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The **mathematical formulations of quantum mechanics** are those mathematical formalisms that permit a rigorous description of quantum mechanics. This mathematical formalism uses mainly a part of functional analysis, especially Hilbert spaces, which are a kind of linear space. Such are distinguished from mathematical formalisms for physics theories developed prior to the early 1900s by the use of abstract mathematical structures, such as infinite-dimensional Hilbert spaces (L^{2} space mainly), and operators on these spaces. In brief, values of physical observables such as energy and momentum were no longer considered as values of functions on phase space, but as eigenvalues; more precisely as spectral values of linear operators in Hilbert space.^{ [1] }

- History of the formalism
- The "old quantum theory" and the need for new mathematics
- The "new quantum theory"
- Later developments
- Mathematical structure of quantum mechanics
- Postulates of quantum mechanics
- Pictures of dynamics
- Representations
- Time as an operator
- Spin
- Pauli's principle
- The problem of measurement
- The relative state interpretation
- List of mathematical tools
- Notes
- References

These formulations of quantum mechanics continue to be used today. At the heart of the description are ideas of * quantum state * and *quantum observables*, which are radically different from those used in previous models of physical reality. While the mathematics permits calculation of many quantities that can be measured experimentally, there is a definite theoretical limit to values that can be simultaneously measured. This limitation was first elucidated by Heisenberg through a thought experiment, and is represented mathematically in the new formalism by the non-commutativity of operators representing quantum observables.

Prior to the development of quantum mechanics as a separate theory, the mathematics used in physics consisted mainly of formal mathematical analysis, beginning with calculus, and increasing in complexity up to differential geometry and partial differential equations. Probability theory was used in statistical mechanics. Geometric intuition played a strong role in the first two and, accordingly, theories of relativity were formulated entirely in terms of differential geometric concepts. The phenomenology of quantum physics arose roughly between 1895 and 1915, and for the 10 to 15 years before the development of quantum mechanics (around 1925) physicists continued to think of quantum theory within the confines of what is now called classical physics, and in particular within the same mathematical structures. The most sophisticated example of this is the Sommerfeld–Wilson–Ishiwara quantization rule, which was formulated entirely on the classical phase space.

In the 1890s, Planck was able to derive the blackbody spectrum, which was later used to avoid the classical ultraviolet catastrophe by making the unorthodox assumption that, in the interaction of electromagnetic radiation with matter, energy could only be exchanged in discrete units which he called quanta. Planck postulated a direct proportionality between the frequency of radiation and the quantum of energy at that frequency. The proportionality constant, *h*, is now called Planck's constant in his honor.

In 1905, Einstein explained certain features of the photoelectric effect by assuming that Planck's energy quanta were actual particles, which were later dubbed photons.

All of these developments were phenomenological and challenged the theoretical physics of the time. Bohr and Sommerfeld went on to modify classical mechanics in an attempt to deduce the Bohr model from first principles. They proposed that, of all closed classical orbits traced by a mechanical system in its phase space, only the ones that enclosed an area which was a multiple of Planck's constant were actually allowed. The most sophisticated version of this formalism was the so-called Sommerfeld–Wilson–Ishiwara quantization. Although the Bohr model of the hydrogen atom could be explained in this way, the spectrum of the helium atom (classically an unsolvable 3-body problem) could not be predicted. The mathematical status of quantum theory remained uncertain for some time.

In 1923, de Broglie proposed that wave–particle duality applied not only to photons but to electrons and every other physical system.

The situation changed rapidly in the years 1925–1930, when working mathematical foundations were found through the groundbreaking work of Erwin Schrödinger, Werner Heisenberg, Max Born, Pascual Jordan, and the foundational work of John von Neumann, Hermann Weyl and Paul Dirac, and it became possible to unify several different approaches in terms of a fresh set of ideas. The physical interpretation of the theory was also clarified in these years after Werner Heisenberg discovered the uncertainty relations and Niels Bohr introduced the idea of complementarity.

Werner Heisenberg's matrix mechanics was the first successful attempt at replicating the observed quantization of atomic spectra. Later in the same year, Schrödinger created his wave mechanics. Schrödinger's formalism was considered easier to understand, visualize and calculate as it led to differential equations, which physicists were already familiar with solving. Within a year, it was shown that the two theories were equivalent.

