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Regularity for convex viscosity solutions of Lagrangian mean curvature equation

Arunima Bhattacharya Department of Mathematics, Phillips Hall
the University of North Carolina at Chapel Hill, NC
[email protected]
 and  Ravi Shankar Department of Mathematics, Fine Hall
Princeton University, Princeton, NJ
[email protected]
Abstract.

We show that convex viscosity solutions of the Lagrangian mean curvature equation are regular if the Lagrangian phase has Hölder continuous second derivatives.

1. Introduction

We establish regularity for convex viscosity solutions of the Lagrangian mean curvature equation

(1.1) F(D2u)=i=1narctanλi=ψ(x)F(D^{2}u)=\sum_{i=1}^{n}\arctan\lambda_{i}=\psi(x)

under the assumption that ψ:B1(0)[0,nπ/2)\psi:B_{1}(0)\to[0,n\pi/2) is in C2,α(B1(0))C^{2,\alpha}(B_{1}(0)) for some α(0,1)\alpha\in(0,1). Here λi\lambda_{i}’s are the eigenvalues of the Hessian matrix D2uD^{2}u and then the phase ψ\psi becomes a potential for the mean curvature of the Lagrangian submanifold L=(x,Du(x))nL=(x,Du(x))\subset\mathbb{C}^{n}. The induced Riemannian metric gg can be written as g=In+(D2u)2g=I_{n}+(D^{2}u)^{2} or

gij=δij+uikδklulk.g_{ij}=\delta_{ij}+u_{ik}\delta^{kl}u_{lk}.

In [HL82, (2.19)], the mean curvature vector H\vec{H} of this Lagrangian submanifold was shown to be

(1.2) H=Jgψ\vec{H}=J\nabla_{g}\psi

where g\nabla_{g} is the gradient operator for the metric gg and JJ is the complex structure, or the π2\frac{\pi}{2} rotation matrix in n\mathbb{C}^{n}. Note that by our assumption on ψ\psi, |H||H| is bounded.

When the phase is constant, denoted by cc, uu solves the special Lagrangian equation

(1.3) i=1narctanλi=c\sum_{i=1}^{n}\arctan\lambda_{i}=c

or equivalently,

cosc12k+1n(1)kσ2k+1sinc02kn(1)kσ2k=0.\cos c\sum_{1\leq 2k+1\leq n}(-1)^{k}\sigma_{2k+1}-\sin c\sum_{0\leq 2k\leq n}(-1)^{k}\sigma_{2k}=0.

Equation (1.3) originates in the special Lagrangian geometry of Harvey- Lawson [HL82]. The Lagrangian graph (x,Du(x))n(x,Du(x))\subset\mathbb{C}^{n} is called special when the argument of the complex number (1+iλ1)(1+iλn)(1+i\lambda_{1})...(1+i\lambda_{n}) or the phase ψ\psi is constant, and it is special if and only if (x,Du(x))(x,Du(x)) is a (volume minimizing) minimal surface in (n,dx2+dy2)(\mathbb{C}^{n},dx^{2}+dy^{2}) [HL82].

A dual form of (1.3) is the Monge-Ampère equation

(1.4) i=1nlnλi=c.\sum_{i=1}^{n}\ln\lambda_{i}=c.

This is the potential equation for special Lagrangian submanifolds in (n,dxdy)(\mathbb{C}^{n},dxdy) as introduced in [Hit97]. The gradient graph (x,Du(x))(x,Du(x)) is volume maximizing in this pseudo-Euclidean space, as shown by Warren [War10]. In the 1980s, Mealy [Mea89] showed that an equivalent algebraic form of the above equation is the potential equation for his volume maximizing special Lagrangian submanifolds in (n,dx2dy2)(\mathbb{C}^{n},dx^{2}-dy^{2}).

The regularity of solutions is a fundamental problem for these geometrically and analytically significant equations. Our main results are the following:

Theorem 1.1.

Let uu be a convex viscosity solution of (1.1) on B1(0)nB_{1}(0)\subset\mathbb{R}^{n}, where ψC2,α(B1)\psi\in C^{2,\alpha}(B_{1}). Then uC4,α(B1)u\in C^{4,\alpha}(B_{1}).

We use the above regularity to prove the following interior estimate.

Theorem 1.2.

Let uu be a C4,αC^{4,\alpha} convex solution of (1.1) on B1(0)nB_{1}(0)\subset\mathbb{R}^{n}, where ψC2,α(B1)\psi\in C^{2,\alpha}(B_{1}). Then uu satisfies the following Hessian estimate

(1.5) |D2u(0)|C(n,α,oscB1/2(u),ψC2,α(B1/2)).\displaystyle|D^{2}u(0)|\leq C(n,\alpha,osc_{B_{1/2}}(u),\|\psi\|_{C^{2,\alpha}(B_{1/2})}).

We state the following application of our result.

Application. Lagrangian mean curvature flow:
We specialize to ψ(x)=κx+c\psi(x)=\kappa\cdot x+c. In this case, the gradient graph (x,Du(x))(x,Du(x)) corresponds to a translating soliton for Lagrangian mean curvature flow. Indeed, if u(x,t)u(x,t) solves the potential equation

ut=i=1narctanλi(x,t),u_{t}=\sum_{i=1}^{n}\arctan\lambda_{i}(x,t),

then the gradient graph X(t)=(x,Du(x,t))X(t)=(x,Du(x,t)) solves the Lagrangian mean curvature equation

(Xt)=H,(X_{t})^{\bot}=H,

where H=JgψH=J\nabla_{g}\psi is the mean curvature, and \bot is the projection onto the normal space of {(x,Du(x,t))}xn×n\{(x,Du(x,t))\}_{x}\subset\mathbb{R}^{n}\times\mathbb{R}^{n}; see [CCH12, pg 203]. Now let u(x,0)=u(x)u(x,0)=u(x) solve (1.1) for ψ(x)=κx+c\psi(x)=\kappa\cdot x+c. Then u(x,t)=u(x)+t(κx+c)u(x,t)=u(x)+t(\kappa\cdot x+c), so (x,Du(x,t))=(x,Du(x))+t(0,κ)(x,Du(x,t))=(x,Du(x))+t(0,\kappa) is a translating soliton with “constant” mean curvature κ\kappa. We conclude that translating Lagrangian solitons with convex potentials and “vertical” speeds (0,κ)(0,\kappa) are smooth. Local a priori estimates for convex solutions to Lagrangian mean curvature flow were found in [NY11].

The convexity of the special Lagrangian equation plays a dominant role in its regularity theory. The arctangent operator is concave if uu is convex, or if the Hessian has a lower bound λ0\lambda\geq 0. Bao and Chen [BC03] showed regularity for convex W2,pW^{2,p} strong solutions. For smooth convex solutions of (1.3), Hessian estimates have been obtained by Chen-Warren-Yuan [CWY09]. Recently in [CSY19], Chen-Shankar-Yuan confirmed that convex viscosity solutions of (1.3) are smooth. The semiconvex singular solutions constructed by Wang-Yuan [WY13] show that the convexity condition is necessary. Similarly, if in (1.3) we have critical phase |c|=(n2)π/2|c|=(n-2)\pi/2 or supercritical phase |c|>(n2)π/2|c|>(n-2)\pi/2, then F(D2u)F(D^{2}u) has convex level sets, but it was shown by Yuan [Yua06] that this fails for subcritical phases |c|<(n2)π/2|c|<(n-2)\pi/2. For critical and supercritical phases, Hessian estimates for (1.3) have been obtained by Warren-Yuan [WY09, WY10] and Wang-Yuan [WY14], see also [Li19]. For subcritical phases, C1,αC^{1,\alpha} solutions of (1.3) were constructed by Nadirashvili-Vlăduţ [NV10] and Wang-Yuan [WY13]. Hessian lower bounds also play a role in the dual equation (1.4). The Monge-Ampére type equation detD2u=h(x)\det D^{2}u=h(x) has Pogorelov-type singular C12/nC^{1-2/n} convex viscosity solutions whose graphs contain a line. However, under the necessary strict convexity assumption λ>0\lambda>0, interior regularity was obtained by Pogorelov [Pog78] for a smooth enough right hand side h(x)h(x), by Urbas [Urb88] if h(x)h(x) is Lipschitz and u(x)C(12/n)+u(x)\in C^{(1-2/n)^{+}}, and by Caffarelli [Caf90] if h(x)h(x) is merely Hölder.

