Introduction
The stability problem of switching systems has attracted considerable attention during the past two decades. A switching system is composed of several systems with a switching signal to orchestrate among them. In studying such systems, we have learned that switching can produce very interesting and complex dynamical behaviors that might be beyond our imagination.
The stability analysis problem of switching systems can be classified into two categories; see [7], [12]. Firstly, we are concerned with the so-called absolute stability problem that whether it is possible to construct a switching law to achieve destabilization. In the spirit of variational approach, the absolute stability problem requires to investigate if the extremal trajectory is convergent, which is constructed so that each point on it gets away from the origin as far as possible. If so, then we can confirm that the overall switching system will stay stable for an arbitrary switching signal. Secondly, the stability analysis problem is purely intended to characterize the evolution of switching signal over time and its effect on stability. An important aspect of the time-evolution of switching signal is the density of the switching points distributed within an interval of time, which can be captured in terms of average dwell-times. To guarantee the stability of the overall system, conventionally, the multiple Lyapunov functions approach is used to derive constraint conditions on the average dwell-time; see, e.g., [7], [11], [12], [14]. The mechanism of this methodology is to make the period between any two successive switching points long enough so as to allow the overshoot caused by switching to fade. However, this may lead to conservatism because without knowing the phase of the overshoot, we actually suppress it simply according to the worst case.
In the present paper, we shall investigate the stability problem for a switching system composed of two planar linear subsystems, which are triggered into activation alternatively and periodically. In the research field of switching systems, the planar case indeed constitutes the most developed branch because a set of dedicated methods allow us to gain deep insight into the stability problem beyond simply using a general method to address it; see [2]–[5], [9], [10]. Within the context of periodic switching, we shall establish the mutual constraint conditions on the dwell-times of the subsystems to ensure the stability of the overall system. An invariant that plays a key role in describing the interrelations of the subsystem matrices is involved in the stability criteria. This signifies that the overall switching dynamics in a strong way depends on the interrelation of the subsystem matrices as well as the types of their eigenvalues. Moreover, the derived stability criteria do not depend on the particular choice of the coordinates and, therefore, allow a system to speak for itself.
As we know, the stability conditions derived through the multiple Lyapunov functions approach usually account for the effect of average dwell-time on stability in a linear manner. The result in [8] showed that conditions that are linear in the average dwell-time may be very restricted. Actually, the results posed in the present paper demonstrate that the dwell-times of the subsystems actually influence the overall switching dynamics in a highly nonlinear manner. Therefore, we are able to precisely determine the stability margin in the space constituted by the dwell-times and hence assess stability in a necessary and sufficient sense. On the other hand, to ensure this stability, the existing methods usually require the stable subsystems to play the dominant role in the overall switching dynamics, among others. For the sake of generality, we will not suppose the subsystems to be stable because this assumption turns out to be restricted. To demonstrate the theoretical results, we shall construct an example to show that two unstable subsystems with quite long periods to stay active may generate stable dynamics.
The remainder of this paper is organized as follows. In Section 2, we introduce the basic definitions and formulate the problem. In Section 3, we present the stability conditions in the time-domain space and give some explanations to the matters relevant to the results. An example is included in Section 4 to illustrate the theoretical results. Finally, this work is briefly summarized in Section 5.
