Energy level

Energy level
This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Energy_level".

This article is about orbital (electron) energy levels. For compounds' energy levels, see chemical potential.

A quantum mechanical system or particle that is bound, confined spacially, can only take on certain discrete values of energy, as opposed to classical particles, which can have any energy. These are called energy levels. The term is most commonly used for the energy levels (electron configuration) of electrons in atoms or molecules, which are bound by the electric field of the nucleus. The energy spectrum of a system with energy levels is said to be quantized.

If the potential energy is set to zero at infinity, the usual convention, then bound electron states have negative potential energy.

Energy levels are said to be degenerate, if the same energy level is obtained by more than one quantum mechanical state. They are then called degenerate energy levels.

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1 Explanation
2 Atoms
- 2.1 Intrinsic energy levels
- 2.2 Energy levels due to external fields
3 Molecules
4 Crystalline Materials
5 See also

Explanation

Quantized energy levels result from the relation between a particle's energy and its wavelength. For a confined particle, for example an electron in an atom, the wave function has the form of standing waves. Only stationary states with energies corresponding to integral numbers of wavelengths can exist; for other states the waves interfere destructively, resulting in zero probability density. Elementary examples that show mathematically how energy levels come about are the particle in a box and the quantum harmonic oscillator.

The following sections give an overview of the most important factors that determine the energy levels of atoms and molecules.

Atoms

Intrinsic energy levels

Orbital state energy level

Assume an electron in a given atomic orbital. The energy of its state is mainly determined by the electrostatic interaction of the (negative) electron with the (positive) nucleus. The energy levels of an electron around a nucleus are given by :

$E_n = - h c R_{\infty} \frac{Z^2}{n^2} \$ ,

where $R_{\infty} \$ is the Rydberg constant (typically between 1 eV and 10³ eV), Z is the charge of the atom's nucleus, $n \$ is the principal quantum number, e is the charge of the electron, $h$ is Planck's constant, and c is the speed of light.

The Rydberg levels depend only on the principal quantum number $n \$ .

Fine structure splitting

Fine structure arises from relativistic kinetic energy corrections, spin-orbit coupling (an electrodynamic interaction between the electron's spin and motion and the nucleus's electric field) and the Darwin term (contact term interaction of s-shell electrons inside the nucleus). Typical magnitude $10 - 3$ eV.

Hyperfine structure

Spin-nuclear-spin coupling (see hyperfine structure). Typical magnitude $10 - 4$ eV.

Electrostatic interaction of an electron with other electrons

If there is more than one electron around the atom, electron-electron-interactions raise the energy level. These interactions are often neglected if the spatial overlap of the electron wavefunctions is low.

Energy levels due to external fields

Zeeman effect

Main article: Zeeman effect

The interaction energy is: $U = - μ B$ with $μ = q L / 2 m$

Zeeman effect taking spin into account

This takes both the magnetic dipole moment due to the orbital angular momentum and the magnetic momentum arising from the electron spin into account.

Due to relativistic effects (Dirac equation), the magnetic moment arising from the electron spin is $μ = - μ B g s$ with $g$ the gyro-magnetic factor (about 2). $μ = μ l + g μ s$ The interaction energy therefore gets $U B = - μ B = μ B B (m l + g m s)$ .

Stark effect

Interaction with the external electric field causes:see Stark effect

Molecules

Roughly speaking, a molecular energy state, i.e. an eigenstate of the molecular Hamiltonian, is the sum of an electronic, vibrational, rotational, nuclear and translational component, such that:

$E = E_\mathrm{electronic}+E_\mathrm{vibrational}+E_\mathrm{rotational}+E_\mathrm{nuclear}+E_\mathrm{translational}\,$

where $E electronic$ is an eigenvalue of the electronic molecular Hamiltonian (the value of the potential energy surface) at the equilibrium geometry of the molecule.

The molecular energy levels are labelled by the molecular term symbols.

The specific energies of these components vary with the specific energy state and the substance.

In molecular physics and quantum chemistry, an energy level is a quantized energy of a bound quantum mechanical state.

Crystalline Materials

Crystalline solids are found to have energy bands, instead of or in addition to energy levels. Electrons can take on any energy within an unfilled band. At first this appears to be an exception to the requirement for energy levels. However as shown in band theory, energy bands are actually made up of many descrete energy levels which are too close together to resolve. Within a band the number of levels is of the order of the number of atoms in the crystal, so although electrons are actually restricted to these energies, they appear to be able to take on a continuum of values. The important energy levels in a crystal are the top of the valence band, the bottom of the conduction band, the Fermi energy, the vacuum level, and the energy levels of any defect states in the crystal.

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