Abstract
In this article, we obtain sharp conditions for the existence of the high-order derivatives (k-th order) of intersection local time \( \widehat{\alpha }^{(k)}(0)\) of two independent d-dimensional fractional Brownian motions \(B^{H_1}_t\) and \(\widetilde{B}^{H_2}_s\) of Hurst parameters \(H_1\) and \(H_2\), respectively. We also study their exponential integrability.
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1 Introduction and Main Result
Intersection local time or self-intersection local time when the two processes are the same are important subjects in probability theory and their derivatives have received much attention recently, see, e.g., [9, 11,12,13]. Jung and Markowsky [6, 7] discussed Tanaka formula and occupation time formula for derivative self-intersection local time of fractional Brownian motions. On the other hand, several authors paid attention to the renormalized self-intersection local time of fractional Brownian motions, see, e.g., Hu et al. [3, 4].
Motivated by Jung and Markowsky [6] and Hu [2], higher-order derivative of intersection local time for two independent fractional Brownian motions is studied in this paper.
To state our main result we let \(B^{H_1}=\{B^{H_1}_t, t\ge 0\}\) and \(\widetilde{B}^{H_2}=\{\widetilde{B}^{H_2}_t, t \ge 0 \}\) be two independent d-dimensional fractional Brownian motions of Hurst parameters \(H_1, H_2\in (0, 1)\), respectively. This means that \(B^{H_1}\) and \(\widetilde{B}^{H_2}\) are independent centered Gaussian processes with covariance
(similar identity for \(\tilde{B}\)). In this paper we concern with the derivatives of intersection local time of \(B^{H_1}\) and \(\widetilde{B}^{H_2}\), defined by
where \(k=(k_1, \ldots , k_d)\) is a multi-index with all \(k_i\) being nonnegative integers and \(\delta \) is the Dirac delta function of d-variables. In particular, we consider exclusively the case when \(x=0\) in this work. Namely, we are studying
where \(\delta ^{(k)}(x)=\frac{\partial ^k}{\partial x_1^{k_1}\ldots \partial x_d^{k_d}}\delta (x)\) is k-th order partial derivative of the Dirac delta function. Since \(\delta (x)=0\) when \(x\not =0\) the intersection local time \(\hat{\alpha } (0)\) (when \(k=0\)) measures the frequency that processes \(B^{H_1}\) and \(\widetilde{B}^{H_2}\) intersect each other.
Since the Dirac delta function \(\delta \) is a generalized function, we need to give a meaning to \(\hat{\alpha }^{(k)}(0)\). To this end, we approximate the Dirac delta function \(\delta \) by
where and throughout this paper, we use \(px=\sum _{j=1}^d p_jx_j\) and \(|p|^2=\sum _{j=1}^d p_j^2\). Thus, we approximate \(\delta ^{(k)}\) by
We say that \(\hat{\alpha }^{(k)} (0)\) exists (in \(L^2\)) if
converges to a random variable (denoted by \(\hat{\alpha }^{(k)} (0)\)) in \(L^2\) when \(\varepsilon \downarrow 0\).
Here is the main result of this work.
Theorem 1
Let \(B^{H_1}\) and \(\widetilde{B}^{H_2}\) be two independent d-dimensional fractional Brownian motions of Hurst parameter \(H_1\) and \(H_2\), respectively.
-
(i)
Assume \(k =(k_1, \ldots , k_d)\) is an index of nonnegative integers (meaning that \(k_1, \ldots , k_d\) are nonnegative integers) satisfying
$$\begin{aligned} \frac{H_1H_2}{H_1+H_2} (|k|+d)< 1, \end{aligned}$$(1.5)where \(|k|=k_1+\cdots +k_d\). Then, the k-th order derivative intersection local time \(\hat{\alpha }^{(k)}(0)\) exists in \(L^p(\Omega )\) for any \(p\in [1, \infty )\).
-
(ii)
Assume condition (1.5) is satisfied. There is a strictly positive constant \(C_{d,k,T}\in (0, \infty )\) such that
$$\begin{aligned} \begin{aligned} \mathbb {E} \left[ \exp \left\{ C_{d,k,T}\left| \widehat{\alpha }^{(k)}(0)\right| ^{\beta }\right\} \right] <\infty , \end{aligned} \end{aligned}$$where \(\beta =\frac{H_1+H_2}{2dH_1H_2}\).
-
(iii)
If \(\hat{\alpha }^{(k)}(0)\in L^1(\Omega )\), where \(k=(0, \ldots , 0,k_i, 0,\ldots ,0)\) with \(k_i\) being even integer, then condition (1.5) must be satisfied.
Remark 1
-
(i)
When \(k=0\), we have that \(\widehat{\alpha }^{(0)}(0)\) is in \(L^p\) for any \(p\in [1, \infty )\) if \(\frac{H_1H_2}{H_1+H_2} d<1\). In the special case \(H_1=H_2=H\), this condition becomes \(Hd<2\), which is the condition obtained in Nualart et al. [8].
-
(ii)
When \(H_1=H_2=\frac{1}{2}\), we have the exponential integrability exponent \(\beta =2/d\), which implies an earlier result [2, Theorem 9.4].
-
(iii)
Part (iii) of the theorem states that the inequality (1.5) is also a necessary condition for the existence of \(\hat{\alpha }^{(k)}(0)\). This is the first time for such a statement.
2 Proof of the Theorem
Proof of Parts (i) and (ii)
This section is devoted to the proof of the theorem. We shall first find a good bound for \({\mathbb {E}}\left| \widehat{\alpha }^{(k)}(0)\right| ^n\) which gives a proof for (i) and (ii) simultaneously. We introduce the following notations.
We also denote \(s=(s_1,\ldots ,s_n)\), \(t=(t_1,\ldots ,t_n)\), \(ds=ds_1\ldots ds_n\) and \(dt=dt_1\ldots dt_n\).
Fix an integer \(n\ge 1\). Denote \(T_n=\{0<t,s <T\}^n\). We have
The expectations in the above exponent can be computed by
where
denote, respectively, covariance matrices of n-dimensional random vectors \((B^{H_1,i}_{s_1},\ldots ,B^{H_1,i}_{s_n})\) and that of \((\widetilde{B}^{H_2,i}_{t_1},\ldots , \widetilde{B}^{H_2,i}_{t_n})\). Thus, we have
where
Here we recall \(x=(x_1, \ldots , x_n)\) and \(x^k_i=x_1^{k_i} \ldots x_n^{k_i}\). For each fixed i let us compute integral \(I_i(t,s)\) first. Denote \(B=Q_1+Q_2\). Then B is a strictly positive definite matrix, and hence \(\sqrt{B}\) exists. Making substitution \(\xi =\sqrt{B}x\). Then
To obtain a nice bound for the above integral, let us first diagonalize B:
where \(\varLambda =\hbox {diag}\{\lambda _1 ,\ldots ,\lambda _n \}\) is a strictly positive diagonal matrix with \({\lambda }_1\le {\lambda }_2\le \cdots \le {\lambda }_d\) and \(Q =(q_{ij})_{1\le i,j\le d} \) is an orthogonal matrix. Hence, we have \(\det (B)={\lambda }_1\ldots {\lambda }_d\). Denote
Hence,
Therefore, we have
Since both \(Q_1\) and \(Q_2\) are positive definite, we see that
where \( {\lambda }_1(Q_i)\) is the smallest eigenvalue of \(Q_i\), \(i=1, 2\). This means that
This implies
Consequently, we have
for any \(\rho \in [0,1]\).
Now we are going to find a lower bound for \({\lambda }_1(Q_1)\) (\({\lambda }_1(Q_2)\) can be dealt with the same way. We only need to replace s by t). Without loss of generality we can assume \(0\le s_1<s_2<\cdots <s_n\le T\). From the definition of \(Q_1\) we have for any vector \(u=(u_1, \ldots , u_d)^T\),
Now we use Proposition 1 in “Appendix” to conclude
Consider the function
where
It is easy to see that the matrix \(G^TG\) has a minimum eigenvalue independent of n. Thus, this function f attains its minimum value \(f_\mathrm{min} \) independent of n on the sphere \(u_1^2+\cdots +u_n^2=1\). It is also easy to see that \(f_\mathrm{min}>0\).
As a consequence we have
In a similar way we have
The integral in (2.2) can be bounded as
Substitute (2.3)-(2.5) into (2.2) we obtain
for possibly a different constant C, independent of n.
Next we obtain a lower bound for \(\mathrm {det}(B) \). According to [2, Lemma 9.4]
for any two symmetric positive definite matrices \(Q_1\) and \(Q_2\) and for any \(\gamma \in [0, 1]\). Now it is well known that (see also the usages in [2,3,4]).
and
As a consequence, we have
Thus,
where \(\Delta _n=\left\{ 0<s_1<\cdots <s_n\le T\right\} \) denotes the simplex in \([0, T]^n\). We choose \(\rho =\gamma =\frac{H_2}{H_1+H_2}\) to obtain
where
By Lemma 4.5 of [5], we see that if
then
where
Substituting this bound we obtain
where C is a constant independent of T and n and \(C_T\) is a constant independent of n.
For any \(\beta >0\), the above inequality implies
From this bound we conclude that there exists a constant \(C_{d,T,k}>0\) such that
when \(C_{d, T, k}\) is sufficiently small (but strictly positive), where \(\beta =\frac{H_1+H_2}{2dH_1H_2}\). \(\square \)
Proof of part (iii)
Without loss of generality, we consider only the case \(k=(k_1,0, \ldots , 0)\) and we denote \(k_i\) by k. By the definition of k-order derivative local time of independent d-dimensional fractional Brownian motions, we have
Thus, we have
Integrating with respect to \(\xi \), we find
for some constant \(c_{k, d}\in (0,\infty )\).
We are going to deal with the above integral. Assume first \(0<H_1\le H_2<1\). Making substitution \(t=u^{\frac{H_2}{H_1}}\) yields
Using polar coordinate \(u=r\cos \theta \) and \(s=r\sin \theta \), where \(0\le \theta \le \frac{\pi }{2}\) and \(0\le r\le T\) we have
since the planar domain \(\left\{ (r, \theta ), 0\le r\le T\wedge T^{\frac{H_1}{H_2}}, 0\le \theta \le \frac{\pi }{2}\right\} \) is contained in the planar domain \(\left\{ (s,u), 0\le s\le T, 0\le u\le T ^{\frac{H_1}{H_2}} \right\} \). The integral with respect to r appearing in (2.7) is finite only if \(-(k+d)H_2 +\frac{H_2}{H_1}>-1\), namely only when the condition (1.5) is satisfied. The case \(0<H_2\le H_1<1\) can be dealt similarly. This completes the proof of our main theorem. \(\square \)
3 Appendix
In this section, we recall some known results that are used in this paper. The following lemma is Lemma 8.1 of [1].
Lemma 1
Let \(X_1\), \(\dots \), \(X_n\) be jointly mean zero Gaussian random variables, and let \( Y_1=X_1,\ Y_2=X_2-X_1,\ldots ,Y_n=X_n-X_{n-1}\). Then
where \(\sigma _{j}^2=\mathrm{Var}(Y_j)\) and R is the determinant of the covariance matrix of \(\{X_i,i=1,\ldots ,n\}\), which is also given by the following product of conditional variances
The following lemma is from [4], Lemma A.1.
Lemma 2
Let \((\Omega , \mathcal {F}, P)\) be a probability space and let F be a square integrable random variable. Suppose that \(\mathcal {G}_1\subset \mathcal {G}_2\) are two \(\sigma \)-fields contained in \(\mathcal {F}\). Then
The following is Lemma 7.1 of [10] applied to fractional Brownian motion.
Lemma 3
If \((B_t, 0\le t<\infty )\) is the fractional Brownian motion of Hurst H, then
Combining the above three lemmas we have the following
Proposition 1
Let \((B_t, 0\le t<\infty )\) be the fractional Brownian motion of Hurst H and let \(0\le s_1<\cdots<s_n<\infty \). Then there is a constant c independent of n such that
Proof
Let \(X_i=B_{s_{i}} -B_{s_{i-1}}\) (\(B_{s_{-1}}=0\) by convention). From Lemma 2 we see
where \(\mathcal {F}_t=\sigma (B_s, s\le t)\). From the definition of R we see \(R\ge c^n \prod _{i=1}^n \sigma _i^2\). The proposition is proved by applying Lemma 1. \(\square \)
The following lemma is Lemma 4.5 of [5].
Lemma 4
Let \(\alpha \in (-1+\varepsilon ,1)^m\) with \(\varepsilon >0\) and set \(\mid \alpha \mid =\sum _{i=1}^m\alpha _i\). Denote \(T_m(t)=\{(r_1,r_2,\ldots ,r_m)\in \mathbb {R}^m:0<r_1<\cdots<r_m<t\}\). Then there is a constant \(\kappa \) such that
where by convention, \(r_0=0\).
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Jingjun Guo acknowledges the support of National Natural Science Foundation of China #71561017, the Youth Academic Talent Plan of Lanzhou University of Finance and Economics. Yaozhong Hu is partially supported by a Grant from the Simons Foundation #209206 and by a General Research Fund of University of Kansas. Yanping Xiao acknowledges the support of Basic Charge of Research for Northwest Minzu University #31920170035.
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Guo, J., Hu, Y. & Xiao, Y. Higher-Order Derivative of Intersection Local Time for Two Independent Fractional Brownian Motions. J Theor Probab 32, 1190–1201 (2019). https://doi.org/10.1007/s10959-017-0800-2
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DOI: https://doi.org/10.1007/s10959-017-0800-2
Keywords
- Fractional Brownian motion
- Intersection local time
- k-th derivative of intersection local time
- Exponential integrability