Glossary of elementary quantum mechanics

Quantum mechanics
$\sigma_x \sigma_p \ge \frac{\hbar}{2}$ Uncertainty principle
Introduction Glossary History
Background Classical mechanics Old quantum theory Bra–ket notation Hamiltonian Interference
Fundamentals Complementarity Decoherence Entanglement Energy level Measurement Nonlocality Quantum number State Superposition Symmetry Tunnelling Uncertainty Wave function (collapse)
Experiments Afshar Bell's inequality Davisson–Germer Double-slit Elitzur–Vaidman Franck–Hertz Mach–Zehnder Popper Quantum eraser (delayed-choice) Schrödinger's cat Stern–Gerlach Wheeler's delayed-choice
Formulations Overview Heisenberg Interaction Matrix Phase-space Schrödinger Sum-over-histories (path integral)
Equations Dirac Klein–Gordon Pauli Rydberg Schrödinger
Interpretations Overview Consistent histories Copenhagen de Broglie–Bohm Ensemble Hidden-variable Many-worlds Objective collapse Bayesian Quantum logic Relational Stochastic Scale relativity Transactional
Advanced topics Quantum chaos Quantum computing Density matrix Quantum field theory Fractional quantum mechanics Quantum information science Relativistic quantum mechanics Scattering theory Quantum statistical mechanics
Scientists Aharonov Bell Blackett Bloch Bohm Bohr Born Bose de Broglie Candlin Compton Dirac Davisson Debye Ehrenfest Einstein Everett Fock Fermi Feynman Glauber Gutzwiller Heisenberg Hilbert Jordan Kramers Pauli Lamb Landau Laue Moseley Millikan Onnes Planck Rabi Raman Rydberg Schrödinger Sommerfeld von Neumann Weyl Wien Wigner Zeeman Zeilinger

This is a glossary for the terminology often encountered in undergraduate quantum mechanics courses.

Cautions:

Different authors may have different definitions for the same term.
The discussions are restricted to Schrödinger picture and non-relativistic quantum mechanics.
Notation:
- $| x \rangle$ - position eigenstate
- $| \alpha \rangle, | \beta \rangle, | \gamma \rangle ...$ - wavefunction of the state of the system
- $\Psi$ - total wavefunction of a system
- $\psi$ - wavefunction of a system (maybe a particle)
- $\psi_\alpha(x,t)$ - wavefunction of a particle in position representation, equal to $\langle x | \alpha \rangle$

Formalism

Kinematical postulates

a complete set of wavefunctions: A basis of the Hilbert space of wavefunctions with respect to a system.

bra: The Hermitian conjugate of a ket is called a bra. $\langle \alpha| = (|\alpha \rangle)^\dagger$ . See "bra–ket notation".

Bra–ket notation: The bra–ket notation is a way to represent the states and operators of a system by angle brackets and vertical bars, for example, $| \alpha \rangle$ and $| \alpha \rangle \langle \beta|$ .

Density matrix

Physically, the density matrix is a way to represent pure states and mixed states. The density matrix of pure state whose ket is

|\alpha \rangle

|\alpha \rangle \langle \alpha|

Mathematically, a density matrix has to satisfy the following conditions:

$\operatorname{Tr}(\rho) = 1$
$\rho^\dagger = \rho$

Density operator: Synonymous to "density matrix".

Dirac notation: Synonymous to "bra–ket notation".

Hilbert space: Given a system, the possible pure state can be represented as a vector in a Hilbert space. Each ray (vectors differ by phase and magnitude only) in the corresponding Hilbert space represent a state.^{[nb 1]}

Ket: A wavefunction expressed in the form $|a\rangle$ is called a ket. See "bra–ket notation".