Schrödinger himself initially did not understand the fundamental probabilistic nature of quantum mechanics, as he thought that the absolute square of the wave function of an electron should be interpreted as the charge density of an object smeared out over an extended, possibly infinite, volume of space. It was Max Born who introduced the interpretation of the absolute square of the wave function as the probability distribution of the position of a *pointlike* object. Born's idea was soon taken over by Niels Bohr in Copenhagen who then became the "father" of the Copenhagen interpretation of quantum mechanics. Schrödinger's wave function can be seen to be closely related to the classical Hamilton–Jacobi equation. The correspondence to classical mechanics was even more explicit, although somewhat more formal, in Heisenberg's matrix mechanics. In his PhD thesis project, Paul Dirac ^{ [2] } discovered that the equation for the operators in the Heisenberg representation, as it is now called, closely translates to classical equations for the dynamics of certain quantities in the Hamiltonian formalism of classical mechanics, when one expresses them through Poisson brackets, a procedure now known as canonical quantization.

To be more precise, already before Schrödinger, the young postdoctoral fellow Werner Heisenberg invented his matrix mechanics, which was the first correct quantum mechanics–– the essential breakthrough. Heisenberg's matrix mechanics formulation was based on algebras of infinite matrices, a very radical formulation in light of the mathematics of classical physics, although he started from the index-terminology of the experimentalists of that time, not even aware that his "index-schemes" were matrices, as Born soon pointed out to him. In fact, in these early years, linear algebra was not generally popular with physicists in its present form.

Although Schrödinger himself after a year proved the equivalence of his wave-mechanics and Heisenberg's matrix mechanics, the reconciliation of the two approaches and their modern abstraction as motions in Hilbert space is generally attributed to Paul Dirac, who wrote a lucid account in his 1930 classic * The Principles of Quantum Mechanics *. He is the third, and possibly most important, pillar of that field (he soon was the only one to have discovered a relativistic generalization of the theory). In his above-mentioned account, he introduced the bra–ket notation, together with an abstract formulation in terms of the Hilbert space used in functional analysis; he showed that Schrödinger's and Heisenberg's approaches were two different representations of the same theory, and found a third, most general one, which represented the dynamics of the system. His work was particularly fruitful in all kinds of generalizations of the field.

The first complete mathematical formulation of this approach, known as the Dirac–von Neumann axioms, is generally credited to John von Neumann's 1932 book * Mathematical Foundations of Quantum Mechanics *, although Hermann Weyl had already referred to Hilbert spaces (which he called *unitary spaces*) in his 1927 classic paper and book. It was developed in parallel with a new approach to the mathematical spectral theory based on linear operators rather than the quadratic forms that were David Hilbert's approach a generation earlier. Though theories of quantum mechanics continue to evolve to this day, there is a basic framework for the mathematical formulation of quantum mechanics which underlies most approaches and can be traced back to the mathematical work of John von Neumann. In other words, discussions about *interpretation* of the theory, and extensions to it, are now mostly conducted on the basis of shared assumptions about the mathematical foundations.

The application of the new quantum theory to electromagnetism resulted in quantum field theory, which was developed starting around 1930. Quantum field theory has driven the development of more sophisticated formulations of quantum mechanics, of which the ones presented here are simple special cases.

- Path integral formulation
- Phase-space formulation of quantum mechanics & geometric quantization
- quantum field theory in curved spacetime
- axiomatic, algebraic and constructive quantum field theory
- C*-algebra formalism
- Generalized statistical model of quantum mechanics

A related topic is the relationship to classical mechanics. Any new physical theory is supposed to reduce to successful old theories in some approximation. For quantum mechanics, this translates into the need to study the so-called classical limit of quantum mechanics. Also, as Bohr emphasized, human cognitive abilities and language are inextricably linked to the classical realm, and so classical descriptions are intuitively more accessible than quantum ones. In particular, quantization, namely the construction of a quantum theory whose classical limit is a given and known classical theory, becomes an important area of quantum physics in itself.

Finally, some of the originators of quantum theory (notably Einstein and Schrödinger) were unhappy with what they thought were the philosophical implications of quantum mechanics. In particular, Einstein took the position that quantum mechanics must be incomplete, which motivated research into so-called hidden-variable theories. The issue of hidden variables has become in part an experimental issue with the help of quantum optics.

