my-server
← Wiki

Two-electron atom

In atomic physics, a two-electron atom or helium-like ion is a quantum mechanical system consisting of one nucleus with a charge of Ze and just two electrons. This is the first case of many-electron systems where the Pauli exclusion principle plays a central role.

It is an example of a three-body problem.

The first few two-electron atoms are:

Schrödinger equation

The Schrödinger equation for any two-electron system, such as the neutral Helium atom (He, Z = 2), the negative Hydrogen ion (H<sup>−</sup>, Z = 1), or the positive Lithium ion (Li<sup>+</sup>, Z = 3) is: For a more rigorous mathematical derivation of the Schrödinger equation, see also.

where r<sub>1</sub> is the position of one electron (r<sub>1</sub> = |r<sub>1</sub>| is its magnitude), r<sub>2</sub> is the position of the other electron (r<sub>2</sub> = is the magnitude), r<sub>12</sub> = is the magnitude of the separation between them given by

μ is the two-body reduced mass of an electron with respect to the nucleus of mass M

and Z is the atomic number for the element (not a quantum number).

The cross-term of two Laplacians

is known as the mass polarization term, which arises due to the motion of atomic nuclei. The wavefunction is a function of the two electron's positions:

There is no closed form solution for this equation.

Spectrum

The optical spectrum of the two electron atom has two systems of lines. A para system of single lines, and an ortho system of triplets (closely spaced group of three lines). The energy levels in the atom for the single lines are indicated by <sup>1</sup>S<sub>0</sub> <sup>1</sup>P<sub>1</sub> <sup>1</sup>D<sub>2</sub> <sup>1</sup>F<sub>3</sub> etc., and for the triplets, some energy levels are split: <sup>3</sup>S<sub>1</sub> <sup>3</sup>P<sub>2</sub> <sup>3</sup>P<sub>1</sub> <sup>3</sup>P<sub>0</sub> <sup>3</sup>D<sub>3</sub> <sup>3</sup>D<sub>2</sub> <sup>3</sup>D<sub>1</sub> <sup>3</sup>F<sub>4</sub> <sup>3</sup>F<sub>3</sub> <sup>3</sup>F<sub>2</sub>. Alkaline earths and mercury also have spectra with similar features, due to the two outer valence electrons.

See also

References