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Dual Variational Formulations for a Large Class of Non-Convex Models in the Calculus of Variations

A peer-reviewed version of this preprint was published in:
Mathematics 2022, 11(1), 63. https://doi.org/10.3390/math11010063

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04 January 2023

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04 January 2023

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Abstract
This article develops dual variational formulations for a large class of models in variational optimization. The results are established through basic tools of functional analysis, convex analysis and duality theory. The main duality principle is developed as an application to a Ginzburg-Landau type system in superconductivity in the absence of a magnetic field. In the first sections, we develop new general dual convex variational formulations, more specifically, dual formulations with a large region of convexity around the critical points which are suitable for the non-convex optimization for a large class of models in physics and engineering. Finally, in the last section we present some numerical results concerning the generalized method of lines applied to a Ginzburg-Landau type equation.
Keywords: 
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1. Introduction

In this section we establish a dual formulation for a large class of models in non-convex optimization.
The main duality principle is applied to the Ginzburg-Landau system in superconductivity in an absence of a magnetic field.
Such results are based on the works of J.J. Telega and W.R. Bielski [2,3,13,14] and on a D.C. optimization approach developed in Toland [15].
About the other references, details on the Sobolev spaces involved are found in [1]. Related results on convex analysis and duality theory are addressed in [5,6,7,9,12]. Finally, similar models on the superconductivity physics may be found in [4,11].
Remark 1.
It is worth highlighting, we may generically denote
Ω [ ( γ 2 + K I d ) 1 v * ] v * d x
simply by
Ω ( v * ) 2 γ 2 + K d x ,
where I d denotes a concerning identity operator.
Other similar notations may be used along this text as their indicated meaning are sufficiently clear.
Also, 2 denotes the Laplace operator and for real constants K 2 > 0 and K 1 > 0 , the notation K 2 K 1 means that K 2 > 0 is much larger than K 1 > 0 .
Finally, we adopt the standard Einstein convention of summing up repeated indices, unless otherwise indicated.
In order to clarify the notation, here we introduce the definition of topological dual space.
Definition 1
(Topological dual spaces). Let U be a Banach space. We shall define its dual topological space, as the set of all linear continuous functionals defined on U. We suppose such a dual space of U, may be represented by another Banach space U * , through a bilinear form · , · U : U × U * R (here we are referring to standard representations of dual spaces of Sobolev and Lebesgue spaces). Thus, given f : U R linear and continuous, we assume the existence of a unique u * U * such that
f ( u ) = u , u * U , u U .
The norm of f , denoted by f U * , is defined as
f U * = sup u U { | u , u * U | : u U 1 } u * U * .
At this point we start to describe the primal and dual variational formulations.
Let Ω R 3 be an open, bounded, connected set with a regular (Lipschitzian) boundary denoted by Ω .
Firstly we emphasize that, for the Banach space Y = Y * = L 2 ( Ω ) , we have
v , v * L 2 = Ω v v * d x , v , v * L 2 ( Ω ) .
For the primal formulation we consider the functional J : U R where
J ( u ) = γ 2 Ω u · u d x + α 2 Ω ( u 2 β ) 2 d x u , f L 2 .
Here we assume α > 0 , β > 0 , γ > 0 , U = W 0 1 , 2 ( Ω ) , f L 2 ( Ω ) . Moreover we denote
Y = Y * = L 2 ( Ω ) .
Define also G 1 : U R by
G 1 ( u ) = γ 2 Ω u · u d x ,
G 2 : U × Y R by
G 2 ( u , v ) = α 2 Ω ( u 2 β + v ) 2 d x + K 2 Ω u 2 d x ,
and F : U R by
F ( u ) = K 2 Ω u 2 d x ,
where K γ .
It is worth highlighting that in such a case
J ( u ) = G 1 ( u ) + G 2 ( u , 0 ) F ( u ) u , f L 2 , u U .
Furthermore, define the following specific polar functionals specified, namely, G 1 * : [ Y * ] 2 R by
G 1 * ( v 1 * + z * ) = sup u U u , v 1 * + z * L 2 G 1 ( u ) = 1 2 Ω [ ( γ 2 ) 1 ( v 1 * + z * ) ] ( v 1 * + z * ) d x ,
G 2 * : [ Y * ] 2 R by
G 2 * ( v 2 * , v 0 * ) = sup ( u , v ) U × Y u , v 2 * L 2 + v , v 0 * L 2 G 2 ( u , v ) = 1 2 Ω ( v 2 * ) 2 2 v 0 * + K d x + 1 2 α Ω ( v 0 * ) 2 d x + β Ω v 0 * d x ,
if v 0 * B * where
B * = { v 0 * Y * : 2 v 0 * + K > K / 2 in Ω } .
At this point, we give more details about this calculation.
Observe that
G 2 * ( v 2 * , v 0 * ) = sup ( u , v ) U × Y u , v 2 * L 2 + v , v 0 * L 2 G 2 ( u , v ) = sup ( u , v ) U × Y u , v 2 * L 2 + v , v 0 * L 2 α 2 Ω ( u 2 β + v ) 2 d x K 2 Ω u 2 d x .
Defining w = u 2 β + v , we have v = w u 2 + β , so that
G 2 * ( v 2 * , v 0 * ) = sup ( u , v ) U × Y u , v 2 * L 2 + v , v 0 * L 2 α 2 Ω ( u 2 β + v ) 2 d x K 2 Ω u 2 d x = sup ( u , w ) U × Y u , v 2 * L 2 + w u 2 + β , v 0 * L 2 α 2 Ω ( w ) 2 d x K 2 Ω u 2 d x = u ˜ , v 2 * L 2 + w ˜ u ˜ 2 + β , v 0 * L 2 α 2 Ω ( w ˜ ) 2 d x K 2 Ω u ˜ 2 d x ,
where ( u ˜ , w ˜ ) are solution of equations (optimality conditions for such a quadratic optimization problem)
v 0 * α w ˜ = 0 ,
and
v 2 * ( 2 v 0 * + K ) u ˜ = 0 ,
and therefore
w ˜ = v 0 * α ,
and
u ˜ = v 2 * 2 v 0 * + K .
Replacing such results into (7) we obtain
G * ( v 1 * , v 0 * ) = 1 2 Ω ( v 2 * ) 2 2 v 0 * + K d x + 1 2 α Ω ( v 0 * ) 2 d x + β Ω v 0 * d x ,
if v 0 * B * .
Finally, F * : Y * R is defined by
F * ( z * ) = sup u U u , z * L 2 F ( u ) = 1 2 K Ω ( z * ) 2 d x .
Define also
A * = { v * = ( v 1 * , v 2 * , v 0 * ) [ Y * ] 2 × B * : v 1 * + v 2 * f = 0 , in Ω } ,
J * : [ Y * ] 4 R by
J * ( v * , z * ) = G 1 * ( v 1 * + z * ) G 2 * ( v 2 * , v 0 * ) + F * ( z * )
and J 1 * : [ Y * ] 4 × U R by
J 1 * ( v * , z * , u ) = J * ( v * , z * ) + u , v 1 * + v 2 * f L 2 .

2. The Main Duality Principle, a Convex Dual Formulation and the Concerning Proximal Primal Functional

Our main result is summarized by the following theorem.
Theorem 1.
Considering the definitions and statements in the last section, suppose also ( v ^ * , z ^ * , u 0 ) [ Y * ] 2 × B * × Y * × U is such that
δ J 1 * ( v ^ * , z ^ * , u 0 ) = 0 .
Under such hypotheses, we have
δ J ( u 0 ) = 0 ,
v ^ * A *
and
J ( u 0 ) = inf u U J ( u ) + K 2 Ω | u u 0 | 2 d x = J * ( v ^ * , z ^ * ) = sup v * A * J * ( v * , z ^ * ) .
Proof. 
Since
δ J 1 * ( v ^ * , z ^ * , u 0 ) = 0
from the variation in v 1 * we obtain
( v ^ 1 * + z ^ * ) γ 2 + u 0 = 0 in Ω ,
so that
v ^ 1 * + z ^ * = γ 2 u 0 .
From the variation in v 2 * we obtain
v ^ 2 * 2 v ^ 0 * + K + u 0 = 0 , in Ω .
From the variation in v 0 * we also obtain
( v ^ 2 * ) 2 ( 2 v ^ 0 * + K ) 2 v ^ 0 * α β = 0
and therefore,
v ^ 0 * = α ( u 0 2 β ) .
From the variation in u we get
v ^ 1 * + v ^ 2 * f = 0 , in Ω
and thus
v ^ * A * .
Finally, from the variation in z * , we obtain
( v ^ 1 * + z ^ * ) γ 2 + z ^ * K = 0 , in Ω .
so that
u 0 + z ^ * K = 0 ,
that is,
z ^ * = K u 0 in Ω .
From such results and v ^ * A * we get
0 = v ^ 1 * + v ^ 2 * f = γ 2 u 0 z ^ * + 2 ( v 0 * ) u 0 + K u 0 f = γ 2 u 0 + 2 α ( u 0 2 β ) u 0 f ,
so that
δ J ( u 0 ) = 0 .
Also from this and from the Legendre transform proprieties we have
G 1 * ( v ^ 1 * + z ^ * ) = u 0 , v ^ 1 * + z ^ * L 2 G 1 ( u 0 ) ,
G 2 * ( v ^ 2 * , v ^ 0 * ) = u 0 , v ^ 2 * L 2 + 0 , v 0 * L 2 G 2 ( u 0 , 0 ) ,
F * ( z ^ * ) = u 0 , z ^ * L 2 F ( u 0 )
and thus we obtain
J * ( v ^ * , z ^ * ) = G 1 * ( v ^ 1 * + z ^ * ) G 2 * ( v ^ 2 * , v ^ 0 * ) + F * ( z ^ * ) = u 0 , v ^ 1 * + v ^ 2 * + G 1 ( u 0 ) + G 2 ( u 0 , 0 ) F ( u 0 ) = u 0 , f L 2 + G 1 ( u 0 ) + G 2 ( u 0 , 0 ) F ( u 0 ) = J ( u 0 ) .
Summarizing, we have got
J * ( v ^ * , z ^ * ) = J ( u 0 ) .
On the other hand
J * ( v ^ * , z ^ * ) = G 1 * ( v ^ 1 * + z ^ * ) G 2 * ( v ^ 2 * , v ^ 0 * ) + F * ( z ^ * ) u , v ^ 1 * + z ^ * L 2 u , v ^ 2 * L 2 0 , v 0 * L 2 + G 1 ( u ) + G 2 ( u , 0 ) + F * ( z ^ * ) = u , f L 2 + G 1 ( u ) + G 2 ( u , 0 ) u , z ^ * L 2 + F * ( z ^ * ) = u , f L 2 + G 1 ( u ) + G 2 ( u , 0 ) F ( u ) + F ( u ) u , z ^ * L 2 + F * ( z ^ * ) = J ( u ) + K 2 Ω u 2 d x u , z ^ * L 2 + F * ( z ^ * ) = J ( u ) + K 2 Ω u 2 d x K u , u 0 L 2 + K 2 Ω u 0 2 d x = J ( u ) + K 2 Ω | u u 0 | 2 d x , u U .
Finally by a simple computation we may obtain the Hessian
2 J * ( v * , z * ) ( v * ) 2 < 0
in [ Y * ] 2 × B * × Y * , so that we may infer that J * is concave in v * in [ Y * ] 2 × B * × Y * .
Therefore, from this, (13) and (14), we have
J ( u 0 ) = inf u U J ( u ) + K 2 Ω | u u 0 | 2 d x = J * ( v ^ * , z ^ * ) = sup v * A * J * ( v * , z ^ * ) .
The proof is complete. □

3. A Primal Dual Variational Formulation

In this section we develop a more general primal dual variational formulation suitable for a large class of models in non-convex optimization.
Consider again U = W 0 1 , 2 ( Ω ) and let G : U R and F : U R be three times Fréchet differentiable functionals. Let J : U R be defined by
J ( u ) = G ( u ) F ( u ) , u U .
Assume u 0 U is such that
δ J ( u 0 ) = 0
and
δ 2 J ( u 0 ) > 0 .
Denoting v * = ( v 1 * , v 2 * ) , define J * : U × Y * × Y * R by
J * ( u , v * ) = 1 2 v 1 * G ( u ) 2 2 + 1 2 v 2 * F ( u ) 2 2 + 1 2 v 1 * v 2 * 2 2
Denoting L 1 * ( u , v * ) = v 1 * G ( u ) and L 2 * ( u , v * ) = v 2 * F ( u ) , define also
C * = ( u , v * ) U × Y * × Y * : L 1 * ( u , v 1 * ) 1 K and L 2 * ( u , v 1 * ) 1 K ,
for an appropriate K > 0 to be specified.
Observe that in C * the Hessian of J * is given by
{ δ 2 J * ( u , v * ) } = G ( u ) 2 + F ( u ) 2 + O ( 1 / K ) G ( u ) F ( u ) G ( u ) 2 1 F ( u ) 1 2 ,
Observe also that
det 2 J * ( u , v * ) v 1 * v 2 * = 3 ,
and
det { δ 2 J * ( u , v * ) } = ( G ( u ) F ( u ) ) 2 + O ( 1 / K ) = ( δ 2 J ( u ) ) 2 + O ( 1 / K ) .
Define now
v ^ 1 * = G ( u 0 ) ,
v ^ 2 * = F ( u 0 ) ,
so that
v ^ 1 * v ^ 2 * = 0 .
From this we may infer that ( u 0 , v ^ 1 * , v ^ 2 * ) C * and
J * ( u 0 , v ^ * ) = 0 = min ( u , v * ) C * J * ( u , v * ) .
Moreover, for K > 0 sufficiently big, J * is convex in a neighborhood of ( u 0 , v ^ * ) .
Therefore, in the last lines, we have proven the following theorem.
Theorem 2.
Under the statements and definitions of the last lines, there exist r 0 > 0 and r 1 > 0 such that
J ( u 0 ) = min u B r 0 ( u 0 ) J ( u )
and ( u 0 , v ^ 1 * , v ^ 2 * ) C * is such that
J * ( u 0 , v ^ * ) = 0 = min ( u , v * ) U × [ Y * ] 2 J * ( u , v * ) .
Moreover, J * is convex in
B r 1 ( u 0 , v ^ * ) .

4. One More Duality Principle and a Concerning Primal Dual Variational Formulation

In this section we establish a new duality principle and a related primal dual formulation.
The results are based on the approach of Toland, [15].

4.1. Introduction

Let Ω R 3 be an open, bounded, connected set with a regular (Lipschitzian) boundary denoted by Ω .
Let J : V R be a functional such that
J ( u ) = G ( u ) F ( u ) , u V ,
where V = W 0 1 , 2 ( Ω ) .
Suppose G , F are both three times Fréchet differentiable convex functionals such that
2 G ( u ) u 2 > 0
and
2 F ( u ) u 2 > 0
u V .
Assume also there exists α 1 R such that
α 1 = inf u V J ( u ) .
Moreover, suppose that if { u n } V is such that
u n V
then
J ( u n ) + , as n .
At this point we define J * * : V R by
J * * ( u ) = sup ( v * , α ) H * { u , v * + α } ,
where
H * = { ( v * , α ) V * × R : v , v * V + α F ( v ) , v V } .
Observe that ( 0 , α 1 ) H * , so that
J * * ( u ) α 1 = inf u V J ( u ) .
On the other hand, clearly we have
J * * ( u ) J ( u ) , u V ,
so that we have got
α 1 = inf u V J ( u ) = inf u V J * * ( u ) .
Let u V .
Since J is strongly continuous, there exist δ > 0 and A > 0 such that,
α 1 J * * ( v ) J ( v ) A , v B δ ( u ) .
From this, considering that J * * is convex on V, we may infer that J * * is continuous at u, u V .
Hence J * * is strongly lower semi-continuous on V, and since J * * is convex we may infer that J * * is weakly lower semi-continuous on V.
Let { u n } V be a sequence such that
α 1 J ( u n ) < α 1 + 1 n , n N .
Hence
α 1 = lim n J ( u n ) = inf u V J ( u ) = inf u V J * * ( u ) .
Suppose there exists a subsequence { u n k } of { u n } such that
u n k V , as k .
From the hypothesis we have
J ( u n k ) + , as k ,
which contradicts
α 1 R .
Therefore there exists K > 0 such that
u n V K , u V .
Since V is reflexive, from this and the Katutani Theorem, there exists a subsequence { u n k } of { u n } and u 0 V such that
u n k u 0 , weakly in V .
Consequently, from this and considering that J * * is weakly lower semi-continuous, we have got
α 1 = lim inf k J * * ( u n k ) J * * ( u 0 ) ,
so that
J * * ( u 0 ) = min u V J * * ( u ) .
Define G * , F * : V * R by
G * ( v * ) = sup u V { u , v * V G ( u ) } ,
and
F * ( v * ) = sup u V { u , v * V F ( u ) } .
Defining also J * : V R by
J * ( v * ) = F * ( v * ) G * ( v * ) ,
from the results in [15], we may obtain
inf u V J ( u ) = inf v * V * J * ( v * ) ,
so that
J * * ( u 0 ) = inf u V J * * ( u ) = inf u V J ( u ) = inf v * V * J * ( v * ) .
Suppose now there exists u ^ V such that
J ( u ^ ) = inf u V J ( u ) .
From the standard necessary conditions, we have
δ J ( u ^ ) = 0 ,
so that
G ( u ^ ) u F ( u ^ ) u = 0 .
Define now
v 0 * = F ( u ^ ) u .
From these last two equations we obtain
v 0 * = G ( u ^ ) u .
From such results and the Legendre transform properties, we have
u ^ = F * ( v 0 * ) v * ,
u ^ = G * ( v 0 * ) v * ,
so that
δ J * ( v 0 * ) = F * ( v 0 * ) v * G * ( v 0 * ) v * = u ^ u ^ = 0 ,
G * ( v 0 * ) = u ^ , v 0 * V G ( u ^ )
and
F * ( v 0 * ) = u ^ , v 0 * V F ( u ^ )
so that
inf u V J ( u ) = J ( u ^ ) = G ( u ^ ) F ( u ^ ) = inf v * V * J * ( v * ) = F * ( v 0 * ) G * ( v 0 * ) = J * ( v 0 * ) .

4.2. The Main Duality Principle and a Related Primal Dual Variational Formulation

Considering these last statements and results, we may prove the following theorem.
Theorem 3.
Let Ω R 3 be an open, bounded, connected set with a regular (Lipschitzian) boundary denoted by Ω .
Let J : V R be a functional such that
J ( u ) = G ( u ) F ( u ) , u V ,
where V = W 0 1 , 2 ( Ω ) .
Suppose G , F are both three times Fréchet differentiable functionals such that there exists K > 0 such that
2 G ( u ) u 2 + K > 0
and
2 F ( u ) u 2 + K > 0
u V .
Assume also there exists u 0 V and α 1 R such that
α 1 = inf u V J ( u ) = J ( u 0 ) .
Assume K 3 > 0 is such that
u 0 < K 3 .
Define
V ˜ = { u V : u K 3 } .
Assume K 1 > 0 is such that if u V ˜ then
max F ( u ) , G ( u ) , F ( u ) , F ( u ) , G ( u ) , G ( u ) K 1 .
Suppose also
K max { K 1 , K 3 } .
Define F K , G K : V R by
F K ( u ) = F ( u ) + K 2 Ω u 2 d x ,
and
G K ( u ) = G ( u ) + K 2 Ω u 2 d x ,
u V .
Define also G K * , F K * : V * R by
G K * ( v * ) = sup u V { u , v * V G K ( u ) } ,
and
F K * ( v * ) = sup u V { u , v * V F K ( u ) } .
Observe that since u 0 V is such that
J ( u 0 ) = inf u V J ( u ) ,
we have
δ J ( u 0 ) = 0 .
Let ε > 0 be a small constant.
Define
v 0 * = F K ( u 0 ) u V * .
Under such hypotheses, defining J 1 * : V × V * R by
J 1 * ( u , v * ) = F K * ( v * ) G K * ( v * ) + 1 2 ε G K * ( v * ) v * u 2 2 + 1 2 ε F K * ( v * ) v * u 2 2 + 1 2 ε G K * ( v * ) v * F K * ( v * ) v * 2 2 ,
we have
J ( u 0 ) = inf u V J ( u ) = inf ( u , v * ) V × V * J 1 * ( u , v * ) = J 1 * ( u 0 , v 0 * ) .
Proof. 
Observe that from the hypotheses and the results and statements of the last subsection
J ( u 0 ) = inf u V J ( u ) = inf v * Y * J K * ( v * ) = J K * ( v 0 * ) ,
where
J K * ( v * ) = F K * ( v * ) G K * ( v * ) , v * V * .
Moreover we have
J 1 * ( u , v * ) J K * ( v * ) , u V , v * V * .
Also from hypotheses and the last subsection results,
u 0 = F K * ( v 0 * ) v * = G K * ( v 0 * ) v * ,
so that clearly we have
J 1 * ( u 0 , v 0 * ) = J K * ( v 0 * ) .
From these last results, we may infer that
J ( u 0 ) = inf u V J ( u ) = inf v * V * J K * ( v * ) = J K * ( v 0 * ) = inf ( u , v * ) V × V * J 1 * ( u , v * ) = J 1 * ( u 0 , v 0 * ) .
The proof is complete.
Remark 2.
At this point we highlight that J 1 * has a large region of convexity around the optimal point ( u 0 , v 0 * ) , for K > 0 sufficiently large and corresponding ε > 0 sufficiently small.
Indeed, observe that for v * V * ,
G K * ( v * ) = sup u V { u , v * V G K ( u ) } = u ^ , v * V G K ( u ^ )
where u ^ V is such that
v * = G K ( u ^ ) u = G ( u ^ ) + K u ^ .
Taking the variation in v * in this last equation, we obtain
1 = G ( u ) u ^ v * + K u ^ v * ,
so that
u ^ v * = 1 G ( u ) + K = O 1 K .
From this we get
2 u ^ ( v * ) 2 = 1 ( G ( u ) + K ) 2 G ( u ) u ^ v * = 1 ( G ( u ) + K ) 3 G ( u ) = O 1 K 3 .
On the other hand, from the implicit function theorem
G K * ( v * ) v * = u + [ v * G K ( u ^ ) ] u ^ v * = u ,
so that
2 G K * ( v * ) ( v * ) 2 = u ^ v * = O 1 K
and
3 G K * ( v * ) ( v * ) 3 = 2 u ^ ( v * ) 2 = O 1 K 3 .
Similarly, we may obtain
2 F K * ( v * ) ( v * ) 2 = O 1 K
and
3 F K * ( v * ) ( v * ) 3 = O 1 K 3 .
Denoting
A = 2 F K * ( v 0 * ) ( v * ) 2
and
B = 2 G K * ( v 0 * ) ( v * ) 2 ,
we have
2 J 1 * ( u 0 , v 0 * ) ( v * ) 2 = A B + 1 ε 2 A 2 + 2 B 2 2 A B ,
2 J 1 * ( u 0 , v 0 * ) u 2 = 2 ε ,
and
2 J 1 * ( u 0 , v 0 * ) ( v * ) u = 1 ε ( A + B ) .
From this we get
det ( δ 2 J * ( v 0 * , u 0 ) ) = 2 J 1 * ( u 0 , v 0 * ) ( v * ) 2 2 J 1 * ( u 0 , v 0 * ) u 2 2 J 1 * ( u 0 , v 0 * ) ( v * ) u 2 = 2 A B ε + 2 ( A B ) 2 ε 2 = O 1 ε 2 0
about the optimal point ( u 0 , v 0 * ) .

5. A Convex Dual Variational Formulation

In this section, again for Ω R 3 an open, bounded, connected set with a regular (Lipschitzian) boundary Ω , γ > 0 , α > 0 , β > 0 and f L 2 ( Ω ) , we denote F 1 : V × Y R , F 2 : V R and G : V × Y R by
F 1 ( u , v 0 * ) = γ 2 Ω u · u d x K 2 Ω u 2 d x + K 1 2 Ω ( γ 2 u + 2 v 0 * u f ) 2 d x + K 2 2 Ω u 2 d x ,
F 2 ( u ) = K 2 2 Ω u 2 d x + u , f L 2 ,
and
G ( u , v ) = α 2 Ω ( u 2 β + v ) 2 d x + K 2 Ω u 2 d x .
We define also
J 1 ( u , v 0 * ) = F 1 ( u , v 0 * ) F 2 ( u ) + G ( u , 0 ) ,
J ( u ) = γ 2 Ω u · u d x + α 2 Ω ( u 2 β ) 2 d x u , f L 2 ,
and F 1 * : [ Y * ] 3 R , F 2 * : Y * R , and G * : [ Y * ] 2 R , by
F 1 * ( v 2 * , v 1 * , v 0 * ) = sup u V { u , v 1 * + v 2 * L 2 F 1 ( u , v 0 * ) } = 1 2 Ω v 1 * + v 2 * + K 1 ( γ 2 + 2 v 0 * ) f 2 ( γ 2 K + K 2 + K 1 ( γ 2 + 2 v 0 * ) 2 ) d x K 1 2 Ω f 2 d x ,
F 2 * ( v 2 * ) = sup u V { u , v 2 * L 2 F 2 ( u ) } = 1 2 K 2 Ω ( v 2 * ) 2 d x ,
and
G * ( v 1 * , v 0 * ) = sup ( u , v ) V × Y { u , v 1 * L 2 v , v 0 * L 2 G ( u , v ) } = 1 2 Ω ( v 1 * ) 2 2 v 0 * + K d x + 1 2 α Ω ( v 0 * ) 2 d x + β Ω v 0 * d x
if v 0 * B * where
B * = { v 0 * Y * : v 0 * K / 2 and γ 2 + 2 v 0 * < ε I d } ,
for some small real parameter ε > 0 and where I d denotes a concerning identity operator.
Finally, we also define J 1 * : [ Y * ] 2 × B * R ,
J 1 * ( v 2 * , v 1 * , v 0 * ) = F 1 * ( v 2 * , v 1 * , v 0 * ) + F 2 * ( v 2 * ) G * ( v 1 * , v 0 * ) .
Assuming
K 2 K 1 K max { 1 / ( ε 2 ) , 1 , γ , α }
by directly computing δ 2 J 1 * ( v 2 * , v 1 * , v 0 * ) we may obtain that for such specified real constants, J 1 * in convex in v 2 * and it is concave in ( v 1 * , v 0 * ) on Y * × Y * × B * .
Considering such statements and definitions, we may prove the following theorem.
Theorem 4.
Let ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) Y * × Y * × B * be such that
δ J 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) = 0
and u 0 V be such that
u 0 = v ^ 1 * + v ^ 2 * + K 1 ( γ 2 + 2 v 0 * ) f K 2 K γ 2 + K 1 ( γ 2 + 2 v ^ 0 * ) 2 .
Under such hypotheses, we have
δ J ( u 0 ) = 0 ,
so that
J ( u 0 ) = inf u V J ( u ) + K 1 2 Ω ( γ 2 u + 2 v ^ 0 * u f ) 2 d x = inf v 2 * Y * sup ( v 1 * , v 0 * ) Y * × B * J 1 * ( v 2 * , v 1 * , v 0 * ) = J 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) .
Proof. 
Observe that δ J 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) = 0 so that, since J 1 * is convex in v 2 * and concave in ( v 1 * , v 0 * ) on Y * × Y * × B * , we obtain
J 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) = inf v 2 * Y * sup ( v 1 * , v 0 * ) Y * × B * J 1 * ( v 2 * , v 1 * , v 0 * ) .
Now we are going to show that
δ J ( u 0 ) = 0 .
From
J 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) v 2 * = 0 ,
we have
u 0 + v ^ 2 * K 2 = 0 ,
and thus
v ^ 2 * = K 2 u 0 .
From
J 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) v 1 * = 0 ,
we obtain
u 0 v ^ 1 * f 2 v ^ 0 * + K = 0 ,
and thus
v ^ 1 * = 2 v ^ 0 * u 0 K u 0 + f .
Finally, denoting
D = γ 2 u 0 + 2 v ^ 0 * u 0 f ,
from
J 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) v 0 * = 0 ,
we have
2 D u 0 + u 0 2 v ^ 0 * α β = 0 ,
so that
v ^ 0 * = α ( u 0 2 β 2 D u 0 ) .
Observe now that
v ^ 1 * + v ^ 2 * + K 1 ( γ 2 + 2 v ^ 0 * ) f = ( K 2 K γ 2 + K 1 ( γ 2 + 2 v ^ 0 * ) 2 ) u 0
so that
K 2 u 0 2 v ^ 0 u 0 K u 0 + f = K 2 u 0 K u 0 γ 2 u 0 + K 1 ( γ 2 + 2 v ^ 0 * ) ( γ 2 u 0 + 2 v ^ 0 * u 0 f ) .
The solution for this last system of equations (30) and (31) is obtained through the relations
v ^ 0 * = α ( u 0 2 β )
and
γ 2 u 0 + 2 v ^ 0 * u 0 f = D = 0 ,
so that
δ J ( u 0 ) = γ 2 u 0 + 2 α ( u 0 2 β ) u 0 f = 0
and
δ J ( u 0 ) + K 1 2 Ω ( γ 2 u 0 + 2 v ^ 0 * u 0 f ) 2 d x = 0 ,
and hence, from the concerning convexity in u on V,
J ( u 0 ) = min u V J ( u ) + K 1 2 Ω ( γ 2 u + 2 v ^ 0 * u f ) 2 d x .
Moreover, from the Legendre transform properties
F 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) = u 0 , v ^ 2 * + v ^ 1 * L 2 F 1 ( u 0 , v ^ 0 * ) ,
F 2 * ( v ^ 2 * ) = u 0 , v ^ 2 * L 2 F 2 ( u 0 ) ,
G * ( v ^ 1 * , v ^ 0 * ) = u 0 , v ^ 1 * L 2 0 , v ^ 0 * L 2 G ( u 0 , 0 ) ,
so that
J 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) = F 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) + F 2 * ( v ^ 2 * ) G * ( v ^ 1 * , v ^ 0 * ) = F 1 ( u 0 , v ^ 0 * ) F 2 ( u 0 ) + G ( u 0 , 0 ) = J ( u 0 ) .
Joining the pieces, we have got
J ( u 0 ) = inf u V J ( u ) + K 1 2 Ω ( γ 2 u + 2 v ^ 0 * u f ) 2 d x = inf v 2 * Y * sup ( v 1 * , v 0 * ) Y * × B * J 1 * ( v 2 * , v 1 * , v 0 * ) = J 1 * ( v ^ 2 * , v ^ 1 * , v ^ 0 * ) .
The proof is complete.
Remark 3.
We could have also defined
B * = { v 0 * Y * : v 0 * K / 2 and γ 2 + 2 v 0 * > ε I d } ,
for some small real parameter ε > 0 . In this case, γ 2 + 2 v 0 * is positive definite, whereas in the previous case, γ 2 + 2 v 0 * is negative definite.

6. Another Convex Dual Variational Formulation

In this section, again for Ω R 3 an open, bounded, connected set with a regular (Lipschitzian) boundary Ω , γ > 0 , α > 0 , β > 0 and f L 2 ( Ω ) , we denote F 1 : V × Y R , F 2 : V R and G : Y R by
F 1 ( u , v 0 * ) = γ 2 Ω u · u d x + u 2 , v 0 * L 2 + K 1 2 Ω ( γ 2 u + 2 v 0 * u f ) 2 d x + K 2 2 Ω u 2 d x ,
F 2 ( u ) = K 2 2 Ω u 2 d x + u , f L 2 ,
and
G ( u 2 ) = α 2 Ω ( u 2 β ) 2 d x .
We define also
J 1 ( u , v 0 * ) = F 1 ( u , v 0 * ) F 2 ( u ) u 2 , v 0 * L 2 + G ( u 2 ) ,
J ( u ) = γ 2 Ω u · u d x + α 2 Ω ( u 2 β ) 2 d x u , f L 2 ,
A + = { u V : u f > 0 , a . e . in Ω } ,
V 2 = { u V : u K 3 } ,
V 1 = A + V 1 ,
and F 1 * : [ Y * ] 2 R , F 2 * : Y * R , and G * : Y * R , by
F 1 * ( v 2 * , v 0 * ) = sup u V { u , v 2 * L 2 F 1 ( u , v 0 * ) } = 1 2 Ω v 2 * + K 1 ( γ 2 + 2 v 0 * ) f 2 ( γ 2 + 2 v 0 * + K 2 + K 1 ( γ 2 + 2 v 0 * ) 2 ) d x K 1 2 Ω f 2 d x ,
F 2 * ( v 2 * ) = sup u V { u , v 2 * L 2 F 2 ( u ) } = 1 2 K 2 Ω ( v 2 * + f ) 2 d x ,
and
G * ( v 0 * ) = sup v Y { v , v 0 * L 2 G ( v ) } = 1 2 α Ω ( v 0 * ) 2 d x + β Ω v 0 * d x
At this point we define
B 1 * = { v 0 * Y * : v 0 * K / 2 } ,
B 2 * = { v 0 * Y * : γ 2 + 2 v 0 * + K 1 ( γ 2 + 2 v 0 * ) 2 > 0 } ,
B 3 * = { v 0 * Y * : 1 / α + 4 K 1 [ u ( v 2 * , v 0 * ) 2 ] + 100 / K 2 0 , v 2 * E 1 * } ,
where
u ( v 2 * , v 0 * ) = φ 1 φ ,
φ 1 = ( v 2 * + K 1 ( γ 2 + 2 v 0 * ) f )
and
φ = ( γ 2 + 2 v 0 * + K 1 ( γ 2 + 2 v 0 * ) 2 + K 2 ) ,
Finally, we also define
E 1 * = { v 2 * Y * : v 2 * ( 5 / 4 ) K 2 } .
E 2 * = { v 2 * Y * : f v 2 * > 0 , a . e . in Ω } ,
E * = E 1 * E 2 * ,
B * = B 1 * B 3 * ,
and J 1 * : E * × B * R , by
J 1 * ( v 2 * , v 0 * ) = F 1 * ( v 2 * , v 0 * ) + F 2 * ( v 2 * ) G * ( v 0 * ) .
Moreover, assume
K 2 K 1 K K 3 max { 1 , γ , α } .
By directly computing δ 2 J 1 * ( v 2 * , v 0 * ) we may obtain that for such specified real constants, J 1 * is concave in v 0 * on E * × B * .
Indeed, recalling that
φ = ( γ 2 + 2 v 0 * + K 1 ( γ 2 + 2 v 0 * ) 2 + K 2 ) ,
φ 1 = ( v 2 * + K 1 ( γ 2 + 2 v 0 * ) f ) ,
and
u = φ 1 φ ,
we obtain
2 J 1 * ( v 2 * , v 0 * ) ( v 2 * ) 2 = 1 / K 2 1 / φ > 0 ,
in E * × B 3 * and
2 J 1 * ( v 2 * , v 0 * ) ( v 0 * ) 2 = 4 u 2 K 1 1 / α + O ( 1 / K 2 ) < 0 ,
in E * × B * .
Considering such statements and definitions, we may prove the following theorem.
Theorem 5.
Let ( v ^ 2 * , v ^ 0 * ) E * × ( B * B 2 * ) be such that
δ J 1 * ( v ^ 2 * , v ^ 0 * ) = 0
and u 0 V 1 be such that
u 0 = v ^ 2 * + K 1 ( γ 2 + 2 v ^ 0 * ) f K 2 + 2 v ^ 0 * γ 2 + K 1 ( γ 2 + 2 v ^ 0 * ) 2 .
Under such hypotheses, we have
δ J ( u 0 ) = 0 ,
so that
J ( u 0 ) = inf u V 1 J ( u ) + K 1 2 Ω ( γ 2 u + 2 v ^ 0 * u f ) 2 d x = inf v 2 * E * sup v 0 * B * J 1 * ( v 2 * , v 0 * ) = J 1 * ( v ^ 2 * , v ^ 0 * ) .
Proof. 
Observe that δ J 1 * ( v ^ 2 * , v ^ 0 * ) = 0 so that, since J 1 * concave in v 0 * on E * × B * , v 0 * B 2 * and J 1 * is quadratic in v 2 * , we get
sup v 0 * B * J 1 * ( v ^ 2 * , v 0 * ) = J 1 * ( v ^ 2 * , v ^ 0 * ) = inf v 2 * E * J 1 * ( v 2 * , v ^ 0 * ) .
Consequently, from this and the Min-Max Theorem, we obtain
J 1 * ( v ^ 2 * , v ^ 0 * ) = inf v 2 * E * sup v 0 * B * J 1 * ( v 2 * , v 0 * ) = sup v 0 * B * inf v 2 * E * J 1 * ( v 2 * , v 0 * ) .
Now we are going to show that
δ J ( u 0 ) = 0 .
From
J 1 * ( v ^ 2 * , v ^ 0 * ) v 2 * = 0 ,
we have
u 0 + v ^ 2 * K 2 = 0 ,
and thus
v ^ 2 * = K 2 u 0 .
Finally, denoting
D = γ 2 u 0 + 2 v ^ 0 * u 0 f ,
from
J 1 * ( v ^ 2 * , v ^ 0 * ) v 0 * = 0 ,
we have
2 D u 0 + u 0 2 v ^ 0 * α β = 0 ,
so that
v ^ 0 * = α ( u 0 2 β 2 D u 0 ) .
Observe now that
v ^ 2 * + K 1 ( γ 2 + 2 v ^ 0 * ) f = ( K 2 γ 2 + 2 v ^ 0 * + K 1 ( γ 2 + 2 v ^ 0 * ) 2 ) u 0
so that
K 2 u 0 2 v ^ 0 u 0 K u 0 + f = K 2 u 0 K u 0 γ 2 u 0 + K 1 ( γ 2 + 2 v ^ 0 * ) ( γ 2 u 0 + 2 v ^ 0 * u 0 f ) .
The solution for this last equation is obtained through the relation
γ 2 u 0 + 2 v ^ 0 * u 0 f = D = 0 ,
so that from this and (49), we get
v ^ 0 * = α ( u 0 2 β ) .
Thus,
δ J ( u 0 ) = γ 2 u 0 + 2 α ( u 0 2 β ) u 0 f = 0
and
δ J ( u 0 ) + K 1 2 Ω ( γ 2 u 0 + 2 v ^ 0 * u 0 f ) 2 d x = 0 ,
and hence, from the concerning convexity in u on V,
J ( u 0 ) = min u V J ( u ) + K 1 2 Ω ( γ 2 u + 2 v ^ 0 * u f ) 2 d x .
Moreover, from the Legendre transform properties
F 1 * ( v ^ 2 * , v ^ 0 * ) = u 0 , v ^ 2 * L 2 F 1 ( u 0 , v ^ 0 * ) ,
F 2 * ( v ^ 2 * ) = u 0 , v ^ 2 * L 2 F 2 ( u 0 ) ,
G * ( v ^ 0 * ) = u 0 2 , v ^ 0 * L 2 G ( u 0 2 ) ,
so that
J 1 * ( v ^ 2 * , v ^ 0 * ) = F 1 * ( v ^ 2 * , v ^ 0 * ) + F 2 * ( v ^ 2 * ) G * ( v ^ 0 * ) = F 1 ( u 0 , v ^ 0 * ) F 2 ( u 0 ) u 0 2 , v ^ 0 * L 2 + G ( u 0 2 ) = J ( u 0 ) .
Joining the pieces, we have got
J ( u 0 ) = inf u V 1 J ( u ) + K 1 2 Ω ( γ 2 u + 2 v ^ 0 * u f ) 2 d x = inf v 2 * E * sup v 0 * B * J 1 * ( v 2 * , v 0 * ) = J 1 * ( v ^ 2 * , v ^ 0 * ) .
The proof is complete.

9. One More Duality Principle Suitable for the Primal Formulation Global Optimization

In this section we establish one more duality principle and related convex dual formulation suitable for a global optimization of the primal variational formulation.
Let Ω R 3 be an open, bounded, connected set with a regular (Lipschitzian) boundary denoted by Ω .
For the primal formulation, we define V = W 0 1 , 2 ( Ω ) and consider a functional J : V R where
J ( u ) = γ 2 Ω u · u d x + α 2 Ω ( u 2 β ) 2 d x u , f L 2 .
Here we assume f L 2 ( Ω ) , and define Y = Y * = L 2 ( Ω )
V 2 = { u V : u K 3 } ,
A + = { u V : u f > 0 , a . e . in Ω } ,
and
V 1 * = A + V 1 ,
for an appropriate constant K 3 > 0 to be specified.
Define also the functionals F 1 : V R , F 2 : V × Y R and G : Y R by
F 1 ( u ) = K 2 2 Ω ( 2 u ) 2 d x u , f L 2 ,
F 2 ( u , v 3 * , v 0 * ) = γ 2 Ω u · u d x u 2 , v 0 * L 2 + K 2 2 Ω ( 2 u ) 2 d x K 1 2 Ω ( γ 1 2 u + 2 v 3 * u h 1 ) 2 d x ,
and
G ( u 2 ) = α 2 Ω ( u 2 β ) 2 d x ,
for appropriate positive constants K 1 , K 2 , K 3 to be specified.
Moreover, define F 1 * : Y * R , and F 2 * : [ Y * ] 2 R and G * : Y * R , by
F 1 * ( v 2 * ) = sup u V { u , v 2 * L 2 F 1 ( u ) } = 1 2 K 2 Ω ( v 2 * + f ) 2 4 d x ,
and
F 2 * ( v 2 * , v 3 * , v 0 * ) = sup u V { u , v 2 * L 2 F 2 ( u , v 3 * , v 0 * ) } = 1 2 Ω ( v 2 * + K 1 ( γ 1 2 + 2 v 3 * ) h 1 ) 2 K 2 4 + γ 2 2 v 0 * K 1 ( γ 1 2 + 2 v 3 * ) 2 K 1 2 Ω h 1 2 d x
for appropriate γ 1 > 0 and H 1 L 2 ( Ω ) , and
G * ( v 0 * ) = sup v Y { v , v 0 * L 2 G ( v ) } = 1 2 α Ω ( v 0 * ) 2 d x + β Ω v 0 * d x .
Furthermore, we define
D * = { v 2 * Y * : v 2 * ( 3 / 2 ) K 2 } ,
B * = v 3 * Y * : v 3 * K 4 ,
for an appropriate constant K 4 > 0 to be specified.
Define also
C 1 * = { v 0 * Y * : v 0 * K 4 } .
and J 1 * : D * × C 1 * R by
J 1 * ( v 2 * , v 3 * , v 0 * ) = F 1 * ( v 2 * ) + F 2 * ( v 2 * , v 3 * , v 0 * ) G * ( v 0 * ) .
Moreover, assuming K 2 K 1 K 4 max { 1 , K 3 , α , β , γ , γ 1 , f , h 1 } .
By directly computing δ 2 J 1 * ( v 2 * , v 3 * , v 0 * ) denoting
A = 2 K 1 h 1 ,
B = 4 K 1 ( γ 1 2 + 2 v 3 * ) ,
φ = K 2 4 γ 2 + 2 v 0 * + K 1 ( γ 1 2 + 2 v 3 * ) 2 ) ,
φ 1 = v 2 * K 1 ( γ 1 2 + 2 v 3 * ) h 1 ,
u = φ 1 φ ,
we may obtain, considering that φ < 0
2 J 1 * ( v 2 * , v 3 * , v 0 * ) ( v 3 * ) 2 = 4 K 1 u 2 ( A u B ) 2 φ > 0
on D * × B * .
Moreover,
2 J 1 * ( v 2 * , v 3 * , v 0 * ) ( v 2 * ) 2 2 J 1 * ( v 2 * , v 3 * , v 0 * ) ( v 3 * ) 2 2 J 1 * ( v 2 * , v 3 * , v 0 * ) v 2 * v 3 * 2 = O K 1 2 H 1 + K 1 H 2 K 2 φ ,
where
H 1 = ( 8 ( h 1 2 + 4 h 1 ( γ 1 2 + 2 v 3 * ) u 3 [ ( γ 1 2 + 2 v 3 * ) 2 u ] u ) ,
and
H 2 = [ ( γ 2 + 2 v 0 * ) u ] u .
At a critical point we have H 1 = 0 and
H 2 = f u 0 > 0 , a . e in Ω .
With such results, we may define the restrictions
C 2 * = { v 0 * Y * : H 1 ( v 2 * , v 3 * , v 0 * ) 0 , v 2 * D * , v 3 * B * } .
C 3 * = { v 0 * Y * : H 2 ( v 2 * , v 3 * , v 0 * ) 0 , v 2 * D * , v 3 * B * } .
Here, we define C * = C 1 * C 2 * C 3 * .
On the other hand, clearly we have
2 J 1 * ( v 2 * , v 3 * , v 0 * ) ( v 0 * ) 2 < 0
From such results, we may obtain that J 1 * in convex in ( v 2 * , v 3 * ) and it is concave in v 0 * on D * × B * × C * .

