Research article Topical Sections

The directed preparation of TiO2 nanotubes film on FTO substrate via hydrothermal method for gas sensing application

  • In this research, we directly synthesized TiO2 nanotubes film on Fluorine doped Tin oxide (FTO) substrate via hydrothermal method from commercial TiO2 in NaOH solution at 135 ℃ for 24 hours. The samples were characterized by X-ray diffraction (XRD) pattern, field emission scanning electron microscopy (FESEM) and transmitting electron microscopy (TEM). The average diameter of TiO2 nanotubes (TNTs) is about 10–12 nm and their length is about a few hundred nanometers. The sensitivity ability of TNTs increases as the gas concentration increases and developing to the highest sensitivity of TNTs is 2.4 at 700 ppm of the ethanol concentration. The same as the gas concentration, the sensitivity of TNTs increases when the temperature increases. Besides, the sensitivity of samples at 250 ℃ is doubled compared to samples determined at 100 ℃.

    Citation: Pham Van Viet, Le Van Hieu, Cao Minh Thi. The directed preparation of TiO2 nanotubes film on FTO substrate via hydrothermal method for gas sensing application[J]. AIMS Materials Science, 2016, 3(2): 460-469. doi: 10.3934/matersci.2016.2.460

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  • In this research, we directly synthesized TiO2 nanotubes film on Fluorine doped Tin oxide (FTO) substrate via hydrothermal method from commercial TiO2 in NaOH solution at 135 ℃ for 24 hours. The samples were characterized by X-ray diffraction (XRD) pattern, field emission scanning electron microscopy (FESEM) and transmitting electron microscopy (TEM). The average diameter of TiO2 nanotubes (TNTs) is about 10–12 nm and their length is about a few hundred nanometers. The sensitivity ability of TNTs increases as the gas concentration increases and developing to the highest sensitivity of TNTs is 2.4 at 700 ppm of the ethanol concentration. The same as the gas concentration, the sensitivity of TNTs increases when the temperature increases. Besides, the sensitivity of samples at 250 ℃ is doubled compared to samples determined at 100 ℃.


    For each $ 1\leq k\leq N $, the $ k $-Hessian operator acting on $ u \in C^2(\Omega) $ with $ \Omega \subseteq {\mathbb R}^N $ open is defined by

    $ Sk(D2u):=σk(λ(D2u)):=1i1<<ikNλi1(D2u)λik(D2u)
    $
    (1.1)

    where $ \lambda(D^2u) $ indicates the $ N $-vector of ordered eigenvalues of the Hessian matrix $ D^2u $ and $ \sigma_k(\lambda) $ is the elementary symmetric polynomial, which is homogeneous of degree $ k $. For example, one has

    $ S_1(D^2u) = \Delta u = {\rm tr}(D^2u)\ \quad \mbox{and} \quad S_N(D^2u) = {\rm det}(D^2u). $

    Before describing the scope of this paper, let us mention that, for each $ k > 1 $, the $ k $-Hessian is fully nonlinear and is (degenerate) elliptic only when constrained in a suitable sense. More precisely, in general one does not have

    $ XYSk(X)Sk(Y)
    $
    (1.2)

    if $ X, Y $ are free to range over all of $ \mathcal{S}(N) $, the space of $ N \times N $ symmetric matrices. However, one will have (1.2) if one constrains $ X $ (and hence $ Y $) to belong to

    $ Σk:={AS(N): λ(A)¯Γk}
    $
    (1.3)

    where

    $ Γk:={λRN: σj(λ)>0, j=1,,k}.
    $
    (1.4)

    This leads us to work in the context of admissible viscosity solutions, using the notion of elliptic sets as introduced by Krylov [23]. This notion has given rise to the development of an organic theory of viscosity solutions with admissibility constraints beginning with Harvey-Lawson [11] for pure second order operators on Euclidean space and generalized to general operators on Riemannian manifolds in [13]. In the terminology of [7], $ \Sigma_k $ is a (constant coefficient) pure second order subequation constraint set which requires that $ \Sigma_k \subset \mathcal{S}(N) $ be a proper closed subset satisfying the positivity property

    $ AΣk  A+PΣk  for each PP,  P:={PS(N): P0}
    $
    (1.5)

    and the topological property

    $ Σk=¯Σk,
    $
    (1.6)

    which is the closure in $ \mathcal{S}(N) $ of the interior of $ \Sigma_k $.

    In the nonlinear potential theory language of [11], one would say that $ u \in \mathrm{USC}(\Omega) $ is $ \Sigma_k $-subharmonic at $ x_0 $ if $ u $ is $ k $-convex at $ x_0 \in \Omega $ in the sense of Definition 2.1. Moreover, one has the following coherence property: if $ u \in \mathrm{USC}(\Omega) $ is twice differentiable in $ x_0 $ then

    $ u is Σk-subharmonic at x0    D2u(x0)Σk;
    $
    (1.7)

    that is, the classical and viscosity notions of $ k $-convexity coincide at points of twice differentiability. We notice that the reverse implication $ (\Leftarrow) $ depends on the positivity property (1.5) of $ \Sigma_k $. The topological property (1.6) is sufficient for the local construction of classical strict subsolutions $ \varphi $; that is, $ S_k(D^2 \varphi) < 0 $. It also plays and important role in the Harvey-Lawson duality which leads to an elegant formulation of supersolutions by duality (see Remark 2.12 and Proposition 3.2 of [7] for details).

    The main purpose of this paper is to study the principal eigenvalue associated to the operator $ -S_k $ with homogeneous Dirichlet data in bounded domains $ \Omega $ by using maximum principle methods. We shall consider $ \Omega \subset {\mathbb R}^N $ whose boundaries are of class $ C^2 $ and $ (k-1) $-convex. The notion of principal eigenvalue that we will define is inspired by that of Berestycki, Nirenberg and Varadhan in their groundbreaking paper [1].

    More precisely, for each $ k \in \{1, \ldots, N\} $ fixed, using the notion of $ k $-convexity in a viscosity sense, we introduce

    $ \Phi_k^{-}(\Omega) : = \{ \psi \in \mathrm{USC}(\Omega): \psi \ \text{is $k$-convex and negative in} \ \Omega\}. $

    We can then consider

    $ \Lambda_k: = \{ \lambda \in {\mathbb R}: \ \exists \psi \in \Phi_k^{-}(\Omega)\ \text{with} \ S_k(D^2 \psi) + \lambda \psi |\psi|^{k-1} \geq 0 \ \text{in} \ \Omega \}, $

    where the inequality above is again in the admissible viscosity sense, and define our candidate for a (generalized) principal eigenvalue by

    $ \lambda_1^{-}: = \sup \Lambda_k. $

    We will prove that $ \lambda_1^{-} $ is an upper bound for the validity of the minimum principle in $ \Omega $; that is, we will show that for any $ \lambda < \lambda_1^{-} $ the operator $ F[\cdot] = S_k(D^2\cdot)+\lambda \cdot |\cdot|^{k-1} $ satisfies the minimum principle in $ \Omega $ (see Theorem 5.4). Moreover, in Theorem 6.6 we will show that $ \lambda_1^{-} $ is actually an eigenvalue for the operator $ -S_k $ in the sense that there exists $ \psi_1 < 0 $ in $ \Omega $ such that

    $ \left\{ Sk(D2ψ1)+λ1ψ1|ψ1|k1=0in Ωψ1=0on Ω.
    \right. $

    Notice that is the linear case $ k = 1 $ this conforms to the usual notion of eigenvalue. If $ k $ is odd integer, then $ S_k $ is an odd operator and we would have a maximum principle characterization for $ \lambda_1^+ $; that is, a principal eigenvalue which corresponds to a positive concave principal eigenfunction.

    We should mention that the $ k $-Hessians are variational and hence it is possible to give a variational characterization of the principal eigenvalue through a generalized Rayleigh quotient. This was done by Lions [26] for $ k = N $ and by Wang [32] for general $ k $. Using the minimum principle, we prove that both characterizations coincide (see Corollary 5.7). Hence the existence of the eigenfunction corresponding to the so-called eigenvalue is just a consequence of this equality, using the results in [26,32].

    Nonetheless, we wish to give a proof of the existence that is independent of the variational characterization. Indeed, the interest in defining the principal eigenvalue by way of (5.4) is twofold. On the one hand, it allows one to prove the minimum principle for $ \lambda $ below $ \lambda_1^{-} $ while on the other hand, it strongly suggests that it may be possible to extend the results to a class of fully non linear operators that are not variational, but which may include the $ k $-Hessians. For example, with $ 0 < \alpha\leq \beta $ and $ S_{\alpha, \beta} = \{A\in \mathcal{S}(N): \ \alpha I\leq A\leq \beta I\} $, one might consider the operators defined by

    $ \sigma_k^+(D^2u): = \sup\limits_{A\in S_{\alpha,\beta}}\sigma_k(\lambda(AD^2u)). $

    This will be the subject of a subsequent paper.

    We should also mention that the challenges for a viscosity solution approach to the existence of a solution $ \psi_1 $ to the eigenvalue problem

    $ {Sk(D2ψ1)+λ1ψ1|ψ1|k1=0in Ωψ1=0on Ω
    $
    (1.8)

    include the lack of global monotonicity in the Hessian $ D^2 \psi_1 $ and the "wrong" monotonicity in $ \psi_1 $. The argument will involve an iterative construction that has its origins in [2,3] and was used with success in degenerate settings in [4]. At some point in the argument, a compactness property is needed for the sequence of $ k $-convex solutions to the approximating equations. The needed compactness property follows from a global Hölder estimate on the sequence of approximating solutions. Unfortunately, using merely maximum principle methods, we are able to prove the estimate only in the case when $ k > \frac{N}{2} $. See Remark 6.4 for a discussion of this point, including the use of some measure theoretic techniques (to augment the maximum principle techniques developed herein) in order establish existence in the nonlinear range $ 1 < k \leq \frac{N}{2} $.

    In all that follows, $ \Omega $ will be a bounded open domain in $ {\mathbb R}^N $, $ \mathcal{S}(N) $ is the space of $ N \times N $ symmetric matrices with real entries and

    $ λ1(A)λN(A)
    $
    (2.1)

    are the $ N $ eigenvalues of $ A \in \mathcal{S}(N) $ written in increasing order. The spaces of upper, lower semi-continuous functions on $ \Omega $ taking values in $ [-\infty, +\infty), (-\infty, +\infty] $ will be denoted by $ \mathrm{USC}(\Omega), \mathrm{LSC}(\Omega) $ respectively.

    We begin by describing the subset $ \Sigma_k \subset \mathcal{S}(N) $ which serves to define $ k $-convex functions by way of a viscosity constraint on the Hessian of $ u \in \mathrm{USC}(\Omega) $. For $ k \in \{1, \ldots, N\} $ denote by

    $ σk(λ):=1i1<<ikNλi1λik
    $
    (2.2)

    the kth-elementary symmetric function of $ \lambda \in {\mathbb R}^N $ and consider the open set defined by

    $ Γk:={λRN: σj(λ)>0, j=1,,k},
    $
    (2.3)

    which is clearly a cone with vertex at the origin and satisfies

    $ Γ+ΓNΓN1Γ1
    $
    (2.4)

    where $ \Gamma^+ : = \{ \lambda \in {\mathbb R}^N: \ \lambda_i > 0 \ \ \text{for each} \ i \} $ is the positive cone in $ {\mathbb R}^N $. The obvious inclusion $ \Gamma^+ \subset \Gamma_N $ is, in fact, an identity (2.14), as will be discussed below.

    Additional fundamental properties of the cones $ \Gamma_k $ are most easily seen by using other alternate characterizations of (2.3). First, the homogeneous polynomials (2.2) are examples of hyperbolic polynomials in the sense of Gårding. More precisely, for each fixed $ k $, $ \sigma_k $ is homogeneous of degree $ k $ and is hyperbolic in the direction $ a = (1, \ldots, 1) \in {\mathbb R}^N $; that is, the degree $ k $ polynomial in $ t \in {\mathbb R} $ defined by

    $ σk(ta+λ)=1i1<<ikN(t+λi1)(t+λik)
    $
    (2.5)

    has $ k $ real roots for each $ \lambda \in {\mathbb R}^N $. The cone $ \Gamma_k $ can be defined as

    $ Γk is the connected component of {λRN:σk(λ)>0} containing (1,,1),
    $
    (2.6)

    from which it follows that

    $ λΓk    σk(λ)=0.
    $
    (2.7)

    The form (2.6) of $ \Gamma_k $ corresponds to Gårding's original definition for a general hyperbolic polynomial for which the form (2.3) results in the special case of the $ k $th- elementary symmetric function $ \sigma_k $. The reader might wish to consult section 1 of Caffarelli-Nirenberg-Spruck [5].

    Gårding's beautiful theory of hyperbolic polynomials in [9] applied to $ \sigma_k $ includes two important consequences; namely convexity

    $  the cone Γk is convex
    $
    (2.8)

    and (strict) monotonicity

    $ σk(λ+μ)>σk(λ)  for each λ,μΓk.
    $
    (2.9)

    Since $ \Gamma^+ \subset \Gamma_k $ for each $ k $ and $ \Gamma_k $ is a cone, one has that $ \Gamma_k $ is a monotonicity cone for itself; that is,

    $ Γk+ΓkΓk
    $
    (2.10)

    and, in particular,

    $ Γ++ΓkΓk,
    $
    (2.11)

    which, with the monotonicity (2.9) for $ \mu \in \Gamma^+ $, gives rise to the degenerate ellipticity of $ k $-Hessian operators as it will be recalled below.

    Moreover, Korevaar [21] has characterized $ \Gamma_k $ as

    $ Γk={λRN: σk(λ)>0,σkλi1(λ)>0,,k1σkλi1λik1(λ)>0 for all {1i1<<ik1N}}
    $
    (2.12)

    which implies that

    $ Nk+1j=1λij>0  on Γk  for all  {1i1<<ik1N}.
    $
    (2.13)

    When $ k = N $ this says that each $ \lambda_i > 0 $ for each $ i $ and hence

    $ ΓN=Γ+.
    $
    (2.14)

    Additional characterizations of $ \Gamma_k $, interesting and useful identities and inequalities involving $ \sigma_k $ can be found in [5,18,19,20,25,30,31,33]. For a modern and self-contained account of Gårding's theory and its relation to the Dirichlet problem one can consult [12] and [14].

