THE MONGE-AMP ERE SYSTEM CONVEX INTEGRATION IN ARBITRARY DIMENSION AND CODIMENSION MARTA LEWICKA

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THE MONGE-AMP`
ERE SYSTEM: CONVEX INTEGRATION IN
ARBITRARY DIMENSION AND CODIMENSION
MARTA LEWICKA
Abstract. In this paper, we study flexibility of the weak solutions to the Monge-Amp`ere
system (MA) via convex integration. This system of Pdes is an extension of the Monge-Amp`ere
equation in d= 2 dimensions, naturally arising from the prescribed curvature problem, and
closely related to the classical problem of isometric immersions (II).
Our main result achieves density, in the set of subsolutions, of the H¨older regular C1so-
lutions to the weak formulation (VK) of (MA), for all α < 1
1+d(d+1)/k where dis an arbitrary
dimension and kis an arbitrary codimension of the problem. This result seems to be opti-
mal, from the technical viewpoint, for the corrugation-based convex integration scheme. In
particular, it covers the codimension interval k1, d(d+ 1), so far uncharted even for the
system (II), since the regularity C1with any α < 1 proved by K¨allen in [7], strictly requires
a large codimension kd(d+ 1). We also reproduce K¨allen’s result in the context of (MA).
At k= 1, our result agrees with the regularity C1for (II) with any α < 1
1+d(d+1) , proved
by Conti, Delellis and Szekelyhidi in [2]. Finally, our results extend the initial findings by the
author and Pakzad in [10] for (MA) and d= 2, k = 1.
As an application of our results for (VK), we derive an energy scaling bound in the quanti-
tative immersability of Riemannian metrics, for nonlinear energy functionals modelled on the
energies of deformations of thin prestrained films in the nonlinear elasticity [8].
1. Introduction
This paper concerns regularity of weak solutions to a multi-dimensional version of the Monge-
Amp`ere equation, which arises from the prescribed curvature problem and is closely related to
the problem of isometric immersions and the dimension reduction of thin films. Namely, given
a matrix field A:ωRd×d
sym on a domain ωRd, we look for vector fields wand vsuch that:
v:ωRk, w :ωRd,
1
2(v)Tv+ symw=Ain ω. (VK)
When d= 2, k = 1, the left hand side above is the von K´arm´an content whose energy measures
the stretching of a thin film with midplate ω, subject to the out of plane displacement vand
the in plane displacement w. Taking curl curl of both sides of (VK) yields then the Monge-
Amp`ere equation: det2v=curl curl Aon ω, which reflects matching the leading order term
in the expansion of the Gaussian curvature κof surfaces {(x, ϵv(x)); xω)} ⊂ R3with the
given scalar function f=curl curl A. We note that one can achieve any sufficiently regular
fby imposing A=(∆1f)Id2. For arbitrary d, k 1, the situation is similar: applying a
multi-dimensional operator C2(see the formula in (1.4)) to both sides of (VK), leads to the
system which equates the leading order term in the expansion of the full Riemann curvature
M.L. was partially supported by NSF grant DMS-2006439. AMS classification: 35Q74, 53C42, 35J96, 53A35.
1
arXiv:2210.04363v3 [math.AP] 24 Feb 2024
2 MARTA LEWICKA
tensor of the manifold {(x, ϵv(x)); xω)} ⊂ Rd+kwith the table F=C2(A) : ωRd4:
v:ωRk,
Det 2v.
=ijv, ∂jtv⟩−⟨itvjsvij,st:1...d =Fin ω. (MA)
Again, any Fsatisfying the symmetries and Bianchi’s identities can be achieved this way.
The closely related problem to (VK) and (MA) is the problem of finding an isometric immersion
uof the given Riemannian metric g:ωRd×d
sym,>, into a higher dimensional space Rd+k:
u:ωRd+k,
(u)Tu=gin ω. (II)
This problem reduces to (VK) when gathering the leading (lowest order) terms in the ϵ-
expansions, for the family of Riemannian metrics {gϵ= Idd+ 2ϵ2A}ϵ0and the family of
metrics generated by the immersions {uϵ= (idd+ϵ2w, ϵv)}ϵ0. When posed in arbitrary di-
mension dbut low codimension k= 1, it has been shown in [3, Theorem 1.1] that any local
subsolution to (II) can be uniformly approximated by a sequence of solutions {un}
n=1 of regu-
larity C1, for any H¨older exponent α < 1
1+2dwhere d=d(d+ 1)/2 is the dimension of Rd×d
sym.
