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Exercise:
In astrophysics so called radio recombination lines i.e. transitions from high n states to lower states are routinely observed. The observed spectral lines for hydrogen are labelled Hnalpha for transitions nto n-. vspacemm Calculate the wavelength for the Halpha line.

Solution:
The photon energy is E_gamma E_leftfracn^-fracn-^ right E_fracn-^-n^n^n-^ E_ frac-n+nn-^ frachclambda Solving for the wavelength yields lambda laF frachcEgr times fracntimesn+^-timesn+ resultlaP-
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Exercise:
In astrophysics so called radio recombination lines i.e. transitions from high n states to lower states are routinely observed. The observed spectral lines for hydrogen are labelled Hnalpha for transitions nto n-. vspacemm Calculate the wavelength for the Halpha line.

Solution:
The photon energy is E_gamma E_leftfracn^-fracn-^ right E_fracn-^-n^n^n-^ E_ frac-n+nn-^ frachclambda Solving for the wavelength yields lambda laF frachcEgr times fracntimesn+^-timesn+ resultlaP-
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Attributes & Decorations
Branches
quantum physics
Tags
energy level, hydrogen, photon, wavelength
Difficulty
(2, default)
Points
0 (default)
Language
ENG (English)
Type
Calculative / Quantity
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