Mixed state

A mixed state is a statistical ensemble of pure state.

criterion:

Pure state:

\operatorname{Tr}(\rho^2) = 1

Mixed state:

\operatorname{Tr}(\rho^2) < 1

Normalizable wavefunction: A wavefunction $|\alpha' \rangle$ is said to be normalizable if $\langle \alpha'| \alpha' \rangle < \infty$ . A normalizable wavefunction can be made to be normalized by $|a' \rangle \to \alpha = \frac{|\alpha' \rangle}{\sqrt{\langle \alpha'|\alpha' \rangle}}$ .

Normalized wavefunction: A wavefunction $| a \rangle$ is said to be normalized if $\langle a| a \rangle = 1$ .

Pure state: A state which can be represented as a wavefunction / ket in Hilbert space / solution of Schrödinger equation is called pure state. See "mixed state".

Quantum numbers: a way of representing a state by several numbers, which corresponds to a complete set of commuting observables.; A common example of quantum numbers is the possible state of an electron in a central potential: $(n, l, m, s)$ , which corresponds to the eigenstate of observables $H$ (in terms of $r$ ), $L$ (magnitude of angular momentum), $L_z$ (angular momentum in $z$ -direction), and $S_z$ .

Spin wavefunction

Part of a wavefunction of particle(s). See "total wavefunction of a particle".

Spinor

Synonymous to "spin wavefunction".

Spatial wavefunction

Part of a wavefunction of particle(s). See "total wavefunction of a particle".

State: A state is a complete description of the observable properties of a physical system.; Sometimes the word is used as a synonym of "wavefunction" or "pure state".

State vector: synonymous to "wavefunction".

Statistical ensemble: A large number of copies of a system.

System: A sufficiently isolated part in the universe for investigation.

Tensor product of Hilbert space: When we are considering the total system as a composite system of two subsystems A and B, the wavefunctions of the composite system are in a Hilbert space $H_A \otimes H_B$ , if the Hilbert space of the wavefunctions for A and B are $H_A$ and $H_B$ respectively.

Total wavefunction of a particle: For single-particle system, the total wavefunction $\Psi$ of a particle can be expressed as a product of spatial wavefunction and the spinor. The total wavefunctions are in the tensor product space of the Hilbert space of the spatial part (which is spanned by the position eigenstates) and the Hilbert space for the spin.

Wavefunction

The word "wavefunction" could mean one of following:

A vector in Hilbert space which can represent a state; synonymous to "ket" or "state vector".
The state vector in a specific basis. It can be seen as a covariant vector in this case.
The state vector in position representation, e.g. $\psi_\alpha(x_0) = \langle x_0 | \alpha \rangle$ , where $| x_0 \rangle$ is the position eigenstate.

Dynamics

Main article: Schrödinger equation

Degeneracy: See "degenerate energy level".

Degenerate energy level: If the energy of different state (wavefunctions which are not scalar multiple of each other) is the same, the energy level is called degenerate.; There is no degeneracy in 1D system.

Energy spectrum

The energy spectrum refers to the possible energy of a system.

For bound system (bound states), the energy spectrum is discrete; for unbound system (scattering states), the energy spectrum is continuous.

related mathematical topics: Sturm–Liouville equation

Hamiltonian $\hat H$: The operator represents the total energy of the system.

Schrödinger equation

i\hbar\frac{\partial}{\partial t} |\alpha\rangle = \hat H | \alpha \rangle

-- (1)

(1) is sometimes called "Time-Dependent Schrödinger equation" (TDSE).

Time-Independent Schrödinger Equation (TISE)

A modification of the Time-Dependent Schrödinger equation as an eigenvalue problem. The solutions are energy eigenstate of the system.