On the other hand, as showed in [7], regularity C1with any α < 1 can be achieved in suf-
ficiently high codimension k; however even for the local result this argument strictly requires
k2d, whereas it yields no outcome for k < 2d. These two results, albait both relying
on convex integration, use different constructions of the cascade of perturbations: Kuiper’s
corrugations in [3] and Nash’s spirals in [7], and one cannot be deduced from the other.
To our knowledge, there has been no result for the codimension interval k(1,2d) interpolat-
ing the regularity in [3] and [7], or even improving the exponent 1
1+2dwithout the requirement
k2d. The purpose of our paper is to achieve precisely this goal, for the system (VK).
Our main result states that any C1-regular pair (v, w) which is a subsolution of (VK), can
be uniformly approximated by a sequence of solutions {(vn, wn)}
n=1 of regularity C1for any
older exponent α < 1
1+2d/k , in case of arbitrary dand k. Our proof only uses corrugations,
extending the construction in [3] in an optimal manner. Clearly, the obtained critical regularity
exponent 1/2 at k= 2dis inferior to the exponent 1 from a version of the same construction
as in [7], that we also demonstrate in our paper. We expect that the superposition of both
techniques should yield a tighter interpolation, which is the subject of the ongoing research.
We state our results and offer further discussion in the subsections below.
1.1. Convex integration by corrugations, arbitrary d and k. The following theorem is
our main result. We refer to it as flexibility of (VK) up to C1,1
1+2d/k :
Theorem 1.1. Let ωRdbe an open, bounded domain. Given two vector fields v∈ C1(¯ω, Rk),
w∈ C1(¯ω, Rd)and a matrix field A∈ C0 (¯ω, Rd×d
sym), assume that:
D=A1
2(v)Tv+ symwsatisfies D> c Iddon ¯ω,
for some c > 0, in the sense of matrix inequalities. Fix ϵ > 0and let:
0< α < min nβ
2,1
1 + d(d+ 1)/k o.
THE MONGE-AMP`
ERE SYSTEM: CONVEX INTEGRATION IN ARBITRARY DIMENSION AND CODIMENSION3
Then, there exists ˜v∈ C1(¯ω, Rk)and ˜w∈ C1(¯ω, Rd)such that the following holds:
˜vv0ϵ, ˜ww0ϵ, (1.1)1
A1
2(˜v)T˜v+ sym˜w= 0 in ¯ω. (1.1)2
This result generalizes [10, Theorem 1.1], where we proved flexibility for (VK) up to C1,1
7in
dimensions d= 2, k= 1. In that special case, motivated by theory of elasticity, the left hand
side of (VK) represents the von K´arm´an stretching content 1
2v⊗ ∇v+ symwwritten in
terms of the scalar out-of-plane displacement vand the in-plane displacement wof the middle
plate ωof a thin film. The case d= 2 is special and flexibility (in codimension 1) of (VK)
holds up to C1,1
5as shown in [2, Theorem 1.1] using the conformal equivalence of 2-dimensional
metrics to the Euclidean metric. In our follow-up extension [9] of the present work, we likewise
show that any k1 allow for flexibility up to C1,1
1+4/k when d= 2. After the completion
of our both works, we learned of the very recent preprint [1] in which flexibility of (VK) for
d= 2, k = 1 has been futher improved to hold up to C1,1
3.
The main new technical ingredient allowing for the flexibility range stated in Theorem 1.1, is
the following “stage”-type construction in the convex integration algorithm for (VK):
Theorem 1.2. Let the vector fields v∈ C2(¯ω, Rk),w∈ C2(¯ω, Rd)and the matrix field A
C0(¯ω, Rd×d
sym)be given on an open, bounded domain ωRd. Assume that:
D=A1
2(v)Tv+ symwsatisfies 0<∥D01.
