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Mathematical Social Sciences 61 (2011) 97–103

Contents lists available atScienceDirect

Mathematical Social Sciences

journal homepage:www.elsevier.com/locate/econbase

Optimal timing of regime switching in optimal growth models: A Sobolev space approach

Erol Dogan

a

, Cuong Le Van

b,c

, Cagri Saglam

a,

aDepartment of Economics, Bilkent University, Turkey

bCNRS, Paris School of Economics, France

cExeter University Business School, United Kingdom

a r t i c l e i n f o

Article history:

Received 20 July 2009 Received in revised form 20 November 2010 Accepted 22 November 2010 Available online 5 December 2010

JEL classification:

C61 O41 Keywords:

Multi-stage optimal control Sobolev spaces

Optimal growth models

a b s t r a c t

This paper analyses the optimal timing of switching between alternative and consecutive regimes in optimal growth models. We derive the appropriate necessary conditions for such problems by means of standard techniques from the calculus of variations and some basic properties of Sobolev spaces.

© 2010 Elsevier B.V. All rights reserved.

1. Introduction

Many decision processes arising in economics involve a finite number of discrete changes both in the structure of the system and the objective functional over the course of the planning horizon.

This paper presents the necessary conditions for the optimal timing of switches between these alternative regimes which are of particular importance.

Some early contributions to the optimal regime switching prob- lems have proposed multi-stage optimal control techniques that recall the Pontryagin maximum principle from a dynamic pro- gramming perspective (see Tomiyama, 1985; Tomiyama and Rossana, 1989;Makris,2001;Saglam,2010). The main idea is to reduce a two-stage problem into a standard one with a dynamic programming approach, first by solving the post-switch problem and then attaching its value function to the pre-switch one with the Pontryagin maximum principle concluding at the intermediate steps. The illustrations of this technique on technology adoption problems can be found inBoucekkine et al. (2004,2010).

We proceed in entirely different lines with the existing litera- ture. In particular, we utilize some basic properties of the Sobolev

Corresponding author. Tel.: +90 3122901598; fax: +90 3122665140.

E-mail addresses:edogan@bilkent.edu.tr(E. Dogan),

Cuong.Le-Van@univ-paris1.fr(C. Le Van),csaglam@bilkent.edu.tr(C. Saglam).

space Wloc1,1, and treat the problem by the standard tools of the calculus of variations. Our approach allows us to avoid the strict assumption that the value function be twice continuously differen- tiable. Yet, we are able to cover the three important aspects of the regime switching problems that have not been considered at the same time in the literature mentioned above: the infinite horizon for the objective functional to be maximized, the possibility of mul- tiple regime switches and the explicit dependence of the constraint functions and the objective functional on these switching instants.

Except for the switching in the technology regime and the objective functional, our optimization framework is identical to the so-called reduced form optimal growth models which have been extensively used in economics due to their simple mathematical structure and generality (seeMcKenzie,1986;Stokey and Lucas, 1989). Our crucial choice of the topological space is relevant for many optimal growth models, e.g. the Ramsey model, in which the feasible capital paths are proved to belong to this space and the feasible consumption paths belong to L1(seeAskenazy and Le Van, 1999, page 42). The Sobolev space Wloc1,1also turns out to be a powerful tool to extract the usual transversality conditions as necessary optimality conditions for such infinite horizon optimal growth problems (seeLe Van et al., 2007). Combining these with the standard tools of calculus of variations gets through the control problem of multiple regime switches without needing to decompose it in many auxiliary problems in a simple and unified

0165-4896/$ – see front matter©2010 Elsevier B.V. All rights reserved.

doi:10.1016/j.mathsocsci.2010.11.005

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manner. We prove that, in addition to the standard optimality conditions such as Euler–Lagrange, two specific sets of necessary conditions that characterize the optimal timing of regime switches emerge: continuity and the matching conditions. These are nothing but extensions of the Weierstrass–Erdmann corner conditions.

Indeed, we show that Weierstrass–Erdmann corner conditions extend to the problems with switches.

