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In [[quantum mechanics]], the '''position operator''' is the [[operator (physics)|operator]] that corresponds to the position [[observable]] of a [[particle (physics)|particle]]. The [[eigenvalue]] of the operator is the [[position vector]] of the particle.<ref>{{cite book |title=Quanta: A handbook of concepts|first1=P.W. |last1=Atkins|publisher=Oxford University Press|year=1974|isbn=0-19-855493-1}}</ref> | |||
==Introduction== | |||
In one dimension, the wave function <math> \psi </math> represents the [[probability amplitude|probability density]] of finding the particle at position <math> x </math>. Hence the [[expected value]] of a measurement of the position of the particle is | |||
:<math> \langle x \rangle = \int_{-\infty}^{+\infty} x |\psi|^2 dx = \int_{-\infty}^{+\infty} \psi^* x \psi dx </math> | |||
Accordingly, the quantum mechanical [[Operator (physics)#Operators_in_quantum_mechanics | operator]] corresponding to position is <math> \hat{x} </math>, where | |||
:<math> (\hat{x} \psi)(x) = x\psi(x) </math> | |||
==Eigenstates== | |||
The eigenfunctions of the position operator, represented in position basis, are [[dirac delta functions]]. | |||
To show this, suppose <math> \psi </math> is an eigenstate of the position operator with eigenvalue <math> x_0 </math>. We write the eigenvalue equation in position coordinates, | |||
:<math> \hat{x}\psi(x) = x \psi(x) = x_0 \psi(x) </math> | |||
recalling that <math> \hat{x} </math> simply multiplies the function by <math> x </math> in position representation. Since <math> x </math> is a variable while <math> x_0 </math> is a constant, <math> \psi </math> must be zero everywhere except at <math> x = x_0 </math>. The normalized solution to this is | |||
:<math> \psi(x) = \delta(x - x_0) </math> | |||
Although such a state is physically unrealizable and, strictly speaking, not a function, it can be thought of as an "ideal state" whose position is known exactly (any measurement of the position always returns the eigenvalue <math> x_0 </math>). Hence, by the [[uncertainty principle]], nothing is known about the momentum of such a state. | |||
==Three dimensions== | |||
The generalisation to three dimensions is straightforward. The wavefunction is now <math> \psi(\bold{r},t) </math> and the expectation value of the position is | |||
:<math> \langle \bold{r} \rangle = \int \bold{r} |\psi|^2 d^3 \bold{r} </math> | |||
where the integral is taken over all space. The position operator is | |||
:<math>\bold{\hat{r}}\psi=\bold{r}\psi</math> | |||
==Momentum space== | |||
In [[momentum space]], the position operator in one dimension is | |||
:<math> \hat{x} = i\hbar\frac{d}{dp} </math> | |||
==Formalism== | |||
Consider, for example, the case of a [[spin (physics)|spin]]less particle moving in one spatial dimension (i.e. in a line). The [[state space (physics)|state space]] for such a particle is [[Lp space|''L''<sup>2</sup>('''R''')]], the [[Hilbert space]] of [[complex number|complex-valued]] and [[Square-integrable function|square-integrable]] (with respect to the [[Lebesgue measure]]) [[Function (mathematics)|function]]s on the [[real line]]. The position operator, ''Q'', is then defined by:<ref>{{cite book |title=Quantum Mechanics Demystified|first1=D. |last1=McMahon|edition=2nd|publisher=Mc Graw Hill|year=2006|isbn=0 07 145546 9}}</ref><ref>{{cite book |title=Quantum Mechanics|first1=Y. |last1=Peleg|first2=R.|last2= Pnini|first3=E.|last3= Zaarur|first4=E.|last4= Hecht|edition=2nd|publisher=McGraw Hill|year=2010|isbn=978-0071623582}}</ref> | |||
:<math> Q (\psi)(x) = x \psi (x) </math> | |||
with domain | |||
:<math>D(Q) = \{ \psi \in L^2({\mathbf R}) \,|\, Q \psi \in L^2({\mathbf R}) \}.</math> | |||
Since all [[continuous function]]s with [[compact support]] lie in ''D(Q)'', ''Q'' is [[densely-defined operator|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 of an operator|spectrum]] consists of the entire [[real line]] and that ''Q'' has purely [[continuous spectrum]], therefore no discrete [[eigenvalues]]. The three dimensional case is defined analogously. We shall keep the one-dimensional assumption in the following discussion. | |||
==Measurement== | |||
As with any quantum mechanical [[observable]], in order to discuss [[measurement]], we need to calculate the spectral resolution of ''Q'': | |||
