Research Article A Robust Weak Taylor Approximation Delay Differential Equations

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Hindawi Publishing Corporation
Abstract and Applied Analysis
Volume 2013, Article ID 750147, 8 pages
http://dx.doi.org/10.1155/2013/750147
Research Article
A Robust Weak Taylor Approximation
Scheme for Solutions of Jump-Diffusion Stochastic
Delay Differential Equations
Yanli Zhou,1 Yonghong Wu,1 Xiangyu Ge,2 and B. Wiwatanapataphee3
1
Department of Maths and Statistics, Curtin University, Perth, WA 6845, Australia
School of Statistics & Maths, Zhongnan University of Economics and Law, Wuhan 430073, China
3
Department of Mathematics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand
2
Correspondence should be addressed to Yanli Zhou; ylzhou8507@gmail.com and B. Wiwatanapataphee; scbww@mahidol.ac.th
Received 1 December 2012; Revised 13 March 2013; Accepted 14 March 2013
Academic Editor: Xinguang Zhang
Copyright © 2013 Yanli Zhou et al. This is an open access article distributed under the Creative Commons Attribution License,
which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Stochastic delay differential equations with jumps have a wide range of applications, particularly, in mathematical finance. Solution
of the underlying initial value problems is important for the understanding and control of many phenomena and systems in the
real world. In this paper, we construct a robust Taylor approximation scheme and then examine the convergence of the method in a
weak sense. A convergence theorem for the scheme is established and proved. Our analysis and numerical examples show that the
proposed scheme of high order is effective and efficient for Monte Carlo simulations for jump-diffusion stochastic delay differential
equations.
1. Introduction
Stochastic delay differential equation models play a very
important role in the study of many fields such as economics
and finance, chemistry, biology, microelectronics, and control theories. Models of this type can more accurately describe
many phenomena in the real world by taking into account
the effect of time delay and random noise. By time delay, it
means a certain period of time is required for the effect of an
action to be observed after the moment when the action takes
place. This phenomenon exists in most systems in almost any
area of science; for example, a patient shows symptoms of an
illness days or even weeks after he/she was infected. Similarly,
random noises appear in almost all real world phenomena
and systems, for example, the motion of molecules and the
price of assets in financial markets. Hence, study of SDDEs is
an important undertaking in order to understand real world
phenomena and systems precisely.
Over the last couple of decades, a lot of work has been
carried out to study differential equations with delay and/
or random noises, for example, [1–5]. The best-known and
well-studied theory and systems include the delay differential
equations (DDEs) presented by Kolmanvskii and Myshkis [6]
and their stochastic generalizations and the stochastic delay
differential equations (SDDEs) established by Mohammed
[7, 8], Mao [9, 10], and Mohammed and Scheutzow [11]. Other
SDDEs theories of interest include, for instance, the so-called
SDDEs with Markovian switching and Poisson jumps. These
models have been investigated in the literature [12–14].
Analytical solutions of SDDEs can hardly be obtained. It
is thus important to develop and study discrete-time approximation methods for solving SDDEs. Discrete-time approximations may be divided into two categories: weak approximations and strong approximations [15]. Some implicit and
explicit numerical approximation methods for SDDEs in
strong approximation sense were derived by Küchler and
Platen [16]. Weak numerical methods for SDDEs have been
studied by Küchler and Platen. The Monte Carlo simulation
method has also been developed as a powerful simulation
method for SDEs, while weak numerical approximations are
required for Monte Carlo simulation [9, 17–20].
2
Abstract and Applied Analysis
In this paper, we extend a fully weak approximation
method for SDDEs to the type of jump-diffusion SDDEs:
𝑑X (𝑑) = a (𝑑, X (𝑑) , X (𝑑 − 𝛾)) 𝑑𝑑
+ b (𝑑, X (𝑑) , X (𝑑 − 𝛾)) 𝑑W𝑑
(1)
+ ∫ c (𝑑, X (𝑑− ) , 𝜐) π‘πœ‘ (π‘‘πœ, 𝑑𝑑)
πœ€
subject to the initial condition
𝑋 (πœƒ) = πœ’ (πœƒ)
for πœƒ ∈ [−𝛾, 0] ,
(2)
where 𝑑 ∈ [0, 𝑇], 𝛾 is the time delay which is assumed to be
constant at all time, W𝑑 = {(π‘Šπ‘‘1 , . . . , π‘Šπ‘‘π‘š ), 𝑑 ∈ [0, 𝑇]} is an Aadapted π‘š-dimensional Wiener process, and π‘πœ‘ denotes the
Poisson random measure. Also here we denote by X(𝑑− ) the
almost sure left-hand limit of X(𝑑). The coefficient a(𝑑, π‘₯, π‘₯π‘Ÿ ) :
[0, 𝑇] × R𝑑 × R𝑑 → R𝑑 and c(𝑑, π‘₯, 𝜐) : [0, 𝑇] × R𝑑 × πœ€ →
R𝑑 are 𝑑-dimensional vectors of Borel measurable functions.
Further, b(𝑑, π‘₯, π‘₯π‘Ÿ ) defined on [0, 𝑇] × R𝑑 × R𝑑 is a 𝑑 × π‘šmatrix of Borel measurable function.
The main contributions of this work include construction
of a numerical approximation method for weak solutions of
SDDEs with jump-diffusion, and establishment of a theoretical result for the convergence of the scheme.
The remaining part of this paper is organised as follows. In the following section, we give the conditions for
the existence and uniqueness of the solution of the jumpdiffusion SDDEs (1) which is applicable to any cases where
solution exists, and present various lemmas to be used later
for the proof of the convergence theorem. We then introduce,
in Section 3, a general weak approximation scheme, where
the simplified stochastic Taylor approximation scheme with
order 𝛽 is constructed; followed by a convergence theorem
and its proof. In Section 4, we give a numerical example
to demonstrate the application and the convergence of the
numerical scheme.
where (πœπ‘– , πœ‰π‘– ), for 𝑖 ∈ {1, 2, 3, . . . , π‘πœ‘ (𝑑)}, are a sequence of pairs
of jump times and corresponding values generated by the
Poisson random measure π‘πœ‘ .
Definition 1. Given a filtered probability space (Ω, A, A, 𝑃), a
stochastic process given by X = {X(𝑑), 𝑑 ∈ [−𝛾, 𝑇]} is known
as a solution of (1) subject to the initial condition (2) if X is
A-adapted, the integrals in the equation are well defined, and
equalities (3) and (2) hold almost surely. Moreover, if any two
solution processes X(𝑖) = {X(𝑖) (𝑑), 𝑖 ∈ 1, 2} are indistinguishable on [−𝛾, 𝑇] with the same initial segment πœ’ and the same
path on [0, 𝑇], and
σ΅„©
σ΅„©
𝑃 ( sup 󡄩󡄩󡄩󡄩𝑋(1) (𝑑) − 𝑋(2) (𝑑)σ΅„©σ΅„©σ΅„©σ΅„© > 0) = 0,
𝑑∈[0,𝑇]
(4)
where β€– ⋅ β€– is the Euclidean norm, then if (1) has a solution,
it is a unique solution for this initial value problem.