In order to show how our approach allows us to derive prop- erly and easily the necessary conditions for an infinite horizon multi-stage problem depending explicitly on the switching instant, we first analyze the optimal timing of technology adoption under embodiment and exogenously growing technology frontier. We show that the optimal timing of a technology upgrade depends crucially on how the growth advantage deriving from switching to a new economy with a higher degree of embodiment com- pares to the resulting obsolescence cost and the technology specific expertise loss. Later, we analyze an environmental control problem à laBoucekkine et al.(2010) that considers the trade-off between economic performance and environmental quality from the per- spective of a government over a finite time horizon.

The paper is organized as follows. Section2presents the con- sidered optimization problem, derives our necessary conditions of optimality for a two-stage problem, and compares them with the existing literature. Section3extends these results to the case of multiple regime switches. Section4 provides applications to an optimal adoption problem under embodiment with exogenously growing technology frontier and an environmental control prob- lem with the trade-off between economic performance and envi- ronmental quality. Finally, Section5concludes.

2. Model

We consider the optimal timing of switching between alterna- tive and consecutive regimes in a continuous time reduced form model:

max

x(.),t1

t1 t0

V1

(

x

(

t

), ˙

x

(

t

),

t

,

t1

)

ertdt

+

tf t1

V2

(

x

(

t

), ˙

x

(

t

),

t

,

t1

)

ertdt subject to

x

(

t0

) =

x0

,

(

x

(

t

), ˙

x

(

t

)) ∈

Dt1

(

t

) ⊂

R2

,

x

(

t

) ≥

0

,

a.e. on

[

t0

,

tf

] ,

tf

≤ ∞ ,

where Dt1

(

t

) = (

x

,

y

) |

ff12((xx,,yy,,tt,,tt11) ≥) ≥00,,for tfor t0ftt><tt11

, and fiare Rm valued, for m

1. Throughout, we adapt the notation that the symbol

denotes ‘‘all components are greater than or equal to...’’, and

>

denotes ‘‘all components are strictly greater than...’’.

We recall some of the general definitions, notations and the results that will be useful in our analysis fromBrezis(1983). We will say that a measurable function, x

: [

t0

,

tf

] →

R is locally integrable if

|

x

|

is integrable on any bounded interval and write x

L1loc. Llocwill denote functions essentially bounded on finite intervals. By Cck

(

a

,

b

)

, we denote the set of k times continuously differentiable functions, say x, in an open interval

(

a

,

b

)

with supp x

= {

t

R+

: |

x

(

t

)| >

0

} ⊂ (

a

,

b

)

. For any x

L1loc

,

x is the weak derivative of x if

h

Cc1

(

t0

,

tf

), 

tt0f x

(

t

h

(

t

)

dt

=

− 

tf

t0 x

(

t

)

h

(

t

)

dt. For a function x

Cc1

(

t0

,

tf

)

, the weak derivative is identical with the ordinary derivative.

W1,1

W1,1

(

t0

,

tf

) ≡ {

x

L1

:

xexists and x

L1

}

with the norm defined by

x

‖ = 

tf

t0

|

x

|

dt

+ 

tf t0

|

x

|

dt, is the Sobolev space that we will be frequently referring to in our analysis. Wloc1,1 is similarly defined on

(

t0

,

tf

)

to be

{

x

L1loc

:

xexists and x

L1loc

}

. Two important properties of the Sobolev space will prove to be crucial in our analysis. As the ele- ments of this space are equivalence classes, for any function x

W1,1, there is a continuous representativex which is equal to x

˜

almost everywhere. We will be talking about this representative, whenever we refer to an element of this space. Secondly, weak derivative coincides with the usual derivative almost everywhere andx

˜ (

b

) = ˜

x

(

a

) + 

abxdt. Thus, the elements of this space are ab- solutely continuous functions on finite intervals. In fact, on a finite open interval, the set of absolutely continuous functions and the Sobolev space W1,1are the same.

