Research Article Poincaré Map and Periodic Solutions of First-Order Impulsive

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Hindawi Publishing Corporation
Abstract and Applied Analysis
Volume 2013, Article ID 382592, 11 pages
http://dx.doi.org/10.1155/2013/382592
Research Article
Poincaré Map and Periodic Solutions of First-Order Impulsive
Differential Equations on Moebius Stripe
Yefeng He and Yepeng Xing
Department of Mathematics, Shanghai Normal University, Shanghai 200234, China
Correspondence should be addressed to Yepeng Xing; ypxing-jason@hotmail.com
Received 12 December 2012; Accepted 1 January 2013
Academic Editor: Yonghui Xia
Copyright © 2013 Y. He and Y. Xing. 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.
This paper is mainly concerned with the existence, stability, and bifurcations of periodic solutions of a certain scalar impulsive
differential equations on Moebius stripe. Some sufficient conditions are obtained to ensure the existence and stability of oneside periodic orbit and two-side periodic orbit of impulsive differential equations on Moebius stripe by employing displacement
functions. Furthermore, double-periodic bifurcation is also studied by using Poincaré map.
1. Introduction
Many systems in physics, chemistry, biology, and information
science have impulsive dynamical behavior due to abrupt
jumps at certain instants during the evolving processes. This
complex dynamical behavior can be modeled by impulsive
differential equations. The theory of impulsive differential
systems has been developed by numerous mathematicians
(see [1–9]). As to the stability theory and boundary value
problems to impulsive differential equations, There have been
extensive studies in this area. However, there are very few
works on the qualitative theory of impulsive differential
equations and impulsive semidynamical systems. Recently,
Bonotto and Federson have given a version of the PoincaréBendixson Theorem for impulsive semidynamical systems
in [10, 11]. As it is known, the method of Poincaré map
plays an important role in the research of qualitative theory
and is a natural means to study the existence of periodic
solutions and its asymptotic stability. However, due to the
complexity of the associated impulsive dynamic models, this
approach has only been applied successfully to Raibert’s
one-legged-hopper (see [12–14]) predator-prey models (see
[15–18]), and so forth. The bifurcation theory for ordinary
differential equations or smooth systems appeared during the
last decades (see, e.g., [19]); however, little is known about
the bifurcation theory of impulsive differential equations due
to its complexity (see [20]). In this paper, we mainly study
a certain scalar impulsive differential equations on Moebius
stripe undergoing impulsive effects at fixed time:
𝑑π‘₯
= 𝑓 (𝑑, π‘₯) ,
𝑑𝑑
Δπ‘₯|𝑑=πœπ‘˜ = πΌπ‘˜ (π‘₯) ,
𝑑 =ΜΈ πœπ‘˜ ,
(1)
π‘˜ ∈ Z+ ,
where 0 ≤ πœπ‘˜ < πœπ‘˜+1 , π‘˜ ∈ Z+ are fixed with πœπ‘˜ → +∞
as, π‘˜ → +∞, and Δπ‘₯|𝑑=πœπ‘˜ = π‘₯(πœπ‘˜+ ) − π‘₯(πœπ‘˜ ). Hu and Han
(see [20]) investigated the existence of periodic solutions and
bifurcations of (1) under the assumptions that 𝑓(𝑑, π‘₯) and
πΌπ‘˜ (π‘₯) are periodic; that is, the following assumption holds.
(H∗ ) There exist a constant 𝑇 > 0, a positive integer π‘ž,
and two mutual coprime positive integers π‘š and 𝑛 such that
𝑓 (𝑑 + 𝑇, π‘₯) = 𝑓 (𝑑, π‘₯) ,
∀𝑑 ∈ R+ , π‘₯ ∈ R,
πΌπ‘˜+π‘ž (π‘₯) = πΌπ‘˜ (π‘₯) , πœπ‘˜+π‘ž − πœπ‘˜ = 𝑇,
π‘š (π‘‘π‘˜+π‘ž − π‘‘π‘˜ ) = 𝑛𝑇,
∀π‘˜ ∈ Z+ , π‘₯ ∈ R, (2)
π‘˜ ≥ 1.
In this paper, we assume that the following conditions hold.
(H1) Assume that both 𝑓(𝑑, π‘₯) and 𝑓π‘₯ (𝑑, π‘₯) are continuous
scalar functions on R × R, πΌπ‘˜ (π‘₯) : R → R, π‘˜ ∈ Z are odd,
continuous functions; that is, πΌπ‘˜ (−π‘₯) = −πΌπ‘˜ (π‘₯), π‘˜ ∈ Z+ .
2
Abstract and Applied Analysis
(H2) There exists a constant 𝑇 > 0, a positive integer π‘ž
such that
𝑓 (𝑑 + 𝑇, −π‘₯) = −𝑓 (𝑑, π‘₯) ,
∀𝑑 ∈ R, π‘₯ ∈ R,
πΌπ‘˜+π‘ž (π‘₯) = πΌπ‘˜ (π‘₯) , πœπ‘˜+π‘ž − πœπ‘˜ = 𝑇,
+
∀π‘˜ ∈ Z , π‘₯ ∈ R.
(3)
From (H2), we have 𝑓(𝑑, π‘₯) is 2𝑇 periodic and πœπ‘˜+π‘ž − πœπ‘˜ = 2𝑇.
Hence assumption (H∗ ) holds naturally. However, we show
some new and fruitful results of system (1) with the condition
(H1)-(H2). For example, we obtain the existence and stability
of 2𝑇 periodic solutions to system (1) by double-periodic
bifurcation.
This paper is organized as follows. In Section 2, for the sake
of self-containedness of the paper, we present some basic
definitions of impulsive differential equations. In Section 3,
we describe the scalar impulsive differential equations on
Moebius stripe and define the Poincaré map. Then we prove
several essential lemmas and give sufficient conditions to
ensure the existence and stability of one-side and two-side
orbits of impulsive differential equation on Moebius stripe.
In Section 4, we are mainly concerned with the doubleperiodic bifurcation impulsive differential equations on Moebius stripe.
2. Preliminaries
For the sake of self-containedness of the paper, we present
the basic definitions and notations of the theory of impulsive differential equations we need (see [1, 2, 8]). We also
include some fundamental results which are necessary for
understanding the theory.
Let R, Z, and Z+ be the sets of real numbers, integers, and
positive integers, respectively. Denote by πœƒ = {πœƒπ‘– } a strictly
increasing sequence of real numbers such that the set A of
indexes 𝑖 is an interval in Z.
Definition 1. A function πœ™ : R → R𝑛 , 𝑛 ∈ R, is from the set
𝑃𝐢(R, πœƒ) if
(i) it is left continuous;
(ii) it is continuous, except, possibly, points of πœƒ, where it
has discontinuities of the first kind.
The last definition means that if πœ™(𝑑) ∈ 𝑃𝐢(R, πœƒ), then the
right limit πœ™(πœƒπ‘– +) = lim𝑑 → πœƒπ‘–+ πœ™(𝑑) exists and πœ™(πœƒπ‘– (−)) = πœ™(πœƒπ‘– ),
where πœ™(πœƒπ‘– −) = lim𝑑 → πœƒπ‘–− πœ™(𝑑), for each πœƒπ‘– ∈ πœƒ.
Definition 2. A function πœ™ : R → R𝑛 is from the set
𝑃𝐢1 (R, πœƒ) if πœ™(𝑑), πœ™σΈ€  (𝑑) ∈ 𝑃𝐢(R, πœƒ), where the derivative at
points of πœƒ is assumed to be the left derivative.
In what follows, in this section, 𝐽 ∈ R is an interval in R.
For simplicity of notation, πœƒ is not necessary a subset of 𝐽.
Definition 3. The solution πœ™(𝑑) is stable if to any πœ€ > 0 and
𝑑0 ∈ 𝐽 there corresponds 𝛿(𝑑0 , πœ€) > 0 such that for any other
solution πœ“(𝑑) of (1) with β€–πœ™(𝑑0 ) − πœ“(𝑑0 )β€– < 𝛿(𝑑0 , πœ€) we have
β€–πœ™(𝑑) − πœ“(𝑑)β€– < πœ€ for 𝑑 ≥ 𝑑0 ; the solution πœ™(𝑑) is uniformly
stable, if 𝛿(𝑑0 , πœ€) can be chosen independently of 𝑑0 .
→
𝑛
Figure 1: Moebius stripe.
Definition 4. The solution πœ™(𝑑) is asymptotically stable if it is
stable in the sense of Definition 3 and there exists a positive
number πœ…(𝑑0 ) such that if πœ“(𝑑) is any other solution of (1)
with β€–πœ™(𝑑0 ) − πœ“(𝑑0 )β€– < πœ…(𝑑0 ), then β€–πœ™(𝑑) − πœ“(𝑑)β€– → 0 as
𝑑 → ∞; if πœ…(𝑑0 ) can be chosen to be independent of 𝑑0
and πœ™(𝑑) is uniformly stable, then πœ™(𝑑) is said to be uniformly
asymptotically stable.
Definition 5. The solution πœ™(𝑑) is unstable if there exist
numbers πœ€0 > 0 and 𝑑0 ∈ 𝐽 such that for any 𝛿 > 0 there
exists a solution 𝑦𝛿 (𝑑), β€–πœ™(𝑑0 ) − 𝑦𝛿 (𝑑0 )β€– < 𝛿, of (1) such that
either it is not continuable to ∞ or there exists a moment 𝑑1 ,
𝑑1 > 𝑑0 such that β€–πœ™(𝑑1 ) − 𝑦𝛿 (𝑑1 )β€– ≥ 𝛿.
