Quantum numbers describe values of conserved quantities in the dynamics of a quantum system. In the case of electrons, the quantum numbers can be defined as "the sets of numerical values which give acceptable solutions to the Schrödinger wave equation for the hydrogen atom". In more general cases, quantum numbers correspond to eigenvalues of operators that commute with the Hamiltonian--quantities that can be known with precision at the same time as the system's energy[note 1]--and their corresponding eigenspaces. Together, a specification of all of the quantum numbers of a quantum system fully characterize a basis state of the system, and can in principle be measured together.
An important aspect of quantum mechanics is the quantization of many observable quantities of interest.[note 2] In particular, this leads to quantum numbers that take values in discrete sets of integers or half-integers; although they could approach infinity in some cases. This distinguishes quantum mechanics from classical mechanics where the values that characterize the system such as mass, charge, or momentum, all range continuously. Quantum numbers often describe specifically the energy levels of electrons in atoms, but other possibilities include angular momentum, spin, etc. An important family is flavour quantum numbers - internal quantum numbers which determine the type of a particle and its interactions with other particles through the fundamental forces. Any quantum system can have one or more quantum numbers; it is thus difficult to list all possible quantum numbers.
The question of how many quantum numbers are needed to describe any given system has no universal answer. Hence for each system, one must find the answer for a full analysis of the system. A quantized system requires at least one quantum number. The dynamics (time evolution) of any quantum system are described by a quantum Hamiltonian, H. There is one quantum number of the system corresponding to the energy; that is to say, the eigenvalue of the Hamiltonian. There is also one quantum number for each linearly independent operator O that commutes with the Hamiltonian. A complete set of commuting observables (CSCO) that commute with the Hamiltonian grant the quantum system all its quantum numbers. To each operator of the CSCO corresponds a quantum number choosing one of its eigenvalues, so these are all the quantum numbers that the system can have.
In general, there is more than one way to choose a set of linearly independent complete set of commuting operators. Consequently, different sets of quantum numbers may be used for the description of the same system in different situations.
Four quantum numbers can describe an electron in an atom completely:
The spin-orbital interaction, however, relates these numbers. Thus, a complete description of the system can be given with fewer quantum numbers, if orthogonal choices are made for these basis vectors.
It is important to specify the electron being referred to. This may, for example, be the highest occupied orbital electron; the actual differentiating electron; or the differentiating electron according to the aufbau approximation. In lanthanum, for example, the electrons involved are in the 6s; 5d; and 4f orbitals, respectively. In this case the principle quantum numbers are 6, 5, and 4. The "differentiating electron" means the electron that differentiates an element from the previous one.
The model used here describes electrons using four quantum numbers, n, ℓ, mℓ, ms, given below. It is also the common nomenclature in the classical description of nuclear particle states (e.g. protons and neutrons). A quantum description of molecular orbitals require different quantum numbers, because the Hamiltonian and its symmetries are quite different.
For particles in a time-independent potential (see Schrödinger equation), it also labels the nth eigenvalue of Hamiltonian (H), that is the energy, E with the contribution due to angular momentum (the term involving J2) left out. This number therefore has a dependence only on the distance between the electron and the nucleus (i.e., the radial coordinate, r). The average distance increases with n, and hence quantum states with different principal quantum numbers are said to belong to different shells.
In chemistry and spectroscopy, ℓ = 0 is called an s orbital, ℓ = 1 a p orbital, ℓ = 2 a d orbital, and ℓ = 3 an f orbital.
The value of ℓ ranges from 0 to n - 1, so the first p orbital (ℓ = 1) appears in the second electron shell (n = 2), the first d orbital (ℓ = 2) appears in the third shell (n = 3), and so on:
A quantum number beginning in n = 3,ℓ = 0, describes an electron in the s orbital of the third electron shell of an atom. In chemistry, this quantum number is very important, since it specifies the shape of an atomic orbital and strongly influences chemical bonds and bond angles.The azimuthal quantum number can also denote the number of angular nodes present in an orbital. For example, for p orbitals, ℓ = 1 and thus the amount of angular nodes in a p orbital = 1.
The values of mℓ range from -ℓ to ℓ, with integer intervals:
The s subshell (ℓ = 0) contains only one orbital, and therefore the mℓ of an electron in an s orbital will always be 0. The p subshell (ℓ = 1) contains three orbitals (in some systems, depicted as three "dumbbell-shaped" clouds), so the mℓ of an electron in a p orbital will be -1, 0, or 1. The d subshell (ℓ = 2) contains five orbitals, with mℓ values of -2, -1, 0, 1, and 2.
An electron has spin number s = , consequently ms will be ±, referring to "spin up" and "spin down" states. Each electron in any individual orbital must have different quantum numbers because of the Pauli exclusion principle, therefore an orbital never contains more than two electrons.
There are no universal fixed value for mℓ and ms values. Rather, the mℓ and ms values are arbitrary. The only requirement is that the naming schematic used within a particular set of calculations or descriptions must be consistent (e.g. the orbital occupied by the first electron in a p orbital could be described as mℓ = -1 or mℓ = 0 or mℓ = 1, but the mℓ value of the next unpaired electron in that orbital must be different; yet, the mℓ assigned to electrons in other orbitals again can be mℓ = -1 or mℓ = 0 or mℓ = 1).