    Clearly the closed Gårding cone $ \overline{\Gamma}_k $ is also convex with

    $ ¯Γ+=¯ΓN¯ΓN1¯Γ1
    $
    (2.15)

    and by continuity the monotonicity properties extend to say

    $ ¯ΓN+¯Γk¯Γk  and  σk(λ+μ)σk(λ)  for each λ¯Γk,μ¯ΓN.
    $
    (2.16)

    For $ A \in \mathcal{S}(N) $ denote by $ \lambda(A): = (\lambda_1(A), \ldots, \lambda_N(A)) $ the vector of eigenvalues (2.1) and define the $ k $-convexity constraint set by

    $ Σk:={AS(N): λ(A)¯Γk}.
    $
    (2.17)

    For $ u \in C^2(\Omega) $, one says that $ u $ is $ k $-convex on $ \Omega $ if

    $ D2u(x)Σk  for each xΩ
    $
    (2.18)

    and we will say that $ u \in C^2(\Omega) $ is strictly $ k $-convex on $ \Omega $ if $ D^2u(x) $ lies in the interior $ \Sigma_k^{\circ} $ of $ \Sigma_k $ for each $ x \in \Omega $. Notice that

    $ ΣNΣN1Σ1
    $
    (2.19)

    where

    $ Σ1=H:={AS(N): tr(A)0}  and  ΣN=P:={AS(N): λ1(A)0};
    $
    (2.20)

    that is, $ 1 $-convex functions are classically subharmonic (with respect to the Laplacian) and $ N $-convex functions are ordinary convex functions. This consideration carries over to $ u \in \mathrm{USC}(\Omega) $ where one defines $ k $-convexity by interpreting (2.18) in the viscosity sense.

    Definition 2.1. Given $ u \in \mathrm{USC}(\Omega) $, we say that $ u $ is $ k $-convex at $ x_0 \in \Omega $ if for every $ \varphi $ which is $ C^2 $ near $ x_0 $

    $  uφ has a local maximum in x0    D2φ(x0)Σk.
    $
    (2.21)

    We say that $ u $ is $ k $-convex on $ \Omega $ if this pointwise condition holds for each $ x_0 \in \Omega $.

    Remark 2.2. In the viscosity language of superjets, the condition (2.21) means

    $ (p,A)J2,+u(x0)    AΣk,
    $
    (2.22)

    and there are obviously many equivalent formulations. For example, one can restrict to upper test functions $ \varphi $ which are quadratic and satisfy $ \varphi(x_0) = u(x_0) $. See Appendix A of [7] for a discussion of this point in the context of viscosity subsolutions with admissibility constraints. Moreover, since $ \Sigma_k $ is closed, one also has

    $ (p,A)¯J2,+u(x0)    AΣk;
    $
    (2.23)

    where, as usual, $ (p, A) \in \overline{J}^{2, +}u(x_0) $ means that there exists $ \{x_k, p_k, A_k\}_{k \in {\mathbb N}} $ such that $ (p_k, A_k) \in J^{2, +}u(x_k) $ and $ (x_k, p_k, A_k) \to (x_0, p, A) $ as $ k \to +\infty $.

    The $ k $-convex constraint $ \Sigma_k $ will be used as an admissibility constraint for the solutions of $ k $-Hessian equations considered here. One defines the $ k $-Hessian operator by

    $ Sk(A):=σk(λ(A))for AS(N) and k{1,,N},
    $
    (2.24)

    where $ \lambda(A) $ is the vector of eigenvalues of $ A $ and $ \sigma_k $ is given by (2.2). Notice that

    $ Sj(A)0 for each AΣk and each j=1,k.
    $
    (2.25)

    In particular $ S_k $ is non-negative on $ \Sigma_k $. Important special cases are

    $ S1(A):=tr(A)andSN(A):=det(A).
    $
    (2.26)

    The following Lemma gives the fundamental structural properties of $ \Sigma_k $ and $ S_k $.

    Lemma 2.3. For each fixed $ k \in \{1, \ldots, N\} $, one has the following properties.

    $ (a) \; \Sigma_k $ is a closed convex cone with vertex at the origin.

    $ (b) \; \Sigma_k $ is an elliptic set; that is, $ \Sigma_k \subsetneq \mathcal{S}(N) $, is closed, non empty and satisfies the positivity property

    $ AΣk    A+PΣk  foreach PP,
    $
    (2.27)

    where $ \mathcal{P} $ are the non negative matrices as defined in (2.20).

    $ (c) \; \Sigma_k $ satisfies the topological property

    $ Σk=¯Σk,
    $
    (2.28)

    where $ \Sigma_k^{\circ}: = \{A \in \mathcal{S}(N): \lambda(A) \in \Gamma_k \} $ is the interior of $ \Sigma_k $.

    $ (d) $ The $ k $-Hessian is $\underline{increasing \; along\; \Sigma_k }$; that is,

    $ Sk(A+P)Sk(A)  foreach AΣk and PP.
    $
    (2.29)

    Moreover, the inequality in (2.29) is strict if $ P \in \mathcal{P}^{\circ} $; that is, if $ P > 0 \ \text{in} \ \mathcal{S}(N) $.

    Proof. Part (a) follows from the corresponding properties for $ \overline{\Gamma}_k $. For the claims in part (b), $ \Sigma_k $ is closed by part (a). Each $ \Sigma_k $ is non empty since $ \Sigma_k \supset \Sigma_N = \mathcal{P} $ as noted in (2.19) and (2.20). Clearly $ \Sigma_1 \subsetneq \mathcal{S}(N) $ and hence the same is true for the other values of $ k $ by (2.19). The property (2.28) also clearly holds since $ \Sigma_k $ is a closed convex cone with non-empty interior.

    For the property (2.27), if $ A \in \Sigma_k $ and $ P \geq 0 $ then $ \lambda_i(A+P) \geq \lambda_i(A) $ for each $ i = 1, \ldots, N $ and hence using (2.16) with $ \lambda : = \lambda(A) \in \overline{\Gamma}_k $ and $ \mu : = \lambda(A + P) - \lambda(A) \in \overline{\Gamma}_N $ gives for each $ j = 1, \ldots, k $

    $ σj(λ(A+P))=σj(λ(A)+λ(A+P)λ(A))σj(λ(A))0,
    $
    (2.30)

    which gives the positivity property (2.27).

    The monotonicity formula (2.29) follows from (2.30) with $ j = k $ and the definition of the $ k $-Hessian operator $ S_k(A): = \sigma_k(\lambda(A)) $. When $ P \in \mathcal{P}^{\circ} $, $ \lambda_i(A+P) > \lambda_i(A) $ for each $ i = 1, \ldots, N $ and the inequality in (2.29) becomes strict.

    As noted in the introduction, the notion of elliptic sets was introduced by Krylov [23] and starting with the groundbreaking paper Harvey-Lawson [11], has given birth to a nonlinear potential theory approach to viscosity solutions with admissibility constraints. In the terminology of [7], $ \Sigma_k $ is a (constant coefficient) pure second order subequation constraint set which requires that $ \Sigma_k \subset \mathcal{S}(N) $ be a proper closed subset satisfying the positivity property (2.27) and the topological property (2.28). Moreover, being also a convex cone, $ \Sigma_k $ is a monotonicity cone subequation and $ \Sigma_k $ is the maximal monotonicity cone for both $ \Sigma_k $ and for its dual monotonicity constraint set $ \widetilde{\Sigma}_{k} $ as defined below in (2.36) (see Proposition 4.5 of [7]). One has reflexivity ($ {\mathop \Sigma \limits^ \approx _k} = {\Sigma _k} $) if topological property (2.28) holds (see Proposition 3.2 of [7], for example). The following fact, mentioned in the introduction, is worth repeating here.

    Remark 2.4. In the nonlinear potential theory language of [11], one says that $ u \in \mathrm{USC}(\Omega) $ is $ \Sigma_k $-subharmonic at $ x_0 $ if $ u $ is $ k $-convex at $ x_0 \in \Omega $ in the sense of Definition 2.1. In addition, one has the coherence property: if $ u \in \mathrm{USC}(\Omega) $ is twice differentiable in $ x_0 $ then

    $ u is Σk-subharmonic at x0    D2u(x0)Σk.
    $
    (2.31)

    We now turn to the definition of $ \Sigma_k $-admissible viscosity subsolutions and supersolutions for the type of equations involving $ k $-Hessian operators $ S_k $ that we will treat. The definitions make sense for any constant coefficient pure second order subequation. The main point is to indicate the role of the $ k $-convexity constraint $ \Sigma_k $ which insures the positivity property for $ S_k $, which corresponds to the degenerate ellipticity of $ S_k $ when the Hessian is constrained to $ \Sigma_k $.

    Definition 2.5. Let $ \Omega \subset {\mathbb R}^N $ be an open set and let $ f: \Omega \times {\mathbb R} \times {\mathbb R}^N \to {\mathbb R} $ be continuous. Consider the equation

    $ Sk(D2u)f(x,u,Du)=0.
    $
    (2.32)

    (a) A function $ u \in \mathrm{USC}(\Omega) $ is said to be a $ \Sigma_k $-admissible subsolution of (2.32) at $ x_0 \in \Omega $ if for every $ \varphi $ which is $ C^2 $ near $ x_0 $

    $ uφ has a local maximum in x0    Sk(D2φ(x0))f(x0,u(x0),Dφ(x0))0and D2φ(x0)Σk.
    $
    (2.33)

    (b) A function $ u \in \mathrm{LSC}(\Omega) $ is said to be a $ \Sigma_k $-admissible supersolution of (2.32) at $ x_0 \in \Omega $ if for every $ \varphi $ which is $ C^2 $ near $ x_0 $

    $ uφ has a local minimum in x0    Sk(D2φ(x0))f(x0,u(x0),Dφ(x0))0or D2φ(x0)Σk.
    $
    (2.34)

    (c) A function $ u \in C(\Omega) $ is said to be a $ \Sigma_k $-admissible solution of (2.32) at $ x_0 $ if both (2.33) and (2.34) hold.

    One says that $ u $ is a $ \Sigma_k $ admissible (sub-, super-) solution on $ \Omega $ if the corresponding statement holds for each $ x_0 \in \Omega $.

    A fundamental example involves $ f \equiv 0 $.

    Example 2.6. [$ k $-convex and co-$ k $-convex functions] By (2.33), a function $ u \in \mathrm{USC}(\Omega) $ is a $ \Sigma_k $-admissible subsolution of

    $ Sk(D2u)=0  in Ω
    $
    (2.35)

    precisely when $ u $ is $ k $-convex in $ \Omega $ (which is equivalent to $ u $ being $ \Sigma_k $-subharmonic in $ \Omega $). On the other hand, $ \Sigma_k $-admissible supersolutions of (2.35) can be stated in terms of the Dirichet dual of Harvey-Lawson [11]

    $ ˜Σk:=(Σk)c=(Σk)c,
    $
    (2.36)

    where $ \widetilde{\Sigma}_k $ is also a constant coefficient pure second order subequation. Using (2.34) and (2.36), one can show that $ u \in \mathrm{LSC}(\Omega) $ is a $ \Sigma_k $-admissible supersolution of (2.35) if and only if

    $  uUSC(Ω) is ˜Σk-subharmonic in Ω.
    $
    (2.37)

    One says that $ u $ is $ \Sigma_k $-superharmonic in $ \Omega $ and that $ v: = -u $ is a co-$ k $-convex function in $ \Omega $. This claim follows from the Correspondence Principle in Theorem 10.14 of [7] which in our pure second order situation requires three hypotheses. The first hypothesis is that $ (S_k, \Sigma_k) $ is a compatible operator-subequation pair since $ S_k \in C(\Sigma_k) $ with

    $ infΣkSk=0  and  Σk={AΣk:Sk(A)=0},
    $
    (2.38)

    which follow from the definitions of $ S_k $ and $ \Sigma_k $. The second hypothesis is that the pair is $ \mathcal{M} $-monotone for some convex cone subequation $ \mathcal{M} $, which is true for $ \mathcal{M} = \mathcal{P} $ in this case. Third hypothesis is that $ S_k $ is tolpologically tame which means that $ \{A \in \Sigma_k: S_k(A) = 0\} $ has non-empty interior, which follows from the strict monotonicity of $ S_k $ in the interior of $ \Sigma_k $.

    A few additional remarks about Definition 2.5 are in order. First we note that, of course, there are various equivalent formulations in terms of different spaces of (upper, lower) test functions $ \varphi $ for $ u $ in $ x_0 $ in the spirit of Remark 2.2.

    Remark 2.7. Concerning the $ \Sigma_k $-admissibility, notice that:

    (a) the part $ D^2 \varphi(x_0) \in \Sigma_k $ of the subsolution condition (2.33) is precisely (2.21) so that $ u $ is automatically $ k $-convex in $ x_0 $;

    (b) the supersolution condition (2.34) can be rephrased as

    $ uφ has a local minimum in x0    Sk(D2φ(x0))f(x0,u(x0),Dφ(x0))0if D2φ(x0)Σk;
    $
    (2.39)

    that is, it is enough to use lower test functions which are $ k $-convex in $ x_0 $.

    The admissible supersolution definition takes its inspiration from Krylov [23] and was developed in [6] for equations of the form $ F(x, D^2u) = 0 $. In the convex Monge-Ampère case $ k = N $ of (2.32), an analogous definition was given by Ishii-Lions [17]. One good way to understand the supersolution definition (2.34) (or (2.39)) was pointed out in the convex case in [17] and concerns the following coherence property.

    Remark 2.8. Suppose that $ u \in C^2(\Omega) $ is a classical supersolution in $ \Omega $; that is,

    $ Sk(D2u(x))f(x,u(x),Du(x))0,  xΩ.
    $
    (2.40)

    If $ \varphi \in C^2(\Omega) $ is a lower test function for $ u $ in $ x_0 $ ($ u - \varphi $ has local minimum in $ x_0 $), while one has $ D^2 u(x_0) \geq D^2 \varphi(x_0) $ from elementary calculus, one cannot use this to deduce

    $ S_k(D^2\varphi(x_0)) - f(x,u(x_0),Du(x_0)) \leq 0 $

    $\underline{\rm{unless}} \; D^2 \varphi(x_0) \in \Sigma_k $.

    As a final remark, we note that our main focus will be for the equation

    $ Sk(D2u)+λu|u|k1=0.
    $
    (2.41)

    where $ k \in \{1, \ldots, N\} $ and $ \lambda \in {\mathbb R} $ is a spectral parameter, which will be positive in the interesting cases and associated to (2.41) we will often have a homogeneous Dirichlet condition on $ \partial \Omega $. We will have cause to consider negative and $ k $-convex subsolutions to (2.41) as well as non negative supersolutions. Obviously, this means using Definition 2.5 with $ f(x, u, Du) = -\lambda u|u|^{k-1} $ where the positivity of $ \lambda $ and negativity of $ u $ is compatible with the $ \Sigma_k $ convexity of (sub)solutions $ u $.

