Short Topical Videos
Order of Magnitude Interaction of Radiation and Matter
We’ll start with the Bohr atom. We begin by quantizing angular momentum:
If we balance the force required to keep the in a circular orbit with the electric force:
A Rydberg is the energy required to ionize an H atom from the ground state. It is . We can estimate it by integrating the electric force from to , but in reality, there is another factor of 2:
Fine Structure comes from the interaction of the magnetic moment of the with the a caused by the Lorentz-transformed Coulomb field of the proton (generated by the ’s motion). The energy of a dipole interaction is , so we’d expect that:
To estimate B: , and ( is the fine structure constant):
Estimating : The of a dipole goes as , so , where is the classical radius. Estimating that the rest mass energy of the should be about the electrostatic potential energy left in the , :
We can estimate by reverting to Maxwell’s equation:
Again, we estimate that , and because the electron spin is quantized, . After some algebra, we get that:
(Bohr magneton for )
(Bohr magneton for nucleus) Getting back to the energy:
Instead of using the Bohr magneton, we use the intrinsic magnetic moment (spin) of the nucleus:
Note that Fine and Hyperfine are magnetic dipole transitions. level transitions are electric dipole transitions. Magnetic dipole transitions are generally weaker.
- Vibrational Transitions in Molecules:
Our general technique with vibrational transitions is to model them as harmonic oscillators. Thus, they should have the characteristic harmonic energy series:
For a harmonic oscillator, . We estimate that since the force for a spring is , and that force should be about the Coulomb force on ’s. If we say that atoms stretch with respect to each other about a Bohr radius:
where A is the atomic mass # of our atoms.
- Rotational Transitions in Molecules:
The thing to remember is that angular momentum comes in units of .