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Exercises · 2.20

Q.Calculate the wavelength of an electron moving with a velocity of 2.05×107 m s−12.05 \times 10^{7}\ m\ s^{-1}.

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The de Broglie wavelength of a moving particle is given by λ=h/p\lambda = h / p, where pp is the momentum. For an electron at 2.05×107 m/s2.05 \times 10^{7}\ \text{m/s}, the wavelength comes out to 3.55×10−11 m3.55 \times 10^{-11}\ \text{m}.

The idea here is the de Broglie hypothesis — that every moving particle has a wave associated with it. For an electron, which has a tiny mass, even a moderate speed gives a measurable wavelength. The formula is straightforward: λ=hmv\lambda = \frac{h}{mv}, where hh is Planck’s constant, mm is the electron’s mass, and vv is its velocity.

Let’s work through it.

  1. Write down what’s given.

    Velocity, v=2.05×107 m/sv = 2.05 \times 10^{7}\ \text{m/s}.

    Mass of an electron, me=9.1×10−31 kgm_e = 9.1 \times 10^{-31}\ \text{kg} (standard value).

    Planck’s constant, h=6.626×10−34 J sh = 6.626 \times 10^{-34}\ \text{J s}.

  2. Recall the de Broglie relation.

    λ=hp=hmv\lambda = \frac{h}{p} = \frac{h}{mv}

    This is the central formula. No relativity needed here because vv is about 0.068c0.068c (well below 0.1c0.1c), so the classical momentum mvmv is accurate.

  3. Plug in the numbers.

    First, compute the momentum:

p=mv=(9.1×10−31)×(2.05×107)p = mv = (9.1 \times 10^{-31}) \times (2.05 \times 10^{7})

Multiply the coefficients: 9.1×2.05=18.6559.1 \times 2.05 = 18.655.

Multiply the powers of ten: 10−31×107=10−2410^{-31} \times 10^{7} = 10^{-24}.

So p=18.655×10−24=1.8655×10−23 kg m/sp = 18.655 \times 10^{-24} = 1.8655 \times 10^{-23}\ \text{kg m/s}.

  1. Now find the wavelength.

λ=hp=6.626×10−341.8655×10−23\lambda = \frac{h}{p} = \frac{6.626 \times 10^{-34}}{1.8655 \times 10^{-23}}

Divide the coefficients: 6.626/1.8655≈3.5526.626 / 1.8655 \approx 3.552.

Divide the powers: 10−34/10−23=10−1110^{-34} / 10^{-23} = 10^{-11}.

So λ≈3.552×10−11 m\lambda \approx 3.552 \times 10^{-11}\ \text{m}.

  1. Round to appropriate significant figures. …

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