    In order to construct suitable barriers for $ k $-Hessian operators, we will exploit a suitable notion of strict boundary convexity which is stated in terms of the positivity of the relevant elementary symmetric function of the principal curvatures. More precisely, given $ \Omega \subset {\mathbb R}^N $ a bounded domain with $ \partial \Omega \in C^2 $, we denote by

    $ (κ1(y),,κN1(y))  with yΩ
    $
    (2.42)

    the principal curvatures (relative to the inner unit normal $ \nu(y) $) which are defined as the eigenvalues of the self-adjoint shape operator $ S $ on the tangent space $ T(y) $ defined by

    $ S(X):=DXν,  XT(y).
    $
    (2.43)

    If the boundary is represented locally near a fixed point $ y_0 \in \partial \Omega $ as the graph of a suitable function $ \phi $, the principle curvatures $ \kappa_i(y_0) $ are the eigenvalues of the Hessian of $ \phi $ at the relevant point. This will be recalled in the next subsection (as will special coordinate systems well adapted for calculations near the boundary).

    The needed concept of convexity is the following notion.*

    *This is known uniform $ (k-1) $-convexity as in the works of Trudinger beginning with [27] (see also [28]).

    Definition 2.9. Let $ k \in \{2, \ldots, N\} $. $ \Omega \subset {\mathbb R}^N $ with $ \partial \Omega \in C^2 $ is said to be strictly $ (k-1) $-convex if

    Here and below, we will use the same symbol $ \sigma_j $ for the jth-elementary symmetric function on $ {\mathbb R}^{N-1} $ and $ {\mathbb R}^{N} $.

    $ σj(κ1(y),,κN1(y))>0  for each yΩ  and each j=1,k1;
    $
    (2.44)

    that is, for each $ j = 1, \ldots, k - 1 $, each jth-mean curvature is everywhere strictly positive on $ \partial \Omega $.

    Notice that strict $ (N-1) $-convexity is ordinary strict convexity of $ \partial \Omega $. One importance of this convexity is that it ensures the existence of functions which are $ C^2 $, vanish on the boundary and strictly $ k $-convex near the boundary. This fact will be used in Proposition 4.2 below and depends in part on the following fact.

    Lemma 2.10. If $ \Omega \subset {\mathbb R}^N $ is a bounded strictly $ (k-1) $-convex domain with $ \partial \Omega \in C^2 $, then there exists $ R > 0 $ such that

    $ σj(κ1(y),,κN1(y),R)>0  foreach yΩ  andeach j=1,k;
    $
    (2.45)

    that is,

    $ (κ1(y),,κN1(y),R)Γk  foreach yΩ.
    $
    (2.46)

    Proof. With the conventions that $ \sigma_0(\cdot) = 1 $ and $ \sigma_j(\lambda) = 0 $ if $ \lambda \in {\mathbb R}^n $ with $ j > n $, one has the elementary identity

    $ σj(κ1,,κN1,R)=Rσj1(κ1,,κN1)+σj(κ1,,κN1),  j=1,,k.
    $
    (2.47)

    If $ 1 \leq j < k \leq N $, for each $ R > 0 $ both terms on the right hand side of (2.47) are positive on $ \partial \Omega $ by the convexity assumption (2.44). If $ 1 \leq j = k < N $, the first term on the right hand side of (2.47) is positive by (2.44) and both terms are continuous functions on $ \partial \Omega $ which is compact, which gives the claim (2.45) if $ R $ is large enough. In the remaining case $ j = k = N $, the second term in the right hand side of (2.47) vanishes, while the first term is positive for every $ R > 0 $ by (2.44).

    We note that if $ \partial \Omega $ is connected then the conclusion (2.45) holds under the weaker convexity assumption

    $ σk(κ1,,κN1)>0  on Ω.
    $
    (2.48)

    See Remark 1.2 of [5] for a proof of this fact, which also makes use of (2.47).

    As a final consideration, we make a comparison with the natural notion of strict $ \overrightarrow{{\Sigma}}_k $-convexity, as defined in section 5 of Harvey-Lawson [11]. This notion is defined in terms of an elliptic cone $ \overrightarrow{{\Sigma}} $ which is an elliptic subset of $ \mathcal{S}(N) $ (as defined in Lemma (2.3) (a)) which is also a pointed cone in the sense that

    $ A \in \overrightarrow{{\Sigma}} \ \ \Leftrightarrow \ \ t A \in \overrightarrow{{\Sigma}} \ \ \text{for each} \ t \geq 0. $

    Given an elliptic set $ \Sigma $ there is an associated elliptic cone $ \overrightarrow{{\Sigma}} $ which can be defined as the closure of the set

    $ \{ A \in \mathcal{S}(N): \ \exists t_0 \gt 0 \ \ \text{with} \ tA \in \Sigma \ \text{for each} \ t \geq t_0 \} $

    It is easy to see that if $ \Sigma $ is an elliptic cone, then $ \overrightarrow{{\Sigma}} = \Sigma $.

    One says that $ \partial \Omega $ is strictly $ \overrightarrow{{\Sigma}} $-convex at $ x \in \partial \Omega $ if there exists a local defining function $ \rho $ for the boundary near $ x $ such that

    More precisely, $ \rho \in C^2(B_r(x)) $ for some $ r > 0 $ and $ \Omega \cap B_r(x) = \{ y \in B_r(x): \ \rho(y) < 0 \} $ and $ D \rho \neq 0 $ on $ B_r(x) $.

    $ D2ρ(x)|TxΩ=B|TxΩ  for some BΣ,
    $
    (2.49)

    which is to say that $ \rho $ is strictly $ \overrightarrow{{\Sigma}} $ convex near $ x \in \partial \Omega $. In [11], it is shown that solvability of the Dirichlet problem on $ \Omega $ for $ \Sigma $-harmonic functions holds if $ \partial \Omega $ is strictly $ \overrightarrow{{\Sigma}} $ and $ \overrightarrow{{\widetilde{\Sigma}}} $ convex where $ \widetilde{\Sigma} = - \left(\Sigma^{\circ} \right)^c $ is the Dirichlet dual of $ \Sigma $ (as defined in (2.36)).

    Proposition 2.11. For $ \Omega \subset {\mathbb R}^N $ bounded with $ \partial \Omega \in C^2 $, one has

    $ Ω isstrictly (k1)convex  Ω isstrictly Σk and ˜Σ convex.
    $
    (2.50)

    Proof. Since $ \Sigma_k $ and $ \widetilde{\Sigma}_{k} $ are elliptic sets and pointed cones, they are themselves elliptic cones and hence

    $ Σk=Σkand˜Σk=˜Σk.
    $
    (2.51)

    From (2.19) and (2.20) one has for each $ k \in \{1, \ldots, N \} $

    $ P=ΣNΣkΣ1=H
    $
    (2.52)

    and by the definition of the dual one also has

    $ H=˜H˜Σ1˜Σk˜ΣN=˜P
    $
    (2.53)

    and hence

    $ Σk˜Σk  for each k{1,,N}.
    $
    (2.54)

    From (2.51) and (2.54) one has that $ \overrightarrow{{\Sigma}}_k \subset \overrightarrow{{\widetilde{\Sigma}}}_k $ and hence strict $ (k-1) $-convexity is precisely what the general Harvey-Lawson theory requires since $ \overrightarrow{{\Sigma}}_k^{\circ} = \Sigma_k^{\circ} $.

    Consider $ \Omega \subset {\mathbb R}^N $ a bounded domain with $ C^2 $ boundary with principal curvatures $ \{ \kappa_i(y)\}_{i = 1}^{N-1} $, unit inner normal $ \nu(y) $ and tangent space $ T(y) $ at each $ y \in \partial \Omega $. Denote the distance function to the boundary by

    $ d(x):=dist(x,Ω),  xRN.
    $
    (2.55)

    Following section 14.6 of [10], will recall some known facts concerning the calculation of $ \kappa_i(y_0) $ at a fixed boundary point $ y_0 $ and the notion of a principal coordinate system near $ y_0 $ which yields nice formula for the Hessian of $ d $ in suitable tubular neighborhoods of the boundary.

    With $ y_0 \in \partial \Omega $ fixed, choose coordinates $ x = (x', x_N) \in {\mathbb R}^{N-1} \times {\mathbb R} = {\mathbb R}^N $ such that the inner unit normal is $ \nu(y_0) = (0, 1) $. Then there exists an open neighborhood $ \mathcal{N}_0 $ of $ y_0 $ and a function

    $ ϕ:N0T(y0)R of class C2 with Dϕ(y0)=0
    $
    (2.56)

    so that

    $ ΩN(y0)={(x,ϕ(x)):  xN0T(y0)}
    $
    (2.57)

    and

    $ the principal curvatures {κi(y0)}N1i=1 are the eigenvalues of D2ϕ(y0).
    $
    (2.58)

    In a principal coordinate system at $ y_0 $, where one takes the axes $ x_1, \ldots, x_{N-1} $ along the associated eigenvectors for $ D^2 \phi(y_0^{\prime}) $, one has

    $ D2ϕ(y0)=diag[κ1(y0),,κN1(y0)].
    $
    (2.59)

    The following properties of bounded $ C^2 $ domains are well known and will be used repeatedly in the sequel. For the proofs, see Lemma 14.16 and Lemma 14.17 of [10].

    Lemma 2.12. Let $ \Omega \subset {\mathbb R}^N $ be a bounded domain with $ C^2 $ boundary. Then there exists $ \delta > 0 $ such that:

    (a) $ \partial \Omega $ satisfies a uniform interior (and uniform exterior) sphere condition with balls of radius bounded below by $ \delta $ so that the principal curvatures satisfy for each $ i \in \{1, \ldots, N-1 \} $

    $ |κi(y)|1δ  foreach yΩ;
    $
    (2.60)

    (b) the distance function $ d(\cdot): = {\rm dist}(\cdot, \partial \Omega) $ satisfies

    $ dC2(¯Ωδ)
    $
    (2.61)

    and

    $  |Dd(x)|=1foreachxΩδ
    $
    (2.62)

    where

    $ Ωδ:={xΩ, 0<d(x)<δ};
    $
    (2.63)

    (c) for each $ x \in \Omega_{\delta} $

    $ thereexistsauniquey=y(x)Ωsuchthatd(x)=|xy|;
    $
    (2.64)

    (d) from (2.62) one has that $ D^2d(x_0) $ has a zero eigenvalue associated to the eigenvector $ D d(x_0) $ for each $ x_0 \in \Omega_{\delta} $ and using a principal coordinate system based at the point $ y_0 = y(x_0) $, which realizes the distance from $ x_0 $ to the boundary, one has $ D d(x_0) = (0, \ldots, 0, 1) $ and

    $ D2d(x0)=diag[κ11κ1d,,κN11κN1d,0],
    $
    (2.65)

    where $ \kappa_i = \kappa_i(y_0) $, $ d = d(x_0) $ and $ 1 - \kappa_i d > 0 $ since $ d < \delta $ and $ \kappa_i $ satisfies (2.60).

    Managing $ S_k $ is facilitated by using the principal coordinate systems near the boundary discussed above. Also radial functions are often handy for comparison arguments used in Hopf-type boundary estimates and Hölder regularity arguments, as we will see. In this subsection, we record two lemmas for future use.

    Lemma 2.13. Let $ \Omega \subset {\mathbb R}^N $ be a bounded domain with $ C^2 $ boundary. For any $ g \in C^2((0, \delta)) $ and any $ x_0 \in \Omega_{\delta} $ one has the following formula for the composition $ v = g \circ d $ and for each $ j = 1, \ldots, N $

    $ Sj(D2v(x0))=σj(κ11κ1dg(d),,κN11κN1dg(d),g(d)),
    $
    (2.66)

    where again $ \kappa_i = \kappa_i(y_0) $ and $ d = d(x_0) $ in a principal coordinate system based at $ y_0 \in \partial \Omega $ which realizes the distance to $ x_0 \in \Omega_{\delta} $ as in Lemma 2.12.

    Proof. For $ g \in C^2 $ the Hessian of the composition $ v = g \circ d $ in $ \Omega_{\delta} $ is given by

    $ D2v=g(d)D2d+g(d)DdDd
    $
    (2.67)

    which has eigenvalues $ \lambda_N(D^2v) = g^{\prime\prime}(d) $ and $ \lambda_i(D^2v) = g^\prime(d)e_i(d) $ where $ \{e_i(d)\}_{i = 1}^{N-1} $ are the first $ N-1 $ eigenvalues of $ D^2 d $ whose expression at $ x_0 \in \Omega_{\delta} $ in a principal coordinate system based at $ y_0 = y(x_0) $ is given by (2.65) and hence

    $ D2v(x0)=diag[κ11κ1dg(d),,κN11κN1dg(d),g(d)],
    $
    (2.68)

    from which (2.66) follows by the definition of $ S_j $.

    Lemma 2.14. For radial functions $ w(x) = h(|x - x_0|) $ with $ h\in C^2 $, the eigenvalues of $ D^2w $ in any punctured neighborhood of $ x_0 $ are §

    §Note that $ h^{\prime \prime}(r) = h^{\prime}(r)/r $ is possible; for example, if $ h(r) = r^2 $. In that case, there is only one distinct eigenvalue with multiplicity $ N $.

    $ h(r)withmultiplicityoneandh(r)/rwithmultiplicityN1,
    $
    (2.69)

    where $ r: = |x - x_0| $ and hence

    Here and below, $ { \left(nk

    \right) : = \frac{n!}{k! (n - k)!}} $ for integers satisfying $ n \geq k \geq 0 $.

    $ Sk(D2w(x))=h(r)(h(r)r)k1(N1k1)+(h(r)r)k(N1k);
    $
    (2.70)

    that is,

    $ Sk(D2w(x))=(h(r)r)k1(N1k1)[h(r)+h(r)rNkk].
    $
    (2.71)

    Proof. The claim in (2.69) is well known, from which (2.70) and (2.71) follow easily.

    As suggested in the title, we will make use of various comparison and maximum principles for $ \Sigma_k $-admissible viscosity subsolutions and supersolution in the sense of Definition 2.5 and the subsequent remarks and examples. While they will be special cases of the results in [6,7,11], for the convenience of the reader we will give the precise statements and some indication of the proofs. In all that follows $ \Omega $ will be an open bounded domain in $ {\mathbb R}^N $.

    We begin the most basic comparison result, which concerns a $ \Sigma_k $-subharmonic and $ \Sigma_k $-superharmonic pair, as presented in Example 2.6.

