Research Article Bifurcation Analysis of an SIR Epidemic Model with the Contact Transmission Function Guihua Li1 and Gaofeng Li2 1 School of Science, North University of China, Taiyuan, Shanxi 030051, China 2 Xinjiang Agriculture Second Division Korla Hospital, Korla, Xinjiang 841000, China Correspondence should be addressed to Guihua Li; ttl1013@163.com Received 8 December 2013; Accepted 23 December 2013; Published 21 January 2014 Academic Editor: Kaifa Wang Copyright © 2014 G. Li and G. Li. 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. We consider an SIR endemic model in which the contact transmission function is related to the number of infected population. By theoretical analysis, it is shown that the model exhibits the bistability and undergoes saddle-node bifurcation, the Hopf bifurcation, and the Bogdanov-Takens bifurcation. Furthermore, we find that the threshold value of disease spreading will be increased, when the half-saturation coefficient is more than zero, which means that it is an effective intervention policy adopted for disease spreading. However, when the endemic equilibria exist, we find that the disease can be controlled as long as we let the initial values lie in the certain range by intervention policy. This will provide a theoretical basis for the prevention and control of disease. 1. Introduction The classical SIR model for disease transmission has been widely studied. It is one of the most important issues that the dynamical behaviors are changed by the different incidence rate in epidemic system. For the incidence rate, we divided into two categories: one is that Capasso and Serio [1] proposed the infection force which is a saturated curve, described “crowding effect” or “protection measures;” the other is the infection force that describes the effect of “intervention policy,” for example, closing schools and restaurants and postponing conferences (see Figure 1). For the model with the saturated infection force, 𝑎𝐼2 /(𝑏 + 𝐼2 ), which is one of the typical infection forces, the rich dynamical behaviors were founded by Ruan and Wang [2] and Tang et al. [3]. The model with the incidence rate can be suited for many infectious diseases, including measles, mumps, rubella, chickenpox, and influenza. For more research literatures about nonlinear infection rate see [4–9]. However, for some parasite-host models, by observing macro- and microparasitic infections, one