To guarantee the existence of a unique solution of the
jump-diffusion SDDE (1), we assume that the coefficients of
(1) satisfy the following Lipschitz conditions:
󡄨󡄨
󡄨 󡄨
󡄨
󡄨
󡄨
󡄨󡄨a (𝑑, y1 , z1 ) − a (𝑑, y2 , z2 )󡄨󡄨󡄨 ≤ 𝐢1 (󡄨󡄨󡄨y1 − y2 󡄨󡄨󡄨 + 󡄨󡄨󡄨z1 − z2 󡄨󡄨󡄨) ,
󡄨󡄨
󡄨 󡄨
󡄨
󡄨
󡄨
󡄨󡄨b (𝑑, y1 , z1 ) − b (𝑑, y2 , z2 )󡄨󡄨󡄨 ≤ 𝐢2 (󡄨󡄨󡄨y1 − y2 󡄨󡄨󡄨 + 󡄨󡄨󡄨z1 − z2 󡄨󡄨󡄨) ,
󡄨
󡄨2
∫ 󡄨󡄨󡄨c (𝑑, y1 , z1 , 𝜐) − c (𝑑, y2 , z2 , 𝜐)󡄨󡄨󡄨 πœ‘ (π‘‘πœ)
πœ€
2
(5)
2
≤ 𝐢3 ((𝑦1 − 𝑦2 ) + (𝑧1 − 𝑧2 ) )
for 𝑑 ∈ [0, 𝑇] and x1 , x2 , y1 , y2 ∈ R𝑑 , as well as the growth
conditions
󡄨
󡄨󡄨
󡄨 󡄨
󡄨󡄨a (𝑑, y, z)󡄨󡄨󡄨 ≤ 𝐷1 (1 + 󡄨󡄨󡄨y󡄨󡄨󡄨 + |z|) ,
󡄨
󡄨󡄨
󡄨 󡄨
󡄨󡄨b (𝑑, y, z)󡄨󡄨󡄨 ≤ 𝐷2 (1 + 󡄨󡄨󡄨y󡄨󡄨󡄨 + |z|) ,
(6)
󡄨2
󡄨
∫ 󡄨󡄨󡄨c (𝑑, y, z, 𝜐)󡄨󡄨󡄨 πœ‘ (π‘‘πœ) ≤ 𝐷3 (1 + 𝑦2 + 𝑧2 )
πœ€
2. Preliminaries
In this section, we present some basic concepts and definitions to be used in later sections, then establish the conditions
for the existence and uniqueness of solution to the Jumpdiffusion SDDEs (1), and then give some lemmas to be used
later for the proof of the convergence theorem. In this work,
we assume that the 𝑑-dimensional vector valued function for
the initial condition, πœ’ = {πœ’(𝑠), 𝑠 ∈ [−𝛾, 0]}, is right continuous and has left-hand limits.
From (1), we have the following integral form of the jumpdiffusion equation SDDE:
𝑑
X (𝑑) = X (0) + ∫ a (𝜏, X (𝜏) , X (𝜏 − 𝛾)) π‘‘πœ
𝑑
0
π‘πœ‘ (𝑑)
+ ∑ c (πœπ‘– , X (πœπ‘–− ) , πœ‰π‘– ) ,
𝑖=1
󡄨2
󡄨
σ΅„© σ΅„©2
𝐸 (σ΅„©σ΅„©σ΅„©πœ‚σ΅„©σ΅„©σ΅„©C ) = 𝐸 ( sup σ΅„¨σ΅„¨σ΅„¨πœ‚ (𝑠)󡄨󡄨󡄨 ) < ∞.
𝑠∈[−𝛾,0]
(7)
Following the work in [7, 10], the following theorem can
be established for the existence and uniqueness of a solution
to the problem defined by (1) and (2).
0
+ ∫ b (𝜏, X (𝜏) , X (𝜏 − 𝛾)) 𝑑W𝜏
for y, z ∈ R𝑑 , 𝑑 ∈ [0, 𝑇].
We denote by C = C([−𝛾, 0], R𝑑 ) the Banach space of all
𝑑-dimensional continuous functions πœ‚ on [−𝛾, 0] equipped
with the supremum norm β€–πœ‚β€–C = sup𝑠∈[−𝛾,0] |πœ‚(𝑠)|. Furthermore, we suppose that the set 𝐿 2 (Ω, C, A0 ) of R𝑑 -valued
continuous process πœ‚ = {πœ‚(𝑠), 𝑠 ∈ [−𝛾, 0]} is A0 -measurable
with
(3)
Theorem 2. Suppose that the Lipschitz conditions and the
growth conditions are satisfied, and the initial condition πœ’ is
in 𝐿 2 (Ω, C, A0 ). Then (1) subject to the initial condition (2)
admits a unique solution.
Abstract and Applied Analysis
3
Now we present some lemmas to be used later for the
proof of the convergence theorem. Consider a right continuous process π‘ŒΔ π‘™ = {π‘ŒΔ π‘™ (𝑑), 𝑑 ∈ [−𝛾, 𝑇]}. π‘ŒΔ π‘™ is called a discrete-time numerical approximation with maximum step size
Δ π‘™ , if it is obtained by using a time discretization π‘‘Δ π‘™ , and
Δ
the random variable π‘Œπ‘‘π‘› 𝑙 is F𝑑𝑛 -measurable for 𝑛 ∈ {1, . . . ,
Δ
Δ
𝑁}. Further, π‘Œπ‘‘π‘›+1𝑙 can be expressed as a function of π‘Œπ‘‘−𝑙𝑙 ,
Δ𝑙
Δ
, . . . , π‘Œπ‘‘π‘› 𝑙
π‘Œπ‘‘−𝑙+1
and the discrete-time 𝑑𝑛 .
Because of dealing with the approximation of solutions of
jump-diffusion SDDEs, we introduce a concept of weak order
convergence due to Kloeden and Platen [15].
Definition 3. A discrete-time approximation π‘ŒΔ π‘™ converges
weakly towards 𝑋 at time 𝑇 with order 𝛽 > 0 if for each 𝑔 ∈
C𝑝 there is a constant 𝐢, independent of Δ π‘™ , such that
󡄨󡄨
󡄨
󡄨󡄨𝐸 (𝑔 (𝑋 (𝑇))) − 𝐸 (𝑔 (π‘ŒΔ π‘™ (𝑇)))󡄨󡄨󡄨 ≤ 𝐢(Δ π‘™ )𝛽 ,
󡄨
󡄨
(8)
where C𝑝 denotes the set of all polynomials 𝑔 : R𝑑 → R.
