1. Introduction
In [
1], Nobert Wiener introduced the concept of “integration in function space”. At present, the space of real-valued continuous functions
equipped with a Gaussian measure is called the Wiener space. In [
2], Yeh introduced a generalized Wiener space
related to a generalized Brownian motion process (henceforth, GBMP) associated with continuous functions
and
. This theory for the function space
was developed further by Chang and Chung in [
3,
4] and was used extensively in [
5,
6,
7,
8,
9] with various related results. The authors in [
5] derived simple formulas for conditional function space integrals of functionals on the generalized Wiener space
and its applications. In [
6], the authors studied relationships among the integral transforms, convolution products, first variation, and inverse transforms of functionals on
. Chang [
7] proposed the conditional generalized Fourier–Feynman transform of functionals in Fresnel-type classes. In [
8,
9], the authors investigated generalized integral transforms of functionals on
, and extended generalized Fourier–Feynman transforms with a first variation (the Gâteaux derivative) on the function space
.
Let be a probability space. The stochastic process Y on and an interval is called a GBMP, provided the following apply:
- (i)
-a.e.;
- (ii)
For
, the random vector
has a normal distribution with the following density function:
where
,
, and
are suitable continuous real-valued functions on
.
We note that the GBMP
Y determined by the functions
and
is Gaussian with mean
and covariance
. Let
be the complete generalized Wiener space, where
is the continuous sample paths of the GBMP
Y. In the case of
and
, the function space
reduces to the classical Wiener space
. In
Section 2, we will provide a more detailed construction of the function space
.
Many physical problems can be represented by the conditional Wiener integral
of the Wiener integrable functionals
F on
, which have the following form:
where
, and
is a sufficiently smooth function on
. It is known from [
10,
11] that the function
on
defined by
forms a solution to the partial differential equation
under an appropriate initial condition at
. The Kac’s result described above was extended by Chang and Chung in [
3,
4].
On the other hand, the Cameron–Martin translation theorem [
12] and several analogies [
13,
14] describe how and when the Wiener measure
changes under translation with specific elements in the Wiener space
. This translation theorem was developed for the Yeh–Wiener [
15], abstract Wiener [
16], conditional Wiener [
17,
18], analytic Feynman [
19,
20], and conditional analytic Feynman [
21] integrals. Furthermore, a translation theorem on the generalized Wiener space
was first established by Chang and Chung in [
3] and improved in [
9].
In [
3,
4], Chang and Chung used the
n-dimensional conditioning function
to study a generalized heat equation and a translation theorem for the conditional function space integral of functionals on the function space
.
This study aims to present a translation theorem for conditional function space integrals on the function space
. To achieve this, we use the conditioning function with the following form:
where
is an orthonormal subset of the Cameron–Martin space in
, and
denotes the Paley–Wiener–Zygmund (henceforth, PWZ) stochastic integral. We also derive a translation theorem for conditional generalized analytic Feynman integrals of functionals
F on
. To establish the translation theorem for the conditional generalized analytic Feynman integral on the function space, we assume that the conditional generalized analytic Feynman integral that appears in the theorem exists because the drift term
of the GBMP makes establishing the existence of the conditional Feynman integral very difficult. The function
defining the GBMP is interpreted as the “drift” of the GBMP. Thus, in
Section 6, we provide explicit examples of functionals on
to which the translation theorems can be applied. Our formulas and results are more complicated than the corresponding formulas and results in the previous research because the generalized Wiener process used in this study is nonstationary in time and subject to drift
, which can be used to explain the position of the Ornstein–Uhlenbeck process in an external force field [
22]. However, by choosing
and
on
, the function space
reduces to the Wiener space
; thus, the expected results on
are immediate corollaries of our results.
The generalized Wiener space is fundamentally different from the classical Wiener space as it is induced by a GBMP that incorporates a non-trivial drift function. The presence of this drift means that the underlying process is neither stationary nor centered and introduces significant mathematical complexity that prior work on does not address.