Notation: Throughout this paper, we use the following notations. Let
Problem Formulation
Consider the planar switching system described as follows \begin{equation} \dot {x}(t)=A_{\sigma (t)}x(t),\quad x\in \mathbf {R}^{2}. \end{equation}
\begin{align}&\hspace {-0.5pc}\Big \{(\sigma (t_{0}),t_{0}=0),(\sigma (t_{1}),t_{1}),\notag \\&\qquad \qquad \qquad \quad \cdots,(\sigma (t_{k}),t_{k}) \big |\lim \limits _{k\rightarrow +\infty }t_{k}=+\infty \Big \}. \qquad \end{align}
\begin{align} e^{A_{\sigma (t_{k})}(t-t_{k})}e^{A_{\sigma (t_{k-1})}(t_{k}-t_{k-1})}\cdots e^{A_{\sigma (t_{0})}(t_{1}-t_{0})},\quad t\in \big[t_{k},t_{k+1}\big). \notag \\ {}\end{align}
Definition 1:
A switching rule is said to be periodic if the interval between two successive switching points satisfies \begin{equation*} t_{k+1}-t_{k}=\begin{cases} \tau _{1},& \sigma (t_{k})=1\\ \tau _{2},& \sigma (t_{k})=2 \end{cases},\quad k\geq 0 \end{equation*}
Hereafter, the switching signals will be considered to be periodic, and the system in (1) will be considered to be a periodic switching system unless otherwise specified. Therefore, our first observation is that when driven by a periodic switching signal, system (1) is asymptotically stable if and only if the eigenvalues of
Definition 2:
The periodic switching system in (1) is said to be asymptotically stable if the unit of its transition matrix
Within this context, the paper is devoted to characterize the joint effects of the dwell-times
Main Results
The following fact plays a key role in deriving our results, which can be directly checked.
Lemma 1[4]:
For two-dimensional square matrices \begin{equation*} \det (X+Y)=\det (X)+\det (Y)+\text {tr}(X)\text {tr}(Y)-\text {tr}(XY). \end{equation*}
Using Lemma 1 and the fact \begin{align} m(\mu):=&\det (e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}}-\mu I)\notag \\=&\mu ^{2}-\mu \text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})+e^{ \text {tr}(A_{1})\tau _{1}}e^{\text {tr}(A_{2})\tau _{2}}. \end{align}
\begin{equation*} [\text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})]^{2}-4e^{ \text {tr}(A_{1})\tau _{1}}e^{\text {tr}(A_{2})\tau _{2}}. \end{equation*}
Lemma 2:
The equation \begin{align} [\text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})]^{2}-4e^{ \text {tr}(A_{1})\tau _{1}}e^{\text {tr}(A_{2})\tau _{2}}<&0,\notag \\ e^{ \text {tr}(A_{1})\tau _{1}}e^{\text {tr}(A_{2})\tau _{2}}<&1; \end{align}
\begin{align} [\text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})]^{2}-4e^{ \text {tr}(A_{1})\tau _{1}}e^{ \text {tr}(A_{2})\tau _{2}}\geq&0,\notag \\ m(1)>0,~m(-1)>&0,\notag \\ -1<\frac {1}{2} \text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})<&1. \end{align}
Remark 1:
The inequalities in (5) correspond to that \begin{align*} |\text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})|\geq&2e^{ \text {tr}(A_{1})\tau _{1}/2}e^{\text {tr}(A_{2})\tau _{2}/2},\\ \left |{\text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})}\right |<&1+e^{ \text {tr}(A_{1})\tau _{1}}e^{\text {tr}(A_{2})\tau _{2}}, \end{align*}
\begin{equation*} \left |{\text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})}\right |<2. \end{equation*}
One can straightforwardly derive the following conclusions.
