by peter hill 14 years ago
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Bohr model
1. e- orbit + nucleus in 1/r^2 potential like planets.
a. circular orbits
b. does not radiate or decay
2. Electrons jump between orbits with photons E=hf
a. jump to closer orbit emit photon
b. jump to distant orbit absorb photon
(jump = disappear and rematterialize)
3. Orbits are restricted to l =nh/2p n = 1,2,3.....
(l is angular momentum = speed*mass * radius)
Summary of laws
Hydrogen lines
Explanation
HSC : 1/wavelength =R (1/n1^2-1/n2^2)
E(eV) = 13.6(1/n1^2- 1/n2^2)
wavelength = 91.15
(1/n1^2-1/n2^2)
= 91.15xn1^2xn2^2 / (n2^2-n1^2)