The authors in [
23] introduced the octonion linear canonical transform to expand transformation theory to higher algebraic structures. In [
24,
25], the authors proposed a piecewise scheme for Chebyshev finite-difference time-domain methods in computational mathematics and worked on homogeneity pursuit in functional-coefficient quantile regression models with censored panel data. The researcher in [
26] applied neural ordinary differential equations for robust parameter estimation with physical priors. The authors in [
27] developed quantum stochastic differential equations related to annihilation and creation operators. In [
28,
29], the researcher focused on quantum stochastic processes, including boson field implementations, Girsanov transforms, and covariant semigroups. The researchers in [
30,
31] developed white noise differential equations and the quantum Lévy Laplacian with heat equation connections. Our findings could be useful in the field of infinite dimensional analysis and further advance generalized Fourier transform [
23], difference equations [
24], linear data models [
25], ordinary differential equations [
26], stochastic differential equations [
27], quantum field theory [
28,
29], white noise differential equations [
30,
31], etc. If we construct rather rigorous mathematical interpretations associated with elaborate stochastic processes such as the GBMP, then various mathematical theories and related results based on the research [
23,
24,
25,
26,
27,
28,
29,
30,
31] will be more relevant to real-world problems.
The theoretical application in this article is also used to derive a corresponding translation theorem for the conditional generalized analytic Feynman integral, which is non-trivial and provides a toolkit for performing rigorous calculations in functional integration within this generalized setting.
2. Definitions and Preliminaries
2.1. Backgrounds
Two functions,
and
, were given in
Section 1. We assume that the function
is continuous and of bounded variation on
with
, and the function
is continuous, monotone, increasing, and of bounded variation on
with
. Then, considering Theorems 12.2 and 14.2 from [
32], there exists a probability space
and an additive process
Y on
and the interval
where
is a Gaussian measure such that the probability distribution of
with
is normally distributed with mean
and variance
. The stochastic process
Y on
and
is called a GBMP. The GBMP
Y is determined using
, and
is a Gaussian process with mean function
and covariance function
.
Let
be the space of continuous sample paths of the GBMP
Y determined by
and
. The function space
is equivalent to the Banach space of continuous functions
x on
with
under the supremum norm. Let
be the Borel
-field on
. Then, as explained in [
32], pp. 18–21,
Y induces a probability measure
on the measurable space
. Hence,
is the function space induced by
Y. We then complete this function space to obtain
, where
is the set of all
-Carathéodory measurable subsets of
. It is worth noting that, by choosing
and
on
, one can see that the GBMP reduces to a standard Brownian motion.
In this study, we assume the following:
- (i)
The mean function
of the GBMP
Y is absolutely continuous on
and satisfies the requirement
where
denotes the total variation function of
on
;
- (ii)
The derivative of is of class ;
- (iii)
The variance function of the GBMP Y is continuously differentiable on ;
- (iv)
For each , .
Then, it follows that, for any cylinder set
of the form
with a subdivision
of
and a Borel set
,
where
.
Let
be the linear space (equivalence classes) of Lebesgue measurable functions
w on
, which satisfy the conditions
where
.
For
, let
Then,
is an inner product on
and
is a norm on
. In particular, it is worth noting that
if and only if
-a.e. on
, where
denotes the Lebesgue measure on
. Furthermore,
is a separable Hilbert space. Using the assumptions on the functions
and
, one can see that the functions
and
are elements of the Hilbert space
. It is worth noting that the function
,
does not satisfy requirement (
1), even though its derivative is an element of
.
Let
be a complete orthonormal set of functions in
,
such that the
s are of bounded variation on
. Then, for
and
, we define the PWZ stochastic integral
as
if the limit exists. For each
, the PWZ stochastic integral
exists for
-a.e.
. For each
, the PWZ stochastic integral
is a non-degenerate Gaussian random variable with mean
and variance
. If
is an orthogonal set of functions in
, then the random variables,
, are independent. Furthermore, if
is of bounded variation on
, then the PWZ stochastic integral
equals the Riemann–Stieltjes integral
. Also, we note that, for
,
In particular, for each and , it follows that and .
