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&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Quantum book backlink|Atomic and spectroscopy}}&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Hyperfine structure&amp;#039;&amp;#039;&amp;#039; refers to small shifts and splittings of otherwise degenerate electronic energy levels in atoms, molecules, and ions due to interactions between the [[Physics:Atomic nucleus|nucleus]] and the surrounding electron cloud.&lt;br /&gt;
&lt;br /&gt;
These shifts are typically much smaller than those of [[Physics:Fine structure|fine structure]] and arise from electromagnetic multipole interactions, primarily involving nuclear magnetic dipole and electric quadrupole moments.&lt;br /&gt;
&lt;br /&gt;
[[File:Fine hyperfine levels yellow.png|thumb|400px|Fine and hyperfine structure in the hydrogen atom]]&lt;br /&gt;
&lt;br /&gt;
==Overview==&lt;br /&gt;
&lt;br /&gt;
In atomic systems, hyperfine structure originates from:&lt;br /&gt;
&lt;br /&gt;
* interaction between the [[Physics:Nuclear magnetic moment|nuclear magnetic dipole moment]] and magnetic fields produced by electrons  &lt;br /&gt;
* interaction between the [[Physics:Quadrupole|nuclear electric quadrupole moment]] and the electric field gradient  &lt;br /&gt;
&lt;br /&gt;
In molecules, additional contributions arise from:&lt;br /&gt;
&lt;br /&gt;
* nuclear spin–spin interactions  &lt;br /&gt;
* nuclear spin–rotation coupling  &lt;br /&gt;
&lt;br /&gt;
Hyperfine structure is fundamentally weaker than fine structure and reflects the coupling between nuclear and electronic degrees of freedom.&lt;br /&gt;
&lt;br /&gt;
==Magnetic dipole interaction==&lt;br /&gt;
&lt;br /&gt;
For a nucleus with spin &amp;lt;math&amp;gt;\mathbf{I}&amp;lt;/math&amp;gt;, the magnetic dipole moment is&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\boldsymbol{\mu}_I = g_I \mu_N \mathbf{I}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;g_I&amp;lt;/math&amp;gt; is the nuclear &amp;#039;&amp;#039;g&amp;#039;&amp;#039;-factor and &amp;lt;math&amp;gt;\mu_N&amp;lt;/math&amp;gt; the nuclear magneton.&lt;br /&gt;
&lt;br /&gt;
The interaction Hamiltonian is:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\hat{H}_D = -\boldsymbol{\mu}_I \cdot \mathbf{B}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\mathbf{B}&amp;lt;/math&amp;gt; is the magnetic field generated by electrons.&lt;br /&gt;
&lt;br /&gt;
In the effective angular momentum form, this becomes:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\hat{H}_D = \hat{A}\,\mathbf{I} \cdot \mathbf{J}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
leading to the hyperfine energy shift:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\Delta E = \frac{1}{2}A\left[F(F+1) - I(I+1) - J(J+1)\right]&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where:&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;math&amp;gt;\mathbf{J}&amp;lt;/math&amp;gt; = total electronic angular momentum  &lt;br /&gt;
* &amp;lt;math&amp;gt;\mathbf{F} = \mathbf{I} + \mathbf{J}&amp;lt;/math&amp;gt; = total angular momentum  &lt;br /&gt;
&lt;br /&gt;
This interaction satisfies the [[Physics:Landé interval rule|Landé interval rule]].&lt;br /&gt;
&lt;br /&gt;
==Electric quadrupole interaction==&lt;br /&gt;
&lt;br /&gt;
For nuclei with spin &amp;lt;math&amp;gt;I \ge 1&amp;lt;/math&amp;gt;, an electric quadrupole moment exists.&lt;br /&gt;
&lt;br /&gt;