For any 𝑑0 ∈ R, we assume that there exists a π‘˜ ∈ Z+ ,
such that πœπ‘˜−1 < 𝑑0 ≤ πœπ‘˜ ; then the initial value problem (IVP)
to first-order impulsive differential equations (1) is given as
𝑑π‘₯
= 𝑓 (𝑑, π‘₯) ,
𝑑𝑑
𝑑 =ΜΈ πœπ‘˜ ,
Δπ‘₯|𝑑=πœπ‘˜ = πΌπ‘˜ (π‘₯) ,
π‘˜ ∈ Z+ ,
(4)
π‘₯ (𝑑0+ ) = π‘₯0 .
In what followed, we use π‘₯(𝑑, 𝑑0 , π‘₯0 ) to denote the solution of
IVP (4).
In [20], Hu and Han investigated system (1) under the
assumption (H∗ ) and obtained the following stability results
for the periodic solutions.
Theorem 6 (see [20]). Let π‘₯(𝑑, 𝑑0 , π‘₯0∗ ) be a periodic solution
of system (1) with period T. If 0 < |𝑃󸀠 (π‘₯0∗ )| < 1 (>1), then it
is uniformly asymptotically stable (unstable), where 𝑃(π‘₯0 ) =
π‘₯(𝑑0 + 𝑛𝑇+ , 𝑑0 , π‘₯0 ) is the Poincaré map of system (1).
3. Poincaré Map and Periodic Solutions
In this section, we describe the scalar impulsive differential
equations on Moebius stripe and define the Poincaré map.
Then we prove several essential lemmas and give sufficient
conditions to ensure the existence and stability of oneside and two-side orbits (Figure 2) of impulsive differential
equation on Moebius stripe.
Abstract and Applied Analysis
3
Lemma 7. Assume that conditions (H1), (H2) hold. Suppose
that π‘₯(𝑑, 𝑑0 , π‘₯0 ) is a solution of (1) satisfying initial value
π‘₯(𝑑0+ ) = π‘₯0 . Then −π‘₯(𝑑 + 𝑇, 𝑑0 , π‘₯0 ) is also a solution of (1), and
−π‘₯ (𝑑 + 𝑇, 𝑑0 , π‘₯0 ) = π‘₯ (𝑑, 𝑑0 , −π‘₯ (𝑑0 + 𝑇, 𝑑0 , π‘₯0 )) ,
𝑑 ∈ R.
(5)
Proof. Let πœ‘(𝑑) ≡ −π‘₯(𝑑 + 𝑇, 𝑑0 , π‘₯0 ), πœ“(𝑑) ≡ π‘₯(𝑑, 𝑑0 , −π‘₯(𝑑0 +
𝑇, 𝑑0 , π‘₯0 )). Then for 𝑑 =ΜΈ πœπ‘˜ , π‘˜ ∈ Z, we have by (H2) that
𝑑π‘₯ (𝑑 + 𝑇, 𝑑0 , π‘₯0 )
π‘‘πœ‘ (𝑑)
= −
𝑑𝑑
𝑑𝑑
= − 𝑓 (𝑑 + 𝑇, π‘₯ (𝑑 + 𝑇, 𝑑0 , π‘₯0 ))
π‘₯
π‘₯0
𝑂
Figure 2: Figure of one-side and two-side orbits.
Δπœ‘|𝑑=πœπ‘˜ = − π‘₯ (πœπ‘˜ + 𝑇+ , 𝑑0 , π‘₯0 ) + π‘₯ (πœπ‘˜ + 𝑇, 𝑑0 , π‘₯0 )
+
= − π‘₯ (πœπ‘˜+π‘ž
, 𝑑0 , π‘₯0 ) + π‘₯ (πœπ‘˜+π‘ž , 𝑑0 , π‘₯0 )
π‘˜∈Z+
= − πΌπ‘˜ (π‘₯ (πœπ‘˜+π‘ž , 𝑑0 , π‘₯0 )) = −πΌπ‘˜ (π‘₯ (πœπ‘˜ + 𝑇, 𝑑0 , π‘₯0 ))
= πΌπ‘˜ (−π‘₯ (πœπ‘˜ + 𝑇, 𝑑0 , π‘₯0 )) = πΌπ‘˜ (πœ‘ (πœπ‘˜ )) .
(7)
Thus, we proved that πœ‘(𝑑) ≡ −π‘₯(𝑑 + 𝑇, 𝑑0 , π‘₯0 ) is a solution of
(1). On the other hand, it is obvious that
(8)
Hence, by uniqueness theorem we have that πœ‘(𝑑) ≡ πœ“(𝑑), 𝑑 ∈
R. This completes the proof.
Let 𝐷 denotes the stripe area on the plain {(𝑑, π‘₯) | (𝑑, π‘₯) ∈
R × R} between two lines 𝑑 = 𝑑0 and 𝑑 = 𝑑0 + 𝑇; that is,
(9)
Assume that π‘₯(𝑑, 𝑑0 , π‘₯0 ) exists for all 𝑑 ∈ [𝑑0 , +∞). Define
𝐿 0 = {(𝑑, π‘₯(𝑑, 𝑑0 , π‘₯0 )) | 𝑑0 ≤ 𝑑 ≤ 𝑑0 + 𝑇}. In general, we denote
𝐿 π‘˜ (π‘˜ ≥ 1) by
(10)
π‘˜∈Z+
(13)
define a flow on 𝑀2 . From this point of view, we call (1)
satisfying (H1) and (H2) an impulsive dynamical system on
Moebius stripe (see Figure 1).
Definition 8 (Poincaré Map). Let π‘₯(𝑑, 𝑑0 , π‘₯0 ) be the solution of
(IVP) (4). Assume that there exists an interval 𝐽 such that for
any π‘₯0 ∈ 𝐽, π‘₯(𝑑, 𝑑0 , π‘₯0 ) exists on [𝑑0 , 𝑑0 + 𝑇]. A map 𝑃 : 𝐽 → R
is called a Poincaré map of system (1) if for any π‘₯0 ∈ 𝐽
𝑃 (π‘₯0 ) = −π‘₯ (𝑑0 + 𝑇+ , 𝑑0 , π‘₯0 ) .
(14)
Definition 9. A closed curve 𝛾+ (π‘₯0 ) is called a one-side
periodic orbit on 𝑀2 if 𝛾+ (π‘₯0 ) = 𝐿 0 . And a closed curve
𝛾+ (π‘₯0 ) is called a two-side periodic orbit on 𝑀2 if 𝛾+ (π‘₯0 ) =
𝐿 0 ∪ 𝐿 1 =ΜΈ 𝐿 1 .
From Definitions 8 and 9, we can easily prove the
following assertion.
Lemma 10. One of following alternatives is valid:
(i) 𝛾+ (π‘₯0 ) is a one-side periodic orbit;
where π‘₯π‘˜ = π‘₯(𝑑0 + 𝑇+ , 𝑑0 , −π‘₯π‘˜−1 ), 𝑑 ≥ 𝑑0 .
It follows from Lemma 7 that 𝐿 π‘˜ has the form
𝐿 π‘˜ = {(𝑑, (−1)π‘˜ π‘₯ (𝑑 + π‘˜π‘‡, 𝑑0 , π‘₯0 )) | 𝑑0 ≤ 𝑑 ≤ 𝑑0 + 𝑇} .
two elements (𝑑0 , π‘₯) and (𝑑0 + 𝑇, −π‘₯) on 𝐷 as the same point
(or sticking (𝑑0 , π‘₯) and (𝑑0 + 𝑇, −π‘₯) together). Thus 𝑀2 is a
surface with only one side or the well-known Moebius stripe.
Obviously, by Lemma 7 the union
⋃ 𝐿 π‘˜ = ⋃ {(𝑑, (−1)π‘˜ π‘₯ (𝑑 + π‘˜π‘‡, 𝑑0 , π‘₯0 )) | 𝑑0 ≤ 𝑑 ≤ 𝑑0 + 𝑇}
= − πΌπ‘˜+π‘ž (π‘₯ (πœπ‘˜+π‘ž , 𝑑0 , π‘₯0 ))
𝐿 π‘˜ = {(𝑑, π‘₯ (𝑑, 𝑑0 , −π‘₯π‘˜ )) | 𝑑0 ≤ 𝑑 ≤ 𝑑0 + 𝑇} ,
𝑑
(6)
For 𝑑 = πœπ‘˜ , π‘˜ ∈ Z+ , it follows from (H1), (H2) that πœπ‘˜ + 𝑇 =
πœπ‘˜+π‘ž , π‘˜ ∈ Z+ and
𝐷 = {(𝑑, π‘₯) | 𝑑0 ≤ 𝑑 ≤ 𝑑0 + 𝑇, −∞ < π‘₯ < +∞} .
2𝑇
−π‘₯0
= 𝑓 (𝑑, −π‘₯ (𝑑 + 𝑇, 𝑑0 , π‘₯0 )) = 𝑓 (𝑑, πœ‘ (𝑑)) .
πœ‘ (𝑑) |𝑑=𝑑0 = −π‘₯ (𝑑0 + 𝑇, 𝑑0 , π‘₯0 ) = πœ“ (𝑑) |𝑑=𝑑0 .