finds that the infection rate is an increasing function of the parasite dose, usually sigmoidal in shape [10, 11]. So we will build a model with sigmoidal incidence rate which is taken into account “crowding effect” and “saturated effect.” According to the parasite-host model which is proposed by Anderson and May (1979) [12, 13], the model is as follows: 𝑑𝑆 𝑑𝑡 = 𝐴 − 𝑑𝑆 − 𝛽 (𝐼) 𝑆, 𝑑𝐼 𝑑𝑡 = 𝛽 (𝐼) 𝑆 − (𝑑 + 𝛾 + 𝜖) 𝐼, 𝑑𝑅 𝑑𝑡 = 𝛾𝐼 − 𝑑𝑅, (1) where 𝑆, 𝐼, 𝑅 are susceptible hosts, infected hosts, and removed hosts, respectively. 𝐴 is the birth rate of susceptible host, 𝑑 is the natural death rate of a population, 𝛾 is the removal rate, and 𝜖 is the per capita infection-related death rate. If we denote infection force 𝛽(𝐼) = 𝑔(𝐼)𝐼, 𝑔(𝐼) can be explained as the rate of valid contact. At the beginning of disease, most people have poor awareness of prevention, then the rate of valid contact 𝑔(𝐼) can be first increasing then tends to a certain value. As the time flies, people are gradually aware of the seriousness and take measures to prevent and control development of the disease and will reduce to be contact with infected, so the rate of contact 𝑔(𝐼) is first increasing then Hindawi Publishing Corporation Abstract and Applied Analysis Volume 2014,Article ID 930541, 7 pages http://dx.doi.org/10.1155/2014/930541 2 Abstract and Applied Analysis 𝛽(I) 𝛽 O I (a) Case 0 ≤ 𝑎 𝛽(I) 𝛽 O I1/a (b) Case −2√ 𝑏 < 𝑎 < 0 Figure 1: The plotting for the contact transmission function 𝛽(𝐼). decreasing. In short time, it does not tend to zero, but tends to a nonzero constant. To simplify the study, we take 𝑔 (𝐼) = 𝛽𝐼2 𝑏 + 𝑎𝐼 + 𝐼2 , (2) where 𝑏 > 0 and −2√ 𝑏 < 𝑎. If 𝑎 ≥ 0, 𝑔(𝐼) is increasing monotonically and tends to 𝛽. If −2√ 𝑏 < 𝑎 < 0, 𝑔(𝐼) is first increasing then decreasing and tends to 𝛽 (see Figure 1). Then model (1) becomes 𝑑𝑆 𝑑𝑡 = 𝐴 − 𝑑𝑆 − 𝛽𝑆𝐼3 𝑏 + 𝑎𝐼 + 𝐼2 , 𝑑𝐼 𝑑𝑡 = 𝛽𝑆𝐼3 𝑏 + 𝑎𝐼 + 𝐼2 − (𝑑 + 𝛾 + 𝜖) 𝐼, 𝑑𝑅 𝑑𝑡 = 𝛾𝐼 − 𝑑𝑅, (3) where 𝛽 is the valid contact coefficient. When 𝑎 = 0 and 𝑏 = 0, model (3) becomes 𝑑𝑆 𝑑𝑡 = 𝐴 − 𝑑𝑆 − 𝛽𝑆𝐼, 𝑑𝐼 𝑑𝑡 = 𝛽𝑆𝐼 − 𝜇𝐼, 𝑑𝑅 𝑑𝑡 = 𝛾𝐼 − 𝑑𝑅, (4) where 𝜇 = 𝑑 + 𝛾 + 𝜖. We know that 𝑅0 = 𝛽𝐴/𝑑𝜇 is the basic reproduction number of (4). It is easy to see that there is a unique positive equilibrium 𝐼∗ in system (4) when 𝑅0 > 1 and there is no positive equilibrium when 𝑅0 ≤ 1. In the next sections, we will study that parameters 𝑎 and 𝑏 would have any effect on the dynamic behaviors of model (3). The