The Wigner distribution of a square-integrable complex function is the time-frequency function
|
(1)
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Its marginal integrals, interpreted weakly when necessary, recover the position and frequency energy densities,
|
(2)
| |||
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(3)
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where
is the Fourier transform with kernel
. If
, both marginals are probability
density functions. Under this normalization, the real-valued Wigner distribution
is a quasiprobability distribution, since it need not be nonnegative and therefore
need not be a joint probability density
function.
For a normalized wave function , the momentum convention used in quantum mechanics is
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(4)
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where
is momentum and
is the reduced Planck constant (Case 2008, p. 938). The factor
ensures that the integral of
over phase space is 1.
For the quantum harmonic oscillator with Hamiltonian
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(5)
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where
and
,
the normalized stationary wave functions are scaled Hermite
functions. Their Wigner functions are
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(6)
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where ,
1, 2,
,
is a Laguerre polynomial,
, and
(Curtright et al. 1998). The ground
state
gives a positive Gaussian function, whereas
the first excited state has
. A coherent state, obtained by displacing
the ground state to position
and momentum
, has the Gaussian function
(Case 2008, pp. 940-942)
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(7)
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For a time-independent Hamiltonian with
a polynomial of degree
at most 2, the exact quantum evolution of the Wigner function
obeys the classical transport equation
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(8)
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where
is the Poisson bracket. The quantum corrections
vanish because they contain derivatives of
of order at least 3 (Case 2008, pp. 941-942). If
is the flow determined by Hamilton's
equations, then
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(9)
|
For the harmonic oscillator this is a rigid clockwise rotation in the scaled coordinates with angular speed
, for every initial state. In particular, a coherent state's
Gaussian function retains its shape while its
center follows the classical orbit.