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In [[atomic physics]], a '''two-electron atom''' or '''helium-like ion''' is a [[quantum mechanical]] system consisting of one [[Atomic nucleus|nucleus]] with a [[Electrical charge|charge]] of ''Z[[Elementary charge|e]]'' 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: | |||
{| | |||
|- | |||
| ''Z''=1: || H<sup>–</sup> || [[hydrogen anion]] | |||
|- | |||
| ''Z''=2: || He || '''[[helium atom]]''' | |||
|- | |||
| ''Z''=3: || Li<sup>+</sup> || [[lithium]] ion | |||
|- | |||
| ''Z''=4: || Be<sup>2+</sup> || [[beryllium]] ion | |||
|- | |||
| ''Z''=5: || B<sup>3+</sup> || [[boron]] ion | |||
|- | |||
|} | |||
==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:<ref name="Bransden">Physics of Atoms and Molecules, B.H. Bransden, C.J.Joachain, Longman, 1983, ISBN 0-582-44401-2</ref> For a more rigorous mathematical derivation of Schrödinger's equation, see also.<ref name="Bransden"/> | |||
:<math> E\psi = -\hbar^2\left[\frac{1}{2\mu}\left(\nabla_1^2 +\nabla_2^2 \right) + \frac{1}{M}\nabla_1\cdot\nabla_2\right] \psi + \frac{e^2}{4\pi\epsilon_0}\left[ \frac{1}{r_{12}} -Z\left( \frac{1}{r_1}+\frac{1}{r_2} \right) \right] \psi </math> | |||
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> = |'''r'''<sub>2</sub>| is the magnitude), ''r''<sub>12</sub> = |'''r'''<sub>12</sub>| is the magnitude of the separation between them given by | |||
:<math> |\bold{r}_{12}| = |\bold{r}_2 - \bold{r}_1 | \,\!</math> | |||
''μ'' is again the two-body reduced mass of an electron with respect to the nucleus of mass ''M'', so this time | |||
:<math> \mu = \frac{m_e M}{m_e+M} \,\!</math> | |||
and ''Z'' is the [[atomic number]] for the element (not a [[quantum number]]). | |||
The cross-term of two laplacians | |||
:<math>\frac{1}{M}\nabla_1\cdot\nabla_2\,\!</math> | |||
is known as the ''mass polarization term'', which arises due to the motion of [[Atomic nucleus|atomic nuclei]]. The wavefunction is a function of the two electron's positions: | |||
:<math> \psi = \psi(\bold{r}_1,\bold{r}_2) </math> | |||
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>.<ref name="Herzberg">{{cite book|last=Herzberg|first=Gerhard|coauthors=J W T Spinks|title=Atomic Spectra and Atomic Structure|edition=2|year=1944|publisher=Dover Publications|location=New York|page=75}}</ref> Alkaline earths and Mercury also have spectra with similar features, due to the two outer valence electrons.<ref name="Herzberg"/> | |||
==References== | |||
<references/> | |||
==See also== | |||
*[[Hydrogen-like atom]] | |||
*[[Helium atom]] | |||
[[Category:Atoms]] | |||
[[Category:Quantum models]] |
Revision as of 06:42, 15 November 2013
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:
Z=1: | H– | hydrogen anion |
Z=2: | He | helium atom |
Z=3: | Li+ | lithium ion |
Z=4: | Be2+ | beryllium ion |
Z=5: | B3+ | boron ion |
Schrödinger equation
The Schrödinger equation for any two-electron system, such as the neutral Helium atom (He, Z = 2), the negative Hydrogen ion (H–, Z = 1), or the positive Lithium ion (Li+, Z = 3) is:[1] For a more rigorous mathematical derivation of Schrödinger's equation, see also.[1]
where r1 is the position of one electron (r1 = |r1| is its magnitude), r2 is the position of the other electron (r2 = |r2| is the magnitude), r12 = |r12| is the magnitude of the separation between them given by
μ is again the two-body reduced mass of an electron with respect to the nucleus of mass M, so this time
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 1S0 1P1 1D2 1F3 etc., and for the triplets, some energy levels are split: 3S1 3P2 3P1 3P0 3D3 3D2 3D1 3F4 3F3 3F2.[2] Alkaline earths and Mercury also have spectra with similar features, due to the two outer valence electrons.[2]
References
- ↑ 1.0 1.1 Physics of Atoms and Molecules, B.H. Bransden, C.J.Joachain, Longman, 1983, ISBN 0-582-44401-2
- ↑ 2.0 2.1 20 year-old Real Estate Agent Rusty from Saint-Paul, has hobbies and interests which includes monopoly, property developers in singapore and poker. Will soon undertake a contiki trip that may include going to the Lower Valley of the Omo.
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