The Zeeman Effect.

Contents

*   Theory

*   Interesting and Helpful  Links

 

Theory

There are three quantum numbers that are needed to solve the Schroedinger equation for stationary states. They are n,l and m. For atoms with the inner shells filled, or they screen the coulomb potential, the energy of these eigenstates only depends on n and l but not on m. This means that there are degenerate energy states, that is, there are more than one state with the same energy value for that one value of m.

In the presence of an external magnetic field the energy is changed. The energy of one of these states is given by the equation where H is the external field. The angle between L and H is quantized so it can only take 2l + 1 values. Not a continum of values.  For an explanation of discrete values. The application of the external field lifts the degeneracy and splits the energy levels. See below.

The far left lines are two energy levels that are unsplit. They are then split into 3 and 5 lines respectivly in the middle of the picture when an extenal field is added, field not shown. On the right the picture shows the allowed transitons.

Note all energy spacings are equal, that is a = b.

 
 

The light that is emitted by these transitions will make spectrum lines when observed. This spectrum is from what is called the normal Zeeman effect.

There is also the Anomolous Zeeman effect. This arrises when the Magnetic moment of the electron is taken into effect. The spin angular momentum of the electron  S is coupled to the Angular momentum by the relation J = L + S. The consequence of this is that the energy levels  now are not equidistant. Now the energy levels are given by the equation  where g is the Lande g factor. For an explanation of this energy  The result of this equation is that now the energy is dependant on (gμH) which is constant, but also in mj which is no longer constant. This results in more lines and lines that are not of the same energy.

For lines see picture below.

On the left is the Normal Zeeman effect. The one line is split into three when an external field is added.

On the right is the Anomalous Zeeman effect that takes electron spin into account.

 
 

One interesting fact about the Zeeman effectg is that the light has differing polarization depending on wheather it is viewed parallel to or normal to the external magnetic field. When viewed parallel to field the light is linearly polarized. When viewed normal to field the light is circularly polarized.

See picture below.                

 

For explanation and experimental setup

 

 

Interesting and Helpful Links

Another good theory explanation and experimental setup

For how Zeeman is used in astronomy

For how Zeeman is used in Atomic Spectra

Paper on use of Zeeman in stellar CN cloud investigation

How Zeeman is used to investigate stellar magnetic fields

Paper on OH stellar cloud investigation

 

 

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