2.2. Generalized Analytic Feynman Integral
We denote the function space integral of a -measurable functional F using whenever the integral exists.
A subset S of is called a scale-invariant measurable set provided is -measurable for all , and a scale-invariant measurable set N is called a scale-invariant null set provided for all . A property that holds except on a scale-invariant null set is said to hold scale invariance almost everywhere (s-a.e.). A functional F is said to be scale-invariant measurable provided that F is defined on a scale-invariant measurable set, and is -measurable for every .
It was pointed out in [
33] that the concept of scale-invariant measurability, rather than Borel or Wiener measurability, is accurate for the analytic Feynman integration theory. Hence, throughout this study, we always assume that each functional
that we consider satisfies the following conditions:
and
Also, let , , and denote the set of complex numbers, complex numbers with a positive real part, and non-zero complex numbers with a nonnegative real part, respectively. Furthermore, for each , denotes the principal square root of .
Definition 1. Let a functional F on satisfy conditions (3) and (4). If there exists a function analytic in such thatfor all , then is defined to be the analytic function space integral of F over with parameter λ, and, for , we write Let be a real number and F be a functional on such that the analytic function space integral exists for all . If the following limit exists, we call it the generalized analytic Feynman integral of F with parameter q and write the following: 2.3. Conditional Function Space Integrals
We now state the definitions of the conditional function space integral and the conditional generalized analytic Feynman integral.
Definition 2. Let be a -measurable function with a probability distribution that is absolutely continuous with respect to the Lebesgue measure on . Let F be a -valued μ-integrable functional on . Then, the conditional integral of F given X, denoted by , is a Lebesgue measurable function of , unique up to null sets in , satisfying the following equation: for all Borel sets B in Let
n be a positive integer and
be an orthonormal set of functions in the Hilbert space
. Throughout this study, we will use the following conditioning function: For each positive integer
n, let
be given by
We now define the conditional generalized analytic Feynman integral of functionals F on .
Definition 3. Let functional satisfy conditions (3) and (4) and let be given by Equation (5). For and , letdenote the conditional function space integral of given If, for a.e. , there exists a function analytic in λ on such that for all , then is defined to be the conditional analytic function space integral of F given with parameter λ. For , we writeif, for a fixed real , the limitexists for a.e. . We will denote the value of this limit by , and we call it the conditional generalized analytic Feynman integral of F given X with parameter q. We define by for , and we write for .
In [
5], Chang, Choi, and Skoug derived a formula for expressing conditional function space integrals in terms of ordinary function space integrals. We provide a modified result from [
5], Theorem 3.4, which plays an important role in this paper. The proof given in [
5] with the current hypotheses on
and
and the definition of the PWZ stochastic integral also works here.
Theorem 1. Let X be given by Equation (5) and let F be a μ-integrable functional on . Then, Remark 1. Equation (6) is indeed a very simple formula equating the conditional function space integral in terms of an ordinary function space integral. Let
F be a functional on
which satisfies conditions (
3) and (
4). Then, one can easily see from (
6) that, for all
,
for a.e.
. Thus, we have the following:
and
where, in (
7) and (
8), the existence of either side implies the existence of the other side and their equality.
3. Translation Theorems for Conditional Function Space Integrals
Due to their nature, Gaussian measures on function spaces do not have the property of translation invariance. However, as first shown by Cameron and Martin in [
12], they enable the computation of the Radon–Nikodym derivatives of measures resulting from certain translations. In particular, there is a specific class of functions which, along with translation results, yields an equivalent Gaussian measure. In the case of ordinary Wiener space
, this collection of allowable translates coincides with the Sobolev space
of functions vanishing at 0 with square-integrable weak derivatives on
. For the generalized Wiener space
, similar but more complicated results hold.
We start this section with translation theorems on the function space . We then use this translation theorem to obtain conditional function space integration formulas.
