Appendix 1: Proof of Lemma 1
Solving Eq. 17, one can find that ψ
i
=P
i
B
ql
can be expressed in the form as stated in the lemma, and under the condition that \( \frac{1} {{p_{i} }} > > f \geqslant 1 \),
γ
ji
can be represented as:
$$ \gamma _{{ji}} = \frac{{a_{{2i}} f^{2}_{i} + a_{{1i}} f_{i} + a_{{0i}} }} {{f^{2}_{i} + (\alpha _{{1i}} + \beta _{{1i}} )f_{i} + (\alpha _{{1i}} \beta _{{1i}} + \beta _{{2i}} ) + (\alpha _{{1i}} \beta _{{2i}} )f^{{ - 1}}_{i} }},\quad j = 1,2,3 $$
$$ \gamma _{{ji}} = \frac{{b_{{3i}} f^{3}_{i} + b_{{2i}} f^{2}_{i} + b_{{1i}} f_{i} + b_{{0i}} }} {{f^{3}_{i} + (\alpha _{{1i}} + \beta _{{1i}} )f^{2}_{i} + (\alpha _{{1i}} \beta _{{1i}} + \beta _{{2i}} )f_{i} + \alpha _{{1i}} \beta _{{2i}} }},\quad j = 4,5 $$
where
a
ji
(j=0,1,2) and
b
ki
(k=0,1,2,3) are constants independent of f
i
. Since
α
1i
,β
1i
,β
2i
>0, obviously, the denominator of γ
ji
is larger than zero, so γ
ji
is continuous in f
i
and can be bounded by constants that are independent of f
i
. □
Appendix 2: Proof of Lemma 2
From (5), we have
$$ \begin{aligned} {\left\| \Delta \right\|} \leqslant {\left\| {M(\theta ) - M(\theta _{{\text{d}}} )} \right\|}{\left\| {\ddot{\theta }_{{\text{d}}} } \right\|} + {\left\| {M(\theta _{{\text{d}}} )\ddot{\theta }_{{\text{d}}} - M_{0} (\theta _{{\text{d}}} )\ddot{\theta }_{{\text{d}}} } \right\|} & \\ + {\left\| {C(\theta ,\dot{\theta }) - C(\theta _{{\text{d}}} ,\dot{\theta }_{{\text{d}}} )} \right\|}{\left\| {\dot{\theta }_{{\text{d}}} } \right\|} + {\left\| {C(\theta _{{\text{d}}} ,\dot{\theta }_{{\text{d}}} )\dot{\theta }_{{\text{d}}} - C_{0} (\theta _{{\text{d}}} ,\dot{\theta }_{{\text{d}}} )\dot{\theta }_{{\text{d}}} } \right\|} & \\ + {\left\| {g(\theta ) - g(\theta _{{\text{d}}} )} \right\|} + {\left\| {g(\theta _{{\text{d}}} ) - g_{0} (\theta _{{\text{d}}} )} \right\|} & \\ \end{aligned} $$
Suppose the desired trajectory is bounded and satisfies
$$ {\left\| {\theta _{d} } \right\|} \leqslant c_{1} ,{\left\| {\ifmmode\expandafter\dot\else\expandafter\.\fi{\theta }_{d} } \right\|} \leqslant c_{2} ,{\left\| {\ifmmode\expandafter\ddot\else\expandafter\"\fi{\theta }_{d} } \right\|} \leqslant c_{3} $$
where
c
1,
c
2, and
c
3 are constants. In view of Properties 1–3 in Sect. 2, there exist positive constants
k
M,
k
M1,
k
c,
k
c1,
k
c2 satisfying
$$ {\left\| \Delta \right\|} \leqslant k_{{\text{M}}} c_{3} + k_{{{\text{M}}1}} c_{3} {\left\| e \right\|} + k_{{\text{C}}} c_{2} + k_{{{\text{C}}1}} c_{2} {\left\| {\dot{e}} \right\|} + k_{{{\text{C}}2}} c^{2}_{2} {\left\| e \right\|} + k_{{\text{g}}} + k_{{{\text{g}}1}} {\left\| e \right\|} $$
From Property 1 and Property 3(3), there exist positive constants
k
c3,
k
M2 such that