We now give some auxiliary results to prepare for the
proof of the weak convergence theorem to be presented.
Lemma 4. For 𝑛 ∈ {−𝑙 + 1, . . . , 0, 1, . . . , 𝑁} and z ∈ R𝑑 , we
have
+∫
(9)
∫
𝑛−1 πœ€
𝑛−1,𝑧
L−1
) πœ‘ (π‘‘πœ) π‘‘πœ
𝜐 𝑒 (𝜏, X𝜏
| A𝑛−1 ) = 0
for (𝜏, z) ∈ [−𝛾, 𝑑] × R𝑑 and 𝑒(𝜏, z) = 𝐸(𝑔(Xπ‘‡πœ,𝑧 )A𝜏 ).
The proof of the lemma for the case with no delay was
established by Platen and Bruti-Liberati [21], and a similar
procedure can be used for the proof of this lemma.
Lemma 5. Given 𝑝 ∈ {1, 2, 3, . . .}, there is a bounded constant
𝑀 satisfying
󡄨2π‘ž Μƒ
󡄨
π‘ž
2π‘ž
− z󡄨󡄨󡄨󡄨 | A
𝐸 (󡄨󡄨󡄨󡄨X𝑛𝑛−1,𝑧
−
𝑛−1 ) ≤ 𝑀 (1 + |z| ) (Δ π‘™ )
(10)
for π‘ž ∈ {1, . . . , 𝑝} and 𝑛 ∈ {−𝑙 + 1, . . . , 0, 1, . . . , 𝑁}.
The proof of (10) can be obtained by following that
of a lemma for SDEs with jumps but with no delay in
[15]. The following results are similar to what was given in
Mikulevičius and Platen [22].
Lemma 6. Given 𝑝 ∈ {1, 2, 3, . . .}, there is a finite constant 𝑀
satisfying
󡄨 󡄨2π‘ž
𝐸 ( sup |𝜁 (𝑑)|2π‘ž ) ≤ 𝑀 (1 + 󡄨󡄨󡄨Y0 󡄨󡄨󡄨 )
−𝛾≤𝑑≤𝑇
for every π‘ž ∈ {1, . . . , 𝑝}.
󡄨󡄨 󡄨
󡄨󡄨
󡄨2π‘ž
Δ
󡄨󡄨
󡄨󡄨 󡄨󡄨
Δ σ΅„¨2π‘ž
𝑧,π‘Œ 𝑙
Δ σ΅„¨
̃𝑧 )󡄨󡄨󡄨
󡄨󡄨𝐸 (󡄨󡄨Fp (𝜁 (𝑧) − Y𝑧 𝑙 )󡄨󡄨󡄨󡄨 + 󡄨󡄨󡄨󡄨Fp (X𝑧 𝑧 − Y𝑧 𝑙 )󡄨󡄨󡄨󡄨 | A
󡄨󡄨
󡄨󡄨
󡄨
󡄨
󡄨
󡄨 󡄨2π‘Ÿ
π‘žπ‘˜
≤ 𝑀 (1 + 󡄨󡄨󡄨󡄨YΔ𝑧 𝑙 󡄨󡄨󡄨󡄨 ) (Δ π‘™ )
(12)
for each π‘ž ∈ {1, . . . , 𝑝}, π‘˜ ∈ {1, . . . , 2(𝛽 + 1)}, p ∈ π‘ƒπ‘˜ = {1, 2, ...,
𝑑}π‘˜ , and 𝑧 ∈ [−π‘Ÿ, 𝑇], where 𝐹p (y) = ∏π‘˜β„Ž=1 π‘¦π‘β„Ž for all y = (𝑦1 ,
..., 𝑦𝑑 )𝑇 ∈ R𝑑 and p = (𝑝1 , ..., π‘π‘˜ ) ∈ π‘ƒπ‘˜ .
The proof of estimate (12) can be established by following
ItoΜ‚’s formula for SDEs with jumps but with no delay as in [15].
Lemma 8. For p ∈ π‘ƒπ‘˜ , there exist π‘Ÿ ∈ {1, 2, . . .} and a finite
constant 𝑀 satisfying
󡄨󡄨
󡄨󡄨
Δ
𝑛−1,π‘Œ 𝑙
Δ𝑙
󡄨󡄨
̃𝑑 )󡄨󡄨󡄨
) − FP (X𝑑 𝑛−1 − YΔ𝑑𝑛−1 ) | A
󡄨󡄨𝐸 (FP (𝜁 (𝑑) − Y𝑛−1
󡄨󡄨
󡄨󡄨
󡄨 (13)
󡄨󡄨 Δ π‘™ σ΅„¨σ΅„¨π‘Ÿ
𝛽
≤ 𝑀 (1 + 󡄨󡄨󡄨Y𝑛−1 󡄨󡄨󡄨 ) (Δ π‘™ )
for each π‘˜ ∈ {1, . . . , 2𝛽 + 1}, 𝑛 ∈ {−𝑙 + 1, . . . , 0, 1, . . . , 𝑁}, and
𝑑 ∈ [𝑑𝑛−1 , 𝑑𝑛 ).
3. The Jump-Adapted Weak Taylor
Approximation Scheme
) − 𝑒 (𝑛 − 1, z)
𝐸 (𝑒 (𝑛, X𝑛𝑛−1,𝑧
−
𝑛
Lemma 7. Given 𝑝 ∈ {1, 2, . . .}, there is π‘Ÿ ∈ {1, 2, 3, . . .} and a
bounded constant 𝑀 satisfying
(11)
In Monte Carlo simulations for functionals of jump-diffusion
SDDEs, one uses numerical approximations evaluated only at
discretization time. Here, we first give a jump adapted weak
approximation Taylor scheme of order 𝛽, and then study the
basic properties of the discrete Taylor approximation in a
weak order sense.