The convexity of uu creates its own challenges in proving regularity, since it is unstable under smooth approximations of the boundary value. To use the method of a priori estimates, one would solve the Dirichlet problem for a modified concave equation F~(D2u)=ψ(x)\tilde{F}(D^{2}u)=\psi(x), where f~(λ)=arctanλ\tilde{f}(\lambda)=\arctan\lambda for λ0\lambda\geq 0 and =λ=\lambda for λ<0\lambda<0. If we approximate the boundary data and find the smooth solution of this problem, it may no longer be convex, and therefore lacks a connection to the original problem. Although a priori estimates are available for (1.1) and (1.3), estimates for F~\tilde{F} are unknown.

In showing regularity for convex solutions of (1.3), the authors of [CSY19] managed to avoid a priori estimates altogether. The basic idea was to change variables using the Lewy-Yuan rotation of the gradient graph, x¯+iDu¯(x¯)=eiπ/4(x+iDu(x))\bar{x}+iD\bar{u}(\bar{x})=e^{-i\pi/4}(x+iDu(x)), such that the Hessian bounds decreased from 0λ+0\leq\lambda\leq+\infty to 1λ¯1-1\leq\bar{\lambda}\leq 1. Since minimal graphical tangent cones with such bounds are flat, they were able to deduce regularity in new coordinates using ideas from [Yua01]. One problem, however, is that defining such a rotation is unclear if convex uu is not C1C^{1}. To adapt to the lower regularity setting, it was shown in [CSY19] that in the smooth case, u¯(x¯)\bar{u}(\bar{x}) can be constructed using the Legendre transform, which is still well defined in the Lipschitz case.

Extending the constant phase (1.3) results to variable phases (1.1) is subtle, and not always possible. Interior regularity for solutions of (1.1) with a C1,1C^{1,1} supercritical and critical phase were recently obtained in [Bha21, Bha22, BMS22], but C1,αC^{1,\alpha} singular solutions are known if ψ\psi has Hölder regularity [Bha21, Remark 1.3]. In fact, these singular solutions are convex, so Theorem 1.1 is not valid unless ψ(x)\psi(x) is sufficiently smooth. Moreover, in our companion paper [BS20], we exhibit convex C1,αC^{1,\alpha} singular solutions which solve an equation with ψ=f(x,Du)\psi=f(x,Du) depending also on the gradient. In such cases, ff is smooth in both arguments. Convex singular solutions do not exist for analogous uniformly elliptic PDEs F(D2u)=f(x,Du)F(D^{2}u)=f(x,Du). The non-uniform ellipticity of the arctangent operator in (1.3) makes the PDE highly sensitive to the structure of the variable phase. Nevertheless, the results of this paper show that no conditions on ψ(x)\psi(x) are needed for regularity of convex viscosity solutions, apart from some smoothness such as C2,αC^{2,\alpha}.

In proving Theorem 1.1, the treatment of the variable phase is delicate, and the technique does not always work. The key step to deduce C1,1C^{1,1} regularity, or λmax(D2u)<\lambda_{max}(D^{2}u)<\infty, is to show that in rotated coordinates, λ¯max\bar{\lambda}_{max} never saturates its upper bound of 11. For constant phases, this is done using the strong maximum principle for Δg¯\Delta_{\bar{g}}-subharmonic λ¯max\bar{\lambda}_{max}. For variable phases, subharmonicity only holds up to extra terms, such as D2ψ¯(emax,emax)D^{2}\bar{\psi}(e_{max},e_{max}). If ψ\psi is convex, then subharmonicity is restored, but Theorem 1.1 does not assume any conditions on ψ\psi other than C2,αC^{2,\alpha} smoothness. To handle these terms, we carefully account for the coordinate change, and relate D2ψ¯D^{2}\bar{\psi} to D2ψD^{2}\psi, for example. It turns out that the resulting expression vanishes when λ¯max\bar{\lambda}_{max} saturates its upper bound, restoring the maximum principle. To understand how this could happen, observe that for a convex singular solution, the forward map x¯=xcosα+Du(x)sinα\bar{x}=x\cos\alpha+Du(x)\sin\alpha has large Jacobian matrix in the λmax\lambda_{max} directions. It follows that the inverse map has small Jacobian in those directions, so the rotated phase ψ¯(x¯)=ψx(x¯)\bar{\psi}(\bar{x})=\psi\circ x(\bar{x}) will inherit this flatness.

This paper is divided into the following sections. In section 2, we formulate the Lewy-Yuan rotation for the Lipschitz potential u(x)u(x). In section 3, we establish regularity of the rotated potential u¯(x¯)\bar{u}(\bar{x}). In section 4, we deduce regularity of the original potential u(x)u(x), thereby proving Theorem 1.1. In section 5, we prove the Hessian estimate (1.5).

Acknowledgments. The authors are grateful to Yu Yuan for his guidance, support, and helpful discussions. The authors thank D. H. Phong for helpful comments and suggestions. AB acknowledges the support of the AMS-Simons Travel Grant. RS was partially supported by the NSF Graduate Research Fellowship Program under grant No. DGE-1762114. The authors thank the anonymous referee for the referee’s thorough feedback.

2. Rotation for Lipschitz potential

We formulate Lewy-Yuan rotation for the convex function uu solving (1.1), using the idea introduced in [CSY19]; we refer to sections 2.1 and 2.2 in that paper for various details in this section. If u(x)u(x) is smooth on Ω\Omega, then the gradient graph z=(x,Du(x))z=(x,Du(x)) is a Lagrangian submanifold of n\mathbb{C}^{n}, and if uu is convex, then the downward rotation z¯=eiπ/4z\bar{z}=e^{-i\pi/4}z yields another Lagrangian submanifold (x¯,Du¯(x¯))(\bar{x},D\bar{u}(\bar{x})) with smooth potential u¯(x¯)\bar{u}(\bar{x}) on x¯(Ω)\bar{x}(\Omega). Because the canonical angles decrease by an angle of π/4\pi/4

arctanλ¯i(D2u¯)=arctanλi(D2u)π/4,\arctan\bar{\lambda}_{i}(D^{2}\bar{u})=\arctan\lambda_{i}(D^{2}u)-\pi/4,

it follows that the rotation sends solutions of (1.1) to solutions u¯(x¯)\bar{u}(\bar{x}) of another Lagrangian mean curvature equation, which now is uniformly elliptic by the Hessian bounds

(2.1) InD2u¯In.\displaystyle-I_{n}\leq D^{2}\bar{u}\leq I_{n}.

This makes regularity theory tractable in new coordinates using the ideas developed in [Yua01].