organization of this paper is as follows. In the next section, we analyze the existence and stability of the endemic equilibria for model (3). Then we discuss conditions for the Hopf bifurcation and the Bogdanov-Takens bifurcation in Sections 3. Section 4 presents numerical simulations to indicate dynamical behaviors and bifurcation structures, and gives with a brief discussion. 2. Existence and Stability of Equilibria We consider the positive equilibria of (3). Setting the right hand sides of system (3) to zero, we find that the first and second equations of system (3) do not include 𝑅, so we only consider 𝐴 − 𝑑𝑆 − 𝛽𝑆𝐼3 𝑏 + 𝑎𝐼 + 𝐼2 = 0, 𝛽𝑆𝐼3 𝑏 + 𝑎𝐼 + 𝐼2 − 𝜇𝐼 = 0. (5) From the above two equations, except for the disease-free equilibrium (DFE) at (𝐴/𝑑, 0), any endemic equilibrium (EE), if exists, is the intersection of the following two curves in the positive quadrant 𝑆 = 𝐴 − 𝜇𝐼 𝑑 , 𝑆 = 𝜇 (𝑏 + 𝑎𝐼 + 𝐼2 ) 𝛽𝐼2 . (6) From (6), 𝐼 must satisfy the following equation: 𝐻 (𝐼) := 𝛽𝐼3 + 𝑑 (1 − 𝑅0) 𝐼2 + 𝑑𝑎𝐼 + 𝑑𝑏 = 0. (7) Thus the intersection of two curves (6) is transformed into the positive root of (7). The derivative of 𝐻󸀠 (𝐼) is 𝐻󸀠 (𝐼) := 3𝛽𝐼2 + 2𝑑 (1 − 𝑅0) 𝐼 + 𝑑𝑎. (8) In the following, we consider three cases according to the sign of 𝑎. By calculation, we have the following three theorems. Set 𝑎1 = 𝑑2 (1 − 𝑅0) 2 − 3𝛽𝑎𝑑, 𝑎2 = 27𝛽2 𝑑𝑏 − 𝑑𝑏 (1 − 𝑅0) (3𝛽𝑎𝑑 − 2𝑎1) . (9) Theorem 1. Suppose 𝑎 > 0. Then we have the following. (a) If 𝑅0 ≤ 1 + √3𝛽𝑎/𝑑, then system (3) has no endemic equilibrium. Abstract and Applied Analysis 3 (b) If 𝑅0 > 1 + √3𝛽𝑎/𝑑, then we have the following. (i) When 2𝑎3/2 1 < 𝑎2, system (3) has no endemic equilibrium. (ii) When 2𝑎3/2 1 = 𝑎2, system (3) has a unique endemic equilibrium. (iii) When 2𝑎3/2 1 > 𝑎2, system (3) has two endemic equilibria 𝐸1(𝑆1, 𝐼1), 𝐸2(𝑆2, 𝐼2). Theorem 2. Suppose 𝑎 = 0. Then we have the following. (a) If 𝑅0 < 1+ 3 √27𝛽2 𝑏/4𝑑2, then system (3) has no endemic equilibrium. (b) If 𝑅0 = 1 + 3 √27𝛽2 𝑏/4𝑑2, then system (3) has a unique endemic equilibrium. (c) If 𝑅0 > 1 + 3 √27𝛽2 𝑏/4𝑑2, then system (3) has two endemic equilibria 𝐸1(𝑆1, 𝐼1), 𝐸2(𝑆2, 𝐼2). Theorem 3. Suppose −2√ 𝑏 < 𝑎 < 0. Then we have the following. (a) If 2𝑎3/2 1 < 𝑎2, then system (3) has no endemic equi- librium. (b) If 2𝑎3/2 1 = 𝑎2, then system (3) has a unique endemic equilibrium 𝐸∗ (𝑆∗ , 𝐼∗ ). (c) If 2𝑎3/2 1 > 𝑎2, then system (3) has two endemic equilibria 𝐸1(𝑆1, 𝐼1), 𝐸2(𝑆2, 𝐼2), where 𝐼1 < 𝐼∗ < 