Position operator
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In
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 chemistry, ...
, the position operator is the operator that corresponds to the position observable of a
particle In the physical sciences, a particle (or corpuscule in older texts) is a small localized object which can be described by several physical or chemical properties, such as volume, density, or mass. They vary greatly in size or quantity, from ...
. When the position operator is considered with a wide enough domain (e.g. the space of
tempered distributions Distributions, also known as Schwartz distributions or generalized functions, are objects that generalize the classical notion of functions in mathematical analysis. Distributions make it possible to differentiate functions whose derivatives d ...
), its
eigenvalue In linear algebra, an eigenvector () or characteristic vector of a linear transformation is a nonzero vector that changes at most by a scalar factor when that linear transformation is applied to it. The corresponding eigenvalue, often denote ...
s are the possible
position vector In geometry, a position or position vector, also known as location vector or radius vector, is a Euclidean vector that represents the position of a point ''P'' in space in relation to an arbitrary reference origin ''O''. Usually denoted x, r, or ...
s of the particle. In one dimension, if by the symbol , x \rangle we denote the unitary eigenvector of the position operator corresponding to the eigenvalue x, then, , x \rangle represents the state of the particle in which we know with certainty to find the particle itself at position x. Therefore, denoting the position operator by the symbol X in the literature we find also other symbols for the position operator, for instance Q (from Lagrangian mechanics), \hat \mathrm x and so on we can write X, x\rangle = x , x\rangle, for every real position x. One possible realization of the unitary state with position x is the Dirac delta (function) distribution centered at the position x, often denoted by \delta_x. In quantum mechanics, the ordered (continuous) family of all Dirac distributions, i.e. the family \delta = (\delta_x)_, is called the (unitary) position basis (in one dimension), just because it is a (unitary) eigenbasis of the position operator X. Note that even though this family is ordered by the continuous coordinate x, the
cardinality In mathematics, the cardinality of a set is a measure of the number of elements of the set. For example, the set A = \ contains 3 elements, and therefore A has a cardinality of 3. Beginning in the late 19th century, this concept was generalized ...
of this basis set is Aleph nought, instead of
Aleph one In mathematics, particularly in set theory, the aleph numbers are a sequence of numbers used to represent the cardinality (or size) of infinite sets that can be well-ordered. They were introduced by the mathematician Georg Cantor and are named a ...
. This is because the Dirac distributions in this family are required to be square-integrable (see the relevant section below), which means that the Hilbert space spanned by this basis has countably infinite many basis states. One way to understand this is to treat the Dirac delta functions as the limit of very tiny lattice segments of the continuous position space, and therefore as the lattice spatial period goes to zero, the number of these lattice sites goes to countable infinity. It is fundamental to observe that there exists only one linear continuous endomorphism X on the space of tempered distributions such that X(\delta_x) = x \delta_x, for every real point x. It's possible to prove that the unique above endomorphism is necessarily defined by X(\psi) = \mathrm x \psi, for every tempered distribution \psi, where \mathrm x denotes the coordinate function of the position line defined from the real line into the complex plane by \mathrm x : \Reals \to \Complex : x \mapsto x .


Introduction

In one dimension for a particle confined into a straight line the square modulus , \psi, ^2 = \psi^* \psi , of a normalized square integrable wave-function \psi : \Reals \to \Complex , represents the probability density of finding the particle at some position x of the real-line, at a certain time. In other terms, if at a certain instant of time the particle is in the state represented by a square integrable wave function \psi and assuming the wave function \psi be of L^2-norm equal 1, \, \psi\, ^2 = \int_^ , \psi, ^2 d \mathrm x = 1, then the probability to find the particle in the position range ,b/math> is \pi_X (\psi)( ,b =\int_a^b , \psi, ^2 d \mathrm x . Hence the
expected 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 ...
of a measurement of the position X for the particle is the value \langle X \rangle_ = \int_\R \mathrm x , \psi, ^2 d \mathrm x = \int_\R \psi^* \mathrm x \psi \, d \mathrm x, where: # the particle is assumed to be in the state \psi ; # the function \mathrm x , \psi, ^2 is supposed integrable, i.e. of class L^1; # we indicate by \mathrm x the coordinate function of the position axis. Additionally, the quantum mechanical operator corresponding to the observable position X is denoted also by X = \hat , and defined \left(\hat \psi\right) (x) = x\psi(x) , for every wave function \psi and for every point x of the real line. The
circumflex The circumflex () is a diacritic in the Latin and Greek scripts that is also used in the written forms of many languages and in various romanization and transcription schemes. It received its English name from la, circumflexus "bent around" ...
over the function \mathrm x on the left side indicates the presence of an operator, so that this equation may be read: ''The result of the position operator X acting on any wave function \psi equals the coordinate function \mathrm x multiplied by the wave-function \psi .'' Or more simply: ''The operator X multiplies any wave-function \psi by the coordinate function \mathrm x .'' Note 1. To be more explicit, we have introduced the coordinate function \mathrm x : \Reals \to \Complex : x \mapsto x , which simply imbeds the position-line into the complex plane. It is nothing more than the ''canonical embedding'' of the real line into the complex plane. Note 2. The expected value of the position operator, upon a wave function (state) \psi can be reinterpreted as a scalar product: \langle X \rangle_ = \int_\R \mathrm x , \psi, ^2 = \int_\R \psi^* (\mathrm x \psi) = \langle \psi , X(\psi) \rangle , assuming the particle in the state \psi \in L^2 and assuming the function \mathrm x \psi be of class L^2 which immediately implies that the function \mathrm x , \psi, ^2 Is integrable, i.e. of class L^1. Note 3. Strictly speaking, the observable position X can be point-wisely defined as \left(\hat \psi\right) (x) = x\psi(x) , for every wave function \psi and for every point x of the real line, upon the wave-functions which are precisely point-wise defined functions. In the case of equivalence classes \psi \in L^2 the definition reads directly as follows \hat \psi = \mathrm x \psi , for every wave-function \psi \in L^2.