𝑇
(ii) π‘₯0 is a fixed point of 𝑃; that is, 𝑃(π‘₯0 ) = π‘₯0 ;
(11)
We now introduce an equivalence relation ∼ on 𝐷 such
that for (𝑑, π‘₯), (𝑑󸀠 , π‘₯σΈ€  ) ∈ 𝐷
󡄨
󡄨
(12)
(𝑑, π‘₯) ∼ (𝑑󸀠 , π‘₯σΈ€  ) iff 󡄨󡄨󡄨󡄨𝑑 − 𝑑󸀠 󡄨󡄨󡄨󡄨 = 𝑇, π‘₯ = −π‘₯σΈ€  .
Then we denote the corresponding quotient space by 𝑀2 .
From geometric point of view, 𝑀2 is obtained by considering
(iii) π‘₯(𝑑 + 𝑇, 𝑑0 , π‘₯0 ) = −π‘₯(𝑑, 𝑑0 , π‘₯0 ), 𝑑 ∈ R.
Proof. We prove it from (i) ⇒ (ii) ⇒ (iii) ⇒ (i). Assume
(i) is true; that is, 𝛾+ (π‘₯0 ) is a one-side periodic orbit. Then by
Definition 9 we have that
−π‘₯ (𝑑0 + 𝑇+ , 𝑑0 , π‘₯0 ) = π‘₯ (𝑑0+ , 𝑑0 , π‘₯0 ) = π‘₯0 ,
that is, 𝑃(π‘₯0 ) = π‘₯0 . Hence (ii) is valid.
(15)
4
Abstract and Applied Analysis
Next, we suppose that (ii) is fulfilled; that is, −π‘₯(𝑑0 +
𝑇+ , 𝑑0 , π‘₯0 ) = π‘₯0 . Then by Lemma 7 we know
π‘₯ (𝑑 + 𝑇, 𝑑0 , π‘₯0 ) = π‘₯ (𝑑, 𝑑0 , −π‘₯ (𝑑0 + 𝑇+ , 𝑑0 , π‘₯0 ))
= −π‘₯ (𝑑, 𝑑0 , π‘₯0 ) .
𝑑 ∈ [𝑑0 , 𝑑0 + 𝑇] .
𝑑
π‘₯ (𝑑, 𝑑0 , π‘₯0 ) = π‘₯0 + ∫ 𝑓 (𝑠, π‘₯ (𝑠, 𝑑0 , π‘₯0 )) 𝑑𝑠.
𝑑0
(16)
Thus, (iii) is proved.
Finally, if (iii) is true, then π‘₯(𝑑0 + 𝑇+ , 𝑑0 , π‘₯0 ) = −π‘₯0 . By the
uniqueness of solution of IVP (4), we know
π‘₯ (𝑑, 𝑑0 , −π‘₯ (𝑑0 + 𝑇+ , 𝑑0 , π‘₯0 )) = π‘₯ (𝑑, 𝑑0 , π‘₯0 ) ,
can be expressed as
(17)
Thus we obtain that 𝛾+ (π‘₯0 ) is a one-side periodic orbit.
The proof is completed.
Differentiate between both sides of the above equation with
respect to π‘₯0 , we have
𝑑
πœ•π‘₯ (𝑑, 𝑑0 , π‘₯0 )
πœ•π‘₯ (𝑠, 𝑑0 , π‘₯0 )
= 1 + ∫ 𝑓π‘₯ (𝑠, π‘₯ (𝑠, 𝑑0 , π‘₯0 )) ⋅
𝑑𝑠.
πœ•π‘₯0
πœ•π‘₯0
𝑑0
(22)
Let 𝑧(𝑑) = πœ•π‘₯(𝑑, 𝑑0 , π‘₯0 )/πœ•π‘₯0 , then for 𝑑 ∈ [𝑑0 , πœπ‘— ), 𝑧(𝑑) is the
solution of IVP to ordinary differential equation
𝑑𝑧
= 𝑓π‘₯ (𝑑, π‘₯) 𝑧,
𝑑𝑑
Similarly, as proof of Lemma 10, we have the following
lemma.
(i) 𝛾+ (π‘₯0 ) is a two-side periodic orbit;
(ii) π‘₯0 is a 2-periodic point of 𝑃; that is, 𝑃(π‘₯0 ) =ΜΈ π‘₯0 ,
𝑃2 (π‘₯0 ) = π‘₯0 ;
(iii) π‘₯(𝑑 + 2𝑇, 𝑑0 , π‘₯0 ) = π‘₯(𝑑, 𝑑0 , π‘₯0 ), 𝑑 ∈ R. And there exists
a 𝑑0 , such that π‘₯(𝑑0 + 𝑇+ , 𝑑0 , π‘₯0 ) =ΜΈ − π‘₯0 .
Remark 12. From Lemmas 10 and 11, we see that a one-side
periodic orbit must be a two-side periodic orbit since
2
implies 𝑃 (π‘₯0 ) = 𝑃 (𝑃 (π‘₯0 )) = 𝑃 (π‘₯0 ) = π‘₯0 .
(18)
Nevertheless, the converse is not true.
From Remark 12, we give the definition of stability of the
mentioned orbits.
Definition 13. Let 𝛾+ (π‘₯0 ) be a periodic orbit of system (1)
(one-side or two-side). Then 𝛾+ (π‘₯0 ) of system (1) is called
stable (asymptotically stable or unstable) if 𝛾+ (π‘₯0 ) as a 2𝑇
periodic solution is stable (asymptotically stable or unstable).
Theorem 14. Assume π‘₯(𝑑, 𝑑0 π‘₯0 ) is the solution of IVP (4) and
let 𝑧(𝑑) = πœ•π‘₯(𝑑, 𝑑0 , π‘₯0 )/πœ•π‘₯0 . Then 𝑧(𝑑) is a solution to the
following IVP of impulsive differential equations:
𝑑𝑧
= 𝑓π‘₯ (𝑑, π‘₯) 𝑧,
𝑑𝑑
Δ𝑧|𝑑=πœπ‘˜ = πΌπ‘˜σΈ€  (π‘₯) ,
(19)
Proof. Let 𝐽 = (𝑑0 , +∞) and π½π‘˜ = (πœπ‘˜−1 , πœπ‘˜ ], π‘˜ ∈ Z+ . Without
losing generality, we assume that 𝑑0 ∈ 𝐽𝑗 for some 𝑗 ≥ 1. The
solution of IVP
π‘₯ (𝑑0+ ) = π‘₯0
𝑑
𝑧 (𝑑) = exp ∫ 𝑓π‘₯ (𝑠, π‘₯ (𝑠, 𝑑0 , π‘₯0 )) 𝑑𝑠.
(24)
𝑑0
Since 𝑧(𝑑) is left continuous on [𝑑0 , ∞), we have
πœπ‘—
𝑧 (πœπ‘— ) = exp ∫ 𝑓π‘₯ (𝑠, π‘₯ (𝑠, 𝑑0 , π‘₯0 )) 𝑑𝑠.
(25)
𝑑0
For 𝑑 ∈ 𝐽𝑗+1 , π‘₯(𝑑, 𝑑0 , π‘₯0 ) is a solution of system
𝑑π‘₯
= 𝑓 (𝑑, π‘₯) ,
𝑑𝑑
(26)
π‘₯ (πœπ‘— ) = π‘₯1 ,
where π‘₯1 = π‘₯(πœπ‘—+ , 𝑑0 , π‘₯0 ) = π‘₯(πœπ‘— , 𝑑0 , π‘₯0 ) + 𝐼𝑗 (π‘₯(πœπ‘— , 𝑑0 , π‘₯0 )).
Thus, we have
π‘₯ (𝑑, 𝑑0 , π‘₯0 ) ≡ π‘₯ (𝑑, πœπ‘— , π‘₯1 )
𝑑
= π‘₯1 + ∫ 𝑓 (𝑠, π‘₯ (𝑠, πœπ‘— , π‘₯1 )) 𝑑𝑠,
𝑑 ∈ 𝐽𝑗+1 .
(27)
𝑧 (𝑑0 ) = 1.
𝑑π‘₯
= 𝑓 (𝑑, π‘₯) ,
𝑑𝑑
(23)
Thus
πœπ‘—
𝑑 =ΜΈ π‘‘π‘˜ ,
π‘˜ ∈ Z+ ,
𝑑 =ΜΈ π‘‘π‘˜ ,
𝑧 (𝑑0 ) = 1.
Lemma 11. One of following alternatives is valid:
𝑃 (π‘₯0 ) = π‘₯0
(21)
Similarly, we have 𝑑 ∈ (πœπ‘— , πœπ‘—+1 ),
πœ•π‘₯ (𝑑, 𝑑0 , π‘₯0 ) πœ•π‘₯ (𝑑, πœπ‘— , π‘₯1 )
=
πœ•π‘₯1
πœ•π‘₯1
𝑑
= exp ∫ 𝑓π‘₯ (𝑠, π‘₯ (𝑠, πœπ‘— , π‘₯1 )) 𝑑𝑠
πœπ‘—
(20)
𝑑
= exp ∫ 𝑓π‘₯ (𝑠, π‘₯ (𝑠, 𝑑0 , π‘₯0 )) 𝑑𝑠.
