The wave functions capable of representing a given quantum system belong to a function space
which should be specified precisely. In order that the probability distribution of position P
and
momentum Π
have meaning, it is necessary and sufficient that the normalization
condition
could be applied to the wave function ψ(r). We are thus led to the following definition of wave
function space:
Definition 1.1. The wave functions of wave mechanics are the square integrable functions
of configuartion space, that is to say the functions ψ(q1,…,qR) such that the integral
∫
2dτ converges.
Where dτ denotes the volume element dq1dq2…dqR. Also, note that the Fourier transform
ϕ(p1,…,pR) of such a function always exists: it is a square integrable function possessing the same
normalization as ψ(q1,…,qR).
We could restrict the function space somewhat more by requiring the wave functions to be
normalized to unity (eq. 1). Hwever, it turns out to be more convenient to relax this normalization
condition; this can be done, as we shall see below, at the price of a slight modification in the
definition of the statistical distributions and probabilities.
In the langage of mathematics, the function space defined above is a Hilbet space. It possesses
indeed the properties characteristic of such a space, as shown below.
In the first place, it is a linear space. If ψ1 and ψ2 are two square integrable functions,
their sum, the product of each by a complex number and, more enerally, any linear
combinations
where λ1 and λ2 are arbitrarily chosen complex numbers, are also square-integrable
functions.
In the second place, one can define a scalar product in that space. By definition, the scalar product
of the function ψ by the function ϕ is
If it is zero, the functions ϕ and ψ are said t be orthogonal. The norm Nψ of a funcion ψ is the
scalar product of this function by itself:
The fundamental properties of the scalar product are as follows:
a) the scalar product of ϕ and ψ is the complex conjugate of the scalar product of ψ by ϕ,
namely
b) the scalar product of ψ by ϕ is linear with respect to ψ, in other words
c) the norm of a function ψ is a real, non-negative number:
and if < ψ,ψ >= 0, we have necessarily ψ = 0.
All the above properties are easily deduced from the very definition of the scalar product itself.
From properties (a) and (b) one easily shows that the scalar product < ϕ,ψ > does not depend
linearly, but antilinearly on ϕ:
From the properties (a),(b), and (c) follows a very important property of the scalar produt, the
Schwarz inequality
Equality obtains when the functions ϕ and ψ are multiples of each other, and only in that case.
The Schwarz inequality insures that the integral (2) defining the scalar product convertges when
the functions ϕ and ψ are square integrable functions.
In addition to the fact that it is linear and that one can define a scalar product there, the space of
square integrable functions possesses the property of being complete; this is what allows us to
identify it as a Hilbert space. To be complete means that any set of suare integrable functions
satisfying the Cauchy criterion, converges (in the quadratic mean) toward a square integrable
function. Conversely, any square integrable function can be considered as the limit (in the
quadratic mean) of a converging series( in the sense of Cauchy) of square integrable functions
(separability).
1.1 References
[1] Messiah, Albert. ”Quantum mechanics: Volume I.” Amsterdam, North-Holland Pub. Co.; New
York, Interscience Publishers, 1961-62.
This entry is a derivative of the Public domain work [1].