First we define the jump-adapted time discretization. Let
𝑇 > π‘Ÿ > 0. The jump adapted time discretization used
throughout this paper is
(𝑑)Δ = {𝑑𝑖 : 𝑖 = −𝑙, −𝑙 + 1, . . . , 0, 1, 2, . . . , 𝑁}
(14)
with the maximum step size Δ π‘™ ∈ (0, 1). We choose the time
discretization in such a way that all jump times are at the
nodes of the time discretization. If the discretization node 𝑑𝑖
is not a jump time, then 𝑑𝑖 is A𝑑𝑖−1 -measurable. Otherwise, 𝑑𝑖 is
A𝑑𝑖− -measurable. Also, throughout the paper, we denote the
set of all multiindices 𝛼 by
Mπ‘š = {(𝑗1 , . . . , 𝑗𝑙 ) : 𝑗𝑖 ∈ {0, 1, 2, . . . , π‘š} , 𝑖 ∈ {1, 2, . . . , 𝑙}
for 𝑙 ∈ N} ∪ {V} ,
(15)
where the element 𝛼 = (𝑗1 , 𝑗2 , . . . , 𝑗𝑙 ) is called a multiindex of
length 𝑙 = 𝑙(𝛼) ∈ N and V has zero length. In the following,
by a component 𝑗 ∈ {0, 1, 2, . . . , π‘š} of a multi-index we refer
to the integration with respect to the 𝑗th Wiener process in a
multiple stochastic integral. A component with 𝑗 = 0 corresponds to integration with respect to time 𝑑.
4
Abstract and Applied Analysis
Now define the following operators for the coefficient
functions:
𝐿0 =
𝑑
𝑑
πœ•
πœ•
πœ•
+ ∑π‘Žπ‘– (𝑑, π‘₯, π‘₯𝑙 ) 𝑖 + ∑π‘Žπ‘– (𝑑 − 𝑙, π‘₯𝑙 , π‘₯2𝑙 ) 𝑖
πœ•π‘‘ 𝑖=1
πœ•π‘₯ 𝑖=1
πœ•π‘₯𝑙
+
2(𝛽+1)
Proof. For 𝛽 ∈ {1, 2, 3, . . .} and 𝑔 ∈ C𝑝
the ItoΜ‚ process below:
1 𝑑 π‘š 𝑖𝑗
πœ•2
∑ ∑ 𝑏 (𝑑, π‘₯, π‘₯𝑙 ) 𝑏𝛾𝑗 (𝑑, π‘₯, π‘₯𝑙 ) 𝑖 𝛾
2 𝑖,𝛾=1 𝑗=1
πœ•π‘₯ πœ•π‘₯
𝑑
π‘š
2(𝛽+1)
(R𝑑 , R) there is a positive
and 𝛼 ∈ Γ𝛽 . Then for any 𝑔 ∈ C𝑃
constant 𝐢, which does not depend on Δ, such that
󡄨󡄨
󡄨
󡄨󡄨𝐸 (𝑔 (𝑋 (𝑇))) − 𝐸 (𝑔 (π‘ŒΔ π‘™ (𝑇)))󡄨󡄨󡄨 ≤ 𝐢(Δ π‘™ )𝛽 .
(20)
󡄨
󡄨
𝑧,𝑦
X𝑑
𝑑
πœ•
πœ•
πΏπ‘˜ = ∑π‘π‘–π‘˜ (𝑑, π‘₯, π‘₯𝑙 ) 𝑖 + ∑π‘π‘–π‘˜ (𝑑 − 𝑙, π‘₯𝑙 , π‘₯2𝑙 ) 𝑖 .
πœ•π‘₯ 𝑖=1
πœ•π‘₯𝑙
𝑖=1
(16)
A subset A ∈ M is the hierarchical set, and its corresponding remainder set 𝐴(M) is defined by 𝐴(M) = {𝛼 ∈
Mπ‘š \A : −𝛼 ∈ A}. For each 𝛽 ∈ 1, 2, 3, . . ., we can then define
the hierarchical set Γ𝛽 = {𝛼 ∈ Mπ‘š : 𝑙(𝛼) ≤ 𝛽}. The weak
Taylor method of order 𝛽 is then constructed as follows:
Y(𝑛+1)− = Y𝑛 + ∑ 𝑓𝛼 (𝑛, Y𝑛 , Y𝑛−𝑙 ) 𝐼𝛼 ,
(17)
Y𝑛+1 = Y(𝑛+1)− + ∫ 𝑐 (𝑛, Y(𝑛+1)− , 𝜐) π‘πœ‘ (π‘‘πœ, (𝑛 + 1)) ,
πœ€
where
(18)
The multiple stochastic integral is then defined recursively as follows:
𝐼𝛼,𝑑
if 𝑙 = 0
if 𝑙 ≥ 1, 𝑗𝑙 = 0
𝑧
+∫ ∫
𝑧
πœ€
𝑧,𝑦
c (X𝑒−
, 𝜐) π‘πœ‘
(21)
(π‘‘πœ, 𝑑𝑒) .
0,𝑋
Then we can get 𝑒(0, 𝑋0 ) = 𝐸(𝑔(𝑋𝑇 0 )) = 𝐸(𝑔(𝑋𝑇 )).
Define also the process 𝜁 = 𝜁(𝑑), 𝑑 ∈ (−𝛾, 𝑇), by
𝑑
𝑑
{
{
𝑑
{
{
{∫ 𝐼 𝑑𝑧
= { 0 𝛼−,𝑧
{ 𝑑
{
{
{∫ 𝐼 π‘‘π‘Šπ‘—π‘™
{ 0 𝛼−,𝑧 𝑧
𝑧
𝑑
1
πœ•
+ ∑ ∑ 𝑏𝑖𝑗 (𝑑 − 𝑙, π‘₯𝑙 , π‘₯2𝑙 ) 𝑏𝛾𝑗 (𝑑 − 𝑙, π‘₯𝑙 , π‘₯2𝑙 ) 𝑖 𝛾 ,
2 𝑖,𝛾=1 𝑗=1
πœ•π‘₯𝑙 πœ•π‘₯𝑙
𝑓 (𝑑, π‘₯)
if 𝑙 (𝛼) = 0
{
{ 𝑗
1
𝑓𝛼 (𝑑, π‘₯, 𝑒) = {𝐿 𝑓−𝛼 (𝑑, π‘₯, 𝑒) if 𝑙 (𝛼) ≥ 1,
{
𝑗1 ∈ 0, 1, . . . , π‘š.
{
𝑑
= y + ∫ a (X𝑒𝑧,𝑦 ) 𝑑𝑒 + ∫ b (X𝑒𝑧,𝑦 ) 𝑑W𝑒
2
𝛼∈Γ𝛽
𝑑
(R𝑑 , R), consider
(19)
if 𝑙 ≥ 1, 𝑗𝑙 ∈ 1, . . . , π‘š,
𝜁 (𝑑) = 𝜁 (𝑑𝑛 ) + ∑ 𝐼𝛼 (𝑓𝛼 (𝑛, πœπ‘› , πœπ‘›−𝑙 ))
𝛼∈Γ𝛽
+ ∫ ∫ 𝑐 (𝑛, 𝜁(𝑛+1)− , 𝜐) π‘πœ‘ (π‘‘πœ, (𝑛 + 1))
𝑛
2(𝛽+1)
(R𝑑 , R),
that the coefficients, π‘Žπ‘˜ , π‘π‘˜π‘— , π‘π‘˜ , are in the space C𝑃
for 𝑗 ∈ {1, 2, . . . , π‘š} and π‘˜ ∈ {1, 2, . . . , 𝑑}, and the coefficient
functions 𝑓𝛼 , with 𝑓(𝑑, y) = y, satisfy the growth condition
|𝑓𝛼 (𝑑, y)| ≤ 𝑀(1 + |y|), with 𝑀 < ∞, for all 𝑑 < 𝑇, y ∈ R𝑑 ,
πœ€
for 𝑛 ∈ {−𝑙, −𝑙+1, . . . , 0, 1, . . . , 𝑁−1}, 𝑑 ∈ (𝑑𝑛 , 𝑑𝑛+1 ], 𝜁(0) = π‘Œ0 ,
and 𝜁(𝑑𝑛 ) = π‘Œπ‘‘π‘› for 𝑛 ∈ {−𝑙, . . . , 0, 1, 2, . . . , 𝑁}.