Definition 1. A pair

(

x

˜ (.),

t1

˜ )

is admissible if x

˜ (

t

) ∈

Wloc1,1,x

˙

˜ (

t

) ∈

Lloc, satisfy the constraints

x

˜ (

t0

) =

x0

, (

x

˜ (

t

), ˙

x

˜ (

t

)) ∈

Dt1

(

t

) ⊂

R2

,

x

˜ (

t

) ≥

0

,

a.e. on

[

t0

,

tf

] ,

tf

≤ +∞ ,

and

t1

t0

V1(x

˜(t), ˙x

˜(t),t,t1)ertdt+

tf

t1

V2(x

˜(t), ˙x

˜(t),t,t1)ertdt< +∞.

A pair

(

x

(.),

t1

)

is an optimal solution if it is admissible and if the value of the objective function corresponding to any admissible pair is not greater than that of

(

x

(.),

t1

).

From now on, x will always refer to the optimal values unless otherwise stated. We have the following set of assumptions.

Assumption 1. Vi

:

R4

R is C1and fi

:

R4

Rmis continuous for i

=

1

,

2.

Assumption 2 (Interiority). x

(

t

) >

0

,

fi

(

x

, ˙

x

,

t

,

t1

) >

0 uniformly in the sense of the space Lon any bounded interval for i

=

1

,

2 (i.e., on any bounded interval there exists an

ε >

0 such that x

(

t

) > ε ,

fi

(

x

, ˙

x

,

t

,

t1

) > ε

, on their respective domains, almost everywhere on the interval).

The following proposition gives the Euler–Lagrange equation for the problem that incorporates a change in the objective functional at an instant in a very elementary way within our functional framework. To ease the notation, the third and the fourth argument of Vi(i

=

1

,

2) will be suppressed whenever we do not need them.

Proposition 1 (Euler–Lagrange). UnderAssumptions 1and2, the optimal x

(

t

)

satisfies

(

Vx˙

(

x

, ˙

x

)

ert

)

=

Vx

(

x

, ˙

x

)

ert

,

(1) almost everywhere on any bounded interval

(

a

,

b

)

, where V should be read as V1whenever t

<

t1and V2whenever t

>

t1.

Proof. The proof follows from Dana and Le Van (2003), but it is based on the use of weak derivatives to handle the switching between alternative regimes.

Consider any bounded interval

(

a

,

b

)

on

(

t0

,

tf

)

. Take any h

Cc1

(

a

,

b

)

, and assume that it is extended to zero outside of

(

a

,

b

).

For

| λ|

small x

+ λ

h

>

0, clearly. Moreover, for

| λ|

small, for an appropriate

ϵ, (

x

+ λ

h

, ˙

x

+ λ˙

h

)

is in an open ball of radius

ϵ

centered at

(

x

, ˙

x

)

, for each t

∈ (

a

,

b

)

so that fi

(

x

+ λ

h

, ˙

x

+ λ˙

h

,

t

,

t1

) >

0, for i

=

1

,

2.

Define

ϕ(λ) = 

abV

(

x

+ λ

h

, ˙

x

+ λ˙

h

)

ertdt

= ϕ

1

(λ)+ϕ

2

(λ)

, and write

ϕ

1

(λ) = 

at1V1

(

x

+ λ

h

, ˙

x

+ λ˙

h

)

ertdt

, ϕ

2

(λ) = 

tb1V2

(

x

+ λ

h

, ˙

x

+ λ˙

h

)

ertdt. For any sequence of real numbers

λ

n

0, fixing any t

,

V

(

x

+ λ

nh

, ˙

x

+ λ

nh

˙ ) −

V

(

x

, ˙

x

) λ

n

=

Vx

(

x

+ ¯ λ

nh

, ˙

x

+ ¯ λ

nh

˙ )

h

+

V˙x

(

x

+ ¯ λ

nh

, ˙

x

+ ¯ λ

nh

˙ )˙

h

,

for some 0

< |¯λ

n

| < |λ

n

|

, by Mean Value Theorem.

