Hydrogen-like atom
A hydrogen-like ion is any atomic nucleus with one electron and thus is isoelectronic with hydrogen. Except for the hydrogen atom itself (which is neutral), these ions carry the positive charge , where is the atomic number of the atom. Examples of hydrogen-like ions are He^{+}, Li^{2+}, Be^{3+} and B^{4+}. Because hydrogen-like ions are two-particle systems with an interaction depending only on the distance between the two particles, their (non-relativistic) Schrödinger equation can be solved in analytic form, as can the (relativistic) Dirac equation. The solutions are one-electron functions and are referred to as hydrogen-like atomic orbitals.^{[1]}
Other systems may also be referred to as "hydrogen-like atoms", such as muonium (an electron orbiting a muon), positronium (an electron and a positron), certain exotic atoms (formed with other particles), or Rydberg atoms (in which one electron is in such a high energy state that it sees the rest of the atom practically as a point charge).
Schrödinger solution
In the solution to the Schrödinger equation, which is non-relativistic, hydrogen-like atomic orbitals are eigenfunctions of the one-electron angular momentum operator L and its z component L_{z}. A hydrogen-like atomic orbital is uniquely identified by the values of the principal quantum number n, the angular momentum quantum number l, and the magnetic quantum number m. The energy eigenvalues do not depend on l or m, but solely on n. To these must be added the two-valued spin quantum number m_{s} = ±½, setting the stage for the Aufbau principle. This principle restricts the allowed values of the four quantum numbers in electron configurations of more-electron atoms. In hydrogen-like atoms all degenerate orbitals of fixed n and l, m and s varying between certain values (see below) form an atomic shell.
The Schrödinger equation of atoms or atomic ions with more than one electron has not been solved analytically, because of the computational difficulty imposed by the Coulomb interaction between the electrons. Numerical methods must be applied in order to obtain (approximate) wavefunctions or other properties from quantum mechanical calculations. Due to the spherical symmetry (of the Hamiltonian), the total angular momentum J of an atom is a conserved quantity. Many numerical procedures start from products of atomic orbitals that are eigenfunctions of the one-electron operators L and L_{z}. The radial parts of these atomic orbitals are sometimes numerical tables or are sometimes Slater orbitals. By angular momentum coupling many-electron eigenfunctions of J^{2} (and possibly S^{2}) are constructed.
In quantum chemical calculations hydrogen-like atomic orbitals cannot serve as an expansion basis, because they are not complete. The non-square-integrable continuum (E > 0) states must be included to obtain a complete set, i.e., to span all of one-electron Hilbert space.^{[2]}
In the simplest model, the atomic orbitals of hydrogen-like ions are solutions to the Schrödinger equation in a spherically symmetric potential. In this case, the potential term is the potential given by Coulomb's law:
where
- ε_{0} is the permittivity of the vacuum,
- Z is the atomic number (number of protons in the nucleus),
- e is the elementary charge (charge of an electron),
- r is the distance of the electron from the nucleus.
After writing the wave function as a product of functions:
(in spherical coordinates), where are spherical harmonics, we arrive at the following Schrödinger equation:
where is, approximately, the mass of the electron (more accurately, it is the reduced mass of the system consisting of the electron and the nucleus), and is the reduced Planck constant.
Different values of l give solutions with different angular momentum, where l (a non-negative integer) is the quantum number of the orbital angular momentum. The magnetic quantum number m (satisfying ) is the (quantized) projection of the orbital angular momentum on the z-axis. See here for the steps leading to the solution of this equation.
Non-relativistic wavefunction and energy
In addition to l and m, a third integer n > 0, emerges from the boundary conditions placed on R. The functions R and Y that solve the equations above depend on the values of these integers, called quantum numbers. It is customary to subscript the wave functions with the values of the quantum numbers they depend on. The final expression for the normalized wave function is:
where:
- are the generalized Laguerre polynomials in the definition given here.
- where α is the fine structure constant. Here, is the reduced mass of the nucleus-electron system, that is, where is the mass of the nucleus. Typically, the nucleus is much more massive than the electron, so (But for positronium )
- function is a spherical harmonic.
parity due to angular wave function is .
Quantum numbers
The quantum numbers n, l and m are integers and can have the following values:
For a group-theoretical interpretation of these quantum numbers, see this article. Among other things, this article gives group-theoretical reasons why and .
Angular momentum
Each atomic orbital is associated with an angular momentum L. It is a vector operator, and the eigenvalues of its square L^{2} ≡ L_{x}^{2} + L_{y}^{2} + L_{z}^{2} are given by:
The projection of this vector onto an arbitrary direction is quantized. If the arbitrary direction is called z, the quantization is given by:
where m is restricted as described above. Note that L^{2} and L_{z} commute and have a common eigenstate, which is in accordance with Heisenberg's uncertainty principle. Since L_{x} and L_{y} do not commute with L_{z}, it is not possible to find a state that is an eigenstate of all three components simultaneously. Hence the values of the x and y components are not sharp, but are given by a probability function of finite width. The fact that the x and y components are not well-determined, implies that the direction of the angular momentum vector is not well determined either, although its component along the z-axis is sharp.
