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&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Short description|Quantum description of atoms with more than one electron including electron interactions and approximate methods}}&lt;br /&gt;
&lt;br /&gt;
{{Quantum book backlink|Atomic and spectroscopy}}&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Multi-electron atoms&amp;#039;&amp;#039;&amp;#039; are atomic systems containing more than one electron, where the simple analytical solutions of the [[Physics:Quantum Hydrogen atom|hydrogen atom]] no longer apply. The presence of multiple electrons introduces [[Physics:Coulomb&amp;#039;s law|Coulomb]] interactions between electrons, leading to complex energy structures and requiring approximation methods to solve the [[Physics:Schrödinger equation|Schrödinger equation]].&amp;lt;ref name=&amp;quot;Griffiths&amp;quot;&amp;gt;{{cite book |last=Griffiths |first=D. J. |title=Introduction to Quantum Mechanics |publisher=Cambridge University Press |year=2018}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
[[File:Quantum_multi_electron_atoms.jpg|thumb|400px|Multi-electron atoms exhibit complex energy structures due to electron–electron interactions, screening effects, and exchange symmetry, requiring approximate quantum methods for accurate description.]]&lt;br /&gt;
&lt;br /&gt;
== Electron–electron interactions ==&lt;br /&gt;
&lt;br /&gt;
In multi-electron atoms, each electron interacts not only with the nucleus but also with all other electrons. The Hamiltonian takes the form:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;H = \sum_i \left( -\frac{\hbar^2}{2m} \nabla_i^2 - \frac{Ze^2}{4\pi \epsilon_0 r_i} \right) + \sum_{i&amp;lt;j} \frac{e^2}{4\pi \epsilon_0 r_{ij}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where the second summation represents electron–electron repulsion.&amp;lt;ref name=&amp;quot;Sakurai&amp;quot;&amp;gt;{{cite book |last=Sakurai |first=J. J. |title=Modern Quantum Mechanics |publisher=Cambridge University Press |year=2017}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This interaction prevents exact analytical solutions and leads to correlated electron motion.&lt;br /&gt;
&lt;br /&gt;
== Screening and effective nuclear charge ==&lt;br /&gt;
&lt;br /&gt;
Electrons partially shield each other from the nuclear charge. As a result, each electron experiences an effective nuclear charge &amp;lt;math&amp;gt;Z_{\mathrm{eff}}&amp;lt;/math&amp;gt;, which is smaller than the actual nuclear charge &amp;lt;math&amp;gt;Z&amp;lt;/math&amp;gt;. This effect explains:&lt;br /&gt;
&lt;br /&gt;
* Orbital energy ordering  &lt;br /&gt;
* Periodic trends in atomic structure  &lt;br /&gt;
* Variations in ionization energies  &lt;br /&gt;
&lt;br /&gt;
Screening leads to deviations from hydrogen-like energy levels.&amp;lt;ref name=&amp;quot;Atkins&amp;quot;&amp;gt;{{cite book |last=Atkins |first=P. |title=Physical Chemistry |publisher=Oxford University Press |year=2018}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Approximation methods ==&lt;br /&gt;
&lt;br /&gt;
Because exact solutions are not possible, several approximation techniques are used:&lt;br /&gt;
&lt;br /&gt;
=== Hartree and Hartree–Fock methods ===&lt;br /&gt;
These methods approximate the total wavefunction as a product (or antisymmetrized product) of single-electron orbitals. The Hartree–Fock method includes exchange effects arising from electron indistinguishability.&amp;lt;ref name=&amp;quot;Szabo&amp;quot;&amp;gt;{{cite book |last=Szabo |first=A. |last2=Ostlund |first2=N. S. |title=Modern Quantum Chemistry |publisher=Dover |year=1996}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
=== Central field approximation ===&lt;br /&gt;
The atom is approximated as electrons moving in an average spherically symmetric potential, simplifying the many-body problem.&lt;br /&gt;
&lt;br /&gt;
=== Configuration interaction ===&lt;br /&gt;
Improves accuracy by combining multiple electron configurations to account for electron correlation effects.&lt;br /&gt;
&lt;br /&gt;
== Pauli principle and exchange symmetry ==&lt;br /&gt;
&lt;br /&gt;
Electrons are [[Physics:Fermion|fermions]] and must obey the [[Physics:Pauli exclusion principle|Pauli exclusion principle]]. The total wavefunction must be antisymmetric under particle exchange:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\Psi(\mathbf{r}_1, \mathbf{r}_2) = -\Psi(\mathbf{r}_2, \mathbf{r}_1)&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This requirement leads to:&lt;br /&gt;
&lt;br /&gt;
* Electron shell structure  &lt;br /&gt;
* Spin pairing  &lt;br /&gt;
* Exchange energy contributions  &lt;br /&gt;
&lt;br /&gt;
== Spectral structure and complexity ==&lt;br /&gt;
&lt;br /&gt;
Multi-electron atoms exhibit:&lt;br /&gt;
&lt;br /&gt;
* Fine and hyperfine structure splitting  &lt;br /&gt;
* Complex spectral line patterns  &lt;br /&gt;
* Term symbols describing total angular momentum  &lt;br /&gt;
&lt;br /&gt;
These features arise from combined effects of electron interactions, spin–orbit coupling, and external perturbations.&amp;lt;ref name=&amp;quot;Bransden&amp;quot;&amp;gt;{{cite book |last=Bransden |first=B. H. |last2=Joachain |first2=C. J. |title=Physics of Atoms and Molecules |publisher=Pearson |year=2003}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Significance ==&lt;br /&gt;
&lt;br /&gt;
Understanding multi-electron atoms is essential for:&lt;br /&gt;
&lt;br /&gt;
* Atomic spectroscopy  &lt;br /&gt;
* Chemistry and bonding  &lt;br /&gt;
* Laser physics  &lt;br /&gt;
* Astrophysical spectra interpretation  &lt;br /&gt;
&lt;br /&gt;
They form the foundation for real atomic systems beyond hydrogen and connect quantum mechanics to observable material properties.&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
{{#invoke:PhysicsQC|tocHeadingAndList|Physics:Quantum basics/See also}}&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{reflist|3}}&lt;br /&gt;
&lt;br /&gt;
{{Author|Harold Foppele}}&lt;br /&gt;
[[Category:Quantum mechanics]]&lt;br /&gt;
[[Category:Atomic physics]]&lt;br /&gt;
&lt;br /&gt;
{{Sourceattribution|Physics:Quantum Multi-electron atoms|1}}&lt;/div&gt;</summary>
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