$$ {\left\| { - M^{{ - 1}} C\dot{e} + (M^{{ - 1}} - b_{0} )u_{0} } \right\|} \leqslant k_{{{\text{C}}3}} {\left\| {\dot{e}} \right\|}^{2} + k_{{{\text{M}}2}} {\left\| {u_{0} } \right\|} $$
So we have
$$ {\left\| {\tilde{q}} \right\|} \leqslant k_{{{\text{q}}1}} + k_{{{\text{q}}2}} {\left\| e \right\|} + k_{{{\text{q}}3}} {\left\| {\dot{e}} \right\|} + k_{{{\text{q}}4}} {\left\| {\dot{e}} \right\|}^{2} + k_{{{\text{q}}5}} {\left\| {u_{0} } \right\|}^{2} $$
where
k
q1,
k
q2, ...,
k
q5 are bounded positive constants. □
Appendix 3: Proof of Lemma 3
Because
b
0≥λ
min(M
−1), which implies that \( \bar{\delta }(b^{{ - 1}}_{0} M^{{ - 1}} ) \leqslant I \), we have
$$ \bar{\delta }[b^{{ - 1}}_{0} M^{{ - 1}} - I] \leqslant 1 - b^{{ - 1}}_{0} \lambda _{{\min }} (M^{{ - 1}} ) $$
From Assumption (C), it follows that
$$ \ifmmode\expandafter\bar\else\expandafter\=\fi{\delta }[b^{{ - 1}}_{0} M^{{ - 1}} - I] \leqslant 1 - \varepsilon _{\Delta } $$
Therefore the conclusion holds. □
Appendix 4: Proof of Lemma 4
From (20), if \( f_{i} \geqslant {\mathop {\max }\limits_{j = 1}^3 }(\gamma _{{j\max }} )^{2} \), then
$$ {\text{ }}\frac{{k_{{{\text{q}}1}} }} {{b_{0} {\sqrt {f_{i} } }}}{\sum\limits_{i = 1}^3 {\gamma _{{i\max }} } } \leqslant \frac{{3k_{{{\text{q}}1}} }} {{b_{0} }} $$
(21)
Meanwhile, if
$$ \mu \geqslant \gamma _{{4\max }} + \gamma _{{5\max }} $$
which is satisfied under Assumption (A), then we have
$$ \frac{{k_{{{\text{q}}1}} }} {{b_{0} }}[1 + {(\gamma _{{4\max }} + \gamma _{{5\max }} )} \mathord{\left/ {\vphantom {{(\gamma _{{4\max }} + \gamma _{{5\max }} )} \mu }} \right. \kern-\nulldelimiterspace} \mu ] \leqslant \frac{{2k_{{{\text{q}}1}} }} {{b_{0} }} $$
(22)
Combining (21) and (22) results in
$$ \mu _{0} \leqslant \frac{{5k_{{{\text{q}}1}} }} {{b_{0} }} $$
□
Appendix 5: Proof of Theorem 1
Consider the following Lyapunov function candidate
$$ V = X^{T} PX = {\sum\limits_{i = 1}^n {V_{i} } },\quad V_{i} = X^{T}_{i} P_{i} X_{i} $$
where
$$ X = {\left[ {X^{T}_{1} ,X^{T}_{2} , \cdots ,X^{T}_{n} } \right]}^{T} ,\quad \;P = {\left[ {\begin{array}{*{20}c} {{P_{1} }} & {{}} & {{}} \\ {{}} & { \ddots } & {{}} \\ {{}} & {{}} & {{P_{n} }} \\ \end{array} } \right]} $$
(23)
The derivative of V, along the solution of the controlled system (16), is given by
$$ \begin{array}{*{20}l} {{\dot{V}} \hfill} & { = \hfill} & {{{\sum\limits_{i = 1}^n {\dot{V}_{i} } } = {\sum\limits_{i = 1}^n {( - X^{T}_{i} X_{i} + 2X^{T}_{i} P_{i} B_{{{\text{q}}i}} q_{i} )} }} \hfill} \\ {{} \hfill} & { \leqslant \hfill} & {{ - (e^{T} e + \dot{e}^{T} \dot{e} + u^{T}_{0} u_{0} + v^{T}_{0} v_{0} + \tilde{v}^{T} \tilde{v}) + 2\left\{ {{\sum\limits_{i = 1}^n {\frac{1} {{f_{i} b_{0} }}} }\gamma _{{1i}} e_{i} q_{i} } \right.