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E. Dogan et al. / Mathematical Social Sciences 61 (2011) 97–103 99

Now, Vx and V˙x are continuous and they are restricted to a bounded rectangle in R2, due to the continuity of x and the boundedness of

˙

x. So, Vx

(

x

+ ¯ λ

nh

, ˙

x

+ ¯ λ

nh

˙ )

and Vx˙

(

x

+ ¯ λ

nh

, ˙

x

+ ¯ λ

nh

˙ )˙

h are bounded in L

(

a

,

b

)

when n is large enough.

Thus, there exists K

R, such that

|

V(x+λnhx+λλn˙h)−V(xx)

n

| ≤

K

,

a.e. on

(

a

,

b

)

. Then, we may apply Dominated Convergence Theorem to the sequence

ϕ

1

n

) − ϕ

1

(

0

) λ

n

=

t1 a

V1

(

x

+ λ

nh

, ˙

x

+ λ

nh

˙ ) −

V1

(

x

, ˙

x

) λ

n

ertdt

,

concluding that

ϕ

1

(λ)

is differentiable at 0 with the derivative,

lim

n→∞

t1 a

V1

(

x

+ λ

nh

, ˙

x

+ λ

nh

˙ ) −

V1

(

x

, ˙

x

) λ

n

ertdt

=

t1 a

(

Vx1

(

x

, ˙

x

)

hert

+

Vx˙1

(

x

, ˙

x

hert

)

dt

.

By repeating the same steps on

(

t1

,

b

)

one may also find that

ϕ

2

(

0

) = 

tb1

(

Vx2

(

x

, ˙

x

)

hert

+

Vx˙2

(

x

, ˙

x

hert

)

dt.

Hence, we easily obtain that

ϕ

(

0

) = 

ab

(

Vx

(

x

, ˙

x

)

hert

+

Vx˙

(

x

, ˙

x

hert

)

dt

.

Now,

b

a V

(

x

+ λ

h

, ˙

x

+ λ˙

h

)

ertdt

− 

b

a V

(

x

, ˙

x

)

ertdt

= ϕ(λ) − ϕ(

0

)

, so that

ϕ(.)

is maximized at 0. Since

ϕ(.)

is differentiable at zero,

ϕ

(

0

) =

b a

(

Vx

(

x

, ˙

x

)

erth

+

Vx˙

(

x

, ˙

x

)

erth

˙ )

dt

=

0

.

(2) As h

Cc1

(

a

,

b

)

was arbitrary,

(

V˙x

(

x

, ˙

x

)

ert

)

=

Vx

(

x

, ˙

x

)

ert, i.e. Vx

(

x

, ˙

x

)

ertis the weak derivative of V˙x

(

x

, ˙

x

)

erton

(

a

,

b

)

.  By means of the Euler–Lagrange equation, we are able to derive an important result for the problems with switches, known as the first Weierstrass–Erdmann condition.

Corollary 1 (Continuity Condition). LetAssumptions 1and2be sat- isfied. Then V˙x

(

x

, ˙

x

)

ertis continuous everywhere, and in particular, at the switching instant.

Proof. The Euler–Lagrange equation implies V˙x

(

x

, ˙

x

)

ert

Wloc1,1 so that V˙x

(

x

, ˙

x

)

ert is absolutely continuous on any bounded interval and hence continuous everywhere. 

The following results and the set of assumptions that impose more regularity on x

(

t

)

, will be crucial in establishing the optimality conditions with respect to the switching instant.

Corollary 2. The optimal x

(

t

)

is locally Lipschitz, i.e., Lipschitz on any bounded interval.

Proof. Since x

(

t

)

is admissible,

x

(

t

)|

is bounded locally. Hence, for any bounded

(

a

,

b

) ⊂ (

t0

,

tf

)

, there is some K such that for all t

∈ (

a

,

b

), |˙

x

(

t

)| ≤

K and thus

|

x

(

b

) −

x

(

a

)| = | 

abxdt

˙ | ≤

K

|

b

a

| .



In what follows, some global properties of the functions Vi (i

=

1

,

2) will be needed. Because of this, we continue with the following modification ofAssumption 1. We write V2i for the derivative of Viwith respect to the second variable, and V22i for the derivative of V2iwith respect to the second variable.

Assumption 3. V2iis C1and V22i is invertible (i.e., either V22i

<

0 or V22i

>

0) on R

×

R

× [

t

,

t

]

for t

,

tfinite in

[

t0

,

tf

]

, and i

=

1

,

2

.

Proposition 2. If the optimal x is Lipschitz on bounded open intervals, then x is C2except possibly at t1

.

Proof. SeeButtazzo et al.(1998), Proposition 4.4, page 135. 

Note thatAssumption 3assumes a global invertibility condi- tion, which may be violated in applications. If, however, the so- lution of the Euler–Lagrange equation happens to be C1then one may utilize a local invertibility criterion as the following variant of Proposition 2demonstrates.

Proposition 3. For any bounded interval I, if V2i is C1 on some neighborhood of the path

(

x

, ˙

x

,

t

)

, V22i is invertible along the path

(

x

, ˙

x

,

t

)

, for t

I, i

=

1

,

2, and x is C1(except possibly at t1), then x is C2(except possibly at t1).

Proof. SeeButtazzo et al.(1998), Proposition 4.2, page 135.  So whenever global invertibility and smoothness conditions of Assumption 3are violated one may replaceAssumption 3with the assumptions ofProposition 3. In this case, one may also restrict the domain of Assumption 1 to a small enough neighborhood around the optimal path, if necessary. This simply follows from the fact that the proof of the Euler–Lagrange equation utilizes the assumption only in such a neighborhood. In fact, it is this version that we utilize in the technology adoption and the environmental control problems presented in Section4.

Assumption 4. There exists an integrable function g

(

t

)

on

[

t0

,

tf

]

and some interval I

⊂ [

t0

,

tf

]

, such that t1is in the interior of I, and

s

I

, ∀

t

, |

Vsi

(

x

, ˙

x

,

t

,

s

)|

ert

g

(

t

)

, for i

∈ {

1

,

2

}

(in the case of t1

= ∞

, the interval I is of the form,

[

N

, +∞)

for some N

< +∞

).

Note that if the planning horizon is finite, i.e., tf

< ∞

, Assumption 5 is automatically satisfied. The next proposition, which is a variant of the second Weierstrass–Erdmann corner conditions, will be proved under Assumptions 1–4, by the so- called ‘‘variation of the independent variable’’ technique. In the next proposition, recall also thatAssumption 3can be replaced with the assumptions ofProposition 3, andAssumption 1can be replaced to be satisfied in a neighborhood of the optimal path, whenever convenient.

Proposition 4 (Matching Condition). UnderAssumptions 1–4, opti- mal pair

(

x

,

t1

)

satisfies

xV˙x1

V1

]

t1ert1

− [˙

xVx˙2

V2

]

t1ert1

=

t1 t0

Vt11ertdt

+

tf t1

Vt21ertdt (3)

whenever t0

<

t1

<

tf

.

Proof. Take any h

Cc1

(

t0

,

tf

)

, and define a function

τ(

t

, ϵ) =

t

− ϵ

h

(

t

)

on

[

t0

,

tf

]

(h is extended to zero outside

(

t0

,

tf

)

). Note that

τ(

t0

, ε) =

t0and

τ(

tf

, ε) =

tf. For

| ϵ|

small enough,

τ

t

(

t

, ϵ) =

1

− ϵ

h

(

t

) >

0 (we continue to use subscripts for derivatives). Thus, for all such small

| ϵ|

, the mapping

τ(., ϵ)

is a C1diffeomorphism of

[

t0

,

tf

]

. Write

ζ (

s

, ϵ)

, for the inverse of this mapping, and denote

τ(

t1

, ϵ) =

s1.

