Glossary of elementary quantum mechanics
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This is a glossary for the terminology often encountered in undergraduate
quantum mechanics Quantum mechanics is a fundamental theory in physics that provides a description of the physical properties of nature at the scale of atoms and subatomic particles. It is the foundation of all quantum physics including quantum chemistr ...
courses. Cautions: * Different authors may have different definitions for the same term. * The discussions are restricted to
Schrödinger picture In physics, the Schrödinger picture is a formulation of quantum mechanics in which the state vectors evolve in time, but the operators (observables and others) are mostly constant with respect to time (an exception is the Hamiltonian which may ...
and non-
relativistic quantum mechanics In physics, relativistic quantum mechanics (RQM) is any Poincaré covariant formulation of quantum mechanics (QM). This theory is applicable to massive particles propagating at all velocities up to those comparable to the speed of light  ...
. * Notation: ** , x \rangle - position eigenstate ** , \alpha \rangle, , \beta \rangle, , \gamma \rangle ... - wave function of the state of the system ** \Psi - total wave function of a system ** \psi - wave function of a system (maybe a particle) ** \psi_\alpha(x,t) - wave function of a particle in position representation, equal to \langle x , \alpha \rangle


Formalism


Kinematical postulates

; a complete set of wave functions : A
basis Basis may refer to: Finance and accounting * Adjusted basis, the net cost of an asset after adjusting for various tax-related items *Basis point, 0.01%, often used in the context of interest rates * Basis trading, a trading strategy consisting ...
of the Hilbert space of wave functions 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 In quantum mechanics, a density matrix (or density operator) is a matrix that describes the quantum state of a physical system. It allows for the calculation of the probabilities of the outcomes of any measurement performed upon this system, using ...
: 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 is , \alpha \rangle \langle \alpha, . : Mathematically, a density matrix has to satisfy the following conditions: :* \operatorname(\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.Exception: superselection rules ; Ket : A wave function 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: ; Normalizable wave function : A wave function , \alpha' \rangle is said to be normalizable if \langle \alpha', \alpha' \rangle < \infty. A normalizable wave function can be made to be normalized by , a' \rangle \to \alpha = \frac. ; Normalized wave function : A wave function , a \rangle is said to be normalized if \langle a, a \rangle = 1. ;
Pure state In quantum physics, a quantum state is a mathematical entity that provides a probability distribution for the outcomes of each possible measurement on a system. Knowledge of the quantum state together with the rules for the system's evolution in t ...
: 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 In quantum physics and chemistry, quantum numbers describe values of conserved quantities in the dynamics of a quantum system. Quantum numbers correspond to eigenvalues of operators that commute with the Hamiltonian—quantities that can be k ...
: a way of representing a state by several numbers, which corresponds to a
complete set of commuting observables In quantum mechanics, a complete set of commuting observables (CSCO) is a set of commuting operators whose common eigenvectors can be used as a basis to express any quantum state. In the case of operators with discrete spectra, a CSCO is a set of c ...
. : A common example of quantum numbers is the possible state of an electron in a central potential: (n, \ell, 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 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 State may refer to: Arts, entertainment, and media Literature * ''State Magazine'', a monthly magazine published by the U.S. Department of State * ''The State'' (newspaper), a daily newspaper in Columbia, South Carolina, United States * ''Our S ...
: 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 In physics, specifically statistical mechanics, an ensemble (also statistical ensemble) is an idealization consisting of a large number of virtual copies (sometimes infinitely many) of a system, considered all at once, each of which represents a ...
: A large number of copies of a system. ; System : A sufficiently isolated part in the universe for investigation. ;
Tensor product In mathematics, the tensor product V \otimes W of two vector spaces and (over the same field) is a vector space to which is associated a bilinear map V\times W \to V\otimes W that maps a pair (v,w),\ v\in V, w\in W to an element of V \otime ...
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 H_A \otimes H_B, if the Hilbert space of the wave functions for A and B are H_A and H_B respectively. ; Total wave function of a particle : For single-particle system, the total wave function \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: :# 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 physics, especially in multilinear algebra and tensor analysis, covariance and contravariance describe how the quantitative description of certain geometric or physical entities changes with a change of basis. In modern mathematical notation ...
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