Theorem 2 ([
3,
9])
. (Translation theorems for function space integral). Let X be given by (5) and let F be a μ-integrable functional on . Then, for any function in ,and With the current hypotheses on and and the definition of the PWZ stochastic integral, we have the following lemma:
Lemma 1 ([
5])
. The processes and are independent. Remark 2. Lemma 1 makes an interesting observation about the process . The process has been widely used to approximate the generalized Brownian motion , while has been applied to a Brownian bridge process.
We are obliged to point out the facts that, for each
, the PWZ stochastic integral
is a Gaussian random variable with mean
and variance
and that, if
is an orthogonal set of functions in
, then the random variables
s are independent. Thus, applying the change of variables theorem, the Fubini theorem, and the integration formula,
and we have the following lemma:
Lemma 2. Given an orthonormal set of functions in and a function in , it follows that In our next theorem, we establish a translation theorem for the conditional function space integral.
Theorem 3. Let X and F be as in Theorem 2. Then, for any function in ,where . Proof. Using Equations (
6), (
9), and (
2) and applying Lemma 1, it follows that
Using (
6) and (
11), Equation (
13) can be rewritten as
as desired. □
Corollary 1. Let X and F be as in Theorem 2. Then, it follows that, for any function in , Proof. Let
. Then, using (
12) with
F replaced by
G, it follows that
From this, we obtain the following:
Replacing
with
in (
15), we have Equation (
14) as desired. □
Remark 3. Using techniques similar to those used in the proof of Theorem 3, we can establish Equation (14) without using Equation (12). Also, Equation (12) can be established using Equation (14). 4. Conditional Function Space Integration Formulas
In [
3], Chang and Chung extended the results of [
34,
35] to the function space
using the vector-valued conditioning function
given by
The conditioning function
given by (
16) can be represented by the conditioning function
X given by (
5) with a specific choice of
s.
Let
be a partition of
. For each
, let
Then,
is an orthonormal set of functions in
; thus, the conditioning function
given by
is a specific example of our conditioning function used in the previous section. Given a vector
, let
for each
. Then, it follows that
From this, it also follows that, for any
,
and, for any
,
with
.
Given a vector
, let
for each
. Then, it follows that, for each
,
where
, and
In view of Theorem 1 and with the above setting, we have the following corollary:
Corollary 2. Let F be a μ-integrable functional on . Then, the conditioning function given by equation (18) yields the conditioning function given by (16), and it follows the following conditional function space integration formula:where and are given by (21) and (20), respectively. Lemma 3. For each , let be given by (17). Then, it follows thatand, for any function in , Corollary 3 ([
3])
. Let F be a μ-integrable functional on , and, given a partition of and a vector , let , , , and be as above. Then, it follows that, for any function in ,where . Proof. Using (
16), (
14), (
19), (
22), and (
23), one can derive Equation (
24). □
Corollary 4. Let F be a μ-integrable functional on , and, given a partition of and a vector , let , , , and be as above. Then, it follows that, for any function in ,where . Proof. Using (
16), (
12), (
19), (
22), and (
23), one can also derive Equation (
25). □
Example 1. Let be the linear operator defined by Then, we see that the adjoint operator of S is given by Using an integration with the part formula, it follows that Let be an orthonormal set of functions in and let . Also, for , let . Then, using Equation (14) with on , we obtain the following: Using Equation (26), we immediately obtain the conditional function space integration formula In particular, using (27) with replaced by , and integration with the part formula, we obtain the following:where . The functional discussed in Example 1 arises naturally in quantum mechanics.
As mentioned in
Section 1 above, the formulas with the one-dimensional conditioning function
is more relevant in heat and Schrödinger equation theories and other applications.
Consider the conditioning function
given by
. This conditioning function
will play a good role between the previous and current research for conditional function space integrals because
Notice that is an orthonormal set in .
Example 2. Let F be a μ-integrable functional on and let be a function in . Then, Equation (24) reduces the following formula for : Replacing η with in Equation (28), it also follows that In particular, setting , we have the conditional function space integration formula Example 3. Let F be a μ-integrable functional on and let be a function in . Then, Equation (25) reduces the formula Replacing η with in Equation (30), it also follows that Also, setting , we have One can easily see that Equation (31) with replaced with coincides with Equation (29).