    Theorem 3.1. Suppose that $ u \in \mathrm{USC}(\overline{\Omega}) $ and $ v \in \mathrm{LSC}(\overline{\Omega}) $ are a $ \Sigma_k $-admissible viscosity subsolution/supersolution pair for the homogeneous equation $ S_k(D^2 u) = 0 $ in $ \Omega $. Then the comparison principle holds; that is,

    $ uv  on Ω    uv  on Ω.
    $
    (3.1)

    Proof. The hypothesis is equivalent to saying that $ u $ and $ v $ are $ \Sigma_k $-subharmonic and $ \Sigma_k $-superharmonic in $ \Omega $, as discussed in Example 2.6. Since $ \Sigma_k $ is a pure second order subequation, one has the comparison principle (3.1) as a corollary of the comparison principle of [11] (see also Theorem 9.3 of [7]). The main ingredients in the proof are that $ -v $ is $ \widetilde{\Sigma}_k $-subharmonic and that $ w: = u - v $ is $ \widetilde{\mathcal{P}} $-subharmonic (coming from the $ \mathcal{P} $-monotonicity of $ \Sigma_k $ and its dual), for which the zero maximum principle holds

    $ w0  on Ω    w0  on Ω.
    $
    (3.2)

    See section 7 of [7] for details in the general case of $ \widetilde{\mathcal{M}} $-monotone subequations.

    As noted in (2.20), the admissibility constraint sets satisfy

    $ \Sigma_k \subset \Sigma_1 = \mathcal{H} \ \ \text{for each} \ k = 1, \ldots, N $

    and hence each $ u $ which is $ \Sigma_k $-subharmonic on $ \Omega $ will be $ \mathcal{H} $-subharmonic on $ \Omega $ and hence $ u $ satisfies the mean value inequality

    $ u(x0)1|Br(x0)|Br(x0)u(x)dx  for each Br(x0)Ω.
    $
    (3.3)

    An immediate consequence of (3.3) is the strong maximum principle.

    Theorem 3.2. For each $ u \in \mathrm{USC}(\Omega) $ which is $ \Sigma_k $-subharmonic ($ k $-convex) on a bounded domain (open, connected set) one has

    $ ifthereexistsx0Ωwithu(x0)=supΩu,thenuisconstantinΩ.
    $
    (3.4)

    In particular, if $ u \in \mathrm{USC}(\overline{\Omega}) $ is $ \Sigma_k $-subharmonic ($ k $-convex) in $ \Omega $ then

    $ u0  on Ω    u<0  in Ω  or  u0  in  Ω.
    $
    (3.5)

    Remark 3.3. Notice that (3.5) is the strong form of the zero maximum principle

    $ u0  on Ω    u0  on Ω.
    $
    (3.6)

    The weak form (3.6) of the zero maximum principle is also a simple corollary the comparison principle in Theorem 3.1. Indeed, one compares the $ \Sigma_k $-subarmonic $ u $ with the smooth function $ v \equiv 0 $. Since $ \widetilde{\Sigma_k} $ also satisfies the positivity property (2.27), the coherence property of Remark 2.4 holds and hence $ v \equiv 0 $ is $ \Sigma_k $-superharmonic since $ 0 = S_k(-v) \in \widetilde{\Sigma_k} $.

    We conclude this section with a comparison result which is tailored for some of the pointwise estimates we will need.

    Theorem 3.4. Let $ c \geq 0 $ be fixed. Suppose that $ u \in \mathrm{LSC}(\overline{\Omega}) $ satisfies

    By this we mean that $ u $ is a $ \Sigma_k $-admissible viscosity supersolution of the equation $ S_k(D^2u) - c = 0 $.

    $ Sk(D2u)c  in Ω.
    $
    (3.7)

    Suppose that $ v \in C^2(\Omega) \cap C(\overline{\Omega}) $ is a strictly $ k $-convex strict subsolution, that is,

    $ D2v(x)Σk  and  Sk(D2v(x))>c  forall xΩ.
    $
    (3.8)

    Then, one has the comparison principle

    $ vu  on Ω    vu  on Ω.
    $
    (3.9)

    Proof. Suppose not, then $ v - u \in \mathrm{USC}(\overline{\Omega}) $ will have a (positive) maximum at some interior point $ x_0 \in \Omega $. Hence $ u - v $ will have a (negative) minimum at $ x_0 $. Choose $ \varphi = v $ in Definition 2.5 (b) of a $ \Sigma_k $-admissible supersolution $ u $ to find

    $ S_k(D^2v(x_0)) \leq c \ \ \text{or} \ \ D^2 v(x) \not\in \Sigma_k^{\circ}, $

    which contradicts (3.8).

    Some variants of these principles will also be present in some of the proofs.

    For the minimum principle characterization of Theorem 5.4 and for the global Hölder regularity result of Theorem 6.3, we will make use of various barrier functions which provide some needed one-sided bounds near the boundary $ \partial \Omega $ of bounded $ C^2 $ domains. The arguments are standard, but the details involve having a sufficiently robust calculus for the $ k $-Hessian.

    The first estimate is a form of the Hopf lemma which will be applied to the subsolutions $ \psi $ competing in the Definition of the principal eigenvalue when we prove the minimum principle characterization of Theorem 5.4.

    Proposition 4.1. Given $ \lambda \geq 0 $. Suppose that $ \psi \in \mathrm{USC}(\overline{\Omega}) $ is a $ k $-convex subsolution i.e., a $ \Sigma_k $-admissible subsolution in the sense of Definition 2.5 of

    $ {Sk(D2ψ)+λψ|ψ|k1=0in Ωψ=0on Ω
    $
    (4.1)

    which is negative on $ \Omega $. Then

    $ there exists C1>0 such that ψ(x)C1d(x) for all xΩδ/2,
    $
    (4.2)

    where $ \Omega_{\delta/2} $ is the tubular neighborhood defined as in (2.63) with $ \delta > 0 $ such that the conclusions of Lemma 2.12 hold in the larger neighborhood $ \Omega_{\delta} $.

    Proof. One uses the usual argument of comparing $ \psi $ with a smooth radial function $ w $ which is a strict supersolution of (4.1) and dominates $ \psi $ on the boundary of an annular region within the good tubular neighborhood $ \Omega_{\delta} $ (see Proposition 2.5 of [4], for example). For completeness, we give the argument.

    For each $ x_0 \in \Omega_{\delta/2} $, denote by $ y_0 = y_0(x_0) \in \partial \Omega $ which realizes the distance to the boundary and by $ z_0 = z_0(x_0) = y_0 + \delta(x_0 - y_0)/|x_0 - y_0| $ the center of an interior ball such that

    $ Bδ(z0)Ωand¯Bδ(z0)(RNΩ)={y0}.
    $
    (4.3)

    Consider the smooth negative radially symmetric function

    $ w(x)=C0(emδem|xz0|)  for each xA:=Bδ(z0)¯Bδ/2(z0),
    $
    (4.4)

    where $ C_0 $ and $ m $ are chosen to satisfy

    $ C0supΩΩδ/2ψemδemδ/2
    $
    (4.5)

    and

    $ m>2(Nk)kδ.
    $
    (4.6)

    One has $ w(x)\geq \psi(x) $ on $ \partial \mathcal{A} $; which is trivial on the outer boundary where $ w $ vanishes and the choice of $ C_0 $ in (4.5) is used on the inner boundary which is contained in $ \Omega \setminus \Omega_{\delta/2} $. The key point is to show that

    $ w(x)ψ(x) on A.
    $
    (4.7)

    Suppose, by contradiction, that $ \psi-w $ has a positive maximum point at $ \bar{x} $ in the interior of $ \mathcal{A} $. By Definition 2.5(a) of the $ \Sigma_k $-admissible subsolution $ \psi $ of the PDE, one has

    $ S_k(D^2w(\bar{x}))\geq -\lambda\psi(\bar{x})|\psi(\bar{x})|^{k-1}\geq 0 $

    But, using the radial calculation (2.71) with $ h(r) = C_0(e^{- m \delta} - e^{-mr}) $ and $ r = x - z_0 $, with the choice on $ m $ in (4.6) where $ r > \delta/2 $, one has

    $ S_k(D^2w(x)) = \frac{C_0^k m^ke^{-mkr}}{r^k}\left(N1k1
    \right)\left[-mr+ \frac{N-k}{k} \right] \lt 0 $

    which yields a contradiction. Hence, for $ x_0 \in \Omega_{\delta/2} $ one has

    $ \psi(x_0) \leq w(x_0) = C_0 e^{-m \delta} \left(1 - e^{m d(x_0)} \right) \leq C_0 e^{-m \delta} (-m d(x_0)) $

    and one can take $ C_1 = - mC_0e^{-m \delta} $.

    The next estimate gives a lower bound near the boundary for the supersolutions treated in the minimum principle characterization of Theorem 5.4.

    Proposition 4.2. Let $ \Omega $ be a bounded strictly $ (k-1) $-convex domain and $ \lambda \geq 0 $. Suppose that $ u \in \mathrm{LSC}(\overline{\Omega}) $ is a $ \Sigma_k $-admissible supersolution ** of

    **By this we mean that $ u $ is a $ \Sigma_k $-admissible supersolution of $ S_k(D^2 u) + \lambda u |u|^{k-1} = 0 $ in $ \Omega $ in the sense of Definition 2.5(b) and that $ u \geq 0 $ on $ \partial \Omega $.

    $ {Sk(D2u)+λu|u|k1=0in Ωu=0on Ω.
    $
    (4.8)

    Then

    $ there exist C2>0 and d0>0 such that u(x)C2d(x) for all xΩd0,
    $
    (4.9)

    where, as always, $ \Omega_{d_0}: = \{ x \in \Omega: \ 0 < d(x) < d_0 \} $.

    Before giving the proof, a pair of remarks are in order. Since $ u(x) \geq 0 = -C_2d(x) $ for each $ x \in \partial \Omega $, the lower bound in (4.9) holds trivially there. Moreover, having $ u > 0 $ at boundary points facilitates having a negative lower bound and the interesting case concerns $ u \equiv 0 $ on $ \partial \Omega $.

    Proof of Proposition 4.2: Since $ \partial \Omega \in C^2 $, by Lemma 2.12, there exists $ \delta > 0 $ such that $ d \in C^2(\overline{\Omega}_{\delta}) $. Consider the comparison function $ \varphi \in C^2(\overline{\Omega}_{\delta}) $ defined by

    $ φ(x):=etd(x)1:=g(d(x)) with t>0 sufficiently large.
    $
    (4.10)

    Claim: For $ t $ sufficiently large and $ d_0 $ sufficiently small, one has:

    $ D2φ(x0)Σk  foreach x0Ωd0;
    $
    (4.11)
    $ φu  on Ωd0;
    $
    (4.12)
    $ Sk(D2φ)+λφ|φ|k1>0  in Ωd0
    $
    (4.13)

    That is, on a sufficiently small tubular domain $ \Omega_{d_0} $, the function $ \varphi $ is a $ C^2 $ strictly $ k $-convex strict subsolution of the eigenvalue equation which is dominated by the supersolution $ u $ on $ \partial \Omega_{d_0} $.

    Given the claim, the $ \Sigma_k $-admissible supersolution $ u $ must satisfy

    $ uφ on Ωd0.
    $
    (4.14)

    Indeed, if (4.14) were to be false, then $ u - \varphi \in \mathrm{LSC}(\overline{\Omega}_{d_0}) $ would have its (negative) minimum at some $ x_0 \in \Omega_{d_0} $ (using (4.12)). By Definition 2.5(b), one would then have

    $ S_k(D^2 \varphi(x_0)) + \lambda \varphi(x_0) |\varphi(x_0)|^{k-1} \leq 0 \ \ \text{or} \ \ D^2 \varphi(x_0) \not\in \Sigma_k^{\circ}, $

    which contradicts (4.13)–(4.11). The relation (4.14) gives the barrier estimate (4.9) since

    $ u(x) \geq \varphi(x): = e^{-t d(x)} - 1 \geq -C_2 d(x), \ \ x \in \Omega_{d_0} $

    if $ C_2 $ is chosen to satisfy $ C_2 \geq t $.

    Thus it remains only to verify the Claim. We begin with the strict $ k $-convexity of $ \varphi $ claimed in (4.11). Using Lemma 2.13 on $ \varphi = g \circ d $ and calculating the needed derivatives of $ g(d) : = e^{-td} - 1 $, on $ \Omega_{\delta} $ one has for each $ j = 1, \ldots, k $

    $ Sj(D2φ(x0))=tjejtd(x0)σj(κ1(y0)1κ1(y0)d(x0),,κN1(y0)1κN1(y0)d(x0),t),
    $
    (4.15)

    where again we use a principal coordinate system based at $ y_0 = y(x_0) \in \partial \Omega $ which realizes the distance to $ x_0 \in \Omega_{\delta} $. Now, using the strict $ (k-1) $-convexity of $ \partial \Omega $, by Lemma 2.10 there exists $ R > 0 $ and $ \beta_0 > 0 $ so that

    $ σj(κ1(y0),,κN1(y0),R)β0>0  for each y0Ω  and each j=1,k.
    $
    (4.16)

    We have used the continuity of each $ \sigma_j $ and the compactness of $ \partial \Omega $ to pick up the positive lower bound $ \beta_0 $. Since each $ \sigma_j $ (with $ 1 \leq j \leq k $) is increasing in $ \Gamma_k $ with respect to $ \lambda_N $, we can freely replace $ R $ by any $ t \geq R $ in (4.16). Again by continuity and compactness, we can choose $ d_0 \leq \delta $ so that for each $ x_0 \in \Omega_{d_0} $ and for each $ j = 1, \ldots k $, one has

    $ σj(κ1(y0)1κ1(y0)d(x0),,κN1(y0)1κN1(y0)d(x0),R)β02>0.
    $
    (4.17)

    Indeed, with

    $ μ:=maxy0Ωmax1iN1|κi(y0)|
    $
    (4.18)
    $ p:=(κ1(y0)1κ1(y0)d(x0),,κN1(y0)1κN1(y0)d(x0))  and  q:=(κ1(y0),,κN1(y0)),
    $

    by choosing $ d_0 \leq 1/(2 \mu) $, for every $ x_0 \in \overline{\Omega}_{d_0} $ one has

    $ |pq|2N1μd0,
    $

    which can be made as small as needed to ensure that (4.17) follows from (4.16) (by taking $ d_0 $ even smaller if needed).

    By choosing $ t : = R $ in (4.15) and using (4.17), one has

    $ Sj(D2φ(x0))RjejRd0β02>0   for each x0Ωd0 and j=1,k,
    $
    (4.19)

    and hence the strict $ k $-convexity of $ \varphi $ on $ \Omega_{d_0} $.

    Next we verify the claim (4.12) concerning boundary values. The claim is trivial on the outer boundary $ \partial \Omega $ where $ \varphi $ vanishes and $ u \geq 0 $. On the compact inner boundary (where $ d(x) = d_0 $), by reducing $ d_0 $ if need be, we can assume that $ u \geq -1/2 $ (since $ u $ is lower semi-continuous and is non-negative on $ \partial \Omega $). Hence it suffices to choose $ t > 0 $ large enough so that

    $ \varphi = e^{-td_0} - 1 \leq -1/2 \leq u. $

    Recall that we may freely increase $ t \geq R $ without spoiling the $ k $-convexity of $ \varphi $ as noted above.

    Finally, we need to verify the subsolution claim (4.13) which using the negativity of $ \varphi $ is equivalent to

    $ Sk(D2φ(x0))>λ|φ(x0)|k  for each x0Ωd0.
    $
    (4.20)

    Using (4.15) and (4.17) with $ j = k $, for each $ x_0 \in \Omega_{d_0} $, we have

    $ Sk(D2φ(x0))=tkektd(x0)σk(κ1(y0)1κ1(y0)d(x0),,κN1(y0)1κN1(y0)d(x0),t)>tkektd(x0)β02.
    $
    (4.21)

    Now, on $ \Omega_{d_0} $ (where $ d(x_0) < d_0 $), we have

    $ λ|φ(x0)|k=λ(1etd(x0))k<λ(1etd0)k.
    $
    (4.22)

    Combining (4.21) with (4.22), we will have (4.20) provided that

    $ t^k e^{-kt d(x_0)} \frac{\beta_0}{2} \gt \lambda \left( 1 - e^{-t d_0}\right)^k, $

    which holds if $ d_0 $ is chosen small enough.

    The final boundary estimate we will need is similar to the preceding estimate and will be employed in the proof of the uniform Hölder regularity for a sequence of solutions tending to a principal eigenfunction, see Theorems 6.3 and 6.6.

    Proposition 4.3. Let $ \Omega $ be a bounded strictly $ (k-1) $-convex domain and let $ f \geq 0 $ be a bounded continuous function on $ \Omega $. Suppose that $ u \in \mathrm{LSC}(\overline{\Omega}) $ is a $ \Sigma_k $-admissible supersolution of

    $ {Sk(D2u)=fin Ωu=0on Ω
    $
    (4.23)

    Then there exist $ d_0 > 0 $ and $ C_3 > 0 $ such that

    $ u(x)C3d(x) for all xΩd0,
    $
    (4.24)

    where, as always, $ \Omega_{d_0}: = \{ x\in \Omega: \ 0 < d(x) < d_0\} $.

    Proof. Consider the family of comparison functions used in Proposition 4.2; that is,

    $ φ(x)=etd(x)1  with t>0 sufficiently large.
    $
    (4.25)

    We have seen in (4.19) that there exists $ d_0 > 0 $ sufficiently small such that

    $ D2φ(x0)Σk  for each x0Ωd0.
    $
    (4.26)

    In particular, if we choose $ t = 1/d_0 $ in (4.21) (so that $ t $ is large if $ d_0 $ is small) we have

    $ Sk(φ(x0))>dk0ekβ02>supΩf  for each x0Ωd0,
    $
    (4.27)

    provided that $ d_0 $ is chosen small enough. Using (4.26) and (4.27), for $ d_0 $ sufficiently small, we have that $ \varphi(\cdot) = e^{-d(\cdot)/d_0} - 1 \in C^2(\Omega_{d_0}) \cap C(\overline{\Omega}_{d_0}) $ is a strictly $ k $-convex strict subsolution of the equation

    $ Sk(D2u)=c:=supΩf  in Ωd0.
    $
    (4.28)

    By hypothesis, $ u \in \mathrm{LSC}(\overline{\Omega}) $ is also a $ \Sigma_k $-admissible supersolution of (4.28) and hence by the comparison principle of Theorem 3.4 we will have

    $  u(x)φ(x)=ed(x)/d01 for all xΩd0,
    $
    (4.29)

    provided that this inequality holds on the boundary; that is,

    $  u(x)φ(x)=ed(x)/d01 for all xΩd0.
    $
    (4.30)

    For the boundary inequality (4.30), on the outer boundary $ \partial \Omega $ we have $ u \geq 0 = \varphi $ since $ u $ is a supersolution of (4.23) and $ d(x) = 0 $ on $ \partial \Omega $. On the inner boundary $ \partial \Omega_{d_0} \cap \Omega $ (where $ d(x) = d_0 $) we have

    $ φ(x)=e11:=ε<0.
    $
    (4.31)

    Since $ u \in \mathrm{LSC}(\overline{\Omega}) $ with $ u \geq 0 $ on $ \partial \Omega $ there exits $ \delta = \delta(\varepsilon) > 0 $ such

    $ u(x)>ε  for each xΩ such that dist(x,Ω)<δ.
    $
    (4.32)

    Choosing $ d_0 $ even smaller so that $ d_0 \leq \delta $ in (4.32) then shows that (4.30) holds on the inner boundary $ \partial \Omega_{d_0} \cap \Omega $ as well.

    Finally, the comparison estimate (4.29) gives the barrier estimate (4.24) for $ C_3 > 1/d_0 $.

    In all that follows, $ \Omega \subset {\mathbb R}^N $ will be a bounded open domain with $ C^2 $ boundary which is strictly $ (k-1) $-convex in the sense of Definition 2.9. Denote by

    $ Φk(Ω):={ψUSC(Ω):ψ is k-convex and negative in Ω},
    $
    (5.1)

    where the notion of $ k $-convexity is that of Definition 2.1. Notice that since $ \psi $ is bounded from above (by zero) on $ \Omega $ one can extend $ \psi $ to a $ \mathrm{USC}(\overline{\Omega}) $ function in a canonical way by letting

    $ ψ(x0):=lim supxx0xΩu(x),  for each x0Ω.
    $
    (5.2)

    In particular, since $ \psi < 0 $ on $ \Omega $ this extension also satisfies

    $ ψ0  on Ω.
    $
    (5.3)

    We will freely make use of this extension so that Proposition 4.1 (Hopf's Lemma) applies to give the boundary estimate (4.2) for the canonical extension of $ \psi \in \Phi_k^{-}(\Omega) $.

    The following definition gives a candidate for the principal eigenvalue associated to a negative $ k $-convex eigenfunction of the $ k $-Hessian $ S_k(D^2u) = \sigma_k(\lambda(D^2u)) $.

    Definition 5.1. For each $ k \in \{1, \ldots, N\} $ fixed, define

    $ λ1(Sk,Σk):=supΛk
    $
    (5.4)

    where

    $ Λk:={λR: ψΦk(Ω) with Sk(D2ψ)+λψ|ψ|k10 in Ω}.
    $
    (5.5)

    The meaning of the differential inequality in (5.5) is in the viscosity sense; that is, for each $ x_0 \in \Omega $ and for each $ \varphi $ which is $ C^2 $ near $ x_0 $ one has that

    $  ψφ has a local maximum in x0    Sk(D2φ(x0))+λψ(x0)|ψ(x0)|k10
    $
    (5.6)

    Moreover, since $ \psi \in \Phi_k^-(\Omega) $ is $ k $-convex, $ \psi $ is a $ \Sigma_k $-admissible subsolution of the PDE in the sense of Definition 2.5 (a), whose canonical extension to the boundary (5.2) is admissible for Proposition 4.1 (as noted above).

    About the definition, a few elementary remarks are in order which we record in the following lemma.

    Lemma 5.2. Let $ \lambda_1^-(S_k, \Sigma_k) $ and $ \Lambda_k $ be as in Definition 5.1. Then the following facts hold.

    (a) $(- \infty, \lambda_1^-(S_k, \Sigma_k))\subset \Lambda_k $, or equivalently, if $ \lambda < \lambda_1^-(S_k, \Sigma_k) $ then there exists $ \psi \in \mathrm{USC}(\Omega) $ which is $ k $-convex and negative in $ \Omega $ and satisfies

    $ Sk(D2ψ)+λψ|ψ|k10  in Ω.
    $
    (5.7)

    (b) If $ \Omega $ (which is bounded) is contained in $ B_R(0) $ then one has the estimate

    $ λ1(Sk,Σk)2kCN,kR2kwhere  CN,k=(Nk).
    $
    (5.8)

    In particular, $ \lambda_1^-(S_k, \Sigma_k) $ is positive.

    Proof. For the part (a), we first claim that if $ \lambda \in \Lambda_k $ then $ (-\infty, \lambda] \subset \Lambda_k $. By the definition of $ \Lambda_k $, there is $ \psi \in \Phi^{-}_k(\Omega) $ as defined in (5.1) which satisfies (5.7). If $ \lambda^* < \lambda $ then this $ \psi \in \Phi^{-}_k(\Omega) $ satisfies (5.7) with $ \lambda^* $ in place of $ \lambda $. Indeed, for each $ x_0 \in \Omega $ and each $ \varphi $ which is $ C^2 $ near $ x_0 $ one has (5.6) and hence

    $ S_k(D^2 \varphi(x_0)) +\lambda^* \psi(x_0) |\psi(x_0)|^{k-1} + (\lambda - \lambda^*) \psi(x_0) |\psi(x_0)|^{k-1} \geq 0, $

    but the last term is negative and hence the claim.

    Now, if $ \lambda < \lambda_1^-(S_k, \Sigma_k) $ then by the definition of $ \lambda_1^-(S_k, \Sigma_k) $ there must exist $ \lambda^* = \lambda + \varepsilon^* $ between $ \lambda $ and $ \lambda_1^-(S_k, \Sigma_k) $ which belongs to $ \Lambda_k $ and hence $ \lambda + \varepsilon \in \Lambda_k $ for each $ \varepsilon \in [0, \varepsilon^*] $ by the claim proved above, which completes the proof of part (a).

    For part (b), consider the convex (and hence $ k $-convex) function $ \psi(x): = |x|^2 - R^2 $ which is negative on $ \Omega \subset B_R(0) $. One has $ D^2 \psi(x) = 2I $ for each $ x \in \Omega $ and hence

    $ S_k(D^2 \psi(x)) + \lambda \psi(x) |\psi(x)|^{k-1} = 2^k C_{N,k} - \lambda (R^2 - |x|^2)^k \geq 2^k C_{N,k}- \lambda R^{2k} \geq 0, $

    provided $ \lambda R^{2k} \leq 2^k C_{N, k} $. The claim (5.8) follows.

    Remark 5.3. While the lower bound (5.8) shows that $ \lambda_1^{-}(S_k, \Sigma_k) $ is positive, in Theorem 7.1 we will also give an upper bound for $ \lambda_1^{-}(S_k, \Sigma_k) $ on domains which contain some ball $ B_R(0) $ which shows that $ \lambda_1^{-}(S_k, \Sigma_k) < + \infty $.

    We are now ready for the main result of this section, which we state in the nonlinear case i.e., $ k > 1 $.

    Theorem 5.4. Let $ k \in \{2, \ldots, N\} $ and let $ \Omega $ be a strictly $ (k-1) $-convex domain in $ {\mathbb R}^N $. For every $ \lambda < \lambda_1^{-}(S_k, \Sigma_k) $ and for every $ u \in \mathrm{LSC}(\overline{\Omega}) $ which is $ \Sigma_k $-admissible supersolution of

    $ Sk(D2u)+λu|u|k1=0  in Ω,
    $
    (5.9)

    one has the following minimum principle

    $ u0  on Ω    u0  in Ω.
    $
    (5.10)

    Before giving the proof, a pair of remarks are in order.

    Remark 5.5. If $ \lambda \leq 0 $, then the gradient-free equation (5.9) is proper elliptic on the constraint set $ {\mathbb R} \times \Sigma_k $ and the maximum/minimum principle for $ ({\mathbb R} \times \Sigma_k) $-admissible viscosity subsolutions/supersolutions of (5.9) follows from [7] (see section 11.1). Hence, we will restrict attention to the interesting case

    $ 0<λ<λ1(Sk,Σk).
    $
    (5.11)

    Proof of Theorem 5.4. We argue by contradiction. Assume that

    $ there exists xΩ such that u(x)<0
    $
    (5.12)

    and so $ u \in \mathrm{LSC}(\overline{\Omega}) $ will have a negative minimum on $ \overline{\Omega} $ in some interior point $ \bar{x} \in \Omega $. Let $ \psi \leq 0 $ on $ \partial \Omega $ be a $ \Sigma_k $-admissible subsolution of

    $ Sk(D2ψ)+˜λψ|ψ|k10  in Ω  for a fixed ˜λ(λ,λ1(Sk,Σk)).
    $
    (5.13)

    We will compare $ u $ with $ \gamma \psi $ where

    $ γ(0,γ:=supΩuψ)
    $
    (5.14)

    is to be suitably chosen and $ \psi \in \mathrm{USC}(\overline{\Omega}) $ is $ k $-convex, negative in $ \Omega $. Notice that such values of $ \widetilde{\lambda} > 0 $ exist by (5.11) and that such a $ \psi $ exists by Lemma 5.2 (a), where we take the canonical $ \mathrm{USC} $ extension to the boundary of (5.2) so that (5.3) also holds for $ \psi $.

    Notice also that if $ \psi $ solves (5.13) then so does $ \gamma \psi $. Indeed, for each $ x_0 \in \Omega $, if $ \gamma \psi - \varphi $ has a local max in $ x_0 $ then $ \psi - \frac{1}{\gamma} \varphi $ with $ \gamma > 0 $ does too and hence

    $ γkSk(D2φ(x0))+˜λψ(x0)|ψ(x0)|k10,
    $
    (5.15)

    which gives (5.13) for $ \gamma \psi $ by multiplying (5.15) by $ \gamma^k > 0 $.