If we do not assume that uu is in C1C^{1}, then the subdifferential (x,u(x))(x,\partial u(x)), i.e., the slopes of tangent planes touching uu from below at xx, is not a graph over Ω\Omega (for example, if u(x)=|x|u(x)=|x|, then u(0)=B¯1(0)\partial u(0)=\bar{B}_{1}(0)). Nevertheless, if we rotate the subdifferential (x,u(x))(x,\partial u(x)) downwards by π/4\pi/4, then we still obtain a gradient graph (x¯,Du¯(x¯))(\bar{x},D\bar{u}(\bar{x})), where u¯C1,1\bar{u}\in C^{1,1} and is given explicitly by

(2.2) su¯(x¯)c2|x¯|2=[su(x)+c2|x|2](x¯),x¯x¯(Ω),s\bar{u}(\bar{x})-\frac{c}{2}|\bar{x}|^{2}=-\left[su(x)+\frac{c}{2}|x|^{2}\right]^{*}(\bar{x}),\qquad\bar{x}\in\bar{x}(\Omega),

where c=cosπ/4c=\cos\pi/4, s=sinπ/4s=\sin\pi/4, and

f(x¯)=supx[xx¯f(x)],x¯f(Ω)f^{*}(\bar{x})=\sup_{x}[x\cdot\bar{x}-f(x)],\qquad\bar{x}\in\partial f(\Omega)

is the Legendre transform of convex f(x)f(x); see [CSY19, Proposition 2.1]. The image domain Ω¯=x¯(Ω)=u~(Ω)\bar{\Omega}=\bar{x}(\Omega)=\partial\tilde{u}(\Omega) is open and connected by [CSY19, Lemma 2.1], which comes from the fact that

(2.3) u~(x):=su+c2|x|2\tilde{u}(x):=su+\frac{c}{2}|x|^{2}

is strictly convex.

The transform (2.2) is order preserving, fgf¯g¯f\leq g\to\bar{f}\leq\bar{g}, hence, it preserves uniform limits. It follows that u¯(x¯)\bar{u}(\bar{x}) satisfies the same Hessian bounds (2.1) as in the smooth case. We could then use interpolation to see that Du¯nDu¯D\bar{u}_{n}\to D\bar{u} locally uniformly provided unuu_{n}\to u uniformly, but this also follows from strict convexity, as in [CSY19, Proposition 2.3], i.e. if x¯u~(a)v~(b)\bar{x}\in\partial\tilde{u}(a)\cap\partial\tilde{v}(b) for u,vu,v convex, then

(2.4) |ba|222(|u~v~|(a)+|u~v~|(b)).\displaystyle|b-a|^{2}\leq 2\sqrt{2}(|\tilde{u}-\tilde{v}|(a)+|\tilde{u}-\tilde{v}|(b)).

The smallness of |Du¯Dv¯||D\bar{u}-D\bar{v}| would then follow from reverse rotation a=sx¯+cDu¯a=-s\bar{x}+cD\bar{u}.

Following [CSY19, Propositions 2.2,2.3], we show that viscosity solutions are preserved under this rotation.

Proposition 2.1.

Let u(x)u(x) be a convex viscosity solution of (1.1) in B1.2(0)B_{1.2}(0). Then the π/4\pi/4-rotation u¯\bar{u} in (2.2) is a corresponding viscosity solution of

(2.5) F¯(D2u¯)=i=1narctanλ¯i(D2u¯)=ψ¯(x¯,Du¯)=ψ(x)nπ/4\bar{F}(D^{2}\bar{u})=\sum_{i=1}^{n}\arctan\bar{\lambda}_{i}(D^{2}\bar{u})=\bar{\psi}(\bar{x},D\bar{u})=\psi(x)-n\pi/4

in open Ω¯=u~(B1(0))\bar{\Omega}=\partial\tilde{u}(B_{1}(0)), where u~\tilde{u} is as defined in (2.3).

Proof.

We first prove the following claim.

Claim 1.

We show that u¯\bar{u} is a supersolution of (2.5) in Ω¯\bar{\Omega}.

Let P¯\bar{P} be a quadratic polynomial touching u¯\bar{u} from below locally somewhere on the open set Ω¯,\bar{\Omega}, say at the origin 0¯u~(0).\bar{0}\in\partial\tilde{u}(0). Since at 0¯\bar{0}, D2P¯D2u¯InD^{2}\bar{P}\leq D^{2}\bar{u}\leq I_{n}, we assume D2P¯<InD^{2}\bar{P}<I_{n}, by subtracting ε|x¯|2\varepsilon|\bar{x}|^{2} from P¯\bar{P}, and then letting ε0\varepsilon\rightarrow 0. This guarantees the existence of its pre-rotated quadratic polynomial P,P, and also confirms that P¯\bar{P} touches u¯\bar{u} from below in an open neighborhood of the closed set u~(0).\partial\tilde{u}(0). We still have DP¯(0¯)=Du¯(0¯)D\bar{P}(\bar{0})=D\bar{u}(\bar{0}). Using the order preservation of α\alpha-rotation that is also valid for reverse rotation, and continuity of the gradient mapping u~\partial\tilde{u} in [Roc97, Corollary 24.5.1], we see that the pre-rotated quadratic polynomial PP touches uu at x=0x=0 from below in an open neighborhood of 0B1(0).0\in B_{1}(0). Using the fact that uu is a supersolution of (1.1) we get

i=1narctanλi(D2P)ψ(0),\sum_{i=1}^{n}\arctan\lambda_{i}(D^{2}P)\leq\psi(0),

which in turn implies

F¯(D¯2P¯)=i=1narctanλ¯i(D2P¯)ψ(0)nπ/4=ψ¯(0¯,DP¯(0¯)).\bar{F}(\bar{D}^{2}\bar{P})=\sum_{i=1}^{n}\arctan\bar{\lambda}_{i}(D^{2}\bar{P})\leq\psi(0)-n\pi/4=\bar{\psi}(\bar{0},D\bar{P}(\bar{0})).

Therefore, the claim holds good.

Claim 2.

We show that u¯\bar{u} is a subsolution of (2.5) in Ω¯\bar{\Omega}.

The first part of this proof is the same as [CSY19, Prop 2.3, Step1] where a convolution uεu_{\varepsilon} of uu is considered and the smooth α\alpha-rotation u¯ε\bar{u}_{\varepsilon} is shown to be well defined on Ω¯=u~(B1(0))Du~ε(B1.1(0))\overline{\Omega}=\partial\tilde{u}(B_{1}(0))\subset D\tilde{u}_{\varepsilon}(B_{1.1}(0)) for ε>0\varepsilon>0 small enough.
Next, observe that (1.1) is concave when uu is a convex function. Applying [CC95, Theorem 5.8], we see that the solid convex average uε=uρεu_{\varepsilon}=u*\rho_{\varepsilon} is a subsolution of

F(D2uε)ψε(x)=ψρε(x)F(D^{2}u_{\varepsilon})\geq\psi_{\varepsilon}(x)=\psi*\rho_{\varepsilon}(x)

for ε>0\varepsilon>0 small enough. Combining [CSY19, Prop 2.1] with the first part of this proof, we see that the smooth α\alpha-rotation u¯ε\bar{u}_{\varepsilon} is a subsolution of

F¯(D2u¯ε)=i=1narctanλ¯i(D2u¯ε)ψ¯ε(x¯ε,Du¯ε)=ψε(xε)nα,\bar{F}(D^{2}\bar{u}_{\varepsilon})=\sum_{i=1}^{n}\arctan\bar{\lambda}_{i}(D^{2}\bar{u}_{\varepsilon})\geq\bar{\psi}_{\varepsilon}(\bar{x}_{\varepsilon},D\bar{u}_{\varepsilon})=\psi_{\varepsilon}(x_{\varepsilon})-n\alpha,

in Ω¯\overline{\Omega}, where xε=cx¯sDu¯ε(x¯)x_{\varepsilon}=c\bar{x}-sD\bar{u}_{\varepsilon}(\bar{x}). By (2.4), xεx=cx¯sDu¯(x¯)x_{\varepsilon}\to x=c\bar{x}-s\,D\bar{u}(\bar{x}) uniformly on Ω¯\bar{\Omega}, so ψε(xε(x¯))ψ(x(x¯))\psi_{\varepsilon}(x_{\varepsilon}(\bar{x}))\to\psi(x(\bar{x})) uniformly on Ω¯\bar{\Omega}. Since u¯εu¯\bar{u}_{\varepsilon}\to\bar{u} uniformly on Ω¯\bar{\Omega}, and they are viscosity subsolutions of locally uniformly convergent equations F¯(D2u¯ε)=fε(x¯)\bar{F}(D^{2}\bar{u}_{\varepsilon})=f_{\varepsilon}(\bar{x}), it follows from [CC95, Proposition 2.9] that u¯\bar{u} is a subsolution of the limiting equation (2.5).

Therefore, from claims 1 and 2, we see that u¯\bar{u} is a viscosity solution of (2.5) in Ω¯\bar{\Omega}. ∎

In the remainder, we abbreviate the rotated phase by

(2.6) ψ¯(x¯)\displaystyle\bar{\psi}(\bar{x}) :=ψ¯(x¯,Du¯(x¯))=ψ(x(x¯,Du¯(x¯)))nπ/4\displaystyle:=\bar{\psi}(\bar{x},D\bar{u}(\bar{x}))=\psi(x(\bar{x},D\bar{u}(\bar{x})))-n\pi/4
=ψ(x¯Du¯(x¯))2)nπ/4.\displaystyle=\psi\left(\frac{\bar{x}-D\bar{u}(\bar{x}))}{\sqrt{2}}\right)-n\pi/4.

In particular, since u¯C1,1\bar{u}\in C^{1,1}, we see that ψ¯\bar{\psi} is Lipschitz, so far.

3. Regularity of the rotated potential

We first show that u¯VMO(B1/2)\bar{u}\in VMO(B_{1/2}) followed by u¯C2,α(B1/2)\bar{u}\in C^{2,\alpha}(B_{1/2}). We recall the notion of VMO functions.

Definition 1 (Vanishing mean oscillation).

Let Ωn\Omega\subset\mathbb{R}^{n}. A locally integrable function vv is in VMO(Ω)VMO(\Omega) with modulus ω(r,Ω)\omega(r,\Omega) if

ω(r,Ω)=supx0Ω,0<rR1|Br(x0)Ω|Br(x0)Ω|v(x)vx0,r|0, as r0\omega(r,\Omega)=\sup_{x_{0}\in\Omega,0<r\leq R}\frac{1}{|{B_{r}(x_{0})\cap\Omega}|}\int_{B_{r}(x_{0})\cap\Omega}|v(x)-v_{x_{0},r}|\rightarrow 0,\text{ as $r\rightarrow 0$}

where vx0,rv_{x_{0},r} is the average of vv over Br(x0)Ω.B_{r}(x_{0})\cap\Omega.

Proposition 3.1 (VMO Estimates).

Let u¯\bar{u} be a C1,1C^{1,1} viscosity solution of (2.5) in B1(0)nB_{1}(0)\subset\mathbb{R}^{n}, where |D2u¯|1|D^{2}\bar{u}|\leq 1 and ψ¯(x¯)\bar{\psi}(\bar{x}) is continuous. Then D2u¯VMO(B1/2)D^{2}\bar{u}\in VMO(B_{1/2}) and the VMOVMO modulus of u¯\bar{u}, denoted by ω(r)0\omega(r)\rightarrow 0 as r0r\rightarrow 0.

Proof.

Suppose the contrary is true. Then we can find ε>0\varepsilon>0 and sequences {x¯kx¯}B1/2\{\bar{x}_{k}\rightarrow\bar{x}_{\infty}\}\subset B_{1/2}, {rk0}\{r_{k}\rightarrow 0\}, and a family of C1,1C^{1,1} viscosity solutions {u¯k}\{\bar{u}_{k}\} of (2.5) with |D2u¯k|1|D^{2}\bar{u}_{k}|\leq 1, such that

1|Brk|Brk|D2u¯k(D2u¯k)x¯k,rk|ε.\frac{1}{|B_{r_{k}}|}\int_{B_{r_{k}}}|D^{2}\bar{u}_{k}-(D^{2}\bar{u}_{k})_{\bar{x}_{k},r_{k}}|\geq\varepsilon.

Next, we blow up {u¯k}\{\bar{u}_{k}\}. For |y¯|1rk|\bar{y}|\leq\frac{1}{r_{k}}, we set

v¯k(y¯)=u¯k(x¯k+rky¯)u¯k(x¯k).rky¯u¯k(x¯k)rk2.\bar{v}_{k}(\bar{y})=\frac{\bar{u}_{k}(\bar{x}_{k}+r_{k}\bar{y})-\nabla\bar{u}_{k}(\bar{x}_{k}).r_{k}\bar{y}-\bar{u}_{k}(\bar{x}_{k})}{r_{k}^{2}}.

Here, v¯k\bar{v}_{k} is a viscosity solution of

i=1narctanλ¯i(D2v¯k(y¯))=ψ¯(x¯k+rky¯).\sum_{i=1}^{n}\arctan\bar{\lambda}_{i}(D^{2}\bar{v}_{k}(\bar{y}))=\bar{\psi}(\bar{x}_{k}+r_{k}\bar{y}).

By continuity of ψ¯\bar{\psi}, the right hand side converges uniformly to ψ¯(x¯)\bar{\psi}(\bar{x}_{\infty}), while the left hand side can be extended outside of |D2v¯|1|D^{2}\bar{v}|\leq 1 to a uniformly elliptic operator. Meanwhile, for any fixed s>0s>0, we use D2v¯kL(Brk)1\|D^{2}\bar{v}_{k}\|_{L^{\infty}(B_{r_{k}})}\leq 1 and v¯k(0)=Dv¯k(0)=0\bar{v}_{k}(0)=D\bar{v}_{k}(0)=0 to find a C1,α(Bs)C^{1,\alpha}(B_{s}) convergent subsequence. By the diagonalization method, we find a subsequence, also denoted v¯k\bar{v}_{k}, which converges locally uniformly in C1,αC^{1,\alpha} on n\mathbb{R}^{n} to v¯\bar{v} as kk\to\infty. Viscosity solutions are closed under C0C^{0} uniform limits and locally uniformly convergent, uniformly elliptic sequences of PDEs [CC95, Proposition 2.9], so on any fixed ball, we find that v¯\bar{v} is a viscosity solution of the special Lagrangian equation (1.3)

i=1narctanλ¯i(D2v¯(y))=ψ¯(x¯).\sum_{i=1}^{n}\arctan\bar{\lambda}_{i}(D^{2}\bar{v}(y))=\bar{\psi}(\bar{x}_{\infty}).

We also have Wloc2,pW^{2,p}_{loc} convergence. Applying the W2,δW^{2,\delta} estimate from [CC95, Prop 7.4], we get

D2v¯kD2v¯Lδ(Bs/2)C(s)v¯kv¯L(Bs)||D^{2}\bar{v}_{k}-D^{2}\bar{v}||_{L^{\delta}(B_{s/2})}\leq C(s)||\bar{v}_{k}-\bar{v}||_{L^{\infty}(B_{s})}

where the RHS goes to 0 as kk\rightarrow\infty. Using the fact that |D2v¯k|,|D2v¯|1|D^{2}\bar{v}_{k}|,|D^{2}\bar{v}|\leq 1, we see that for any p>0p>0, D2v¯kD2v¯Lp(Bs/2)||D^{2}\bar{v}_{k}-D^{2}\bar{v}||_{L^{p}(B_{s/2})} approaches 0 as kk\rightarrow\infty.