These relations do not give the total angular momentum of the electron. For that, electron spin must be included.
This quantization of angular momentum closely parallels that proposed by Niels Bohr (see Bohr model) in 1913, with no knowledge of wavefunctions.
Including spin-orbit interaction
Template:Rellink In a real atom the spin interacts with the magnetic field created by the electron movement around the nucleus, a phenomenon known as spin-orbit interaction. When one takes this into account, the spin and angular momentum are no longer conserved, which can be pictured by the electron precessing. Therefore one has to replace the quantum numbers l, m and the projection of the spin m_{s} by quantum numbers that represent the total angular momentum (including spin), j and m_{j}, as well as the quantum number of parity.
See the next section on the Dirac equation for a solution that includes the coupling.
Solution to Dirac equation
In 1928 in England Paul Dirac found an equation that was fully compatible with Special Relativity. The equation was solved for hydrogen-like atoms the same year by the German Walter Gordon. Instead of a single (possibly complex) function as in the Schrödinger equation, one must find four complex functions that make up a bispinor. The first and second functions (or components of the spinor) correspond (in the usual basis) to spin "up" and spin "down" positive-energy states, whereas the third and fourth correspond to spin up and spin down negative-energy states.
The terms "spin up" and "spin down" are relative to a chosen direction, conventionally the z direction. An electron may be in a superposition of spin up and spin down, which corresponds to the spin axis pointing in some other direction. The spin state may depend on location.
An electron in the vicinity of a nucleus necessarily has non-zero amplitudes for the negative energy components. Far from the nucleus these may be small, but near the nucleus they become large.
The eigenfunctions of the Hamiltonian, which means functions with a definite energy (and which therefore do not evolve except for a phase shift), are characterized not by the quantum number n only (as for the Schrödinger equation), but by n and a quantum number j, the total angular momentum quantum number. The quantum number j determines the sum of the squares of the three angular momenta to be j(j+1) (times ħ^{2}, see Planck constant). These angular momenta include both orbital angular momentum (having to do with the angular dependence of ψ) and spin angular momentum (having to do with the spin state). The splitting of the energies of states of the same principal quantum number n due to differences in j is called fine structure.
The orbitals for a given state can be written using two radial functions and two angle functions. The radial functions depend on both the principal quantum number n and an integer k, defined as:
where ℓ is the azimuthal quantum number that ranges from 0 to n−1. The angle functions depend on k and on a quantum number m which ranges from −j/2 to j/2 by steps of 1. The states are labeled using the letters S, P, D, F et cetera to stand for states with ℓ equal to 0, 1, 2, 3 et cetera (see azimuthal quantum number), with a subscript giving j. For instance, the states for n=4 are given in the following table (these would be prefaced by n, for example 4S_{1/2}):
m = −7/2 | m = −5/2 | m = −3/2 | m = −1/2 | m = 1/2 | m = 3/2 | m = 5/2 | m = 7/2 | |
---|---|---|---|---|---|---|---|---|
k = 3, ℓ = 3 | F_{5/2} | F_{5/2} | F_{5/2} | F_{5/2} | F_{5/2} | F_{5/2} | ||
k = 2, ℓ = 2 | D_{3/2} | D_{3/2} | D_{3/2} | D_{3/2} | ||||
k = 1, ℓ = 1 | P_{1/2} | P_{1/2} | ||||||
k = 0 | ||||||||
k = −1, ℓ = 0 | S_{1/2} | S_{1/2} | ||||||
k = −2, ℓ = 1 | P_{3/2} | P_{3/2} | P_{3/2} | P_{3/2} | ||||
k = −3, ℓ = 2 | D_{5/2} | D_{5/2} | D_{5/2} | D_{5/2} | D_{5/2} | D_{5/2} | ||
k = −4, ℓ = 3 | F_{7/2} | F_{7/2} | F_{7/2} | F_{7/2} | F_{7/2} | F_{7/2} | F_{7/2} | F_{7/2} |
These can be additionally labeled with a subscript giving m. There are 2n^{2} states with principal quantum number n, 4j+2 of them with any allowed j except the highest (j=n−1/2) for which there are only 2j+1. Since the orbitals having given values of n and j have the same energy according to the Dirac equation, they form a basis for the space of functions having that energy.
The energy, as a function of n and |k| (equal to j+1/2), is:
(The energy of course depends on the zero-point used.) The Schrödinger solution corresponds to replacing the inner bracket in the second expression by 1. The accuracy of the energy difference between the lowest two hydrogen states calculated from the Schrödinger solution is about 9 ppm (90 μeV too low, out of around 10 eV), whereas the accuracy of the Dirac equation for the same energy difference is about 3 ppm (too high). The Schrödinger solution always puts the states at slightly higher energies than the more accurate Dirac equation. The Dirac equation gives some levels of hydrogen quite accurately (for instance the 4P_{1/2} state is given an energy only about Template:Val eV too high), others less so (for instance, the 2S_{1/2} level is about Template:Val eV too low).^{[3]} The modifications of the energy due to using the Dirac equation rather than the Schrödinger solution is of the order of α^{2}, and for this reason α is called the fine structure constant.
The solution to the Dirac equation for quantum numbers n, k, and m, is: