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NCERT Exemplar · Q24

Q.Relativistic corrections become necessary when the expression for the kinetic energy 12mv2\frac{1}{2}mv^2 becomes comparable with mc2mc^2, where mm is the mass of the particle. At what de Broglie wavelength will relativistic corrections become important for an electron?

(a) λ=10 nm\lambda = 10\ \text{nm}
(b) λ=10−1 nm\lambda = 10^{-1}\ \text{nm}
(c) λ=10−4 nm\lambda = 10^{-4}\ \text{nm}
(d) λ=10−6 nm\lambda = 10^{-6}\ \text{nm}
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Relativistic corrections set in when 12mv2∼mc2\tfrac{1}{2}mv^2\sim mc^2, i.e. when the de Broglie wavelength falls to about the electron's Compton wavelength (∼10−3\sim 10^{-3} nm). Among the options the picometre-range choice is (C) 10−410^{-4} nm.

When do relativistic corrections matter?

Newtonian kinetic energy 12mv2\tfrac{1}{2}mv^2 is a good approximation only while it is small compared with the rest energy mc2mc^2. Corrections become important when the two are comparable:

12mv2∼mc2.\frac{1}{2}mv^2 \sim mc^2.

Turn the condition into a wavelength

Write the kinetic energy through the momentum, K=p22mK=\dfrac{p^2}{2m}, and set it comparable to mc2mc^2:

p22m∼mc2⇒p∼2 mc.\frac{p^2}{2m}\sim mc^2 \quad\Rightarrow\quad p\sim\sqrt{2}\,mc.

The de Broglie wavelength at this momentum is

λ=hp∼h2 mc,\lambda = \frac{h}{p} \sim \frac{h}{\sqrt{2}\,mc},

which is essentially the electron's Compton wavelength λC=hmc\lambda_C=\dfrac{h}{mc} (up to the factor 2\sqrt{2}).

Put in the numbers

λ∼6.63×10−342 (9.11×10−31)(3×108)≈1.7×10−12 m=1.7×10−3 nm.\lambda \sim \frac{6.63\times10^{-34}}{\sqrt{2}\,(9.11\times10^{-31})(3\times10^{8})} \approx 1.7\times10^{-12}\ \text{m} = 1.7\times10^{-3}\ \text{nm}. …

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