The quadrupole Hamiltonian is:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\hat{H}_Q = -e\,T^2(Q)\cdot T^2(q)&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where:&lt;br /&gt;
&lt;br /&gt;
* &amp;lt;math&amp;gt;T^2(Q)&amp;lt;/math&amp;gt; describes the nuclear quadrupole moment  &lt;br /&gt;
* &amp;lt;math&amp;gt;T^2(q)&amp;lt;/math&amp;gt; describes the electric field gradient  &lt;br /&gt;
&lt;br /&gt;
This interaction reflects deviations from spherical nuclear charge distributions.&lt;br /&gt;
&lt;br /&gt;
==Molecular hyperfine structure==&lt;br /&gt;
&lt;br /&gt;
In molecules, hyperfine structure includes additional contributions:&lt;br /&gt;
&lt;br /&gt;
===Spin–spin interaction===&lt;br /&gt;
Magnetic coupling between nuclei:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\hat{H}_{II} = -\sum_{\alpha \ne \alpha&amp;#039;} \boldsymbol{\mu}_\alpha \cdot \mathbf{B}_{\alpha&amp;#039;}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
===Spin–rotation interaction===&lt;br /&gt;
Coupling between nuclear spins and molecular rotation:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\hat{H}_{IR} \propto \mathbf{I} \cdot \mathbf{T}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
These effects are important in rotational spectroscopy.&lt;br /&gt;
&lt;br /&gt;
==Experimental observation==&lt;br /&gt;
&lt;br /&gt;
Hyperfine structure is observed in:&lt;br /&gt;
&lt;br /&gt;
* atomic spectra  &lt;br /&gt;
* molecular spectroscopy  &lt;br /&gt;
* [[Physics:Electron paramagnetic resonance|electron paramagnetic resonance]]  &lt;br /&gt;
* [[Physics:Nuclear magnetic resonance|nuclear magnetic resonance]]  &lt;br /&gt;
&lt;br /&gt;
A key example is the 21 cm hydrogen line in astrophysics.&lt;br /&gt;
&lt;br /&gt;
==Applications==&lt;br /&gt;
&lt;br /&gt;
===Atomic clocks===&lt;br /&gt;
The SI second is defined via the hyperfine transition of caesium-133:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;f = \frac{\Delta E}{h}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
One second equals exactly:&lt;br /&gt;
&lt;br /&gt;
9192631770 cycles of this transition.&lt;br /&gt;
&lt;br /&gt;
===Astrophysics===&lt;br /&gt;
Hyperfine transitions probe the interstellar medium and molecular clouds.&lt;br /&gt;
&lt;br /&gt;
===Quantum computing===&lt;br /&gt;
Hyperfine states serve as long-lived qubits in trapped-ion systems.&lt;br /&gt;
&lt;br /&gt;
===Precision physics===&lt;br /&gt;
Measurements of hyperfine splitting provide tests of quantum electrodynamics.&lt;br /&gt;
&lt;br /&gt;
==History==&lt;br /&gt;
&lt;br /&gt;
Hyperfine structure was first described theoretically by [[Biography:Enrico Fermi|Enrico Fermi]] in 1930.&amp;lt;ref&amp;gt;E. Fermi (1930), &amp;quot;Über die magnetischen Momente der Atomkerne&amp;quot;. Z. Physik 60, 320–333.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The nuclear quadrupole moment was introduced in 1935 by H. Schüler and T. Schmidt.&amp;lt;ref&amp;gt;H. Schüler &amp;amp; T. Schmidt (1935), &amp;quot;Über Abweichungen des Atomkerns von der Kugelsymmetrie&amp;quot;. Z. Physik 94, 457–468.&amp;lt;/ref&amp;gt;&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:Atomic physics]]&lt;br /&gt;
[[Category:Quantum mechanics]]&lt;br /&gt;
&lt;br /&gt;
{{Sourceattribution|Physics:Quantum Hyperfine structure|1}}&lt;/div&gt;</summary>
		<author><name>imported&gt;WikiHarold</name></author>
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