Basic properties

In the above definition, as the careful reader can immediately remark, does not exist any clear specification of domain and co-domain for the position operator (in the case of a particle confined upon a line). In literature, more or less explicitly, we find essentially three main directions for this fundamental issue. # The position operator is defined on the subspace D_X of L^2 formed by those equivalence classes \psi whose product by the imbedding \mathrm x lives in the space L^2 as well. In this case the position operator X : D_X \to L^2 : \psi \mapsto \mathrm x \psi reveals not continuous (unbounded with respect to the topology induced by the canonical scalar product of L^2 ), with no eigenvectors, no eigenvalues, consequently with empty eigenspectrum (collection of its eigenvalues). # The position operator is defined on the space \mathcal S_1 of complex valued Schwartz functions (smooth complex functions defined upon the real-line and rapidly decreasing at infinity with all their derivatives). The product of a Schwartz function by the imbedding \mathrm x lives always in the space \mathcal S_1 , which is a subset of L^2 . In this case the position operator X : \mathcal S_1 \to \mathcal S_1 : \psi \mapsto \mathrm x \psi reveals ''continuous'' (with respect to the canonical topology of \mathcal S_1 ), injective, with no eigenvectors, no eigenvalues, consequently with void eigenspectrum (collection of its eigenvalues). It is (fully) self-adjoint with respect to the scalar product of L^2 in the sense that \langle X (\psi), \phi\rangle = \langle \psi, X(\phi)\rangle, for every \psi and \phi belonging to its domain \mathcal S_1 . # This is, in practice, the most widely adopted choice in Quantum Mechanics literature, although never explicitly underlined. The position operator is defined on the space \mathcal S'_1 of complex valued tempered distributions (topological dual of the Schwartz function space \mathcal S_1 ). The product of a temperate distribution by the imbedding \mathrm x lives always in the space \mathcal S'_1 , which contains L^2 . In this case the position operator X : \mathcal S'_1 \to \mathcal S'_1 : \psi \mapsto \mathrm x \psi reveals continuous (with respect to the canonical topology of \mathcal S'_1 ), surjective, endowed with complete families of eigenvectors, real eigenvalues, and with eigenspectrum (collection of its eigenvalues) equal to the real line. It is self-adjoint with respect to the scalar product of L^2 in the sense that its transpose operator ^tX : \mathcal S_1 \to \mathcal S_1 : \phi \mapsto \mathrm x \phi , which is the position operator on the Schwartz function space, is self-adjoint: \left\langle\left. \,^tX (\phi)\\psi \right\rangle = \left\langle \phi, \,^tX(\psi)\right\rangle , for every (test) function \phi and \psi belonging to the space \mathcal S_1 .