𝐼2. Remark 4. From Theorems 1 and 2, we can find that the basic reproduction number for the model (3) is less than that of the standard model. It means that the disease will spread more easily. For Theorem 3, it is obvious that the disease can exist if 𝑅0 < 1. For disease-free equilibrium (DFE), it is easy to calculate that the Jacobian matrix of system (3) at DFE has eigenvalues 𝜆1 = −𝑑 and 𝜆2 = −𝜇. Hence, DFE is always stable. In the following, the stability of the endemic equilibrium in system (3) will be studied. Firstly, evaluating the Jacobian matrix of system (3) at 𝐸(𝑆, 𝐼) gives 𝐽 = ( 𝑗11 𝑗12 𝑗21 𝑗22 ) 󵄨󵄨󵄨󵄨󵄨󵄨󵄨󵄨(𝑆,𝐼) , (10) where 𝑗11 = −𝑑 − 𝛽𝐼3 𝑏 + 𝑎𝐼 + 𝐼2 , 𝑗12 = −𝜇 − 𝜇 (2𝑏 + 𝑎𝐼) 𝑏 + 𝑎𝐼 + 𝐼2 , 𝑗21 = 𝛽𝐼3 𝑏 + 𝑎𝐼 + 𝐼2 , 𝑗22 = 𝜇 (2𝑏 + 𝑎𝐼) 𝑏 + 𝑎𝐼 + 𝐼2 . (11) Its characteristic equation is 𝑃 (𝜆) = 𝜆2 − tr (𝐽) 𝜆 + det (𝐽) = 0, (12) where det (𝐽) = 𝛽𝜇𝐼3 − 𝑑𝑎𝜇𝐼 − 2𝑑𝑏𝜇 𝑏 + 𝑎𝐼 + 𝐼2 , (13) tr (𝐽) = −𝛽𝐴𝐼2 + 𝑎𝜇2 𝐼 + 2𝑏𝜇2 𝜇 (𝑏 + 𝑎𝐼 + 𝐼2) . (14) It is easy to calculate 𝛽𝜇𝐼∗3 − 𝑑𝑎𝜇𝐼∗ − 2𝑑𝑏𝜇 = 𝜇 [𝐼∗ 𝐻󸀠 (𝐼∗ ) − 2𝐻 (𝐼∗ )] = 0; (15) that is, det(𝐽)| 𝐼=𝐼∗ = 0. Now suppose that the model has two endemic equilibria 𝐸1(𝑆1, 𝐼1), 𝐸2(𝑆2, 𝐼2), with 𝐼1 < 𝐼∗ < 𝐼2 < 𝐴/𝜇; that is, in Theorem 1, the item (b) (iii) holds or Theorems 2 and 3, the item 𝑐 holds. If 𝐽𝑖 (𝑖 = 1, 2) is the Jacobian matrix at (𝑆𝑖, 𝐼𝑖), then (13) gives det (𝐽𝑖) = 𝛽𝜇𝐼3 − 𝑑𝑎𝜇𝐼 − 2𝑑𝑏𝜇 𝑏 + 𝑎𝐼 + 𝐼2 󵄨󵄨󵄨󵄨󵄨󵄨󵄨󵄨󵄨 𝐼=𝐼𝑖 . (16) Thus, it is easily obtained that det(𝐽1) is negative and det(𝐽2) is positive. We can immediately conclude that the endemic equilibrium 𝐸1 with low number of infected individuals is always a saddle, and that the endemic equilibrium 𝐸2 with high number of infected individuals is a node or focus but the stability of 𝐸2 is determined by tr(𝐽2). From (14), we notice that the sign of the trace of 𝐽2 is determined by tr 1 := −𝛽𝐴𝐼2 + 𝑎𝜇2 𝐼 + 2𝑏𝜇2 . (17) Set 𝑏0 := 𝑎𝜇2 + 𝜇√ 𝑎2 𝜇2 + 8𝛽𝐴𝑏 2𝛽𝐴 , 𝑏1 := −𝑑 (1 − 𝑅0) + √ 𝑎1 3𝛽𝜇 , 𝑟0 := 𝛽𝐴 (𝑎𝑏0 (𝐴 + 1) + 𝐴𝑏) , 𝑟1 := 𝑑 (𝑅0 − 1) (2 + 𝐴) (𝑎 + 2𝑏0 (1 − 𝑅0)) . (18) Theorem 5. Assume that (3) has two endemic equilibria. Then 𝐸2 is asymptotically stable if one of the following is satisfied. (a) 𝑏0 < 𝑏1; (b) 𝑏0 > 𝑏1 and 𝑟0 > 𝑟1. Further, 𝐸2 is unstable if 𝑏0 > 𝑏1 and 𝑟0 < 𝑟1. Proof. If 𝑏0 < 𝑏1, then −𝛽𝐴𝐼∗2 + 𝑎𝜇2 𝐼∗ + 2𝑏𝜇2 < 0. It follows from 𝐼2 > 𝐼∗ that tr 1 < 0. Hence, 𝐸2 is asymptotically stable in this case. If 𝑏0 > 𝑏1, we have 𝑏0 > 𝐼∗ . By direct calculations we see that 𝑟0 > 𝑟1 implies 𝐼2 > 𝑏0, which leads to tr 1 < 0. Therefore, 𝐸2 is asymptotically stable if condition (b) holds. Similarly, if 𝑏0 < 𝑏1 and 𝑟0 < 𝑟1, we have 𝐼2 > 𝑏0, which leads to tr 1 > 0. It follows that 𝐸2 is unstable. 