Part of a series of articles about
Quantum mechanics
${\displaystyle i\hslash \frac{d}{dt}|\mathrm{\Psi }⟩=\hat{H}|\mathrm{\Psi }⟩}$ Schrödinger equation
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 Bell's inequality CHSH inequality Davisson–Germer Double-slit Elitzur–Vaidman Franck–Hertz Leggett inequality Leggett–Garg inequality 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 Bayesian Consciousness causes collapse Consistent histories Copenhagen de Broglie–Bohm Ensemble Hidden-variable Many-worlds Objective-collapse Quantum logic Superdeterminism Relational Transactional
Advanced topics Relativistic quantum mechanics Quantum field theory Quantum information science Quantum computing Quantum chaos EPR paradox Density matrix Scattering theory Quantum statistical mechanics Quantum machine learning
Scientists Aharonov Bell Bethe Blackett Bloch Bohm Bohr Born Bose de Broglie Compton Dirac Davisson Debye Ehrenfest Einstein Everett Fock Fermi Feynman Glauber Gutzwiller Heisenberg Hilbert Jordan Kramers Lamb Landau Laue Moseley Millikan Onnes Pauli Planck Rabi Raman Rydberg Schrödinger Simmons Sommerfeld von Neumann Weyl Wien Wigner Zeeman Zeilinger
v t e

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

Cautions:

• Different authors may have different definitions for the same term.
• The discussions are restricted toSchrödinger picture and non-relativistic quantum mechanics.
• Notation:
  • ${\displaystyle |x⟩}$ - position eigenstate
  • ${\displaystyle |\alpha ⟩,|\beta ⟩,|\gamma ⟩...}$ - wave function of the state of the system
  • ${\displaystyle \mathrm{\Psi }}$ - total wave function of a system
  • ${\displaystyle \psi }$ - wave function of a system (maybe a particle)
  • ${\displaystyle {\psi }_{\alpha }(x,t)}$ - wave function of a particle in position representation, equal to${\displaystyle ⟨x|\alpha ⟩}$

a complete set of wave functions

Abasis of theHilbert space of wave functions with respect to a system.

bra

The Hermitian conjugate of a ket is called a bra.${\displaystyle ⟨\alpha |=(|\alpha ⟩{)}^{†}}$. 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,${\displaystyle |\alpha ⟩}$ and${\displaystyle |\alpha ⟩⟨\beta |}$.

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${\displaystyle |\alpha ⟩}$ is${\displaystyle |\alpha ⟩⟨\alpha |}$.

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

• ${\displaystyle \mathrm{Tr}(\rho )=1}$
• ${\displaystyle {\rho }^{†}=\rho }$

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 aHilbert space. Each ray (vectors differ by phase and magnitude only) in the correspondingHilbert space represent a state.^{[nb 1]}

Ket

A wave function expressed in the form${\displaystyle |a⟩}$ is called a ket. See "bra–ket notation".

Mixed state

A mixed state is a statistical ensemble of pure state.

criterion:

• Pure state:${\displaystyle \mathrm{Tr}({\rho }^2)=1}$
• Mixed state:

Normalizable wave function

A wave function${\displaystyle |{\alpha }^{\prime }⟩}$ is said to be normalizable if. A normalizable wave function can be made to be normalized by${\displaystyle |a^{\prime }⟩\to \alpha =\frac{|{\alpha }^{\prime }⟩}{\sqrt{⟨{\alpha }^{\prime }|{\alpha }^{\prime }⟩}}}$.

Normalized wave function

A wave function${\displaystyle |a⟩}$ is said to be normalized if${\displaystyle ⟨a|a⟩=1}$.

Pure state

A state which can be represented as a wave function / 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 acomplete set of commuting observables.

A common example of quantum numbers is the possible state of an electron in a central potential:${\displaystyle (n,\ell ,m,s)}$, which corresponds to the eigenstate of observables${\displaystyle H}$ (in terms of${\displaystyle r}$),${\displaystyle L}$ (magnitude of angular momentum),${\displaystyle L_z}$ (angular momentum in${\displaystyle z}$-direction), and${\displaystyle S_z}$.

Spin wave function

Part of a wave function of particle(s). See "total wave function of a particle".

