Abstract
For Hölder continuous functions W(t, x) and \(\varphi _t\), we define nonlinear integral \(\int _a^b W(dt, \varphi _t)\) via fractional calculus. This nonlinear integral arises naturally in the Feynman-Kac formula for stochastic heat equations with random coefficients (Hu and Lê, Nonlinear Young integrals and differential systems in Hölder media. Trans. Am. Math. Soc. (in press)). We also define iterated nonlinear integrals.
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1 Introduction
Let \(\{\varphi _t\,, t\ge 0\}\) be a Hölder continuous function and let \(\{W(t,x), t\ge 0\,, x\in \mathbb {R}^d\}\) be another jointly Hölder continuous function of several variables (see (10) for the precise statement about the assumption on W). The aim of this paper is to define the nonlinear Young integral \(\int _a^b W(dt, \varphi _t)\) by using fractional calculus.
This paper can be considered as supplementary to authors’ recent paper [5], where the nonlinear Young integral is introduced to establish the Feynman-Kac formula for general stochastic partial differential equations with random coefficients, namely,
where W is a Hölder continuous function of several variables (which can be a sample path of a Gaussian random field) and
with the coefficients \(a_{ij}\) and \(b_i\) depending on W. The terminal condition for the Eq. (1) is \(u(T, x)=u_T(x)\) for some given function \(u_T(x)\).
To motivate our study of the nonlinear Young integral, let us recall a basic result in [5] on the Feynman-Kac formula: Let \({\sigma }(t,x)=({\sigma }_{ij}(t,x,W))_{1\le i,j\le d}\) satisfy \(a(t,x,W)={\sigma }(t,x,W) {\sigma }(t,x,W)^T\) (we omit the explicit dependence of \({\sigma }\) on W). Consider the following stochastic differential equation
where \((B_t\,, 0\le t\le T)\) is a standard Brownian motion and \(\delta B_t\) denotes the Itô differential. Then it is proved in [5] that under some conditions b and \({\sigma }\) and W (which are verified for certain Gaussian random field W), the nonlinear integral \(\int _r^T W(d s, X_s^{r,x})\) is well-defined and exponentially integrable and \(u(r,x)=\mathbb {E}^B \left\{ u_T(X_T^{r,x})\exp \left[ \int _r^T W(d s, X_s^{r,x})\right] \right\} \) is a Feynman-Kac solution to (1) with \(u(T, x)=u_T(x)\). One of the main tasks in that paper is the study of the nonlinear Young integral \(\int _r^T W(d s, X_s^{r,x})\). To this end we used the Riemann sum approximation and the sewing lemma of [2]. In this paper, we shall study the nonlinear Young integral \(\int _a^b W(dt, \varphi _t)\) by means of fractional calculus. This approach may provide more detailed properties of the solutions to the equations (see [6, 7]).
Under certain conditions, we shall prove that the two nonlinear Young integrals, defined by Riemann sums (through sewing lemma) or by fractional calculus, are the same (see Proposition 2).
To expand the solution of a (nonlinear) differential equation with explicit remainder term we need to define (iterated) multiple integrals (see [3]). We shall also give a definition of the iterated nonlinear Young integrals. Some elementary estimates are also obtained.
The paper is organized as follows. Section 2 briefly recalls some preliminary material on fractional calculus that are needed later. Section 3 deals with the nonlinear Young integrals and Sect. 4 is concerned with iterated nonlinear Young integrals.
2 Fractional Integrals and Derivatives
In this section we recall some results from fractional calculus.
Let \(-\infty <a<b<\infty \), \({\alpha }>0\) and \(p\ge 1\) be real numbers. Denote by \(L^p(a, b)\) the space of all measurable functions on (a, b) such that
Denote by C([a, b]) the space of continuous functions on [a, b]. Let \(f\in L^{1}\left( [a,b]\right) \). The left-sided fractional Riemann-Liouville integral \(I_{a+}^{\alpha }f \) is defined as
and the right-sided fractional Riemann-Liouville integral \(I_{b-}^{\alpha }f \) is defined as
where \(\left( -1\right) ^{-\alpha }=e^{-i\pi \alpha }\) and \( \varGamma \left( \alpha \right) =\int _{0}^{\infty }r^{\alpha -1}e^{-r}d r\) is the Euler gamma function. Let \(I_{a+}^{\alpha }(L^{p})\) (resp. \( I_{b-}^{\alpha }(L^{p})\)) be the image of \(L^{p}(a,b)\) by the operator \( I_{a+}^{\alpha }\) (resp. \(I_{b-}^{\alpha }\)). If \(f\in I_{a+}^{\alpha }\left( L^{p}\right) \ \) (resp. \(f\in I_{b-}^{\alpha }\left( L^{p}\right) \)) and \(0<\alpha <1\), then the (left-sided or right-sided) Weyl derivatives are defined (respectively) as
and
where \(a\le t\le b\) (the convergence of the integrals at the singularity \( s=t\) holds point-wise for almost all \(t\in \left( a,b\right) \) if \(p=1\) and moreover in \(L^{p}\)-sense if \(1<p<\infty \)).
