CONDITIONAL FOURIER-FEYNMAN TRANSFORM AND CONVOLUTION PRODUCT OVER WIENER PATHS IN
ABSTRACT WIENER SPACE : AN L p THEORY
Dong Hyun Cho
Abstract. In this paper, using a simple formula, we evaluate the conditional Fourier-Feynman transforms and the conditional con- volution products of cylinder type functions, and show that the conditional Fourier-Feynman transform of the conditional convolu- tion product is expressed as a product of the conditional Fourier- Feynman transforms. Also, we evaluate the conditional Fourier- Feynman transforms of the functions of the forms
exp
Z
T 0θ(s, x(s))ds
, exp
Z
T 0θ(s, x(s))ds
φ(x(T )),
exp
Z
T 0θ(s, x(s))dζ(s)
, exp
Z
T 0θ(s, x(s))dζ(s)
φ(x(T )) which are of interest in Feynman integration theories and quantum mechanics.
1. Introduction and preliminaries
Let C 0 [0, T ] denote the classical Wiener space, that is, the space of real-valued continuous functions x(t) on [0, T ] with x(0) = 0. The con- cept of conditional Wiener integral on Wiener space was introduced by Yeh in [18, 19]. By a conditional Wiener integral we mean the condi- tional expectation E[F |X] of a real or complex-valued Wiener integrable function F conditioned by a Wiener measurable function X on C 0 [0, T ],
Received January 5, 2003. Revised March 12, 2003.
2000 Mathematics Subject Classification: 28C20.
Key words and phrases: conditional analytic Feynman integral, conditional convo- lution product, conditional Fourier-Feynman transform, conditional Wiener integral, cylinder type function, simple formula for conditional Wiener integral.
Research supported by the Basic Science Research Institute Program, Korea Re-
search Foundation under Grant KRF 2001-005-D20004.
which is given as a function on the value space of X. We shall be con- cerned exclusively with X given by X(x) = (x(t 1 ), . . . , x(t k )), where 0 < t 1 < · · · < t k = T for any fixed positive integer k. In [14], Park and Skoug derived a simple formula for the conditional Wiener integral with the conditioning function X. They then used this formula to express conditional Wiener integrals directly in terms of ordinary Wiener inte- grals. In [15], Park and Skoug introduced the concept of a conditional Fourier-Feynman transform and the concept of a conditional convolu- tion product and obtained several formulas relating these concepts; in particular see equations (3.13) and (4.11) in [15]. In [5], using ideas and formulas developed in [15], Chang and Skoug examined the effects that drift had on conditional Fourier-Feynman transforms and conditional convolution products. In section 4 of [5] and in section 4 of [15] the au- thors established various formulas involving conditional transforms and conditional convolution products for functions in the Banach algebra S which was introduced by Cameron and Storvick in [1].
In [12], Kuelbs and Lepage introduced C 0 (B), the space of continuous functions on [0, T ] into B which vanish at 0. In [16], Ryu established various properties involving C 0 (B). In [20], Yoo introduced the Banach algebra S B ′′ which corresponds to Cameron and Storvick’s space S ′′ in [1]. Chang and his coworkers introduced the class A (p) n,s (1 ≤ p ≤ ∞) of cylinder type functions defined on C 0 (B), and then established rela- tionships between the Fourier-Feynman transform and the convolution product of functions in A (p) n,s ([4]).
In [2], Chang and his coworkers defined the L 1 conditional Fourier- Feynman transform and the conditional convolution product on the space C 0 (B), and they investigate relationships between them.
In this paper, we define the L p conditional Fourier-Feynman trans- form on C 0 (B) for 1 < p ≤ ∞, and we evaluate the L p conditional Fourier-Feynman transforms and the conditional convolution products of functions in A (p) n,s , and then, we show that the conditional Fourier- Feynman transform of the conditional convolution product can be ex- pressed as a product of the conditional Fourier-Feynman transforms for these functions. Also, for 1 ≤ p ≤ ∞, we evaluate the L p conditional Fourier-Feynman transforms of the functions of the forms
exp
Z T 0
θ(s, x(s))ds
, exp
Z T 0
θ(s, x(s))ds
φ(x(T )), exp
Z T 0
θ(s, x(s))dζ(s)
, exp
Z T 0
θ(s, x(s))dζ(s)
φ(x(T ))
which are of interest in Feynman integration theories and quantum me- chanics.
Let (Ω, A, P ) be a probability space, let B be a real normed linear space with norm k · k and let B(B) be the Borel σ-field on B. Let X : (Ω, A, P ) → (B, B(B)) be a random variable and let F : Ω → C be an integrable function. Let P X be the probability distribution of X on (B, B(B)) and let D be the σ-field {X −1 (A) : A ∈ B(B)}. Let P D be the probability measure induced by P , that is, P D (E) = P (E) for E ∈ D.
By the definition of conditional expectation there exists a D-measurable function E[F |X](the conditional expectation of F given X) defined on Ω such that the relation
Z
E
E [F |X](ω) dP D (ω) = Z
E
F (ω) dP (ω)
holds for every E ∈ D. But there exists a P X -integrable function ψ defined on B which is unique up to P X -a.e. such that E[F |X](ω) = (ψ◦X)(ω) for P D -a.e. ω in Ω. ψ is also called the conditional expectation of F given X and without loss of generality, it is denoted by E[F |X](ξ) for ξ ∈ B. Throughout this paper, we will consider the function ψ as the conditional expectation of F given X.
2. Wiener paths in abstract Wiener space
Let (H, B, m) be an abstract Wiener space([13]). Let {e j : j ≥ 1} be a complete orthonormal set in the real separable Hilbert space H such that e j ’s are in B ∗ , the dual space of real separable Banach space B. For each h ∈ H and y ∈ B, define the stochastic inner product (h, y) ∼ by
(h, y) ∼ =
lim n→∞ P n
j=1 hh, e j i(y, e j ), if the limit exists;
0, otherwise,
where (·, ·) denotes the dual pairing between B and B ∗ ([11]). Note that for each h(6= 0) in H, (h, ·) ∼ is a Gaussian random variable on B with mean zero, variance |h| 2 ; also (h, y) ∼ is essentially independent of the choice of the complete orthonormal set used in its definition and further, (h, λy) ∼ = (λh, y) ∼ = λ(h, y) ∼ for all λ ∈ R. It is well-known that if {h 1 , h 2 , . . . , h n } is an orthogonal set in H, then the random variables (h j , ·) ∼ ’s are independent. Moreover, if both h and y are in H, then (h, y) ∼ = hh, yi.
Let C 0 (B) denote the set of all continuous functions on [0, T ] into B
which vanish at 0. Then C 0 (B) is a real separable Banach space with
the norm kxk C0(B) ≡ sup 0≤t≤T kx(t)k B . The minimal σ-field making the
mapping x → x(t) measurable is B(C 0 (B)), the Borel σ-field on C 0 (B).