    Step 1: Show that $ \gamma' > 0 $ defined in (5.14) is finite: that is, one has

    $ supΩuψ<+.
    $
    (5.16)

    We begin by noting that $ \psi < 0 $ on $ \Omega $ and we have assumed that $ u $ has a negative minimum at $ \bar{x} \in \Omega $ so that the ratio is positive in $ \bar{x} $. Near the boundary, we make use of the boundary estimates of Proposition 4.1 for $ \psi $ and Proposition 4.2 for $ u $ to say that there exist $ C_1, C_2 > 0 $ such that

    $ ψ(x)C1d(x) for all xΩδ/2
    $
    (5.17)

    and

    $ u(x)C2d(x) for all xΩd0,
    $
    (5.18)

    where $ \delta > 0 $ is the parameter of Lemma 2.12 defining a good tubular neighborhood of $ \partial \Omega \in C^2 $ and $ d_0 \leq \delta $ depends on $ \mu $ (as defined in (4.18), which bounds the absolute values of the principal curvatures of $ \partial \Omega $), the monotonicity properties of $ \sigma_j $ for $ j \leq k $ on $ \overline{\Gamma}_k $ and their moduli of continuity. Hence, by picking

    $ \rho \leq \min \{ d_0, \delta/2 \} $

    and recalling that $ -\psi > 0 $ on $ \Omega $, we can use both (5.17) and (5.18) on $ \Omega_{\rho} $ to find

    $ \frac{u(x)}{\psi(x)} = \frac{-u(x)}{-\psi(x)} \leq \frac{C_2 \, d(x)}{C_1 \, d(x)} = \frac{C_2}{C_1} \ \ \text{for all} \ x \in \Omega_{\rho}; $

    that is

    $ supΩρuψC2C1<+.
    $
    (5.19)

    Now, on the compact set $ K : = \overline{\Omega \setminus \Omega_{\rho}} $ where $ -\psi \in \mathrm{LSC}(K) $ and positive and $ -u \in \mathrm{USC}(K) $ one has the existence of $ \widetilde{C}_1 > 0 $ and $ \widetilde{C}_2 $ such that

    $ -\psi(x) \geq \widetilde{C}_1 \gt 0 \ \ \text{and} \ \ -u(x) \leq \widetilde{C}_2 \ \ \text{for each} \ x \in K $

    to find

    $ supKuψ˜C2˜C1<+.
    $
    (5.20)

    Combining (5.19) with (5.20) gives the needed (5.16).

    Step 2: Reduce the proof to showing that there exists $ \widetilde{x} \in \Omega $ such that $ u(\widetilde{x}) < 0 $ and

    $ λ|u(˜x)|kγk˜λ|ψ(˜x)|k.
    $
    (5.21)

    Indeed, recalling that $ u(\widetilde{x}), \psi(\widetilde{x}) < 0 $, $ 0 < \lambda < \widetilde{\lambda} < \lambda_1^{-} $ and $ \gamma^{\prime} : = \sup_{\Omega}(u/\psi) $, from (5.21) one finds

    $ ˜λλγk(u(˜x)ψ(˜x))k(γ)k.
    $
    (5.22)

    Now, choose the free parameter $ \gamma \in (0, \gamma^{\prime}) $ to satisfy

    $ γ>(λ˜λ)1/kγ,
    $
    (5.23)

    which can be done since $ \gamma \in (0, \gamma^{\prime}) $ and $ (\lambda/\widetilde{\lambda})^{1/k} < 1 $. Raising the inequality (5.23) to power $ k $ and multiplying by $ \widetilde{\lambda} > 0 $ gives a contradiction to the inequality (5.22). This completes the proof of the theorem, modulo showing that such an $ \widetilde{x} $ exists.

    Step 3: Exhibit $ \widetilde{x} \in \Omega $ such that $ u(\widetilde{x}) < 0 $ and (5.21) holds.

    In order to find $ \tilde{x} \in \Omega $ such that (5.21) holds when comparing $ u $ to $ \gamma \psi $, we make use of the classical viscosity device of looking at the maximum values of the family of upper semicontinuous functions defined by doubling variables and with an increasing (in $ j \in {\mathbb N} $) quadratic penalization

    $ Ψj(x,y):=γψ(x)u(y)j2|xy|2,  (x,y)¯ΩׯΩ, jN.
    $
    (5.24)

    For simplicity of notation, we will suppress the free parameter $ \gamma \in (0, \gamma^{\prime}) $ in the notation for $ \Psi_j $ (as well in certain $ \gamma $-dependent quantities below), thinking of $ \gamma \in (0, \gamma^{\prime}) $ as arbitrary, but fixed.

    First, notice that for each $ j \in {\mathbb N} $, $ \Psi_j \in \mathrm{USC}(\overline{\Omega} \times \overline{\Omega}) $ will have a maximum value

    $ Mj:=max(x,y)¯ΩׯΩΨj(x,y)<+.
    $
    (5.25)

    Claim: For each $ j \in {\mathbb N} $, the maximum $ M_j $ defined in (5.25) is positive.

    For each fixed $ \gamma \in (0, \gamma^{\prime}) $, we will show that

    $ Ψj(x,x):=γψ(x)u(x).
    $
    (5.26)

    must have a positive value in the interior of $ \Omega $, and hence the claim. Assume to the contrary that $ \Psi_j (x, x) \leq 0 $ on $ \Omega $; that is, for each $ x \in \Omega $, assume that

    $ \gamma \psi(x) \leq u(x) \ \ \Leftrightarrow \ \ \frac{u(x)}{\psi(x)} \leq \gamma, $

    since $ \psi < 0 $ on $ \Omega $. This implies that $ \gamma^{\prime} $ which is the sup of $ u/\psi $ satisfies $ \gamma^{\prime}\leq\gamma $. However this is a contradiction since $ \gamma < \gamma^{\prime} $, which completes the claim.

    Hence, using the claim, for each fixed $ \gamma \in (0, \gamma^{\prime}) $, there exists $ \bar{x} \in \Omega $ such that

    $ Mj:=max¯ΩׯΩΨjΨj(ˉx,ˉx)=γψ(ˉx)u(ˉx):=ˉm>0, jN.
    $
    (5.27)

    Notice that the maximum values $ M_j $ decrease as $ j $ increases so that

    $ M:=limj+Mj=infjNMjˉm>0.
    $
    (5.28)

    Using the finiteness of the limit $ M_{\infty} $ and the fact that $ u \geq 0 $ and $ \psi \leq 0 $ on $ \partial \Omega $ one has the following standard facts (see, for example, Lemma 3.1 of [8]).

    Lemma 5.6. For each $ j \in {\mathbb N} $ consider any pair $ (x_j, y_j) \in \overline{\Omega} \times \overline{\Omega} $ such that

    $ Mj:=max¯ΩׯΩΨj=Ψj(xj,yj).
    $
    (5.29)

    One has

    $ limj+j|xjyj|2=0  and  hence  (xjyj)0 as j+;
    $
    (5.30)
    $ (xj,yj)Ω×Ω  for  all j sufficiently  large;
    $
    (5.31)

    and for any accumulation point $ \tilde{x} $ of the bounded sequence $ \{x_j\}_{j \in {\mathbb N}} $ one has

    $ 0<ˉmM=γψ(˜x)u(˜x)=max(x,y)¯ΩׯΩ(γψ(x)u(y))
    $
    (5.32)

    and hence $ \tilde{x} \in \Omega $ since $ \gamma \psi, -u \leq 0 $ on $ \partial \Omega $.

    Proof. For completeness, we sketch the argument. The claim (5.30) follows from the fact that for each $ j \in {\mathbb N} $ one has

    $ M_{j/2} \geq \Psi_{j/2}(x_j,y_j) = M_j + \frac{j}{4} |x_j - y_j|^2 $

    and hence by (5.28)

    $ 0 \leq \frac{j}{4} |x_j - y_j|^2 \leq M_{j/2} - M_j \to 0 $

    Next, by (5.29) with $ \Psi_j $ as defined in (5.24), one has

    $ M_j = \gamma \psi(x_j) - u(y_j) - \frac{j}{2} |x_j - y_j|^2 \geq \bar{m} \gt 0 $

    and hence (5.30) yields

    $ \gamma \psi(x_j) - u(y_j) \gt 0 \ \ \text{for all sufficiently large} \ j. $

    Hence for large $ j $ one has (5.31) since $ \gamma \psi, -u \leq 0 $ on $ \partial \Omega $ and $ x_j - y_j \to 0 $ as $ j \to + \infty $. Finally, for the claim (5.32), if $ x_{j_k} \to \tilde{x} $ as $ k \to + \infty $, then so does $ y_{j_k} $ and using (5.30) plus the fact that $ \gamma \psi, -u \in \mathrm{USC}(\overline{\Omega}) $ yields

    $ M_{\infty} = \limsup\limits_{k \to + \infty} \left(\gamma \psi (x_{j_k}) - u(y_{j_k}\right) \leq \gamma \psi(\tilde{x}) - u(\tilde{x}) = \Psi_{j_k}(\tilde{x}, \tilde{x}) \leq M_{j_k}, \ \ \forall \, k \in {\mathbb N}. $

    One can now exhibit $ \widetilde{x} \in \Omega $ such that $ u(\widetilde{x}) < 0 $ and (5.21) holds. The idea is to apply Ishii's lemma (as given in the discussion of the formulas (3.9) and (3.10) in Crandall-Ishii-Lions [8]) along positive interior (local) maximum points of $ \Psi_j $ and using that $ \gamma \psi $ and $ u $ are viscosity sub and supersolutions in $ \Omega $. More precisely, if

    $ \Psi_j(x,y) : = \gamma \psi(x) - u(y) - \frac{j}{2} |x-y|^2 \in \mathrm{USC}(\overline{\Omega} \times \overline{\Omega}) $

    has a local maximum in $ (x_j, y_j) \in \Omega \times \Omega $, then by Lemma 5.6, for large $ j $ these local maxima lie in $ \Omega \times \Omega $ and by Ishii's lemma there exist $ X_j, Y_j \in \mathcal{S}(N) $ such that

    $ (j(xjyj),Xj)¯J2,+γψ(xj)  and  (j(xjyj),Yj)¯J2,u(yj)
    $
    (5.33)

    where

    $ XjYj  in S(N).
    $
    (5.34)

    Furthermore, by the last part of Lemma 5.6, there exists $ \widetilde{x} \in \Omega $ such that, up to a subsequence,

    $ (xj,yj)˜x  as j+.
    $
    (5.35)

    Now, since $ \gamma \psi $ is $ \Sigma_k $-subharmonic ($ k $-convex) in $ \Omega $, for each $ x \in \Omega $ and for every $ p \in {\mathbb R}^N $ one has

    $ (p,A)J2,+γψ(x)  AΣk,
    $
    (5.36)

    but $ \Sigma_k $ is closed and from the first statement of (5.33) it follows that

    $ XjΣk.
    $
    (5.37)

    By the positivity property (2.27), combining (5.34) and (5.37) yields

    $ YjΣk.
    $
    (5.38)

    We remark that this is the key observation that indicates why Ishii's lemma continues to be useful in the case of viscosity solutions with admissibility constraints satisfying the positivity property (2.27).

    Next, using that $ \gamma \psi $ and $ u $ are $ \Sigma_k $-admissible subsolutions and supersolutions of (5.13) and (5.9) respectively, one has for all large $ j $

    $ Sk(Xj)+˜λγkψ(xj)|ψ(xj)|k10
    $
    (5.39)

    and

    $ Sk(Yj)+λu(yj)|u(yj)|k10
    $
    (5.40)

    where we have used the fact that $ Y_j \in \Sigma_k $ in the supersolution definition (see Definition 2.5 (b)). Using (5.39), (5.40) and the monotonicity property (2.29) of $ S_k $ on $ \Sigma_k $ (which applies by (5.37) and (5.34)), for all large $ j \in {\mathbb N} $ we have

    $ ˜λγk(ψ(xj)|ψ(xj)|k1Sk(Xj)Sk(Yj)u(yj)λ|u(yj)|k1.
    $
    (5.41)

    Since $ \psi < 0 $ on $ \Omega $, all of the expressions in (5.41) are positive and hence

    $ u(yj)<0  for all large j.
    $
    (5.42)

    Now since $ -\psi > 0 $ is $ \mathrm{LSC}(\Omega) $ and $ -u \in \mathrm{USC}(\Omega) $, from (5.41) one finds

    $ 0<˜λγk(ψ(˜x))klim infj+˜λγk(ψ(xj))klim supj+λ(u(yj))kλ(u(˜x))k,
    $
    (5.43)

    which gives the needed inequality (5.21). Finally, since $ u $ is $ \mathrm{LSC}(\Omega) $, by (5.42), we have $ u(\widetilde{x}) \leq 0 $, but it cannot vanish by (5.43). Thus $ u(\widetilde{x}) < 0 $ as needed.

    An immediate consequence of the minimum principle are the following characterizations of the principal eigenvalue of $ S_k $ discussed by Wang [32] and Lions [26] (in the case $ k = N $) using the variational structure of $ S_k $. See also Jacobsen [22] for a bifurcation approach.

    Corollary 5.7. Let $ \Omega $ be as in Theorem 5.4 and let $ k \geq 2 $. Then $ \lambda_1^{-}(S_k, \Sigma_k) $ as defined by (5.4) and (5.5) is equal to $ \lambda_1^{(k)} $ defined by

    $ λ(k)1:=infuΦk0(Ω){ΩuSk(D2u)dx:  ||u||Lk+1(Ω)=1},
    $
    (5.44)

    where $ \Phi_0^k(\Omega) = \{ u \in C^2(\Omega): S_k(D^2 u) \in \Gamma_k \ \ {\rm and} \ \ u = 0 \ {\rm on} \ \partial \Omega \} $ and $ \Gamma_k $ is the open cone (2.3). When $ k = N $, one has

    $  λ(N)1:=inf{λa1: aC(¯Ω,S(N)) such that  a>0,detaNN in ¯Ω,}
    $
    (5.45)

    and $ \lambda_1^a $ is the first eigenvalue of the uniformly elliptic operator $ - \sum_{i, j = 1}^N a_{ij} D_{ij} $.

    Proof. Since there exists a $ k $-convex principal eigenfunction $ \psi_1 $ which is negative in the interior and vanishes on the boundary, by the definition of $ \lambda_1^{-}(S_k, \Sigma_k) $, one has $ \lambda_1^{(k)} \leq \lambda_1^{-}(S_k, \Sigma_k) $. If $ \lambda_1^{(k)} < \lambda_1^{-}(S_k, \Sigma_k) $, then $ \psi_1 $ would be a $ \Sigma_k $-admissible supersolution of (5.9) with $ \lambda = \lambda_1^{(k)} $ and hence $ \psi_1 \geq 0 $ in $ \Omega $ by the minimum principle (5.9), which is absurd.

    Even though Corollary 5.7 shows that a negative principal eigenfunction $ \psi_1 $ exists for $ \lambda_1^{-} = \lambda_1^{-}(S_k, \Sigma_k) $, in order to illustrate a general method which should apply also to non variational perturbations of $ S_k $, we will give an alternative proof of the existence of $ \psi_1 $ by maximum principle methods for $ \Sigma_k $-admissible viscosity solutions.