It is clear that if f is Hölder continuous of order \(\mu >{\alpha }\), then the two Weyl derivatives exist.
For any \({\beta }\in (0,1)\), we denote by \(C^{{\beta }}([a,b])\) the space of \( {\beta }\)-Hölder continuous functions on the interval [a, b]. We will make use of the notation
(which is a seminorm) and
where \(f:\mathbb {R} \rightarrow \mathbb {R}\) is a given continuous function.
It is well-known that \(C^{{\beta }}([a,b])\) with the Hölder norm \( \Vert f\Vert _{\beta ;a,b } +\Vert f\Vert _{\infty ;a,b }\) is a Banach space. However, it is not separable.
Using the fractional calculus, we have (see [9] and also [3])
Proposition 1
Let \(0<{\alpha }<1\). If f and g are continuously differentiable functions on the interval [a, b], then
where \(g_{b-}\left( t\right) =g\left( t\right) -g\left( b\right) \).
In what follows \(\kappa \) denotes a universal generic constant depending only on \({\lambda }, \tau , {\alpha }\) and independent of W, \(\varphi \) and a, b. The value of \(\kappa \) may vary from occurrence to occurrence.
For two function \(f, g:[a, b]\rightarrow \mathbb {R}\), we can define the Riemann-Stieltjes integral \(\int _a^b f(t) dg(t)\). Here we recall a result which is well-known (see for example [3, 9] or [6, 7]).
Lemma 1
Let f and g be Hölder continuous functions of orders \(\alpha \) and \(\beta \) respectively. Suppose that \(\alpha +\beta >1\). Then the Riemann-Stieltjes integral \( \int _a^bf(t)dg(t)\) exists and for any \({\gamma }\in (1- \beta ,\alpha )\), we have
Moreover, there is a constant \(\kappa \) such that
Proof
We refer to [9] or [3] for a proof of (8). We shall outline a proof of (9). Let \(\gamma \) be such that \(\alpha >\gamma >1-\beta \). Applying fractional integration by parts formula (8), we obtain
From (5) and (6) it is easy to see that
and
Therefore
The integrals on the right hand side can be computed by making the substitution \(t=b-(b-a)s\). Hence we derive (9).
We also need the following lemma in the proofs of our main results.
Lemma 2
Let \( f(s,t), a\le s< t\le b\) be a measurable function of s and t such that
Then
Proof
An application of Fubini’s theorem yields
which is the lemma.
3 Nonlinear Integral
In this section we shall use fractional calculus to define the (pathwise) nonlinear integral \(\int _{a}^{b}W(d t,\varphi _{t})\). This method only relies on regularity of the sample paths of W and \(\varphi \). More precisely, it is applicable to stochastic processes with Hölder continuous sample paths.
Another advantage of this approach is that in the theory of stochastic processes it is usually difficult to obtain almost sure type of results. If the sample paths of the process is Hölder continuous, then one can apply this approach to each sample path and almost surely results are then automatic.
In what follows, we shall use W to denote a deterministic function \(W: \mathbb {R}\times \mathbb {R}^d\rightarrow \mathbb {R}^d\). We make the following assumption on the regularity of W:
- \(\varvec{(W)}\) :
-
There are constants \(\tau , {\lambda }\in (0, 1]\) such that for all finite \(a<b\) and for all compact sets K of \(\mathbb {R}^d\), the seminorm
$$\begin{aligned}&\Vert W\Vert _{ \tau , {\lambda }; a, b, K } \nonumber \\ :&=\sup _{\begin{array}{c} a\le s<t\le b\\ x,y\in K ;x\ne y \end{array}}\frac{ \left| W(s,x)-W(t,x)-W(s,y) + W(t,y)\right| }{ |t-s|^{\tau }|x-y|^{\lambda }}\nonumber \\&\qquad + \sup _{\begin{array}{c} a\le s<t\le b\\ x\in K \end{array}}\frac{ \left| W(s,x)-W(t,x)\right| }{ |t-s|^{\tau }}+\sup _{\begin{array}{c} a\le t\le b\\ x,y\in K;x\ne y \end{array}}\frac{ \left| W(t,y) - W(t,x)\right| }{ |x-y|^{\lambda }}, \end{aligned}$$(10)is finite.