By the definition of the functional 𝑒 and the terminal
condition of the stochastic process 𝑋, we have
󡄨
󡄨
Δ
𝐻 = 󡄨󡄨󡄨󡄨𝐸 (𝑔 (Y𝑇 𝑙 )) − 𝐸 (𝑔 (X𝑇 ))󡄨󡄨󡄨󡄨
(23)
󡄨
󡄨
Δ
= 󡄨󡄨󡄨󡄨𝐸 (𝑒 (𝑇, Y𝑇 𝑙 ) − 𝑒 (0, X0 ))󡄨󡄨󡄨󡄨 .
Since Y0 converges towards X0 weakly with order 𝛽, one
has
󡄨󡄨
𝑁
󡄨󡄨
𝐻 ≤ 󡄨󡄨󡄨𝐸 ( ∑ (𝑒 (𝑛, Y𝑛 ) − 𝑒 (𝑛, Y𝑛− ) + 𝑒 (𝑛, Y𝑛− )
󡄨󡄨
𝑛=−𝑙+1
󡄨
(24)
󡄨󡄨
󡄨󡄨
𝛽
− 𝑒 (𝑛 − 1, Y𝑛−1 )) )󡄨󡄨󡄨 + 𝐾(Δ π‘™ ) .
󡄨󡄨
󡄨
By Lemma 4, we can write
󡄨󡄨
𝑁
󡄨󡄨
𝐻 ≤ 󡄨󡄨󡄨𝐸 ( ∑ { [𝑒 (𝑛, Y𝑛 ) − 𝑒 (𝑛, Y𝑛− )
󡄨󡄨
𝑛=−𝑙+1
󡄨
+𝑒 (𝑛, Y𝑛− ) − 𝑒 (𝑛 − 1, Y𝑛−1 )]
𝑛−1,π‘Œπ‘›−1
− [𝑒 (𝑛, X𝑛−
where 𝛼− is obtained from 𝛼 by deleting its last component,
while −𝛼 is obtained from 𝛼 by deleting its first component.
Now, we give the weak convergence theorem of the Taylor
approximation with order 𝛽.
Theorem 9. Given 𝛽 ∈ {1, 2, . . .}, let π‘ŒΔ π‘™ = {π‘Œπ‘›Δ π‘™ , 𝑛 ∈ [−𝑙, . . . ,
0, 1, . . . , 𝑁]} be the results obtained from the Taylor scheme
(17) corresponding to (t)Δ with maximum step size Δ l ∈ (0, 1).
Suppose that 𝐸(|Xπœ‰ |𝑖 ) < ∞ for πœ‰ ∈ (−𝛾, 0), 𝑖 ∈ {1, 2, . . .}, and
YΔπœ‰ converges to Xπœ‰ weakly with order 𝛽 ∈ {1, 2, . . .}. Assume
(22)
𝑑
+∫
𝑛
) − 𝑒 (𝑛 − 1, Y𝑛−1 )
𝑛−1,π‘Œπ‘›−1
)
∫ L−1
𝜐 𝑒 (𝑧, X𝑧
𝑛−1 πœ€
󡄨󡄨
󡄨󡄨
𝛽
×πœ‘ (π‘‘πœ) 𝑑𝑧] } )󡄨󡄨󡄨 + 𝐾(Δ π‘™ ) .
󡄨󡄨
󡄨
(25)
From the properties of stochastic integrals, we obtain
𝑁
𝐸 ( ∑ [𝑒 (𝑛, Y𝑛 ) − 𝑒 (𝑛, Y𝑛− )])
𝑛=−𝑙
(26)
𝑇
= 𝐸 (∫ ∫
−π‘Ÿ πœ€
L−1
𝜐 𝑒 (𝑧, 𝜁 (𝑧)) πœ‘ (π‘‘πœ) 𝑑𝑧) .
Abstract and Applied Analysis
5
π‘˜,π‘˜
(Z) ∈ (0, 1)
where πœƒp,𝑛 (Z) is a 𝑑 × π‘‘ diagonal matrix with πœƒp,𝑛
Therefore, we have
𝑛−1,π‘Œ
𝛽
𝐻 ≤ 𝐻1 + 𝐻2 + 𝐾(Δ π‘™ ) ,
(27)
where
󡄨󡄨
𝑁
󡄨󡄨
𝐻1 = 󡄨󡄨󡄨𝐸 ( ∑ { [𝑒 (𝑛, Y𝑛− ) − 𝑒 (𝑛, Y𝑛−1 )]
󡄨󡄨
𝑛=−𝑙+1
󡄨
for π‘˜ ∈ {1, 2, 3, . . . , 𝑑} and Z = Y𝑛− and X𝑛− 𝑛−1 , respectively.
Therefore, according to the properties of expectation and
absolute value, we get
𝑁
2𝛽+1
𝑛=−𝑙+1
π‘˜=1
𝐻1 ≤ 𝐸 ( ∑ { ∑
󡄨󡄨
󡄨󡄨
𝑛−1,π‘Œ
− [𝑒 (𝑛, X𝑛− 𝑛−1 ) − 𝑒 (𝑛, Y𝑛−1 )]} )󡄨󡄨󡄨 ,
󡄨󡄨
󡄨
1
󡄨
󡄨
∑ 󡄨󡄨󡄨󡄨(πœ•π‘¦p 𝑒 (𝑛, Y𝑛−1 ))󡄨󡄨󡄨󡄨
π‘˜! p∈π‘ƒπ‘˜
× (𝐹p (Y𝑛− − Y𝑛−1 )
(28)
𝑛−1,π‘Œπ‘›−1
−𝐹p (X𝑛−
󡄨󡄨
𝑇
󡄨
−1
𝐻2 = 󡄨󡄨󡄨󡄨𝐸 (∫ ∫ {[𝐿−1
𝜐 𝑒 (𝑧, 𝜁 (𝑧)) − 𝐿 𝜐 𝑒 (𝑧, Y𝑧 )]
󡄨󡄨
−π‘Ÿ πœ€
󡄨
𝑛−1,π‘Œ
󡄨
󡄨 󡄨
× σ΅„¨σ΅„¨σ΅„¨π‘…π‘› (Y𝑛− )󡄨󡄨󡄨 + 󡄨󡄨󡄨󡄨𝑅𝑛 (X𝑛− 𝑛−1 )󡄨󡄨󡄨󡄨 })
𝑧,π‘Œπ‘§
−1
− [𝐿−1
𝜐 𝑒 (𝑧, X𝑧 ) − 𝐿 𝜐 𝑒 (𝑧, Y𝑧 )]} (29)
󡄨󡄨
󡄨
× πœ‘ (π‘‘πœ) 𝑑𝑧)󡄨󡄨󡄨󡄨 .