E \alpha \rangle = \hat H | \alpha \rangle

-- (2)

Dynamics related to single particle in a potential / other spatial properties

In this situation, the SE is given by the form

i\hbar\frac{\partial}{\partial t} \Psi_\alpha(\mathbf{r},\,t) = \hat H \Psi = \left(-\frac{\hbar^2}{2m}\nabla^2 + V(\mathbf{r})\right)\Psi_\alpha(\mathbf{r},\,t) = -\frac{\hbar^2}{2m}\nabla^2\Psi_\alpha(\mathbf{r},\,t) + V(\mathbf{r})\Psi_\alpha(\mathbf{r},\,t)

It can be derived from (1) by considering

\Psi_\alpha(x,t) := \langle x |\alpha\rangle

and

\hat H := -\frac{\hbar^2}{2m}\nabla^2 + \hat V

Bound state

A state is called bound state if its position probability density at infinite tends to zero for all the time. Roughly speaking, we can expect to find the particle(s) in a finite size region with certain probability. More precisely,

| \psi( \mathbf{r}, t) |^2 \to 0

when

|\mathbf{r}| \to +\infty

, for all

t >0

There is a criterion in terms of energy:

Let

E

be the expectation energy of the state. It is a bound state iff

E < \operatorname{min}\{ V( r \to - \infty ) , V( r \to + \infty ) \}

Position representation and momentum representation: Position representation of a wavefunction: $\Psi_\alpha(x,t) := \langle x |\alpha\rangle$ ,; momentum representation of a wavefunction: $\tilde{\Psi}_\alpha(p,t) := \langle p |\alpha\rangle$ ;; where $| x \rangle$ is the position eigenstate and $| p \rangle$ the momentum eigenstate respectively.; The two representations are linked by Fourier transform.

Probability amplitude: Synonymous to "probability density".

Probability current

Having the metaphor of probability density as mass density, then probability current

J

is the current:

J(x,t) = \frac{i \hbar}{2m} ( \psi \frac{\partial \psi^*}{\partial x} - \frac{\partial \psi}{\partial x} \psi )

The probability current and probability density together satisfy the continuity equation:

\frac{\partial }{\partial t}|\psi(x,t)|^2 + \nabla \cdot \mathbf{J(x,t)} = 0

Probability density: Given the wavefunction of a particle, $|\psi(x,t)|^2$ is the probability density at position $x$ and time $t$ . $|\psi(x_0,t)|^2 \, dx$ means the probability of finding the particle near $x_0$ .

Scattering state

The wavefunction of scattering state can be understood as a propagating wave. See also "bound state".

There is a criterion in terms of energy:

Let

E

be the expectation energy of the state. It is a scattering state iff

E > \operatorname{min}\{ V( r \to - \infty ) , V( r \to + \infty ) \}

Square-integrable

Square-integrable is a necessary condition for a function being the position/momentum representation of a wavefunction of a bound state of the system.

Given the position representation

\Psi(x,t)

of a state vector of a wavefunction, square-integrable means:

1D case:

\int_{-\infty}^{+\infty} |\Psi(x,t)|^2 \, dx < +\infty

3D case:

\int_{V} |\Psi(\mathbf{r},t)|^2 \, dV < +\infty

Stationary state

A stationary state of a bound system is an eigenstate of Hamiltonian operator. Classically, it corresponds to standing wave. It is equivalent to the following things:^{[nb 2]}

an eigenstate of the Hamiltonian operator
an eigenfunction of Time-Independent Schrödinger Equation
a state of definite energy
a state which "every expectation value is constant in time"
a state whose probability density ( $|\psi(x,t)|^2$ ) does not change with respect to time, i.e. $\frac{d}{dt}|\Psi(x,t)|^2 = 0$

Measurement postulates

Main article: Measurement in quantum mechanics

Born's rule: The probability of the state $| \alpha \rangle$ collapse to an eigenstate $| k \rangle$ of an observable is given by $|\langle k | \alpha \rangle|^2$ .
Collapse: "Collapse" means the sudden process which the state of the system will "suddenly" change to an eigenstate of the observable during measurement.
Eigenstates: An eigenstate of an operator $A$ is a vector satisfied the eigenvalue equation: $A |\alpha \rangle = c |\alpha \rangle$ , where $c$ is a scalar.; Usually, in bra–ket notation, the eigenstate will be represented by its corresponding eigenvalue if the corresponding observable is understood.