} \hfill} \\ {{} \hfill} & {{} \hfill} & {\begin{aligned} & + {\sum\limits_{i = 1}^n {\frac{1} {{f_{i} b_{0} }}} }\gamma _{{2i}} \dot{e}_{i} q_{i} + {\sum\limits_{i = 1}^n {\frac{1} {{f_{i} b_{0} }}} }\gamma _{{3i}} u_{{0i}} q_{i} \\ & + {\sum\limits_{i = 1}^n {\frac{1} {{{\sqrt {f_{i} } }b_{0} }}(1 + \frac{{\gamma _{{4i}} }} {\mu })v_{{0i}} q_{i} + \left. {{\sum\limits_{i = 1}^n {\frac{{\gamma _{{5i}} }} {{{\sqrt {f_{i} } }b_{0} \mu }}\tilde{v}_{i} q_{i} } }} \right\}} } \\ \end{aligned} \hfill} \\ {{} \hfill} & { = \hfill} & {{ - (e^{T} e + \dot{e}^{T} \dot{e} + u^{T}_{0} u_{0} + v^{T}_{0} v_{0} + \tilde{v}^{T} \tilde{v})} \hfill} \\ {{} \hfill} & {{} \hfill} & {{ + 2\left[ {e^{T} {\text{diag}}{\left\{ {\frac{{\gamma _{{1i}} }} {{f_{i} b_{0} }}} \right\}} + \dot{e}^{T} {\text{diag}}{\left\{ {\frac{{\gamma _{{2i}} }} {{f_{i} b_{0} }}} \right\}} + u^{T}_{0} {\text{diag}}{\left\{ {\frac{{\gamma _{{3i}} }} {{f_{i} b_{0} }}} \right\}}} \right.} \hfill} \\ {{} \hfill} & {{} \hfill} & {{ + v^{T}_{0} {\text{diag}}{\left\{ {\frac{1} {{{\sqrt {f_{i} } }b_{0} }}(1 + \frac{{\gamma _{{4i}} }} {\mu })} \right\}} + \left. {\tilde{v}^{T} {\text{diag}}{\left\{ {\frac{{\gamma _{{5i}} }} {{{\sqrt {f_{i} } }b_{0} \mu }}} \right\}}} \right]q} \hfill} \\ \end{array} $$
(24)
From Lemma 2 and the definition of
γ
jmax
in Lemma 4, (24) becomes
$$ \begin{array}{*{20}l} {{\dot{V}} \hfill} & { \leqslant \hfill} & {{ - ({\left\| e \right\|}^{2} + {\left\| {\dot{e}} \right\|}^{2} + {\left\| {u_{0} } \right\|}^{2} + {\left\| {v_{0} } \right\|}^{2} + {\left\| {\tilde{v}} \right\|}^{2} )} \hfill} \\ {{} \hfill} & {{} \hfill} & {{ + 2\left\{ {\left[ {\frac{1} {{f_{i} b_{0} }}} \right.} \right.(\gamma _{{1\max }} {\left\| e \right\|} + \gamma _{{2\max }} {\left\| {\dot{e}} \right\|} + \gamma _{{3\max }} {\left\| {u_{0} } \right\|})} \hfill} \\ {{} \hfill} & {{} \hfill} & {{\left. { + \frac{1} {{{\sqrt {f_{i} } }b_{0} }}(1 + \frac{{\gamma _{{4\max }} }} {\mu }){\left\| {v_{0} } \right\|} + \frac{{\gamma _{{5\max }} }} {{b_{0} \mu }}{\left\| {\tilde{v}} \right\|}} \right] \cdot {\left\| {\tilde{q}} \right\|}} \hfill} \\ {{} \hfill} & {{} \hfill} & {\begin{aligned} & + \left[ {\frac{1} {{{\sqrt {f_{i} } }}}} \right.(\gamma _{{1\max }} {\left\| e \right\|} + \gamma _{{2\max }} {\left\| {\dot{e}} \right\|} + \gamma _{{3\max }} {\left\| {u_{0} } \right\|}) \\ & + \left. {(1 + \frac{{\gamma _{{4\max }} }} {\mu }){\left\| {v_{0} } \right\|} + \left. {\frac{{\gamma _{{5\max }} }} {\mu }{\left\| {\tilde{v}} \right\|}} \right] \cdot {\left\| {b^{{ - 1}}_{0} (M^{{ - 1}} - b_{0} I)} \right\|} \cdot {\left\| {\tilde{v}} \right\|}} \right\} \\ \end{aligned} \hfill} \\ \end{array} $$
(25)
In the view of Lemma 1 and Lemma 3, (25) becomes