A physical system is generally described by three basic ingredients: states; observables; and dynamics (or law of time evolution) or, more generally, a group of physical symmetries. A classical description can be given in a fairly direct way by a phase space model of mechanics: states are points in a symplectic phase space, observables are real-valued functions on it, time evolution is given by a one-parameter group of symplectic transformations of the phase space, and physical symmetries are realized by symplectic transformations. A quantum description normally consists of a Hilbert space of states, observables are self-adjoint operators on the space of states, time evolution is given by a one-parameter group of unitary transformations on the Hilbert space of states, and physical symmetries are realized by unitary transformations. (It is possible, to map this Hilbert-space picture to a phase space formulation, invertibly. See below.)

The following summary of the mathematical framework of quantum mechanics can be partly traced back to the Dirac–von Neumann axioms. The postulates are canonically presented in six statements, though there are many important points to each. ^{ [3] }

Each physical system is associated with a (topologically) separable complex Hilbert space *H* with inner product ⟨*φ*|*ψ*⟩. Rays (that is, subspaces of *complex* dimension 1) in *H* are associated with quantum states of the system.

Postulate I

The state of an isolated physical system is represented, at a fixed time , by a state vector belonging to a Hilbert space called the *state space*.

In other words, quantum states can be identified with equivalence classes of vectors of length 1 in *H*, where two vectors represent the same state if they differ only by a phase factor. *Separability* is a mathematically convenient hypothesis, with the physical interpretation that countably many observations are enough to uniquely determine the state. "A quantum mechanical state is a *ray* in projective Hilbert space, not a *vector*. Many textbooks fail to make this distinction, which could be partly a result of the fact that the Schrödinger equation itself involves Hilbert-space "vectors", with the result that the imprecise use of "state vector" rather than *ray* is very difficult to avoid."^{ [4] }

The Hilbert space of a composite system is the Hilbert space tensor product of the state spaces associated with the component systems (for instance, J. M. Jauch, *Foundations of quantum mechanics*, section 11.7). For a non-relativistic system consisting of a finite number of distinguishable particles, the component systems are the individual particles.

Physical observables are represented by Hermitian matrices on *H*. Since these operators are Hermitian, the measurement is always a real value. If the spectrum of the observable is discrete, then the possible results are *quantized*.

Postulate II

Every measurable physical quantity is described by a Hermitian operator acting in the state space . This operator is an observable, meaning that its eigenvectors form a basis for .

By spectral theory, we can associate a probability measure to the values of *A* in any state *ψ*. We can also show that the possible values of the observable *A* in any state must belong to the spectrum of *A*. The expectation value (in the sense of probability theory) of the observable *A* for the system in state represented by the unit vector *ψ* ∈ *H* is .

Postulate III

The result of measuring a physical quantity must be one of the eigenvalues of the corresponding observable .

In the special case *A* has only discrete spectrum, the possible outcomes of measuring *A* are its eigenvalues. More precisely, if we represent the state *ψ* in the basis formed by the eigenvectors of *A*, then the square of the modulus of the component attached to a given eigenvector is the probability of observing its corresponding eigenvalue.

Postulate IV

When the physical quantity is measured on a system in a normalized state , the probability of obtaining an eigenvalue (denoted for discrete spectra and for continuous spectra) of the corresponding observable is given by *amplitude squared* of the appropriate wave function (projection onto corresponding eigenvector).

More generally, a state can be represented by a so-called density operator, which is a trace class, nonnegative self-adjoint operator *ρ* normalized to be of trace 1. The expected value of *A* in the state *ρ* is .

When a measurement is performed, only one result is obtained (according to some interpretations of quantum mechanics). This is modeled mathematically as the processing of additional information from the measurement, confining the probabilities of an immediate second measurement of the same observable. In the case of a discrete, non-degenerate spectrum, two sequential measurements of the same observable will always give the same value assuming the second immediately follows the first. Therefore the state vector must change as a result of measurement, and *collapse* onto the eigensubspace associated with the eigenvalue measured.

