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Question
The terminology of different parts of the electromagnetic spectrum is given in the text. Use the formula E=hν (for energy of a quantum of radiation: photon) and obtain the photon energy in units of eV for different parts of the electromagnetic spectrum. In what way are the different scales of photon energies that you obtain related to the sources of electromagnetic radiation?
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Solution
Photon energy (Forλ=1m)
=6.63×10−34×3×1081.6×10−19eV=1.24×10−6eV
Photon energy for other wavelengths in the figure for electromagnetic spectrum can be obtained by multiplying approximate powers often. Energy of a photon that a source produces indicates the spacings of the relevant energy levels of the source. For example, λ=10−12 corresponds to photon energy =1.24×106eV=1.24MeV This indicates that nuclear energy levels (transition between which causes γ-ray emission) are typically spaced by 1 MeV or so. Similarly, a visible wavelength λ=5×10−7m, corresponds to photon energy= 2.5 eV. This implies that energy levels (transition between which gives visible radiation) are typically spaced by a few eV.
=6.63×10−34×3×1081.6×10−19eV=1.24×10−6eV
Photon energy for other wavelengths in the figure for electromagnetic spectrum can be obtained by multiplying approximate powers often. Energy of a photon that a source produces indicates the spacings of the relevant energy levels of the source. For example, λ=10−12 corresponds to photon energy =1.24×106eV=1.24MeV This indicates that nuclear energy levels (transition between which causes γ-ray emission) are typically spaced by 1 MeV or so. Similarly, a visible wavelength λ=5×10−7m, corresponds to photon energy= 2.5 eV. This implies that energy levels (transition between which gives visible radiation) are typically spaced by a few eV.
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