Corollary 1:
If \begin{equation*} |\text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})|<2e^{ \text {tr}(A_{1})\tau _{1}/2}e^{\text {tr}(A_{2})\tau _{2}/2}; \end{equation*}
\begin{align*} |\text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})|\geq&2e^{ \text {tr}(A_{1})\tau _{1}/2}e^{\text {tr}(A_{2})\tau _{2}/2}, \\ \left |{ \text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})}\right |<&1+e^{ \text {tr}(A_{1})\tau _{1}}e^{\text {tr}(A_{2})\tau _{2}}. \end{align*}
Corollary 2:
There exist dwell-times
Proof:
As \begin{equation*} 2e^{\text {tr}(A_{1})\tau _{1}/2}e^{\text {tr}(A_{2})\tau _{2}/2}\leq | \text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})|<2. \end{equation*}
Remark 2:
From the perspective of assigning the distribution of the eigenvalues of
From the Cayley-Hamilton theorem, one can deduce the following expansions (cf. [8]):\begin{equation*} e^{A_{1}\tau _{1}}=f_{1}(\tau _{1})I+g_{1}(\tau _{1})A_{1}, \end{equation*}
\begin{equation*} e^{A_{2}\tau _{2}}=f_{2}(\tau _{2})I+g_{2}(\tau _{2})A_{2}. \end{equation*}
\begin{align} e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}}=&f_{1}(\tau _{1})f_{2}(\tau _{2})I+f_{2}(\tau _{2})g_{1}(\tau _{1})A_{1}\notag \\&\quad +\,f_{1}(\tau _{1})g_{2}(\tau _{2})A_{2} +g_{1}(\tau _{1})g_{2}(\tau _{2})A_{1}A_{2}, \qquad \end{align}
\begin{align}&\hspace {-2pc}\text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})=2f_{1}(\tau _{1})f_{2}(\tau _{2})+f_{2}(\tau _{2})g_{1}(\tau _{1}) \text {tr}(A_{1})\notag \\&\quad ~+\,f_{1}(\tau _{1})g_{2}(\tau _{2}) \text {tr}(A_{2})+g_{1}(\tau _{1})g_{2}(\tau _{2}) \text {tr}(A_{1}A_{2}). \end{align}
According to the type of the equilibrium point of each subsystem, for the function \begin{align} g_{i}(s)=&\begin{cases} \dfrac {1}{\sqrt {\Delta _{i}}/2}e^{ \text {tr}(A_{i})s/2}\sinh (\sqrt {\Delta _{i}}s/2),& \Delta _{i}>0,\\ \dfrac {1}{\sqrt {-\Delta _{i}}/2}e^{ \text {tr}(A_{i})s/2}\sin (\sqrt {-\Delta _{i}}s/2),& \Delta _{i}<0. \end{cases}\notag \\ {}\end{align}
\begin{align} f_{i}(s)=&\dot {g}_{i}(s)- \text {tr}(A_{i})g_{i}(s)=e^{ \text {tr}(A_{i})s/2}\notag \\&\times \begin{cases} \left [{-\dfrac { \text {tr}(A_{i})}{\sqrt {\Delta _{i}}}\sinh (\sqrt {\Delta _{i}}s/2)+\cosh (\sqrt {\Delta _{i}}s/2)}\right ],\\ \qquad \quad \Delta _{i}>0,\\ \left [{-\dfrac { \text {tr}(A_{i})}{\sqrt {-\Delta _{i}}}\sin (\sqrt {-\Delta _{i}}s/2)+\cos (\sqrt {-\Delta _{i}}s/2)}\right ],\\ \qquad \quad \Delta _{i}<0. \end{cases} \!\!\!\notag \\ {}\end{align}
\begin{equation} \lambda ^{i}_{1,2}=\begin{cases} (\text {tr}(A_{i})\pm \sqrt {\Delta _{i}})/2,& \Delta _{i}>0,\\ (\text {tr}(A_{i})\pm \text {j}\sqrt {-\Delta _{i}})/2,& \Delta _{i}<0. \end{cases} \end{equation}
\begin{equation*} g_{i}(s)=(e^{\lambda ^{i}_{1}s}-e^{\lambda ^{i}_{2}s})/\sqrt {\Delta _{i}}, \end{equation*}