$$ \begin{array}{*{20}l} {{\ifmmode\expandafter\dot\else\expandafter\.\fi{V}} \hfill} & { \leqslant \hfill} & {{ - ({\left\| e \right\|}^{2} + {\left\| {\ifmmode\expandafter\dot\else\expandafter\.\fi{e}} \right\|}^{2} + {\left\| {u_{0} } \right\|}^{2} + {\left\| {v_{0} } \right\|}^{2} + {\left\| { \ifmmode\expandafter\tilde\else\expandafter\~\fi{v}} \right\|}^{2} )} \hfill} \\ {{} \hfill} & {{} \hfill} & {{ + 2\left\{ {[\frac{1} {{f_{i} b_{0} }}(\gamma _{{1\max }} {\left\| e \right\|} + \gamma _{{2\max }} {\left\| {\ifmmode\expandafter\dot\else\expandafter\.\fi{e}} \right\|} + \gamma _{{3\max }} {\left\| {u_{0} } \right\|})} \right.} \hfill} \\ {{} \hfill} & {{} \hfill} & {{ + \frac{1} {{{\sqrt {f_{i} } }b_{0} }}(1 + \frac{{\gamma _{{4\max }} }} {\mu }){\left\| {v_{0} } \right\|} + \frac{{\gamma _{{5\max }} }} {{b_{0} \mu }}{\left\| { \ifmmode\expandafter\tilde\else\expandafter\~\fi{v}} \right\|}]} \hfill} \\ {{} \hfill} & {{} \hfill} & {{ \cdot [k_{{{\text{q}}1}} + k_{{{\text{q}}2}} {\left\| e \right\|} + k_{{{\text{q}}3}} {\left\| {\ifmmode\expandafter\dot\else\expandafter\.\fi{e}} \right\|} + k_{{{\text{q}}4}} {\left\| {\ifmmode\expandafter\dot\else\expandafter\.\fi{e}} \right\|}^{2} + k_{{{\text{q}}5}} {\left\| {u_{0} } \right\|}]} \hfill} \\ {{} \hfill} & {{} \hfill} & {\begin{aligned} & + \frac{1} {{{\sqrt {f_{i} } }}}(\gamma _{{1\max }} {\left\| e \right\|} + \gamma _{{2\max }} {\left\| {\ifmmode\expandafter\dot\else\expandafter\.\fi{e}} \right\|} + \gamma _{{3\max }} {\left\| {u_{0} } \right\|}){\left\| { \ifmmode\expandafter\tilde\else\expandafter\~\fi{v}} \right\|} \\ & + \left. {\ifmmode\expandafter\bar\else\expandafter\=\fi{\delta }(b^{{ - 1}}_{0} (M^{{ - 1}} - b_{0} I))[(1 + \frac{{\gamma _{{4\max }} }} {\mu }){\left\| {v_{0} } \right\|} + \frac{{\gamma _{{5\max }} }} {\mu }{\left\| { \ifmmode\expandafter\tilde\else\expandafter\~\fi{v}} \right\|}] \cdot {\left\| { \ifmmode\expandafter\tilde\else\expandafter\~\fi{v}} \right\|}} \right\} \\ \end{aligned} \hfill} \\ \end{array} $$
(26)
Define
k
sum=k
q1+k
q2+k
q3+k
q5 and
k=[k
q2,
k
q3,
k
q5]T and let
k
i
denote the ith element of the vector k. Then (26) is further expressed as
$$ \dot{V} \leqslant - \mu _{1} {\left\| e \right\|}^{2} - \mu _{2} {\left\| {\dot{e}} \right\|}^{2} - \mu _{3} {\left\| {u_{0} } \right\|}^{2} - \mu _{4} {\left\| {v_{0} } \right\|}^{2} - \mu _{5} {\left\| {\tilde{v}} \right\|}^{2} + \frac{{\mu _{0} }} {{{\sqrt {f_{i} } }}} $$
(27)
where
μ
0 is defined as (20),