πœπ‘—
(28)
Abstract and Applied Analysis
5
Theorem 17. Assume that the conditions (H1), (H2) hold. Let
𝛾+ (π‘₯0 ) be a periodic orbit of system (1) and πΌπ‘˜σΈ€  (π‘₯(πœπ‘˜ , 𝑑0 , π‘₯0 )) =ΜΈ −
Note
πœ•π‘₯1 πœ• [π‘₯ (πœπ‘— , 𝑑0 , π‘₯0 ) + 𝐼𝑗 (π‘₯ (πœπ‘— , 𝑑0 , π‘₯0 ))]
=
πœ•π‘₯0
πœ•π‘₯ (πœπ‘— , 𝑑0 , π‘₯0 )
⋅
𝑑 +2𝑇
1. Then (i) ∫𝑑 0
πœ•π‘₯ (πœπ‘— , 𝑑0 , π‘₯0 )
(29)
πœ•π‘₯0
= (1 + 𝐼𝑗󸀠 (π‘₯ (πœπ‘— , 𝑑0 , π‘₯0 )))
πœ•π‘₯ (πœπ‘— , 𝑑0 , π‘₯0 )
πœ•π‘₯0
We obtain for 𝑑 ∈ (πœπ‘— , πœπ‘—+1 ) that
𝑑π‘₯
= π‘Ž (𝑑) π‘₯ + 𝑏 (𝑑) ,
𝑑𝑑
(30)
𝑑
Δπ‘₯|𝑑=πœπ‘˜ = π‘π‘˜ π‘₯ (πœπ‘˜ ) ,
⋅ exp ∫ 𝑓π‘₯ (𝑠, π‘₯ (𝑠, 𝑑0 , π‘₯0 )) 𝑑𝑠.
𝑑0
(31)
𝑑0
By Definitions 9 and (31), we conclude the following
assertion.
Corollary 15. Assume that conditions (H1), (H2) hold. Then
𝑑0 <πœπ‘˜ ≤𝑑0 +𝑇
⋅ exp ∫
𝑑0 +𝑇
𝑑0
Μƒ π‘Ž(𝑑 + 𝑇) = π‘Ž(𝑑) and 𝑏(𝑑 + 𝑇) = −𝑏(𝑑) for 𝑑 ∈ R;
(H1)
Μƒ π‘Ž(𝑑) and 𝑏(𝑑) are continuous;
(H2)
Assume that π‘₯(𝑑, 𝑑0 , π‘₯0 ) is a one-side periodic solution of
system (34), by the method of variation of constants formula
(see [1]), we get
π‘₯ (𝑑, 𝑑0 , π‘₯0 )
= ∏ (1 + π‘π‘˜ )
(1 + πΌπ‘˜σΈ€  (π‘₯ (πœπ‘˜ , 𝑑0 , π‘₯0 )))
𝑑0 <πœπ‘˜ ≤𝑑
(32)
𝑓π‘₯ (𝑑, π‘₯ (𝑑, 𝑑0 , π‘₯0 )) 𝑑𝑑.
𝑑
⋅ exp ∫ π‘Ž (𝑑) 𝑑𝑑
𝑑0
𝑑
𝑠
𝑑0
𝑑0
× [π‘₯0 + ∫ exp (− ∫ π‘Ž (𝑒) 𝑑𝑒) 𝑏 (𝑠) 𝑑𝑠] ,
2
has
π‘˜∈Z ,
Μƒ πœπ‘˜+π‘ž − πœπ‘˜ = 𝑇, for all π‘˜ ∈ Z+ .
(H4)
where 𝑑 ∈ 𝐽. Then the proof is completed.
∏
(34)
+
Μƒ π‘π‘˜+π‘ž = π‘π‘˜ , for all π‘˜ ∈ Z+ ;
(H3)
⋅ exp ∫ 𝑓π‘₯ (𝑠, π‘₯ (𝑠, 𝑑0 , π‘₯0 )) 𝑑𝑠,
𝑃󸀠 (π‘₯0 ) = −
𝑑 =ΜΈ πœπ‘˜ ,
where πœπ‘˜ < πœπ‘˜+1 (π‘˜ ≥ 1), πœπ‘˜ → +∞, π‘˜ → +∞, π‘π‘˜ =ΜΈ − 1 and
there exists a constant 𝑇 > 0, a positive integer π‘ž, such that
the following conditions are satisfied:
Deducing in a similar way, we get
𝑑
+
Example 18. Consider the linear periodic impulsive differential equations on Moebius stripe as follows:
πœ•π‘₯ (𝑑, 𝑑0 , π‘₯0 ) πœ•π‘₯ (𝑑, πœπ‘— , π‘₯1 )
=
πœ•π‘₯0
πœ•π‘₯0
πœ•π‘₯ (𝑑, 𝑑0 , π‘₯0 )
= ∏ (1 + πΌπ‘˜σΈ€  (π‘₯ (πœπ‘— , 𝑑0 , π‘₯0 )))
πœ•π‘₯0
𝑑0 <πœπ‘˜ ≤𝑑
+
Proof. If 𝛾+ (π‘₯0 ) is a two-side periodic orbit; that is, π‘₯(𝑑, 𝑑0 , π‘₯0 )
is a 2𝑇 periodic solution of (1). Since both (H1) and (H2)
hold, we know that (1) is a periodic impulsive differential
equation. Then by (33) and Theorem 6, the conclusion is
straightforward.
.
= (1 + 𝐼𝑗󸀠 (π‘₯ (πœπ‘— , 𝑑0 , π‘₯0 )))
𝑓π‘₯ (𝑑, π‘₯(𝑑, 𝑑0 , π‘₯0 ))𝑑𝑑 < − ∑𝑑0 <πœπ‘˜ ≤𝑑0 +2𝑇 ln |1
0
σΈ€ 
πΌπ‘˜ (π‘₯(πœπ‘˜ , 𝑑0 , π‘₯0 ))| implies 𝛾+ (π‘₯0 ) is asymptotically stable,
𝑑 +2𝑇
(ii) ∫𝑑 0 𝑓π‘₯ (𝑑, π‘₯(𝑑, 𝑑0 , π‘₯0 ))𝑑𝑑 > − ∑𝑑0 <πœπ‘˜ ≤𝑑0 +2𝑇 ln |1
0
πΌπ‘˜σΈ€  (π‘₯(πœπ‘˜ , 𝑑0 , π‘₯0 ))| implies 𝛾+ (π‘₯0 ) is unstable.
As usual, one uses the notion 𝑃 (π‘₯0 ) = 𝑃(𝑃(π‘₯0 )). Then one
(35)
σΈ€ 
[𝑃2 (π‘₯0 )] =
∏
𝑑0 <πœπ‘˜ ≤𝑑0 +2𝑇
(1 + πΌπ‘˜σΈ€  (π‘₯ (πœπ‘˜ , 𝑑0 , π‘₯0 )))
𝑑0 +2𝑇
⋅ exp ∫
𝑑0
𝑃 (π‘₯0 )
(33)
𝑓π‘₯ (𝑑, π‘₯ (𝑑, 𝑑0 , π‘₯0 )) 𝑑𝑑.
Definition 16. π‘₯0 is called a hyperbolic fixed point of 𝑃 if
π‘₯0 = 𝑃(π‘₯0 ) and 𝑃󸀠 (π‘₯0 ) =ΜΈ − 1; the corresponding one-side
periodic orbit 𝛾+ (π‘₯0 ) is called hyperbolic one-side periodic
σΈ€ 
orbit. If 𝛾+ (π‘₯0 ) is a two-side periodic orbit with (𝑃2 ) (π‘₯0 ) =ΜΈ 1,
then we call 𝛾+ (π‘₯0 ) a hyperbolic two-side periodic orbit.
=−
(1 + π‘π‘˜ )
∏
𝑑0 <πœπ‘˜ ≤𝑑0 +𝑇
𝑑0 +𝑇
⋅ exp ∫
𝑑0
π‘Ž (𝑑) 𝑑𝑑
× [π‘₯0 + ∫
𝑑0 +𝑇
𝑑0
𝑑
exp (− ∫ π‘Ž (𝑒) 𝑑𝑒) 𝑏 (𝑑) 𝑑𝑑] ,
𝑑0
(36)
6
Abstract and Applied Analysis
𝑃2 (π‘₯0 )
=
∏
𝑑0 <πœπ‘˜ ≤𝑑0 +2𝑇
𝑃2 (π‘₯0 ) = π‘₯0 . So by taking Lemma 11, 𝛾+ (π‘₯0 ) is a two-side
periodic orbit if π‘₯0 =ΜΈ π‘₯0∗ .
The proof is ended.
(1 + π‘π‘˜ )
𝑑0 +2𝑇
π‘Ž (𝑑) 𝑑𝑑
⋅ exp ∫
𝑑0
× [π‘₯0 + ∫
𝑑0 +2𝑇
𝑑0
𝑑
exp (− ∫ π‘Ž (𝑒) 𝑑𝑒) 𝑏 (𝑑) 𝑑𝑑] .
𝑑0
(37)
𝑑 +𝑇
Let 𝐴 = ∏𝑑0 <πœπ‘˜ ≤𝑑0 +𝑇 (1 + π‘π‘˜ ) ⋅ exp ∫𝑑 0
0
have the following theorem.
π‘Ž(𝑑)𝑑𝑑; therefore, we
Μƒ H4)
Μƒ are satisfied, then
Theorem 19. Suppose that (H1–
(i) there exists a unique one-side periodic orbit for system
(34) if 𝐴 =ΜΈ −1, which is asymptotically stable (unstable)
provided 0 < |𝐴| < 1 (|𝐴| > 1),
(ii) if 𝐴2 ≠ 1, (34) has no two-side periodic orbit. If 𝐴 = 1
all the trajectories are two-side periodic orbits expect for
a unique one-side periodic orbit.