About the function \(\varphi \), we assume
- \(\varvec{(\phi )}\) :
-
\(\varphi \) is locally Hölder continuous of order \({\gamma }\in (0, 1]\). That is, the seminorm
$$ \Vert \varphi \Vert _{{\gamma }; a, b}=\sup _{a\le s<t\le b}\frac{|\varphi (t)-\varphi (s)|}{|t-s|^{\gamma }}\,, $$is finite for every \(a<b\).
Among the three terms appearing in \(\varvec{(W)}\), we will pay special attention to the first term. Thus, we denote
If a, b is clear from the context, we frequently omit the dependence on a, b. In addition, throughout the paper, the compact set K can be chosen to be any compact set containing the image of \(\varphi \) on the interval of integration. Thus we omit the dependence on K as well. For instance, \(\Vert W\Vert _{ \tau , {\lambda }}\) is an abbreviation for \(\Vert W\Vert _{ \tau , {\lambda }; a,b, K}\), \(\Vert \varphi \Vert _{\gamma }\) is an abbreviation for \(\Vert \varphi \Vert _{\gamma ;a,b}\) and so on. We shall assume that a and b are finite. Thus it is easy to see that for any \(c\in [a, b]\)
Thus assumption \(\varvec{(\phi )}\) also implies that
Remark 1
Given a stochastic process indexed by (t, x), it is possible to obtain almost sure regularity of the type (10) by a multiparameter Garsia-Rodemich-Rumsey inequality. Indeed, this has been explored in [4], see also the last section of [5].
One of our main results in this section is to define \(\int _{a}^{b}W(d t,\varphi _{t})\) under the condition \({\lambda }{\gamma }+\tau >1\) through a fractional integration by parts technique. The following definition is motivated from Lemma 1.
Definition 1
We define
whenever the right hand side makes sense.
Remark 2
Assume \(d=1\). Let \(W(t, x)=g(t) x\) be of the product form and let \(\varphi (t)=f(t)\), where g is a Hölder continuous function of exponent \(\tau \) and f is a Hölder continuous function of exponent \({\lambda }\). If \(1-\tau <{\alpha }<{\lambda }\), then
Thus from (8), \(\int _a^b W(d t, \varphi _t)\) is an extension of the classical Young integral \(\int _a^b f(t) dg(t)\) (see [3, 8, 9]). For general d, if \(W(t,x)=\sum _{i=1}^d g_i(t)x_i\) and \(\varphi _i(t)=f_i(t)\), then it is easy to see that \(\int _a^b W(d t, \varphi _t)=\displaystyle \sum _{i=1}^d \int _a^b f_i(t) dg_i(t)\).
The following result clarifies the context in which Definition 1 is justified.
Theorem 1
Assume the conditions \(\varvec{(W)}\) and \(\varvec{(\phi )}\) are satisfied. In addition, we suppose that \({\lambda }{\gamma }+\tau >1\). Let \(\alpha \in (1- \tau ,\lambda \tau )\). Then the right hand side of (11) is finite and is independent of \(\alpha \in (1-\tau , {\lambda })\). As a consequence, we have
where \(W_{b-}\left( t,x\right) =W\left( t,x\right) -W\left( b,x\right) \). Moreover, there is a universal constant \(\kappa \) depending only on \(\tau , {\lambda }\) and \({\alpha }\), but independent W, \(\varphi \) and a, b such that
where \(\Vert W\Vert _{\tau , {\lambda }\,; a, b}=\Vert W\Vert _{\tau , {\lambda }\,; a, b, K}\) and K is the closure of the image of \((\varphi _t, a\le t\le b)\).
Proof
We denote \(\Vert W\Vert =\Vert W\Vert _{\tau ,\lambda ;a,b}\). First by the definitions of fractional derivatives (5) and (6), we have
and
Thus the right hand side of (11) is
The condition \(\varvec{(W)}\) implies
Similarly, we also have
The assumptions \(\varvec{(W)}\) and \(\varvec{(\phi )}\) also imply
This implies
Using
we can estimate \(I_4\) as follows.