Eigenstates

The eigenfunctions of the position operator (on the space of tempered distributions), represented in position space, are
Dirac delta functions In mathematics, the Dirac delta distribution ( distribution), also known as the unit impulse, is a generalized function or distribution over the real numbers, whose value is zero everywhere except at zero, and whose integral over the entire ...
. ''Informal proof.'' To show that possible eigenvectors of the position operator should necessarily be Dirac delta distributions, suppose that \psi is an eigenstate of the position operator with eigenvalue x_0 . We write the eigenvalue equation in position coordinates, \hat\psi(x) = \mathrm x \psi(x) = x_0 \psi(x) recalling that \hat simply multiplies the wave-functions by the function \mathrm x , in the position representation. Since the function \mathrm x is variable while x_0 is a constant, \psi must be zero everywhere except at the point x_0 . Clearly, no continuous function satisfies such properties, and we cannot simply define the wave-function to be a complex number at that point because its L^2-norm would be 0 and not 1. This suggest the need of a "functional object" ''concentrated'' at the point x_0 and with integral different from 0: any multiple of the Dirac delta centered at x_0 .
Q.E.D. Q.E.D. or QED is an initialism of the Latin phrase , meaning "which was to be demonstrated". Literally it states "what was to be shown". Traditionally, the abbreviation is placed at the end of mathematical proofs and philosophical arguments in pri ...
The normalized solution to the equation \mathrm x \psi = x_0 \psi is \psi(x) = \delta(x - x_0), or better \psi = \delta _. Proof. Here we prove rigorously that \mathrm x \delta_ = x_0 \delta_ . Indeed, recalling that the product of any function by the Dirac distribution centered at a point is the value of the function at that point times the Dirac distribution itself, we obtain immediately \mathrm x \delta_ = \mathrm x (x_0) \delta_ =x_0 \delta_ . Q.E.D. Meaning of the Dirac delta wave. Although such Dirac states are physically unrealizable and, strictly speaking, they are not functions, Dirac distribution centered at x_0 can be thought of as an "ideal state" whose position is known exactly (any measurement of the position always returns the eigenvalue x_0 ). Hence, by the
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 ...
, nothing is known about the momentum of such a state.


Three dimensions

The generalisation to three dimensions is straightforward. The space-time wavefunction is now \psi(\mathbf, t) and the expectation value of the position operator \hat \mathbf at the state \psi is \left\langle \hat \mathbf \right\rangle _\psi = \int \mathbf , \psi, ^2 d^3 \mathbf where the integral is taken over all space. The position operator is \mathbf\psi = \mathbf\psi.


Momentum space

Usually, in quantum mechanics, by representation in the momentum space we intend the representation of states and observables with respect to the canonical unitary momentum basis \eta = \left(\left (2\pi\hbar)^ e^\rightright) _. In momentum space, the position operator in one dimension is represented by the following differential operator \left(\hat\right)_P = i\hbar\frac = i\frac, where: * the representation of the position operator in the momentum basis is naturally defined by \left(\hat\right)_P (\psi)_P = \left(\hat\psi\right)_P , for every wave function (tempered distribution) \psi; * \mathrm p represents the coordinate function on the momentum line and the wave-vector function \mathrm k is defined by \mathrm k = \mathrm p / \hbar .


Formalism in ''L''2(R, C)

Consider, for example, the case of a
spin Spin or spinning most often refers to: * Spinning (textiles), the creation of yarn or thread by twisting fibers together, traditionally by hand spinning * Spin, the rotation of an object around a central axis * Spin (propaganda), an intentionally ...
less particle moving in one spatial dimension (i.e. in a line). The state space for such a particle contains the ''L''2-space (
Hilbert space In mathematics, Hilbert spaces (named after David Hilbert) allow generalizing the methods of linear algebra and calculus from (finite-dimensional) Euclidean vector spaces to spaces that may be infinite-dimensional. Hilbert spaces arise natural ...
) L^2(\Reals,\Complex) of
complex-valued In mathematics, a complex number is an element of a number system that extends the real numbers with a specific element denoted , called the imaginary unit and satisfying the equation i^= -1; every complex number can be expressed in the form ...
and square-integrable (with respect to the
Lebesgue measure In measure theory, a branch of mathematics, the Lebesgue measure, named after French mathematician Henri Lebesgue, is the standard way of assigning a measure to subsets of ''n''-dimensional Euclidean space. For ''n'' = 1, 2, or 3, it coincides wi ...
) functions on the
real line In elementary mathematics, a number line is a picture of a graduated straight line that serves as visual representation of the real numbers. Every point of a number line is assumed to correspond to a real number, and every real number to a po ...
. The position operator in L^2(\Reals, \Complex) , Q : D_Q \to L^2(\Reals, \Complex) : \psi \mapsto \mathrm q \psi, is pointwise defined by: Q (\psi)(x) = x \psi (x) = \mathrm q(x) \psi (x), for each pointwisely defined square integrable class \psi \in D_Q and for each real number , with domain D_Q = \left\, where \mathrm q : \Reals \to \Complex is the coordinate function sending each point x \in \R to itself. Since all
continuous function In mathematics, a continuous function is a function such that a continuous variation (that is a change without jump) of the argument induces a continuous variation of the value of the function. This means that there are no abrupt changes in val ...
s with
compact support In mathematics, the support of a real-valued function f is the subset of the function domain containing the elements which are not mapped to zero. If the domain of f is a topological space, then the support of f is instead defined as the smalle ...
lie in ''D''(''Q''), ''Q'' is densely defined. ''Q'', being simply multiplication by ''x'', is a self-adjoint operator, thus satisfying the requirement of a quantum mechanical observable. Immediately from the definition we can deduce that the
spectrum A spectrum (plural ''spectra'' or ''spectrums'') is a condition that is not limited to a specific set of values but can vary, without gaps, across a continuum. The word was first used scientifically in optics to describe the rainbow of colors ...
consists of the entire
real line In elementary mathematics, a number line is a picture of a graduated straight line that serves as visual representation of the real numbers. Every point of a number line is assumed to correspond to a real number, and every real number to a po ...
and that ''Q'' has purely
continuous spectrum In physics, a continuous spectrum usually means a set of attainable values for some physical quantity (such as energy or wavelength) that is best described as an interval of real numbers, as opposed to a discrete spectrum, a set of attainable ...
, therefore no discrete
eigenvalues In linear algebra, an eigenvector () or characteristic vector of a linear transformation is a nonzero vector that changes at most by a scalar factor when that linear transformation is applied to it. The corresponding eigenvalue, often denote ...
. The three-dimensional case is defined analogously. We shall keep the one-dimensional assumption in the following discussion.