Proof. For the sake of convenience, we denote
𝐡1 = ∫
𝑑0 +𝑇
𝑑0
𝑑
exp (− ∫ π‘Ž (𝑒) 𝑑𝑒) 𝑏 (𝑑) 𝑑𝑑,
𝑑0
𝑑0 +2𝑇
𝐡2 = ∫
𝑑0
(38)
𝑑
exp (− ∫ π‘Ž (𝑒) 𝑑𝑒) 𝑏 (𝑑) 𝑑𝑑.
𝑑0
Remark 20. If π‘π‘˜ ≡ 0, π‘˜ ∈ Z+ , in (34); that is, (34)
reduces to an ordinary differential equation. We see that
𝑑 +𝑇
𝐴 = exp ∫𝑑 0 π‘Ž(𝑑)𝑑𝑑. Hence 𝐴 =ΜΈ − 1 holds automatically, and
0
therefore (34) always has a unique one-side periodic orbit.
Μƒ H4)
Μƒ be fulfilled and 𝐴 = 1. Then
Corollary 21. Let (H1–
𝐡2 = ∫
𝑑0 +2𝑇
𝑑0
𝑃 (π‘₯0 ) = −𝐴 (π‘₯0 + 𝐡1 ) ,
𝑃2 (π‘₯0 ) = 𝐴2 (π‘₯0 + 𝐡2 ) . (39)
Obviously, 𝑃(π‘₯0 ) = π‘₯0 has a unique solution for any π‘₯0 ∈ R
if 𝐴 =ΜΈ − 1, and 𝑃2 (π‘₯0 ) = π‘₯0 has a unique solution for any
π‘₯0 ∈ R if 𝐴2 =ΜΈ 1. Observing that any two-side periodic orbit
obtained under the assumption 𝐴2 ≠ 1 must be a one-side
periodic orbit since 𝐴2 =ΜΈ 1 implies 𝐴 =ΜΈ − 1, together with
Remark 12, we have (34) has no two-side periodic orbit.
It follows from (36) that 𝑃󸀠 (π‘₯0 ) = −𝐴. Then by Theorem 6
we have the one-side orbit is asymptotically stable (unstable)
provided 0 < |𝐴| < 1 (|𝐴| > 1).
Next, let 𝐴 = 1. By taking (36) and (37) into account, we
have
𝑃 (π‘₯0 ) = −π‘₯0 − ∫
𝑑0 +𝑇
𝑑0
𝑑
exp (− ∫ π‘Ž (𝑒) 𝑑𝑒) 𝑏 (𝑑) 𝑑𝑑
𝑑0 +2𝑇
𝑃2 (π‘₯0 ) = π‘₯0 + ∫
𝑑0
𝑑
(40)
exp (− ∫ π‘Ž (𝑒) 𝑑𝑒) 𝑏 (𝑑) 𝑑𝑑
𝑑0
≡ π‘₯0 + 𝐡2 .
Suppose that 𝑃 has a unique fixed point π‘₯0∗ = −𝐡1 /2, from
the above we have −𝐡1 /2 + 𝐡2 = −𝐡1 /2, then 𝐡2 ≡ 0 and
(41)
Theorem 22. Suppose that conditions (H1)–(H3) hold, then
(i) system (1) has at most one one-side periodic orbit;
(ii) if any solution π‘₯(𝑑, 𝑑0 , π‘₯0 ) of (1) with |π‘₯0 | ≤ |𝑃(0)| is
well defined on 𝑑 ∈ [𝑑0 , 𝑑0 + 𝑇], then system (1) must
has a unique one-side periodic orbit.
Proof. We first prove that system (1) cannot have two oneside periodic orbits. Suppose 𝛾1+ (π‘₯0∗ ) : π‘₯ = π‘₯(𝑑, 𝑑0 , π‘₯0∗ ), 𝑑 ∈
[𝑑0 , 𝑑0 + 𝑇] and 𝛾2+ (π‘₯0 ) : π‘₯ = π‘₯(𝑑, 𝑑0 , π‘₯0 ), 𝑑 ∈ [𝑑0 , 𝑑0 + 𝑇] are two
one-side periodic orbits system (1). Then
π‘₯ (𝑑0 + 𝑇, 𝑑0 , π‘₯0 ) = −π‘₯0 . (42)
Without losing generality, we assume π‘₯0 > π‘₯0∗ , then it follows
from uniqueness theorem of ordinary differential equations
that π‘₯ = π‘₯(𝑑, 𝑑0 , π‘₯0 ) and π‘₯(𝑑, 𝑑0 , π‘₯0∗ ) cannot intersect when 𝑑 is
not an impulsive time. Therefore we have
π‘₯ (𝑑, 𝑑0 , π‘₯0 ) > π‘₯ (𝑑, 𝑑0 , π‘₯0∗ ) ,
𝑑0 ≤ 𝑑 ≤ 𝜏1 .
(43)
Note π΅π‘˜ (π‘₯) = π‘₯ + πΌπ‘˜ (π‘₯) is strictly increasing, we get
π‘₯ (𝜏1+ , 𝑑0 , π‘₯0 ) > π‘₯ (𝜏+ , 𝑑0 , π‘₯0∗ ) .
(44)
In a similar way, we can prove that π‘₯(𝑑, 𝑑0 , π‘₯0 ) > π‘₯(𝑑, 𝑑0 , π‘₯0∗ ),
𝑑0 ≤ 𝑑 ≤ 𝑑0 + 𝑇. That is, the curve {(𝑑, π‘₯) | π‘₯ = π‘₯(𝑑, 𝑑0 , π‘₯0 ),
𝑑0 ≤ 𝑑 ≤ 𝑑0 + 𝑇} always stays above curve {(𝑑, π‘₯) | π‘₯ =
π‘₯(𝑑, 𝑑0 , π‘₯0∗ ), 𝑑0 ≤ 𝑑 ≤ 𝑑0 + 𝑇}. This contradicts (42). We put
it in another way that
π‘₯0 > π‘₯0∗ 󳨐⇒ 𝑃 (π‘₯0 ) > 𝑃 (π‘₯0∗ ) .
𝑑0
≡ −π‘₯0 − 𝐡1 ,
𝑑0
Now we are in position to consider nonlinear impulsive
system on Meobius stripe. To explore the uniqueness of oneside periodic orbit, we induce the following condition.
(H3) Operator π΅π‘˜ : R → R, π΅π‘˜ (π‘₯) = π‘₯ + πΌπ‘˜ (π‘₯) is strictly
increasing, for all π‘˜ ∈ Z+ .
π‘₯ (𝑑0 + 𝑇, 𝑑0 , π‘₯0∗ ) = −π‘₯0∗ ,
Then
𝑑
exp (− ∫ π‘Ž (𝑒) d𝑒) 𝑏 (𝑑) 𝑑𝑑 = 0.
(45)
Thus, (1) has at most a one-side periodic orbit.
Further, let the solution π‘₯(𝑑, 𝑑0 , π‘₯0 ) of system (1) be all
defined on 𝑑 ∈ [𝑑0 , 𝑑0 + 𝑇]. If 𝑃(0) = 0, the conclusion is
proved. We assume that 𝑃(0) > 0, then we know 𝑃(π‘₯0 ) < 𝑃(0)
if 0 < π‘₯0 ≤ 𝑃(0). Note
𝑃2 (0) − 𝑃 (0) = 𝑃 (𝑃 (0)) − 𝑃 (0) < 𝑃 (0) − 𝑃 (0) = 0.
(46)
Abstract and Applied Analysis
7
π‘₯
there exists a transformation of system (1) that
𝑑𝑦
= 𝑓 (𝑑, 𝑦 + π‘₯ (𝑑)) − 𝑓 (𝑑, π‘₯ (𝑑)) ≡ 𝑔 (𝑑, 𝑦) ,
𝑑𝑑
π‘₯0
Δ𝑦|𝑑=πœπ‘˜ = πΌπ‘˜ (𝑦 + π‘₯ (πœπ‘˜ )) − πΌπ‘˜ (π‘₯ (πœπ‘˜ )) ≡ β„Žπ‘˜ (𝑦) ,
𝑂
−π‘₯0
𝑑π‘₯
= 𝐹 (𝑑, π‘₯, πœ€) ,
𝑑𝑑
Figure 3: A one-side periodic orbit.
Δπ‘₯|𝑑=πœπ‘˜ = ΜƒπΌπ‘˜ (π‘₯ (πœπ‘˜ ) , πœ€) ,
We obtain that 𝑃(π‘₯0 ) − π‘₯0 have opposite signs between π‘₯0 = 0
and π‘₯0 = 𝑃(0), and then it follows from the continuity of
𝑃 that there exists π‘₯0∗ ∈ (0, 𝑃(0)) such that 𝑃(π‘₯0∗ ) = π‘₯0∗ .
Similarly, we can prove 𝑃 has a fixed point in the case of
𝑃(0) < 0. The proof is completed.
Theorem 23. Assume that conditions (H1)–(H3) hold. Furthermore, suppose there exists a positive number 𝑁 such that
𝑓 (𝑑, −𝑁) ≥ 0,
−2𝑁 ≤ πΌπ‘˜ (𝑁) ≤ 0,
𝑑 ∈ [𝑑0 , 𝑑0 + 𝑇] ,
(47)
∀π‘˜ ∈ Z+ .
(48)
Then (1) has a unique one-side periodic orbit.
