Momentum operator

In quantum mechanics, momentum is an operator which maps the wave function $ψ (x, t)$ to another function. If this new function is a constant $p$ multiplied by the original wave function $ψ$ , then $p$ is the eigenvalue of the momentum operator, and $ψ$ is the eigenfunction of the momentum operator. In quantum mechanics, the set of eigenvalues of an operator are the possible results measured in an experiment. The momentum operator is an example of a differential operator, for the case of one particle in one dimension, the definition is

{\hat {p}}=-i\hbar {\frac {\partial }{\partial x}}

where $ħ$ is Planck's reduced constant, $i$ the imaginary unit, and partial derivatives (denoted by "reverse 6") are used instead of a total derivative ( $d / dx$ ) since the wave function is also a function of time. The "hat" indicates an operator. The "application" of the operator on the wave function is as follows:

{\hat {p}}\psi =-i\hbar {\frac {\partial \psi }{\partial x}}

It is usual to think of the p-operator as "multiplying" the function, but this is not what is happening. The derivative of the function is taken.

At the time quantum mechanics was developed in the 1920s, the momentum operator was found by many theoretical physicists, including Niels Bohr, Arnold Sommerfeld, Erwin Schrödinger, and Eugene Wigner.

Origin from De Broglie plane waves

The momentum and energy operators can be constructed in the following way.^[1]

One dimension

Starting in one dimension, using the plane wave solution to Schrödinger's equation:

\psi =e^{i(kx-\omega t)}

The first order partial derivative with respect to space is

{\frac {\partial \psi }{\partial x}}=ike^{i(kx-\omega t)}=ik\psi

By expressing $k$ from the De Broglie relation:

p=\hbar k

the formula for the derivative of $ψ$ becomes:

{\frac {\partial \psi }{\partial x}}=i{\frac {p}{\hbar }}\psi

This suggests the operator equivalence:

{\hat {p}}=-i\hbar {\frac {\partial }{\partial x}}

so the momentum value $p$ is a scalar factor, the momentum of the particle and the value that is measured, is the eigenvalue of the operator.

Since the partial derivative is a linear operator, the momentum operator is also linear, and because any wavefunction can be expressed as a superposition of other states, when this momentum operator acts on the entire superimposed wave, it yields the momentum eigenvalues for each plane wave component, the momenta add to the total momentum of the superimposed wave.

Three dimensions

The derivation in three dimensions is the same, except the gradient operator del is used instead of one partial derivative. In three dimensions, the plane wave solution to Schrödinger's equation is:

\psi =e^{i({\mathbf {k}}\cdot {\mathbf {r}}-\omega t)}

and the gradient is

{\begin{aligned}\nabla \psi &={\mathbf {e}}_{x}{\frac {\partial \psi }{\partial x}}+{\mathbf {e}}_{y}{\frac {\partial \psi }{\partial y}}+{\mathbf {e}}_{z}{\frac {\partial \psi }{\partial z}}\\&=ik_{x}\psi {\mathbf {e}}_{x}+ik_{y}\psi {\mathbf {e}}_{y}+ik_{z}\psi {\mathbf {e}}_{z}\\&={\frac {i}{\hbar }}\left(p_{x}{\mathbf {e}}_{x}+p_{y}{\mathbf {e}}_{y}+p_{z}{\mathbf {e}}_{z}\right)\psi \\&={\frac {i}{\hbar }}{\mathbf {\hat {p}}}\psi \end{aligned}}

where $e x, e y$ and $e z$ are the unit vectors for the three spatial dimensions, hence

{\mathbf {\hat {p}}}=-i\hbar \nabla

This momentum operator is in position space because the partial derivatives were taken with respect to the spatial variables.

Definition (position space)

Properties

Hermiticity

The momentum operator is always a Hermitian operator when it acts on physical (in particular, normalizable) quantum states.^[4]

(In certain artificial situations, such as the quantum states on the semi-infinite interval [0,∞), there is no way to make the momentum operator Hermitian.^[5] This is closely related to the fact that a semi-infinite interval cannot have translational symmetry—more specifically, it does not have unitary translation operators. See below.)and to discuss the classical observable momentum in this case is meaningless.^[6]

Canonical commutation relation

Further information: Canonical commutation relation

One can easily show that by appropriately using the momentum basis and the position basis:

\left[{\hat {x}},{\hat {p}}\right]={\hat {x}}{\hat {p}}-{\hat {p}}{\hat {x}}=i\hbar .

The Heisenberg uncertainty principle defines limits on how accurately the momentum and position of a single observable system can be known at once. In quantum mechanics, position and momentum are conjugate variables.