Measurement theory in ''L''2(R, C)

As with any quantum mechanical observable, in order to discuss position
measurement Measurement is the quantification of attributes of an object or event, which can be used to compare with other objects or events. In other words, measurement is a process of determining how large or small a physical quantity is as compared ...
, we need to calculate the spectral resolution of the position operator X : D_X \to L^2(\Reals, \Complex) : \psi \mapsto \mathrm x \psi which is X = \int_\R \lambda \, d \mu_X(\lambda) = \int_\R \mathrm x \, \mu_X = \mu_X (\mathrm x), where \mu_X is the so-called spectral measure of the position operator. Since the operator of X is just the multiplication operator by the embedding function \mathrm x, its spectral resolution is simple. For a
Borel subset In mathematics, a Borel set is any set in a topological space that can be formed from open sets (or, equivalently, from closed sets) through the operations of countable union, countable intersection, and relative complement. Borel sets are name ...
B of the real line, let \chi _B denote the
indicator function In mathematics, an indicator function or a characteristic function of a subset of a set is a function that maps elements of the subset to one, and all other elements to zero. That is, if is a subset of some set , one has \mathbf_(x)=1 if x\i ...
of B. We see that the projection-valued measure \mu_X : \mathcal(\R) \to \mathrm^\perp \left(L^2(\Reals, \Complex)\right) is given by \mu_X(B)(\psi) = \chi_B \psi , i.e., the orthogonal projection \mu_X(B) is the multiplication operator by the indicator function of B. Therefore, if the
system A system is a group of interacting or interrelated elements that act according to a set of rules to form a unified whole. A system, surrounded and influenced by its environment, is described by its boundaries, structure and purpose and express ...
is prepared in a state \psi, then the
probability Probability is the branch of mathematics concerning numerical descriptions of how likely an event is to occur, or how likely it is that a proposition is true. The probability of an event is a number between 0 and 1, where, roughly speaking, ...
of the measured position of the particle belonging to a
Borel set In mathematics, a Borel set is any set in a topological space that can be formed from open sets (or, equivalently, from closed sets) through the operations of countable union, countable intersection, and relative complement. Borel sets are na ...
B is \, \mu_X(B)(\psi)\, ^2 = \, \chi_B \psi\, ^2 = \int_B , \psi, ^2\ \mu =\pi_X(\psi)(B), where \mu is the Lebesgue measure on the real line. After any measurement aiming to detect the particle within the subset B, the wave function collapses to either \frac = \frac or \frac, where \, \cdot \, is the Hilbert space norm on L^2(\Reals, \Complex).


See also

* Position and momentum space *
Momentum operator In quantum mechanics, the momentum operator is the operator associated with the linear momentum. The momentum operator is, in the position representation, an example of a differential operator. For the case of one particle in one spatial dimensi ...
*
Translation operator (quantum mechanics) In quantum mechanics, a translation operator is defined as an operator which shifts particles and fields by a certain amount in a certain direction. More specifically, for any displacement vector \mathbf x, there is a corresponding translation ope ...


References

{{DEFAULTSORT:Position Operator Quantum mechanics