Further, Brownian motion in B induces a probability measure m B on (C 0 (B), B(C 0 (B))) which is mean-zero Gaussian. We will find a concrete form of m B . Let ~t = (t 1 , t 2 , . . . , t k ) be given with 0 = t 0 < t 1 < t 2 <
· · · < t k ≤ T . Let T ~ t : B k → B k be given by T ~ t (x 1 , x 2 , . . . , x k )
=
(t 1 − t 0 )
12x 1 , (t 1 − t 0 )
12x 1 + (t 2 − t 1 )
12x 2 , . . . ,
k
X
j=1
(t j − t j−1 )
12x j
. We define a set function ν ~ t on B(B k ) by
ν ~ t (B) =
k
Y
1
m
!
T ~ −1
t (B)
for B ∈ B(B k ). Then ν ~ t is a Borel measure. Let f ~ t : C 0 (B) → B k be the function defined by
f ~ t (x) = (x(t 1 ), x(t 2 ), . . . , x(t k )).
For Borel subsets B 1 , B 2 , . . . , B k of B, f ~ t −1 ( Q k
j=1 B j ) is called the I-set with respect to B 1 , B 2 , . . . , B k . Then the collection I of all I-sets is a semi-algebra. We define a set function m B on I by
m B
f ~ −1
t
k
Y
j=1
B j
= ν ~ t
k
Y
j=1
B j
.
Then m B is well-defined and countably additive on I. Using Carath´eod- ory extension process, we have a Borel measure m B on B(C 0 (B)).
Now, we introduce Wiener integration theorem without proof. For the proof see [16].
Theorem 1 (Wiener integration theorem). Let ~t = (t 1 , t 2 , . . . , t k ) be given with 0 = t 0 ≤ t 1 ≤ t 2 ≤ · · · ≤ t k ≤ T and let f : B k → C be a Borel measurable function. Then
Z
C
0(B)
f(x(t 1 ), x(t 2 ), . . . , x(t k )) dm B (x)
= ∗
Z
B
k(f ◦ T ~ t )(x 1 , x 2 , . . . , x k ) d
k
Y
j=1
m
(x 1 , x 2 , . . . , x k ),
where by = we mean that if either side exists, then both sides exist and ∗ they are equal.
Let τ : 0 = t 0 < t 1 < · · · < t k = T be a partition of [0, T ] and let x be in C 0 (B). Define the polygonal function [x] of x on [0, T ] by
(1) [x](t) =
k
X
j=1
χ (tj−1,t
j] (t)
x(t j−1 ) + t − t j−1
t j − t j−1 (x(t j ) − x(t j−1 ))
, where t ∈ [0, T ]. For each ~ξ = (ξ 1 , . . . , ξ k ) ∈ B k , let [~ ξ] be the polygonal function of ~ ξ on [0, T ] given by (1) with replacing x(t j ) by ξ j for j = 0, 1, . . . , k (ξ 0 = 0).
The following lemmas are useful to the next sections. For the detailed proof, see [3].
Lemma 2. If {x(t) : 0 ≤ t ≤ T } is the Wiener process on C 0 (B) × [0, T ], then {x(t) − [x](t) : t j−1 ≤ t ≤ t j }, where j = 1, . . . , k, are stochastically independent.
Lemma 3. Let F be defined and integrable on C 0 (B). Let X τ : C 0 (B) → B k be a random variable given by X τ (x) = (x(t 1 ), . . . , x(t k )).
Then for every Borel measurable subset B of B k , µ τ (B) ≡
Z
X
τ−1(B)
F (x) dm B (x) = Z
B
E [F (x − [x] + [~ξ])] dP Xτ(~ ξ), where P Xτ is the probability distribution of X τ on (B k , B(B k )).
is the probability distribution of X τ on (B k , B(B k )).
By the definition of conditional expectation and Lemma 3, we have E [F |X τ ](~ ξ ) = E[F (x − [x] + [~ξ])] for P Xτ-a.e. ~ ξ.
(2)
The function E[F |X τ ] is called the conditional Wiener integral of F given X τ . Note that, for the definition of the conditional Wiener integral, X τ
may be any random variable defined on C 0 (B). The equation (2) is called a simple formula for conditional Wiener integral on the space C 0 (B).
For λ > 0 and ~ ξ ∈ B k , suppose E[F (λ −12·)|X τ (λ −12·)](~ξ) exists. From (2) we have
·)](~ξ) exists. From (2) we have
E[F (λ −12·)|X τ (λ −12·)](~ξ) = E[F (λ −12(x − [x]) + [~ξ])]
·)](~ξ) = E[F (λ −12(x − [x]) + [~ξ])]
for a.e. ~ ξ ∈ B k . If, for ~ ξ ∈ B k , E[F (λ −12(x − [x]) + [~ξ])] has the analytic extension J λ (~ ξ) on C + ≡ {λ ∈ C : Re λ > 0}, then we write
J λ (~ ξ) = E anwλ[F |X τ ](~ ξ)
for λ ∈ C + . In this case, we call J λ (~ ξ) a version of conditional analytic Wiener integral of F given X τ .
For non-zero real q and ~ ξ ∈ B k , if the limit
λ→−iq lim E anw
λ[F |X τ ](~ ξ)
exists, where λ approaches to −iq through C + , then we write
λ→−iq lim E anw
λ[F |X τ ](~ ξ) = E anfq[F |X τ ](~ ξ).
In this case, we call E anfq[F |X τ ](~ ξ) a version of conditional analytic Feynman integral of F given X τ .
3. Conditional Fourier-Feynman transform of cylinder type functions
In this section, we define L p (1 < p ≤ ∞) conditional Fourier-Feynman transform over Wiener paths in abstract Wiener space and evaluate them for cylinder type functions. We also evaluate conditional convolution products for these type of functions.
A subset E of C 0 (B) is called a scale-invariant null set if m B (λE) = 0 for any λ > 0 and a property is said to hold s-a.e. if it holds except for a scale-invariant null set.
For a given real number p with 1 < p ≤ ∞, suppose p and p ′ are related by 1 p + p 1′ = 1 (possibly p ′ = 1 if p = ∞). Let G n and G be measurable functions such that, for each γ > 0,
n→∞ lim Z
C
0(B) |G n (γx) − G(γx)| p
′dm B (x) = 0.
Then we write
l.i.m.
n→∞ (w s p
′)(G n ) ≈ G
and call G the scale-invariant limit in the mean of order p ′ . A similar definition is understood when n is replaced by a continuously varying parameter.
Let H be a real separable infinite dimensional Hilbert space, let n be a positive integer and let {h 1 , . . . , h n } be an orthonormal set in H. For 1 ≤ p < ∞ let A (p) n,s be the space of all cylinder type functions F defined on C 0 (B) of the form
(3) F (x) = f ((h 1 , x(s)) ∼ , . . . , (h n , x(s)) ∼ )
for s-a.e. x in C 0 (B) where f : R n → R is in L p (R n ) and s ∈ (0, T ].
Let A (0) n,s be the space of all functions of the form (3) with f ∈ C 0 (R n ), the space of continuous functions on R n which vanish at infinity and let A (∞) n,s be the space of all functions of the form (3) with f ∈ L ∞ (R n ), the space of essentially bounded functions on R n . Note that, without loss of generality, we can take f to be Borel measurable.