Fourier transform

One can show that the Fourier transform of the momentum in quantum mechanics is the position operator. The Fourier transform turns the momentum-basis into the position-basis. The following discussion uses the bra–ket notation:

Let $\psi = \psi(x)$ be a wave packet $\langle \psi |\psi \rangle$ = 1, $\psi '$ the Fourier transform of $\psi$ :

\langle \psi |{\hat {p}}|\psi \rangle =h\langle \psi '|{\hat {x}}|\psi '\rangle

So momentum = h x spatial frequency, which is similar to energy = h x temporal frequency.

\langle x|{\hat {p}}|\psi \rangle =-i\hbar {\frac {d}{dx}}\psi (x)

The same applies for the position operator in the momentum basis:

\langle p|{\hat {x}}|\psi \rangle =i\hbar {\frac {d}{dp}}\psi (p)

and other useful relations:

\langle p|{\hat {x}}|p'\rangle =i\hbar {\frac {d}{dp}}\delta (p-p')

\langle x|{\hat {p}}|x'\rangle =-i\hbar {\frac {d}{dx}}\delta (x-x')

where $δ$ stands for Dirac's delta function.

Derivation from infinitesimal translations

4-momentum operator

Inserting the 3d momentum operator above and the energy operator into the 4-momentum (as a 1-form with $(+ - - -)$ metric signature):

P_{\mu }=\left({\frac {E}{c}},-{\mathbf {p}}\right)

obtains the 4-momentum operator;

{\hat {P}}_{\mu }=\left({\frac {1}{c}}{\hat {E}},-{\mathbf {\hat {p}}}\right)=i\hbar \left({\frac {1}{c}}{\frac {\partial }{\partial t}},\nabla \right)=i\hbar \partial _{\mu }

where $\partial μ$ is the 4-gradient, and the $- iħ$ becomes $+ iħ$ preceding the 3-momentum operator. This operator occurs in relativistic quantum field theory, such as the Dirac equation and other relativistic wave equations, since energy and momentum combine into the 4-momentum vector above, momentum and energy operators correspond to space and time derivatives, and they need to be first order partial derivatives for Lorentz covariance.

The Dirac operator and Dirac slash of the 4-momentum is given by contracting with the gamma matrices:

\gamma ^{\mu }{\hat {P}}_{\mu }=i\hbar \gamma ^{\mu }\partial _{\mu }={\hat {P}}=i\hbar \partial \!\!\!/

If the signature was $(- + + +)$ , the operator would be

{\hat {P}}_{\mu }=\left(-{\frac {1}{c}}{\hat {E}},{\mathbf {\hat {p}}}\right)=-i\hbar \left({\frac {1}{c}}{\frac {\partial }{\partial t}},\nabla \right)=-i\hbar \partial _{\mu }

instead.

References

↑ Quantum Physics of Atoms, Molecules, Solids, Nuclei and Particles (2nd Edition), R. Resnick, R. Eisberg, John Wiley & Sons, 1985, ISBN 978-0-471-87373-0
↑ Quantum Mechanics Demystified, D. McMahon, Mc Graw Hill (USA), 2006, ISBN 0-07-145546-9
↑ Quantum Physics of Atoms, Molecules, Solids, Nuclei and Particles (2nd Edition), R. Resnick, R. Eisberg, John Wiley & Sons, 1985, ISBN 978-0-471-87373-0
↑ See Lecture notes 1 by Robert Littlejohn for a specific mathematical discussion and proof for the case of a single, uncharged, spin-zero particle. See Lecture notes 4 by Robert Littlejohn for the general case.
↑ Bonneau,G., Faraut, J., Valent, G. (2001). "Self-adjoint extensions of operators and the teaching of quantum mechanics". American Journal of Physics. 69 (3): 322–331. arXiv:quant-ph/0103153. Bibcode:2001AmJPh..69..322B. doi:10.1119/1.1328351.
↑ Z.Y.Wang (2016). "Generalized momentum equation of quantum mechanics". Optical and Quantum Electronics. 48 (2): 1–9. doi:10.1007/s11082-015-0261-8.

Operators in physics

General

Space and time	Parity Time evolution D'Alembert operator

Particles	C-symmetry

Operators for operators	Ladder operator Anti-symmetric operator

Quantum

Fundamental	Position Momentum Rotation

Energy	Total energy Kinetic energy Hamiltonian

Angular momentum	Spin Orbital Total

Electromagnetism	Transition dipole moment

Optics	Displacement Squeeze Quantum correlator Hanbury Brown and Twiss effect

Particle physics	Creation and annihilation Casimir invariant

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