4 Abstract and Applied Analysis 0.75 0.70 0.65 0.60 0.55 0.50 0.45 1.45 1.46 1.47 1.48 1.49 1.50 I R0R1 Figure 2: The bifurcation curves the palne of (𝐼, 𝑅0). 3. Bifurcation of the System 3.1. Hopf Bifurcation. When the condition (b) (ii) in Theorem 1 and the condition (b) in Theorems 2 and 3 hold and 𝑟0 = 𝑟1, there are a pair of purely imaginary eigenvalues (Figure 2). Thus for suitable parameter values a Hopf bifurcation may occur, which means that there is a periodic solution around the larger nontrivial equilibrium. In order to determine the type of the Hopf bifurcation, we set 𝑞1 := 𝜌𝑝3 (3𝛽𝑏𝐴 + 𝑎2 − 4𝑏) (2𝑏𝜇𝑝 + 𝑎𝜌𝐴) 2 , 𝑞2 := −2𝛽𝑆2 [(𝑎2 − 𝑏) 𝑏𝐼4 2 + 4𝑎𝑏𝐼3 2 + 6𝑏2 𝐼2 2 − 𝑏3 ] (𝑏 + 𝑎𝐼2 + 𝐼2) 4 . (19) Then we consider the transformation 𝑋 = 𝑆 − 𝑆2, 𝑌 = 𝐼 − 𝐼2 to move (𝑆2, 𝐼2) to the origin of (𝑋, 𝑌). After some manipulations, the model can be transformed into the following equations: 𝑑𝑋 𝑑𝑡 = 𝑎11 𝑋 + 𝑎12 𝑌 − 𝐶 (𝑋, 𝑌) , 𝑑𝑌 𝑑𝑡 = 𝑏11 𝑋 + 𝑏12 𝑌 + 𝐶 (𝑋, 𝑌) , (20) where 𝐶(𝑋, 𝑌) represents the higher order terms and 𝑎11 = −𝑑 − 𝛽𝐼3 2 𝑏 + 𝑎𝐼2 + 𝐼2 2 , 𝑎12 = −𝜇 − 𝜇 (2𝑏 + 𝑎𝐼2) 𝑏 + 𝑎𝐼2 + 𝐼2 2 , 𝑏11 = 𝛽𝐼3 2 𝑏 + 𝑎𝐼2 + 𝐼2 2 , 𝑏12 = 𝜇 (2𝑏 + 𝑎𝐼2) 𝑏 + 𝑎𝐼2 + 𝐼2 2 . (21) Suppose 𝑟0 = 𝑟1. Then tr (𝐽) = −𝑑 − 𝛽𝐼3 2 𝑏 + 𝑎𝐼2 + 𝐼2 2 + 𝜇 (2𝑏 + 𝑎𝐼2) 𝑏 + 𝑎𝐼2 + 𝐼2 2 = 0. (22) By defining 𝜌 = 𝛽𝐼3 2 /(𝑏 + 𝑎𝐼2 + 𝐼2 2 ) and 𝑝 = 𝜇(2𝑏 + 𝑎𝐼2)/(𝑏 + 𝑎𝐼2 + 𝐼2 2 ), it can be seen that 𝑎11 = −𝑑 − 𝜌, 𝑎12 = −𝜇 − 𝑝, 𝑏11 = 𝜌, 𝑏12 = 𝑝, 𝑑 = 𝑝 − 𝜌. (23) Set 𝜔 = √det (𝐽2) = √ 𝜇𝜌 − 𝑑𝑝. (24) Then the eigenvalues of 𝐽2 are 𝜆1 = 𝜔𝑖 and 𝜆2 = −𝜔𝑖. Now, using the transformation 𝑢 = 𝑋, V = −(1/𝜔)(𝑎11 𝑋+ 𝑎12 𝑌) to (20), we obtain 𝑑𝑢 𝑑𝑡 = −𝜔V + 𝐹1 (𝑢, V) , 𝑑V 𝑑𝑡 = 𝜔𝑢 + 𝐹2 (𝑢, V) , (25) where 𝐹1 (𝑢, V) = −𝐶 (𝑢, 𝜔V − 𝑝𝑢 𝜇 + 𝑝 ) , 𝐹2 (𝑢, V) = 𝜇 𝜔 𝐶 (𝑢, 𝜔V − 𝑝𝑢 𝜇 + 𝑝 ) . (26) If 𝜎 = 1 16 [ 𝜕3 𝐹1 𝜕𝑢3 + 𝜕3 𝐹2 𝜕𝑢 𝜕V2 + 𝜕3 𝐹2 𝜕𝑢2 𝜕V + 𝜕3 𝐹2 𝜕V3 ] + 1 16𝜔 [ 𝜕2 𝐹1 𝜕𝑢 𝜕V ( 𝜕2 𝐹1 𝜕𝑢2 + 𝜕2 𝐹1 𝜕V2 )− 𝜕2 𝐹2 𝜕𝑢 𝜕V ( 𝜕2 𝐹2 𝜕𝑢2 + 𝜕2 𝐹2 𝜕V2 ) − 𝜕2 𝐹1 𝜕𝑢2 𝜕2 𝐹2 𝜕𝑢2 + 𝜕2 𝐹1 𝜕V2 𝜕2 𝐹2 𝜕V2 ] 󵄨󵄨󵄨󵄨󵄨󵄨󵄨󵄨󵄨 𝑢=0,V=0 , (27) by some tedious calculations, we see that the sign of 𝜎 is determined by 𝜉, where 𝜉 = 𝐴2 𝑞1 (2𝑑𝜌𝑞1 + 𝜇𝑝2 (2𝑑𝑝 − 𝜇𝜌 − 4𝑝2 )) + 𝑝2 (𝑝3 (𝜇 + 𝑑) (𝜇 + 𝑝) 2 − 3𝑞2 𝜌𝐴2 𝜔2 ) . (28) By the results in [14], the direction of the Hopf bifurcation is determined by the sign of 