$$ \mu _{i} = \left\{ {\begin{array}{*{20}l} {{1 - {\rho _{i} } \mathord{\left/ {\vphantom {{\rho _{i} } {{\sqrt {f_{i} } }}}} \right. \kern-\nulldelimiterspace} {{\sqrt {f_{i} } }}} \hfill} & {{(i = 1,3)} \hfill} \\ {{1 - ( \ifmmode\expandafter\tilde\else\expandafter\~\fi{\rho }_{i} + {\rho _{i} )} \mathord{\left/ {\vphantom {{\rho _{i} )} {{\sqrt {f_{i} } }}}} \right. \kern-\nulldelimiterspace} {{\sqrt {f_{i} } }}} \hfill} & {{(i = 2)} \hfill} \\ {{1 - \ifmmode\expandafter\bar\else\expandafter\=\fi{\delta }(b^{{ - 1}}_{0} (M^{{ - 1}} - b_{0} I))(1 + {\gamma _{{4\max }} } \mathord{\left/ {\vphantom {{\gamma _{{4\max }} } \mu }} \right. \kern-\nulldelimiterspace} \mu ) - {\rho _{i} } \mathord{\left/ {\vphantom {{\rho _{i} } {{\sqrt {f_{i} } }}}} \right. \kern-\nulldelimiterspace} {{\sqrt {f_{i} } }}} \hfill} & {{(i = 4)} \hfill} \\ {{1 - \ifmmode\expandafter\bar\else\expandafter\=\fi{\delta }(b^{{ - 1}}_{0} (M^{{ - 1}} - b_{0} I))[1 + {(\gamma _{{4\max }} + 2\gamma _{{5\max }} )} \mathord{\left/ {\vphantom {{(\gamma _{{4\max }} + 2\gamma _{{5\max }} )} \mu }} \right. \kern-\nulldelimiterspace} \mu ] - {\rho _{i} } \mathord{\left/ {\vphantom {{\rho _{i} } {{\sqrt {f_{i} } }}}} \right. \kern-\nulldelimiterspace} {{\sqrt {f_{i} } }}} \hfill} & {{(i = 5)} \hfill} \\ \end{array} } \right. $$
(28)
$$ \rho _{i} = \left\{ {\begin{array}{*{20}c} {\frac{1} {{{\sqrt {f_{i} } }b_{0} }}[\gamma _{{i\max }} k_{{{\text{sum}}}} + k_{i} {\sum\limits_{j = 1}^3 {\gamma _{{j\max }} } }] + \frac{{k_{i} }} {{b_{0} }}[1 + \frac{{\gamma _{{4\max }} + \gamma _{{5\max }} }} {\mu }] + \gamma _{{i\max }} }{(i = 1,2,3)} \\ {\frac{1} {{b_{0} }}[1 + \frac{{\gamma _{{4\max }} }} {\mu }]k_{{{\text{sum}}}} }{(i = 4)} \\ {{\sum\limits_{j = 1}^3 {\gamma _{{j\max }} } } + \frac{{\gamma _{{5\max }} k_{{{\text{sum}}}} }} {{b_{0} \mu }}}{(i = 5)} \\ \end{array} } \right. $$
(29)
$$ \begin{aligned} \tilde{\rho }_{2} = \frac{2} {{\lambda _{b} }}[\frac{{\gamma _{{1\max }} }} {{{\sqrt {f_{i} } }}}{\left\| e \right\|} + \frac{{\gamma _{{2\max }} }} {{{\sqrt {f_{i} } }}}{\left\| {\dot{e}} \right\|} + \frac{{\gamma _{{3\max }} }} {{{\sqrt {f_{i} } }}}{\left\| {u_{0} } \right\|} + (1 + \frac{{\gamma _{{4\max }} }} {\mu }){\left\| {v_{0} } \right\|} & \\ \quad \;\; + \frac{{\gamma _{{5\max }} }} {\mu }{\left\| {\tilde{v}} \right\|}]k_{{{\text{q}}4}} & \\ \end{aligned} $$
(30)
Define \( Y = {\left[ {e^{T} ,\dot{e}^{T} ,u^{T}_{0} ,v^{T}_{0} ,\tilde{v}^{T} } \right]}^{T} = {\left[ {Y^{T}_{1} ,Y^{T}_{2} ,Y^{T}_{3} ,Y^{T}_{4} ,Y^{T}_{5} } \right]}^{T} \), then under Assumption (A), we have
$$ \ifmmode\expandafter\tilde\else\expandafter\~\fi{\rho }_{2} \leqslant \phi _{1} {\sum\limits_{j = 1}^5 {{\left\| {Y_{i} } \right\|}} } \leqslant {\sqrt 5 }\phi _{1} {\left\| Y \right\|} $$
(31)
where \( \phi _{1} = 2k_{{{\text{q}}4}} b^{{ - 1}}_{0} {\mathop {\max }\limits_{} }\,\{ \gamma _{{1\max }} ,\gamma _{{2\max }} ,\gamma _{{3\max }} ,2\} \), is a bounded constant independent of f
i
.