Fix two constants M, σ such that:
Mmax{∥v2,w2,1}and σ1.
Then, there exist ˜v∈ C2(¯ω, Rk)and ˜w∈ C2(¯ω, Rd)such that, denoting:
˜
D=A1
2(˜v)T˜v+ sym˜w,
the following holds:
˜vv1C∥D1/2
0,˜ww1C∥D∥1/2
0(1 + ∥∇v0),(1.2)1
∥∇2˜v0CMσd/k,∥∇2˜w0CM σd/k(1 + ∥∇v0),(1.2)2
˜
D0CA0
Mβ∥Dβ/2
0+∥D0
σ,(1.2)3
where d=d(d+ 1)/2and where the constants Cdepend only on d, k and ω.
We briefly outline how our construction differs from [10] and [3]. There, a stage consisted of
precisely d“steps”, each cancelling one of the rank-one “primitive” deficits in the decompo-
sition of D. The initially chosen frequency of perturbation was multiplied by a factor σat
each step, leading to the increase of the second derivative by σdand thus to the exponent d
replacing d/k in (1.2)2, while the remaining error in Dwas of order 1, leading to (1.2)3.
Presently, we first observe that ksuch deficits may be cancelled at once, by using klinearly
independent codimensions. Further, when all the first order primitive deficits are cancelled, one
may proceed to cancelling the second order deficits obtained as the one-dimensional decompo-
sitions of the error between the original and the decreased D; the corresponding frequencies
must be then increased by the factor σ1/2, precisely due to the decrease of Dby the factor
4 MARTA LEWICKA
1. One may inductively proceed in this fashion, cancelling even higher order deficits, and
adding k-tuples of single codimension perturbations, for a total of N=lcm(k, d) steps. The
frequencies get increased by the factor of σover each multiple of k, leading to the increase of
the second derivatives by σ, and by the factor of σ1/2over each multiple of d, where the deficit
decreases by the factor of 1. In the final count, the total increase of the second derivatives
has the factor σN/k, while the decrease of the deficit has the factor 1N/d. The relative
change of order is thus (N/k)/(N/d) = d/k, as stated in Theorem 1.2.
We point out that for this scheme to work, it is essential to use the optimal “step”-type
construction in which the chosen one-dimensional primitive deficit is cancelled at the expense
of introducing least error possible. Our previous definition from [10] would not work for this
purpose, and we need to superpose three corrugations rather than two.
1.2. Convex integration by spirals, k 2d.For a large codimension, one can reach flexi-
bility of (VK) up to C1,1, motivated by a similar result for (II) in [7]:
Theorem 1.3. In the context of Theorem 1.1, assume that the codimension ksatisfies k
2d=d(d+ 1). Then, the same result is valid for any exponent in the range:
0< α < min nβ
2,1o.
The “stage” construction allowing for flexibility as above, is the counterpart of Theorem 1.4:
Theorem 1.4. Let ωRdand kbe as in Theorem 1.3. Fix an exponent δ > 0. Then, there
exists σ0>1depending only on ωand δ, such that we have the following. Given v∈ C2(¯ω, Rk),
w∈ C2(¯ω, Rd),A∈ C0(¯ω, Rd×d
sym)and given two constants M, σ wih the properties:
D=A1
2(v)Tv+ symwsatisfies 0<∥D01,
Mmax{∥v2,w2,1}, σ σ0,
there exist ˜v∈ C2(¯ω, Rk),˜w∈ C2(¯ω, Rd)such that, denoting:
˜
D=A1
2(˜v)T˜v+ sym˜w,
the following bounds are valid, with constants Cdepending only on d, k, ω and δ:
˜vv1C∥D1/2
0,˜ww1C∥D1/2
0(1 + ∥∇v0),(1.3)1
∥∇2˜v0CMσδ,∥∇2˜w0CMσδ(1 + ∥∇v0),(1.3)2
˜
D0CA0
Mβ∥Dβ/2
0+∥D0
σ.(1.3)3
An outline of this construction, based on the approach in [7], is as follows. Firstly, each rank-one
“primitive” deficit is cancelled using two codimensions, via spiral-like perturbations of the fields
v, w, rather than via one-dimensional corrugations. This allows for a better order in the second
order deficit. Since we now have 2dcodimensions available, we may rank-one decompose the
new deficit as well and cancel it right away by adjusting the original perturbations. Proceeding
this way, it is possible to cancel arbitrarily high order of deficits, keeping the frequency at a
chosen value σwhile assuring that Dis decreased by the factor 1N, for arbitrarily large N.
THE MONGE-AMP`
ERE SYSTEM: CONVEX INTEGRATION IN ARBITRARY DIMENSION AND CODIMENSION5
1.3. The Monge-Amp´ere system. We now proceed to interpreting Theorem 1.1 in the
context of the Monge-Amp´ere system. We introduce this new system of partial differential
equations as the strong formulation of (VK). Recall that for a matrix field A= [Aij ]i,j=1...2:
R2R2×2, the scalar field curl curlA is defined by taking the curl operator on each row of
A, and then applying another curl on thus formed two-dimensional vector field:
curl curlA= curl1A12 2A11, ∂1A22 2A21
=11A22 12A21 12A12 +22A11.
It is well known that the kernel of curl curl when restricted to R2×2
sym matrix fields, consists
precisely of symmetric gradients. We will be concerned with the following generalization of
curl curl, serving the same characterisation in higher dimensions:
Definition 1.5. Given a d-dimensional square matrix field A= [Aij ]i,j=1...d :ωRd×don a
domain ωRd, we define C2(A) : ωRd4by:
C2(A)ij,st =isAjt +jtAis itAjs jsAit for all i, j, s, t = 1 . . . d. (1.4)
It can be checked that the components of the Riemann curvature tensor of a family of metrics
Idd+ϵA on ω, are given, to the leading order, by the components of C2(A):
Riem(Idd+ϵA)ij,st =ϵ
2C2(A)ij,st +O(ϵ2) for all i, j, s, t = 1 . . . d. (1.5)
For dimension d= 2, the above formula yields the linearization of the Gaussian curvature:
κ(Id2+ϵA) = ϵ
2curl curlA+O(ϵ2). We have the following:
Lemma 1.6. Let ωRdbe an open, bounded, contractible domain with Lipschitz boundary.
Given a symmetric matrix field AL2(ω, Rd×d
sym), the following conditions are equivalent:
(i) A= symwfor some wH1(ω, Rd),
(ii) C2(A)=0in the sense of distributions on ω.
Observe that for A= (v)Tvgiven through a vector field v:ωRk, there holds:
C2(v)Tvij,st = 2itv, ∂jsv⟩ − 2isv, ∂jtv.
When d= 2 and k= 1, the above reduces to the familiar formula: curl curl(v⊗ ∇v) =
2 det 2v. Following this motivation, we introduce:
Definition 1.7. For v:ωRkdefined on a domain ωRd, we set Det 2v:ωRd4in:
Det 2vij,st =isv, ∂jtv⟩−⟨itv, ∂jsvfor all i, j, s, t = 1 . . . d. (1.6)
Given F:ωRd4, we call the following system of Pdes, the Mong´e-Amper´e system:
Det 2v=Fon ω.
Lemma 1.6 can be restated in this context as follows. Given a matrix field A:ωRd×d
sym on a
domain ωRd, the problem (VK) is equivalent to (disregarding the regularity questions):
v:ωRk,
Det 2v=C2(A),(MA)
摘要:

THEMONGE-AMP`ERESYSTEM:CONVEXINTEGRATIONINARBITRARYDIMENSIONANDCODIMENSIONMARTALEWICKAAbstract.Inthispaper,westudyflexibilityoftheweaksolutionstotheMonge-Amp`eresystem(MA)viaconvexintegration.ThissystemofPdesisanextensionoftheMonge-Amp`ereequationind=2dimensions,naturallyarisingfromtheprescribedcurv...

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