For convenience, we let
Γ = t p∗− t p∗−1
−1
(t p∗− s)(s − t p∗−1 ) (4)
−1 ) (4)
for t p∗−1 < s < t p
∗ and φ λ (~u) = λ 2π
n2
exp
− λ 2
n
X
j=1
u 2 j
(λ
12∈ C + ) (5)
where ~u = (u 1 , . . . , u n ) ∈ R n and λ ∈ C ∼ + ≡ {λ ∈ C : Re λ ≥ 0} − {0}.
Also, we let for ~ ξ ∈ B k
~
w ξ ~ = (w ~ ξ1 , . . . , w ξn ~ ) = ((h 1 , [~ ξ](s)) ∼ , . . . , (h n , [~ ξ](s)) ∼ ) (6)
and
~
w y = (w y1 , . . . , w yn ) = ((h 1 , y(s)) ∼ , . . . , (h n , y(s)) ∼ ) (7)
for y in C 0 (B).
Definition 4. Let F be defined on C 0 (B) and let X τ be given as in Lemma 3. For λ ∈ C + and for s-a.e. ~ ξ ∈ B k let
T λ [F |X τ ](y, ~ ξ) = E anwλ[F (y + ·)|X τ ](~ ξ)
for s-a.e. y ∈ C 0 (B) if it exists. For non-zero real q and for s-a.e. ~ ξ ∈ B k , we define the L 1 conditional Fourier-Feynman transform T q (1) [F |X τ ] of F given X τ by the formula
T q (1) [F |X τ ](y, ~ ξ) = lim
λ→−iq T λ [F |X τ ](y, ~ ξ)
if it exists for s-a.e. y ∈ C 0 (B) and for 1 < p ≤ ∞ we define the L p conditional Fourier-Feynman transform T q (p) [F |X τ ] of F given X τ by the formula
T q (p) [F |X τ ](·, ~ξ) ≈ l.i.m.
λ→−iq (w p s
′)(T λ [F |X τ ](·, ~ξ)),
where λ approaches to −iq through C + .
Theorem 5. Let F ∈ A (p) n,s (1 ≤ p ≤ ∞) be given by (3). Let X τ be given as in Lemma 3 and let t p∗−1 < s ≤ t p
∗ for some p ∗ ∈ {1, . . . , k}.
Then, for any λ ∈ C + and for s-a.e. ~ ξ ∈ B k , T λ [F |X τ ](y, ~ ξ) exists for s-a.e. y ∈ C 0 (B) and T λ [F |X τ ](·, ~ξ) ∈ A (p) n,s . Moreover, when t p∗−1 <
s < t p∗, we have
T λ [F |X τ ](y, ~ ξ) = (φ λΓ ∗ f)( ~ w y + ~ w ξ ~ ) (8)
and, when s = t p∗, we have
T λ [F |X τ ](y, ~ ξ) = F (y + [~ ξ]) = f ( ~ w y + ~ w ~ ξ ), (9)
where Γ, φ λΓ , w ~ ~ ξ and w ~ y are given by (4), (5), (6) and (7), respectively.
Proof. Let t p∗−1 < s < t p
∗ and let λ > 0. Using the same method in the proof of Theorem 4.2 in [2], we have
E[F (y + λ −12(x − [x]) + [~ξ])] = (φ λΓ ∗ f)( ~ w y + ~ w ~ ξ )
for s-a.e. ~ ξ ∈ B k and for s-a.e. y ∈ C 0 (B). By Morera’s theorem, we have (8). The fact T λ [F |X τ ](·, ~ξ) ∈ A (p) n,s follows from Young’s inequality in [7, p.232].
When s = t p∗, the equation (9) follows easily since E[F (y + λ −12(x − [x]) +~[ξ])] = F (y + [~ ξ]) for λ > 0.
(x − [x]) +~[ξ])] = F (y + [~ ξ]) for λ > 0.
Theorem 6. For 1 ≤ p ≤ 2 let F ∈ A (p) n,s be given by (3) and let
1
p + p 1
′= 1(p ′ = ∞ if p = 1). Let X τ be given as in Lemma 3 and let t p∗−1 < s ≤ t p
∗ for some p ∗ ∈ {1, . . . , k}. Then, for any non-zero real q, and for s-a.e. ~ ξ ∈ B k , T q (p) [F |X τ ](y, ~ ξ ) exists for s-a.e. y ∈ C 0 (B).
Moreover, when t p∗−1 < s < t p
∗, we have
T q (p) [F |X τ ](y, ~ ξ) = (φ −iqΓ ∗ f)( ~ w y + ~ w ξ ~ )
with T q (p) [F |X τ ](·, ~ξ) ∈ A (p n,s′) (in fact, T q (1) [F |X τ ](·, ~ξ) ∈ A (0) n,s ) and, when s = t p
∗, we have
T q (p) [F |X τ ](y, ~ ξ) = F (y + [~ ξ]) = f ( ~ w y + ~ w ξ ~ ) (10)
with T q (p) [F |X τ ](·, ~ξ) ∈ A (p) n,s , where Γ, φ −iqΓ , w ~ ~ ξ and w ~ y are given by (4), (5), (6) and (7), respectively.
Proof. When p = 1, the result follows from Theorem 4.2 in [2].
Let 1 < p ≤ 2, t p∗−1 < s < t p
∗. Then, for γ > 0, for s-a.e. ~ ξ in B k and by Theorems 1, 5, we have
λ→−iq lim Z
C
0(B) |(φ λΓ ∗ f)(γ ~ w y + ~ w ~ ξ ) − (φ −iqΓ ∗ f)(γ ~ w y + ~ w ξ ~ )| p
′dm B (y)
= lim
λ→−iq
Z
B |(φ λΓ ∗ f)(γ √
s((h 1 , x 1 ) ∼ , . . . , (h n , x 1 ) ∼ ) + ~ w ~ ξ )
−(φ −iqΓ ∗ f)(γ √
s((h 1 , x 1 ) ∼ , . . . , (h n , x 1 ) ∼ ) + ~ w ~ ξ )| p′dm(x 1 )
≤ lim
λ→−iq
1
2πsγ 2
n2
k(φ λΓ ∗ f)(· + ~ w ξ ~ ) − (φ −iqΓ ∗ f)(· + ~ w ~ ξ )k p p′′
which converges to 0 as λ approaches to −iq through C + , by Lemmas 1.1, 1.2 in [10] and since (h j , ·) ∼ is normally distributed with mean 0, variance 1.
When s = t p∗, the result follows trivially by Theorem 5.
Remark 1. (10) holds for 1 ≤ p ≤ ∞.
Next we establish an inverse conditional Fourier-Feynman transform theorem for functions in A (p) n,s .