𝜎. Therefore, we have the following result. Theorem 6. Suppose one condition of (c) in Theorem (6) holds and 𝑟0 = 𝑟1. If 𝜉 ̸= 0, then a curve of periodic solutions bifurcates from the endemic equilibrium 𝐸2 such that Abstract and Applied Analysis 5 (i) for 𝜉 < 0, system (3) undergoes a supercritical Hopf bifurcation; (ii) for 𝜉 > 0, system (3) undergoes a subcritical Hopf bifurcation. Remark 7. Theorems 5 and 6 imply the occurrence of the Allee effect because endemic equilibrium 𝐸2 and the diseasefree equilibrium can be stable at the same time, or a stable limit cycle and the disease-free equilibrium can be stable at the same time. 3.2. Bogdanov-Takens Bifurcations. The purpose of this subsection is to study the Bogdanov-Takens bifurcation of (3) when there is a unique degenerate positive equilibrium. Assume that (H1) (1) 𝑎 > 0, 𝑅0 > 1 + √3𝛽𝑎/𝑑 and 2𝑎3/2 1 = 𝑎2; (2) 𝑎 = 0 and 𝑅0 = 1 + 3 √27𝛽2 𝑏/4𝑑2; (3) 𝑎 < 0 and 2𝑎3/2 1 = 𝑎2. Then system (3) admits a unique positive equilibrium (𝑆∗ , 𝐼∗ ) if one of (H1) is satisfied. The Jacobian matrix of (3) at this point is 𝐽 = ( −𝑑 − 𝛽𝐼∗3 𝑏 + 𝑎𝐼∗ + 𝐼∗2 −𝜇 − 𝜇 (2𝑏 + 𝑎𝐼∗ ) 𝑏 + 𝑎𝐼∗ + 𝐼∗2 𝛽𝐼∗3 𝑏 + 𝑎𝐼∗ + 𝐼∗2 𝜇 (2𝑏 + 𝑎𝐼∗ ) 𝑏 + 𝑎𝐼∗ + 𝐼∗2 ) . (29) Since we are interested in codimension 2 bifurcations, we assume further (H2) 𝑟0 = 𝑟1 By (15), we have det (𝐽) = 𝛽𝜇𝐼∗3 − 𝑑𝑎𝜇𝐼∗ − 2𝑑𝑏𝜇 𝑏 + 𝑎𝐼∗ + 𝐼∗2 = 0. (30) Furthermore, (H2) implies that tr (𝐽) = −𝛽𝐴𝐼∗2 + 𝑎𝜇2 𝐼∗ + 2𝑏𝜇2 𝜇 (𝑏 + 𝑎𝐼∗ + 𝐼∗2) = 0. (31) Thus, (H1) and (H2) imply that the Jacobian matrix has a zero eigenvalue with multiplicity 2. This suggests that (3) may admit a Bogdanov-Takens bifurcation. The next theorem will confirm this. Theorem 8. Suppose that (H1) and (H2) hold. Then the equilibrium (𝑆∗ , 𝐼∗ ) of (3) is a cusp of codimension 2; that is, it is a Bogdanov-Takens singularity. Proof. In order to translate the interior equilibrium (𝑆∗ , 𝐼∗ ) to the origin, we set 𝑥 = 𝑆 − 𝑆∗ , 𝑦 = 𝐼 − 𝐼∗ . Expanding the right-hand side of the system (3) in a Taylor series about the origin, we obtain 𝑑𝑥 𝑑𝑡 = 𝑎11 𝑥 + 𝑎12 𝑦 + 𝑎21 𝑥𝑦 + 𝑎22 𝑦2 + 𝑃1 (𝑥, 𝑦) , 𝑑𝑦 𝑑𝑡 = − 𝑎2 11 𝑎12 𝑥 − 𝑎11 𝑦 − 𝑎21 𝑥𝑦 − 𝑎22 𝑦2 + 𝑃2 (𝑥, 𝑦) , (32) where 𝑃𝑖(𝑥, 𝑦) is a smooth function in (𝑥, 𝑦) at least of order three and 𝑎11 = −𝑑 − 𝛽𝐼∗3 𝑏 + 𝑎𝐼∗ + 𝐼∗2 < 0, 𝑎12 = −𝜇 − 𝜇 (2𝑏 + 𝑎𝐼∗ ) 𝑏 + 𝑎𝐼∗ + 𝐼∗2 2 < 0, 𝑎21 = −𝛽𝐼∗2 (3𝑏 + 2𝑎𝐼∗ + 𝐼∗2 ) (𝑏 + 𝑎𝐼∗ + 𝐼∗2) 2 < 0, 𝑎22 = −2𝛽𝑆∗ 𝐼∗ [3𝑏2 + 3𝑎𝑏𝐼∗ + (𝑎2 − 𝑏) 𝐼∗2 ] (𝑏 + 𝑎𝐼∗ + 𝐼∗2) 3 . (33) Set 𝑋 = 𝑥, 𝑌 = 𝑎11 𝑥 + 