These rules are summarized as follows:
|Name||Symbol||Orbital meaning||Range of values||Value examples|
|Principal quantum number||n||shell||1 n||n = 1, 2, 3, ...|
|Azimuthal quantum number (angular momentum)||ℓ||subshell (s orbital is listed as 0, p orbital as 1 etc.)||0 ℓ n - 1||for n = 3: |
ℓ = 0, 1, 2 (s, p, d)
|Magnetic quantum number (projection of angular momentum)||mℓ||energy shift (orientation of the subshell's shape)||-ℓ mℓℓ||for ℓ = 2: |
mℓ = -2, -1, 0, 1, 2
|Spin quantum number||ms||spin of the electron (- = "spin down", = "spin up")||-s mss||for an electron s = , |
so ms = -, +
Example: The quantum numbers used to refer to the outermost valence electrons of a carbon (C) atom, which are located in the 2p atomic orbital, are; n = 2 (2nd electron shell), ℓ = 1 (p orbital subshell), mℓ = 1, 0, -1, ms = (parallel spins).
Results from spectroscopy indicated that up to two electrons can occupy a single orbital. However two electrons can never have the same exact quantum state nor the same set of quantum numbers according to Hund's rules, which addresses the Pauli exclusion principle. A fourth quantum number with two possible values was added as an ad hoc assumption to resolve the conflict; this supposition could later be explained in detail by relativistic quantum mechanics and from the results of the renowned Stern-Gerlach experiment.
Many different models have been proposed throughout the history of quantum mechanics, but the most prominent system of nomenclature spawned from the Hund-Mulliken molecular orbital theory of Friedrich Hund, Robert S. Mulliken, and contributions from Schrödinger, Slater and John Lennard-Jones. This system of nomenclature incorporated Bohr energy levels, Hund-Mulliken orbital theory, and observations on electron spin based on spectroscopy and Hund's rules.
When one takes the spin-orbit interaction into consideration, the L and S operators no longer commute with the Hamiltonian, and their eigenvalues therefore change over time. Thus another set of quantum numbers should be used. This set includes
which gives the total angular momentum through the relation
analogous to the above and satisfies
This is the eigenvalue under reflection: positive (+1) for states which came from even ℓ and negative (-1) for states which came from odd ℓ. The former is also known as even parity and the latter as odd parity, and is given by
For example, consider the following 8 states, defined by their quantum numbers:
|n||ℓ||mℓ||ms||ℓ + s||ℓ - s||mℓ + ms|
The quantum states in the system can be described as linear combination of these 8 states. However, in the presence of spin-orbit interaction, if one wants to describe the same system by 8 states that are eigenvectors of the Hamiltonian (i.e. each represents a state that does not mix with others over time), we should consider the following 8 states:
|odd||coming from state (1) above|
|odd||coming from states (2) and (3) above|
|-||odd||coming from states (4) and (5) above|
|-||odd||coming from state (6) above|
|odd||coming from states (2) and (3) above|
|-||odd||coming from states (4) and (5) above|
|even||coming from state (7) above|
|-||even||coming from state (8) above|
In nuclei, the entire assembly of protons and neutrons (nucleons) has a resultant angular momentum due to the angular momenta of each nucleon, usually denoted I. If the total angular momentum of a neutron is jn = ℓ + s and for a proton is jp = ℓ + s (where s for protons and neutrons happens to be again (see note)), then the nuclear angular momentum quantum numbers I are given by:
Note: The orbital angular momenta of the nuclear (and atomic) states are all integer multiples of ? while the intrinsic angular momentum of the neutron and proton are half-integer multiples. It should be immediately apparent that the combination of the intrinsic spins of the nucleons with their orbital motion will always give half-integer values for the total spin, I, of any odd-A nucleus and integer values for any even-A nucleus.
The reason for the unusual fluctuations in I, even by differences of just one nucleon, are due to the odd and even numbers of protons and neutrons - pairs of nucleons have a total angular momentum of zero (just like electrons in orbitals), leaving an odd or even number of unpaired nucleons. The property of nuclear spin is an important factor for the operation of NMR spectroscopy in organic chemistry, and MRI in nuclear medicine, due to the nuclear magnetic moment interacting with an external magnetic field.
Elementary particles contain many quantum numbers which are usually said to be intrinsic to them. However, it should be understood that the elementary particles are quantum states of the standard model of particle physics, and hence the quantum numbers of these particles bear the same relation to the Hamiltonian of this model as the quantum numbers of the Bohr atom does to its Hamiltonian. In other words, each quantum number denotes a symmetry of the problem. It is more useful in quantum field theory to distinguish between spacetime and internal symmetries.
Typical quantum numbers related to spacetime symmetries are spin (related to rotational symmetry), the parity, C-parity and T-parity (related to the Poincaré symmetry of spacetime). Typical internal symmetries[clarification needed] are lepton number and baryon number or the electric charge. (For a full list of quantum numbers of this kind see the article on flavour.)
A minor but often confusing point is as follows: most conserved quantum numbers are additive, so in an elementary particle reaction, the sum of the quantum numbers should be the same before and after the reaction. However, some, usually called a parity, are multiplicative; i.e., their product is conserved. All multiplicative quantum numbers belong to a symmetry (like parity) in which applying the symmetry transformation twice is equivalent to doing nothing (involution).