󡄨󡄨
− Y𝑛−1 ))
𝑁
2𝛽+1
𝑛=−𝑙+1
π‘˜=1
≤ 𝐸( ∑ { ∑
1
󡄨
󡄨
∑ 󡄨󡄨󡄨(πœ•p 𝑒 (𝑛, Y𝑛−1 ))󡄨󡄨󡄨󡄨
π‘˜! p∈π‘ƒπ‘˜ 󡄨 𝑦
In the following, we proceed to estimate 𝐻1 and 𝐻2 in
Steps 1 and 2, respectively, and then complete the proof in Step
3.
󡄨
× σ΅„¨σ΅„¨σ΅„¨σ΅„¨πΈ (𝐹p (Y𝑛− − Y𝑛−1 )
𝑛−1,π‘Œπ‘›−1
− 𝐹p (X𝑛−
Step 1. Let us assume that 𝑒 is so smooth that the deterministic Taylor expansion may be applied. Hence, by expanding
𝑑𝑒 in 𝐻1 , we get
̃𝑛−1 )󡄨󡄨󡄨󡄨
−Y𝑛−1 ) | A
󡄨
󡄨
󡄨 Μƒ
+ 𝐸 (󡄨󡄨󡄨𝑅𝑛 (Y𝑛− )󡄨󡄨󡄨 | A
𝑛−1 )
󡄨󡄨
𝑁 { 2𝛽+1
󡄨󡄨
1
󡄨
𝐻1 = 󡄨󡄨󡄨𝐸 ( ∑ {[ ∑
∑ (πœ•π‘¦P 𝑒 (𝑛, Y𝑛−1 ))
󡄨󡄨
π‘˜!
𝑛=−𝑙+1
󡄨󡄨
{[ π‘˜=1 P∈π‘ƒπ‘˜
󡄨
󡄨 Μƒ
𝑛−1,π‘Œ
+ 𝐸 (󡄨󡄨󡄨󡄨𝑅𝑛 (X𝑛− 𝑛−1 )󡄨󡄨󡄨󡄨 | A
𝑛−1 ) }) .
(32)
× πΉP (Y𝑛− − Y𝑛−1 )
By (31), the Hölder inequality, and Lemma 7, we get
+𝑅𝑛 (Y𝑛− ) ]
󡄨
󡄨 Μƒ
𝐸 (󡄨󡄨󡄨𝑅𝑛 (Y𝑛− )󡄨󡄨󡄨 | A
𝑛−1 )
2𝛽+1
1
−[∑
∑ (πœ•π‘¦P 𝑒 (𝑛, Y𝑛−1 ))
π‘˜!
[ π‘˜=1 P∈π‘ƒπ‘˜
×
𝑛−1,π‘Œ
𝐹P (X𝑛− 𝑛−1
≤𝑀 ∑
− Y𝑛−1 )
󡄨󡄨
󡄨󡄨
𝑛−1,π‘Œ
+ 𝑅𝑛 (X𝑛− 𝑛−1 ) ]})󡄨󡄨󡄨󡄨 ,
󡄨󡄨
󡄨
(30)
1
2 (𝛽 + 1)!
×
∑ πœ•π‘¦p 𝑒 (𝑛, Y𝑛−1 + πœƒp,𝑛 (Z − Y𝑛−1 ))
p∈𝑃2(𝛽+1)
× πΉp (Z − Y𝑛−1 ) ,
󡄨2 Μƒ
× (Y𝑛− −Y𝑛−1 ))󡄨󡄨󡄨 | A
𝑛−1 )]
1/2
1/2
󡄨
󡄨2 Μƒ
× [𝐸 (󡄨󡄨󡄨󡄨𝐹p (Y𝑛− − Y𝑛−1 )󡄨󡄨󡄨󡄨 | A
𝑛−1 )]
1/2
󡄨2π‘Ÿ 󡄨
󡄨2π‘Ÿ Μƒ
󡄨
≤ 𝑀[𝐸 (1 + 󡄨󡄨󡄨Y𝑛−1 󡄨󡄨󡄨 + 󡄨󡄨󡄨Y𝑛− − Y𝑛−1 󡄨󡄨󡄨 | A
𝑛−1 )]
where the remainder term is
𝑅𝑛 (Z) =
p∈𝑃2(𝛽+1)
󡄨
[𝐸 (σ΅„¨σ΅„¨σ΅„¨σ΅„¨πœ•π‘¦p 𝑒 (𝑛, Y𝑛−1 + πœƒp,𝑛 (Y𝑛− )
1/2
󡄨4(𝛽+1) Μƒ
󡄨
× [𝐸 (󡄨󡄨󡄨Y𝑛− − Y𝑛−1 󡄨󡄨󡄨
| A𝑛−1 )]
(31)
𝛽+1
󡄨2π‘Ÿ
󡄨
≤ 𝑀 (1 + 󡄨󡄨󡄨Y𝑛−1 󡄨󡄨󡄨 ) (Δ π‘™ ) .
(33)
6
Abstract and Applied Analysis
Similarly, by Lemma 5 and the Cauchy-Schwarz inequality, we have
𝑇
2𝛽+1
−π‘Ÿ πœ€
π‘˜=1
≤ ∫ ∫ 𝐸( ∑
󡄨 Μƒ
󡄨
𝑛−1,π‘Œ
𝐸 (󡄨󡄨󡄨󡄨𝑅𝑛 (X𝑛− 𝑛−1 )󡄨󡄨󡄨󡄨 | A
𝑛−1 )
󡄨
𝑛−1,π‘Œ
≤ 𝑀 ∑ [𝐸 (σ΅„¨σ΅„¨σ΅„¨σ΅„¨πœ•π‘¦p 𝑒 (𝑛, Y𝑛− + πœƒp,𝑛 (X𝑛− 𝑛−1 )
𝑛−1,π‘Œπ‘›−1
̃𝑧 )󡄨󡄨󡄨󡄨
− 𝐹p (X𝑧𝑧,π‘Œπ‘§ − Y𝑧 ) | A
󡄨
󡄨󡄨
󡄨󡄨 Μƒ
+ 𝐸 (󡄨󡄨𝑅𝑛 (𝜁 (𝑧))󡄨󡄨 | A𝑧 )
󡄨2 Μƒ
−Y𝑛−1 ))󡄨󡄨󡄨󡄨 | A
𝑛−1 )]
1/2
󡄨
󡄨 Μƒ
+𝐸 (󡄨󡄨󡄨󡄨𝑅𝑛 (X𝑧𝑧,π‘Œπ‘§ )󡄨󡄨󡄨󡄨 | A
𝑧 ) ) πœ‘ (π‘‘πœ) 𝑑𝑧.
