The parabolic cylinder functions are a class of functions sometimes called Weber functions. There are a number of slightly different definitions in use by various authors.
Whittaker and Watson (1990, p. 347) define the parabolic cylinder functions
as solutions to the Weber differential
equation
(1)
|
The two independent solutions are given by and
, where
(2)
| |||
(3)
|
which, in the right half-plane , is equivalent to
(4)
|
where
is the Whittaker function (Whittaker and Watson
1990, p. 347; Gradshteyn and Ryzhik 2000, p. 1018) and
is a confluent
hypergeometric function of the first kind.
This function is implemented in the Wolfram Language as ParabolicCylinderD[nu, z].
For
a nonnegative integer
, the solution
reduces to
(5)
| |||
(6)
|
where
is a Hermite polynomial and
is a modified Hermite
polynomial. Special cases include
(7)
| |||
(8)
|
for ,
where
is an modified Bessel function
of the second kind.
Plots of the function in the complex plane are shown above.
The parabolic cylinder functions satisfy the recurrence
relations
(9)
|
(10)
|
The parabolic cylinder function for integral can be defined in terms of an integral by
(11)
|
(Watson 1966, p. 308), which is similar to the Anger function. The result
(12)
|
where
is the Kronecker delta, can also be used to determine
the coefficients in the expansion
(13)
|
as
(14)
|
For
real,
(15)
|
(Gradshteyn and Ryzhik 2000, p. 885, 7.711.3), where is the gamma function
and
is the polygamma function of order 0.
Abramowitz and Stegun (1972, p. 686) define the parabolic cylinder functions as solutions to
(16)
|
sometimes called the parabolic cylinder differential equation (Zwillinger 1995, p. 414; Zwillinger 1997, p. 126). This can be rewritten by completing the square,
(17)
|
Now letting
(18)
| |||
(19)
|
gives
(20)
|
where
(21)
|
Equation (◇) has the two standard forms
(22)
| |||
(23)
|
For a general , the even and odd
solutions to (◇) are
(24)
| |||
(25)
|
where
is a confluent hypergeometric
function of the first kind. If
is a solution to (22), then (23) has solutions
(26)
|
Abramowitz and Stegun (1972, p. 687) define standard solutions to (◇) as
(27)
| |||
(28)
|
(29)
| |||
(30)
| |||
(31)
| |||
(32)
|
In terms of Whittaker and Watson's functions,
(33)
| |||
(34)
|