In the following, the conditions are analyzed that ensure μ
i
>0,
i=1,2,...,5.
Let π
min be a positive constant so that
π
min<min{ε
Δ,1}, and let p̄
i
denote the values of p
i
when
f
i
=1 and μ=γ
4max+2γ
5max. Then under Assumption (A) and the condition that μ≥γ
4max+2γ
5max, we have p
i
≤p̄
i
.
If the following equalities hold
$$ f_{i} \geqslant f_{{{\text{c}}2}} ,{\text{ }}\mu \geqslant \gamma _{{4\max }} + 2\gamma _{{5\max }} $$
(32)
$$ {\left\| Y \right\|} \leqslant {\text{ }}\frac{1} {{{\sqrt {\text{5}} }\phi _{1} }}[(1 - \pi _{{\min }} ){\sqrt {f_{i} } } - \ifmmode\expandafter\bar\else\expandafter\=\fi{\rho }_{2} ] $$
(33)
where
$$ f_{{{\text{c}}2}} = \max {\left\{ {{\mathop {\max }\limits_{i = 1,3} }{\left( {\frac{{\bar{\rho }_{i} }} {{1 - \pi _{{\min }} }}} \right)}^{2} ,\;{\mathop {\max }\limits_{i = 4,5} }{\left( {\frac{{\bar{\rho }_{i} }} {{\varepsilon _{\Delta } - \pi _{{\min }} }}} \right)}^{2} } \right\}} $$
(34)
then by (28) and from Lemma 3, we have
$$ \mu _{i} \geqslant \pi _{{\min }} ,{\text{ }}i = 1,2, \ldots ,5 $$
(35)
Note that (33) defines the attractive region.
If (35) holds and f
i
≥f
c1 from Lemma 4, one sees that (27) can be rewritten as
$$ \dot{V} \leqslant - \pi _{{\min }} {\left\| Y \right\|}^{2} + \frac{{5k_{{{\text{q}}1}} }} {{{\sqrt {f_{i} } }b_{0} }} $$
(36)
Since
$$ {\left\| Y \right\|}^{2} = {\left\| X \right\|}^{2} \geqslant \frac{{X^{T} PX}} {{\lambda _{{\max }} (P)}} = \frac{V} {{\lambda _{{\max }} (P)}} $$
we obtain
$$ \dot{V} \leqslant - \zeta _{{\text{s}}} V + \varepsilon _{{\text{s}}} $$
(37)
and
$$ V(t) \leqslant V(t_{0} ){\text{e}}^{{ - \zeta _{{\text{s}}} (t - t_{0} )}} + \frac{{\varepsilon _{{\text{s}}} }} {{\zeta _{{\text{s}}} }}(1 - {\text{e}}^{{ - \zeta _{{\text{s}}} (t - t_{0} )}} ) $$
(38)
where
$$ \zeta _{{\text{s}}} = \frac{{\pi _{{\min }} }} {{\lambda _{{\max }} (P)}},\quad \varepsilon _{{\text{s}}} = \frac{{5k_{{{\text{q}}1}} }} {{{\sqrt {f_{i} } }b_{0} }} $$
Let
$$ \bar{V} = \max \{ V(t_{0} ),\;5k_{{{\text{q}}1}} b^{{ - 1}}_{0} \zeta ^{{ - 1}}_{{\text{s}}} \} $$
Then under Assumption (A) and from (37) it is known that \( V(t) \leqslant \ifmmode\expandafter\bar\else\expandafter\=\fi{V},\forall t \geqslant t_{0} \) and \( {\mathop {\lim }\limits_{t \to \infty } }V(t) \leqslant \varepsilon _{{\text{s}}} \zeta ^{{ - 1}}_{{\text{s}}} \). Because
$$ {\left\| Y \right\|}^{2} = {\left\| X \right\|}^{2} \leqslant \frac{{X^{T} PX}} {{\lambda _{{\min }} (P)}} = \frac{V} {{\lambda _{{\min }} (P)}} $$
(39)
Y(t) (and X(t) starting from the attractive region given by (33)) can remain inside that region, if
$$ \frac{1} {{{\sqrt {\text{5}} }\phi _{1} }}[(1 - \pi _{{\min }} ){\sqrt {f_{i} } } - \ifmmode\expandafter\bar\else\expandafter\=\fi{\rho }_{2} ] \geqslant {\sqrt {\ifmmode\expandafter\bar\else\expandafter\=\fi{V}\lambda ^{{ - 1}}_{{\min }} (P)} } $$