1/2
󡄨
󡄨2 Μƒ
𝑛−1,π‘Œ
× [𝐸 (󡄨󡄨󡄨󡄨𝐹p (X𝑛− 𝑛−1 − Y𝑛−1 )󡄨󡄨󡄨󡄨 | A
𝑛−1 )]
1/2
󡄨2𝛾 Μƒ
󡄨2π‘Ÿ 󡄨 𝑛−1,π‘Œ
󡄨
≤ 𝑀[𝐸 (1 + 󡄨󡄨󡄨Y𝑛−1 󡄨󡄨󡄨 + 󡄨󡄨󡄨󡄨X𝑛− 𝑛−1 − Y𝑛−1 󡄨󡄨󡄨󡄨 | A
𝑛−1 )]
󡄨4(𝛽+1)
󡄨 𝑛−1,π‘Œ
× [𝐸 (󡄨󡄨󡄨󡄨X𝑛− 𝑛−1 − Y𝑛−1 󡄨󡄨󡄨󡄨
̃𝑛−1 )]
|A
1/2
𝛽+1
󡄨2π‘Ÿ
󡄨
≤ 𝑀 (1 + 󡄨󡄨󡄨Y𝑛−1 󡄨󡄨󡄨 ) (Δ π‘™ ) .
(36)
Similarly, we can estimate the reminders as follows:
󡄨󡄨 󡄨󡄨2π‘Ÿ
𝛽+1
󡄨 Μƒ
󡄨
,
𝐸 (󡄨󡄨󡄨𝑅𝑛 (𝜁 (𝑧))󡄨󡄨󡄨 | A
𝑧 ) ≤ 𝑀 (1 + 󡄨󡄨󡄨Y𝑑𝑧 󡄨󡄨󡄨 ) (𝑧 − 𝑑𝑧 )
(34)
Now, from the Cauchy-Schwarz inequality, Lemmas 8 and
6, and inequalities (33) and (34), we obtain
󡄨
󡄨 Μƒ
󡄨󡄨 󡄨󡄨2π‘Ÿ
𝛽+1
𝐸 (󡄨󡄨󡄨󡄨𝑅𝑛 (X𝑧𝑧,π‘Œπ‘§ )󡄨󡄨󡄨󡄨 | A
.
𝑧 ) ≤ 𝑀 (1 + 󡄨󡄨󡄨Y𝑑𝑧 󡄨󡄨󡄨 ) (𝑧 − 𝑑𝑧 )
𝐻2 ≤ 𝑀 ∫
𝑛=−𝑙+1
𝛽
󡄨 󡄨2𝛾
≤ 𝑀(Δ π‘™ ) (1 + 󡄨󡄨󡄨Y0 󡄨󡄨󡄨 ) ≤ 𝐾(Δ π‘™ ) .
𝛽
Step 2. Now we estimate the term 𝐻2 in inequality (27). By
the jump coefficient 𝑐 and the smooth function 𝑒, applying
the Taylor expansion yields
󡄨󡄨
2𝛽+1
𝑇
󡄨󡄨
1
𝐻2 = 󡄨󡄨󡄨󡄨𝐸 ( ∫ ∫ {[ ∑
∑ (πœ•π‘¦p 𝐿−1
𝜐 𝑒 (𝑧, Y𝑧 ))
π‘˜!
󡄨󡄨
−π‘Ÿ πœ€
p∈𝑃
π‘˜=1
π‘˜
󡄨
× πΉp (𝜁 (𝑧) − Y𝑑𝑧 )
+𝑅𝑛 (𝜁 (𝑧)) ]
2𝛽+1
−[∑
π‘˜=1
1
∑ (πœ•p 𝐿−1 𝑒 (𝑧, Y𝑧 ))
π‘˜! p∈𝑃 𝑦 𝜐
π‘˜
× πΉp (X𝑧𝑧,π‘Œπ‘§ − Y𝑑𝑧 )
󡄨󡄨
󡄨󡄨
+𝑅𝑛 (X𝑧𝑧,π‘Œπ‘§ ) ]} πœ‘ (π‘‘πœ) 𝑑𝑧)󡄨󡄨󡄨󡄨
󡄨󡄨
󡄨
𝑇
−π‘Ÿ
(35)
(37)
Then, by applying the Hölder inequality, Lemmas 8 and
6, inequalities (37) to estimate the inequality above, we get
𝑁
𝛽
󡄨
󡄨2𝛾
𝐻1 ≤ 𝐸 (𝐾 ∑ (1 + 󡄨󡄨󡄨Y𝑛−1 󡄨󡄨󡄨 ) (Δ π‘™ ) )
𝛽
󡄨 󡄨2𝛾
≤ 𝑀(Δ π‘™ ) (1 + 𝐸 ( max 󡄨󡄨󡄨Y𝑛 󡄨󡄨󡄨 ))
−𝑙≤𝑛≤𝑁
π‘˜
󡄨󡄨 p −1
󡄨
󡄨󡄨(πœ•π‘¦ 𝐿 𝜐 𝑒 (𝑧, Y𝑧 ))󡄨󡄨󡄨
󡄨
󡄨
󡄨
× σ΅„¨σ΅„¨σ΅„¨σ΅„¨πΈ (𝐹p (𝜁 (𝑧) − Y𝑧 )
p∈𝑃2(𝛽+1)
× (X𝑛−
1
∑
π‘˜! p∈𝑃
󡄨 󡄨2π‘Ÿ
𝛽
∫ 𝐸 (1 + 󡄨󡄨󡄨󡄨Y𝑑𝑧 󡄨󡄨󡄨󡄨 ) (Δ π‘™ ) πœ‘ (π‘‘πœ) 𝑑𝑧
πœ€
𝑇
󡄨 󡄨2π‘Ÿ
𝛽
≤ 𝑀(Δ π‘™ ) ∫ 𝐸 (1 + max 󡄨󡄨󡄨󡄨Y𝑑𝑛 󡄨󡄨󡄨󡄨 ) (𝑧 − 𝑑𝑧 ) 𝑑𝑧
0≤𝑛≤𝑛𝑇
0
(38)
𝛽
≤ 𝑀(Δ π‘™ ) .