Since v¯\bar{v} solves the special Lagrangian equation with Hessian bounds InD2v¯In-I_{n}\leq D^{2}\bar{v}\leq I_{n} on n\mathbb{R}^{n}, the work of Yuan from the 2000’s now applies [Yua01]. We refer verbatim to [CSY19, pg. 9, Step 1] which shows that v¯\bar{v} is smooth under such conditions. We next apply [Yua02, pg. 122, Step B], which shows that a smooth entire solution of the constant phase equation with bounds (2.1) is quadratic. We briefly summarize the idea here: Using the calibration argument, the C0,1C^{0,1} gradient graph (x¯,Dv¯(x¯))(\bar{x},D\bar{v}(\bar{x})) is volume minimizing. The monotonicity formula [Sim83, Pg 84] combined with the flatness [Yua02, Prop 2.2] of graphical tangent cones with Hessian bounds InD2v¯In-I_{n}\leq D^{2}\bar{v}\leq I_{n}, show that v¯\bar{v} is smooth, by applying the VMO and then C2,αC^{2,\alpha} arguments from [Yua01]. On the other hand, the Hessian bounds also rule out tangent cones at infinity, giving the Bernstein theorem of [Yua02].

Continuing with our proof, we next use the Wloc2,pW^{2,p}_{loc} convergence and D2v¯=const.D^{2}\bar{v}=const. to obtain:

0=1|B1|B1|D2v¯(D2v¯)0,1|=limk1|B1|B1|D2v¯k(D2v¯k)0,1|\displaystyle 0=\frac{1}{|B_{1}|}\int_{B_{1}}|D^{2}\bar{v}-(D^{2}\bar{v})_{0,1}|=\lim_{k\rightarrow\infty}\frac{1}{|B_{1}|}\int_{B_{1}}|D^{2}\bar{v}_{k}-(D^{2}\bar{v}_{k})_{0,1}|
=limk1|Brk|Brk|D2u¯k(D2u¯k)x¯k,rk|ε,\displaystyle=\lim_{k\rightarrow\infty}\frac{1}{|B_{r_{k}}|}\int_{B_{r_{k}}}|D^{2}\bar{u}_{k}-(D^{2}\bar{u}_{k})_{\bar{x}_{k},r_{k}}|\geq\varepsilon,

which is a contradiction. ∎

By translation invariance of the VMO seminorms, D2u¯(x¯+h)D^{2}\bar{u}(\bar{x}+h) will also be in VMO(B1/2)VMO(B_{1/2}) if hh is small. This means we can conclude the following but for the sake of completeness, we provide a proof similar to Proposition 3.1.

Corollary 3.1.

Let hnh\in\mathbb{R}^{n} be sufficiently small, and u¯\bar{u} and ψ¯\bar{\psi} be as defined in Proposition 3.1. Then a continuous function K(.,.)K(.,.) of D2u¯(x¯)D^{2}\bar{u}(\bar{x}) and D2u¯(x¯+h)D^{2}\bar{u}(\bar{x}+h) is in VMO(B1/2)VMO(B_{1/2}).

Proof.

Letting u¯kh(x¯)=u¯k(x¯+h)\bar{u}^{h}_{k}(\bar{x})=\bar{u}_{k}(\bar{x}+h), we repeat the proof of Proposition 3.1, assuming instead that

1|Brk|Brk|K(D2u¯k,D2u¯khk)(K(D2u¯k,D2u¯khk))x¯k,rk|ε.\frac{1}{|B_{r_{k}}|}\int_{B_{r_{k}}}|K(D^{2}\bar{u}_{k},D^{2}\bar{u}^{h_{k}}_{k})-(K(D^{2}\bar{u}_{k},D^{2}\bar{u}^{h_{k}}_{k}))_{\bar{x}_{k},r_{k}}|\geq\varepsilon.

Rescaling as before via v¯k\bar{v}_{k} and v¯khk\bar{v}_{k}^{h_{k}}, we take subsequences and send kk\to\infty to obtain limits v¯\bar{v} and v¯h\bar{v}^{h}. The convergence is in Wloc2,p(n)W^{2,p}_{loc}(\mathbb{R}^{n}), so after a subsequence, we can assume D2v¯kD^{2}\bar{v}_{k} and D2v¯khkD^{2}\bar{v}^{h_{k}}_{k} converge almost everywhere. By the dominated convergence theorem and |D2v¯k|1|D^{2}\bar{v}_{k}|\leq 1, it follows that K(D2v¯k,D2v¯khk)K(D^{2}\bar{v}_{k},D^{2}\bar{v}_{k}^{h_{k}}) converges in Lloc1(n)L^{1}_{loc}(\mathbb{R}^{n}). In fact, v¯\bar{v} and v¯h\bar{v}^{h} are quadratic polynomials, so K(D2v¯,D2v¯h)K(D^{2}\bar{v},D^{2}\bar{v}^{h}) is a constant. Therefore we have

0=1|B1|B1|K(K)0,1|\displaystyle 0=\frac{1}{|B_{1}|}\int_{B_{1}}|K-(K)_{0,1}| =limk1|B1|B1|K(D2v¯k,D2v¯khk)(K(D2v¯k,D2v¯khk))0,1|\displaystyle=\lim_{k\to\infty}\frac{1}{|B_{1}|}\int_{B_{1}}|K(D^{2}\bar{v}_{k},D^{2}\bar{v}_{k}^{h_{k}})-(K(D^{2}\bar{v}_{k},D^{2}\bar{v}_{k}^{h_{k}}))_{0,1}|
=limk1|Brk|Brk|K(D2u¯k,D2u¯khk)(K(D2u¯k,D2u¯khk))x¯k,rk|\displaystyle=\lim_{k\to\infty}\frac{1}{|B_{r_{k}}|}\int_{B_{r_{k}}}|K(D^{2}\bar{u}_{k},D^{2}\bar{u}^{h_{k}}_{k})-(K(D^{2}\bar{u}_{k},D^{2}\bar{u}_{k}^{h_{k}}))_{\bar{x}_{k},r_{k}}|
ε,\displaystyle\geq\varepsilon,

which is a contradiction. ∎

Note that the VMO(B1/2)VMO(B_{1/2}) seminorms of K(D2u¯,D2u¯h)K(D^{2}\bar{u},D^{2}\bar{u}^{h}) are independent of hh if hh is small. The point of KK is we need to take a difference quotient of (2.5).

Proposition 3.2 (C2,αC^{2,\alpha} Estimates).

Let u¯\bar{u} be a C1,1C^{1,1} viscosity solution of (2.5) in B1(0)nB_{1}(0)\subset\mathbb{R}^{n}, where |D2u¯|1|D^{2}\bar{u}|\leq 1 and ψ¯\bar{\psi} is Lipschitz continuous. Then u¯C2,α(B1/2)\bar{u}\in C^{2,\alpha}(B_{1/2}) for all α(0,1)\alpha\in(0,1).

Proof.

