2026, Re-NEET 2026 and NEET 2020. Each shows its answer and solution when you open it, so you can attempt it first. For what the chapter covers and how NEET tests it, see the Dual Nature of Radiation and Matter guide.

NEET 2026 · the full paper

  1. NEET 2026 · Q9

    Match List I with List II:

    List I

    List II

    P) E=hνE = h\nu

    I) de Broglie wavelength

    Q) Diffraction and Interference

    II) Particle nature of light

    R) λ=h/p\lambda = h/p

    III) Wave nature of light

    S) Compton effect

    IV) Energy of photon

    Choose the correct answer from the options given below:

    1. (1)

      P-IV, Q-I, R-II, S-III

    2. (2)

      P-IV, Q-III, R-II, S-I

    3. (3)

      P-I, Q-IV, R-III, S-II

    4. (4)

      P-IV, Q-III, R-I, S-II

    Answer and solution

    Answer: (4)

    E=hνE = h\nu gives the energy of a photon (IV); diffraction and interference demonstrate the wave nature of light (III); λ=h/p\lambda = h/p is the de Broglie wavelength of a particle (I); and the Compton effect confirms the particle nature of light (II). Hence P-IV, Q-III, R-I, S-II, which is option (4).

  2. NEET 2026 · Q42

    For a metal of work function 6.6 eV6.6\ \text{eV}, which of the following wavelengths of incident radiation does not give rise to the photoelectric effect? (Take Planck's constant as 6.6×10−34 J s6.6 \times 10^{-34}\ \text{J s})

    1. (1)

      100 nm

    2. (2)

      150 nm

    3. (3)

      200 nm

    4. (4)

      50 nm

    Answer and solution

    Answer: (3)

    Photoemission requires photon energy hcλ≥W0\dfrac{hc}{\lambda} \geq W_0, i.e. wavelength λ≤hcW0\lambda \leq \dfrac{hc}{W_0}. Here hcW0=6.6×10−34×3×1086.6×1.6×10−19≈187.5 nm\dfrac{hc}{W_0} = \dfrac{6.6\times10^{-34}\times3\times10^{8}}{6.6\times1.6\times10^{-19}} \approx 187.5\ \text{nm}. Any wavelength longer than this cannot eject electrons; 200 nm>187.5 nm200\ \text{nm} > 187.5\ \text{nm}, so it produces no photoelectric effect.

Re-NEET 2026 · the full paper

  1. Re-NEET 2026 · Q8

    A beam of light falls on a metal surface such that photo-electrons are generated. If power of the light source starts to decrease linearly with time tt, then variation of the photocurrent II and magnitude of the stopping potential ∣V∣|V| with time is best represented by:

    1. (1)
      opt A
    2. (2)
      opt B
    3. (3)
      opt C
    4. (4)
      opt D
    Answer and solution

    Answer: (1)

    Photocurrent is set by the NUMBER of photons striking the surface per second, so it is proportional to the source power and falls linearly with tt. Stopping potential, by contrast, depends only on the maximum kinetic energy of the emitted electrons, eV0=hν−ϕ0eV_0 = h\nu - \phi_0, which is fixed by the FREQUENCY and the work function - neither of which changes here. So ∣V∣|V| stays flat while II decays. NCERT Class 12, Dual Nature of Radiation and Matter.

    Why the other options are wrong:

    - (2) treats stopping potential as intensity-dependent, the single most common photoelectric misconception
    - (3) swaps the roles entirely, tying current to frequency and stopping potential to intensity
    - (4) assumes neither quantity responds to the source, ignoring that current tracks photon flux

  2. Re-NEET 2026 · Q18

    A ray of light with wavelength λ\lambda is incident on three different photoelectric cells namely 1, 2 and 3. The threshold wavelength of these photoelectric cells are λ1\lambda_1, λ2\lambda_2, and λ3\lambda_3, respectively and the magnitude of stopping potentials of these cells are V1V_1, V2V_2 and V3V_3, respectively. The relation between λ\lambda and threshold wavelengths are λ1<λ\lambda_1 < \lambda, λ2>λ\lambda_2 > \lambda and λ3≫λ\lambda_3 \gg \lambda. The correct option is:

    1. (1)

      V1=0, V2<V3V_1 = 0,\ V_2 < V_3

    2. (2)

      V1=0, V2>V3V_1 = 0,\ V_2 > V_3

    3. (3)

      V1>V2, V3=0V_1 > V_2,\ V_3 = 0

    4. (4)

      V1<V2, V3=0V_1 < V_2,\ V_3 = 0

    Answer and solution

    Answer: (1)

    Emission occurs only when the incident wavelength is SHORTER than the threshold wavelength. Cell 1 has λ1<λ\lambda_1 < \lambda, so the photons are too weak and V1=0V_1 = 0. For the other two, eV0=hc(1λ−1λth)eV_0 = hc\left(\frac{1}{\lambda} - \frac{1}{\lambda_{th}}\right); a LARGER threshold wavelength means a smaller work function and hence a larger stopping potential. Since λ3≫λ2\lambda_3 \gg \lambda_2, the term 1/λ31/\lambda_3 is nearly zero and V3>V2V_3 > V_2. NCERT Class 12, Dual Nature of Radiation and Matter (Einstein's photoelectric equation).

  3. Re-NEET 2026 · Q19

    A photon and an electron, each of 20 eV energy, move in free space. The ratio of linear momentum of electron pep_e to that of photon pPhp_{Ph}, pepPh\frac{p_e}{p_{Ph}} is: [Take speed of light = 3×108 ms−13 \times 10^8\ \text{ms}^{-1}, charge of electron = −1.6×10−19-1.6 \times 10^{-19} C and mass of electron = 9×10−319 \times 10^{-31} kg]

    1. (1)

      2450\frac{2}{450}

    2. (2)

      1250\frac{1}{250}

    3. (3)

      225

    4. (4)

      275

    Answer and solution

    Answer: (3)

    A photon's momentum is p=Ec=20×1.6×10−193×108≈1.07×10−26 kg m s−1p = \frac{E}{c} = \frac{20 \times 1.6 \times 10^{-19}}{3 \times 10^8} \approx 1.07 \times 10^{-26}\ \text{kg m s}^{-1}. A non-relativistic electron of the same kinetic energy has p=2mE=2(9×10−31)(3.2×10−18)=2.4×10−24 kg m s−1p = \sqrt{2mE} = \sqrt{2(9 \times 10^{-31})(3.2 \times 10^{-18})} = 2.4 \times 10^{-24}\ \text{kg m s}^{-1}. The ratio is therefore about 225 - a massive particle carries far more momentum than a photon of the same energy, because p∝Ep \propto \sqrt{E} for matter but p∝Ep \propto E for light. NCERT Class 12, Dual Nature of Radiation and Matter.

NEET 2020 · the full paper

  1. NEET 2020 · Q143

    An electron is accelerated from rest through a potential difference of V volt. If the de Broglie wavelength of the electron is 1.227 × 10⁻² nm, the potential difference is

    1. (1)

      102^{2} V

    2. (2)

      103^{3} V

    3. (3)

      104^{4} V

    4. (4)

      10 V

    Answer and solution

    Answer: (3)

    For an electron, λ\lambda(nm) = 1.227/V\sqrt{V}. Setting λ=1.227×10−2\lambda = 1.227 \times 10^{-2} nm gives V\sqrt{V} = 100 and V = 104^{4} V. Chapter: Dual Nature of Radiation and Matter.

  2. NEET 2020 · Q146

    Light of frequency 1.5 times the threshold frequency is incident on a photosensitive material. What will be the photoelectric current if the frequency is halved and intensity is doubled?

    1. (1)

      four times

    2. (2)

      one-fourth

    3. (3)

      zero

    4. (4)

      doubled

    Answer and solution

    Answer: (3)

    The new frequency is 0.75ν0_{0}, below the threshold ν0_{0}. No electrons are emitted irrespective of the doubled intensity, so the photoelectric current is zero. Chapter: Dual Nature of Radiation and Matter.

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Questions

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