; 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 Hamiltonian may refer to: * Hamiltonian mechanics, a function that represents the total energy of a system * Hamiltonian (quantum mechanics), an operator corresponding to the total energy of that system ** Dyall Hamiltonian, a modified Hamiltonian ...
\hat H : The operator represents the total energy of the system. ;
Schrödinger equation The Schrödinger equation is a linear partial differential equation that governs the wave function of a quantum-mechanical system. It is a key result in quantum mechanics, and its discovery was a significant landmark in the development of th ...
: The Schrödinger equation relates the Hamiltonian operator acting on a wave function to its time evolution (Equation ): i\hbar\frac , \alpha\rangle = \hat H , \alpha \rangle 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 (Equation ): E , \alpha \rangle = \hat H , \alpha \rangle


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

In this situation, the SE is given by the form i \hbar \frac \Psi_\alpha(\mathbf,\,t) = \hat H \Psi_\alpha(\mathbf,\,t) = \left(-\frac\nabla^2 + V(\mathbf)\right)\Psi_\alpha(\mathbf,\,t) = -\frac\nabla^2\Psi_\alpha(\mathbf,\,t) + V(\mathbf)\Psi_\alpha(\mathbf,\,t) It can be derived from (1) by considering \Psi_\alpha(x,t) := \langle x , \alpha\rangle and \hat H := -\frac \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, t) , ^2 \to 0 when , \mathbf, \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 if and only if E < \operatorname\. ; Position representation and momentum representation :; Position representation of a wave function: \Psi_\alpha(x,t) := \langle x , \alpha\rangle, :; momentum representation of a wave function: \tilde_\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 : A probability amplitude is of the form \langle \alpha , \psi\rangle. ;
Probability current In quantum mechanics, the probability current (sometimes called probability flux) is a mathematical quantity describing the flow of probability. Specifically, if one thinks of probability as a heterogeneous fluid, then the probability current is th ...
: Having the metaphor of probability density as mass density, then probability current J is the current: J(x,t) = \frac \left( \psi \frac - \frac \psi \right) The probability current and probability density together satisfy the continuity equation: \frac , \psi(x,t), ^2 + \nabla \cdot \mathbf(x,t) = 0 ;
Probability density In probability theory, a probability density function (PDF), or density of a continuous random variable, is a function whose value at any given sample (or point) in the sample space (the set of possible values taken by the random variable) can ...
: Given the wave function 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 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 E be the expectation energy of the state. It is a scattering state if and only if E > \operatorname\. ; 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 \Psi(x,t) of a state vector of a wave function, square-integrable means: :* 1D case: \int_^ , \Psi(x,t), ^2 \, dx < +\infty. :* 3D case: \int_ , \Psi(\mathbf,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:Some textbooks (e.g. Cohen Tannoudji, Liboff) define "stationary state" as "an eigenstate of a Hamiltonian" without specific to bound states. :* 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 , \Psi(x,t), ^2 = 0


Measurement postulates

; 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 or its variants may refer to: Concepts * Collapse (structural) * Collapse (topology), a mathematical concept * Collapsing manifold * Collapse, the action of collapsing or telescoping objects * Collapsing user interface elements ** ...
: "Collapse" means the sudden process which the state of the system will "suddenly" change to an eigenstate of the observable during measurement. ;
Eigenstates In quantum physics, a quantum state is a mathematical entity that provides a probability distribution for the outcomes of each possible measurement on a system. Knowledge of the quantum state together with the rules for the system's evolution i ...
: 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 In probability theory, the expected value (also called expectation, expectancy, mathematical expectation, mean, average, or first moment) is a generalization of the weighted average. Informally, the expected value is the arithmetic mean of a l ...
: The expectation value \langle M \rangle 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. : \langle M \rangle can be calculated by: \langle M \rangle = \langle \alpha , M , \alpha \rangle. : If the state is given by a density matrix \rho, \langle M \rangle = \operatorname( M \rho). ;
Hermitian operator In mathematics, a self-adjoint operator on an infinite-dimensional complex vector space ''V'' with inner product \langle\cdot,\cdot\rangle (equivalently, a Hermitian operator in the finite-dimensional case) is a linear map ''A'' (from ''V'' to it ...
: An operator satisfying A = A^\dagger. : Equivalently, \langle \alpha , A, \alpha \rangle = \langle \alpha , A^\dagger , \alpha \rangle for all allowable wave function , \alpha\rangle. ;
Observable In physics, an observable is a physical quantity that can be measured. Examples include position and momentum. In systems governed by classical mechanics, it is a real-valued "function" on the set of all possible system states. In quantum phy ...
: Mathematically, it is represented by a Hermitian operator.