Theorem 7. For 1 ≤ p < ∞ let F ∈ A (p) n,s be given by (3) and let X τ be given as in Lemma 3. Let q be a non-zero real number and let w ~ y be given by (7). For (~ ξ 1 , ~ ξ 2 ) ∈ B k × B k and for y ∈ C 0 (B), let F ~ ξ
1
,~ ξ
2(y) = f ( ~ w y + ~ w 1 + ~ w 2 ), where ~ w 1 = (w 11 , . . . , w 1n ) = ((h 1 , [~ ξ 1 ](s)) ∼ , . . . , (h n , [~ ξ 1 ](s)) ∼ ), ~ w 2 = (w 21 , . . . , w 2n ) = ((h 1 , [~ ξ 2 ](s)) ∼ , . . . , (h n , [~ ξ 2 ](s)) ∼ ). Then we have
(i) for s-a.e. (~ ξ 1 , ~ ξ 2 ) ∈ B k × B k and for γ > 0, we have
λ→−iq lim Z
C
0(B) |T λ [T λ [F |X τ ](·, ~ ξ 1 )|X τ ](γy, ~ ξ 2 ) − F ξ ~
1,~ ξ
2(γy)| p dm B (y) = 0 and
(ii) for s-a.e. (~ ξ 1 , ~ ξ 2 ) ∈ B k × B k and for s-a.e. y ∈ C 0 (B), we have T λ [T λ [F |X τ ](·, ~ ξ 1 )|X τ ](y, ~ ξ 2 ) −→ F ~ ξ1,~ ξ
2(y),
where λ approaches to −iq through C + .
Proof. Let t p∗−1 < s < t p
∗ for some p ∗ ∈ {1, . . . , k} and let ~u =
(u 1 , . . . , u n ) ∈ R n . Then for λ ∈ C + , for s-a.e. (~ ξ 1 , ~ ξ 2 ) ∈ B k × B k and
for s-a.e. y ∈ C 0 (B), using the same method in the proof of Theorem 4.4 in [2], we have
T λ [T λ [F |X τ ](·, ~ ξ 1 )|X τ ](y, ~ ξ 2 )
= |λ| 2 Γ 4πReλ
n2
Z
R
nf (~u) exp
− |λ| 2 Γ 4Reλ
n
X
j=1
(u j − w yj − w 1j − w 2j ) 2
d~ u where Γ is given by (4). Let γ > 0 and for ~v = (v 1 , . . . , v n ) ∈ R n let
k ~ ξ
1
,~ ξ
2(λ, ~v)
= |λ| 2 Γ 4πReλ
n2Z
R
nf (~u) exp
− |λ| 2 Γ 4Reλ
n
X
j=1
(u j − v j − w 1j − w 2j ) 2
d~ u.
Then, by Wiener integration theorem(Theorem 1) and the change of variable theorem, we have
Z
C
0(B) |T λ [T λ [F |X τ ](·, ~ξ 1 )|X τ ](γy, ~ ξ 2 ) − F ~ ξ
1,~ ξ
2(γy)| p dm B (y)
= Z
B |k ~ ξ
1,~ ξ
2(λ, γ √
s((h 1 , x 1 ) ∼ , . . . , (h n , x 1 ) ∼ ))
−f(γ √
s((h 1 , x 1 ) ∼ , . . . , (h n , x 1 ) ∼ ) + ~ w 1 + ~ w 2 )| p dm(x 1 )
=
1
2πsγ 2
n2
Z
R
n|k ~ ξ1,~ ξ
2(λ, ~z) − f(~z + ~ w 1 + ~ w 2 )| p
× exp
− 1 2sγ 2
n
X
j=1
z j 2
d~ z
where ~z = (z 1 , . . . , z n ), since (h j , ·) ∼ is normally distributed with mean 0 and variance 1. Let ǫ = ( |λ| 2Reλ2 Γ )
12 and let ϕ ǫ (~u) = ǫ 1nφ 1 ( ~ u ǫ ), where φ 1 is given by (5). Then, R
R
nφ 1 (~u)d~u = 1 and hence in view of Theorem 1.18 in [17], we have
λ→−iq lim Z
C
0(B) |T λ [T λ [F |X τ ](·, ~ξ 1 )|X τ ](γy, ~ ξ 2 ) − F ~ ξ
1,~ ξ
2(γy)| p dm B (y)
≤ lim
λ→−iq
1
2πsγ 2
n2
k(f ∗ ϕ ǫ )(· + ~ w 1 + ~ w 2 ) − f(· + ~ w 1 + ~ w 2 )k p p
= 0
where λ approaches to −iq through C + . This proves (i). Also, (ii)
follows from Theorem 1.25 in [17].
Suppose that s = t p∗ for some p ∗ ∈ {1, . . . , k} and let γ > 0. Then, for λ ∈ C + , for s-a.e. (~ ξ 1 , ~ ξ 2 ) ∈ B k × B k and for s-a.e. y ∈ C 0 (B), we have
T λ [T λ [F |X τ ](·, ~ ξ 1 )|X τ ](γy, ~ ξ 2 ) = F ~ ξ1,~ ξ
2(γy)
by Theorem 5. Then (i) follows trivially and (ii) follows when γ = 1.
Remark 2. (ii) of Theorem 7 holds for p = ∞.
4. Conditional convolution product and conditional trans- formation of conditional convolution product
Now we define conditional convolution product and investigate re- lationships between conditional convolution product and conditional Fourier Feynman transform.
Definition 8. Let X τ be given as in Lemma 3 and let F, G be defined on C 0 (B). We define the conditional convolution product [(F ∗ G) λ |X τ ] of F, G given X τ by the formula, for s-a.e. ~ ξ ∈ B k
[(F ∗ G) λ |X τ ](y, ~ ξ)
=
E anwλ
F y + · 2
12G y − · 2
12X τ
(~ ξ ), λ ∈ C + ;
E anfq
F y + · 2
12G y − · 2
12X τ
(~ ξ), λ = −iq, q ∈ R − {0}
if they exist for s-a.e. y ∈ C 0 (B).
Using similar method in the proof Theorem 4.5 in [2], we have the following theorem.
Theorem 9. Let F 1 ∈ A (p n,s1) and F 2 ∈ A (p n,s
2) be given by (3) with replacing f by f 1 and f 2 , respectively, and let p 1
1
+ p 1′
1
= 1(1 ≤ p 1 , p 2 ≤
∞). Let X τ be given as in Lemma 3 and let t p∗−1 < s ≤ t p
∗for some p ∗ ∈ {1, . . . , k}. Then, for λ in C + and for s-a.e. ~ ξ ∈ B k , [(F 1 ∗ F 2 ) λ |X τ ](y, ~ ξ) exists for s-a.e. y ∈ C 0 (B). Moreover, when t p∗−1 < s < t p
∗, we have
−1 < s < t p
∗, we have
[(F 1 ∗ F 2 ) λ |X τ ](y, ~ ξ) = Z
R
nf 1
w ~ y + ~ w ~ ξ + ~l 2
12f 2
w ~ y − ~ w ξ ~ − ~l 2
12φ λΓ (~l)d~l
with [(F 1 ∗F 2 ) λ |X τ ](·, ~ξ) ∈ A (1) n,s if p 2 ≤ p ′ 1 and [(F 1 ∗F 2 ) λ |X τ ](·, ~ξ) ∈ A (p n,s2) if p 2 ≥ p ′ 1 , where Γ, φ λΓ , w ~ ~ ξ and w ~ y are given by (4), (5), (6) and (7), respectively, and when s = t p
∗, we have
[(F 1 ∗ F 2 ) λ |X τ ](y, ~ ξ) =
F 1 1
2
12(y + [~ ξ])
F 2 1
2
12(y − [~ξ])
. The following corollary follows from Theorem 9 immediately.