Postulate V

If the measurement of the physical quantity on the system in the state gives the result , then the state of the system immediately after the measurement is the normalized projection of onto the eigensubspace associated with

If *ρ _{ψ}* is the orthogonal projector onto the one-dimensional subspace of

Though it is possible to derive the Schrödinger equation, which describes how a state vector evolves in time, most texts assert the equation as a postulate. Common derivations include using the DeBroglie hypothesis or path integrals.

Postulate VI

The time evolution of the state vector is governed by the Schrödinger equation, where is the observable associated with the total energy of the system (called the Hamiltonian)

- Physical symmetries act on the Hilbert space of quantum states unitarily or antiunitarily due to Wigner's theorem (supersymmetry is another matter entirely).

- Physical observables are represented by Hermitian matrices on
*H*.

- Density operators are those that are in the closure of the convex hull of the one-dimensional orthogonal projectors. Conversely, one-dimensional orthogonal projectors are extreme points of the set of density operators. Physicists also call one-dimensional orthogonal projectors
*pure states*and other density operators*mixed states*.

One can in this formalism state Heisenberg's uncertainty principle and prove it as a theorem, although the exact historical sequence of events, concerning who derived what and under which framework, is the subject of historical investigations outside the scope of this article.

Furthermore, to the postulates of quantum mechanics one should also add basic statements on the properties of spin and Pauli's exclusion principle, see below.

- In the so-called Schrödinger picture of quantum mechanics, the dynamics is given as follows:

The time evolution of the state is given by a differentiable function from the real numbers **R**, representing instants of time, to the Hilbert space of system states. This map is characterized by a differential equation as follows: If |*ψ*(*t*)⟩ denotes the state of the system at any one time *t*, the following Schrödinger equation holds:

where *H* is a densely defined self-adjoint operator, called the system Hamiltonian, *i* is the imaginary unit and *ħ* is the reduced Planck constant. As an observable, *H* corresponds to the total energy of the system.

Alternatively, by Stone's theorem one can state that there is a strongly continuous one-parameter unitary map *U*(*t*): *H* → *H* such that

for all times *s*, *t*. The existence of a self-adjoint Hamiltonian *H* such that

is a consequence of Stone's theorem on one-parameter unitary groups. It is assumed that *H* does not depend on time and that the perturbation starts at *t*_{0} = 0; otherwise one must use the Dyson series, formally written as

where is Dyson's time-ordering symbol.

(This symbol permutes a product of noncommuting operators of the form

into the uniquely determined re-ordered expression

- with

The result is a causal chain, the primary *cause* in the past on the utmost r.h.s., and finally the present *effect* on the utmost l.h.s. .)

- The Heisenberg picture of quantum mechanics focuses on observables and instead of considering states as varying in time, it regards the states as fixed and the observables as changing. To go from the Schrödinger to the Heisenberg picture one needs to define time-independent states and time-dependent operators thus:

It is then easily checked that the expected values of all observables are the same in both pictures

and that the time-dependent Heisenberg operators satisfy

which is true for time-dependent *A* = *A*(*t*). Notice the commutator expression is purely formal when one of the operators is unbounded. One would specify a representation for the expression to make sense of it.

- The so-called Dirac picture or interaction picture has time-dependent
*states*and observables, evolving with respect to different Hamiltonians. This picture is most useful when the evolution of the observables can be solved exactly, confining any complications to the evolution of the states. For this reason, the Hamiltonian for the observables is called "free Hamiltonian" and the Hamiltonian for the states is called "interaction Hamiltonian". In symbols:

The interaction picture does not always exist, though. In interacting quantum field theories, Haag's theorem states that the interaction picture does not exist. This is because the Hamiltonian cannot be split into a free and an interacting part within a superselection sector. Moreover, even if in the Schrödinger picture the Hamiltonian does not depend on time, e.g. *H* = *H*_{0} + *V*, in the interaction picture it does, at least, if *V* does not commute with *H*_{0}, since

- .

So the above-mentioned Dyson-series has to be used anyhow.

The Heisenberg picture is the closest to classical Hamiltonian mechanics (for example, the commutators appearing in the above equations directly translate into the classical Poisson brackets); but this is already rather "high-browed", and the Schrödinger picture is considered easiest to visualize and understand by most people, to judge from pedagogical accounts of quantum mechanics. The Dirac picture is the one used in perturbation theory, and is specially associated to quantum field theory and many-body physics.