Proof. From (47) we have that π‘₯(𝑑, 𝑑0 , π‘₯0 ) will stay inside
[−𝑁, 𝑁] for 𝑑 =ΜΈ πœπ‘˜ , π‘˜ ∈ Z+ . On the other hand, by (H3), we
have that −𝑁 + πΌπ‘˜ (−𝑁) ≤ π‘₯(πœπ‘˜ ) + πΌπ‘˜ (π‘₯(πœπ‘˜ )) ≤ 𝑁 + πΌπ‘˜ (𝑁) for
−𝑁 ≤ π‘₯(πœπ‘˜ ) ≤ 𝑁. Then it follows from (48) that
−𝑁 ≤ 𝑁 + πΌπ‘˜ (𝑁) ≤ 𝑁 ≤ 𝑁,
−𝑁 ≤ −𝑁 + πΌπ‘˜ (−𝑁) = −𝑁 − πΌπ‘˜ (𝑁) ≤ 𝑁
𝑑 =ΜΈ πœπ‘˜ ,
(52)
+
π‘˜∈Z ,
where 𝐹 : R × R × R → R is 𝐢3 with respect to π‘₯,
continuously differentiable with respect to πœ€. ΜƒπΌπ‘˜ : R×R → R
is 𝐢3 (π‘˜ ∈ Z+ ) with respect to π‘₯. Moreover, we suppose
𝐹(𝑑 + 𝑇, −π‘₯, πœ€) = −𝐹(𝑑, π‘₯, πœ€), ΜƒπΌπ‘˜ (π‘₯, πœ€) = ΜƒπΌπ‘˜+π‘ž (π‘₯, πœ€), ΜƒπΌπ‘˜ (−π‘₯) =
−ΜƒπΌπ‘˜ (π‘₯), for all π‘˜ ∈ Z+ , where πœπ‘˜+π‘ž − πœπ‘˜ = 𝑇. For πœ€ = 0, we
have 𝐹(𝑑, π‘₯, 0) = 𝑓(𝑑, π‘₯), ΜƒπΌπ‘˜ (π‘₯, 0) = πΌπ‘˜ (π‘₯). These assumptions
mean (H1) and (H2) hold for 𝐹 and ΜƒπΌπ‘˜ , for all π‘˜ ∈ Z+ .
Furthermore, assume that π‘₯ + ΜƒπΌπ‘˜ (π‘₯, πœ€) is strictly increasing,
then by Theorem 22 we have that system (52) has at most a
one-side periodic orbit.
Suppose that (1) has a one-side periodic orbit and
𝑓(𝑑, 0) = 0. Then by using implicit function theorem in the
Poincaré map of system (52), we know that system (52) has a
one-side periodic orbit when |πœ€| is sufficiently small. Now let
π‘₯∗ (𝑑, πœ€) be the solution of system (52) and 𝑦(𝑑, πœ€) = π‘₯(𝑑, πœ€) −
π‘₯∗ (𝑑, πœ€). Then we can get a transformation of system (52):
𝑑𝑦
= 𝐹 (𝑑, 𝑦 + π‘₯∗ , πœ€) − 𝐹 (𝑑, π‘₯∗ , πœ€) = 𝐺 (𝑑, 𝑦, πœ€) ,
𝑑𝑑
𝑑 =ΜΈ πœπ‘˜ ,
Δ𝑦|𝑑=πœπ‘˜ = ΜƒπΌπ‘˜ (𝑦 + π‘₯∗ (πœπ‘˜ , πœ€) , πœ€)
− ΜƒπΌπ‘˜ (π‘₯∗ (πœπ‘˜ , πœ€) , πœ€) = π»π‘˜ (𝑦, πœ€) ,
(49)
π‘˜ ∈ Z+ .
(53)
(see Figure 3).
By Taylor’s formula, we have
𝐺 (𝑑, 𝑦, πœ€) = 𝐴 1 (𝑑, πœ€) 𝑦 + 𝐴 2 (𝑑, πœ€) 𝑦2
Thus,
󡄨
󡄨 󡄨
󡄨
|𝑃 (0)| = 󡄨󡄨󡄨−π‘₯ (𝑑0 + 𝑇, 0)󡄨󡄨󡄨 = 󡄨󡄨󡄨π‘₯ (𝑑0 + 𝑇, 0)󡄨󡄨󡄨 ≤ 𝑁.
π‘˜ ∈ Z+ ,
(51)
By (H2) and Lemma 10, we know 𝑔(𝑑 + 𝑇, −𝑦) = −𝑔(𝑑, 𝑦),
𝑔(𝑑, 0) = 0, β„Žπ‘˜+π‘ž (𝑦) = β„Žπ‘˜ (𝑦), and πœπ‘˜+π‘ž − πœπ‘˜ = 𝑇, for all π‘˜ ∈ Z+ .
Next, we consider the following perturbed system of
system (1):
𝑑
𝑓 (𝑑, 𝑁) ≤ 0,
𝑑 =ΜΈ πœπ‘˜ ,
+ 𝐴 3 (𝑑, πœ€) 𝑦3 + π‘œ (𝑦3 ) ,
(50)
This implies that 𝑃(π‘₯0 ) is well defined for |π‘₯0 | ≤ |𝑃(0)|. By
Theorem 22, we obtain that (1) has a unique one-side periodic
orbit.
π»π‘˜ (𝑦, πœ€) = π΅π‘˜1 (πœ€) 𝑦 + π΅π‘˜3 (πœ€) 𝑦3 + π‘œ (𝑦3 ) ,
where
𝐴 𝑖 (𝑑, πœ€) =
1 πœ•π‘– 𝐹
(𝑑, π‘₯∗ , πœ€) ,
𝑖! πœ•π‘₯𝑖
π΅π‘˜π‘— (πœ€) =
1 πœ•π‘—ΜƒπΌπ‘˜ ∗
(π‘₯ , πœ€) ,
𝑗! πœ•π‘₯𝑗
4. Double-Period Bifurcation
In this section, we mainly discuss the bifurcation on periodic
orbits. If system (1) has a one-side periodic orbit, without
losing generality, we may assume that 𝑓(𝑑, 0) = 0; that is,
π‘₯ = 0 is the one-side periodic orbit. Actually, if π‘₯(𝑑) is a
one-side periodic orbit, then we let 𝑦 = π‘₯ − π‘₯(𝑑); therefore
(54)
𝐴 𝑖 (𝑑 + 𝑇, πœ€) = (−1)𝑖−1 𝐴 𝑖 (𝑑, πœ€) ,
for π‘˜ ≥ 1, 𝑖 = 1, 2, 3; 𝑗 = 1, 3.
(55)
8
Abstract and Applied Analysis
If πœ€ = 0, then π‘₯∗ = 0. So 𝐴 𝑖 (𝑑, 0) = (1/𝑖!)(πœ•π‘– 𝑓/πœ•π‘₯𝑖 )(𝑑, 0)
(𝑗)
and π΅π‘˜π‘— (0) = (1/𝑗!)πΌπ‘˜ (0), for π‘˜ ≥ 1, 𝑖 = 1, 2, 3, 𝑗 = 1, 3.
Suppose that 𝑦(𝑑, 𝑦0 , πœ€) (𝑑 ≥ 𝑑0 ) is the solution of system
(53) with the initial value 𝑦(𝑑0+ , 𝑦0 , πœ€) = 𝑦0 , 𝑃(𝑦0 , πœ€) is the
Poincaré map of system (53). Note
Μƒ (𝑦0 , πœ€) = 𝑦 (𝑑0 + 2𝑇+ , 𝑦0 , πœ€) = 𝑃2 (𝑦0 , πœ€) .
𝑃
(56)
By the implicit function theorem, there exists a unique
Μƒ
function 𝑦0 = 𝑦1 (πœ€), 𝑦1 (0) = 0 such that (πœ•π‘‘/πœ•π‘¦
0 )(𝑦1 (πœ€), πœ€) =
0. Therefore, for |πœ€| sufficiently small, there is a unique
extremal point 𝑦0 = 𝑦1 (πœ€) near π‘₯ = 0. Moreover, the function
Μƒ , πœ€) takes its minimum (maximum) Δ(πœ€) ≡ 𝑑(𝑦
Μƒ (πœ€), πœ€)
𝑑(𝑦
0
1
∗
only if π‘Ž3 > 0 (<0):
2
Without losing generality, let π‘₯∗ (𝑑, πœ€) = 0 is a nonhyperbolic
solution. That is, 𝑃(0, 0) = 0 and (πœ•π‘ƒ/πœ•π‘¦0 )(0, 0) = −1.
Noting that 𝑃(0, πœ€) = 0, then by Taylor’s formula, we have
Δ (πœ€) = 𝑑0 (πœ€) + π‘œ (πœ€) = 𝐴1 (πœ€) − 1 = −2 [𝐴1 (πœ€) + 1] + π‘œ (πœ€) .
(61)
𝑃 (𝑦0 , πœ€) = 𝐴1 (πœ€) 𝑦0 + 𝐴2 (πœ€) 𝑦02 + 𝐴3 (πœ€) 𝑦03 + π‘œ (𝑦03 ) , (57)
Without loss of generality, we can let π‘Ž3∗ = 𝑑2 (0) > 0 and
then 𝑦0 = 0 is the minimum point of 𝑑(𝑦0 , 0). So there exists
πœ€0 > 0, such that
where 𝐴1 (πœ€) = (πœ•π‘ƒ/πœ•π‘¦0 )(0, πœ€), 𝐴2 (πœ€) = (1/2)(πœ•2 𝑃/πœ•π‘¦02 )(0, πœ€),
and 𝐴3 (πœ€) = (1/6)(πœ•3 𝑃/πœ•π‘¦03 )(0, πœ€).