𝑎12 𝑦. Then (32) is transformed into 𝑑𝑋 𝑑𝑡 = 𝑌 + 𝑐1 𝑋2 + 𝑐2 𝑋𝑌 + 𝑐3 𝑌2 + 𝑄1 (𝑋, 𝑌) , 𝑑𝑌 𝑑𝑡 = −𝑑1 𝑋2 + 𝑑2 𝑋𝑌 + 𝑑3 𝑌2 + 𝑄2 (𝑋, 𝑌) , (34) where 𝑄𝑖 are smooth functions in (𝑋, 𝑌) at least of order three and 𝑐1 = 𝑎11 (𝑎11 𝑎22 − 𝑎12 𝑎21) 𝑎2 12 , 𝑑1 = 𝑎11 (𝑎12 𝑎21 − 𝑎11 𝑎22) (𝑎11 − 𝑎12) 𝑎2 12 , 𝑐2 = 𝑎12 𝑎21 − 2𝑎11 𝑎22 𝑎2 12 , 𝑑2 = (𝑎12 𝑎21 − 2𝑎11 𝑎22) (𝑎11 − 𝑎12) 𝑎2 12 , 𝑐3 = 𝑎22 𝑎2 12 , 𝑑3 = 𝑎22 (𝑎11 − 𝑎12) 𝑎2 12 . (35) Change the variables one more time by letting 𝑋 = 𝑋, 𝑃 = 𝑌 + 𝑐3 𝑌2 ; we have 𝑑𝑋 𝑑𝑡 = 𝑃 + 𝑐1 𝑋2 + 𝑐2 𝑋𝑌 + 𝑄3 (𝑋, 𝑃) , 𝑑𝑃 𝑑𝑡 = −𝑑1 𝑋2 + 𝑑2 𝑋𝑃 + 𝑑3 𝑃2 + 𝑄4 (𝑋, 𝑃) . (36) 6 Abstract and Applied Analysis Let 𝑋 = 𝑋, 𝑍 = 𝑃 − 𝑑3 𝑋𝑃. Then system (36) becomes 𝑑𝑋 𝑑𝑡 = 𝑍 + 𝑐1 𝑋2 + (𝑐2 + 𝑑3) 𝑋𝑍 + 𝑄5 (𝑋, 𝑍) , 𝑑𝑍 𝑑𝑡 = −𝑑1 𝑋2 + 𝑑2 𝑋𝑍 + 𝑄6 (𝑋, 𝑍) . (37) In order to obtain the canonical normal forms, we perform the transformation of variables by 𝑢 = 𝑋 − 𝑐2 + 𝑑3 2 𝑋2 , V = 𝑍 + 𝑐1 𝑋2 . (38) Then, we obtain 𝑑𝑢 𝑑𝑡 = V + 𝑅1 (𝑢, V) , 𝑑V 𝑑𝑡 = −𝑑1 𝑢2 + (𝑑2 + 2𝑐1) 𝑢V + 𝑅2 (𝑢, V) , (39) where 𝑅𝑖 are smooth functions in (𝑢, V) at least of the third order. Note that 𝑑1 > 0 and 𝑑2 + 2𝑐1 = −𝑎11 𝑎21 − 𝑎21 𝑎12 + 2𝑎22 𝑎11 𝑎12 . (40) In addition, by (30) and (31), it is obtained that 𝑎11 = − 𝐴 𝑆∗ , 𝑎12 = −𝜇 − 𝐴 𝑆∗ , 𝑎21 = 𝜇𝐼∗ 𝑆∗ , 𝑎22 = 𝐴 𝑆∗ , 𝐴2 𝑆∗2 = 𝜇𝐼∗ 𝑆∗ (𝜇 + 𝐴 𝑆∗ ) . (41) So 𝑑2 + 2𝑐1 = −𝑎11 𝑎21 − 𝑎21 𝑎12 + 2𝑎22 𝑎11 𝑎12 = 1 𝑎12 𝐴 (𝜇𝐼∗ − 𝐴) 𝑆∗2 > 0. (42) It follows that (3) admits that a Bogdanov-Takens bifurcation from [15, 16] or [17]. 4. Simulations and Conclusions In the following, we use numerical simulations, based upon the MatCont package [18], to reveal how parameters 𝑎 induce bifurcations and limit cycles in system (3). Firstly, by fixing 𝐴 = 2, 𝑑 = 0.1, 𝛽 = 0.8, 𝑏 = 2.4, 𝜖 = 0.6, 𝛾 = 0.2, we plot a 2D-plot of variable 𝐼 versus parameter 𝑎 shown in Figure 3. We find a Hopf bifurcation at 𝑎 = −0.090429, a limit point (fold) bifurcation at 𝑎 = 2.378982. The Lyapunov coefficient is 1.68171 × 10−2 , which means that the periodic orbits are unstable. Furthermore, 𝑎 is fixed −0.13; we observe the orbits of system (3) is how to vary with 𝑡. From Figure 4, we can find −8 −7 −6 −5 −4 −3 −2 −1 0 1 2 3 0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 a I H LP Figure 3: Bifurcation curves in (𝑎, 𝐼) plane by fixed 𝐴 = 2, 𝑑 = 0.1, 𝛽 = 0.8, 𝑏 = 2.4, 𝜖 = 0.6, 𝛾 = 0.2, where H denotes the Hopf bifurcation, LP is the limit point (flod) bifurcation. 