Similar equations can be written for any one-parameter unitary group of symmetries of the physical system. Time would be replaced by a suitable coordinate parameterizing the unitary group (for instance, a rotation angle, or a translation distance) and the Hamiltonian would be replaced by the conserved quantity associated with the symmetry (for instance, angular or linear momentum).

**Summary**:

Evolution | Picture ( ) | ||

of: | Heisenberg | Interaction | Schrödinger |

Ket state | constant | ||

Observable | constant | ||

Density matrix | constant |

The original form of the Schrödinger equation depends on choosing a particular representation of Heisenberg's canonical commutation relations. The Stone–von Neumann theorem dictates that all irreducible representations of the finite-dimensional Heisenberg commutation relations are unitarily equivalent. A systematic understanding of its consequences has led to the phase space formulation of quantum mechanics, which works in full phase space instead of Hilbert space, so then with a more intuitive link to the classical limit thereof. This picture also simplifies considerations of quantization, the deformation extension from classical to quantum mechanics.

The quantum harmonic oscillator is an exactly solvable system where the different representations are easily compared. There, apart from the Heisenberg, or Schrödinger (position or momentum), or phase-space representations, one also encounters the Fock (number) representation and the Segal–Bargmann (Fock-space or coherent state) representation (named after Irving Segal and Valentine Bargmann). All four are unitarily equivalent.

The framework presented so far singles out time as *the* parameter that everything depends on. It is possible to formulate mechanics in such a way that time becomes itself an observable associated with a self-adjoint operator. At the classical level, it is possible to arbitrarily parameterize the trajectories of particles in terms of an unphysical parameter *s*, and in that case the time *t* becomes an additional generalized coordinate of the physical system. At the quantum level, translations in *s* would be generated by a "Hamiltonian" *H* − *E*, where *E* is the energy operator and *H* is the "ordinary" Hamiltonian. However, since *s* is an unphysical parameter, *physical* states must be left invariant by "*s*-evolution", and so the physical state space is the kernel of *H* − *E* (this requires the use of a rigged Hilbert space and a renormalization of the norm).

This is related to the quantization of constrained systems and quantization of gauge theories. It is also possible to formulate a quantum theory of "events" where time becomes an observable (see D. Edwards).

In addition to their other properties, all particles possess a quantity called spin, an *intrinsic angular momentum*. Despite the name, particles do not literally spin around an axis, and quantum mechanical spin has no correspondence in classical physics. In the position representation, a spinless wavefunction has position **r** and time *t* as continuous variables, *ψ* = *ψ*(**r**, *t*). For spin wavefunctions the spin is an additional discrete variable: *ψ* = *ψ*(**r**, *t*, *σ*), where *σ* takes the values;

That is, the state of a single particle with spin *S* is represented by a (2*S* + 1)-component spinor of complex-valued wave functions.

Two classes of particles with *very different* behaviour are bosons which have integer spin (*S* = 0, 1, 2...), and fermions possessing half-integer spin (*S* = 1⁄2, 3⁄2, 5⁄2, ...).

The property of spin relates to another basic property concerning systems of *N* identical particles: Pauli's exclusion principle, which is a consequence of the following permutation behaviour of an *N*-particle wave function; again in the position representation one must postulate that for the transposition of any two of the *N* particles one always should have

i.e., on transposition of the arguments of any two particles the wavefunction should *reproduce*, apart from a prefactor (−1)^{2S} which is +1 for bosons, but (−1) for fermions. Electrons are fermions with *S* = 1/2; quanta of light are bosons with *S* = 1. In nonrelativistic quantum mechanics all particles are either bosons or fermions; in relativistic quantum theories also "supersymmetric" theories exist, where a particle is a linear combination of a bosonic and a fermionic part. Only in dimension *d* = 2 can one construct entities where (−1)^{2S} is replaced by an arbitrary complex number with magnitude 1, called anyons.

Although *spin* and the *Pauli principle* can only be derived from relativistic generalizations of quantum mechanics the properties mentioned in the last two paragraphs belong to the basic postulates already in the non-relativistic limit. Especially, many important properties in natural science, e.g. the periodic system of chemistry, are consequences of the two properties.