Corollary 10. Let F 1 , F 2 ∈ ∪ 1≤p≤∞ A (p) n,s . Let X τ be given as in Lemma 3 and let s = t p∗ for some p ∗ ∈ {1, . . . , k}. Then, for λ in C ∼ +
and for s-a.e. ~ ξ ∈ B k , [(F 1 ∗ F 2 ) λ |X τ ](y, ~ ξ ) exists for s-a.e. y ∈ C 0 (B) and it is given by
[(F 1 ∗ F 2 ) λ |X τ ](y, ~ ξ) =
F 1 1
2
12(y + [~ ξ])
F 2 1
2
12(y − [~ξ])
. Theorem 11. Let X τ be given as in Lemma 3 and let t p∗−1 < s < t p
∗
for some p ∗ ∈ {1, . . . , k}. For s-a.e. ~ξ in B k and for λ in C ∼ + , we have the followings:
1. if F 1 , F 2 ∈ A (1) n,s , then [(F 1 ∗ F 2 ) λ |X τ ](·, ~ξ) ∈ A (1) n,s , 2. if F 1 , F 2 ∈ A (2) n,s , then [(F 1 ∗ F 2 ) λ |X τ ](·, ~ξ) ∈ A (0) n,s ,
3. if F 1 ∈ A (1) n,s and F 2 ∈ A (2) n,s , then [(F 1 ∗ F 2 ) λ |X τ ](·, ~ξ) ∈ A (2) n,s , 4. if F 1 ∈ A (1) n,s and F 2 ∈ A (1) n,s ∩ A (2) n,s , then [(F 1 ∗ F 2 ) λ |X τ ](·, ~ξ) ∈
A (1) n,s ∩ A (2) n,s ,
5. if F 1 ∈ A (1) n,s and F 2 ∈ A (0) n,s , then [(F 1 ∗ F 2 ) λ |X τ ](·, ~ξ) ∈ A (0) n,s . Proof. Let F 1 , F 2 be given by (3) with replacing f by f 1 , f 2 , respec- tively. For λ in C + let
h(λ, ~u, ~ w ξ ~ ) = Z
R
nf 1
~ u + ~ w ξ ~ + ~l 2
12f 2
~ u − ~ w ξ ~ − ~l 2
12φ λΓ (~l)d~l where ~u in R n and Γ, φ λΓ , ~ w ~ ξ are given by (4), (5), (6), respectively.
1. By Theorem 9, it suffices to show that h(λ, ·, ~ w ~ ξ ) is in L 1 (R n ) for λ ∈ C ∼ + . But this fact follows from the following;
Z
R
n|h(λ, ~u, ~ w ξ ~ )|d~u
≤ |λ|Γ 2π
n2
Z
R
nZ
R
nf 1
~ u + ~ w ~ ξ + ~l 2
12f 2
~ u − ~ w ~ ξ − ~l 2
12d~ld~ u
= |λ|Γ 2π
n2
Z
R
nZ
R
nf 1
~v 1 + w ~ ξ ~ 2
12f 2
~v 2 − w ~ ~ ξ 2
12d~v 1 d~v 2
= |λ|Γ 2π
n2kf 1 k 1 kf 2 k 1 , where ~ u+~l
2
12= ~v 1 and ~ u−~l
2
12= ~v 2 , by the change of variable theorem.
2. Note that, for λ ∈ C ∼ + , h(λ, ·, ~ w ξ ~ ) is L ∞ (R n ) since
|h(λ, ~u, ~ w ~ ξ )| ≤ |λ|Γ 2π
n2Z
R
nf 1
~ u + ~ w ~ ξ + ~l 2
12f 2
~ u − ~ w ~ ξ − ~l 2
12d~l
≤ |λ|Γ π
n2
kf 1 k 2 kf 2 k 2
for ~u ∈ R n by H¨older inequality. Thus we have h(λ, ·, ~ w ~ ξ ) ∈ C 0 (R n ) from a standard argument.
3. By Theorem 9, it suffices to show that h(λ, ·, ~ w ~ ξ ) is in L 2 (R n ) for λ ∈ C ∼ + . But this fact follows from the following;
Z
R
n|h(λ, ~u, ~ w ~ ξ )| 2 d~ u
≤ |λ|Γ 2π
n Z
R
nZ
R
nf 1
~ u + ~ w ~ ξ + ~l 2
12f 2
~ u − ~ w ξ ~ − ~l 2
12d~l
2
d~ u
= |λ|Γ 2π
n Z
R
nZ
R
nf 1
~ u + ~ w ~ ξ + ~l 2
12f 2
~ u − ~ w ξ ~ − ~l 2
12d~l
×
Z
R
nf 1
~ u + ~ w ξ ~ + ~z 2
12f 2
~ u − ~ w ξ ~ − ~z 2
12d~ z
d~ u.
Let ~r = ~ u+~l
2
12and ~s = ~ u+~ z
2
12. Then we have Z
R
n|h(λ, ~u, ~ w ξ ~ )| 2 d~ u
≤ |λ|Γ 2π
n
2 n Z
R
n|f 1 (~r + 2 −12w ~ ~ ξ )|
Z
R
n|f 1 (~s + 2 −12w ~ ξ ~ )|
× Z
R
n|f 2 ( √
2~u − ~r − 2 −12w ~ ~ ξ )||f 2 ( √
2~u − ~s − 2 −12w ~ ξ ~ )|d~ud~sd~r
≤ |λ|Γ 2π
n
2
n2kf 1 k 2 1 kf 2 k 2 2
by H¨older inequality.
4. It follows from 1 and 3.
5. It follows immediately and it is trivial.
By Theorems 5 and 9, using similar method in the proof of Theorem 4.8 in [2], we have the following theorem.
Theorem 12. Let F 1 , F 2 ∈ ∪ 1≤p≤∞ A (p) n,s be given by (3) with replac- ing f by f 1 , f 2 , respectively, and let X τ be given as in Lemma 3. Then, for λ in C + and for s-a.e. (~ ξ 1 , ~ ξ 2 ) ∈ B k × B k , we have
T λ [[(F 1 ∗ F 2 ) λ |X τ ](·, ~ξ 1 )|X τ ](y, ~ ξ 2 )
=
T λ [F 1 |X τ ] y
2
12, ξ ~ 2 + ~ ξ 1 2
12T λ [F 2 |X τ ] y
2
12, ξ ~ 2 − ~ξ 1 2
12, for s-a.e. y ∈ C 0 (B).
The following theorem shows that the conditional Fourier-Feynman transform of conditional convolution product of some cylinder type func- tions is a product of conditional transforms. For convenience, if λ =
−iq(q ∈ R−{0}), then we denote [(F 1 ∗F 2 ) λ |X τ ](·, ~ξ 1 ) by [(F 1 ∗F 2 ) q |X τ ](·, ξ ~ 1 ) in the following theorem.
Theorem 13. Let X τ be given as in Lemma 3 and let q be a non-zero real number.