Letting vh=[u¯(x¯+h)u¯(x¯)]/|h|v^{h}=[\bar{u}(\bar{x}+h)-\bar{u}(\bar{x})]/|h|, we obtain the linearized equation

(3.1) Fijhvijh=ψ¯h(x¯),\displaystyle F^{h}_{ij}v^{h}_{ij}=\bar{\psi}^{h}(\bar{x}),

where

Fh=01(I+((1t)D2u¯(x¯)+tD2u¯(x¯+h))2)1𝑑t,ψ¯h(x¯)=ψ¯(x¯+h)ψ¯(x¯)|h|F^{h}=\int_{0}^{1}\Big{(}I+((1-t)D^{2}\bar{u}(\bar{x})+tD^{2}\bar{u}(\bar{x}+h))^{2}\Big{)}^{-1}dt,\qquad\bar{\psi}^{h}(\bar{x})=\frac{\bar{\psi}(\bar{x}+h)-\bar{\psi}(\bar{x})}{|h|}

and we use the Einstein summation notation. For small hh, equation (3.1) holds pointwise (in fact, u¯(x¯)\bar{u}(\bar{x}) is twice differentiable everywhere, which is easily shown using the rescaling procedure in Proposition 3.1) on B1/2B_{1/2}, and can be thought of as a linear equation for vhv^{h} in nondivergence form, with, by Corollary 3.1, VMOlocVMO_{loc} coefficients FijhF^{h}_{ij} and LlocL^{\infty}_{loc} right hand side ψ¯h\bar{\psi}^{h}, each of whose seminorms are independent of hh. Recalling the interior W2,pW^{2,p} estimates due to [CFL91], see also [Vit92, Theorem 2.1], (although these estimates assume solutions are in W02,p(Ω)W^{2,p}_{0}(\Omega), adding a cutoff function as in [GT01, proof of Theorem 9.11] yields standard interior estimates), we deduce that p\forall p large, vhWloc2,pv^{h}\in W^{2,p}_{loc} inside a slightly smaller domain in x¯(B1)\bar{x}(B_{1}) with local estimates independent of hh. Since for difference quotient vhv^{h} we have D2vhLlocpD^{2}v^{h}\in L^{p}_{loc}, it follows that D2u¯Wloc1,pD^{2}\bar{u}\in W^{1,p}_{loc} for all large pp, hence by the Sobolev Embedding Theorem D2u¯Cα(B1/2)D^{2}\bar{u}\in C^{\alpha}(B_{1/2}) for all α(0,1)\alpha\in(0,1). ∎

Now from Schauder theory, the rotated potential u¯(x¯)\bar{u}(\bar{x}) is as regular as the equation allows.

Corollary 3.2.

Let uu be a convex viscosity solution of (1.1) on B1(0)B_{1}(0), where ψ(x)\psi(x) is Lipschitz. Then rotated potential u¯(x¯)\bar{u}(\bar{x}) is a C2,αC^{2,\alpha} solution of (2.5) on x¯(B1(0))\bar{x}(B_{1}(0)) for all α(0,1)\alpha\in(0,1). If ψC2,α\psi\in C^{2,\alpha} for some α(0,1)\alpha\in(0,1), then u¯C4,α\bar{u}\in C^{4,\alpha}.

Indeed, since u¯C1,1\bar{u}\in C^{1,1}, we have Du¯C0,1D\bar{u}\in C^{0,1} and ψ¯C0,1\bar{\psi}\in C^{0,1}, and Proposition 3.2 applies, so Du¯C1,αD\bar{u}\in C^{1,\alpha}. If we also know ψC2,α\psi\in C^{2,\alpha}, then this means ψ¯C1,α\bar{\psi}\in C^{1,\alpha}. Recalling equation (3.1) for the difference quotient of u¯\bar{u}, it follows from Schauder estimates that Du¯C2,αD\bar{u}\in C^{2,\alpha}, so ψ¯C2,α\bar{\psi}\in C^{2,\alpha}. Taking two difference quotients in a similar way, we deduce D2u¯C2,αD^{2}\bar{u}\in C^{2,\alpha}.

4. Proof of Theorem 1.1

The final step is to show that λ¯max<1\bar{\lambda}_{max}<1 on x¯(B1)\bar{x}(B_{1}). Indeed, once we prove this, we can compare with quadratics to convert to original variables. Let Q¯(x¯)\bar{Q}(\bar{x}) touch u¯\bar{u} from above near x¯\bar{x} and suppose, after lowering, that D2Q¯<InD^{2}\bar{Q}<I_{n}. By the order preservation of rotations, we see that Q(x)Q(x) touches uu from above near xx. Moreover, D2Q<D^{2}Q<\infty by the transformation law

D2Q(x)=I+AIAA=D2Q¯(x¯).D^{2}Q(x)=\frac{I+A}{I-A}\,\qquad A=D^{2}\bar{Q}(\bar{x}).

Thus λmax<\lambda_{max}<\infty on B1B_{1}, i.e. uC1,1(B1)u\in C^{1,1}(B_{1}). This means x¯(x)=cx+sDu(x)\bar{x}(x)=cx+sDu(x) is Lipschitz, so the above formula with QQ replaced by uu implies uC2,1(B1)u\in C^{2,1}(B_{1}). This means x¯C1,1\bar{x}\in C^{1,1}, and as before, we deduce uC3,1(B1)u\in C^{3,1}(B_{1}). Since D2u¯C2,α(B1)D^{2}\bar{u}\in C^{2,\alpha}(B_{1}) and x¯C2,1\bar{x}\in C^{2,1}, we conclude that uC4,α(B1)u\in C^{4,\alpha}(B_{1}). We now establish the desired inequality.

Remark 4.1.

We need ψC2,α\psi\in C^{2,\alpha} only for the following proposition.

Proposition 4.1.

Let uu be a convex viscosity solution of (1.1) on B1(0)B_{1}(0), with ψ(x)C2,α\psi(x)\in C^{2,\alpha}. Then λ¯max<1\bar{\lambda}_{max}<1 on x¯(B1(0))\bar{x}(B_{1}(0)).

Proof.

Suppose that λ¯max=1\bar{\lambda}_{max}=1 at a point x¯0\bar{x}_{0}, or more generally that 1=λ¯:=λ¯1==λ¯m>λ¯m+1λ¯n1=\bar{\lambda}:=\bar{\lambda}_{1}=\cdots=\bar{\lambda}_{m}>\bar{\lambda}_{m+1}\geq\cdots\geq\bar{\lambda}_{n} at x¯0\bar{x}_{0}. It follows that the following function is C2,αC^{2,\alpha} for x¯\bar{x} near x0¯\bar{x_{0}}: b¯m:=1m1mln1+λ¯k2\bar{b}_{m}:=\frac{1}{m}\sum_{1}^{m}\ln\sqrt{1+\bar{\lambda}_{k}^{2}}. Fixing x¯\bar{x}, we assume D2u¯D^{2}\bar{u} is diagonal at x¯\bar{x}, with u¯i¯i¯(x¯)=λ¯i(x¯)\bar{u}_{\bar{i}\bar{i}}(\bar{x})=\bar{\lambda}_{i}(\bar{x}). Note that u¯ii¯\bar{u}_{\bar{ii}} refers to the double partial derivatives of the function u¯\bar{u} w.r.t to xi¯\bar{x_{i}}.