Spinor

Synonymous to "spin wave function".

Spatial wave function

Part of a wave function of particle(s). See "total wave function 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 "wave function" or "pure state".

State vector

synonymous to "wave function".

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 wave functions of the composite system are in a Hilbert space${\displaystyle H_A\otimes H_B}$, if the Hilbert space of the wave functions for A and B are${\displaystyle H_A}$ and${\displaystyle H_B}$ respectively.

Total wave function of a particle

For single-particle system, the total wave function${\displaystyle \mathrm{\Psi }}$ of a particle can be expressed as a product of spatial wave function and the spinor. The total wave functions 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.

Wave function

The word "wave function" could mean one of following:

1. A vector in Hilbert space which can represent a state; synonymous to "ket" or "state vector".
2. The state vector in a specific basis. It can be seen as acovariant vector in this case.
3. The state vector in position representation, e.g.${\displaystyle {\psi }_{\alpha }(x_0)=⟨x_0|\alpha ⟩}$, where${\displaystyle |x_0⟩}$ is the position eigenstate.

Degeneracy

See "degenerate energy level".

Degenerate energy level

If the energy of different state (wave functions which are not scalar multiple of each other) is the same, the energy level is called degenerate.

There is no degeneracy in a 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${\displaystyle \hat{H}}$

The operator represents the total energy of the system.

Schrödinger equation

The Schrödinger equation relates the Hamiltonian operator acting on a wave function to its time evolution (Equation1):$${\displaystyle i\hslash \frac{\mathrm{\partial }}{\mathrm{\partial }t}|\alpha ⟩=\hat{H}|\alpha ⟩}$$Equation (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 eigenstates of the system (Equation2):$${\displaystyle E|\alpha ⟩=\hat{H}|\alpha ⟩}$$

In this situation, the SE is given by the form$${\displaystyle i\hslash \frac{\mathrm{\partial }}{\mathrm{\partial }t}{\mathrm{\Psi }}_{\alpha }(\mathbf{r},t)=\hat{H}{\mathrm{\Psi }}_{\alpha }(\mathbf{r},t)=\left(-\frac{{\hslash }^2}{2m}{\mathrm{\nabla }}^2+V(\mathbf{r})\right){\mathrm{\Psi }}_{\alpha }(\mathbf{r},t)=-\frac{{\hslash }^2}{2m}{\mathrm{\nabla }}^2{\mathrm{\Psi }}_{\alpha }(\mathbf{r},t)+V(\mathbf{r}){\mathrm{\Psi }}_{\alpha }(\mathbf{r},t)}$$ It can be derived from (1) by considering${\displaystyle {\mathrm{\Psi }}_{\alpha }(x,t):=⟨x|\alpha ⟩}$ and${\displaystyle \hat{H}:=-\frac{{\hslash }^2}{2m}{\mathrm{\nabla }}^2+\hat{V}}$

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,${\displaystyle |\psi (\mathbf{r},t){|}^2\to 0}$ when${\displaystyle |\mathbf{r}|\to +\mathrm{\infty }}$, for all${\displaystyle t>0}$.

There is a criterion in terms of energy:

Let${\displaystyle E}$ be the expectation energy of the state. It is a bound state if and only if.

Position representation and momentum representation

Position representation of a wave function

${\displaystyle {\mathrm{\Psi }}_{\alpha }(x,t):=⟨x|\alpha ⟩}$,

momentum representation of a wave function

${\displaystyle {\tilde{\mathrm{\Psi }}}_{\alpha }(p,t):=⟨p|\alpha ⟩}$ ;

where${\displaystyle |x⟩}$ is the position eigenstate and${\displaystyle |p⟩}$ the momentum eigenstate respectively.

The two representations are linked byFourier transform.

Probability amplitude

A probability amplitude is of the form${\displaystyle ⟨\alpha |\psi ⟩}$.