The Main Duality Principle and a Related Convex Dual Formulation

Considering the statements and definitions presented in the previous section, we may prove the following theorem.
Theorem 7.
Let ( v ^ 2 * , v ^ 3 * v ^ 0 * ) D * × B * × C * be such that
δ J 1 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) = 0
and u 0 V 1 be such that
u 0 = F 1 * ( v ^ 2 * ) v 2 * .
Assume also
u 0 0 , a . e . in Ω .
Under such hypotheses, we have
δ J ( u 0 ) = 0 ,
γ 1 2 u 0 + 2 v ^ 3 * u 0 h 1 = 0 ,
and
J ( u 0 ) = inf u V 1 J ( u ) = inf ( v 2 * , v 3 * ) D * × B * sup v 0 * C * J 1 * ( v 2 * , v 3 * , v 0 * ) = J 1 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) .
Proof. 
Observe that δ J 1 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) = 0 so that, since J 1 * is convex in ( v 2 * , v 3 * ) D * × B * × C * and
2 J 1 * ( v ^ 2 * , v ^ 3 * , v 0 * ) ( v 0 * ) 2 > 0 , v 0 * C 1 * ,
we obtain
J 1 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) = inf ( v 2 * , v 3 * ) D * × B * J 1 * ( v 2 * , v 3 * , v ^ 0 * ) sup v 0 * C * J 1 * ( v ^ 2 * , v ^ 3 * , v 0 * ) .
Consequently, from this and the Saddle Point Theorem, we obtain
J 1 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) = inf ( v 2 * , v 3 * ) D * × B * sup v 0 * C * J 1 * ( v 2 * , v 3 * , v 0 * ) .
Now we are going to show that
δ J ( u 0 ) = 0 .
From
J 1 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) v 2 * = 0 ,
and
F 1 * ( v ^ 2 * ) v 2 * = u 0
we have
F 2 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) v 2 * u 0 = 0
and
v ^ 2 * = K 2 4 u 0 f .
Observe now that
F 2 * ( v ^ 2 * , v ^ 3 * , v 0 * ) = sup u V { u , v 2 * L 2 F 2 ( u , v 3 * , v 0 * ) } .
Denoting
H ( v 2 * , v 3 * , v ) * , u ) = u , v 2 * L 2 F 2 ( u , v 3 * , v 0 * ) ,
there exists u ^ V such that
H ( v ^ 2 * , v ^ 3 * , v ^ 0 * , u ^ ) u = 0 ,
and
F 2 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) = H ( v ^ 2 * , v ^ 3 * , v ^ 0 * , u ^ ) ,
so that
F 2 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) v 2 * = H ( v ^ 2 * , v ^ 3 * , v ^ 0 * , u ^ ) v 2 * + H ( v ^ 2 * , v ^ 3 * , v ^ 0 * , u ^ ) u u ^ v 2 * = u ^ .
Summarizing, we have got
u 0 = F 2 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) v 2 * = u ^ .
From such results and the Legendre tranform proprieties we get
v 2 * = F 1 ( u 0 ) u
and
v 2 * = F 2 ( u 0 , v ^ 3 * , v ^ 0 * ) u .
On the other hand, from the variation of J 1 * in v 3 * , we have
F 2 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) v 3 * = K 1 ( γ 1 2 u 0 + 2 v ^ 3 * u 0 h 1 ) 2 u 0 + H ( v ^ 2 * , v ^ 3 * , v ^ 0 * , u ^ ) u u ^ v 3 * = K 1 ( γ 1 2 u 0 + 2 v ^ 3 * u 0 h 1 ) 2 u 0 = 0 .
From such results, since
u 0 0 , a . e . in Ω ,
we get
γ 1 2 u 0 + 2 v ^ 3 * u 0 h 1 = 0 , a . e . in Ω .
Finally, from the variation of J 1 * in v 0 * we obtain
F 2 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) v 0 * G * ( v 0 * ) v 0 * = 0 ,
so that
u 0 2 + H ( v ^ 2 * , v ^ 3 * , v ^ 0 * , u ^ ) u u ^ v 0 * v 0 * α β = 0 .
Thus,
v 0 * = α ( u 0 2 β ) .
Consequently, from such last results, we have
0 = v ^ 2 * v ^ 2 * = F 1 ( u 0 ) u F 2 ( u 0 , v ^ 3 * , v ^ 0 * ) u = K 2 4 u 0 f K 2 4 u 0 γ 2 u 0 + 2 v 0 * u 0 = γ 2 u 0 + 2 α ( u 0 2 β ) u 0 f = δ J ( u 0 ) .
Summarizing,
δ J ( u 0 ) = 0 .
Furthermore, also from such last results and the Legendre transform properties, we have
F 1 * ( v ^ 2 * ) = u 0 , v ^ 2 * L 2 F 1 ( u 0 ) ,
F 2 * ( v ^ 2 * , v ^ 3 * v ^ 0 * ) = u 0 , v ^ 2 * L 2 F 2 ( u 0 , v ^ 3 * , v ^ 0 * ) ,
G * ( v ^ 0 * ) = u 0 2 , v 0 * L 2 G ( u 0 2 ) ,
so that
J 1 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) = F 1 * ( v ^ 2 * ) + F 2 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) G * ( v ^ 0 * ) = J ( u 0 ) .
Finally, observe that
J 1 * ( v 2 * , v 3 * , v 0 * ) F 1 ( u ) u , v 2 * L 2 + F 2 * ( v 2 * , v 3 * , v 0 * ) G * ( v 0 * ) ,
u V 1 , v 2 * D * , v 3 * B * , v 0 * C * .
Therefore,
sup v 0 * C * J 1 * ( v 2 * , v 3 * , v 0 * ) sup v 0 * C 1 * { u , v 2 * L 2 + F 1 ( u ) + F 2 * ( v 2 * , v 3 * , v 0 * ) G * ( v 0 * ) } ,
so that
inf ( v 2 * , v 3 * ) D * × B * sup v 0 * C * J 1 * ( v 2 * , v 3 * , v 0 * ) inf ( v 2 * , v 3 * ) D * × B * sup v 0 * C 1 * { u , v 2 * L 2 + F 1 ( u ) + F 2 * ( v 2 * , v 3 * , v 0 * ) G * ( v 0 * ) } = J ( u ) , u V 1 .
Summarizing, we have got
J 1 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) = inf ( v 2 * , v 3 * ) D * × B * sup v 0 * C * J 1 * ( v 2 * , v 3 * , v 0 * ) inf u V 1 J ( u ) .
Joining the pieces, we have got
J ( u 0 ) = inf u V 1 J ( u ) = inf ( v 2 * , v 3 * ) D * × B * sup v 0 * C * J 1 * ( v 2 * , v 3 * , v 0 * ) = J 1 * ( v ^ 2 * , v ^ 3 * , v ^ 0 * ) .
The proof is complete.

11. Conclusions

In the first part of this article we develop duality principles for non-convex variational optimization. In the final concerning sections we propose dual convex formulations suitable for a large class of models in physics and engineering. In the last article section, we present an advance concerning the computation of a solution for a partial differential equation through the generalized method of lines. In particular, in its previous versions, we used to truncate the series in d 2 however, we have realized the results are much better by taking line solutions in series for u f [ x ] and its derivatives, as it is indicated in the present software.
This is a little difference concerning the previous procedure, but with a great result improvement as the parameter ε > 0 is small.
Indeed, with a sufficiently large N (number of lines), we may obtain very good qualitative results even as ε > 0 is very small.

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