O efecto Zeeman é a división dunha liña espectral en varias, na presenza dun campo magnético estático. É equiparable ó efecto Stark, é dicir, a división dunha . Request PDF on ResearchGate | Efecto Zeeman Gravitacional | The study of rotating cosmological models is a subject under constant development due to the . Download Citation on ResearchGate | On Dec 30, , Carlos Calderón Chamochumbi and others published Efecto Zeeman Normal }.

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Note that the transitions shown follow the selection rule which does not allow a change of more than one unit in the quantum number m l. Why aren’t there 5 lines?

The magnetic dipole moment associated with the orbital angular momentum is given by. Considering the quantization of angular momentumthis gives equally spaced energy levels displaced from the zero field level by.

## Zeeman Effect in Hydrogen

This displacement of the energy levels gives the uniformly spaced multiplet splitting of the spectral lines which is zzeeman the Zeeman effect. The magnetic field also interacts with the electron spin magnetic moment, so it contributes to the Zeeman effect in many cases. The electron spin had not been discovered at the time of Zeeman’s original experiments, so the cases where it contributed were considered to be anomalous.

The term ” anomalous Zeeman effect ” has persisted for the cases ececto spin contributes. In general, both orbital and spin moments are involved, and the Zeeman interaction takes the form. The factor of two multiplying the electron spin angular momentum comes from the fact that it is twice as effective in producing magnetic moment.

## Zeeman effect

This factor is called the spin g-factor or gyromagnetic ratio. The evaluation of the scalar product between the angular momenta and the magnetic field here is complicated by the fact that the S and L vectors are both precessing around the magnetic field and are not in general in the same direction. The persistent early spectroscopists worked out a way to calculate the effect of the directions. The resulting geometric factor g L in the final expression above is called the Lande g factor. It allowed them to express the resultant splittings of the spectral lines in terms of the z-component of the total angular momentum, m j.

The above treatment of the Zeeman effect describes the phenomenon when the magnetic fields are small enough that the orbital and spin angular momenta can be considered to be coupled.

For extremely strong magnetic fields this coupling is broken and another approach must be taken. The strong field effect is called the Paschen-Back effect. The Zeeman sfecto for the hydrogen atom offered experimental support for the quantization of angular momentum which arose from the solution of the Schrodinger equation.

While the Zeeman effect in some atoms e. These deviations were labeled the “anomalous Zeeman effect” and were very puzzling to zseman researchers. The explanation of these different patterns of splitting gave additional insight into the effects of electron spin. With efevto inclusion of electron spin in the total angular momentumthe other types of multiplets formed zeeeman of a consistent picture.

So what has been historically called the “anomalous” Zeeman effect is really the normal Zeeman effect when electron spin is included. When the Zeeman effect was observed for hydrogen, the observed splitting was consistent with an electron orbit magnetic moment given by. But when the effects of electron spin were discovered by Goudsmit and Uhlenbeck, they found that the observed spectral features were matched by assigning to the electron spin a magnetic moment.

More precise experiments showed that the value zesman slightly greater than 2, and this fact took on added importance when that departure from 2 was predicted by quantum electrodynamics. In the experimental measurement of the Lamb shiftthe value of g has been determined to be.

First observed by Pieter Zeeman, this splitting is attributed to the interaction between the magnetic field and the magnetic dipole moment associated with the orbital angular momentum. In the absence of the magnetic field, the hydrogen energies depend only upon the principal quantum number nand the emissions occur at a single wavelength. Zeeman Interaction An external magnetic field will exert a torque on a magnetic dipole and the magnetic potential energy which results in The magnetic dipole moment associated with the orbital angular momentum is given by For a magnetic field in the z-direction this gives Considering the quantization of angular momentumthis gives equally spaced energy levels displaced from the zero field level by This displacement of the energy levels gives the uniformly spaced multiplet splitting of the spectral lines which is called the Zeeman effect.

In general, both orbital and spin moments are involved, and the Zeeman interaction takes the form The factor of two multiplying the electron spin angular momentum comes from the fact that it is twice as effective in producing magnetic moment. Index Schrodinger equation concepts.

### Zeeman effect – Wikipedia

Hydrogen Zeeman Example The Zeeman effect for the hydrogen atom offered experimental support for the quantization of zeemann momentum which arose from the solution of the Schrodinger equation.

This type of splitting efectoo observed for spin 0 states since the spin does not contribute to the angular momentum. But when the effects of electron spin were discovered by Goudsmit and Uhlenbeck, they found that the observed spectral features were matched by assigning to the electron spin a magnetic moment where g is approximately 2.

In the experimental measurement of the Lamb shiftthe value of g has been determined to be and is in precise agreement with the calculated values.