PHYSICS F/SCI.+ENGRS.,STAND.-W/ACCESS
PHYSICS F/SCI.+ENGRS.,STAND.-W/ACCESS
6th Edition
ISBN: 9781429206099
Author: Tipler
Publisher: MAC HIGHER
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Chapter 36, Problem 48P

(a)

To determine

The difference in energy between the two possible orientations of an electron in a magnetic field.

(b)

To determine

The wavelength of the photons needed for the electron spin resonance.

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In high static-magnetic field environment, such stellar interiors, the energy levels of a H-atom are modified in such a way that they depend on l and m in addition to n. In this problem assume that the eigenvectors of Ĥo, β and Î₂ are still the usual In, l, m), but the energy is eigenvalue is Enem O Ĥ Φ nem (r,0,0) = EnemÞµlm (1,0,0) 13.6eV ■ E 'nlm = +0.1m 1+ n 。 Znm (1,0,0) = l (l+1)ħ²Þntm (r,0,0) O Î₂nem (r,0,0) = mħÞ, Dnem (1,0,0) 1 2l+1 Consider the n = 2 level. Calculate the energy eigenvalues for all 4 states. Draw a stack of lines in order of increasing energy with the lowest one at the bottom
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Magnets and Magnetic Fields; Author: Professor Dave explains;https://www.youtube.com/watch?v=IgtIdttfGVw;License: Standard YouTube License, CC-BY