    Since the complete argument to solve (1.8) is somewhat involved, perhaps it is worth giving the general idea first. We will show that $ \psi_1 \in C(\overline{\Omega}) $ is the limit as $ n \to +\infty $ (up to an extracted subsequence) of the normalized solutions

    $ w_n : = \frac{v_n}{||v_n||_{\infty}} $

    where each $ v_n \in C(\overline{\Omega}) $ is a $ \Sigma_k $-admissible viscosity solution of the auxiliary problem

    $ {Sk(D2vn)=1λnvn|vn|k1in Ωvn=0on Ω
    $
    (6.1)

    and $ \{ \lambda_n \}_{n \in {\mathbb N}} $ is any fixed sequence of spectral parameters with $ 0 < \lambda_n \nearrow \lambda_1^{-} $ as $ n \to + \infty $. The existence of the solutions $ v_n $ to (6.1) presents the same difficulties as mentioned above for (1.8), but for each fixed $ \lambda \in (0, \lambda_1^-) $ we will show that the problem

    $ {Sk(D2u)=1λu|u|k1in Ωu=0on Ω
    $
    (6.2)

    has a $ \Sigma_k $-admissible solution $ u \in C(\overline{\Omega}) $ by an inductive procedure starting from $ u_0 = 0 $ and then solving

    $ {Sk(D2un)=1λun1|un1|k1:=fnin Ωun=0on Ω
    $
    (6.3)

    for a decreasing sequence of $ \Sigma_k $-admissible solutions $ \{u_n\}_{n \in {\mathbb N}} \subset C(\overline{\Omega}) $ (which are negative in $ \Omega $) and then pass to the limit as $ n \to +\infty $. Notice that the equation in (6.3) is proper as $ u_n $ does not appear explicitly and hence the equation is non increasing in $ u_n $. Moreover, it will turn out that one can pass to the limit along a subsequence provided that there is a uniform Hölder bound on $ ||u_n||_{C^{0, \alpha}(\overline{\Omega})} $ for each $ n \in {\mathbb N} $ and some $ \alpha \in (0, 1] $.

    We begin with the following existence and uniqueness result for the underlying degenerate elliptic Dirichlet problems in (6.3) in the nonlinear case $ k \in \{ 2, \ldots, N\} $. While this result is not new, for completeness we prefer to discuss it.

    Theorem 6.1. Let $ \Omega $ be a strictly $ (k-1) $-convex domain of class $ C^2 $ and let $ f \in C(\overline{\Omega}) $ be a nonnegative function. There exists a unique $ k $-convex solution $ u \in C(\overline{\Omega}) $ of the Dirichlet problem

    $ {Sk(D2u)=fin Ωu=0on Ω.
    $
    (6.4)

    More precisely, there is $ \Sigma_k $-admissible solution $ u \in C(\overline{\Omega}) $ of $ S_k(D^2 u) - f(x) = 0 $ in $ \Omega $ in the sense of Definition 2.5(c) such that $ u = 0 $ on $ \partial \Omega $.

    Proof. The existence and uniqueness for $ \Sigma_k $-admissible viscosity solutions follows from the main results in [6]. See Theorem 1.2 as applied in section 5 of that paper. When $ f > 0 $, one has smooth solutions if $ \partial \Omega $ is smooth as follows from [5].

    Briefly, we give an idea of the proof for completeness sake. A $ \Sigma_k $-admissible viscosity solution of (6.4) is a $ \Theta_k $-harmonic function which vanishes on the boundary where $ \Theta_k: \Omega \to \mathcal{S}(N) $ is the uniformly continuous elliptic map defined by

    $ Θk(x):={AΣk: Fk(x,A):=Sk(A)f(x)0}  for each xΩ.
    $
    (6.5)

    The uniform continuity is with respect to the Hausdorff distance on $ \mathcal{S}(N) $ and follows from the uniform continuity of $ f \in C(\overline{\Omega}) $. Using Propositions 5.1 and 5.3 of [6], one has the equivalence between $ u \in C(\Omega) $ being $ \Theta_k $-harmonic and $ u $ being a $ \Sigma_k $-admissible viscosity solution of $ F_k(x, D^2u) = 0 $ since one can easily verify the needed structural conditions ((1.14)–(1.16) and (1.18)); that is,

    $ Fk(x,A+P)Fk(x,A)  for each xΩ,AΣk,PP;
    $
    (6.6)
    $ for each xΩ there exists AΣk such that Fk(x,A)=0;
    $
    (6.7)
    $ Σk{AS(N): Fk(x,a)0} for each xΩ;
    $
    (6.8)

    and

    $ Fk(x,A)>0  for each xΩ and each AΘk(x).
    $
    (6.9)

    Conditions (6.6)–(6.8) say that $ \Theta_k $ defined by (6.5) is an elliptic branch of the equation $ F_k(x, D^2u) = 0 $ in the sense of Kyrlov [23] (see Proposition 5.1 of [6]) and the non-degeneracy condition (6.9) ensures that $ \Theta_k $-superharmonics are $ \Sigma_k $-admissible viscosity supersolutions of $ F_k(x, D^2u) = 0 $ (see Proposition 5.3 of [6]). Finally the existence of a unique $ u \in C(\overline{\Omega}) $ which is $ \Theta_k $-harmonic taking on the continuous boundary value $ \varphi \equiv 0 $ follows from Perron's method (Theorem 1.2 of [6]) since $ \Theta_k $ is uniformly continuous and the strict $ (k-1) $-convexity implies the needed strict $ \overrightarrow{{\Sigma}}_k $ and $ \overrightarrow{{\widetilde{\Sigma}}}_k $ convexity (which is the content of Proposition 2.11).

    Remark 6.2. Using the language of Harvey-Lawson [16], one could also say that $ (S_k, \Sigma_k) $ is a compatible operator-subequation pair (see Definition 2.4 of [16]) and since the continuous boundary data $ \varphi \equiv 0 $ has its values in $ S_k(\Sigma_k) $, the result follows also from Theorem 2.7 of [16].

    Next we discuss the global Hölder regularity of the unique solution to Theorem 6.1 in the case $ k > N/2 $, which will lead to compactness for bounded sequences of solution.

    Theorem 6.3. Under the assumptions of Theorem 6.1, if $ k > N/2 $ then the unique solution $ u $ to the Dirichlet problem (6.4) belongs to $ C^{0, \alpha}(\overline{\Omega}) $ with $ \alpha : = 2 - N/k > 0 $. In particular, there exists $ C > 0 $ which depends on $ \Omega, \alpha $ and $ \sup_{\Omega}(-u) $ such that

    $ |u(x)u(y)|C|xy|α,   x,y¯Ω.
    $
    (6.10)

    Before giving the proof, we formalize a few observations concerning the restriction $ k > N/2 $ in the statement.

    Remark 6.4. For the proof of the global Hölder bound (6.10), we will adapt the technique developed in the celebrated paper of Ishii and Lions [17]. The key step involves a uniform local interior estimate which uses a comparison principle argument for the solution $ u $ (which is $ \Sigma_k $-subharmonic since $ f \geq 0 $) and a family of comparison functions defined in terms of the auxiliary function $ \phi(x): = |x|^\alpha $, where $ \alpha \in (0, 1] $. One needs that $ \phi $ is $ \Sigma_k $-superharmonic on its domain. It is known that for $ \alpha = 2-\frac{N}{k} $, the function $ \phi $ is a classical $ \Sigma_k $-harmonic away from the origin, but $ \alpha > 0 $ requires the condition $ k > N/2 $. This restriction can be interpreted in terms of the Riesz characteristic of the closed convex cone $ \Sigma_k \subset \mathcal{S}(N) $ as described in Harvey-Lawson [15]. Using the measure theoretic techniques developed by Trudinger and Wang [29,30] and Labutin [24], perhaps it is possible to obtain the global Hölder bound (6.10) if $ k \leq N/2 $. However, our intended focus is limited to maximum principle techniques and hence we have not pursue such improvements here.

    Proof of Theorem 6.3. Since $ u \in C(\overline{\Omega}) $ by Theorem 6.1, the claim that $ u \in C^{0, \alpha}(\overline{\Omega}) $, reduces to proving the estimate (6.10). Notice that $ u $ is $ k $-convex (it is a $ \Sigma_k $-admissible subsolution) and $ u $ vanishes on the boundary and hence $ u \leq 0 $ in $ \Omega $ by Theorem 3.2. If $ f \equiv 0 $, then $ u \equiv 0 $ and the conclusion of Theorem 6.3 holds trivially. Otherwise, $ u < 0 $ in $ \Omega $ by Theorem 3.2 and

    $ ||u||:=supΩ|u|=supΩ(u).
    $
    (6.11)

    For the Hölder estimate (6.10), it suffices to find $ \rho > 0 $ and $ C_{\rho} > 0 $ for which

    $ |u(x)u(y)|Cρ|xy|α,   x,y¯Ω  with |xy|<ρ.
    $
    (6.12)

    In fact, as is well known, if (6.12) holds, then using the boundedness of $ u $ one has

    $ \sup\limits_{\substack{x, y \in \overline{\Omega} \\ x \neq y}} \frac{|u(x) - u(y)|}{|x-y|^{\alpha}} \leq \max \left\{ \frac{2 ||u||_{\infty}}{\rho^{\alpha}}, C_{\rho} \right\}. $

    In order to prove (6.12), first consider the case when $ y $ lies on $ \partial \Omega $ (the argument for $ x \in \partial \Omega $ is the same). In this case, $ u(y) = 0 $ and $ u(x) \leq 0 $. Then the boundary estimate of Proposition 4.3 shows that $ y \in \partial \Omega $ and each $ x \in \Omega_{d_0} $ one has

    $ |u(y)u(x)|=u(x)C3d(x)=C3minzΩ|xz|C3|xy|.
    $
    (6.13)

    By choosing

    $ ρmin{d0,1}  and  CρC3
    $
    (6.14)

    one has (6.12) for each $ \alpha \in (0, 1] $ if $ y $ (or $ x $) lies on the boundary.

    Next, let $ y \in \Omega $ and consider the comparison function

    $ vy(x):=u(y)+Cρ|xy|α
    $
    (6.15)

    One wants determine $ \rho > 0 $ sufficiently small and $ C_{\rho} > 0 $ sufficiently large (recall the restrictions (6.14)) so that

    $ u(x)vy(x)  for each xΩBρ(y)
    $
    (6.16)

    and hence

    $ u(x)u(y)Cρ|xy|α  for each xΩBρ(y).
    $
    (6.17)

    Then, by exchanging the roles of $ x $ and $ y $, one would have

    $ |u(x)u(y)|Cρ|xy|α  for each x,yΩ with |xy|<ρ,
    $
    (6.18)

    which would then complete the proof.

    In order to establish (6.16), notice that $ u $ is a $ \Sigma_k $-admissible solution of $ S_k(D^2u) = f \geq 0 $ in $ \Omega $. In particular, $ u $ is $ \Sigma_k $-subharmonic ($ k $-convex) in $ \Omega $. Moreover, for $ k > N/2 $ one knows that for each $ y \in {\mathbb R}^N $, the function defined by

    $ wk(x):=|xy|2N/k  for xRN{y}
    $
    (6.19)

    is smooth, $ k $-convex and satisfies $ S_k(w_k) \equiv 0 $ on its domain (see section 2 of [30]). The same is obviously true for the translated version $ v_y $ of (6.15) with the choice $ \alpha: = 2 - N/k $ when $ k > N/2 $. Indeed, using the radial formula (2.70) of Lemma 2.14 with $ h(r): = u(y) + C_{\rho} \, r^{\alpha} $ one finds that

    $ Sj(D2vy(x))=(Cρα|xy|α2)j(N1)!j!(Nj)![(α2)j+N]  for each xy.
    $
    (6.20)

    When $ \alpha = 2 - N/k $, this is positive for every $ j = 1, \ldots, k-1 $ and it vanishes for $ j = k $. In particular, $ v_y $ is $ \Sigma_k $-superharmonic in every punctured ball $ \dot{B}_{\rho}(y) = B_{\rho}(y) \setminus \{y\} $. Hence, by the comparison principle (Theorem 3.1) for $ \Sigma_k $ sub and superharmonics we will have

    $ u(x)vy(x)  for each xΩ˙Bρ(y)
    $
    (6.21)

    provided that

    $ uvy  on (Ω˙Bρ(y))
    $
    (6.22)

    where $ \partial(\Omega \cap \dot{B}_{\rho}(y)) = \{y\} \cup (\partial B_{\rho}(y) \cap \Omega) \cup (\partial \Omega \cap \overline{B}_{\rho}(y)) $.

    We analyze the three possibilities. At the point $ y $, one has

    $ u(y) = v_y(y) = u(y) + C_{\rho} \, |y - y|. $

    Next, for $ x \in \partial \Omega \cap \overline{B}_{\rho}(y) $ (which is empty if $ B_{\rho}(y) \subset \subset \Omega $) one has

    $ u(x) = 0 \ \ \text{while} \ v_y(x) = u(y) + C_{\rho} \, |x-y|^{\alpha}, $

    where $ u(y) < 0 $ for $ y \in \Omega $ as noted above. Since $ x \in \partial \Omega $, with $ \rho \leq d_0 $ the condition $ |x-y| < \rho $ means that $ y \in \Omega_{d_0} $ and one can again use the boundary estimate of Proposition 4.3 to estimate $ u(y) $ from below

    $ v_y(x) \geq -C_3 \, |x-y| + C_{\rho} \, |x-y|^{\alpha} \geq (C_{\rho} - C_3)|x - y|^{\alpha} \geq 0, $

    provided that $ \rho \leq 1 $ and $ C_{\rho} \geq C_3 $ as in (6.14). Finally, if $ x \in \partial B_{\rho}(y) \cap \Omega $ we will have $ v_y(x) = u(y) + C_{\rho} \, |x-y|^{\alpha} \geq u(x) $ if

    $ |u(x) - u(y)| \leq C_{\rho} \, \rho^{\alpha}. $

    Having now fixed $ \rho \leq \min \{d_0, 1\} $, since $ |u(x) - u(y)| \leq 2 ||u||_{\infty} $ it is enough to choose

    $ Cρ2||u||ρα,
    $
    (6.23)

    in addition to $ C_{\rho} \geq C_3 $.

    We now implement the iteration scheme (sketched above) to prove the existence of a principal eigenfunction $ \psi_1 $ associated to $ \lambda_1^{-} = \lambda_1^{-}(S_k, \Sigma_k) $ in the "regular case" with $ k > N/2 $.

    Remark 6.5. We will make use of the fact that the sets of $ \Sigma_k $-subharmonic and $ \Sigma_k $-superharmonic functions on $ \Omega $ are closed under the operation of taking uniform limits in $ \Omega $ of sequences. See property (5)' in [11], for example.

