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The free-boundary Brakke flow

  • Nick Edelen EMAIL logo
Veröffentlicht/Copyright: 11. Januar 2018

Abstract

We develop the notion of Brakke flow with free-boundary in a barrier surface. Unlike the classical free-boundary mean curvature flow, the free-boundary Brakke flow must “pop” upon tangential contact with the barrier. We prove a compactness theorem for free-boundary Brakke flows, define a Gaussian monotonicity formula valid at all points, and use this to adapt the local regularity theorem of White [23] to the free-boundary setting. Using Ilmanen’s elliptic regularization procedure [10], we prove existence of free-boundary Brakke flows.

A Appendix

We show how the errors (in space) from straightening the barrier transfer to errors in spacetime. This is in principle standard but the spacetime nature of the perturbation makes it a little more confusing.

Recall the interpolation inequality: if i+2j, then

ri+2j|Ditju|0,Brn,1r+α[u],α,Brn,1+|u|0,Brn,1.

So to control the C,α spacetime norm of u in Brn,1, it suffices to control the top Hölder semi-norms and the C0 norm. Of course, the same kind of interpolation inequality holds for the standard Hölder spaces.

We make use of the following identities:

(A.1)[fg]α,Brn,1[f]α,g(Brn,1)(|Dg|0,Br+r|tg|0,Br)α,
(A.2)α,Brn,1(|Df|0,g(Br)+r|tf|0,g(Br))[g]α,Brn,1,
(A.3)α,Ui=1k[fi]α,Uji|fj|0,U.

The following is a straightforward but tedious application of the inverse function theorem.

Lemma A.1.

Let u:UBrn,1RN-n be C1 in both variables, with

r-1|u|+|Du|+r|tu|1.

Suppose ϕ:B3rNRN satisfies

ϕ=Id+e,r-1|e|+|De|ϵϵ1(n).

Then if we extend ϕ(x,t):=(ϕ(x),t) to act on RN,1 we have ϕ(graph(u))=graph(u~), where

u~(y,t)=u(y+ξ(y,t),t)+η(y,t),

with the estimates

r-1|ξ|+|Dξ|+r|tξ|c(n)ϵ,r-1|η|+|Dη|+r|tη|c(n)ϵ.

If further we have

r+α-1[e],α,Brnϵ,r+α-1[u],α,Brn,11,

then

r+α-1[ξ],α,Br/2n,1c(n,,α)ϵ,r+α-1[η],α,Br/2n,1c(n,α,)ϵ.

Proof.

Write A(x,t)=x+e1(x,u(x,t)) so that

ϕ(x,u(x,t))=(A(x,t),u(x)+e2(x,u(x,t)).

By assumption, we have

(A.4)r-1|A-Id|ϵ,|DA-Id||De1|(1+|Du|)c(n)ϵ

and

(A.5)r|tA|r|De1||tu|c(n)ϵ.

Therefore, by the inverse function theorem an inverse At-1A(,t)-1 exists for each time slice, and we can set

u~(y,t)=u(At-1(y),t)+e2(At-1(y),u(At-1(y,t)))
=:u(y+ξ(y,t),t)+η(y,t).

where

ξ(y,t)=y-At-1(y),η(y,t)=e2(At-1(y),u(At-1(y),t)).

From (A.4) and (A.5) we immediately obtain

r-1|A-1-Id|c(n)ϵ,
|DA-1-Id|c(n)ϵ,
r|tA-1|r|DA-1||tA|c(n)ϵ.

This proves the C1 estimates on ζ. The required C1 estimate on η follows similarly, e.g.:

|tη||De2|(|tA-1|+|tu|+|Du||tA-1|)c(n)ϵr.

To prove the higher order estimates on ζ and η, we proceed as follows. First, by an easy induction one can show that Dtm(A-1) is a linear combination of terms involving (DA)-1, Dae1|(Id,u)A-1, and Dbtc(Id,u)|A-1, where |a|1 in each term. Using relation (A.1), and our assumed bounds for u, we have

(A.6)[(Daei)(Id,u)A-1]α,Br/2n,1c(n,α)[Daei]α,Brn

for any a. Notice the left-hand side is the spacetime Hölder semi-norm, while the right-hand side is the regular Hölder semi-norm. This gives a Hölder bound of the form

r+2m+α-1[DtmA-1]α,Br/2n,1c(n,,m,α)ϵ,

which is the required estimate for ζ.

By similar reasoning, we have that Dtmη is a linear combination of terms involving Dae2|(Id,u)A-1 and Dbtc((Id,u)A-1). Now use (A.6), (A.3) and our assumed regularity of u to obtain the Hölder estimate on η. ∎

Lemma A.2.

Let Mi,M be a sequence in S(n,N), where MiM as free-boundary Brakke flows. Suppose 0 is a regular point of each Mi, and

infir2,α(i,0)>0.

Then 0 is a regular point of M, and the Mi converge to M in C2,α near 0.

If, additionally, the barriers converge in C, then convergence near 0 is smooth.

Proof.

If 0 is uniformly bounded away from the barriers Si, then this follows from the Arzela–Ascoli theorem and interior Schauder estimates. To handle points at the boundary, we will straighten the barrier.

Take 0S, and by replacing i with i-(ζi(0),0) we can assume 0Si also. Pass to a subsequence, rotate by a fixed amount in space, and replace i with i-(0,ti) (with ti0) as necessary, and we have

i(BρN-n×Bρn,1)=graph(u(i)),

where u(i):Qi×IBρn,1 is uniformly bounded in C2,α, and I is either the interval [-ρ2,ρ2] or [-ρ2,0].

Let Φi, Φ be the map (2.2) straightening the barriers Si, S (respectively), centered at 0. Using Lemma A.1, we have

Φi-1(graph(u(i)))=graph(u~(i)),

where u~(i) is uniformly bounded in C2,α also. There is a fixed half-space Hn, so that u~(i):H×I has Neumann boundary conditions in H.

The Arzela–Ascoli theorem implies u~(i) subsequentially converge in C2,α to some map u~:H×I. By the definition of free-boundary convergence, ΦiΦ in C2,α. We deduce that

(BρN-n×Bρn,1)=Φ(graph(u~))=:graph(u).

This shows is proper and C2,α near 0.

The limit u~ is a graphical mean curvature flow in the pullback metric γ=Φ*δ. Therefore u~ satisfies

(A.7)tu~-gklDklu~=0,

where gkl is the inverse to the matrix γ(ek+Dku,el+Dlu). Provided ρ is sufficiently small, by (2.3) this is a parabolic equation, with coefficients as regular as Du~. The usual bootstrap argument then gives C.

Suppose the barriers converge smoothly SiS. Each u~(i) satisfies the graphical mean curvature equation (A.7), with the pullback metric γi=Φi*δ:

tu~(i)=F(DΦi,Du~(i),D2u~(i))

for some analytic F. So the difference w(i)=u~(i)-u~ satisfies a linear PDE

tw(i)=akl(i)Dklw(i)+bk(i)Dkw(i)+ck(i)Dk(Φi-Φ)=:Lw(i).

Convergence of Φi and w(i) implies L is uniformly elliptic, with constant terms going to 0 in C. The usual Schauder estimates then imply w(i)0 in C also. ∎

The following boundary monotonicity formula appears in Allard [2].

Proposition A.3 (Allard [2, Lemma 3.1]).

Let V be an integral n-varifold with free-boundary in SU. For any 0<τ<σrS, and any hCc1(U,R), we have

σ-1Bσ(S)h|DTd|2+dDThDTd+hdtrVD2d+hdSTHDddμV
-τ-1Bτ(S)h|DTd|2+dDThDTd+hdtrVD2d+hdSTHDddμV
=Bσ(S)Bτ(S)DThDTd+htrVD2d+hSTHDddμV.

Here d=d(,S).

In particular, by the dominated convergence theorem,

σ-1Bσ(S)h|DTd|2𝑑μV-limτ0τ-1Bτ(S)h|DTd|2𝑑μV
=Bσ(S)S(1-dσ)(DThDTd+htrVD2d+hSTHDd)𝑑μV.

Proof.

Let X be the vector field

X=ϕ(d)h(x)dDdϕ(d)h(x)(x-ζ(x)),

where ϕ is a cutoff function to be determined. We have

divV(X)=ϕ|DTd|2hd+ϕdDThDTd+ϕh|DTd|2+ϕhdtrVD2d.

Therefore, if

I(ρ)=ϕ(dρ)h(x)|DTd|2𝑑μV,

then

I-ρI=-ϕ𝑑DThDTd+ϕhdtrVD2d+ϕhdSTHDdμV.

Integrating the above relation between τ<σ, and then taking ϕ1[0,1], we obtain

σ-1Bσ(S)h|DTd|2𝑑μV-τ-1Bτ(S)h|DTd|2𝑑μV
=τσρ-2Bρ(S)𝑑DThDTd+hdtrVD2d+hdSTHDddμVdρ.

Apply the standard layer-cake formula to the measure

ν(A)=A𝑑DThDTd+dhtrVD2d+hdSTHDddμV,

to obtain

RHS=Bσ(S)Bτ(S)d-1𝑑ν-σ-1Bσ(S)𝑑ν+τ-1Bτ(S)𝑑ν,

which is the required equality. ∎

Acknowledgements

I express my deepest gratitude to my advisors Simon Brendle and Brian White, and to my friend Otis Chodosh, for their guidance and support. I thank Masashi Mizuno for bringing several references to my attention. This work borrows heavily from a series of lectures given by White at Stanford in Spring 2015, and Ilmanen’s book on elliptic regularization [10].

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Received: 2016-06-20
Revised: 2017-04-17
Published Online: 2018-01-11
Published in Print: 2020-01-01

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