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{{Quantum book backlink|Atomic and spectroscopy}}
Atomic spectra proves that there is more to atomic structure than just the energy-level approach. Structures are formed due to interactions between the atom and its environment, including effects like spin, relativity, and the influence of external fields. The fine structure is concerned with relativistic corrections and the interaction of the atom's spin and orbital angular momenta. Hyperfine structure include the interaction of the atomic nucleus with the electrons. Interaction with different fields create further splittings, resulting from the influence of magnetic and electrical fields. In magnetic fields, this is known as the Zeeman effect; also, it is called the Stark effect for electrical fields.[[File:Quantum Atomic Structure & Spectroscopy1.jpg|thumb|400px|Quantum atomic structure and spectroscopy: orbitals, energy levels, and emission and absorption spectra.]]
=Fine structure=

The '''fine structure''' of atomic spectra arises from relativistic and spin-related corrections to the nonrelativistic Schrödinger equation. These effects lead to small splittings of energy levels that depend on the total angular momentum of the electron.<ref>{{cite book |last=Griffiths |first=David J. |title=Introduction to Quantum Mechanics |publisher=Pearson |year=2018}}</ref>

The fine structure has three main contributions:

* '''Relativistic correction''' to the kinetic energy
* '''Spin–orbit coupling''' between the electron’s spin and orbital motion
* '''Darwin term''', accounting for quantum fluctuations in position

=== Spin–orbit coupling ===

The dominant contribution comes from the interaction between the electron’s spin <math>\mathbf{S}</math> and orbital angular momentum <math>\mathbf{L}</math>.

The interaction energy is proportional to

<math>
\mathbf{L} \cdot \mathbf{S}.
</math>

It is convenient to introduce the total angular momentum

<math>
\mathbf{J} = \mathbf{L} + \mathbf{S}.
</math>

The energy shift depends on the quantum numbers <math>l</math> and <math>j</math>.

=== Energy splitting ===

The corrected energy levels of hydrogen-like atoms can be written as

<math>
E_{n,j} = E_n \left[1 + \frac{\alpha^2}{n^2} \left(\frac{n}{j+1/2} - \frac{3}{4}\right)\right],
</math>

where <math>\alpha</math> is the fine-structure constant.

These splittings explain the closely spaced lines observed in atomic spectra.

=== Physical significance ===

Fine structure:

* reveals relativistic effects in atomic systems,
* introduces total angular momentum <math>j</math>,
* explains detailed spectral line splitting.

It represents the first correction beyond the basic hydrogen atom model.<ref>{{cite book |last=Bransden |first=B. H. |last2=Joachain |first2=C. J. |title=Physics of Atoms and Molecules |publisher=Pearson |year=2003}}</ref>

=Hyperfine structure=

The '''hyperfine structure''' of atomic spectra arises from interactions between the magnetic moments of the nucleus and the electron. These effects produce even smaller energy splittings than fine structure and are essential for high-precision spectroscopy.<ref>{{cite book |last=Bransden |first=B. H. |last2=Joachain |first2=C. J. |title=Physics of Atoms and Molecules |publisher=Pearson |year=2003}}</ref>

=== Nuclear spin and magnetic moment ===

The nucleus possesses a spin <math>\mathbf{I}</math> and an associated magnetic moment. This interacts with the magnetic field produced by the electron’s motion and spin.

The total angular momentum of the atom becomes

<math>
\mathbf{F} = \mathbf{I} + \mathbf{J},
</math>

where <math>\mathbf{J}</math> is the total electronic angular momentum.

=== Magnetic dipole interaction ===

The dominant contribution to hyperfine structure is the magnetic dipole interaction between the nucleus and the electron. The energy shift is proportional to

<math>
\mathbf{I} \cdot \mathbf{J}.
</math>

This leads to splitting of energy levels depending on the quantum number <math>F</math>.

=== Energy levels ===

The hyperfine energy shift can be written as

<math>
E_F = \frac{A}{2} \left[ F(F+1) - I(I+1) - J(J+1) \right],
</math>

where <math>A</math> is the hyperfine coupling constant.

Each fine-structure level is thus split into multiple hyperfine levels.

=== Examples ===

A well-known example is the hydrogen 21 cm line, which arises from hyperfine splitting of the ground state. This transition is of great importance in astrophysics.<ref>{{cite book |last=Foot |first=Christopher J. |title=Atomic Physics |publisher=Oxford University Press |year=2005}}</ref>

=== Physical significance ===

Hyperfine structure:

* probes nuclear properties such as spin and magnetic moment,
* provides extremely precise frequency standards (atomic clocks),
* is crucial in spectroscopy, astrophysics, and quantum metrology.