Since the transformation t

→

t

− ϵ

h

(

t

)

, is monotonic, for

| ϵ|

small enough, the path x

(ζ (

s

, ϵ))

as a function of s

= τ(

t

, ϵ)

, satisfies the constraints of the problem, thanks to the differentiability properties of the functions and continuity (expect possibly for the switching instant) of the solutions involved. Let Wi

(

x

, ˙

x

,

t

,

t1

) =

Vi

(

x

, ˙

x

,

t

,

t1

)

ert

,

i

=

1

,

2. So,

ϕ(ϵ) =

s1 t0

W1

x

(ζ (

s

, ϵ)),

dx

(ζ (

s

, ϵ))

ds

,

s

,

s1

ds

+

tf s1

W2

x

(ζ (

s

, ϵ)),

dx

(ζ (

s

, ϵ))

ds

,

s

,

s1

ds

is maximized at 0 (Note that

τ(

t

,

0

) =

t).

(4)

Sincedx(ζ (dss,ϵ))

= ˙

x

(ζ (

s

, ϵ))ζ

s

(

s

, ϵ)

, we write:

ϕ(ϵ) =

s1 t0

W1

(

x

(ζ(

s

, ϵ)), ˙

x

(ζ(

s

, ϵ))ζ

s

(

s

, ϵ),

s

,

s1

)

ds

+

tf s1

W2

(

x

(ζ (

s

, ϵ)), ˙

x

(ζ(

s

, ϵ))ζ

s

(

s

, ϵ),

s

,

s1

)

ds

.

(4) As

ϕ(ϵ)

is finite and

τ

is a C1 diffeomorphism, the change of variables (seeLang, 1993, p. 505, Theorem 2.6) allows us to transform this equation into the following form:

ϕ(ϵ) =

t1 t0

W1

x

(

t

), ˙

x

(

t

) τ

t

(

1t

, ϵ) , τ(

t

, ϵ), τ(

t1

, ϵ)

τ

t

(

t

, ϵ)

dt

+

tf t1

W2

(

x

(

t

), ˙

x

(

t

) τ

t

(

t1

, ϵ) , τ(

t

, ϵ), τ(

t1

, ϵ))τ

t

(

t

, ϵ)

dt (5) where we use

τ

t

(ζ (

s

, ϵ), ϵ)ζ

s

(

s

, ϵ) =

1

.

Now, in a neighborhood of zero, byAssumptions 1and4, the partial derivatives with respect to

ϵ

of the integrands above,

(

1

− ϵ

h

)

[

Wtih

+ ˙

xWx˙i h

(

1

− ϵ

h

)

2

Wti

1h

(

t1

) ]

Wih

,

will be dominated by an integrable function. This is obvious for the terms multiplied by h or h. For the term,

(

1

− ϵ

h

)

Wti1h

(

t1

)

, this is due to the fact that for

ε

small,

τ(

t1

, ε)

will be in the interval I from Assumption 4, so that some g

(

t

)

dominates the term

|

Wti

1

|

, while

| (

1

− ϵ

h

)

h

(

t1

)|

is already bounded on

[

t0

,

tf

]

. It then follows by the dominated convergence theorem that

ϕ(ϵ)

is differentiable at zero. This derivative is equal to zero, and is given by the following expression (we suppress the arguments of the functions):

ϕ

(

0

) =

t1 t0

[−

Wt1h

+ ˙

xWx˙1h

Wt1

1h

(

t1

) −

W1h

]

dt

+

tf t1

[−

Wt2h

+ ˙

xW˙x2h

Wt2

1h

(

t1

) −

W2h

]

dt

.

(6) By integration by parts, we obtain

t1 t0

xWx˙1

W1

]

hdt

= [˙

xWx˙1

W1

]

t1h

(

t1

)

t1 t0

d

xW˙x1

W1

]

dt hdt

,

tf t1

xW˙x2

W2

]

hdt

= −[˙

xW˙x2

W2

]

t1h

(

t1

)

tf t1

d

xW˙x2

W2

]

dt hdt

.

Plugging these in

ϕ

(

0

)

, we obtain

h

(

t1

)([˙

xWx˙1

W1

]

t1

− [˙

xWx˙2

W2

]

t1

) +

t1 t0

Wt1

d

xW˙x1

W1

]

dt

hdt

+

tf t1

Wt2

d

xWx˙2

W2

]

dt

hdt

=

h

(

t1

) ∫

t1 t0

Wt1

1dt

+

tf t1

Wt2

1dt

 .

