Since we need to consider the photon with the longest wavelength that ends the electron transition in the state with the quantum number n=2 , this will be transition 3−2 since the photon energy formula E=h×λc , (where h is the Planck constant, c is the speed of light, and λ is the wavelength) shows that the photon energy is inversely proportional to the wavelength, and since a larger transition corresponds to a large absorption/release of energy, we choose the smallest transition (transition 1−2> transitions 2−3 ). By the formula λ1=R×(m21−n21) (where R is the Rydberg constant, and n and m are the quantum numbers of the photon state) λ1=3.29×1015×(221−321) =365×3.29×1015 therefore λ=5×3.29×101536=2.19×10−15 m.
E=6.63×10−34×2.19×10−153×108=9.08×10−11 J.
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