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Electronic density
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In quantum mechanics, and in particular quantum chemistry, the electronic density is a measure of the probability of an electron occupying an infinitesimal element of space surrounding any given point. It is a scalar quantity depending upon three spatial variables and is typically denoted as either ?(r) or n(r). The density is determined, through definition, by the normalized N-electron wavefunction which itself depends upon 4N variables (3N spatial and N spin coordinates).

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In quantum mechanics, and in particular quantum chemistry, the electronic density is a measure of the probability of an electron occupying an infinitesimal element of space surrounding any given point. It is a scalar quantity depending upon three spatial variables and is typically denoted as either ?(r) or n(r). The density is determined, through definition, by the normalized N-electron wavefunction which itself depends upon 4N variables (3N spatial and N spin coordinates). Conversely, the density determines the wave function modulo a phase factor, providing the formal foundation of density functional theory.
Definition
The electronic density corresponding to a normalized N-electron wavefunction (with r and s denoting spatial and spin variables respectively) is defined as
where the operator corresponding to the density observable is
In Hartree-Fock and density functional theories the wave function is typically represented as a single Slater determinant constructed from N orbitals, fk, with corresponding occupations nk. In these situations the density simplifies to
General Properties From its definition, the electron density is a non-negative function integrating to the total number of electrons. Further, for a system with kinetic energy T, the density satisfies the inequalities
For finite kinetic energies, the first (stronger) inequality places the square root of the density in the Sobolev space H1(R3). Together with the normalization and non-negativity this defines a space containing physically acceptable densities as
The second inequality places the density in the L3 space. Together with the normalization property places acceptable densities within the intersection of L1 and L3 – a superset of .
Topology The ground state electronic density of an atom is conjectured to be a monotonically decaying function of the distance from the nucleus.
Nuclear cusp condition The electronic density displays cusps at each nucleus in a molecule as a result of the unbounded electron-nucleus Coulomb potential. This behavior is quantified by the Kato cusp condition formulated in terms of the spherically averaged density, , about any given nucleus as
That is, the radial derivative of the spherically averaged density, evaluated at any nucleus, is equal to twice the density at that nucleus multiplied by the negative of the atomic number (Z).
Asymptotic behavior The nuclear cusp condition provides the near-nuclear (small r) density behavior as
The long-range (large r) behavior of the density is also known, taking the form
where I is the ionization energy of the system.
See also
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