The inequalities (15)–(18) imply that for any \({\alpha }\in (1-\tau , {\gamma }{\lambda })\), the right hand side of (11) is well-defined. The inequalities (15)–(18) also yield (13).
To show (12) is independent of \({\alpha }\) we suppose \(\alpha ',\alpha \in (1-\tau ,\lambda \gamma )\), \(\alpha '>\alpha \). Denote \(\beta =\alpha '-\alpha .\) Using Lemma 2, it is straightforward to see that
This proves the theorem.
Now we can improve the equality (13) as in the following theorem
Theorem 2
Let the assumptions \(\varvec{(W)}\) and \(\varvec{(\phi )}\) be satisfied. Let a, b, c be real numbers such that \(a\le c\le b\). Then there is a constant \(\kappa \) depending only on \(\tau , {\lambda }\) and \({\alpha }\), but independent W, \(\varphi \) and a, b, c such that
Proof
Let \(a\le c<d\le b\) and let \(\tilde{\varphi }(t)=\varphi (c) \chi _{[c, d)}(t)\), where \(\chi _{[c, d)}\) is the indicator function on [c, d). Then
This means \(W(t, \tilde{\varphi }(t'))=W(t, \varphi (c) ) \chi _{[c, d)}(t')\). Hence, from (8) we have
Let c be any point in [a, b]. Denote \(\tilde{W}(t,x)=W(t,x)-W(t, \varphi _c)\). Then \(\tilde{W}\) satisfies \(\varvec{(W)}\). As in the Eq. (14), we have
where \(\tilde{I}_2 =I_2\) and \(\tilde{I}_4 =I_4\) are the same as \(I_2\) and \(I_4\) in the proof of Theorem 1. But
From the assumptions \(\varvec{(W)}\) and \(\varvec{(\phi )}\) we see that
This implies that
Similarly, we have
Combining these two inequalities (20) and (21) with the inequalities (17) and (18) we have
which yields (19).
Theorem 3
Let the assumption \(\varvec{(W)}\) be satisfied. Let \(\varphi : [a, b]\rightarrow \mathbb {R}^d\) satisfy
for some \(\ell \in (\gamma , \infty )\) and for some constant \(L\in (0, \infty )\). If \(\tau +{\lambda }\gamma > 1\), then for any \({\beta }< 1+\frac{{\lambda }{\gamma }+\tau -1}{{\gamma }}\ell \) we have
here the constant C does not depend on \(b-a\).
Proof
As in the proof of Theorem 2 we express \(\int _{a}^{b}W(d t,\varphi _{t})-W(b,\varphi _a)+W(a,\varphi _a) \) as the sum of the terms \(\tilde{I}_j\), \(j=1,2,3,4\) (we follow the notation there). First, we explain how to proceed with \(\tilde{I}_4\). We shall use C to denote a generic constant independent of \(b-a\). Denote
First, we know that we have
On the other hand, we also have
when \(a\le r<t<s\le b\). Therefore, from (24) and (25) it follows that for any \({\beta }_1\ge 0\) and \({\beta }_2\ge 0\) with \({\beta }_1+{\beta }_2=1\), we have
If we choose \({\alpha }\) and \({\beta }_1\) such that
then
For any \({\beta }< 1+\frac{{\lambda }{\gamma }+\tau -1}{{\gamma }}\ell \) we can choose \({\alpha }\), \({\beta }_1\), and \({\beta }_2\) such that (26) is satisfied and
The term \(\tilde{I}_2\) can be handled in a similar but easier way and a similar bound can be obtained.
Now, let us consider \(\tilde{I}_3\). We have
This easily yields
A similar estimate holds true for \(\tilde{I}_1\). However, it is easy to verify \(\tau \,+\,{\lambda }\ell >1\,+\,\frac{{\lambda }{\gamma }+\tau -1}{{\gamma }}\ell \) if \(\ell > \gamma \). The theorem is proved.
Next, we show that the nonlinear integral defined in Definition 1 coincides with the limit of Riemann sums. For this purpose, we need some preliminary set up. For every s, t in [a, b], we put \(\mu (s,t)=W(t,\varphi _s)-W(s,\varphi _s)\). Let \(\pi =\{a=t_0<t_1<\cdots <t_n=b\}\) be a partition of [a, b] with mesh size \(|\pi |=\max _{1\le i\le n }|t_{i}-t_{i-1}|\). One can consider the limit of the Riemann sums
whenever it exists. A sufficient condition for convergence of the Riemann sums is provided by following two results of [2], see also [1] for a simple exposition.