The picture given in the preceding paragraphs is sufficient for description of a completely isolated system. However, it fails to account for one of the main differences between quantum mechanics and classical mechanics, that is, the effects of measurement.^{ [5] } The von Neumann description of quantum measurement of an observable *A*, when the system is prepared in a pure state *ψ* is the following (note, however, that von Neumann's description dates back to the 1930s and is based on experiments as performed during that time – more specifically the Compton–Simon experiment; it is not applicable to most present-day measurements within the quantum domain):

- Let
*A*have spectral resolution

where E_{A} is the resolution of the identity (also called projection-valued measure) associated with *A*. Then the probability of the measurement outcome lying in an interval *B* of **R** is |E_{A}(*B*) *ψ*|^{2}. In other words, the probability is obtained by integrating the characteristic function of *B* against the countably additive measure

- If the measured value is contained in
*B*, then immediately after the measurement, the system will be in the (generally non-normalized) state E_{A}(*B*)*ψ*. If the measured value does not lie in*B*, replace*B*by its complement for the above state.

For example, suppose the state space is the *n*-dimensional complex Hilbert space **C**^{n} and *A* is a Hermitian matrix with eigenvalues *λ*_{i}, with corresponding eigenvectors *ψ _{i}*. The projection-valued measure associated with

where *B* is a Borel set containing only the single eigenvalue *λ _{i}*. If the system is prepared in state

Then the probability of a measurement returning the value *λ _{i}* can be calculated by integrating the spectral measure

over *B _{i}*. This gives trivially

The characteristic property of the von Neumann measurement scheme is that repeating the same measurement will give the same results. This is also called the *projection postulate*.

A more general formulation replaces the projection-valued measure with a positive-operator valued measure (POVM). To illustrate, take again the finite-dimensional case. Here we would replace the rank-1 projections

by a finite set of positive operators

whose sum is still the identity operator as before (the resolution of identity). Just as a set of possible outcomes {*λ*_{1} ... *λ _{n}*} is associated to a projection-valued measure, the same can be said for a POVM. Suppose the measurement outcome is

after the measurement, the system now will be in the state

Since the *F _{i} F_{i}** operators need not be mutually orthogonal projections, the projection postulate of von Neumann no longer holds.

The same formulation applies to general mixed states.

In von Neumann's approach, the state transformation due to measurement is distinct from that due to time evolution in several ways. For example, time evolution is deterministic and unitary whereas measurement is non-deterministic and non-unitary. However, since both types of state transformation take one quantum state to another, this difference was viewed by many as unsatisfactory. The POVM formalism views measurement as one among many other quantum operations, which are described by completely positive maps which do not increase the trace.

In any case it seems that the above-mentioned problems can only be resolved if the time evolution included not only the quantum system, but also, and essentially, the classical measurement apparatus (see above).

An alternative interpretation of measurement is Everett's relative state interpretation, which was later dubbed the "many-worlds interpretation" of quantum physics.

Part of the folklore of the subject concerns the mathematical physics textbook Methods of Mathematical Physics put together by Richard Courant from David Hilbert's Göttingen University courses. The story is told (by mathematicians) that physicists had dismissed the material as not interesting in the current research areas, until the advent of Schrödinger's equation. At that point it was realised that the mathematics of the new quantum mechanics was already laid out in it. It is also said that Heisenberg had consulted Hilbert about his matrix mechanics, and Hilbert observed that his own experience with infinite-dimensional matrices had derived from differential equations, advice which Heisenberg ignored, missing the opportunity to unify the theory as Weyl and Dirac did a few years later. Whatever the basis of the anecdotes, the mathematics of the theory was conventional at the time, whereas the physics was radically new.

The main tools include:

- linear algebra: complex numbers, eigenvectors, eigenvalues
- functional analysis: Hilbert spaces, linear operators, spectral theory
- differential equations: partial differential equations, separation of variables, ordinary differential equations, Sturm–Liouville theory, eigenfunctions
- harmonic analysis: Fourier transforms

- ↑ Frederick W. Byron, Robert W. Fuller; Mathematics of classical and quantum physics; Courier Dover Publications, 1992.
- ↑ Dirac, P. A. M. (1925). "The Fundamental Equations of Quantum Mechanics".
*Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences*.**109**(752): 642–653. Bibcode:1925RSPSA.109..642D. doi: 10.1098/rspa.1925.0150 . - ↑ Cohen-Tannoudji, Claude (2019).
*Quantum mechanics. Volume 2*. Bernard Diu, Franck Laloë, Susan Reid Hemley, Nicole Ostrowsky, D. B. Ostrowsky. Weinheim. ISBN 978-3-527-82272-0. OCLC 1159410161. - ↑ Solem, J. C.; Biedenharn, L. C. (1993). "Understanding geometrical phases in quantum mechanics: An elementary example".
*Foundations of Physics*.**23**(2): 185–195. Bibcode:1993FoPh...23..185S. doi:10.1007/BF01883623. - ↑ G. Greenstein and A. Zajonc

**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 chemistry, quantum field theory, quantum technology, and quantum information science.