(40)
By Assumption (A), (40) holds, if
$$ f_{i} \geqslant f_{{{\text{c}}3}} ,\quad f_{{{\text{c}}3}} = \frac{1} {{(1 - \pi _{{\min }} )^{2} }}{\left( {\phi _{1} {\sqrt {5\ifmmode\expandafter\bar\else\expandafter\=\fi{V}\lambda ^{{ - 1}}_{{\min }} (P)} } + \ifmmode\expandafter\bar\else\expandafter\=\fi{\rho }_{2} } \right)}^{2} $$
(41)
In addition, from (37) and (39) we know that the state Y convergences to the set given by
$$ \Omega _{{\text{s}}} = {\left\{ {Y\left| {{\left\| Y \right\|}^{2} \leqslant {\varepsilon _{{\text{s}}} } \mathord{\left/ {\vphantom {{\varepsilon _{{\text{s}}} } {(\zeta _{{\text{s}}} \lambda _{{\min }} (P))}}} \right. \kern-\nulldelimiterspace} {(\zeta _{{\text{s}}} \lambda _{{\min }} (P))}} \right.} \right\}} $$
at a rate not slower than exp(−ξ
s
t/2).
By (39), if
$$ V(t) \leqslant \lambda _{{\min }} (P)\eta $$
then
$$ {\left\| X \right\|}^{2} \leqslant \eta $$
When both of the closed-loop system and the reference model are of zero initial conditions, V(t
0)=0. In this case, from (39), we have \( {\mathop {{\left\| X \right\|}^{2} }\limits_{t \geqslant t_{0} } } < \eta \), if
$$ \frac{{\varepsilon _{{\text{s}}} }} {{\zeta _{{\text{s}}} }} \leqslant \eta \lambda _{{\min }} (P) $$
(42)
In the case of nonzero initial states,
V(t
0)≠0. We can obtain \( {\mathop {{\left\| X \right\|}^{2} }\limits_{t \geqslant T} } < \eta \), if
$$ V(t_{0} ){\text{e}}^{{ - \zeta _{{\text{s}}} (t - t_{0} )}} + \frac{{\varepsilon _{{\text{s}}} }} {{\zeta _{{\text{s}}} }} \leqslant \eta \lambda _{{\min }} (P) $$
(43)
If \( T \geqslant t_{0} + \frac{1} {{\zeta _{{\text{s}}} }}\ln (\frac{{2V(t_{0} )}} {{\eta \lambda _{{\min }} (P)}}) \), we have
$$ V(t_{0} ){\text{e}}^{{ - \zeta _{{\text{s}}} (T - t_{0} )}} \leqslant \frac{1} {2}\eta \lambda _{{\min }} (P) $$
Now to ensure (43) holds, it is required that
$$ \frac{{\varepsilon _{{\text{s}}} }} {{\zeta _{{\text{s}}} }} \leqslant \frac{1} {2}\eta \lambda _{{\min }} (P) $$
(44)
Incorporating (42) and (44) yields
$$ f_{i} \geqslant f_{{{\text{c}}4}} ,\quad f_{{{\text{c}}4}} = {\left( {\frac{{10k_{{{\text{q}}1}} \lambda _{{\max }} (P)}} {{\eta b_{0} \pi _{{\min }} \lambda _{{\min }} (P)}}} \right)}^{2} $$
(45)
From the previous analysis, we see that it is required
$$ f_{i} \geqslant {\mathop {\max }\limits_{j = 1}^4 }f_{{{\text{c}}j}} ,{\text{ }}\mu \geqslant \gamma _{{4\max }} + 2\gamma _{{5\max }} $$
where
f
ci
,
i=1,...,4 are bounded constants and
γ
4max+2γ
5max are bounded by a constant, all independent of
f
i
. When the parameters f
i
and μ
are set such that the above conditions hold, then the robust transient property and robust tracking property can be achieved. So the conclusions of the theorem are proven. □