Question
Given below are some famous numbers associated with electromagnetic radiations in different contexts in physics. State the part of the electromagnetic spectrum to which each belongs.
  1. $21 \ cm \ ($wavelength emitted by atomic hydrogen in interstellar space$)$.
  2. $1057 MHz \ ($frequency of radiation arising from two close energy levels in hydrogen; known as Lamb shift$).$
  3. $2.7 K \ [$temperature associated with the isotropic radiation filling all space $-$ thought to be a relic of the ‘big $-$ bang’ origin of the universe$]$.
  4. $5890 \mathring A - 5896 \mathring A \ [$double lines of sodiu$]$
  5. $14.4 keV \ [$energy of a particular transition in ${57}Fe$ nucleus associated with a famous high resolution spectroscopic method $($Mössbauer spectroscopy$)].$

Answer

  1. Radio waves; it belongs to the short wavelength end of the electromagnetic spectrum.
  2. Radio waves; it belongs to the short wavelength end.
  3. Temperature $, T = 2.7 ^\circ K$
$\lambda_\text{m}$ is given by Planck's law as:
$\lambda_\text{m}=\frac{0.29}{2.7}=0.11 \ \text{ cm}$
This wavelength corresponds to microwaves.
  1. This is the yellow light of the visible spectrum.
  2. Transition energy is given by the relation,
$E = hv$
Where,
$h =$ Planck's constant $= 6.6 \times 10^{-34} Js$
$v =$ Frequency of radiation
Energy $,E = 14.4 K eV$
$\therefore \ \text{v}=\frac{\text{E}}{\text{h}}$
$=\frac{14.4\times10^3\times1.6\times10^{-19}}{6.6\times10{-34}}$
$= 3.4 \times 10^{18} Hz$
This corresponds to $X-$ rays.

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