In quantum mechanics, the **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 physical quantities of a particle, such as position, *x*, and momentum, *p*, can be predicted from initial conditions.

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 the subject. The equation is named after Erwin Schrödinger, who postulated the equation in 1925, and published it in 1926, forming the basis for the work that resulted in his Nobel Prize in Physics in 1933.

In quantum mechanics, a **density matrix** 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 the Born rule. It is a generalization of the more usual state vectors or wavefunctions: while those can only represent pure states, density matrices can also represent *mixed states*. Mixed states arise in quantum mechanics in two different situations: first when the preparation of the system is not fully known, and thus one must deal with a statistical ensemble of possible preparations, and second when one wants to describe a physical system which is entangled with another, as its state can not be described by a pure state.

In quantum mechanics, **wave function collapse** occurs when a wave function—initially in a superposition of several eigenstates—reduces to a single eigenstate due to interaction with the external world. This interaction is called an "observation". It is the essence of a measurement in quantum mechanics which connects the wave function with classical observables like position and momentum. Collapse is one of two processes by which quantum systems evolve in time; the other is the continuous evolution via the Schrödinger equation. Collapse is a black box for a thermodynamically irreversible interaction with a classical environment. Calculations of quantum decoherence show that when a quantum system interacts with the environment, the superpositions *apparently* reduce to mixtures of classical alternatives. Significantly, the combined wave function of the system and environment continue to obey the Schrödinger equation. More importantly, this is not enough to explain wave function collapse, as decoherence does not reduce it to a single eigenstate.

A **wave function** in quantum physics is a mathematical description of the quantum state of an isolated quantum system. The wave function is a complex-valued probability amplitude, and the probabilities for the possible results of measurements made on the system can be derived from it. The most common symbols for a wave function are the Greek letters *ψ* and Ψ.

In physics, the **Heisenberg picture** is a formulation of quantum mechanics in which the operators incorporate a dependency on time, but the state vectors are time-independent, an arbitrary fixed basis rigidly underlying the theory.

In physics, the **Schrödinger picture** is a formulation of quantum mechanics in which the state vectors evolve in time, but the operators are constant with respect to time. This differs from the Heisenberg picture which keeps the states constant while the observables evolve in time, and from the interaction picture in which both the states and the observables evolve in time. The Schrödinger and Heisenberg pictures are related as active and passive transformations and commutation relations between operators are preserved in the passage between the two pictures.

In quantum mechanics, the **canonical commutation relation** is the fundamental relation between canonical conjugate quantities. For example,

In physics, **canonical quantization** is a procedure for quantizing a classical theory, while attempting to preserve the formal structure, such as symmetries, of the classical theory, to the greatest extent possible.

In quantum mechanics, the **interaction picture** is an intermediate representation between the Schrödinger picture and the Heisenberg picture. Whereas in the other two pictures either the state vector or the operators carry time dependence, in the interaction picture both carry part of the time dependence of observables. The interaction picture is useful in dealing with changes to the wave functions and observables due to interactions. Most field-theoretical calculations use the interaction representation because they construct the solution to the many-body Schrödinger equation as the solution to the free-particle problem plus some unknown interaction parts.

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 the force on a massive particle moving in a scalar potential ,

The **Born rule** is a key postulate of quantum mechanics which gives the probability that a measurement of a quantum system will yield a given result. In its simplest form, it states that the probability density of finding a particle at a given point, when measured, is proportional to the square of the magnitude of the particle's wavefunction at that point. It was formulated by German physicist Max Born in 1926.

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 is treated classically.

