Abstract
We consider polyconvex functionals of the Calculus of Variations defined on maps from the three-dimensional Euclidean space into itself. Counterexamples show that minimizers need not to be bounded. We find conditions on the structure of the functional, which force minimizers to be locally bounded.
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1 Introduction
Let us consider polyconvex integrals of the Calculus of Variations. Partial regularity results (that is, the regularity of minimizers up to a subset of the set of definition and the study of the properties of the singular set; see for example Section 4.2 in [1] and Section 1 in [2]) are contained in [3,4,5,6,7,8,9,10]. Only few everywhere regularity results are available: [11] where the everywhere continuity is proved in the two-dimensional case, [12] where Hölder continuity for extremals is dealt with in dimension two, [13] where local boundedness is proved in the three-dimensional case. Global pointwise bounds are in [14,15,16,17,18,19]. Interesting results are contained in [20,21,22,23,24,25]; see also [26, 27]. Let us come back to [13]; in such a paper, the authors make an important step toward regularity: they prove boundedness of minimizers in the three-dimensional case; unfortunately, they make restrictions that rule out the most important polyconvex integral. In the present paper, we find a different set of assumptions, which allows us to deal with such a polyconvex integral. In the next section, we write assumptions and results; in Sect. 3 we collect some preliminaries and, in Sect. 4, we give the proof of the main theorem.
2 Assumptions and Results
In this paper we study the regularity of vectorial local minimizers of integral functionals
where \(\varOmega \subset {\mathbb {R}}^3\) is an open, bounded set, \(v:\varOmega \subset {\mathbb {R}}^3 \rightarrow {\mathbb {R}}^3\), \(v=(v^1, v^2, v^3)\) and Dv is the Jacobian matrix of its partial derivatives
moreover, \(f: \varOmega \times {\mathbb {R}}^{3\times 3} \rightarrow [0, +\infty [\) is a Carathéodory function such that for fixed x
that is
see [28, 29]. When dealing with models in nonlinear elasticity, f is the stored-energy function; moreover, \(\xi , \text{ adj }_2 \xi , \text{ det }\xi \) govern the deformation of line, surface and volume elements respectively. Our model is
where \(\det Dv\) is the determinant of the matrix Dv, and \(\text{ adj }_2 Dv\) denotes the adjugate matrix of order 2, whose components are
with \(\alpha ,\beta \in \{1,2,3\}\setminus \{i\}\), \(\alpha <\beta \), and \(k,\ell \in \{1,2,3\} \setminus \{j\}\), \(k<\ell \). Moreover, \((\text{ adj }_2 Dv)^\alpha \) denotes the \(\alpha -\)row of \(\text{ adj }_2 Dv\), that is
In paper [13], the authors consider densities f for which the following splitting holds true
for suitable nonnegative functions \(F^\alpha , G^\beta , H\). Note that model (3), with \(p \ne 2\), cannot be written as (4); see Lemma A.1 in “Appendix A”. In this paper, we succeed in dealing with model (3) and we prove the following
Theorem 2.1
Let \(\varOmega \) be a bounded and open subset of \({\mathbb {R}}^3\). Assume that \(1\le r< q < p \le 3\) with \(2<p\) and
then all the local minimizers \(u\in W_{loc} ^{1,p} (\varOmega ; {\mathbb {R}}^3)\) of
are locally bounded in \(\varOmega \).
We recall that \(p^*\) is the Sobolev exponent: \(p^* = \frac{n p}{n-p}= \frac{3p}{3-p}\) when \(p<n=3\); moreover, \(p^*\) is any number greater than p when \(p=n=3\), so it can be chosen large enough that (5) is satisfied by assuming only \(1 \le r< q < p\). We notice that we have restricted ourselves to the case \(p\le 3\) because, when \(p>3\), every function in \(W_{loc}^{1,p} (\varOmega )\) is trivially in \(L_{loc}^\infty (\varOmega )\) by the Sobolev theorem. Note that we have existence of minimizers for (6) when \(2 \le p\), \(\frac{p}{p-1} \le q\) and \(1<r\), provided a boundary datum \({\overline{u}} \in W^{1,p}(\varOmega ; {\mathbb {R}}^3)\), with finite energy, has been fixed; see Remark 8.32 (iii) in [29] and Theorem 3.1 in [13]. Condition (5) is satisfied, for example, when \(p=\frac{14}{5}\), \(q=2\), \(r=\frac{3}{2}\) and this gives us the following.