=Zeeman effect=
[[File:Zeeman_effect1.png|thumb|400px|Zeeman effect: splitting of energy levels and spectral lines in an external magnetic field.]]
The '''Zeeman effect''' is the splitting of atomic energy levels in the presence of an external magnetic field. This effect arises from the interaction between the magnetic field and the magnetic moments associated with the angular momentum of the electron.<ref>{{cite book |last=Foot |first=Christopher J. |title=Atomic Physics |publisher=Oxford University Press |year=2005}}</ref>

=== Magnetic interaction ===

An external magnetic field <math>\mathbf{B}</math> interacts with the magnetic moment <math>\boldsymbol{\mu}</math> of the atom, leading to an energy shift

<math>
\Delta E = -\boldsymbol{\mu} \cdot \mathbf{B}.
</math>

For an electron, the magnetic moment is proportional to its angular momentum.

=== Normal Zeeman effect ===

In the simplest case (neglecting spin), the energy shift depends on the magnetic quantum number <math>m</math>:

<math>
\Delta E = m \mu_B B,
</math>

where <math>\mu_B</math> is the Bohr magneton.

This leads to equally spaced splitting of spectral lines.

=== Anomalous Zeeman effect ===

When electron spin is included, the splitting becomes more complex. The energy shift is given by

<math>
\Delta E = g_J \mu_B m_J B,
</math>

where:

* <math>g_J</math> is the Landé g-factor,
* <math>m_J</math> is the magnetic quantum number of total angular momentum.

This case is called the '''anomalous Zeeman effect'''.

=== Landé g-factor ===

The Landé g-factor is

<math>
g_J = 1 + \frac{J(J+1) + S(S+1) - L(L+1)}{2J(J+1)}.
</math>

It accounts for the combined contribution of orbital and spin angular momentum.

=== Spectral splitting ===

The Zeeman effect causes a single spectral line to split into multiple components, corresponding to different values of <math>m_J</math>.

Selection rules determine which transitions are allowed:

* <math>\Delta m = 0</math> (π lines)
* <math>\Delta m = \pm 1</math> (σ lines)

=== Physical significance ===

The Zeeman effect:

* provides evidence for quantized angular momentum,
* allows measurement of magnetic fields,
* is widely used in spectroscopy and astrophysics.

It is one of the key experimental confirmations of quantum theory.<ref>{{cite book |last=Griffiths |first=David J. |title=Introduction to Quantum Mechanics |publisher=Pearson |year=2018}}</ref>

=Stark effect=

The '''Stark effect''' is the splitting or shifting of atomic energy levels due to the presence of an external electric field. It is the electric analogue of the Zeeman effect and provides important insight into the structure of atoms and their interaction with external fields.<ref>{{cite book |last=Foot |first=Christopher J. |title=Atomic Physics |publisher=Oxford University Press |year=2005}}</ref>

== Electric interaction ==

An external electric field <math>\mathbf{E}</math> interacts with the electric dipole moment <math>\mathbf{p}</math> of the atom, producing an energy shift

<math>
\Delta E = -\mathbf{p} \cdot \mathbf{E}.
</math>

For many atomic states, the dipole moment arises from mixing of quantum states.

== Linear Stark effect ==

In some systems, such as hydrogen, the Stark effect can be linear in the electric field:

<math>
\Delta E \propto E.
</math>

This occurs when degenerate states are mixed by the electric field, leading to first-order energy shifts.

== Quadratic Stark effect ==

In most atoms, the Stark effect is quadratic:

<math>
\Delta E \propto E^2.
</math>

This arises when there is no degeneracy, and the energy shift appears only in second-order perturbation theory.

== Perturbation theory ==

The Stark effect is typically analyzed using perturbation theory, where the electric field introduces a perturbation

<math>
\hat{H}' = -e \mathbf{E} \cdot \mathbf{r}.
</math>

The resulting shifts depend on matrix elements of the position operator between atomic states.<ref>{{cite book |last=Griffiths |first=David J. |title=Introduction to Quantum Mechanics |publisher=Pearson |year=2018}}</ref>

== Spectral effects ==

The Stark effect modifies spectral lines by:

* shifting their positions,
* splitting degenerate levels,
* changing transition intensities.

These changes provide information about atomic structure and external electric fields.

== Physical significance ==

The Stark effect:

* probes electric properties of atoms and molecules,
* is used in spectroscopy and plasma diagnostics,
* plays a role in laser physics and quantum control.

Together with the Zeeman effect, it illustrates how external fields reveal the internal structure of quantum systems.

=See also=
{{#invoke:PhysicsQC|tocHeadingAndList|Physics:Quantum basics/See also}}

=References=
{{reflist|3}}

{{Author|Harold Foppele}}

{{Sourceattribution|Quantum Atomic structure and spectroscopy|1}}

Physics:Quantum Atomic structure and spectroscopy - Revision history

imported>WikiHarold: Repair Quantum Collection B backlink template

imported>WikiHarold: Repair Quantum Collection B backlink template