Step 3. Finally, by inequalities (27) and (35) as well as (38), we
have
󡄨
󡄨󡄨
󡄨󡄨𝐸 (𝑔 (𝑋 (𝑇))) − 𝐸 (𝑔 (π‘ŒΔ π‘™ (𝑇)))󡄨󡄨󡄨 ≤ 𝑀(Δ π‘™ )𝛽 .
󡄨
󡄨
(39)
4. A Numerical Example
Here we give an illustrative example to demonstrate the application and the convergence of the proposed numerical
scheme. We consider the following linear SDDE with Poisson
jumps:
𝑑𝑋𝑑 = [(πœ‡ − ]πœ†) 𝑋𝑑 + 𝛼𝑋𝑑−1 ] 𝑑𝑑
+ [πœŽπ‘‹π‘‘ + 𝛽𝑋𝑑−1 ] π‘‘π‘Šπ‘‘ + ]𝑋𝑑 𝑑𝑁,
𝑋 (𝑑) = 𝑑 + 1,
(40)
𝑑 ∈ [−1, 0] ,
where πœ‡, 𝜎, and ] are, respectively, the drift coefficient, the
diffusion coefficient and the jump coefficient; πœ† is the jump
intensity; and 𝛼 and 𝛽 are the delay coefficients.
Abstract and Applied Analysis
7
Table 1: Convergence results for the linear SDDE with jumps.
8
Stepsize 1/β„Ž
Weak error1
Weak error2
210
0.00201
0.00142
2
0.00352
0.00229
212
0.00156
0.00061
214
0.00114
0.00020
By the method for solving linear stochastic differential
equations in [23], the analytical solution for 𝑑 ∈ [0, 1] is
derived as follows:
4.5
𝑑
3.5
+ ∫ Φ(𝑠)−1 π›½π‘ π‘‘π‘Šπ‘  ) ,
0
220
0.00031
0.00002
3
𝑋, π‘Œ1 , π‘Œ2
(41)
𝑑
218
0.00060
0.00004
4
𝑋 (𝑑) = Φ (𝑑) (1 + ∫ Φ(𝑠)−1 (𝛼 − πœŽπ›½) 𝑠𝑑𝑠
0
216
0.00082
0.00009
2.5
2
where
Φ (𝑑) = (] + 1)
𝑁(𝑑)
𝜎2
exp {(πœ‡ − ]πœ† − ) 𝑑 + πœŽπ‘Šπ‘‘ } .
2
1.5
(42)
According to the weak Taylor approximation scheme
(17)–(19) proposed in Section 3, we now expand it with weak
order 1 (well known as Euler scheme):
π‘Œ(𝑛+1)− = π‘Œπ‘› + ((πœ‡ − ]πœ†) π‘Œπ‘› + π›Όβ„Žπ‘›) β„Ž + (πœŽπ‘Œπ‘› + π›½β„Žπ‘›) Δπ‘Šπ‘› ,
π‘Œπ‘›+1 = π‘Œ(𝑛+1)− + ]π‘Œπ‘› Δ𝑁𝑛 .
(43)
Here we have used the jump adapted time discretization, and
β„Ž is the maximum step size.
For higher accuracy and efficiency, one needs to construct
higher order numerical schemes. We now give a Taylor
scheme of weak order two below:
π‘Œ(𝑛+1)− = π‘Œπ‘› + ((πœ‡ − ]πœ†) π‘Œπ‘› + π›Όβ„Žπ‘›) β„Ž
+ (πœŽπ‘Œπ‘› + π›½β„Žπ‘›) Δπ‘Šπ‘›
+ ((πœ‡ − ]πœ†) (πœŽπ‘Œπ‘› + π›½β„Žπ‘›)
β„Ž
+ 𝜎 ((πœ‡ − ]πœ†) π‘Œπ‘› + π›Όβ„Žπ‘›)) Δπ‘Šπ‘›
2
+ (πœ‡ − ]πœ†) ((πœ‡ − ]πœ†) π‘Œπ‘› + π›Όβ„Žπ‘›)
(44)
2
β„Ž
2
0.5
0
0.2
0.4
0.6
0.8
1
𝑑
Explicit solution path
Euler approximation
Second order approximation
Figure 1: Sample paths of linear SDDE with jumps.
number depends on the implemented scheme. We use the
following parameters: 𝛼 = 0.01, 𝛽 = 0.01, πœ‡ = 0.001, 𝜎 = 0.6,
] = 0.002, and πœ† = 0.001.
In Figure 1, we give the sample paths under the two
approximation schemes and the numerical explicit solution
of (40). We can see from the figure that the weak Taylor
scheme path is closer to the analytical solution line than the
Euler scheme.
Now we present the numerical errors generated by the
two numerical schemes presented above. From Table 1, we
notice that, for all the step sizes used in the numerical experiments, the weak Taylor method is more accurate. Moreover,
the errors of the weak order two Taylor method decrease
faster than the Euler scheme.
5. Conclusions
2
(Δπ‘Šπ‘› ) − β„Ž
+ 𝜎 (πœŽπ‘Œπ‘› + π›½β„Žπ‘›)
,
2
π‘Œπ‘›+1 = π‘Œ(𝑛+1)− + ]π‘Œπ‘› Δ𝑁𝑛 .
Next, we study the convergence of the two numerical
schemes presented above by using the weak errors measured
by
πœ€ (β„Ž) = |𝐸 (𝑋 (𝑇)) − 𝐸 (π‘Œ (𝑇))|
1
(45)
and compare the results obtained from these two schemes to
the explicit exact solution. We estimate the weak errors πœ€(β„Ž)
by running a very large number of simulations. The exact
In this work, we have extended previous research on weak
convergence to a more general class of stochastic differential
equations involving both jumps and time delay. We proved
that under the Poisson random measure and a fixed time
delay, a simplified Taylor method gives weak convergence rate
arbitrarily close to order 𝛽. There is much scope for further
work in the context of weak solution of jump-diffusion
SDDEs. For example, it is clearly of great importance to
extend the weak convergence theory to the case where coefficients in the equations are not globally Lipschitz, and to
develop and analyze new methods that maintain good properties of convergence and stability.
8
Acknowledgments
The authors thank the anonymous referees and the editors
for their constructive comments and suggestions. Yanli Zhou
acknowledges financial support from Curtin International
Postgraduate Research Scholarship (CIPRS) and Chinese
Scholarship Council (CSC). Acknowledgement is also made
to the China National Social Science Foundation (SSF) for the
research support (10BJY104).
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