1. Let F 1 , F 2 ∈ A (1) n,s . Then, for s-a.e. (~ ξ 1 , ~ ξ 2 ) ∈ B k × B k , we have T q (1) [[(F 1 ∗ F 2 ) q |X τ ](·, ~ξ 1 )|X τ ](y, ~ ξ 2 )
=
T q (1) [F 1 |X τ ] y 2
12,
~ ξ 2 + ~ ξ 1 2
12T q (1) [F 2 |X τ ] y 2
12,
ξ ~ 2 − ~ξ 1
2
12for s-a.e. y ∈ C 0 (B).
2. Let F 1 ∈ A (1) n,s and F 2 ∈ A (2) n,s . Then, for s-a.e. (~ ξ 1 , ~ ξ 2 ) ∈ B k × B k , we have
T q (2) [[(F 1 ∗ F 2 ) q |X τ ](·, ~ξ 1 )|X τ ](y, ~ ξ 2 )
=
T q (1) [F 1 |X τ ] y 2
12,
~ ξ 2 + ~ ξ 1 2
12T q (2) [F 2 |X τ ] y 2
12,
ξ ~ 2 − ~ξ 1
2
12for s-a.e. y ∈ C 0 (B).
3. Let F 1 ∈ A (1) n,s and F 2 ∈ A (1) n,s ∩ A (2) n,s . Then, for s-a.e. (~ ξ 1 , ~ ξ 2 ) ∈ B k × B k , we have
T q (1) [[(F 1 ∗ F 2 ) q |X τ ](·, ~ξ 1 )|X τ ](y, ~ ξ 2 )
=
T q (1) [F 1 |X τ ] y
2
12, ~ ξ 2 + ~ ξ 1 2
12T q (1) [F 2 |X τ ] y
2
12, ξ ~ 2 − ~ξ 1 2
12and
T q (2) [[(F 1 ∗ F 2 ) q |X τ ](·, ~ξ 1 )|X τ ](y, ~ ξ 2 )
=
T q (1) [F 1 |X τ ] y
2
12, ~ ξ 2 + ~ ξ 1 2
12T q (2) [F 2 |X τ ] y
2
12, ξ ~ 2 − ~ξ 1
2
12for s-a.e. y ∈ C 0 (B).
Proof. The results follow from Corollary 10, Theorems 6, 11 and 12.
5. Stability theories
Let H be an infinite dimensional separable real Hilbert space and let
∆ n = {(s 1 , s 2 , . . . , s n ) ∈ [0, T ] n : 0 = s 0 < s 1 < s 2 < · · · < s n ≤ T } for any fixed n ∈ N.
Let M
′′n = M′′n (∆ n × H n ) be the class of all complex Borel measures on ∆ n × H n and let kµk = var µ, the total variation of µ in M′′n . Let S n,B ′′ = S n,B ′′ (∆ n × H n ) be the space of functions of the form
n . Let S n,B ′′ = S n,B ′′ (∆ n × H n ) be the space of functions of the form
F n (x) = Z
∆
n×H
nexp
i
n
X
j=1
(h j , x(s j )) ∼
dµ Fn(~s,~h) (11)
for s-a.e. x ∈ C 0 (B), where ~s = (s 1 , . . . , s n ), ~h = (h 1 , . . . , h n ) and µ Fn ∈ M
′′n . Here we take kF n k
′′n = inf{kµ F
nk}, where the infimum is taken over all µ Fn’s so that F n and µ Fn are related by (11).
are related by (11).
Let M ′′ = M ′′ (P ∆ n × H n ) be the class of all sequences {µ n } of measures such that each µ n ∈ M
′′n and P ∞
n=1 kµ n k < ∞. Let S B ′′ = S B ′′ (P ∆ n × H n ) be the space of functions of the form
F (x) =
∞
X
n=1
F n (x),
(12)
s -a.e. x ∈ C 0 (B), where each F n ∈ S n,B ′′ and P ∞
n=1 kF n k′′n < ∞. The norm of F is defined by kF k′′ = inf{ P ∞
= inf{ P ∞
n=1 kF n k′′n }, where the infimum is taken over all representations of F given by (12).
Note that if n and l are positive integers then S n,B ′′ ⊂ S n+l,B ′′ and S n,B ′′ ⊂ S B ′′ for all n ∈ N. Moreover we can show that S n,B ′′ is a Banach space and S B ′′ is a Banach algebra.
Theorem 14. Let F n ∈ S n,B ′′ be given by (11) and let X τ be given as in Lemma 3. Let q ∈ R − {0} and 1 ≤ p ≤ ∞. Then, for s-a.e. ~ξ in B k , T q (p) [F n |X τ ](y, ~ ξ ) exists for s-a.e. y ∈ C 0 (B) and it is given by
T q (p) [F n |X τ ](y, ~ ξ) (13)
= X
j
1+···+j
k=n
Z
∆
′n;j1,...,jk×H
nH n (y, ~ ξ, ~s, ~h)G n (−iq, ~τ, ~s,~h)dµ Fn(~s,~h)
where for j 1 + · · · + j k = n
~s = (s 1,1 , . . . , s 1,j1, s 2,1 , . . . , s 2,j2, . . . , s k,1 , . . . , s k,jk);
, . . . , s k,1 , . . . , s k,jk);
(14)
∆ ′ n;j1,...,j
k
(15)
= {~s : 0 = s 1,0 < s 1,1 < · · · < s 1,j1 ≤ t 1 < s 2,1 < · · · < s 2,j2
≤ t 2 < · · · ≤ t k−1 < s k,1 < · · · < s k,jk ≤ t k = T },
(16) ~h = (h 1,1 , . . . , h 1,j1, h 2,1 , . . . , h 2,j2, . . . , h k,1 , . . . , h k,jk);
, . . . , h k,1 , . . . , h k,jk);
(17) H n (y, ~ ξ, ~s, ~h) = exp
i
k
X
α=1 j
αX
β=1
(h α,β , y(s α,β ) + [~ ξ](s α,β )) ∼
,
t 0 = s 1,0 = 0, t α = s α+1,0 = s α,jα+1 (α = 1, . . . , k − 1), (18)
s k,jk+1 = t k = T ;
(19) l α,v = s α,v − s α,v−1 , for α = 1, . . . , k; for v = 1, . . . , j α + 1,
~
τ = (t 1 , . . . , t k );
(20)
G n (λ, ~τ, ~s,~h) (21)
= exp
− 1 2λ
k
X
α=1 j
α+1
X
v=1
l α,v
v−1
X
β=1
t α−1 − s α,β t α − t α−1 h α,β
+
j
αX
β=v
t α − s α,β
t α − t α−1
h α,β
2
with λ ∈ C ∼ + .
Proof. For λ > 0, for s-a.e. ~ ξ in B k and for s-a.e. y in C 0 (B), we have E[F n (y + λ −12(x − [x]) + [~ξ])]
= Z
∆
n×H
nexp
i
n
X
j=1
(h j , y(s j ) + [~ ξ](s j )) ∼
Z
C
0(B)
exp
iλ −12
n
X
j=1
(h j ,
x(s j ) − [x](s j )) ∼
dm B (x)dµ Fn(~s,~h)
by Fubini theorem where ~s = (s 1 , . . . , s n ) and ~h = (h 1 , . . . , h n ). Let ~s,
∆ ′ n;j
1
,...,j
k, ~h and H n be given by (14), (15), (16) and (17), respectively.