Theorem 24. Suppose that 𝑓(𝑑, 0) = 0 and π‘₯ = 0 is a oneside periodic orbit of system (52)πœ€=0 with 𝑃(0, 0) = 0 and
Μƒ σΈ€ σΈ€ σΈ€  (0, 0). If π‘Ž∗ =ΜΈ 0, then
(πœ•π‘ƒ/πœ•π‘¦0 )(0, 0) = −1. Let π‘Ž3∗ = (1/6)𝑃
3
for |πœ€| sufficiently small and [𝐴1 (πœ€) + 1]π‘Ž3∗ > 0 (≤0) implies
that system (52) has a unique (no) two-sides periodic orbit near
π‘₯ = 0, except for a one-side periodic orbit π‘₯∗ (𝑑, πœ€).
σΈ€ 
2
Μƒ (0, πœ€) = [𝑃󸀠 (0, πœ€)]2 = 𝐴 (πœ€):
Proof. As before, we obtain that 𝑃
1
Μƒ
πœ•π‘‘
(πœ€ , 0) > 0,
πœ•π‘¦0 0
Μƒ (±πœ€ , 0) > 0,
𝑑
0
Μƒ 2 ) (𝑦 , 0) > 0 exists. Therefore, there
and for |𝑦0 | ≤ πœ€0 , (πœ•2 𝑑/πœ•π‘¦
0
0
exists a 𝛿0 , such that, for |πœ€| ≤ 𝛿0 , we have
Μƒ
πœ•π‘‘
(πœ€ , πœ€) > 0,
πœ•π‘¦0 0
Μƒ (±πœ€ , πœ€) > 0,
𝑑
0
Μƒ (𝑦0 , πœ€) = 𝑃 (𝑃 (𝑦0 , πœ€) , πœ€)
𝑃
= 𝐴1 (πœ€) 𝑃 (𝑦0 , πœ€) + 𝐴2 (πœ€) 𝑃2 (𝑦0 , πœ€)
3
2
= 𝐴1 (πœ€) 𝑦0 + [𝐴1 (πœ€) + 𝐴1 (πœ€)] 𝐴2 (πœ€) 𝑦02
2
Μƒ
πœ•π‘‘
(−πœ€0 , πœ€) < 0.
πœ•π‘¦0
(63)
For |πœ€| ≤ 𝛿0 and |𝑦0 | ≤ πœ€0 , we have
3
+ 𝐴3 (πœ€) 𝑃 (𝑦0 , πœ€) + π‘œ (𝑃 (𝑦0 , πœ€))
2
Μƒ
πœ•π‘‘
(−πœ€0 , 0) < 0,
πœ•π‘¦0
(62)
Μƒ
πœ•2 𝑑
(𝑦 , πœ€) > 0.
πœ•π‘¦02 0
(58)
2
(64)
From (64), for any |πœ€| ≤ 𝛿0 , we have
+ 𝐴1 [𝐴3 (πœ€) + 2𝐴2 (πœ€) + 𝐴1 (πœ€) 𝐴3 (πœ€)] 𝑦03
Μƒ (𝑦 , πœ€) ,
Δ (πœ€) = min 𝑑
0
+ π‘œ (𝑦03 ) .
|𝑦0 |≤πœ€0
−πœ€0 < 𝑦1 (πœ€) < πœ€0 .
(65)
σΈ€ 
By our assumption, we have 𝐴1 (πœ€) = −1 + 𝐴1 (0)πœ€ + π‘œ(πœ€).
Therefore,
2
Μƒ (𝑦 , πœ€) = 𝑃 (𝑦0 , πœ€) − 𝑦0
𝑑
0
𝑦0
(59)
= 𝑑0 (πœ€) + 𝑑1 (πœ€) 𝑦0 + 𝑑2 (πœ€) 𝑦02 + π‘œ (𝑦02 ) ,
where
2
𝑑0 (πœ€) = 𝐴1 (πœ€) − 1 = −2 [𝐴1 (πœ€) + 1] + π‘œ ([𝐴1 (πœ€) + 1]) ,
2
𝑑1 (πœ€) = [𝐴1 (πœ€) + 𝐴1 (πœ€)] 𝐴2 (πœ€)
And for 𝑦0 ∈ (−πœ€0 , 𝑦1 (πœ€))(∈ (𝑦1 (πœ€), πœ€0 )),
Μƒ
πœ•π‘‘
(𝑦 , πœ€) < 0 (> 0) .
πœ•π‘¦0 0
If Δ(πœ€) > 0, then for all |πœ€| ≤ 𝛿0 and |π‘₯0 | < πœ€0 , we have
Μƒ
0 < Δ(πœ€) ≤ 𝑑.
If Δ(πœ€) = 0, then 𝑦0 = 𝑦1 (πœ€) is the unique solution of
Μƒ
function 𝑑.
If Δ(πœ€) < 0, then there exist a unique 𝑦1 (πœ€) and a unique
𝑦2 (πœ€), such that
σΈ€ 
= 𝑂 (𝐴1 (πœ€) + 1) = −𝐴1 (0) 𝐴2 (0) πœ€ + π‘œ (πœ€) ,
2
Μƒ (𝑦 (πœ€) , πœ€) = 0,
𝑑
𝑖
2
𝑑2 (πœ€) = 𝐴1 (πœ€) [𝐴3 (πœ€) + 2𝐴2 (πœ€) + 𝐴1 (πœ€) 𝐴3 (πœ€)]
2
= − 2 [𝐴2 (0) + 𝐴3 (0)] + π‘œ (1) = π‘Ž3∗ + π‘œ (1) .
(60)
(66)
Μƒ
πœ•π‘‘
(𝑦 (πœ€) , πœ€) =ΜΈ 0,
πœ•π‘¦0 𝑖
𝑖 = 1, 2.
(67)
Thus system (52) has two (no) two-side periodic orbits if
π‘Ž3∗ Δ(πœ€) < 0 (≥0). The conclusion is completed (see Figures
4, 5, and 6).
Abstract and Applied Analysis
9
𝑑
𝑑
−πœ€0
𝑂
πœ€0
−πœ€0
π‘₯0
𝑂
πœ€0
π‘₯0
Δ<0
Δ>0
Figure 6
Figure 4
𝑑
From (69) and (70), we have
𝑑
πœ‘1 (𝑑, πœ€) = exp ∫ 𝐴 1 (𝑒, πœ€) 𝑑𝑒,
𝑑0
𝑑
−πœ€0
𝑂
πœ€0
πœ‘2 (𝑑, πœ€) = πœ‘1 (𝑑, πœ€) ∫ 𝐴 2 (𝑠, πœ€) πœ‘1 (𝑠, πœ€) 𝑑𝑠,
π‘₯0
𝑑0
πœ‘3 (𝑑, πœ€) = πœ‘1 (𝑑, πœ€)
𝑑
Δ=0
× ∫ [2𝐴 2 (𝑠, πœ€) πœ‘2 (𝑠, πœ€) + 𝐴 3 (𝑠, πœ€) πœ‘12 (𝑠, πœ€)] 𝑑𝑠.
𝑑0
Figure 5
(71)
Now we shall calculate 𝐴1 (0) and π‘Ž3∗ in the simplest case,
let π‘ž = 1. For π‘ž > 1 we can calculate them in the same way.
In this case, πΌπ‘˜ ≡ 𝐼 and π΅π‘˜π‘– (𝑦0 , πœ€) = 𝐡𝑖 (𝑦0 , πœ€), 𝑖 = 1, 3. Suppose
𝑦(𝑑, 𝑦0 , πœ€) (𝑑 ≤ 𝑑0 ) is the solution to system (53) with initial
value 𝑦(𝑑0 +, 𝑦0 , πœ€) = 𝑦0 . For 𝑦(𝑑, 0, πœ€) = 0, let
𝑑 ≤ 𝑑0 .
𝐴 2 (𝑑, πœ€) πœ‘12
= πœ‘1 (𝑑0 + 𝑇+ , πœ€) 𝑦0 + πœ‘2 (𝑑0 + 𝑇+ , πœ€) 𝑦02
+ πœ‘3 (𝑑0 + 𝑇+ , πœ€) 𝑦03 + π‘œ (𝑦03 ) ,
(72)
where
πœ‘2 (𝑑0 + 𝑇+ , πœ€) = [1 + 𝐡1 (πœ€)] πœ‘2 (𝑑0 + 𝑇, πœ€)
(𝑑, πœ€) ,
+ 𝐡2 (πœ€) πœ‘12 (𝑑0 + 𝑇, πœ€) ,
πœ‘3σΈ€  (𝑑, πœ€) = 𝐴 1 (𝑑, πœ€) πœ‘3 (𝑑, πœ€) + 2𝐴 2 (𝑑, πœ€) πœ‘1 (𝑑, πœ€) πœ‘2 (𝑑, πœ€)
+ πœ‘3 (𝑑, πœ€) πœ‘13 (𝑑, πœ€) .
πœ‘3 (𝑑0 + 𝑇+ , πœ€) = [1 + 𝐡1 (πœ€)] πœ‘3 (𝑑0 + 𝑇, πœ€)
(69)
πœ‘2 (0, πœ€) = πœ‘3 (0, πœ€) = 0.
+ 2𝐡2 (πœ€) πœ‘1 (𝑑0 + 𝑇, πœ€) πœ‘2 (𝑑0 + 𝑇, πœ€)
+ 𝐡3 (πœ€) πœ‘3 (𝑑0 + 𝑇, πœ€) .