Lemma 3
(The sewing map) Let \(\mu \) be a continuous function on \([0,T]^2\) with values in a Banach space B and \(\varepsilon >0\). Suppose that \(\mu \) satisfies
Then there exists a function \(\mathscr {J}\mu (t)\) unique up to an additive constant such that
We adopt the notation \(\mathscr {J}_a^b \mu =\mathscr {J}\mu (b)-\mathscr {J}\mu (a)\)
Lemma 4
(Abstract Riemann sum) Let \(\pi =\{a=t_0<t_1<\cdots <t_m=b\}\) be an arbitrary partition of [a, b] with \(|\pi |=\sup _{i=0,\ldots ,m-1}|t_{i+1}-t_{i}|\). Define the Riemann sum
then \(J_\pi \) converges to \(\mathscr {J}_a^b\mu \) as \(|\pi |\downarrow 0\) .
Because \(\tau +\lambda \gamma \) is strictly greater than 1, the estimate (19) together with the previous two Lemmas implies
Proposition 2
Assume that \(\varvec{(W)}\) and \(\varvec{(\phi )}\) hold with \(\lambda \gamma +\tau >1\). As the mesh size \(|\pi |\) shrinks to 0, the Riemann sums
converges to \(\int _a^bW(dt,\varphi _t)\).
Remark 3
In [5], the authors define the nonlinear integral \(\int W(dt,\varphi _t)\) via the sewing Lemma 3. The previous proposition shows that the approach using fractional calculus employed here produces an equivalent definition. Let us note that this is possible because of the key estimate (19) and the uniqueness part of the sewing Lemma 3.
It is easy to see from here that
This together with (13) imply easily the following.
Proposition 3
Assume that \(\varvec{(W)}\) and \(\varvec{(\phi )}\) hold with \(\lambda \gamma +\tau >1\). As a function of t, the indefinite integral \(\left\{ \int _{a}^t W(ds,\varphi _{s})\,, \ t\le a\le b\right\} \) is Hölder continuous of exponent \(\tau \).
Further properties can be developed. For instance, we study the dependence of the nonlinear Young integration \(\int W(d s,\varphi _s)\) with respect to the medium W and the integrand \(\varphi \). We state the following two propositions whose proofs are left for readers (see, however, [5] for details).
Proposition 4
Let \(W_1\) and \(W_2\) be functions on \(\mathbb {R}\times \mathbb {R}^d\) satisfying the condition \(\varvec{(W)}\). Let \(\varphi \) be a function in \(C^\gamma (\mathbb {R};\mathbb {R}^d)\) and assume that \(\tau +\lambda \gamma >1\). Then
Proposition 5
Let W be a function on \(\mathbb {R}\times \mathbb {R}^d\) satisfying the condition \(\varvec{(W)}\). Let \(\varphi ^1\) and \(\varphi ^2\) be two functions in \(C^\gamma (\mathbb {R};\mathbb {R}^d)\) and assume that \(\tau +\lambda \gamma >1\). Let \(\theta \in (0,1)\) such that \(\tau +\theta \lambda \gamma >1\). Then for any \(u<v\)
where \(C_1\) is an absolute constant and \(C_2=2^{1-\theta } C_1(\Vert \varphi ^1\Vert _{\gamma }^\lambda +\Vert \varphi ^1\Vert _{\gamma }^\lambda )^\theta \).
4 Iterated Nonlinear Integral
From Remark 2 we see that if \(W(t,x)=\sum _{i=1}^d g_i(t)x_i\) and \(\varphi _i(t)=f_i(t)\), then \(\int _a^b W(d t, \varphi _t)=\displaystyle \sum _{i=1}^d \int _a^b f_i(t) dg_i(t)\). We know that the multiple (iterated) integrals of the form
are well-defined and have applications in expanding the solutions of differential equations (see [3]). What is the extension of the above iterated integrals to the nonlinear integral? To simplify the presentation, we consider the case \(d=1\). General dimensions can be considered in a similar way with more complex notations.
We introduce the following notation. Let
be a simplex in \(\mathbb {R}^n\).