Expectation value

The expectation value

<M>

of the observable M with respect to a state

| \alpha

is the average outcome of measuring

M

with respect to an ensemble of state

| \alpha

<M>

can be calculated by:

<M> = \langle \alpha | M | \alpha \rangle

If the state is given by a density matrix

\rho

<M> = \operatorname{Tr}( M \rho)

Hermitian operator: An operator satisfying $A = A^\dagger$ .; Equivalently, $\langle \alpha | A|\alpha \rangle = \langle \alpha | A^\dagger |\alpha \rangle$ for all allowable wavefunction $|\alpha\rangle$ .

Observable: Mathematically, it is represented by a Hermitian operator.

Quantum Zeno effect: The phenomenon that a frequent measurement leads to "freezing" of the state.

Indistinguishable particles

Exchange

Intrinsically identical particles: If the intrinsic properties (properties that can be measured but are independent of the quantum state, e.g. charge, total spin, mass) of two particles are the same, they are said to be (intrinsically) identical.

Indistinguishable particles: If a system shows measurable differences when one of its particles is replaced by another particle, these two particles are called distinguishable.

Bosons: Bosons are particles with integer spin (s = 0, 1, 2, ... ). They can either be elementary (like photons) or composite (such as mesons, nuclei or even atoms). There are five known elementary bosons: the four force carrying gauge bosons γ (photon), g (gluon), Z (Z boson) and W (W boson), as well as the Higgs boson.

Fermions: Fermions are particles with half-integer spin (s = 1/2, 3/2, 5/2, ... ). Like bosons, they can be elementary or composite particles. There are two types of elementary fermions: quarks and leptons, which are the main constituents of ordinary matter.

Anti-symmetrization of wavefunctions

Symmetrization of wavefunctions

Pauli exclusion principle

Quantum statistical mechanics

Bose–Einstein distribution
Bose–Einstein condensation
Bose–Einstein condensation state (BEC state)
Fermi energy
Fermi–Dirac distribution
Slater determinant

Nonlocality

Entanglement
Bell's inequality
Entangled state
separable state
no cloning theorem

Rotation: spin/angular momentum

Spin

angular momentum
Clebsch–Gordan coefficients
singlet state and triplet state

Approximation methods

adiabatic approximation
Born–Oppenheimer approximation
WKB approximation
time-dependent perturbation theory
time-independent perturbation theory

Historical Terms / semi-classical treatment

Ehrenfest theorem: A theorem connecting the classical mechanics and result dervied from Schrödinger equation.
first quantization: $x \to \hat x , \, p \to i \hbar \frac{\partial}{\partial x}$
wave–particle duality

Uncategorized terms

uncertainty principle
Canonical commutation relations
Path integral

wavenumber

Notes

↑ Exception: superselection rules
↑ Some textbooks (e.g. Cohen Tannoudji, Liboff) define "stationary state" as "an eigenstate of a Hamiltonian" without specific to bound states.

References

Elementary textbooks
- Griffiths, David J. (2004). Introduction to Quantum Mechanics (2nd ed.). Prentice Hall. ISBN 0-13-805326-X.
- Liboff, Richard L. (2002). Introductory Quantum Mechanics. Addison-Wesley. ISBN 0-8053-8714-5.
- Shankar, R. (1994). Principles of Quantum Mechanics. Springer. ISBN 0-306-44790-8.
- Claude Cohen-Tannoudji, Bernard Diu, Frank Laloë (2006). Quantum Mechanics. Wiley-Interscience. ISBN 978-0-471-56952-7.
Graduate textook
- Sakurai, J. J. (1994). Modern Quantum Mechanics. Addison Wesley. ISBN 0-201-53929-2.
Other
- Greenberger, Daniel; Hentschel, Klaus; Weinert, Friedel (Eds.) (2009). Compendium of Quantum Physics - Concepts, Experiments, History and Philosophy. Springer. ISBN 978-3-540-70622-9.
- d'Espagnat, Bernard (2003). Veiled Reality: An Analysis of Quantum Mechanical Concepts (1st ed.). US: Westview Press.

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