(73)
For 𝑦(0, 𝑦0 , πœ€) = 𝑦0 , we know
πœ‘1 (0, πœ€) = 1,
+ 𝐡3 (πœ€) 𝑦3 (𝑑0 + 𝑇, πœ€)
πœ‘1 (𝑑0 + 𝑇+ , πœ€) = [1 + 𝐡1 (πœ€)] πœ‘1 (𝑑0 + 𝑇, πœ€) ,
πœ‘1σΈ€  (𝑑, πœ€) = 𝐴 1 (𝑑, πœ€) πœ‘1 (𝑑, πœ€) ,
(𝑑, πœ€) = 𝐴 1 (𝑑, πœ€) πœ‘2 (𝑑, πœ€) +
+ 𝐡2 (πœ€) 𝑦2 (𝑑0 + 𝑇, πœ€)
(68)
Then for 𝑑 ∈ [𝑑0 , 𝑑0 + 𝑇], taking 𝑦(𝑑, 𝑦0 , πœ€) into system
(53), we can obtain πœ‘1 , πœ‘2 , and πœ‘3 satisfying the following
equations:
πœ‘2σΈ€ 
𝑦 (𝑑0 + 𝑇+ , 𝑦0 , πœ€) = [1 + 𝐡1 (πœ€)] 𝑦 (𝑑0 + 𝑇, πœ€)
+ π‘œ (𝑦3 (𝑑0 + 𝑇, πœ€))
𝑦 (𝑑, 𝑦0 , πœ€) = πœ‘1 (𝑑, πœ€) 𝑦0 + πœ‘2 (𝑑, πœ€) 𝑦02
+ πœ‘3 (𝑑, πœ€) 𝑦03 + π‘œ (𝑦03 ) ,
For 𝑑0 < 𝑑 < 𝑑0 + 𝑇, as we know, we get
(70)
Clearly, 𝐴1 (πœ€) = −πœ‘1 (𝑑0 + 𝑇+ , πœ€), 𝐴2 (πœ€) = −πœ‘2 (𝑑0 + 𝑇+ , πœ€), and
𝐴3 (πœ€) = −πœ‘3 (𝑑0 + 𝑇+ , πœ€).
10
Abstract and Applied Analysis
Theorem 25. Suppose that 𝑓(𝑑, 0) = 0 and π‘₯ = 0 is a oneside periodic solution of system (52)πœ€=0 with 𝑃(0, 0) = 0 and
(πœ•π‘ƒ/πœ•π‘¦0 )(0, 0) = −1. Let
Moreover, we know
∫
𝑑0 +𝑇
𝑑0
𝐴 2 (𝑠, πœ€) πœ‘2 (𝑠, πœ€) 𝑑𝑠
=∫
𝑑0 +𝑇
σΈ€ 
𝐴1 (πœ€) = − (1 + ̃𝐼 (π‘₯∗ , πœ€)) exp ∫
𝑑0
𝐴 2 (𝑠, πœ€) πœ‘1 (𝑠, πœ€)
𝑑0
𝑑0 +𝑇
(74)
𝑠
× [∫ 𝐴 2 (𝑒, πœ€) πœ‘1 (𝑒, πœ€) 𝑑𝑒] 𝑑𝑠
π‘Ž3∗ =
𝐹π‘₯ (𝑑, π‘₯∗ , πœ€) 𝑑𝑑,
𝑠
1 𝑑0 +2𝑇 σΈ€ σΈ€ σΈ€ 
2 ∫ 𝑓 (𝑒,0)𝑑𝑒
𝑓π‘₯ (𝑠, 0) 𝑒 𝑑0 π‘₯
𝑑𝑠 +
∫
6 𝑑0
σΈ€ σΈ€ σΈ€ 
2̃𝐼 (0)
𝑑0
𝑑0 +𝑇
1
= [∫
2 𝑑0
𝑑 +𝑇
Denote Φ(πœ€) = ∫𝑑 0
0
𝑇, πœ€). Then,
If π‘Ž3∗ =ΜΈ 0, then for |πœ€| sufficiently small, [𝐴1 (πœ€) + 1]π‘Ž3∗ > 0 (≤0)
implies that system (52) has a unique (no) two-side periodic
orbit of near π‘₯ = 0, except for a one-side periodic orbit π‘₯∗ (𝑑, πœ€).
𝐴 2 (𝑒, πœ€) πœ‘1 (𝑒, πœ€) 𝑑𝑒] .
𝐴 2 (𝑑, πœ€)πœ‘1 (𝑑, πœ€)𝑑𝑑 and πœ™1 (πœ€) = πœ‘1 (𝑑0 +
πœ‘2 (𝑑0 + 𝑇, πœ€) = πœ™1 (πœ€) Φ (πœ€) ,
𝑑0 +𝑇
𝑑0
𝐴 3 (𝑠, πœ€) πœ‘12 (𝑠, πœ€) 𝑑𝑠.
(75)
Then we can obtain
𝑑0 +𝑇
𝐴1 (πœ€) = − [1 + 𝐡1 (πœ€)] exp (∫
𝑑0
× [Φ (πœ€) + ∫
𝑑0 +𝑇
(76)
𝐴 3 (𝑠, πœ€) πœ‘12
𝑑0
(𝑠, πœ€) 𝑑𝑠]
where
𝑑0 +𝑇
∫𝑑
0
Δ(πœ€)
=
𝑠
𝐡3 (0)
[1 + 𝐡1 (0)]
𝑑0 +𝑇
∫𝑑
0
3
− Δ (0) ,
𝐴 3 (𝑠, πœ€)πœ‘12 (𝑠, πœ€)𝑑𝑠
3
Δπ‘₯|𝑑=π‘˜πœ‹ = −πœ€π‘₯ (π‘˜πœ‹) + (𝑏3 + πœ€) π‘₯ (π‘˜πœ‹) ,
𝑑 =ΜΈ π‘˜πœ‹,
(81)
+
π‘˜∈Z ,
(77)
(78)
Acknowledgments
For 𝐴1 (0) = −1, we can have πœ™1 (0) = 1/(1 + 𝐡1 (0)). Then
𝐴3 (0) = −Φ2 (0) −
𝑑π‘₯
= πœ€2 π‘₯ + |πœ€| (sin 𝑑) π‘₯2 − (1 − 2 cos 2𝑑) π‘₯3 ,
𝑑𝑑
where |πœ€| > 0. It is obvious that for |πœ€| > 0 sufficiently small,
π‘₯ − πœ€π‘₯ + (𝑏3 + πœ€)π‘₯3 is strictly increasing, and then π‘₯∗ (𝑑, πœ€) = 0
is the unique πœ‹-periodic solution. By direct computation, we
have 𝐴 1 (𝑑, πœ€) = πœ€2 , 𝐴 2 (𝑑, πœ€) = |πœ€|(sin 𝑑), 𝐴 3 (𝑑, πœ€) = 2 cos 2𝑑 − 1,
𝐡1 (πœ€) = −πœ€, and 𝐡3 (πœ€) = 𝑏3 + πœ€. Therefore, 𝐴1 (πœ€) + 1 = (πœ€ −
2
1)π‘’πœ€ πœ‹ + 1 = πœ€ + π‘œ(πœ€), π‘Ž3∗ = 2𝑏3 − πœ‹. It follows from Theorem 25
that system (81) has two (no) 2πœ‹-periodic solution of near
π‘₯ = 0 if |πœ€| is sufficiently small and π‘Ž3∗ πœ€ > 0 (≤0).
− 𝐡3 (πœ€) πœ™13 (πœ€) .
𝐴2 (0) = −Φ (0) ,
Corollary 26. (i) Let 𝐴1 (0) = −1, π‘Ž3∗ > 0 (<0). Then π‘₯ = 0 is
a nonhyperbolic one-side periodic orbit of system (48) (πœ€ = 0),
which is asymptotically stable (unstable). (ii) Let 𝐴1 (0) = −1,
[𝐴1 (πœ€) + 1]π‘Ž3∗ > 0, 0 < |πœ€| β‰ͺ 1. Then (𝐴1 (πœ€) + 1) < 0 (>0),
π‘₯∗ (𝑑, πœ€) is a hyperbolic one-side periodic orbit of system (48)
(πœ€ = 0), which is asymptotically stable (unstable. Moreover, the
two-side periodic orbit is unstable (asymptotically stable) near
π‘₯ = 0.
Example 27. Consider
𝐴2 (πœ€) = − [1 + 𝐡1 (πœ€)] πœ™1 (πœ€) Φ (πœ€) ,
2
By virtue of Theorem 25, we can have the following
conclusion.
Finally, we give an example to illustrate it.
𝐴 1 (𝑒, πœ€) 𝑑𝑒) ,
𝐴3 (πœ€) = − [1 + 𝐡1 (πœ€)] πœ™1 (πœ€)
.
(80)
2
πœ‘3 (𝑑0 + 𝑇, πœ€) = πœ™1 (πœ€) Φ2 (πœ€) + ∫
3
σΈ€ 
[1 + ̃𝐼 (0)]
=
𝐴 3 (𝑠, πœ€) exp[2 ∫𝑑 𝐴 1 (𝑒, πœ€)𝑑𝑒]𝑑𝑠. Therefore,
This work was supported by National Natural Science Foundation of China (no. 11271261), Shanghai Natural Science
Foundation (no. 12ZR1421600), and Shanghai Educational
Committee Project (10YZ74).
0
2
π‘Ž3∗ = −2 [𝐴2 (0) + 𝐴3 (0)] = 2Δ (0) +
2𝐡3 (0)
.
3
[1 + 𝐡1 (0)]
References
(79)
By considering (76)–(79), we can easily have the following
theorem when π‘ž = 1.
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