In quantum physics, **unitarity** is the condition that the time evolution of a quantum state according to the Schrödinger equation is mathematically represented by a unitary operator. This is typically taken as an axiom or basic postulate of quantum mechanics, while generalizations of or departures from unitarity are part of speculations about theories that may go beyond quantum mechanics. A **unitarity bound** is any inequality that follows from the unitarity of the evolution operator, i.e. from the statement that time evolution preserves inner products in Hilbert space.

In quantum mechanics, the **expectation value** is the probabilistic expected value of the result (measurement) of an experiment. It can be thought of as an average of all the possible outcomes of a measurement as weighted by their likelihood, and as such it is not the *most* probable value of a measurement; indeed the expectation value may have zero probability of occurring. It is a fundamental concept in all areas of quantum physics.

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 time exhausts all that can be predicted about the system's behavior. A mixture of quantum states is again a quantum state. Quantum states that cannot be written as a mixture of other states are called **pure quantum states**, while all other states are called **mixed quantum states**. A pure quantum state can be represented by a ray in a Hilbert space over the complex numbers, while mixed states are represented by density matrices, which are positive semidefinite operators that act on Hilbert spaces.

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

The **Koopman–von Neumann mechanics** is a description of classical mechanics in terms of Hilbert space, introduced by Bernard Koopman and John von Neumann in 1931 and 1932, respectively.

In quantum mechanics, **dynamical pictures** are the multiple equivalent ways to mathematically formulate the dynamics of a quantum system.

- J. von Neumann,
*Mathematical Foundations of Quantum Mechanics*(1932), Princeton University Press, 1955. Reprinted in paperback form. - H. Weyl,
*The Theory of Groups and Quantum Mechanics*, Dover Publications, 1950. - A. Gleason,
*Measures on the Closed Subspaces of a Hilbert Space*, Journal of Mathematics and Mechanics, 1957. - G. Mackey,
*Mathematical Foundations of Quantum Mechanics*, W. A. Benjamin, 1963 (paperback reprint by Dover 2004). - R. F. Streater and A. S. Wightman,
*PCT, Spin and Statistics and All That*, Benjamin 1964 (Reprinted by Princeton University Press) - R. Jost,
*The General Theory of Quantized Fields*, American Mathematical Society, 1965. - J. M. Jauch,
*Foundations of quantum mechanics*, Addison-Wesley Publ. Cy., Reading, Massachusetts, 1968. - G. Emch,
*Algebraic Methods in Statistical Mechanics and Quantum Field Theory*, Wiley-Interscience, 1972. - M. Reed and B. Simon,
*Methods of Mathematical Physics*, vols I–IV, Academic Press 1972. - T.S. Kuhn,
*Black-Body Theory and the Quantum Discontinuity, 1894–1912*, Clarendon Press, Oxford and Oxford University Press, New York, 1978. - D. Edwards,
*The Mathematical Foundations of Quantum Mechanics*, Synthese, 42 (1979),pp. 1–70. - R. Shankar, "Principles of Quantum Mechanics", Springer, 1980.
- E. Prugovecki,
*Quantum Mechanics in Hilbert Space*, Dover, 1981. - S. Auyang,
*How is Quantum Field Theory Possible?*, Oxford University Press, 1995. - N. Weaver, "Mathematical Quantization", Chapman & Hall/CRC 2001.
- G. Giachetta, L. Mangiarotti, G. Sardanashvily, "Geometric and Algebraic Topological Methods in Quantum Mechanics", World Scientific, 2005.
- David McMahon, "Quantum Mechanics Demystified", 2nd Ed., McGraw-Hill Professional, 2005.
- G. Teschl,
*Mathematical Methods in Quantum Mechanics with Applications to Schrödinger Operators*, https://www.mat.univie.ac.at/~gerald/ftp/book-schroe/, American Mathematical Society, 2009. - V. Moretti, "Spectral Theory and Quantum Mechanics: Mathematical Foundations of Quantum Theories, Symmetries and Introduction to the Algebraic Formulation", 2nd Edition, Springer, 2018.
- B. C. Hall, "Quantum Theory for Mathematicians", Springer, 2013.
- V. Moretti, "Fundamental Mathematical Structures of Quantum Theory". Springer, 2019, https://www.springer.com/it/book/9783030183455#aboutBook
- K. Landsman, "Foundations of Quantum Theory", Springer 2017

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