Corollary 2.1
Let \(\varOmega \) be a bounded and open subset of \({\mathbb {R}}^3\) and let \(u\in W_{loc} ^{1,\frac{14}{5}} (\varOmega ; {\mathbb {R}}^3)\) be a local minimizer of
then u is locally bounded in \(\varOmega \).
In the framework of Corollary 2.1, we have \(\frac{p}{p-1}=\frac{14}{9} < 2 = q\), so the existence of minimizers is guaranteed as in the previous lines. Theorem 2.1 is a particular case of a more general result. Let us note that model (3) suggests we assume the following structure
where F, G and H are Carathéodory nonnegative functions. We assume p-growth with respect to \(\xi \), q-growth with respect to \(\text{ adj }_2\xi \) and r-growth with respect to \(\text{ det }\xi \)
where \(k_1\), \(k_2\), \(k_3\) are constants such that \(k_1, k_3 \in ]0, +\infty [\) and \(k_2 \in [0, +\infty [\) and \(a, b, c:\varOmega \rightarrow [0, +\infty [\) are functions in \(L^\sigma (\varOmega )\), \(\sigma > 1\); as far as exponents p, q, r are concerned, we assume that \(2 < p \le 3\) and \(1 \le r< q < p\). Now we need to control the behavior of F with respect to the sum from below
A weaker condition is needed for G:
We also need to control the behavior of F with respect to the sum from above:
Note that in (14) there is an extra term with the product between \(t_1\) and \(t_2\). When \(q > 2\) we assume
When \(q \le 2\) we do not need the product between \(t_1\) and \(t_2\) any longer; we require subadditivity
Functions F verifying the previous assumptions are \(F(x,t) = \gamma (x) t^{p/2}\) and \(F(x,t) = \gamma (x) (1 + t^2)^{p/4}\), provided \(\gamma (x)\) is positive and away from both 0 and \(+\infty \); similar examples for G and H: see Remarks 3.2, \(\ldots \), 3.7. Our main result is the following
Theorem 2.2
Let \(\varOmega \) be a bounded and open subset of \({\mathbb {R}}^3\) and let f be as in (8); assume that conditions (9)–(16) hold with \(1\le r< q < p \le 3\) such that \(2<p\) and
Then, all the local minimizers \(u\in W_{loc} ^{1,p} (\varOmega ; {\mathbb {R}}^3)\) of I are locally bounded in \(\varOmega \).
Note that \(\frac{1}{\sigma } = 0\), if \(\sigma = \infty \). In our Theorem 2.2, we assume (8); in [13] (4) was in force: in vectorial problems, some structure conditions are due to minimizers which can be unbounded: see De Giorgi’s counterexample [30]; see also [31], Section 3 in [1] and [32]. As far as exponents p, q, r are concerned, (17) is the same as (2.5) in [13] when \(1<q\le 2\); if \(2<q\) then (17) seems to require a bit more than (2.5) in [13]: see comparison (72).
The integrals we consider show a \({\tilde{p}}\) growth from below and a \({\tilde{q}}\) growth from above, so we are in the class of functionals with \({\tilde{p}},{\tilde{q}}\)-growth. It is now well known, as in our result, that a restriction between \({\tilde{p}}\) and \({\tilde{q}}\) must be imposed due to counterexamples in [33,34,35,36,37]; see also [38, 39]; we refer to [1] for a detailed survey on the subject.
3 Preliminaries
In this section, we recall some standard definitions and collect several lemmas useful in our proofs.