Then, by Lemma 2, we have
E[F n (y + λ −12(x − [x]) + [~ξ])]
= X
j
1+···+j
k=n
Z
∆
′n;j1,...,jk×H
nH n (y, ~ ξ, ~s, ~h)
k
Y
α=1
Z
B
jα+1exp
iλ −12
j
αX
β=1
h α,β ,
β
X
v=1
pl α,v x α,v − s α,β − t α−1
t α − t α−1 jα+1
X
v=1
pl α,v x α,v
∼
dm jα+1 (~x α )
dµ Fn(~s,~h)
by Wiener integration theorem (Theorem 1) where ~x α = (x α,1 , . . . , x α,jα+1 ) and l α,v is given by (19) with (18). Let ~τ and G n be given by (20) and (21), respectively. Then we have
E[F n (y + λ −12(x − [x]) + [~ξ])]
= X
j
1+···+j
k=n
Z
∆
′n;j1,...,jk×H
nH n (y, ~ ξ, ~s, ~h)
k
Y
α=1
Z
B
jα+1exp
iλ −12
j
α+1
X
v=1
pl α,v
v−1
X
β=1
t α−1 − s α,β t α − t α−1
h α,β +
j
αX
β=v
t α − s α,β t α − t α−1
h α,β
, x α,v
∼
dm jα+1 (~x α )
dµ Fn(~s,~h)
= X
j
1+···+j
k=n
Z
∆
′n;j1,...,jk×H
nH n (y, ~ ξ, ~s, ~h)G n (λ, ~τ, ~s,~h)dµ Fn(~s,~h) since (h, ·) ∼ is normally distributed with mean 0 and variance |h| 2 (h 6=
0). By Morera’s theorem, we have T λ [F n |X τ ](y, ~ ξ)
= X
j
1+···+j
k=n
Z
∆
′n;j1,...,jk×H
nH n (y, ~ ξ, ~s, ~h)G n (λ, ~τ, ~s,~h)dµ Fn(~s,~h) for λ ∈ C + . For 1 ≤ p ≤ ∞ let T q (p) [F n |X τ ](y, ~ ξ) be given by (13). When p = 1 we have
|T λ [F n |X τ ](y, ~ ξ ) − T q (1) [F n |X τ ](y, ~ ξ )|
≤ X
j
1+···+j
k=n
Z
∆
′n;j1,...,jk×H
n|G n (λ, ~τ, ~s,~h) − G n (−iq, ~τ, ~s,~h)|
d kµ Fnk(~s,~h)
and when 1 < p ≤ ∞, for 1 p + p 1′ = 1 and γ > 0, we have Z
C
0(B) |T λ [F n |X τ ](γy, ~ ξ ) − T q (p) [F n |X τ ](γy, ~ ξ )| p
′dm B (y)
≤
X
j
1+···+j
k=n
Z
∆
′n;j1,...,jk×H
n|G n (λ, ~τ, ~s,~h) − G n (−iq, ~τ, ~s,~h)|
d kµ Fnk(~s,~h)
p′
.
Letting λ → −iq through C + , we have the results by the dominated convergence theorem.
Theorem 15. Let F ∈ S B ′′ be given by (12) and let X τ be given as in Lemma 3. Let q ∈ R − {0} and 1 ≤ p ≤ ∞. Then, for s-a.e. ~ξ in B k , T q (p) [F |X τ ](y, ~ ξ ) exists for s-a.e. y ∈ C 0 (B) and it is given by
T q (p) [F |X τ ](y, ~ ξ) =
∞
X
n=1
T q (p) [F n |X τ ](y, ~ ξ)
(22)
where T q (p) [F n |X τ ] is given by (13) in Theorem 14.
Proof. Without loss of generality, we can assume P ∞
n=1 kµ F
nk < ∞ where F n and µ Fn are related by (11). For λ > 0, for s-a.e. ~ ξ ∈ B k and for s-a.e. y ∈ C 0 (B), we have
T λ [F |X τ ](y, ~ ξ) =
∞
X
n=1
T λ [F n |X τ ](y, ~ ξ) (23)
by Theorem 14 and the dominated convergence theorem. Since P ∞
n=1 T λ [F n |X τ ](y, ~ ξ) converges uniformly on C + by Theorem 14, we have (23) for all λ ∈ C + . For 1 ≤ p ≤ ∞ let T q (p) [F |X τ ](y, ~ ξ) be given by (22). When p = 1 we have
|T λ [F |X τ ](y, ~ ξ ) − T q (1) [F |X τ ](y, ~ ξ )|
≤
∞
X
n=1
X
j
1+···+j
k=n
Z
∆
′n;j1,...,jk×H
n|G n (λ, ~τ, ~s,~h) − G n (−iq, ~τ, ~s,~h)|
d kµ Fnk(~s,~h)
and when 1 < p ≤ ∞, for 1 p + p 1′ = 1 and γ > 0, we have Z
C
0(B) |T λ [F |X τ ](γy, ~ ξ ) − T q (p) [F |X τ ](γy, ~ ξ )| p
′dm B (y)
≤
∞
X
n=1
X
j
1+···+j
k=n
Z
∆
′n;j1,...,jk×H
n|G n (λ, ~τ, ~s,~h) − G n (−iq, ~τ, ~s,~h)|
d kµ Fnk(~s,~h)
p′
.
Letting λ → −iq through C + , we have the results by the dominated convergence theorem.
Let M(H) be the class of all complex Borel measures on H and let G be the set of all C-valued functions θ on [0, T ] × B which have the following form
θ(s, y) = Z
H exp{i(h, y) ∼ }dσ s (h) (24)
where {σ s : s ∈ [0, T ]} is the family from M(H) satisfying the following conditions;
1. for each Borel subset E of H, σ s (E) is a Borel measurable function
of s on [0, T ],
2. kσ s k ∈ L 1 ([0, T ]).
Let θ ∈ G be given by (24) and for s-a.e. x in C 0 (B) let F n (x) =
Z T 0
θ(s, x(s))ds
n (25)
and
F (x) = exp
Z T 0
θ(s, x(s))ds
(26)
where n is any fixed natural number. For any Borel measurable subset E of (0, T ] × H, let
µ(E) = Z T
0
σ s (E (s) )ds,
where E (s) = {h ∈ H : (s, h) ∈ E}. By unsymmetric Fubini theorem ([8]), we have, for s-a.e. x in C 0 (B),
F 1 (x) = Z T
0
θ(s, x(s))ds = Z T
0
Z
H exp{i(h, x(s)) ∼ }dσ s (h)ds
= Z
(0,T ]×H exp{i(h, x(s)) ∼ }dµ(s, h), and kµk ≤ R T
0 kσ s kds, so that F 1 ∈ S 1,B ′′ ⊂ S B ′′ . Moreover, we can show that F n ∈ S n,B ′′ for each n ∈ N. Thus we have the following theorems by Theorems 14 and 15.
Theorem 16. Let F n be given by (25) and let X τ be given as in Lemma 3. Let q ∈ R − {0} and 1 ≤ p ≤ ∞. For any Borel subset E of
∆ n × H n let
µ ′ Fn(E) = n!