\begin{equation*} f_{i}(s)=\frac {1}{2}\left [{-\frac { \text {tr}(A_{i})}{\sqrt {\Delta _{i}}} (e^{\lambda ^{i}_{1}s}-e^{\lambda ^{i}_{2}s})+(e^{\lambda ^{i}_{1}s}+e^{\lambda ^{i}_{2}s})}\right ]. \end{equation*}
We shall derive the constraint conditions on the dwell-times \begin{equation} \mathcal {K}:=2\frac { \text {tr}(A_{1}A_{2})-\frac {1}{2}\text {tr}(A_{1}) \text {tr}(A_{2})}{\sqrt {|\Delta _{1}\Delta _{2}|}}. \end{equation}
Lemma 3[4]:
\begin{equation*} \det ([A_{1},A_{2}])=\begin{cases} \dfrac {1}{4}\left ({1-\mathcal {K}^{2}}\right)\Delta _{1}\Delta _{2}, &\Delta _{1}\Delta _{2}>0\\ \dfrac {1}{4}\left ({1+\mathcal {K}^{2}}\right)\Delta _{1}\Delta _{2}, & \Delta _{1}\Delta _{2}<0. \end{cases} \end{equation*}
In what follows, we shall show that
CASE I:
\begin{align} \text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})=&2e^{\text {tr}(A_{1})\tau _{1}/2}e^{ \text {tr}(A_{2})\tau _{2}/2}\notag \\&\times \big [\mathcal {K}\sinh (\sqrt {\Delta _{1}}\tau _{1}/2)\sinh (\sqrt {\Delta _{2}}\tau _{2}/2)\notag \\&+\,\cosh (\sqrt {\Delta _{1}}\tau _{1}/2)\cosh (\sqrt {\Delta _{2}}\tau _{2}/2)\big ]. \notag \\ {}\end{align}
Proposition 1:
If both \begin{align}&\hspace {-15pc}\big |\mathcal {K}\sinh (\sqrt {\Delta _{1}}\tau _{1}/2)\sinh (\sqrt {\Delta _{2}}\tau _{2}/2)\notag \\ +\cosh (\sqrt {\Delta _{1}}\tau _{1}/2)\cosh (\sqrt {\Delta _{2}}\tau _{2}/2)\big |<&1, \\ e^{\text {tr}(A_{1})\tau _{1}}e^{\text {tr}(A_{2})\tau _{2}}<&1 \end{align}
\begin{align}&\hspace {-2pc}\big |\mathcal {K}\sinh (\sqrt {\Delta _{1}}\tau _{1}/2)\sinh (\sqrt {\Delta _{2}}\tau _{2}/2)\notag \\&+\,\cosh (\sqrt {\Delta _{1}}\tau _{1}/2)\cosh (\sqrt {\Delta _{2}}\tau _{2}/2)\big |\geq 1, \\&\hspace {-2pc}\big |\mathcal {K}\sinh (\sqrt {\Delta _{1}}\tau _{1}/2)\sinh (\sqrt {\Delta _{2}}\tau _{2}/2)\notag \\&+\cosh (\sqrt {\Delta _{1}}\tau _{1}/2)\cosh (\sqrt {\Delta _{2}}\tau _{2}/2)\big |\notag \\<&\cosh (\text {tr}(A_{1})\tau _{1}/2+ \text {tr}(A_{2})\tau _{2}/2), \\&\hspace {-2pc}\big |\mathcal {K}\sinh (\sqrt {\Delta _{1}}\tau _{1}/2)\sinh (\sqrt {\Delta _{2}}\tau _{2}/2)\notag \\&+\,\cosh (\sqrt {\Delta _{1}}\tau _{1}/2)\cosh (\sqrt {\Delta _{2}}\tau _{2}/2)\big |\notag \\<&e^{-\text {tr}(A_{1})\tau _{1}/2}e^{- \text {tr}(A_{2})\tau _{2}/2}. \end{align}
CASE II:
\begin{align} \text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})=&2e^{\text {tr}(A_{1})\tau _{1}/2}e^{ \text {tr}(A_{2})\tau _{2}/2}\notag \\&\times \,\big [\mathcal {K}\sin (\sqrt {-\Delta _{1}}\tau _{1}/2)\sin (\sqrt {-\Delta _{2}}\tau _{2}/2)\notag \\&+\,\cos (\sqrt {-\Delta _{1}}\tau _{1}/2)\cos (\sqrt {-\Delta _{2}}\tau _{2}/2)\big ]. \notag \\ {}\end{align}
Proposition 2:
If both \begin{align}&\hspace {-15pc}\big |\mathcal {K}\sin (\sqrt {-\Delta _{1}}\tau _{1}/2)\sin (\sqrt {-\Delta _{2}}\tau _{2}/2)\notag \\ +\cos (\sqrt {-\Delta _{1}}\tau _{1}/2)\cos (\sqrt {-\Delta _{2}}\tau _{2}/2)\big |<&1, \\ e^{\text {tr}(A_{1})\tau _{1}}e^{\text {tr}(A_{2})\tau _{2}}<&1 \end{align}
\begin{align}&\hspace {-2pc}\big |\mathcal {K}\sin (\sqrt {-\Delta _{1}}\tau _{1}/2)\sin (\sqrt {-\Delta _{2}}\tau _{2}/2)\notag \\&+\cos (\sqrt {-\Delta _{1}}\tau _{1}/2)\cos (\sqrt {-\Delta _{2}}\tau _{2}/2)\big |\geq 1, \\&\hspace {-2pc}\big |\mathcal {K}\sin (\sqrt {-\Delta _{1}}\tau _{1}/2)\sin (\sqrt {-\Delta _{2}}\tau _{2}/2)\notag \\&+\cos (\sqrt {-\Delta _{1}}\tau _{1}/2)\cos (\sqrt {-\Delta _{2}}\tau _{2}/2)\big |\notag \\<&\cosh (\text {tr}(A_{1})\tau _{1}/2+ \text {tr}(A_{2})\tau _{2}/2), \\&\hspace {-2pc}\big |\mathcal {K}\sin (\sqrt {-\Delta _{1}}\tau _{1}/2)\sin (\sqrt {-\Delta _{2}}\tau _{2}/2)\notag \\&+\cos (\sqrt {-\Delta _{1}}\tau _{1}/2)\cos (\sqrt {-\Delta _{2}}\tau _{2}/2)\big |\notag \\<&e^{-\text {tr}(A_{1})\tau _{1}/2}e^{-\text {tr}(A_{2})\tau _{2}/2}. \end{align}
CASE III:
\begin{align} \text {tr}(e^{A_{1}\tau _{1}}e^{A_{2}\tau _{2}})=&2e^{\text {tr}(A_{1})\tau _{1}/2}e^{\text {tr}(A_{2})\tau _{2}/2}\notag \\&\times \big [\mathcal {K}\sinh (\sqrt {\Delta _{1}}\tau _{1}/2)\sin (\sqrt {-\Delta _{2}}\tau _{2}/2)\notag \\&+\,\cosh (\sqrt {\Delta _{1}}\tau _{1}/2)\cos (\sqrt {-\Delta _{2}}\tau _{2}/2)\big ]. \notag \\ {}\end{align}
Proposition 3:
If \begin{align}&\hspace {-15pc}\big |\mathcal {K}\sinh (\sqrt {\Delta _{1}}\tau _{1}/2)\sin (\sqrt {-\Delta _{2}}\tau _{2}/2)\notag \\ +\cosh (\sqrt {\Delta _{1}}\tau _{1}/2)\cos (\sqrt {-\Delta _{2}}\tau _{2}/2)\big |<&1, \\ e^{\text {tr}(A_{1})\tau _{1}}e^{\text {tr}(A_{2})\tau _{2}}<&1 \end{align}
\begin{align}&\hspace {-2pc}\big |\mathcal {K}\sinh (\sqrt {\Delta _{1}}\tau _{1}/2)\sin (\sqrt {-\Delta _{2}}\tau _{2}/2)\notag \\&+\,\cosh (\sqrt {\Delta _{1}}\tau _{1}/2)\cos (\sqrt {-\Delta _{2}}\tau _{2}/2)\big |\geq 1, \\&\hspace {-2pc}\big |\mathcal {K}\sinh (\sqrt {\Delta _{1}}\tau _{1}/2)\sin (\sqrt {-\Delta _{2}}\tau _{2}/2)\notag \\&+\,\cosh (\sqrt {\Delta _{1}}\tau _{1}/2)\cos (\sqrt {-\Delta _{2}}\tau _{2}/2)\big |\notag \\<&\cosh (\text {tr}(A_{1})\tau _{1}/2+\text {tr}(A_{2})\tau _{2}/2), \\&\hspace {-2pc}\big |\mathcal {K}\sinh (\sqrt {\Delta _{1}}\tau _{1}/2)\sin (\sqrt {-\Delta _{2}}\tau _{2}/2)\notag \\&+\,\cosh (\sqrt {\Delta _{1}}\tau _{1}/2)\cos (\sqrt {-\Delta _{2}}\tau _{2}/2)\big |\notag \\<&e^{-\text {tr}(A_{1})\tau _{1}/2}e^{-\text {tr}(A_{2})\tau _{2}/2}. \end{align}
When both subsystems are stable, the inequalities in Propositions 1–3 can be reduced according to Corollary 1. Moreover, to complete this section, we emphasize that instead of solving these inequalities directly, an intuitive way to present the mutual constraint relation between
An Illustrative Example
We now provide an example to typically illustrate Proposition 3.
