In quantum mechanics, the position operator is the operator that corresponds to the position observable of a particle. When the position operator is considered with a wide enough domain (e.g. the space of tempered distributions), its eigenvalues are the possible position vectors of the particle. In one dimension, if by the symbol | x ⟩ {\displaystyle |x\rangle } we denote the unitary eigenvector of the position operator corresponding to the eigenvalue x {\displaystyle x} , then, | x ⟩ {\displaystyle |x\rangle } represents the state of the particle in which we know with certainty to find the particle itself at position x {\displaystyle x} . Therefore, denoting the position operator by the symbol X {\displaystyle X} we can write X | x ⟩ = x | x ⟩ , {\displaystyle X|x\rangle =x|x\rangle ,} for every real position x {\displaystyle x} . One possible realization of the unitary state with position x {\displaystyle x} is the Dirac delta (function) distribution centered at the position x {\displaystyle x} , often denoted by δ x {\displaystyle \delta _{x}} . In quantum mechanics, the ordered (continuous) family of all Dirac distributions, i.e. the family
δ = ( δ x ) x ∈ R , {\displaystyle \delta =(\delta _{x})_{x\in \mathbb {R} },}
is called the (unitary) position basis, just because it is a (unitary) eigenbasis of the position operator X {\displaystyle X} in the space of tempered distributions. It is fundamental to observe that there exists only one linear continuous operator X {\displaystyle X} on the space of tempered distributions to itself, such that
X ( δ x ) = x δ x , {\displaystyle X(\delta _{x})=x\delta _{x},}
for every real point x {\displaystyle x} . It is possible to prove that the unique operator X {\displaystyle X} is necessarily defined by
X ( ψ ) = x ψ , {\displaystyle X(\psi )=\mathrm {x} \psi ,}
for every tempered distribution ψ {\displaystyle \psi } , where x {\displaystyle \mathrm {x} } denotes the coordinate function of the position line – defined as the inclusion of the real line into the complex plane i.e
x : R → C : x ↦ x . {\displaystyle \mathrm {x} :\mathbb {R} \to \mathbb {C} :x\mapsto x.}
Introduction Consider representing the quantum state of a particle at a certain instant of time by a square integrable wave function ψ {\displaystyle \psi } . For now, assume one space dimension (i.e. the particle "confined to" a straight line). If the wave function is normalized, then the square modulus
| ψ | 2 = ψ ∗ ψ , {\displaystyle |\psi |^{2}=\psi ^{*}\psi ,}
represents the probability density of finding the particle at some position x {\displaystyle x} of the real-line, at a certain time. That is, if
‖ ψ ‖ 2 = ∫ − ∞ + ∞ | ψ | 2 d x = 1 , {\displaystyle \|\psi \|^{2}=\int _{-\infty }^{+\infty }|\psi |^{2}d\mathrm {x} =1,}
then the probability to find the particle in the position range [ a , b ] {\displaystyle [a,b]} is
π X ( ψ ) ( [ a , b ] ) = ∫ a b | ψ | 2 d x . {\displaystyle \pi _{X}(\psi )([a,b])=\int _{a}^{b}|\psi |^{2}d\mathrm {x} .}
Hence the expected value of a measurement of the position X {\displaystyle X} for the particle is
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