:<math> Q = \int \lambda d \Omega_Q(\lambda).</math> | |||
Since ''Q'' is just multiplication by ''x'', its spectral resolution is simple. For a [[Borel subset]] ''B'' of the real line, let <math>\chi _B</math> denote the [[indicator function]] of ''B''. We see that the [[projection-valued measure]] Ω<sub>''Q''</sub> is given by | |||
:<math> \Omega_Q(B) \psi = \chi _B \psi ,</math> | |||
i.e. Ω<sub>''Q''</sub> is multiplication by the indicator function of ''B''. Therefore, if the [[system (physics)|system]] is prepared in state ''ψ'', then the [[probability]] of the measured position of the particle being in a [[Borel set]] ''B'' is | |||
:<math> |\Omega_Q(B) \psi |^2 = | \chi _B \psi |^2 = \int _B |\psi|^2 d \mu ,</math> | |||
where ''μ'' is the Lebesgue measure. After the measurement, the wave function [[wave function collapse|collapses]] to either | |||
<math> \frac{\Omega_Q(B) \psi}{ \|\Omega_Q(B) \psi \|} </math> | |||
or | |||
<math> \frac{(1-\chi _B) \psi}{ \|(1-\chi _B) \psi \|} </math>, where <math>\| \cdots \|</math> is the Hilbert space norm on ''L''<sup>2</sup>('''R'''). | |||
==See also== | |||
* [[Position and momentum space]] | |||
* [[Momentum operator]] | |||
==References== | |||
{{reflist}} | |||
{{Physics operator}} | |||
{{DEFAULTSORT:Position Operator}} | |||
[[Category:Quantum mechanics]] |
Revision as of 15:18, 13 September 2013
In quantum mechanics, the position operator is the operator that corresponds to the position observable of a particle. The eigenvalue of the operator is the position vector of the particle.[1]
Introduction
In one dimension, the wave function represents the probability density of finding the particle at position . Hence the expected value of a measurement of the position of the particle is
Accordingly, the quantum mechanical operator corresponding to position is , where
Eigenstates
The eigenfunctions of the position operator, represented in position basis, are dirac delta functions.
To show this, suppose is an eigenstate of the position operator with eigenvalue . We write the eigenvalue equation in position coordinates,
recalling that simply multiplies the function by in position representation. Since is a variable while is a constant, must be zero everywhere except at . The normalized solution to this is
Although such a state is physically unrealizable and, strictly speaking, not a function, it can be thought of as an "ideal state" whose position is known exactly (any measurement of the position always returns the eigenvalue ). Hence, by the uncertainty principle, nothing is known about the momentum of such a state.
Three dimensions
The generalisation to three dimensions is straightforward. The wavefunction is now and the expectation value of the position is
where the integral is taken over all space. The position operator is
Momentum space
In momentum space, the position operator in one dimension is
Formalism
Consider, for example, the case of a spinless particle moving in one spatial dimension (i.e. in a line). The state space for such a particle is L2(R), the Hilbert space of complex-valued and square-integrable (with respect to the Lebesgue measure) functions on the real line. The position operator, Q, is then defined by:[2][3]
with domain
Since all continuous functions with compact support 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 consists of the entire real line and that Q has purely continuous spectrum, therefore no discrete eigenvalues. The three dimensional case is defined analogously. We shall keep the one-dimensional assumption in the following discussion.
Measurement
As with any quantum mechanical observable, in order to discuss measurement, we need to calculate the spectral resolution of Q:
Since Q is just multiplication by x, its spectral resolution is simple. For a Borel subset B of the real line, let denote the indicator function of B. We see that the projection-valued measure ΩQ is given by
i.e. ΩQ is multiplication by the indicator function of B. Therefore, if the system is prepared in state ψ, then the probability of the measured position of the particle being in a Borel set B is
where μ is the Lebesgue measure. After the measurement, the wave function collapses to either
or
, where is the Hilbert space norm on L2(R).
See also
References
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