Definition 2
Let \(\varphi :{\varDelta }_{n, a, b}\rightarrow \mathbb {R}\) be a continuous function. For a fixed \(s_n\in [a, b]\), we can consider \(\varphi (\cdot , s_n)\) as a function of \(n-1\) variables. Assume we can define \(\int _{{\varDelta }_{n-1, a, s_n } } \varphi (s_1, \ldots , s_{n-1}, s_n)W(ds_1, \cdot ) \cdots W(ds_{n-1}, \cdot )\), which is a function of \(s_n\), denoted by \(\phi _{n-1}(s_n)\), then we define
In the case \(W(t,x)=f(t) x\), such iterated integrals have been studied in [3], where an important case is when \(\varphi (s_1, \ldots , s_n) =\rho (s_1)\) for some function \(\rho \) of one variable. This means that \(\varphi (s_1, \ldots , s_n) \) depends only on the first variable. This case appears in the remainder term when one expands the solution of a differential equation and can be dealt with in the following way.
Let \(F_1,F_2,\ldots ,F_n\) be jointly Hölder continuous functions on \([a,b]^2\). More precisely, for each \(i=1,\ldots , n\), \(F_i\) satisfies
We assume that \(\tau +\lambda >1\).
Suppose that F is a function satisfying (29) with \(\tau +\lambda >1\). The nonlinear integral \(\int _a^b F(ds,s)\) can be defined analogously to Definition 1. Moreover, for a Hölder continuous function \(\rho \) of order \(\lambda \), we set \(G(s,t)=\rho (t)F(s,t)\), it is easy to see that
Hence, the integration \(\int \rho (s)F(ds,s)\) is well defined. In addition, it follows from Theorem 2 that the map \(t\mapsto \int _a^t \rho (s)F(ds,s)\) is Hölder continuous of order \(\tau \).
We have then easily
Proposition 6
Let \(\rho \) be a Hölder continuous function of order \(\lambda \). Under the condition (29) and \(\tau >1/2\), the iterated integral
is well defined.
In the simplest case when \(\rho (s)=1\) and \(F_i(s,t)=f(s)\) for all \(i=1,\ldots ,n\), the above integral becomes
Therefore, one would expect that
This estimate turns out to be true for (30).
Theorem 4
Let \(F_1,\ldots ,F_n\) satisfy (29) and \(\rho \) be Hölder continuous with exponent \(\lambda \). We assume that \(\rho (a)=0\). Denote \(\displaystyle {\beta }=\frac{{\lambda }+\tau -1}{\lambda }\) and \(\ell _n=\displaystyle \frac{{\beta }^{n-1}-1}{{\beta }-1}+{\beta }^{n-1} (\tau +{\lambda })\). Then, for any \({\gamma }_n<\ell _n\), there is a constant \(C_n \), independent of a and b (but may depend on \({\gamma }_n\)) such that
Proof
Denote
Thus, we see by definition that
We prove this theorem by induction on n. When \(n=1\), the theorem follows straightforwardly from (19) with the choice \(c=a\). Indeed, we have \(|I^{(1)}_{a,t}|\le C|t-a|^{\lambda +\tau }\) and \(|I^{(1)}_{a,t}-I^{(1)}_{a,s}|\le C|t-s|^{\tau }\).
The passage from n to \(n+1\) follows from the application of (23)–(33) and this concludes the proof of the theorem.
Remark 4
The estimate of Theorem 4 also holds true for the iterated nonlinear Young integral \( I_{a,b}^{(n)}(F_1,\ldots ,F_n) =\int _{a\le s_1\le \cdots \le s_ k\le s } F_1(ds_1, \rho (s_1))F_2(ds_2,s_2)\cdots F_n(ds_n,s_n) \), where \(I_{a,b}^{(k)}(F_1,\ldots ,F_k) =\int _a^b F_k(ds, I_{a,s}^{(k-1)}(F_1,\ldots ,F_{k-1}))\), and \( I_{a,b}^{(1)}(F_1) =\int _a^b F_1(ds , \rho (s ))\).
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Acknowledgments
Y. Hu is partially supported by a grant from the Simons Foundation #209206 and by a General Research Fund of University of Kansas.
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Hu, Y., Lê, K.N. (2016). Nonlinear Young Integrals via Fractional Calculus. In: Benth, F., Di Nunno, G. (eds) Stochastics of Environmental and Financial Economics. Springer Proceedings in Mathematics & Statistics, vol 138. Springer, Cham. https://doi.org/10.1007/978-3-319-23425-0_3
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