Z
∆
nZ
H
nχ E (~s,~h)d
n
Y
j=1
σ sj
(~h)d~s
where ~s = (s 1 , . . . , s n ). Then, for s-a.e. ~ ξ in B k , T q (p) [F n |X τ ](y, ~ ξ) exists for s-a.e. y ∈ C 0 (B) and it is given by (13) with replacing µ Fn by µ ′ F
n
. Theorem 17. Let F be given by (26) and let X τ be given as in Lemma 3. Let q ∈ R − {0} and 1 ≤ p ≤ ∞. Then, for s-a.e. ~ξ in B k , T q (p) [F |X τ ](y, ~ ξ ) exists for s-a.e. y ∈ C 0 (B) and it is given by
T q (p) [F |X τ ](y, ~ ξ) = 1 +
∞
X
n=1
1
n! T q (p) [F n |X τ ](y, ~ ξ)
where T q (p) [F n |X τ ] is given as in Theorem 16.
Let F(B) be the class of all functions of the form φ(x 1 ) =
Z
H exp{i(h, x 1 ) ∼ }dν(h) (27)
for s-a.e. x 1 in B where ν ∈ M(H). For s-a.e. x in C 0 (B) let K n (x) = F n (x)φ(x(T )) and K(x) = F (x)φ(x(T )) (28)
where F n and F are given by (25) and (26), respectively. Then for λ > 0, x, y ∈ C 0 (B) and ~ ξ = (ξ 1 , . . . , ξ k ) ∈ B k , we have
|φ(y(T ) + λ −12(x(T ) − [x](T )) + [~ξ](T ))|
(29)
= |φ(y(T ) + ξ k )| ≤ kνk.
Thus we have the following theorem.
Theorem 18. Let K n , K be given by (28) and let X τ be given as in Lemma 3. Let q ∈ R − {0} and 1 ≤ p ≤ ∞. Then, for s-a.e. ~ξ in B k , both T q (p) [K n |X τ ](y, ~ ξ) and T q (p) [K|X τ ](y, ~ ξ ) exist for s-a.e. y ∈ C 0 (B), and they are given by
T q (p) [K n |X τ ](y, ~ ξ) = T q (p) [F n |X τ ](y, ~ ξ)φ(y(T ) + ξ k ) and
T q (p) [K|X τ ](y, ~ ξ) = T q (p) [F |X τ ](y, ~ ξ)φ(y(T ) + ξ k )
= φ(y(T ) + ξ k ) +
∞
X
n=1
1
n! T q (p) [K n |X τ ](y, ~ ξ), where T q (p) [F n |X τ ] and T q (p) [F |X τ ] are given as in Theorems 16 and 17, respectively.
Let ζ be a complex-valued Borel measure on [0, T ]. Then ζ = µ + ν d
can be decomposed uniquely into the sum of a continuous measure µ and a discrete measure ν d ([6, p.142]). Let δ τj denote the Dirac measure with total mass one concentrated at τ j .
Let G ∗ be the set of all C-valued functions θ on [0, T ] × B which have the form (24) where {σ s : s ∈ [0, T ]} is the family from M(H) satisfying the following conditions;
1. for each Borel subset E of H, σ s (E) is a Borel measurable function of s on [0, T ],
2. kσ s k ∈ L 1 ([0, T ], B([0, T ]), kζk).
In convenience, let
ζ = µ +
r
X
j=1
w j δ τj
(30)
where 0 ≤ τ 1 < · · · < τ r ≤ T and the w j ’s are in C for j = 1, . . . , r(∈ N), and let θ ∈ G ∗ be given by (24). For s-a.e. x in C 0 (B) let
F n (x) =
Z T 0
θ(s, x(s))dζ(s)
n
(31) and
F (x) = exp
Z T 0
θ(s, x(s))dζ(s)
(32) .
Theorem 19. Let F n be given by (31) and let X τ be given as in Lemma 3. Let q ∈ R − {0} and 1 ≤ p ≤ ∞. By reordering τ j ’s, t j ’s and renaming τ j ’s by τ α,u ’s (α = 1, . . . , k; u = 1, . . . , r α ) let 0 ≤ τ 1,1 <
τ 1,2 < · · · < τ 1,r1 ≤ t 1 < τ 2,1 < · · · < τ 2,r2 ≤ t 2 < · · · ≤ t k−1 < τ k,1 <
≤ t 2 < · · · ≤ t k−1 < τ k,1 <
· · · < τ k,rk ≤ t k = T , where r 1 + · · · + r k = r. Then, for s-a.e. ~ ξ in B k , T q (p) [F n |X τ ](y, ~ ξ ) exists for s-a.e. y ∈ C 0 (B) and it is given by
T q (p) [F n |X τ ](y, ~ ξ) (33)
= n! X
q
1+···+q
k=n k
Y
α=1
X
l
0+l
1+···+l
rα=q
αL(q α )W (q α )
X
j
1+···+j
rα+1=l
0Z
∆
l0;j1,...,jrα+1Z
H
qαH qα(y, ~s,~h,~h ′ , ~ ξ, ~ τ α )G qα(−iq, ~s,~h,~h ′ , ~ τ α )
(−iq, ~s,~h,~h ′ , ~ τ α )
d(σ ~ s × σ ~ τα)(~h, ~h ′ )dµ l0(~s)
(~s)
where for q 1 + · · ·+q k = n and for α = 1, . . . , k; for l 0 + l 1 + · · ·+l rα = q α L(q α ) = 1
l 1 ! · · · l rα! (34)
and
w α,u = w r1+···+r
α−1+u (u = 1, . . . , r α );
(35)
W (q α ) =
r
αY
u=1
w l α,uu ;
(36)
for j 1 + · · · + j rα+1 = l 0
~s = (s 0,1 , . . . , s 0,j1, s 1,1 , . . . , s 1,j2, . . . , s rα,1 , . . . , s r
α,j
rα+1);
, . . . , s rα,1 , . . . , s r
α,j
rα+1);
(37)
∆ l0;j
1,...,j
rα+1 = {~s : 0 ≤ t α−1 ≤ s 0,1 ≤ · · · ≤ s 0,j1 ≤ τ α,1 < s 1,1 <
≤ τ α,1 < s 1,1 <
(38)
· · · < s 1,j2 < τ α,2 < · · · < τ α,rα ≤ s rα,1 ≤ · · · ≤ s r
α,j
rα+1 ≤ t α ≤ T },
≤ s rα,1 ≤ · · · ≤ s r
α,j
rα+1 ≤ t α ≤ T },
~h = (h 0,1 , . . . , h 0,j1, h 1,1 , . . . , h 1,j2, . . . , h rα,1 , . . . , h r
α,j
rα+1) (39)
, . . . , h rα,1 , . . . , h r
α,j
rα+1) (39)
and
~
τ α = (τ α,1 , . . . , τ α,rα);
(40)
σ ~ s =
r
αY
u=0 j
u+1Y
v=1
σ su,v, σ ~ τα =
=
r
αY
u=1 l
uY
1
σ τα,u
(41)
and
~h ′ = (h ′ 1,1 , . . . , h ′ 1,l
1
, h ′ 2,1 , . . . , h ′ 2,l
2
, . . . , h ′ rα,1 , . . . , h ′ r
α