4 6 8 10 12 14 16 18 20 0 0.5 1 1.5 2 0 50 S I t −300 −250 −200 −150 −100 −50 Figure 4: Phase trajectory in system (3) by fixed 𝐴 = 2, 𝑑 = 0.1, 𝛽 = 0.8, 𝑏 = 2.4, 𝜖 = 0.6, 𝛾 = 0.2, 𝑎 = −0.13. that the periodic orbits will occur, but the disease will die out when 𝑡 → +∞, though there exist the positive equilibria for system (3). Furthermore, we take 𝑅0 and 𝑎 as bifurcation parameters; from Figure 5, we can show that the system has no positive equilibrium when 𝑅0 and 𝑎 lie in the left side of red curve and two endemic equilibria when they are in the right side of red curve. If parameters 𝑅0 and 𝑎 are between red and green curves, we find that system will undergo Hopf bifurcation. In the paper, we built a model with contact transmission function and obtained the dynamical behaviors. From the analysis, we find that the threshold value of disease spreading will be larger. It means that it is an effective intervention policy adopted for disease spreading. For the disease-free equilibrium is always locally stable and when a positive equilibrium exist and is stable, we can control the disease as long as we let the initial values be in the certain range by intervention policy. If the positive equilibrium is unstable, the Abstract and Applied Analysis 7 0 5 10 15 20 25 30 0 2 4 6 8 10 LP LP H LP H GH GH R0 −2 a Figure 5: Bifurcation figure when 𝑅0 and 𝑎 are taken as bifurcation parameters in system (3) by fixed 𝐴 = 2, 𝑑 = 0.1, 𝛽 = 0.8, 𝑏 = 2.4, 𝜖 = 0.6, 𝛾 = 0.2. disease will die out. This will provide a theoretical basis for the prevention and control of disease. Conflict of Interests The authors declare that there is no conflict of interests regarding the publication of this paper. Acknowledgments This work is supported by the National Science Foundation of China (11201434, 11271369) and Shanxi Scholarship Council of China (2013-087). References [1] V. Capasso and G. Serio, “A generalization of the KermackMcKendrick deterministic epidemic model,” Mathematical Biosciences, vol. 42, no. 1-2, pp. 43–61, 1978. [2] S. Ruan and W. Wang, “Dynamical behavior of an epidemic model with a nonlinear incidence rate,” Journal of Differential Equations, vol. 188, no. 1, pp. 135–163, 2003. [3] Y. Tang, D. Huang, S. Ruan, and W. Zhang, “Coexistence of limit cycles and homoclinic loops in a SIRS model with a nonlinear incidence rate,” SIAM Journal on Applied Mathematics, vol. 69, no. 2, pp. 621–639, 2008. [4] D. Xiao and H. 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