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 In quantum mechanics, identical particles (also called indistinguishable or indiscernible particles) are particles that cannot be distinguished from one another, even in principle. Species of identical particles include, but are not limited to, ...
: If a system shows measurable differences when one of its particles is replaced by another particle, these two particles are called distinguishable. ;
Boson In particle physics, a boson ( ) is a subatomic particle whose spin quantum number has an integer value (0,1,2 ...). Bosons form one of the two fundamental classes of subatomic particle, the other being fermions, which have odd half-integer spi ...
s :Bosons are particles with integer spin (''s'' = 0, 1, 2, ... ). They can either be elementary (like
photon A photon () is an elementary particle that is a quantum of the electromagnetic field, including electromagnetic radiation such as light and radio waves, and the force carrier for the electromagnetic force. Photons are massless, so they a ...
s) or composite (such as
mesons In particle physics, a meson ( or ) is a type of hadronic subatomic particle composed of an equal number of quarks and antiquarks, usually one of each, bound together by the strong interaction. Because mesons are composed of quark subparticles, ...
, 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 In particle physics, the W and Z bosons are vector bosons that are together known as the weak bosons or more generally as the intermediate vector bosons. These elementary particles mediate the weak interaction; the respective symbols are , , and ...
), 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 wave functions ; Symmetrization of wave functions ;
Pauli exclusion principle In quantum mechanics, the Pauli exclusion principle states that two or more identical particles with half-integer spins (i.e. fermions) cannot occupy the same quantum state within a quantum system simultaneously. This principle was formulat ...


Quantum statistical mechanics

;
Bose–Einstein distribution Bose–Einstein may refer to: * Bose–Einstein condensate ** Bose–Einstein condensation (network theory) * Bose–Einstein correlations * Bose–Einstein statistics In quantum statistics, Bose–Einstein statistics (B–E statistics) describ ...
;
Bose–Einstein condensation Bose–Einstein may refer to: * Bose–Einstein condensate ** Bose–Einstein condensation (network theory) * Bose–Einstein correlations * Bose–Einstein statistics In quantum statistics, Bose–Einstein statistics (B–E statistics) describe ...
; Bose–Einstein condensation state (BEC state) ; Fermi energy ;
Fermi–Dirac distribution Fermi–Dirac may refer to: * Fermi–Dirac statistics Fermi–Dirac statistics (F–D statistics) is a type of quantum statistics that applies to the physics of a system consisting of many non-interacting, identical particles that obey the Pa ...
;
Slater determinant In quantum mechanics, a Slater determinant is an expression that describes the wave function of a multi-fermionic system. It satisfies anti-symmetry requirements, and consequently the Pauli principle, by changing sign upon exchange of two elect ...


Nonlocality

; Entanglement ; Bell's inequality ;
Entangled state Quantum entanglement is the phenomenon that occurs when a group of particles are generated, interact, or share spatial proximity in a way such that the quantum state of each particle of the group cannot be described independently of the state of ...
;
separable state In quantum mechanics, separable states are quantum states belonging to a composite space that can be factored into individual states belonging to separate subspaces. A state is said to be entangled if it is not separable. In general, determinin ...
;
no-cloning theorem In physics, the no-cloning theorem states that it is impossible to create an independent and identical copy of an arbitrary unknown quantum state, a statement which has profound implications in the field of quantum computing among others. The theore ...


