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Exercises · 11.10

Q.Light of frequency 7.21×1014 Hz7.21 \times 10^{14}\ \text{Hz} is incident on a metal surface. Electrons with a maximum speed of 6.0×105 m/s6.0 \times 10^{5}\ \text{m/s} are ejected from the surface. What is the threshold frequency for photoemission of electrons?

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The threshold frequency is found by equating the maximum kinetic energy of ejected electrons to the difference between the incident photon energy and the work function. Using Kmax=hf−hf0K_{\text{max}} = hf - hf_0, we get f0=f−Kmaxhf_0 = f - \frac{K_{\text{max}}}{h}. The result is f0=4.74×1014 Hzf_0 = 4.74 \times 10^{14}\ \text{Hz}.

The core idea here is the photoelectric effect: when light hits a metal, each photon gives its energy hfhf to an electron. The electron uses some of that energy to escape the metal (the work function ϕ=hf0\phi = hf_0), and the rest becomes kinetic energy. The maximum kinetic energy occurs for electrons that escape without losing energy to collisions inside the metal.

So the equation is:

Kmax=hf−hf0K_{\text{max}} = hf - hf_0

where f0f_0 is the threshold frequency — the minimum frequency needed to eject any electron at all.

We know f=7.21×1014 Hzf = 7.21 \times 10^{14}\ \text{Hz} and the maximum speed vmax=6.0×105 m/sv_{\text{max}} = 6.0 \times 10^{5}\ \text{m/s}. We need f0f_0.

  1. Find the maximum kinetic energy. The kinetic energy is Kmax=12mevmax2K_{\text{max}} = \frac{1}{2} m_e v_{\text{max}}^2, where me=9.11×10−31 kgm_e = 9.11 \times 10^{-31}\ \text{kg} (electron mass).

Kmax=12(9.11×10−31)(6.0×105)2K_{\text{max}} = \frac{1}{2} (9.11 \times 10^{-31}) (6.0 \times 10^{5})^2

First square the speed: (6.0×105)2=3.6×1011(6.0 \times 10^{5})^2 = 3.6 \times 10^{11}.

Then multiply: 9.11×10−31×3.6×1011=3.2796×10−199.11 \times 10^{-31} \times 3.6 \times 10^{11} = 3.2796 \times 10^{-19}.

Half of that: Kmax=1.6398×10−19 JK_{\text{max}} = 1.6398 \times 10^{-19}\ \text{J}.

Tip

You can also work in electronvolts if you prefer, but joules are fine here since Planck's constant is in J·s. Just be consistent.

  1. Write the photoelectric equation.

hf=hf0+Kmaxhf = hf_0 + K_{\text{max}}

So

hf0=hf−Kmaxhf_0 = hf - K_{\text{max}}

and

f0=f−Kmaxhf_0 = f - \frac{K_{\text{max}}}{h}

  1. Plug in the numbers. Planck's constant h=6.626×10−34 J⋅sh = 6.626 \times 10^{-34}\ \text{J·s}. First compute hfhf:

hf=(6.626×10−34)(7.21×1014)=4.777×10−19 Jhf = (6.626 \times 10^{-34})(7.21 \times 10^{14}) = 4.777 \times 10^{-19}\ \text{J}

(Check: 6.626×7.21≈47.776.626 \times 7.21 \approx 47.77, and 10−34×1014=10−2010^{-34} \times 10^{14} = 10^{-20}, so 4.777×10−194.777 \times 10^{-19} — correct.) …

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