From [Bha21, Lemma 4.1] we get the following:

(4.1) mΔg¯b¯m=Z~+i=1mλ¯i1+λ¯i2ψ¯i¯i¯mi=1mλ¯ig¯i¯i¯ψ¯i¯i¯b¯mm\Delta_{\bar{g}}\bar{b}_{m}=\tilde{Z}+\sum_{i=1}^{m}\frac{\bar{\lambda}_{i}}{1+\bar{\lambda}_{i}^{2}}\bar{\psi}_{\bar{i}\bar{i}}-m\sum_{i=1}^{m}\bar{\lambda}_{i}\bar{g}^{\bar{i}\bar{i}}\bar{\psi}_{\bar{i}}\partial_{\bar{i}}\bar{b}_{m}

where

Z~=km(1+λ¯2)h¯kkk¯2+(i<km+k<im)(3+3λ¯2)h¯iik¯2+km<i2λ¯(1+λ¯λ¯i)λ¯λ¯ih¯iik¯2\displaystyle\tilde{Z}=\sum_{k\leq m}(1+\bar{\lambda}^{2})\bar{h}^{2}_{\overline{kkk}}+(\sum_{i<k\leq m}+\sum_{k<i\leq m})(3+3\bar{\lambda}^{2})\bar{h}_{\overline{iik}}^{2}+\sum_{k\leq m<i}\frac{2\bar{\lambda}(1+\bar{\lambda}\bar{\lambda}_{i})}{\bar{\lambda}-\bar{\lambda}_{i}}\bar{h}^{2}_{\overline{iik}}
+im<k3λ¯λ¯k+λ¯2(λ¯+λ¯k)λ¯λ¯kh¯iik¯2+2[i<j<km(3+3λ¯2)h¯ijk¯2+i<jm<k[1+2λ¯λ¯λ¯k+\displaystyle+\sum_{i\leq m<k}\frac{3\bar{\lambda}-\bar{\lambda}_{k}+\bar{\lambda}^{2}(\bar{\lambda}+\bar{\lambda}_{k})}{\bar{\lambda}-\bar{\lambda}_{k}}{\bar{h}_{\overline{iik}}}^{2}+2\Bigg{[}\sum_{i<j<k\leq m}(3+3\bar{\lambda}^{2})\bar{h}_{\overline{ijk}}^{2}+\sum_{i<j\leq m<k}[1+\frac{2\bar{\lambda}}{\bar{\lambda}-\bar{\lambda}_{k}}+
λ¯2(λ¯+λ¯k)λ¯λ¯k]h¯ijk¯2+im<j<kλ¯[λ¯j+λ¯k+1+λ¯j2λ¯λ¯j+1+λ¯k2λ¯λ¯k]h¯ijk¯2]\displaystyle\frac{\bar{\lambda}^{2}(\bar{\lambda}+\bar{\lambda}_{k})}{\bar{\lambda}-\bar{\lambda}_{k}}]\bar{h}_{\overline{ijk}}^{2}+\sum_{i\leq m<j<k}\bar{\lambda}[\bar{\lambda}_{j}+\bar{\lambda}_{k}+\frac{1+\bar{\lambda}_{j}^{2}}{\bar{\lambda}-\bar{\lambda}_{j}}+\frac{1+\bar{\lambda}_{k}^{2}}{\bar{\lambda}-\bar{\lambda}_{k}}]\bar{h}_{\overline{ijk}}^{2}\Bigg{]}

with

h¯ijk¯=g¯ii¯g¯jjg¯kku¯ijk¯ and g¯ii=11+λ¯i2.\displaystyle\bar{h}_{\overline{ijk}}=\sqrt{\bar{g}^{\overline{ii}}}\sqrt{\bar{g}^{jj}}\sqrt{\bar{g}^{kk}}\bar{u}_{\overline{ijk}}\text{ and }\bar{g}^{ii}=\frac{1}{1+\bar{\lambda}_{i}^{2}}.

Again following the notation introduced in [Bha21, pg 11], for each fixed kk in the above expression, we set t¯i=h¯iik¯\bar{t}_{i}=\bar{h}_{\bar{iik}} and write

H¯k=t¯1++t¯n1+t¯n=t¯+t¯n\displaystyle\bar{H}^{k}=\bar{t}_{1}+...+\bar{t}_{n-1}+\bar{t}_{n}=\bar{t^{\prime}}+\bar{t}_{n}

where H¯k\bar{H}^{k} denotes the kkth component of the mean curvature vector (given by (1.2): H¯k=g¯kkψ¯k¯\bar{H}^{k}=\bar{g}^{kk}\bar{\psi}_{\bar{k}}), i.e. the component of the mean curvature vector along J(ek¯,D¯u¯ek¯)J(\bar{e_{k}},\bar{D}\bar{u}_{\bar{e_{k}}}) with ek¯\bar{e_{k}} being the kthk^{th} eigendirection of D2u¯D^{2}\bar{u}. One can re-write

Z~=(constant phase terms)+Z0~\tilde{Z}=\text{(constant phase terms)}+\tilde{Z_{0}}

where for each fixed kmk\leq m, the kkth term of Z0~\tilde{Z_{0}} is given by

[Z0~]k=2λ¯nλ¯λ¯n[(H¯k)22H¯kt¯].[\tilde{Z_{0}}]_{k}=\frac{2\bar{\lambda}_{n}}{\bar{\lambda}-\bar{\lambda}_{n}}[(\bar{H}^{k})^{2}-2\bar{H}^{k}\bar{t}^{\prime}].

By constant phase terms, we denote terms without dependence on the variable phase ψ(x)\psi(x), which are therefore the same as in the ψ=const.\psi=const. case considered by [CSY19]. The constant phase terms are nonnegative if the Hessian bounds (2.1) are true, as in [CSY19, Section 3].

Using (2.6), we note the following

[Z0~]k=λ¯nλ¯λ¯n(g¯kk¯)2(kψ)2(1λ¯k)222λ¯nλ¯λ¯ng¯kk¯(kψ)(1λ¯k)t¯\displaystyle[\tilde{Z_{0}}]_{k}=\frac{\bar{\lambda}_{n}}{\bar{\lambda}-\bar{\lambda}_{n}}(\bar{g}^{\overline{kk}})^{2}(\partial_{k}\psi)^{2}(1-\bar{\lambda}_{k})^{2}-\frac{2\sqrt{2}\bar{\lambda}_{n}}{\bar{\lambda}-\bar{\lambda}_{n}}\bar{g}^{\overline{kk}}(\partial_{k}\psi)(1-\bar{\lambda}_{k})\bar{t}^{\prime}
(4.2) C(|ψ|C1)(1λ¯k)[(1λ¯k)+1].\displaystyle\geq-C(|\psi|_{C^{1}})(1-\bar{\lambda}_{k})[(1-\bar{\lambda}_{k})+1].

Before dealing with (4.2), we would first like to deal with the second and third terms of (4.1), since (4.2) can be treated similarly.

The third term of (4.1) involving b¯m\nabla\bar{b}_{m} is harmless, so it suffices to lower bound the second term, which will have two contributions. Recalling (2.6),

(4.3) ψ¯ii¯=2x¯i2ψ(x¯Du¯(x¯)2)=12ψaa¯λ¯i+12ψii(1λ¯i)2.\bar{\psi}_{\bar{ii}}=\frac{\partial^{2}}{\partial\bar{x}_{i}^{2}}\psi\left(\frac{\bar{x}-D\bar{u}(\bar{x})}{\sqrt{2}}\right)=-\frac{1}{\sqrt{2}}\psi_{a}\partial_{\bar{a}}\bar{\lambda}_{i}+\frac{1}{2}\psi_{ii}(1-\bar{\lambda}_{i})^{2}.

The first term of (4.3) yields a harmless contribution to the maximum principle:

a=1nψai=1mλ¯i1+λ¯i2a¯λ¯i=ma=1nψaa¯b¯m.\sum_{a=1}^{n}\psi_{a}\sum_{i=1}^{m}\frac{\bar{\lambda}_{i}}{1+\bar{\lambda}_{i}^{2}}\partial_{\bar{a}}\bar{\lambda}_{i}=m\sum_{a=1}^{n}\psi_{a}\partial_{\bar{a}}\bar{b}_{m}.