Probability current

Having the metaphor of probability density as mass density, then probability current${\displaystyle J}$ is the current:${\displaystyle J(x,t)=\frac{i\hslash }{2m}\left(\psi \frac{\mathrm{\partial }{\psi }^{\ast }}{\mathrm{\partial }x}-\frac{\mathrm{\partial }\psi }{\mathrm{\partial }x}\psi \right)}$ The probability current and probability density together satisfy thecontinuity equation:$${\displaystyle \frac{\mathrm{\partial }}{\mathrm{\partial }t}|\psi (x,t){|}^2+\mathrm{\nabla }\cdot \mathbf{J}(x,t)=0}$$

Probability density

Given the wave function of a particle,${\displaystyle |\psi (x,t){|}^2}$ is the probability density at position${\displaystyle x}$ and time${\displaystyle t}$.${\displaystyle |\psi (x_0,t){|}^{2}dx}$ means the probability of finding the particle near${\displaystyle x_0}$.

Scattering state

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

There is a criterion in terms of energy:

Let${\displaystyle E}$ be the expectation energy of the state. It is a scattering state if and only if${\displaystyle E>\min \{V(r\to -\mathrm{\infty }),V(r\to +\mathrm{\infty })\}}$.

Square-integrable

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

Given the position representation${\displaystyle \mathrm{\Psi }(x,t)}$ of a state vector of a wave function, square-integrable means:

• 1D case:.
• 3D case:.

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 (${\displaystyle |\psi (x,t){|}^2}$) does not change with respect to time, i.e.${\displaystyle \frac{d}{dt}|\mathrm{\Psi }(x,t){|}^2=0}$

Born's rule

The probability of the state${\displaystyle |\alpha ⟩}$ collapse to an eigenstate${\displaystyle |k⟩}$ of an observable is given by${\displaystyle |⟨k|\alpha ⟩{|}^2}$.

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${\displaystyle A}$ is a vector satisfied the eigenvalue equation:${\displaystyle A|\alpha ⟩=c|\alpha ⟩}$, where${\displaystyle c}$ 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${\displaystyle ⟨M⟩}$ of the observableM with respect to a state${\displaystyle |\alpha }$ is the average outcome of measuring${\displaystyle M}$ with respect to an ensemble of state${\displaystyle |\alpha }$.

${\displaystyle ⟨M⟩}$ can be calculated by:$${\displaystyle ⟨M⟩=⟨\alpha |M|\alpha ⟩.}$$

If the state is given by a density matrix${\displaystyle \rho }$,${\displaystyle ⟨M⟩=\mathrm{Tr}(M\rho )}$.

Hermitian operator

An operator satisfying${\displaystyle A=A^{†}}$.

Equivalently,${\displaystyle ⟨\alpha |A|\alpha ⟩=⟨\alpha |A^{†}|\alpha ⟩}$ for all allowable wave function${\displaystyle |\alpha ⟩}$.

Observable

Mathematically, it is represented by a Hermitian operator.

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 integerspin (s = 0, 1, 2, ... ). They can either be elementary (likephotons) or composite (such asmesons, 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 theHiggs 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 andleptons, which are the main constituents of ordinary matter.

Anti-symmetrization of wave functions

Symmetrization of wave functions

Pauli exclusion principle

Bose–Einstein distribution

Bose–Einstein condensation

Bose–Einstein condensation state (BEC state)

Fermi energy

Fermi–Dirac distribution

Slater determinant

Entanglement

Bell's inequality

Entangled state

separable state

no-cloning theorem

Spin

angular momentum

Clebsch–Gordan coefficients

singlet state andtriplet state

adiabatic approximation

Born–Oppenheimer approximation

WKB approximation

time-dependent perturbation theory

time-independent perturbation theory

Ehrenfest theorem

A theorem connecting the classical mechanics and result derived from Schrödinger equation.

first quantization

${\displaystyle x\to \hat{x},p\to i\hslash \frac{\mathrm{\partial }}{\mathrm{\partial }x}}$

wave–particle duality

uncertainty principle

Canonical commutation relations

The canonical commutation relations are the commutators between canonically conjugate variables. For example, position${\displaystyle \hat{x}}$ and momentum${\displaystyle \hat{p}}$:$${\displaystyle [\hat{x},\hat{p}]=\hat{x}\hat{p}-\hat{p}\hat{x}=i\hslash }$$

Path integral

wavenumber

• Mathematical formulations of quantum mechanics
• List of mathematical topics in quantum theory
• List of quantum-mechanical potentials
• Introduction to quantum mechanics

• 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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• Quantum mechanics

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