Example 1:
We have \begin{align*}&\hspace {-15pc}\big |0.9756\sinh (1.4361\tau _{1})\sin (1.5612\tau _{2}) \\ +\cosh (1.4361\tau _{1})\cos (1.5612\tau _{2})\big |<&1,\\ e^{-1.5\tau _{1}}e^{0.5\tau _{2}}<&1 \end{align*}
\begin{align*}&\hspace {-2pc}\big |0.9756\sinh (1.4361\tau _{1})\sin (1.5612\tau _{2}) \\&+\,\cosh (1.4361\tau _{1})\cos (1.5612\tau _{2})\big |\geq 1,\\&\hspace {-2pc}\big |0.9756\sinh (1.4361\tau _{1})\sin (1.5612\tau _{2}) \\&+\,\cosh (1.4361\tau _{1})\cos (1.5612\tau _{2})\big | \\<&\cosh (-0.75\tau _{1}+0.25\tau _{2}),\\&\hspace {-2pc}\big |0.9756\sinh (1.4361\tau _{1})\sin (1.5612\tau _{2}) \\&+\,\cosh (1.4361\tau _{1})\cos (1.5612\tau _{2})\big | \\<&e^{0.75\tau _{1}}e^{-0.25\tau _{2}}. \end{align*}
\begin{align}&\hspace {-2pc}\big |0.9756\sinh (1.4361\tau _{1})\sin (1.5612\tau _{2})\qquad \qquad ~\notag \\&+\,\cosh (1.4361\tau _{1})\cos (1.5612\tau _{2})\big |=1, \\&-\,1.5\tau _{1}+0.5\tau _{2}=0, \\&\hspace {-2pc}\big |0.9756\sinh (1.4361\tau _{1})\sin (1.5612\tau _{2})\qquad \qquad ~\notag \\&+\,\cosh (1.4361\tau _{1})\cos (1.5612\tau _{2})\big |\qquad ~\notag \\=&\cosh (-0.75\tau _{1}+0.25\tau _{2}), \\&\hspace {-2pc}\big |0.9756\sinh (1.4361\tau _{1})\sin (1.5612\tau _{2})\qquad \qquad ~\notag \\&+\,\cosh (1.4361\tau _{1})\cos (1.5612\tau _{2})\big |\qquad ~\notag \\=&e^{0.75\tau _{1}}e^{-0.25\tau _{2}}. \end{align}
In Figure 1, the equations in (31) and (32) are depicted and colored in black and red, respectively. They form the boundaries of the regions, which correspond to the complex eigenvalues of
The stability margin corresponding to the complex eigenvalues of
In Figure 3, the equations in (31), (33), and (34) are depicted and colored in black, red, and blue, respectively. These curves form the boundaries of the regions, which correspond to the eigenvalues of
The stability margin corresponding to the real eigenvalues of
As shown in Figures 2 and 4, this example exposes a little surprising phenomenon that two unstable subsystems with quite long periods to stay active can generate a stable state-trajectory.
Conclusion
We considered the stability analysis problem for the planar linear systems undergoing periodic switching. We characterized the stability margin that the dwell-times of subsystems are confined to so that the overall system is asymptotically stable. The main technical preliminary includes a key lemma along with the distribution property of the roots of parabolic functions. Indeed, the expansion of the transition matrix of each subsystem up to the first order of its generator (i.e., the subsystem matrix) enables us to express the stability margin analytically and, moreover, compute it numerically. Finally, an example was worked in detail to illustrate the theoretical results.