Abstract
We consider the existence and Hölder continuity conditions for the k-th-order derivatives of self-intersection local time for d-dimensional fractional Brownian motion, where \(k=(k_1,k_2,\ldots , k_d)\). Moreover, we show a limit theorem for the critical case with \(H=\frac{2}{3}\) and \(d=1\), which was conjectured by Jung and Markowsky [7].
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1 Introduction
Fractional Brownian motion (fBm) on \(\mathbb {R}^d\) with Hurst parameter \(H\in (0,1)\) is a d-dimensional centered Gaussian process \(B^H=\{B_t^H, ~t\ge 0\}\) with component processes being independent copies of a 1-dimensional centered Gaussian process \(B^{H,i}\), \(i=1,2,\ldots ,d\) and the covariance function given by
Note that \(B_t^{\frac{1}{2}}\) is a classical standard Brownian motion. Let \(D=\{(r,s): 0<r<s<t\}\). The self-intersection local time (SLT) of fBm was first investigated in Rosen [11] and formally defined as:
where \(B^H\) is a fBm and \(\delta \) is the Dirac delta function. It was further investigated in Hu [3], Hu and Nualart [4]. In particular, Hu and Nualart [4] showed its existence whenever \(Hd<1\). Moreover, \(\alpha _t(y)\) is Hölder continuous in time of any order strictly less than \(1-H\) with \(d=1\), which can be derived from Xiao [14].
The derivative of self-intersection local time (DSLT) for fBm was first considered in the works by Yan et al. [15] [16], where the ideas were based on Rosen [12]. The DSLT for fBm has two versions: One is extended by the Tanaka formula (see in Jung and Markowsky [7]):
The other is from the occupation-time formula (see Jung and Markowsky [8]):
Motivated by the first-order DSLT for fBm in Jung and Markowsky [8] and the k-th-order derivative of intersection local time (ILT) for fBm in Guo et al. [1], we will consider the following k-th-order DSLT for fBm in this paper
where \(k=(k_1,\ldots ,k_d)\) is a multi-index with all \(k_i\) being nonnegative integers and \(|k|=k_1+k_2+\cdots +k_d\), \(\delta \) is the Dirac delta function of d variables and \(\delta ^{(k)}(y)=\frac{\partial ^k}{\partial y_1^{k_1}\cdots \partial y_d^{k_d}}\delta (y)\) is the k-th-order partial derivative of \(\delta \).
Set
where \(\langle p,x\rangle =\sum _{j=1}^dp_jx_j\) and \(|p|^2=\sum _{j=1}^dp_j^2\).
Since the Dirac delta function \(\delta \) can be approximated by \(f_\varepsilon (x)\), we approximate \(\delta ^{(k)}\) and \(\widehat{\alpha }_t^{(k)}(y)\) by
and
respectively.
If \(\widehat{\alpha }^{(k)}_{t,\varepsilon }(y)\) converges to a random variable in \(L^p\) as \(\varepsilon \rightarrow 0\), we denote the limit by \(\widehat{\alpha }_t^{(k)}(y)\) and call it the k-th DSLT of \(B^H\).
Theorem 1
For \(0<H<1\) and \(\widehat{\alpha }^{(k)}_{t,\varepsilon }(y)\) defined in (1), let \(\#:=\#\{k_i ~is ~odd, ~i=1, 2, \ldots d\}\) denotes the odd number of \(k_i\), for \(i=1, 2, \ldots , d\). If \(H<\min \{\frac{2}{2|k|+d},\frac{1}{|k|+d-\#}, \frac{1}{d}\}\) for \(|k|=\sum _{j=1}^dk_j\), then \(\widehat{\alpha }^{(k)}_{t}(0)\) exists in \(L^2\).
Theorem 2
If \(H(|k|+d)<1\), then \(\widehat{\alpha }^{(k)}_{t}(0)\) exists in \(L^p\), for all \(p\in (0,\infty )\).
Note that if \(d=1\) and \(|k|=1\), the condition for the existence of \(\widehat{\alpha }^{(k)}_{t}(y)\) in Theorems 1 and 2 is consistent with that in Jung and Markowsky [8]. If \(d=2\) and \(|k|=1\) in Theorems 1, we can see \(H<\frac{1}{2}\) is the best possible, since a limit theorem for threshold \(H=\frac{1}{2}\) studied in Markowsky [9].
Theorem 3
Assume that \(H(|k|+d)<1\) and \(t, \tilde{t}\in [0,T]\). Then, \(\widehat{\alpha }^{(k)}_{t}(y)\) is Hölder continuous in y of any order strictly less than \(\min (1,\frac{1-Hd-H|k|}{H})\) and Hölder continuous in t of any order strictly less than \(1-H|k|-Hd\),
where \(\lambda <\min (1,\frac{1-Hd-H|k|}{H})\) and
where \(\beta <1-H|k|-Hd\).
Note that if \(d=1\) and \(k=1\). The results of (2) and (3) in Theorem 3 are consistent with the results in Jung and Markowsky [8]. When \(d=1\) and \(k=0\), the corresponding Hölder continuous in time of any order less than \(1-H\), is the condition obtained in Xiao [14]. Moreover, we believe that our methodology also works well for k-th-order DSLT of solution of stochastic differential equation (SDE) driven by fBm, if the solution of SDE driven by fBm satisfies the property of local nondeterminism. For example, the special linear SDE, the solution is fractional Ornstein–Uhlenbeck processes.
Jung and Markowsky [7] proved that \(\widehat{\alpha }^{(k)}_{t}(0)\) exists in \(L^2\) for \(d=1\) and \(k=1\) with \(0<H<2/3\), and conjectured that for the case \(H>2/3\), \(\varepsilon ^{-\gamma (H)}\widehat{\alpha }^{'}_{t,\varepsilon }(0)\) converges in law to a Gaussian distribution for some suitable constant \(\gamma (H)>0\), and at the critical point \(H=\frac{2}{3}\), the variable \(\log (\frac{1}{\varepsilon })^{-\gamma }\widehat{\alpha }^{'}_{t,\varepsilon }(0)\) converges in law to a Gaussian distribution for some \(\gamma >0\). Later, Jaramillo and Nualart [5] proved the case of \(H>2/3\) as
By the proof of Lemma 1 in Sect. 2, we can see the multinomial terms \((p_{i1}-\frac{\mu p_{i2}}{\rho })^{k_i}\) for \(i=1,2,...,d\), are taken into account. But we are not sure if \(k_i\) is odd or even, there are many difficulties in the integral of \(\int (p_{i1}-\frac{\mu p_{i2}}{\rho })^{k_i}e^{-\frac{\rho p^2_{i1}}{2}}dp_{i1}\); thus, we only consider the limit theorem in case \(d=1\) and \(k=1\) below.
Inspired by the results conjectured in [7] and the functional limit theorem for SLT of fBm given in Jaramillo and Nualart [6]. We will show a limit theorem of the critical case \(H=\frac{2}{3}\).
Theorem 4
For \(\widehat{\alpha }^{(k)}_{t,\varepsilon }(y)\) defined in (1) with \(y=0\). Suppose that \(H=\frac{2}{3}\), \(d=1\) and \(k=1\), then as \(\varepsilon \rightarrow 0\), we have
where \(\sigma ^2=\frac{t^{\frac{4}{3}}}{8\pi }B(2,1/3)\) and \(B(\cdot ,\cdot )\) is a Beta function.
The study of DSLT for fBm has a strong degree of heat, see in [5,6,7,8, 17] and references therein. However, the corresponding results for higher-order derivative have not been studied, except for the higher-order derivative of ILT for two independent fBms and some general Gaussian processes in [1] and [2]. As we all know, SLT and ILT have different integral structures in form. In particular, the independence of two fBms is required for ILT. So that the nondeterminism property which used for higher-order derivative of ILT cannot be used directly here.
To obtain the main results, we would use the methods of sample configuration given in Jung and Markowsky [8] and chaos decomposition provided in Jaramillo and Nualart [5]. Chaos decomposition is more and more mature for the asymptotic properties of SLT (see in Hu [4], Jaramillo and Nualart [5] and the references therein). The sample configuration method gives a way to apply nondeterminism property, and it is very powerful to prove the Hölder regularity. But the corresponding results of higher-order DSLT for d-dimensional fBm still have certain difficulty. The main difficulty lies in the computational complexity of multiple integrals. Moreover, the related results can be extended to the general cases. By the Theorem 4.1 in Jaramillo and Nualart [5] and Theorem 4 here, two limit theorems of the case \(H>\frac{2}{2|k|+d}\) and critical case \(H=\frac{2}{2|k|+d}\), with general \(k=(k_1,\ldots , k_d)\) are left open. Extending these limit theorems to general cases will be worked in the future.
The paper has the following structure. We present some preliminary properties of d-dimensional fBm and some basic lemmas in Sect. 2. Section 3 is to prove the main results. To be exact, we will split this section into four subsections to prove the four theorems given in Sect. 1. Throughout this paper, if not mentioned otherwise, the letter C, with or without a subscript, denotes a generic positive finite constant and may change from line to line.
2 Preliminaries
In this section, we first give some properties of d-dimensional fBm \(B^H\). It is well known that d-dimensional fBm has self-similarity, stationary increments and Hölder continuity. When Hurst parameter \(H>1/2\), \(B^H\) exhibits long memory. When \(H<1/2\), it has short memory. But in this paper, we need the following nondeterminism property.
By Nualart and Xu [10] (see also in Song, Xu and Yu [13]), we can see that for any \(n\in \mathbb {N}\), there exists two constants \(\kappa _{H}\) and \(\beta _{H}\) depending only on n and H, such that for any \(0=s_0<s_1<\cdots < s_n \), \(1\le i \le n\), we have
Next, we present two basic lemmas, which will be used in Sect. 3.
Lemma 1
For any \(\lambda , ~\mu , ~\rho \in \mathbb {R}\) with \(\lambda >0\), \(\rho >0\) and \(\lambda \rho -\mu ^2>0\). For \(k\in \mathbb {Z}^+\), there exists a constant C only depending on k, such that
-
(i)
if k is odd,
$$\begin{aligned} \begin{aligned}&\Big |\int _{\mathbb {R}^2}x^ky^ke^{-\frac{1}{2}(\lambda x^2+\rho y^2+2\mu xy)}dxdy\Big |\\&\quad \le {\left\{ \begin{array}{ll} \frac{C |\mu |^k}{(\lambda \rho -\mu ^2)^{k+\frac{1}{2}}}, &{}\text{ if } \frac{\mu ^2}{\lambda \rho -\mu ^2}\ge 1,\\ \frac{C |\mu |}{(\lambda \rho -\mu ^2)^{\frac{k}{2}+1}}, &{}\text{ if } \frac{\mu ^2}{\lambda \rho -\mu ^2}<1, \end{array}\right. } \end{aligned} \end{aligned}$$(4) -
(ii)
if k is even,
$$\begin{aligned} \begin{aligned}&\Big |\int _{\mathbb {R}^2}x^ky^ke^{-\frac{1}{2}(\lambda x^2+\rho y^2+2\mu xy)}dxdy\Big |\\&\quad \le {\left\{ \begin{array}{ll} \frac{C |\mu |^k}{(\lambda \rho -\mu ^2)^{k+\frac{1}{2}}}, &{}\text{ if } \frac{\mu ^2}{\lambda \rho -\mu ^2}\ge 1,\\ \frac{C }{(\lambda \rho -\mu ^2)^{\frac{k+1}{2}}}, &{}\text{ if } \frac{\mu ^2}{\lambda \rho -\mu ^2}<1. \end{array}\right. } \end{aligned} \end{aligned}$$(5)
Proof
First, we consider the integral with respect to y,
If k is odd, since
we have
where \(C_1, ~C_3, \ldots , ~C_k\) are all positive constants and
For the dx integral,
where the right-hand side is the sum of equal ratio series with the common ratio \(\frac{\mu ^2}{\lambda \rho -\mu ^2}>0\). Then, we get (4).
If k is even,
It is easy to see that
and
For the integral with respect to x,
and
This gives (5). \(\square \)
The next lemma gives the bounds on the quantity of \(\lambda \rho -\mu ^2\), which could be obtained from the Appendix B in [7] or the Lemma 3.1 in [3].
Lemma 2
Let
and
Case (i) Suppose that \(D_1=\{(r,r',s,s')\in [0,t]^4 ~|~ r<r'<s<s'\}\), let \(r'-r=a\), \(s-r'=b\), \(s'-s=c\). Then, there exists a constant \(K_1\) such that
and
Case (ii) Suppose that \(D_2=\{(r,r',s,s')\in [0,t]^4 ~|~ r<r'<s'<s\}\), let \(r'-r=a\), \(s'-r'=b\), \(s-s'=c\). Then, there exists a constant \(K_2\) such that
and
Case (iii) Suppose that \(D_3=\{(r,r',s,s')\in [0,t]^4 ~|~ r<s<r'<s'\}\), let \(s-r=a\), \(r'-s=b\), \(s'-r'=c\). Then, there exists a constant \(K_3\) such that
and
3 Proof of the Main Results
In this section, the proof of Theorems 1, 2, 3 and 4 is taken into account. We will divide this section into four parts and give the proof of the corresponding theorem in each part.
3.1 Proof of Theorem 1
By (1) and the proof of Lemma 1,
where \(\lambda =|s-r|^{2H}, ~\rho =|s'-r'|^{2H}\),
and
for \(i=1, 2, \ldots , d\).
Note that for any \(\varepsilon _1, ~\varepsilon _2>0\),
where
Consequently, if
then \(\widehat{\alpha }^{(k)}_{t,\varepsilon }(0)\) converges in \(L^2\) as \(\varepsilon \rightarrow 0\).
By Lemma 1, we can see that \(\int _{D^2}\prod _{i=1}^d\left| \widetilde{\varXi }_{k_i}\right| dr'dr ds'ds\) is less than
where \(\#=\#\{k_i ~is ~odd, ~i=1, 2, \ldots , d\}\) denotes the odd number of \(k_i\), for \(i=1, 2, \ldots , d\), and \(\#\in \{0, 1, 2, \ldots , d\}\).
Thus, to prove the finiteness of \(\int _{D^2}\prod _{i=1}^d\left| \widetilde{\varXi }_{k_i}\right| dr'dr ds'ds\), we only need to prove
with \(Q=|k|\) and \(Q=\#\).
By Lemma 2, we can see \(D^2\) is the union of the sets \(D_1, ~D_2, ~D_3\).
When \((r,r',s,s')\in D_1\), then the left-hand side of (6) is less than
When \((r,r',s,s')\in D_2\). Note that for the condition \(H<\min \{\frac{2}{2|k|+d},\frac{1}{|k|+d-\#}, \frac{1}{d}\}\), only in the case \(d=1\), H can get the value bigger than \(\frac{1}{2}\), while these the case have been studied in [4] and [7], respectively. So, we only need to consider the case \(H<\frac{1}{2}\).
Thus, the left-hand side of (6) is less than
Since \(H<\frac{1}{2}\), then
Thus,
When \((r,r',s,s')\in D_3\). For \(\alpha , \beta >0\) with \(\alpha +\beta =1\), there exists a positive constant K such that
Thus, the left-hand side of (6) is less than
Note that \(|k|\ge 1\) (where \(|k|=0\) with \(H<\frac{1}{d}\) could deduced from [4]) and \(H<\frac{1}{2}\). When \(Q=0\) (all derivatives were of even order), the result of (6) is obvious by \(H<\frac{1}{|k|+d}\). When \(Q\ge 1\), we have \(2Q(1-H)>1\). So, we first choose \(\varepsilon _0>0\), such that
Then, we can choose
Thus,
which is less than one. This gives (6).
3.2 Proof of Theorem 2
By (1), we have
where \(k=(k_1, \ldots , k_d)\), \(|p_j^k|=\prod _{i=1}^d|p_{ij}|^{k_i}\) for \(j=1,...,n\), \(drds=dr_1\cdots dr_nds_1\cdots ds_n\) and
We use the method of sample configuration as in Jung and Markowsky [8]. Fix an ordering of the set \(\{r_1, s_1, r_2, s_2, \ldots , r_n, s_n\}\), and let \(l_1\le l_2\le \cdots \le l_{2n}\) be a relabeling of the set \(\{r_1, s_1, r_2, s_2, \ldots , r_n, s_n\}\). Let \(u_1 \ldots u_{2n-1}\) be the proper linear combinations of the \(p_{j}\)’s so that
A detailed description of how the u’s are chosen can be found in [8]. Then, by the local nondeterminism of fBm,
Fix j, and let \(j_1\) to be the smallest value such that \(u_{j_1}\) contains \(p_{j}\) as a term and then choose \(j_2\) to be the smallest value strictly larger than \(j_1\) such that \(u_{j_2}\) does not contain \(p_{j}\) as a term. Then, \(p_j = u_{j_1} - u_{j_1-1} = u_{j_2-1} - u_{j_2}\). Similar to Jung and Markowsky [8], we can see that with the convention that \(u_{0}=u_{2n}=0\),
Thus,
and
where
and
Note that we have omitted the terms \(j=0, 2n\) in the final expression in (7) since \(u_0=u_{2n} = 0\). Then,
where \(E^n=\{0<l_1<\cdots<l_{2n}<t\}\), \(|u_j^{\frac{k}{2}\alpha _j}|=\prod _{i=1}^d|u_{ij}|^{\frac{k_i}{2}\alpha _{i,j}}\) and \(dl=dl_1dl_2\cdots dl_{2n}.\)
It is easy to observe that \(\{u_{1}, u_{2},\ldots , u_{2n-1}\}\) is contained in the span of \(\{p_{1}, p_{2}, \ldots , p_{n}\}\) and conversely, so we can let \(\mathcal {A}\) be a subset of \(\{1, \ldots , 2n-1\}\) such that the set \(\{u_j\}_{j \in \mathcal {A}}\) spans \(\{p_{1}, p_{2}, \ldots , p_{n}\}.\) We let \(\mathcal {A}^c\) denote the complement of \(\mathcal {A}\) in \(\{1, \ldots , 2n-1\}\). Note that
where \(|k\alpha _j|=k_1\alpha _{1,j}+\cdots +k_d\alpha _{d,j}\). Then, we perform a linear transformation changing \((p_{1}, ~p_{2}, \ldots , p_{n})\) into an integral with respect to variables \(\{u_{j}\}_{j \in \mathcal {A}}\),
where |J| is the Jacobian determinant of changing variables \((p_{1}, ~p_{2}, \ldots , p_{n})\) to \((u_{j}, j\in \mathcal {A})\).
Therefore, we may reduce the convergence of \(\left| \mathbb {E}[(\widehat{\alpha }^{(k)}_{t,\varepsilon }(0))^n]\right| \) to show the finiteness of
Since
we have
where \(C_{n,H,t}\) is a constant dependent on n, H and t.
Thus, we can see that \(\left| \mathbb {E}[(\widehat{\alpha }^{(k)}_{t,\varepsilon }(0))^n]\right| \) is finite for all \(\varepsilon >0\) under condition \(H(d+|k|)<1\). Then, we need to prove \(\{\widehat{\alpha }^{(k)}_{t,\varepsilon }(0)\}_{\varepsilon >0}\) is a Cauchy sequence.
Notice that for any \(\varepsilon _1, ~\varepsilon _2>0\),
By the dominated convergence theorem and
we can obtain the desired result. This completes the proof.
3.3 Proof of Theorem 3
Let us first prove (2). For any \(\lambda \in [0,1]\), we have the following inequalities:
and
Using the similar methods as in the proof of Theorem 2, we find that
where \(\tilde{\lambda }_l=(\lambda _1,\ldots , \lambda _d)\) with \(\lambda _l=\lambda \) and all other \(\lambda _j=0\). So \(|k+\tilde{\lambda }|=|k|+\lambda \) and \(\varLambda _1\) is less than (with \(\mathcal {A}\) defined as before)
which is finite if \(1-Hd-H|k+\tilde{\lambda }|>0\).
For the proof of (3), let \(\tilde{D}=\{(r,s): 0<r<s<\tilde{t}\}\) and without loss of generality, we assume that \(t<\tilde{t}\). Then,
where we use the Hölder’s inequality in the last inequality with \(\beta <1-H|k|-Hd\).
Using the similar methods as in the proof of Theorem 2, \(\varLambda _2\) is bounded by
Since \(1-\beta >H(|k|+d)\), there exists a constant \(C>0\), such that
3.4 Proof of Theorem 4
In this section, we mainly use the method given in Jaramillo and Nualart [5]. We first give the chaos decomposition of the random variable \(\widehat{\alpha }^{(k)}_{t,\varepsilon }(0)\) defined in (1) with \(d=1\) and \(k=1\). We write
where
with
and
Then, \(\widehat{\alpha }^{'}_{t,\varepsilon }(0)\) has the following chaos decomposition:
where
with \(D=\{(r,s): 0<r<s<t\}\).
For \(q=1\),
where \(\mathfrak {H}\) is the Hilbert space obtained by taking the completion of the step functions endowed with the inner product
For \(q>1\), we have to describe the terms \(\langle f_{2q-1,\varepsilon ,s_1,r_1},f_{2q-1,\varepsilon ,s_2,r_2}\rangle _{\mathfrak {H}^{\otimes (2q-1)}}\), where \(\mathfrak {H}^{\otimes (2q-1)}\) is the \((2q-1)\)-th tensor product of \(\mathfrak {H}\). For every \(x, ~u_1, ~u_2>0\), we define
Then, from Eq. (2.19) in Jaramillo and Nualart [5],
where
Before we give the proof of the main result, we give some useful lemmas below. In the sequel, we just consider the case \(H=\frac{2}{3}\).
Lemma 3
Proof
From Lemma 5.1 in Jaramillo and Nualart [5], we can see
and
where \(D_i\) (i=1, 2, 3) defined in Lemma 2 and \(\varSigma \) is the covariance matrix of \((B^H_s-B^H_r,B^H_{s'}-B^H_{r'})\) with \(\varSigma _{1,1}=\lambda \), \(\varSigma _{2,2}=\rho \), \(\varSigma _{1,2}=\mu \) given in Lemma 2.
Next, we will split the proof into three parts to consider \(V_1(\varepsilon )\), \(V_2(\varepsilon )\) and \(V_3(\varepsilon )\), respectively.
For the \(V_1(\varepsilon )\) term, changing the coordinates \((r, r', s, s')\) by \((r, a=r'-r, b=s-r', c=s'-s)\) and integrating the r variable, we get
Since
and
where we use the Young’s inequality in the second to last inequality.
Then, we have
We will estimate this integral over the regions \(\{b\le (a\vee c)\}\) and \(\{b > (a\vee c)\}\) separately, and we will denote these two integrals by \(\widetilde{V}_{1,1}\) and \(\widetilde{V}_{1,2}\), respectively. If \(b\le (a\vee c)\), without loss of generality, we can assume \(a\ge c\) and thus \(b\le a\). For a given small enough constant \(\varepsilon _1>0\),
where we make the change of variable \(c=c\,\varepsilon ^{-\frac{3}{2}}\) in the last inequality.
By L’Hôspital’s rule, we have
If \(b>(a\vee c)\), we can see that
and
Then,
So, by the above result, we can obtain
For the \(V_2(\varepsilon )\) term, changing the coordinates \((r, r', s, s')\) by \((r, a=r'-r, b=s'-r', c=s-s')\) and integrating the r variable, we get
By
and
we have
We again estimate this integral over the regions \(\{b\le (a\vee c)\}\) and \(\{b > (a\vee c)\}\) separately, and denote these two integrals by \(\widetilde{V}_{2,1}\) and \(\widetilde{V}_{2,2}\), respectively. If \(b\le (a\vee c)\),
Thus,
If \(b>(a\vee c)\), similarly, we have
So, by the above result, we can obtain
For the \(V_3(\varepsilon )\) term. We first change the coordinates \((r, r', s, s')\) by \((r, a=s-r, b=r'-s, c=s'-r')\) and then by
and \(|\varepsilon I+\varSigma |=\varepsilon ^2+\varepsilon (a^{\frac{4}{3}}+c^{\frac{4}{3}})+(ac)^{\frac{4}{3}}-\mu (a+b,a,c)^2\), we can find
where we change the coordinates (a, b, c) by \((\varepsilon ^{-\frac{3}{4}}a, b, \varepsilon ^{-\frac{3}{4}}c)\) in the last equality.
By the definition of \(\mu (a+b,a,c)\), it is easy to find
and
The other part of the integrand in \(V_3(\varepsilon )\) is
Since
as \(\varepsilon \rightarrow 0\). Then, by L’Hôspital’s rule, we have
\(\square \)
Lemma 4
For \(I_1(f_{1,\varepsilon })\) given in (8), then
Proof
Form (8), we can find
where \(V_i^{(1)}(\varepsilon )=2\int _{D_i}\langle f_{1,\varepsilon ,s_1,r_1},f_{1,\varepsilon ,s_2,r_2}\rangle _{\mathfrak {H}}dr_1dr_2ds_1ds_2\) for \(i=1, 2, 3\). Then, we have
since \(H>\frac{1}{2}\) and \(\mu \) can only take positive values.
Combining (14) with (9)–(11), we can see
Thus, we only need to consider \(\frac{1}{(\log \frac{1}{\varepsilon })^2}V_3^{(1)}(\varepsilon )\) as \(\varepsilon \rightarrow 0\).
By the proof of Lemma 5.7 in Jaramillo and Nualart [5], we have
Note that
and
Similar to (12) and (13), we can find that
and
Thus,
\(\square \)
Proof of Theorem 4
we can see
Since \(I_1(f_{1,\varepsilon })\) is Gaussian, then we have, as \(\varepsilon \rightarrow 0\),
Thus,
as \(\varepsilon \rightarrow 0\). This completes the proof.
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Acknowledgements
I would like to sincerely thank my supervisor Professor Fangjun Xu, who has led the way to this work. I am also grateful to the anonymous referee and Associate Editor for their insightful and valuable comments which have greatly improved the presentation of the paper. Q. Yu is supported by National Natural Science Foundation of China (Grant No.11871219, 12071003).
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Yu, Q. Higher-Order Derivative of Self-Intersection Local Time for Fractional Brownian Motion. J Theor Probab 34, 1749–1774 (2021). https://doi.org/10.1007/s10959-021-01093-6
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DOI: https://doi.org/10.1007/s10959-021-01093-6