For the second term of (4.3), we start with

(4.4) 12i=1mλ¯i1+λ¯i2ψii(1λ¯i)2c(x¯)(1λ¯m)2,\frac{1}{2}\sum_{i=1}^{m}\frac{\bar{\lambda}_{i}}{1+\bar{\lambda}_{i}^{2}}\psi_{ii}(1-\bar{\lambda}_{i})^{2}\geq-c(\bar{x})(1-\bar{\lambda}_{m})^{2},

for some locally bounded c(x¯)c(\bar{x}). Next, we note that λ¯m>0\bar{\lambda}_{m}>0 for x¯\bar{x} nearby x0x_{0}. By the convexity of b¯(t):=ln1+t2\bar{b}(t):=\ln\sqrt{1+t^{2}} in [0,1][0,1],

0<b¯(1)b¯(0)10b¯(1)b¯(t)1t,0<\frac{\bar{b}(1)-\bar{b}(0)}{1-0}\leq\frac{\bar{b}(1)-\bar{b}(t)}{1-t},

so putting t=λ¯m(x¯)t=\bar{\lambda}_{m}(\bar{x}) yields

(4.5) (1λ¯m)2C(b¯(1)b¯(λ¯m))2C(mb¯(1)i=1mb¯(λ¯i))2.(1-\bar{\lambda}_{m})^{2}\leq C(\bar{b}(1)-\bar{b}(\bar{\lambda}_{m}))^{2}\leq C(m\bar{b}(1)-\sum_{i=1}^{m}\bar{b}(\bar{\lambda}_{i}))^{2}.

We thus conclude that in a sufficiently small neighborhood of x¯\bar{x},

Δg¯b¯ma(x¯),g¯b¯mg¯c(x¯)(b¯m,maxb¯m)\Delta_{\bar{g}}\bar{b}_{m}\geq\langle a(\bar{x}),\nabla_{\bar{g}}\bar{b}_{m}\rangle_{\bar{g}}-c(\bar{x})(\bar{b}_{m,max}-\bar{b}_{m})

for some bounded continuous a,ca,c, where b¯m,max=b¯m|λ¯1==λ¯m=1\bar{b}_{m,max}=\bar{b}_{m}|_{\bar{\lambda}_{1}=\cdots=\bar{\lambda}_{m}=1}. We make a quick note here: The bound given by (4.2) can be treated in an exactly similar manner as above.

The strong maximum principle still holds because the right side vanishes at an interior maximum, according to [GT01, Lemma 3.4 and Theorem 3.5]. It follows that b¯mb¯m,max\bar{b}_{m}\equiv\bar{b}_{m,max} and λ¯max1\bar{\lambda}_{max}\equiv 1 on an open set containing x¯\bar{x}. Since x¯(B1)\bar{x}(B_{1}) is connected, we conclude this is true everywhere: λ¯max1\bar{\lambda}_{max}\equiv 1. However, because u(x)u(x) is bounded, we can touch it from above somewhere in B1(0)B_{1}(0) by a sufficiently tall quadratic QQ. The rotation Q¯\bar{Q} then touches u¯\bar{u} from above somewhere in x¯(B1)\bar{x}(B_{1}). But D2Q<D^{2}Q<\infty corresponds (see [CSY19, end of section 3]) to D2Q¯<InD^{2}\bar{Q}<I_{n}, a contradiction. ∎

5. Proof of Theorem 1.2

Proof.

We now prove Hessian estimate (1.5) by compactness. If the estimate fails, then there is a sequence of C4,αC^{4,\alpha} convex solutions uku_{k} and C2,αC^{2,\alpha} phases ψk\psi_{k} to (1.1) with

λmax[D2uk(0)],uk(0)=Duk(0)=0\displaystyle\lambda_{max}[D^{2}u_{k}(0)]\to\infty,\qquad u_{k}(0)=Du_{k}(0)=0
ukC1(B1/2(0))+ψkC2,α(B1/2(0))C.\displaystyle\|u_{k}\|_{C^{1}(B_{1/2}(0))}+\|\psi_{k}\|_{C^{2,\alpha}(B_{1/2}(0))}\leq C.

Since ukC1\|u_{k}\|_{C^{1}} is bounded, we can pass to a subsequence and assume uku_{k} converges uniformly to uu on B1/2(0)B_{1/2}(0). Note that uu is necessarily convex, so u~:=12(u+12|x|2)\tilde{u}:=\frac{1}{\sqrt{2}}(u+\frac{1}{2}|x|^{2}), as in Section 2, is uniformly convex. This means u~(Br(0))\partial\tilde{u}(B_{r}(0)) is open and contains Br/2(0)B_{r/\sqrt{2}}(0), for 0<r1/20<r\leq 1/2. Moreover, if we shrink slightly and suppose x¯u~(B1/2δ(0))\bar{x}\in\partial\tilde{u}(B_{1/2-\delta}(0)), then x¯u~k(B1/2(0))\bar{x}\in\partial\tilde{u}_{k}(B_{1/2}(0)) for large enough kk, since if x¯u~k(xk)\bar{x}\in\partial\tilde{u}_{k}(x_{k}), then uniform convexity yields, via (2.4),

|xxk|2Cu~u~kL(B1/2(0)0.|x-x_{k}|^{2}\leq C\|\tilde{u}-\tilde{u}_{k}\|_{L^{\infty}(B_{1/2}(0)}\to 0.

So the rotated sequence u¯k\bar{u}_{k} is defined on arbitrarily large subsets of u~(B1/2(0))\partial\tilde{u}(B_{1/2}(0)), converging uniformly to u¯\bar{u} thereabouts by the order preservation of rotation. It follows that u¯\bar{u} is the locally uniform limit on u~(B1/2(0))\partial\tilde{u}(B_{1/2}(0)) of smooth rotations u¯k\bar{u}_{k}.

The smooth rotations u¯k\bar{u}_{k} have eigenvalues which blowup: λ¯max,k(0)1\bar{\lambda}_{max,k}(0)\to 1. To see this for u¯\bar{u}, we use the C2,αC^{2,\alpha} estimates for u¯k\bar{u}_{k}, noting that ψk\psi_{k} converges to some ψC2,α(B1/2(0))\psi\in C^{2,\alpha}(B_{1/2}(0)) in the norm of C2,α/2(B1/2(0))C^{2,\alpha/2}(B_{1/2}(0)) after taking a subsequence. Along a subsequence, it follows that u¯k\bar{u}_{k} eventually converges locally in C4,α/2C^{4,\alpha/2} to u¯\bar{u} in u~(B1/2(0))\partial\tilde{u}(B_{1/2}(0)), so λ¯(0)=1\bar{\lambda}(0)=1. Moreover, u¯\bar{u} is a C4,αC^{4,\alpha} solution of the rotated equation F¯(D2u)=ψ¯\bar{F}(D^{2}u)=\bar{\psi}, so λ¯max1\bar{\lambda}_{max}\equiv 1 by the strong maximum principle arguments in Proposition 4.1. This is a contradiction, since λ¯max<1\bar{\lambda}_{max}<1 somewhere on u~(B1/2(0))\partial\tilde{u}(B_{1/2}(0)) for bounded convex uu. ∎

Remark 5.1.

In fact, a stronger Hessian estimate than (1.5) holds:

(5.1) |D2u(0)|C1exp[C2(oscB1/2u)2n2]|D^{2}u(0)|\leq C_{1}\exp[C_{2}\,(osc_{B_{1/2}}u)^{2n-2}]

where C1C_{1} and C2C_{2} are positive constants depending on ψC1,1(B1/2)||\psi||_{C^{1,1}(B_{1/2})} and nn. This result follows from the methods in [Bha21]; the proof in [Bha21] goes through if the supercriticality condition |ψ|(n2)π/2+δ|\psi|\geq(n-2)\pi/2+\delta is replaced by the convexity condition D2u0D^{2}u\geq 0. A weaker estimate for such smooth solutions was obtained earlier in [War08, Theorem 8].

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