Rotation: spin/angular momentum

; Spin ;
angular momentum In physics, angular momentum (rarely, moment of momentum or rotational momentum) is the rotational analog of linear momentum. It is an important physical quantity because it is a conserved quantity—the total angular momentum of a closed syst ...
;
Clebsch–Gordan coefficients In physics, the Clebsch–Gordan (CG) coefficients are numbers that arise in angular momentum coupling in quantum mechanics. They appear as the expansion coefficients of total angular momentum eigenstates in an uncoupled tensor product basis. In ...
;
singlet state In quantum mechanics, a singlet state usually refers to a system in which all electrons are paired. The term 'singlet' originally meant a linked set of particles whose net angular momentum is zero, that is, whose overall spin quantum number s=0. A ...
and
triplet state In quantum mechanics, a triplet is a quantum state of a system with a spin of quantum number =1, such that there are three allowed values of the spin component, = −1, 0, and +1. Spin, in the context of quantum mechanics, is not a mechanical r ...


Approximation methods

;
adiabatic approximation In thermodynamics, an adiabatic process (Greek: ''adiábatos'', "impassable") is a type of thermodynamic process that occurs without transferring heat or mass between the thermodynamic system and its environment. Unlike an isothermal process, ...
;
Born–Oppenheimer approximation In quantum chemistry and molecular physics, the Born–Oppenheimer (BO) approximation is the best-known mathematical approximation in molecular dynamics. Specifically, it is the assumption that the wave functions of atomic nuclei and elect ...
;
WKB approximation In mathematical physics, the WKB approximation or WKB method is a method for finding approximate solutions to linear differential equations with spatially varying coefficients. It is typically used for a semiclassical calculation in quantum mecha ...
;
time-dependent perturbation theory In quantum mechanics, perturbation theory is a set of approximation schemes directly related to mathematical perturbation for describing a complicated quantum system in terms of a simpler one. The idea is to start with a simple system for wh ...
;
time-independent perturbation theory In quantum mechanics, perturbation theory is a set of approximation schemes directly related to mathematical perturbation for describing a complicated quantum system in terms of a simpler one. The idea is to start with a simple system for wh ...


Historical Terms / semi-classical treatment

;
Ehrenfest theorem The Ehrenfest theorem, named after Paul Ehrenfest, an Austrian theoretical physicist at Leiden University, relates the time derivative of the expectation values of the position and momentum operators ''x'' and ''p'' to the expectation value of th ...
: A theorem connecting the classical mechanics and result derived from Schrödinger equation. ;
first quantization A first quantization of a physical system is a possibly semiclassical treatment of quantum mechanics, in which particles or physical objects are treated using quantum wave functions but the surrounding environment (for example a potential well o ...
: x \to \hat x , \, p \to i \hbar \frac ;
wave–particle duality Wave–particle duality is the concept in quantum mechanics that every particle or quantum entity may be described as either a particle or a wave. It expresses the inability of the classical concepts "particle" or "wave" to fully describe the b ...


Uncategorized terms

;
uncertainty principle In quantum mechanics, the uncertainty principle (also known as Heisenberg's uncertainty principle) is any of a variety of mathematical inequalities asserting a fundamental limit to the accuracy with which the values for certain pairs of physic ...
;
Canonical commutation relations In quantum mechanics, the canonical commutation relation is the fundamental relation between canonical conjugate quantities (quantities which are related by definition such that one is the Fourier transform of another). For example, hat x,\hat ...
: The canonical commutation relations are the commutators between canonically conjugate variables. For example, position \hat x and momentum \hat p : hat x, \hat p= \hat x \hat p - \hat p \hat x = i \hbar ; Path integral ;
wavenumber In the physical sciences, the wavenumber (also wave number or repetency) is the '' spatial frequency'' of a wave, measured in cycles per unit distance (ordinary wavenumber) or radians per unit distance (angular wavenumber). It is analogous to te ...


See also

* Mathematical formulations of quantum mechanics * List of mathematical topics in quantum theory * List of quantum-mechanical potentials *
Introduction to quantum mechanics Quantum mechanics is the study of matter and its interactions with energy on the scale of atomic and subatomic particles. By contrast, classical physics explains matter and energy only on a scale familiar to human experience, including the be ...


Notes


References

* Elementary textbooks ** ** ** ** * Graduate textook ** * Other ** ** {{DEFAULTSORT:Glossary Of Elementary Quantum Mechanics Quantum Mechanics, Glossary Of Elementary Quantum mechanics Wikipedia glossaries using description lists