First of all, we recall the following
Definition 3.1
A function \(u\in W_{loc} ^{1,1} (\varOmega ; {\mathbb {R}}^3)\) is a local minimizer of (1) if \(f(Du) \in L^1 _{loc} (\varOmega )\) and
for all \(\varphi \in W^{1,1} (\varOmega , {\mathbb {R}}^3)\) with \(\text{ supp } \, \varphi \subset \subset \varOmega \).
All the norms we use on \({\mathbb {R}}^3\) and \({\mathbb {R}}^{3\times 3}\) will be the standard Euclidean ones and denoted by \(| \cdot |\) in all cases. In particular, for matrices \(\xi , \eta \in {\mathbb {R}}^{3\times 3}\) we write \(\langle \xi , \eta \rangle : = \text {trace} (\xi ^T \eta )\) for the usual inner product of \(\xi \) and \(\eta \), and \(| \xi | : = \langle \xi , \xi \rangle ^{\frac{1}{2}}\) for the corresponding Euclidean norm.
Lemma 3.1
For \(a, b\ge 0\) we have that
Proof
When \(m=1\), (19) and (20) are easy. We are left with the case \(1<m\). It is obvious that (19) and (20) hold true both for \(b=0\). We now assume \(b>0\) and we let \(t=a/b\). It suffices to show that for \(t\ge 0\),
In order to prove (21), we let \(h(t) =(t+1)^m- t^m-1 \). Since
and, by \(m>1\),
then \(h(t)\ge 0\) and (21) follows.
Regarding (22), we let \(g(t) =(t+1)^m- t^m-mt-1 \). Since
where we used \(1<m\le 2\) and Remark 3.1, then (22) follows. \(\square \)
Remark 3.1
We recall the well-known inequality: for \(a, b \ge 0\) we have
Lemma 3.2
Fix \(m \in [-\frac{1}{2}, +\infty [\) and consider \(V:{\mathbb {R}} \rightarrow {\mathbb {R}}\) as follows
then, \(V:{\mathbb {R}} \rightarrow {\mathbb {R}}\) is strictly increasing.
Proof
We compute the first derivative
since \(m \ge -\frac{1}{2}\), we have \(V^{\prime }(s) > 0\) for every \(s \in {\mathbb {R}}\). This ends the proof. \(\square \)
Lemma 3.3
Fix \(p \in [2, +\infty [\); consider \(w:{\mathbb {R}}^2 \rightarrow {\mathbb {R}}\) as follows
Then,
Proof
We compute the first partial derivatives:
and
where V is given by (28) with \(m = (p/4) - 1\). Note that \(m \ge - 1/2\) since \(p \ge 2\). Then, V is increasing so that, when \(a\ge 0\) and \(b \ge 0\), we have \(V(a + b) - V(a) \ge 0\) and \(V(a + b) - V(b) \ge 0\). This shows that
Then, \(a \rightarrow w(a,b)\) increases and \(b \rightarrow w(a,b)\) increases too, if we restrict ourselves to \(a \ge 0\) and \(b \ge 0\); thus,
provided \(b \ge 0\) and \(a \ge 0\). This ends the proof. \(\square \)
Corollary 3.1
Fix \(p \in [2, +\infty [\); then,
Proof
We write (31) explicitly and we get (34). \(\square \)
Lemma 3.4
Fix \(p \in ]2, 3]\). If \(a \ge 0\) and \(b \ge 0\), then
Proof
Since \(p \in ]2, 3]\) we have \(\frac{p}{4} \in ]\frac{1}{2}, \frac{3}{4}]\) and we can use (27) with \(m = \frac{p}{4}\):
now \(\frac{p}{2} \in ]1, \frac{3}{2}]\) and we can use (20) with \(m = \frac{p}{2}\):
This ends the proof. \(\square \)
Lemma 3.5
Fix \(q \in ]1, 2]\). Then,
Proof
Since \(q \in ]1, 2]\) we have \(\frac{q}{4} \in ]\frac{1}{4}, \frac{1}{2}]\) and we can use (27) with \(m = \frac{q}{4}\):
now \(\frac{q}{2} \in ]\frac{1}{2}, 1]\) and we can use (27) with \(m = \frac{q}{2}\):
This ends the proof. \(\square \)
Now we are able to give examples of functions F, G, H verifying conditions required in Theorem 2.2.
Remark 3.2
Fix \(p \in ]2,3]\) and define
for \(t \in [0, +\infty [\), where \(\gamma _1 \le \gamma (x) \le \gamma _2\) with \(\gamma _1, \gamma _2 \in ]0, +\infty [\). Then (9), (12), (14) hold true with \(k_1 = \gamma _1\), \(k_2 = 0\), \(k_3 = \frac{p}{2} \gamma _2\), \(a(x) = 0\). Indeed, we use (19) and (20) with \(m = p/2\) in Lemma 3.1 and we are done.
Remark 3.3
Fix \(q \in ]1,3[\) and define
for \(t \in [0, +\infty [\), where \(\gamma _1 \le \gamma (x) \le \gamma _2\) with \(\gamma _1, \gamma _2 \in ]0, +\infty [\). Then, when \(q>2\), (10), (13), (15) hold true with \(k_1 = \gamma _1\), \(k_2 = 0\), \(k_3 = \frac{q}{2} \gamma _2\), \(b(x) = 0\). Indeed, we use (20) with \(m = q/2\) in Lemma 3.1 and we are done. Moreover, when \(q \le 2\), (10), (13), (16) hold true with \(k_1 = \gamma _1\), \(k_2 = 0\), \(k_3 = \gamma _2\), \(b(x) = 0\). Indeed, when \(q \le 2\), we use the well-known inequality (27) with \(m = q/2\) and we are done.
Remark 3.4
Fix \(r \in [1,3[\) and define
for \(s \in {\mathbb {R}}\), where \(\gamma _1 \le \gamma (x) \le \gamma _2\) with \(\gamma _1, \gamma _2 \in ]0, +\infty [\). Then, (11) holds true with \(k_3 = \gamma _2\), \(c(x) = 0\).
Remark 3.5
Fix \(p \in ]2,3]\) and define
for \(t \in [0, +\infty [\), where \(\gamma _1 \le \gamma (x) \le \gamma _2\) with \(\gamma _1, \gamma _2 \in ]0, +\infty [\). Then (9), (12), (14) hold true with \(k_1 = \gamma _1\), \(k_2 = \gamma _2\), \(k_3 = \frac{p}{2} \gamma _2\), \(a(x) = \gamma _2\). Indeed, we use (27) with \(m = p/4\), (34) and (35).
Remark 3.6
Fix \(q \in ]1,3[\) and define
for \(t \in [0, +\infty [\), where \(\gamma _1 \le \gamma (x) \le \gamma _2\) with \(\gamma _1, \gamma _2 \in ]0, +\infty [\). Then, when \(q>2\), (10), (13), (15) hold true with \(k_1 = \gamma _1\), \(k_2 = 0\), \(k_3 = \frac{q}{2} \gamma _2\), \(b(x) = \gamma _2\). Indeed, we use (27) with \(m = q/4\), (35) and we are done. Moreover, when \(q \le 2\), (10), (13), (16) hold true with \(k_1 = \gamma _1\), \(k_2 = 0\), \(k_3 = \gamma _2\), \(b(x) = \gamma _2\). Indeed, when \(q \le 2\), we use (27) with \(m = q/4\), (38) and we are done.
Remark 3.7
Fix \(r \in [1,3[\) and define
for \(s \in {\mathbb {R}}\), where \(\gamma _1 \le \gamma (x) \le \gamma _2\) with \(\gamma _1, \gamma _2 \in ]0, +\infty [\). Then, (11) holds true with \(k_3 = 2^{r/2} \gamma _2\), \(c(x) = 2^{r/2} \gamma _2\).
The following lemma can be found in [13] as Lemma 4.1.
Lemma 3.6
Consider the matrices \(A,B \in {\mathbb {R}} ^{3\times 3}\):
Then, the following estimates hold:
- (a):
-
\(|A|\le |A^1|+|B^2| +|B^3|\),
- (b):
-
\(|\det A| \le |A^1| |({\mathrm{adj}_2 B})^1|\),
- (c):
-
\(|(\mathrm{adj}_2 A)_{2j}| \le |A^1| |B^3|\) and \(|(\mathrm{adj}_2 A)_{3j}| \le |A^1| |B^2|\), for all \(j\in \{ 1,2,3\}\).
In order to get our main result, we have to prove a suitable Caccioppoli-type inequality for any component \(u^\alpha \) of the local minimizer u of functional I (1) on every superlevel set \(\{u^\alpha >k\}\). To this goal, we will use the following lemma (see [13] for a proof).
Lemma 3.7
Let \(\varOmega \) be an open subset of \({\mathbb {R}}^3\). Consider a Carathéodory function \(f: \varOmega \times {\mathbb {R}}^{3\times 3} \rightarrow [0,+\infty [ \). Assume that there exist \(c_1,c_3>0\) and \(c_2\ge 0\) such that, for every \(\xi \in {\mathbb {R}}^{3\times 3}\),
with \(1\le p, 1\le q, 1\le r, \omega (x) \ge 0\).
Let \(u\in W_{loc}^{1,p} (\varOmega ; {\mathbb {R}}^3)\) be such that \(x\rightarrow f(x,Du(x)) \in L_{loc} ^1 (\varOmega )\). Fix \(\eta \in C_0 ^1 (\varOmega )\), \(\eta \ge 0\) and \(k\in {\mathbb {R}}\), and denote, for almost every \(x\in \{u^1>k\} \cap \{\eta >0\}\),
If
and \(\omega \in L_{loc} ^1 (\varOmega )\), then
4 Proof of Theorem 2.2
We want to stress that the proof of our result follows the idea used in [13]: we provide the local boundedness of the minimizers by proving that each component is locally bounded. In the following lemma, we refer to the first component \(u^1\): the core of the proof lies in the following Caccioppoli-type inequality, obtained on every superlevel set \(\{u^1 > k \}\). We keep in mind that \(p^* = \frac{np}{n-p}\) if \(p<n=3\) and \(p^*\) is any number \(>p\) when \(p=n=3\).
Proposition 4.1
(Caccioppoli-type estimate) Let f be as in (8) satisfying (9)–(16) with \(1\le r< q < p \le 3\) such that
Let \(u\in W_{loc}^{1,p} (\varOmega ; {\mathbb {R}}^3)\) be a local minimizer of I. Let \(B_R(x_0) \subset \subset \varOmega \) with \(|B_R(x_0)|<1\); fixed \(k\in {\mathbb {R}}\), denote
Then, there exists \(C =C(k_1, k_2, k_3, p, q, r, p^*)>0\) such that, for every \(0<s<t\le R\):
where
with \(\frac{1}{\sigma } = 0\) if \(\sigma = \infty \).
Proof
The condition \(|B_R(x_0)|=\frac{4\pi R^3}{3} <1\) ensures \(R<1\). Let s, t be such that \(0<s<t\le R\). Consider a cutoff function \(\eta \in C_0^\infty (B_t(x_0))\) satisfying the following assumptions:
Fixing \(k\in {\mathbb {R}}\), define \(w \in W_{loc} ^{1,p} (\varOmega ; {\mathbb {R}}^3)\),
and, for \(\mu = p^*\),
For almost every \(x \in \varOmega \setminus (\{\eta>0\} \cap \{u^1>k\})\) we have \(\varphi =0\), thus
almost everywhere in \(\varOmega \setminus ({\{\eta>0\} \cap \{u^1>k\}} )\).
For almost every \(x\in \{\eta>0\} \cap \{u^1>k\}\) denote
We notice that
Moreover, since for almost every \(x\in \{\eta>0\} \cap \{u^1>k\}\),
and
then, since f is polyconvex, we get that
almost everywhere in \(\{\eta>0\} \cap \{u^1>k\}\).
By the minimality of u, \(f(x,Du) \in L_{loc} ^1 (\varOmega )\); note that in our case we can use Lemma 3.7, deducing that
Therefore, (49) and (51) imply \(f(x,Du+D\varphi ) \in L_{loc}^1 (\varOmega )\).
By the local minimality of u, (49) and (51), recalling that \( A_{k,t} ^1 \) is the set \(\{ x \in B_t (x_0): u^1(x) >k\}\), we have
The inequality above implies
Taking into account the expression of f (see (8)), we obtain from the above inequality that
Denote \({{\tilde{u}}} =(u^2, u^3)\) and
We have
we use (12) with \(t_1=|Du^1|^2\) and \(t_2=|D{\widetilde{u}}|^2\), so that
Note that
by using (14) with \(t_1=|A^1|^2\) and \(t_2=|D{\widetilde{u}}|^2\), we obtain
Furthermore, setting
and noticing
we can write
Applying (13) with \(t_1=|(\text{ adj }_2 Du)^1|^2\) and \(t_2=|{{\tilde{A}}}|^2\), we get
Assumption (15) when \(q> 2\) or (16) when \(q\le 2\), with \(t_1=|\tilde{{\tilde{A}}}|^2\) and \(t_2=|(\text{ adj }_2 Du)^1|^2\), yields
By virtue of (53),(54), (56) and (57), from (52), we get
and then
In order to estimate the first two terms on the right-hand side of (58), we recall that \(\mu = p^*>p\) and
By using the right-hand side of (9) and the fact \(z^p \le 1+z^{p^*} \) if \(z\ge 0\), we obtain
We will write \(d'\) to denote the Hölder conjugate of \(d>1\): \(d'=\frac{d}{d-1}\). Regarding the second term on the right-hand side in (58), notice that
we use Young inequality with \(\frac{p^*}{2}\), \(\left( \frac{p^*}{2}\right) '\) and Hölder inequality with \(\frac{p}{(p-2) \left( \frac{p^*}{2} \right) ' }\), \(\frac{p}{p-(p-2) \left( \frac{p^*}{2} \right) ' }\):
Now we estimate the fourth term in (58). By using (10), (55), Lemma 3.6-(c) and Young inequality with exponents \(\frac{p^*}{q}\) and \(( \frac{p^*}{q})'\), we estimate
Note that \(q( \frac{p^*}{q})'<p\) when \(q<\frac{pp^*}{p+p^*}\) and \(\frac{pp^*}{p+p^*}>1\) if \(p> \frac{2n}{n+1}\).
Moreover, Hölder inequality, with \( \frac{p }{q} \Big / \left( \frac{p^*}{q}\right) ' \) and \(\left( \frac{p }{q} \Big / \left( \frac{p^*}{q}\right) '\right) ' \), yields
therefore, if we note that \((\frac{p^*}{q})' = \frac{p^*}{p^* - q}\), we have
Eventually, if \(q>2\), we have to estimate the sixth term in (58) and we use Lemma 3.6-(c) and Young inequality with exponents \(\frac{p^*}{2}\) and \(\left( \frac{p^*}{2} \right) '\), so having
Observe that \(2< q < \frac{p p^*}{p + p^*}\) implies \(p > \frac{12}{5}\); so we have \(2\left( \frac{p^*}{2} \right) '<p\) and we apply Hölder inequality with exponents \(\frac{p}{2\left( \frac{p^*}{2} \right) '}\) and \(\left( \frac{p}{2\left( \frac{p^*}{2} \right) '}\right) '\),
Furthermore, if \({(q-2)\left( \frac{p^*}{2} \right) '\left( \frac{p}{2\left( \frac{p^*}{2} \right) '}\right) '} <q\), we apply Hölder inequality again with exponents \(\frac{q}{{(q-2)\left( \frac{p^*}{2} \right) '\left( \frac{p}{2\left( \frac{p^*}{2} \right) '}\right) '}}\) and its conjugate:
Therefore, by (64) and (65), (63) becomes
Please, note that the previous condition \({(q-2)\left( \frac{p^*}{2} \right) '\left( \frac{p}{2\left( \frac{p^*}{2} \right) '}\right) '} <q\) means \(q < \frac{p p^*}{p + p^*}\). Finally, r-growth assumption (11) on H(x, .) yields
We compute \(\det A\) with respect to the first row, see Lemma 3.6-(b),
Notice that \(r<p< p^*\) and \(\frac{rp^*}{p^*-r} <q\). By the Young inequality with exponents \(\frac{p^*}{r}\) and \(\frac{p^*}{p^*-r}\), one has
Hölder inequality with \(\frac{q}{\frac{rp^*}{p^*-r} }\) and \(\frac{q}{q- \frac{rp^*}{p^*-r} }\) leads to
Therefore, (67) and (68) imply
By left-hand side inequalities in (9) and (11), using (58), (59), (60), (62), (66) and (69), we conclude
where
and \(C=C(k_1, k_2, k_3, p, q, r, p^*)>0\); moreover, \(1_E(q) = 1\) if \(q \in E\) and \(1_E(q) = 0\) if \(q \notin E\). Now we note that
where the last inequality is granted since \(q \mapsto 1- \frac{q p^*}{p(p^* - q)}\) decreases. Then,
Note that \(\left( \frac{p^*}{2}\right) ' = \frac{p^*}{p^* - 2}\); then, the exponents in (70) can be written as follows
so that (70) turns out to be
where
If \(2< q < \frac{p p^*}{p + p^*}\), we have
and
This ends the proof of Proposition 4.1. \(\square \)
We now proceed with the proof of Theorem 2.2. We fix \(x_0 \in \varOmega \) and \(R_0 < \min \{ \text {dist}(x_0, \partial \varOmega ), \left( \frac{3}{4 \pi } \right) ^{1/3} \}\) such that
where \(B_{\rho }\) is the ball centered at \(x_0\) with radius \(\rho \). Note that \(R_0 < 1\), \(|B_{R_0}| < 1\) and \(B_{R_0} \subset \subset \varOmega \). For every \(R \in (0, R_0]\) we define the decreasing sequence of radii
Fix a positive constant \(d \ge 1\) and define the increasing sequence of positive levels
We define the “excess”
We use our Caccioppoli inequality (48) and Proposition 2.4 of [13]: we get
where the positive constant c is independent of h. See also [40, 41]. Assumption (17) tells us that \(\theta \frac{p^*}{p}>1\); then, we can use Lemma 2.5 of [13] with \(\gamma : = \theta \frac{p^*}{p} - 1\), see also [42]:
provided
Note that
then, we can choose \(d \ge 1\) large enough so that (75) holds true. Thus, we have (74) with \(\gamma > 0\), so that \(J_h \rightarrow 0\) as \(h \rightarrow +\infty \); since \(\frac{R}{2} < \rho _h\) and \(k_h < d\), we also have
then,
so that \(u^1 \le d\) almost everywhere in \(B_{\frac{R}{2}}\). We have proved that \(u^1\) is locally bounded from above. In order to prove that \(u^1\) is locally bounded from below, we note that \(-u\) locally minimizes \(\int _{\varOmega } {\tilde{f}}(x,Dz(x)) \hbox {d}x\), where \({\tilde{f}}(x,\xi ) = f(x,-\xi )\); then, we get that \(-u^1\) is locally bounded from above, so \(u^1\) is locally bounded from below. We have just shown that \(u^1 \in L^{\infty }_{\text {loc}}(\varOmega )\).
Now we turn our attention to the second component \(u^2\). We change the order of the two components \(u^1\) and \(u^2\): we get a new function v as follows:
then,
and \(\det Dv = - \det Du\); moreover \((\text {adj}_2 Dv)^1 = - (\text {adj}_2 Du)^2\), \((\text {adj}_2 Dv)^2 = - (\text {adj}_2 Du)^1\) and \((\text {adj}_2 Dv)^3 = - (\text {adj}_2 Du)^3\), so that
If we write \(C_{1,2}(\xi )\) to denote the matrix obtained from \(\xi \) by inverting line 1 and line 2, we have \(Dv = C_{1,2}(Du)\) and \(\text {adj}_2 Dv = - C_{1,2} (\text {adj}_2 Du)\). Then, v is a local minimizer of \(\int _{\varOmega } \tilde{{\tilde{f}}}(x,Dw(x)) dx\), where \(\tilde{{\tilde{f}}}(x,\xi ) = f(x, C_{1,2}(\xi ))\). Thus, the first component \(v^1\) is locally bounded: \(u^2 = v^1 \in L^{\infty }_{\text {loc}}(\varOmega )\). In a similar way we deal with the third component \(u^3\): we change the order of the two components \(u^1\) and \(u^3\); we get a new function w as follows:
then,
and \(\det Dw = - \det Du\); moreover \((\text {adj}_2 Dw)^1 = - (\text {adj}_2 Du)^3\), \((\text {adj}_2 Dw)^2 = - (\text {adj}_2 Du)^2\) and \((\text {adj}_2 Dw)^3 = - (\text {adj}_2 Du)^1\), so that
If we write \(C_{1,3}(\xi )\) to denote the matrix obtained from \(\xi \) by inverting line 1 and line 3, we have \(Dw = C_{1,3}(Du)\) and \(\text {adj}_2 Dw = - C_{1,3} (\text {adj}_2 Du)\). Then, w is a local minimizer of \(\int _{\varOmega } \tilde{\tilde{{\tilde{f}}}}(x,Dz(x)) dx\), where \(\tilde{\tilde{{\tilde{f}}}}(x,\xi ) = f(x, C_{1,3}(\xi ))\). Thus, the first component \(w^1\) is locally bounded: \(u^3 = w^1 \in L^{\infty }_{\text {loc}}(\varOmega )\). This ends the proof of Theorem 2.2. \(\square \)
5 Conclusions
We have been able to prove boundedness for minimizers of the most important three-dimensional polyconvex integral, provided the growth exponents verify some restrictions. It would be interesting to understand what happens when such restrictions are not in force.
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Acknowledgements
We thank the referee for carefully reading the manuscript and for the useful remarks. M. Carozza, R. Giova and F. Leonetti have been supported by the Gruppo Nazionale per l’Analisi Matematica, la Probabilità e le loro Applicazioni (GNAMPA) of the Istituto Nazionale di Alta Matematica (INdAM). H. Gao thanks NSFC (10371050) and NSF of Hebei Province (A2015201149) for their support. R. Giova has been partially supported by Universitá degli Studi di Napoli “Parthenope” through the Project “Sostegno alla ricerca individuale (annualitá 2015-2016-2017)” and the Project “Sostenibilità, esternalità e uso efficiente delle risorse ambientali”(triennio 2017-2019). F. Leonetti acknowledges also the support of UNIVAQ.
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Appendix: Comparison Between Two Structures
Appendix: Comparison Between Two Structures
Lemma A.1
We assume that \(F^{\alpha }, G^{\alpha }: {\mathbb {R}}^3 \mapsto [0, +\infty [\) and \(H:{\mathbb {R}} \mapsto [0, +\infty [\); let \(p, q, r \in ]0, +\infty [\) with \(p \ne 2\). Then, it is false that
for every \(\xi \in {\mathbb {R}}^{3 \times 3}\).
Proof
We argue by contradiction: if (76) holds true, then we can use (76) with
and we get
with \(\det \xi = 0\), so that
we keep in mind that \(F^{\alpha }, G^{\alpha }, H \ge 0\) and we get
for every \(\alpha = 1, 2, 3\). Now we use (76) with
and we get
with \(\det \xi = 0\), so that
we keep in mind (80) and we get
for every \(t \in {\mathbb {R}}\). In a similar manner, taking
we get
for every \(t \in {\mathbb {R}}\). In the same way, taking
we get
for every \(t \in {\mathbb {R}}\). Eventually, we take
and (76) implies
we use (80), (84), (86), (88) and we get
such an equality is a contradiction, since \(p \ne 2\). This ends the proof of Lemma A.1.
\(\square \)
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Carozza, M., Gao, H., Giova, R. et al. A Boundedness Result for Minimizers of Some Polyconvex Integrals. J Optim Theory Appl 178, 699–725 (2018). https://doi.org/10.1007/s10957-018-1335-0
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DOI: https://doi.org/10.1007/s10957-018-1335-0