For h

(

t1

) ̸=

0

,

xWx˙1

W1

]

t1

− [˙

xWx˙2

W2

]

t1

=

t1 t0

Wt1

1dt

+

tf t1

Wt2

1dt

+

1

h

(

t1

) [∫

t1

t0

Wt1

+

d

xWx˙1

W1

]

dt

hdt

+

tf t1

Wt2

+

d

xWx˙2

W2

]

dt

hdt

]

.

(7)

We will now prove that Wt1

+

dxW

1

˙xW1]

dt

=

0. Indeed, since

d(W˙x1)

dt

=

Wx1by the Euler equation, one has d

xW˙x1

W1

]

dt

= ¨

xW˙x1

+ ˙

xWx1

Wx1x

˙ −

W˙x1x

¨ −

Wt1

= −

Wt1

.

The result follows. Similarly, one gets

Wt2

+

d

xWx˙2

W2

]

dt

=

0

.

Therefore, replacing Wiby Viertin(7)gives(3). 

In order to consider the corner solution cases in which the optimal switching time is at one of the terminal times, we need an additional assumption ensuring that some initial or final segment of an optimal path x, is also admissible under the other regime. Note that, whenever t1is an interior point of

[

t0

,

tf

]

, such a uniformity requirement is not necessary at all, as the inner variation of the optimal path around an interior switching point respects the admissibility condition anyway.

Assumption 5. Let

(

x

,

t1

)

be an optimal pair. If t1

=

t0, there exists a non-degenerate interval t0

I

⊂ [

t0

,

tf

]

and

ϵ >

0, such that,

s

I, and t

<

s

,

f1

(

x

(

t

), ˙

x

(

t

),

t

,

s

) > ϵ.

If t1

=

tf, there exists a non-degenerate interval tf

I

⊂ [

t0

,

tf

]

and

ϵ >

0, such that,

s

I

, ∃¯

t such that, if t

>

s

,

f2

(

x

(

t

), ˙

x

(

t

),

t

,

s

) ≥

0 and if t

¯ >

t

>

s, f2

(

x

(

t

), ˙

x

(

t

),

t

,

s

) > ϵ

(note that we need f1

(

x

(

t

), ˙

x

(

t

),

t

,

s

) > ϵ

on

(

t0

,

s

)

and f2

(

x

(

t

), ˙

x

(

t

),

t

,

s

) > ϵ

on

(

s

, ¯

t

)

in order to allow room for inner variation on finite intervals around the switching point).

Proposition 5. Under Assumptions 1–5, whenever the optimal switching time is at one of the terminal times, the matching condition should be modified as

xV˙x1

V1

]

t=t0ert0

− [˙

xVx˙2

V2

]

t=t0ert0

tf t0

Vt2

1ertdt

,

for t1

=

t0

,

and

xV˙x1

V1

]

t=tfertf

− [˙

xVx˙2

V2

]

t=tfertf

tf t0

Vt11ertdt

,

for t1

=

tf

,

where in the case of tf

= ∞

, the last inequality holds in the limit.

Proof. The proof follows from the calculation of the limit of a directional derivative of the function

ϕ(ϵ)

, which is defined in the proof ofProposition 4, where the limit is taken with respect to a sequence of functions hnreplacing h in

ϕ(ϵ)

. But this calculation is rather tedious and we omit it. 

Remark 1. In order to compare our results with those of the two- stage optimal control approach, define the Hamiltonian of the pre- switch and post-switch phases of the problem as

Hi

(

x

,

p

,

t

,

t1

) = −

Vi

(

x

, ˙

x

,

t

,

t1

)

ert

+

pix

˙ ,

i

=

1

,

2

.

Following fromDana and Le Van(2003), under the conditions that Vi is C2

,

V22i is invertible, say V22i

<

0, for i

=

1

,

2, a solution of the Euler–Lagrange equation is a solution of the corresponding

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