    Theorem 6.6. Suppose that $ k > N/2 $. Let $ \Omega $ be a strictly $ (k-1) $-convex domain of class $ C^2 $. If $ \{v_n\}_{n \in {\mathbb N}} $ is the sequence of $ k $-convex solutions of (6.1) with $ 0 < \lambda_n \nearrow \lambda_1^{-} $ as $ n \to + \infty $, then the normalized sequence defined by $ w_n: = v_n/||v_n||_{\infty} $ admits a subsequence which converges uniformly to a principal eigenfunction $ \psi_1 $ for (1.8), which is negative on $ \Omega $.

    Proof. We divide the proof into two big steps, with several claims to be justified.

    Step 1: For each $ \lambda \in (0, \lambda_1^-) $, show that there exists a $ \Sigma_k $-admissible solution $ u $ to the Dirichlet problem (6.24); that is,

    $ {Sk(D2u)=1λu|u|k1in Ωu=0on Ω.
    $
    (6.24)

    As indicated above, we will look for $ u $ as a decreasing limit of solutions $ \{u_n\}_{n \in {\mathbb N}_0} $ of the Dirichlet problem (6.3), that is,

    $ {Sk(D2un)=1λun1|un1|k1:=fnin Ωun=0on Ω
    $
    (6.25)

    With $ u_0 \equiv 0 $, we apply Theorem 6.1 to find $ u_1 \in C(\overline{\Omega}) $ a $ \Sigma_k $-admissible solution of

    $ \mbox{ $S_k(D^2u_1) = 1$ in $\Omega$ and $u_1 = 0$ on $\partial \Omega$.} $

    Since $ u_1 $ is a $ \Sigma_k $-admissible solution it is necessarily $ k $-convex and hence satisfies the (strong) maximum principle so that $ u_1 \leq 0 $ on $ \overline{\Omega} $ (and $ u_1 < 0 $ in $ \Omega $) and hence

    $ f_2: = 1 - \lambda u_1 |u_1|^{k-1} = 1 + \lambda |u_1|^k \geq 0 $

    and the induction proceeds using Theorem 6.1 to produce the sequence $ \{u_n\}_{n \in {\mathbb N}_0} $ of non-positive $ \Sigma_k $-admissible solutions which also satisfy

    $ un<0  on Ω for each nN.
    $
    (6.26)

    Claim 1: $ \{u_n\}_{n \in {\mathbb N}_0} $ is a decreasing sequence of $ k $-convex functions.

    By construction, all of the functions vanish on $ \partial \Omega $ and are negative in $ \Omega $ for $ n \geq 1 $. We use induction. As we have seen $ u_1 < 0 : = u_0 $ on $ \Omega $. Assuming that $ u_{n} \leq u_{n-1} $ on $ \Omega $, we need to show that $ u_{n+1} \leq u_n $ on $ \Omega $. We have that $ u_{n+1} $ is a $ \Sigma_k $-admissible solution of

    $ S_k(D^2 u_{n+1}) = 1 - \lambda u_n |u_n|^{k-1} = 1 + \lambda |u_n|^{k} \ \ \text{in} \ \Omega, $

    where we have again used $ u_n \leq 0 $, but then the inductive hypothesis yields

    $ unun10    |un|=unun1=|un1|
    $
    (6.27)

    and hence

    $ S_k(D^2 u_{n+1}) \geq 1 + \lambda |u_{n-1}|^k = f_n = S_k(D^2u_n). $

    By the comparison principle, one concludes that $ u_{n+1} \leq u_n $ on $ \Omega $.

    Claim 2: The sequence $ \{u_n\}_{n \in {\mathbb N}} $ is bounded in sup norm; that is, there exists $ M > 0 $ such that

    $ ||un||=supΩ(un)M  foreach nN.
    $
    (6.28)

    We argue by contradiction, assuming that the increasing sequence $ ||u_n||_{\infty} $ satisfies $ \lim_{n \to +\infty} ||u_n||_{\infty} = +\infty $. Since $ u_n < 0 $ on $ \Omega $ for each $ n \in {\mathbb N} $, we can define

    $ vn:=un||un||  so that  ||vn||=1  for each nN.
    $
    (6.29)

    Since the equation $ S_k(D^2u_n) = 1 + \lambda |u_{n-1}|^k $ is homogeneous of degree $ k $, one has

    $ Sk(D2vn)=1||un||k+λ||un1||k||un||k|vn1|k.
    $
    (6.30)

    Now, making again use of the negativity and monotonicity in (6.27) one has

    $ βn:=||un1||k||un||k(0,1]
    $
    (6.31)

    and combining (6.30) with (6.31) yields

    $ Sk(D2vn)=1||un||k+λβn|vn1|k:=gn,
    $
    (6.32)

    where $ g_n\in C(\overline{\Omega}) $ and is non-negative. Since $ k > N/2 $ and since the global Hölder bound of Theorem 6.3 depends only on $ \Omega, \alpha $ and $ ||v_n||_{\infty} \equiv 1 $, the sequence of solutions $ \{v_n\}_{n \in {\mathbb N}} $ is bounded in $ C^{0, 2 - N/k}(\overline{\Omega}) $ and hence admits $ v \in C(\overline{\Omega}) $ and a subsequence such that

    $ vnjv  uniformly on ¯Ω.
    $
    (6.33)

    In addition, $ 0 < \beta_{n_j} \leq 1 $ is increasing so converges to some $ \beta_{\infty} \in (0, 1] $. The uniform limit $ v $ is a $ \Sigma_k $-admissible (super)solution of

    $ \mbox{ $S_k(D^2 v) + \lambda \beta_{\infty} v |v|^{k-1} = 0$ in $\Omega$ $v = 0$ on $\partial \Omega$,} $

    where $ \lambda \beta_{\infty} \leq \lambda < \lambda_1^- $. By the minimum principle characterization of $ \lambda_1^- $, we must have $ v \geq 0 $ in $ \Omega $. However, each $ u_n \in C(\overline{\Omega}) $ is negative in $ \Omega $ and hence has a negative minimum at some interior point $ x_n \in \Omega $ and hence $ v_n(x_n) = -1 $ for each $ n $ which contradicts the fact that uniform limit of (6.33) satisfies $ v \geq 0 $ on $ \Omega $.

    Claim 3: The sequence $ \{ u_n \}_{n \in {\mathbb N}} $ admits a subsequence $ \{u_{n_j}\}_{j \in {\mathbb N}} \subset C(\overline{\Omega}) $ which converges uniformly on $ \overline{\Omega} $ to a $ \Sigma_k $-admissible solution $ u $ of (6.24).

    Exploiting the boundedness of Claim 3 for the sequence $ \{ u_n \}_{n \in {\mathbb N}} $, we can use the same argument involving the global Hölder estimate of Theorem 6.3 to extract a uniformly convergent subsequence with limit $ u \in C(\overline{\Omega}) $ with limit $ u $ which is a $ \Sigma_k $-admissible solution of (6.24). This completes Step 1 of the proof.

    Step 2: Show that there exists $ \psi_1 \in C(\overline{\Omega}) $ which is negative in $ \Omega $ and is a $ \Sigma_k $-admissible solution of (1.8); that is,

    $ {Sk(D2ψ1)+λ1ψ1|ψ1|k1=0in Ωψ1=0on Ω.
    $
    (6.34)

    Consider a sequence $ \{ \lambda_n\}_{n \in {\mathbb N}} \in (0, \lambda_1^-) $ with $ \lambda_n \nearrow \lambda_1^- $ and the associated sequence $ \{ v_n\}_{n \in {\mathbb N}} \subset C(\overline{\Omega}) $ of solutions to (6.24) with $ \lambda = \lambda_n $; that is,

    $ {Sk(D2vn)=1λnvn|vn|k1in Ωvn=0on Ω.
    $
    (6.35)

    Since each $ v_n $ is $ \Sigma_k $-subharmonic in $ \Omega $ and vanishes on the boundary, $ v_n < 0 $ on $ \Omega $ for each $ n $.

    Claim 4: One has $ ||v_n||_{\infty} \to + \infty $ as $ n \to +\infty $.

    We argue by contradiction. If not, then again by the global Hölder bound of Theorem 6.3 we can extract a subsequence of these functions which are $ \Sigma_k $-subharmonic and negative in $ \Omega $ and which converges uniformly on $ \overline{\Omega} $ to a $ \Sigma_k $-admissible solution $ w \in C(\overline{\Omega}) $ to the Dirichlet problem

    $ {Sk(D2w)+λ1w|w|k1=1in Ωw=0on Ω.
    $
    (6.36)

    Since $ w \in C(\overline{\Omega}) $ is non-positive, there exists $ \varepsilon > 0 $ such that

    $ εw|w|k11  in ¯Ω.
    $
    (6.37)

    Hence $ w $ is a $ k $-convex, negative in $ \Omega $ and satisfies (in the $ \Sigma_k $-admissible viscosity sense)

    $ Sk(D2w)+(λ1+ε)w|w|k10,
    $
    (6.38)

    which contradicts the Definition 5.1 of $ \lambda_1^-(S_k, \Sigma_k) $ which is finite by Theorem 7.1. Hence Claim 4 holds.

    Finally, consider the normalized sequence defined by $ w_n: = v_n/||v_n||_{\infty} $ which are $ \Sigma_k $-admissible viscosity solutions of

    $ Sk(D2wn)+λnwn|wn|k1=1||vn||  in Ω    and wn=0  on Ω.
    $
    (6.39)

    The uniformly bounded sequence $ \{w_n\}_{n \in {\mathbb N}} \subset C(\overline{\Omega}) $ admits a subsequence which converges uniformly on $ \overline{\Omega} $ some $ \psi_1 \in C(\overline{\Omega}) $ which is a $ \Sigma_k $-admissible solution of the eigenvalue problem (1.8) as $ \frac{1}{||v_n||_{\infty}} \to 0 $ as $ n \to + \infty $.

    In this section, we will provide an upper bound for the generalized principle eigenvalue $ \lambda_1^-(S_k, \Sigma_k) $ as defined in Definition 5.1. Recall that the lower bound

    $ λ1(Sk,Σk)2kCN,kR2k  with  CN,k=(Nk)
    $
    (7.1)

    was given in Lemma 5.2 for bounded domains $ \Omega $ which are contained in a ball $ B_R(0) $.

    An upper bound will be found by constructing a suitable test function which contradicts the minimum principle of Theorem 5.4 on a ball $ B_R(0) \subset \Omega $ and makes use of the monotonicity of $ \lambda_1^-(S_k, \Sigma_k) $ with respect to set inclusion. More precisely, if we denote by $ \lambda_1^-(\Omega) $ the generalized principal eigenvalue $ \lambda_1^-(S_k, \Sigma_k) $ with respect to the bounded domain $ \Omega $ then one has that

    $ ΩΩ    λ1(Ω)λ1(Ω).
    $
    (7.2)

    Indeed, since

    $ \lambda_1^{-}(\Omega): = \sup \{ \lambda \in {\mathbb R}: \ \exists \, \psi \in \Phi_k^{-}(\Omega) \ \text{with} \ S_k(D^2 \psi) + \lambda \psi |\psi|^{k-1} \geq 0 \ \text{in} \ \Omega\}, $

    if $ \lambda $ admits such a $ \psi $ for $ \Omega $ then it also admits $ \psi $ for $ \Omega^{\prime} $ and hence (7.2) holds. Our upper bound is contained in the following theorem.

    Theorem 7.1. If a bounded domain $ \Omega $ contains the ball $ B_R = B_R(0) $, then

    $ λ1(Ω)2kγN,kCN,kR2k
    $
    (7.3)

    where

    $ CN,k=(Nk)andγN,k:=1N(N+2kk+1)k+1.
    $
    (7.4)

    Proof. Consider the radial test function (as used in [5]) defined by

    $ u(x):=14(R2|x|2)2
    $
    (7.5)

    and let $ r: = |x| $. It suffices to show that $ u $ is a $ \Sigma_k $-admissible supersolution of

    $ Sk(D2u)+λu|u|k1=0 in BR
    $
    (7.6)

    with

    $ λ=2kγN,kCN,kR2k.
    $
    (7.7)

    Indeed, notice that:

    $ uC(RN)  and hence uLSC(¯BR);
    $
    (7.8)
    $ u=0 on BR;
    $
    (7.9)

    and

    $ BRC and BR is strictly (k1)-convex for each k{1,,N}.
    $
    (7.10)

    However,

    $ u<0 on BR
    $
    (7.11)

    and hence $ u $ does not satisfy the minimum principle of of Theorem 5.4 on $ B_R $ and hence one must have

    $ \lambda = 2^k \gamma_{N,k} C_{N,k} R^{-2k} \geq \lambda_1^{-}(B_R) \geq \lambda_1^{-}(\Omega), $

    which would complete the proof.

    Since $ u \in C^2(B_R) $, it will be a $ \Sigma_k $-admissible supersolution of (7.6) provided that

    $ Sk(D2u(x))+λu(x)|u(x)|k10 for each xBR,
    $
    (7.12)

    as follows easily from Remark 2.7 (b) by taking $ \varphi = u $ as the lower test function. Using the radial formula (2.71) with $ h(r): = -(R^2-r^2)^2/4 $ one computes to find

    $ Sk(D2u)+λu|u|k1=(Nk)(R2r2)k1g(r)
    $
    (7.13)

    where

    $ g(r)=R2(1+2kN)r2γN,k2kR2k(R2r2)k+1.
    $
    (7.14)

    We will have the needed inequality (7.12) if we show that $ g $ defined in (7.14) satisfies

    $ g(r)0  for each r[0,R)  where again γN,k=1N(N+2kk+1)k+1.
    $
    (7.15)

    Notice that $ g(R) = -\frac{2k}{N} R^2 < 0 $ and $ g(0) = R^2(1 - 2^{-k} \gamma_{N, k}) \leq 0 $ provided that

    $ ˜γN,k:=2kγN,k=12kN(N+2kk+1)k+11  for each k{1,,N}.
    $
    (7.16)

    The lower bounds in (7.16) do hold. To see this, the cases $ N = 1 $ and $ N = 2 $ are easily checked. Next, a simple computation shows that $ \widetilde{\gamma}_{N, 1} \geq 1 $ for all $ N $. Finally, rewriting $ \widetilde{\gamma}_{N, k} $ as

    $ \widetilde{\gamma}_{N,k} = \frac{2}{N} \left( 1 + \frac{N/2 - 1}{k+1} \right)^{k+1}, $

    one sees that $ \widetilde{\gamma}_{N, k} $ strictly increasing in $ k $ if $ N \geq 3 $ and hence $ \widetilde{\gamma}_{N, k} \geq \widetilde{\gamma}_{N, 1} \geq 1 $ also for $ N \geq 3 $.

    It remains to check that $ g \leq 0 $ on $ (0, R) $ and we simplify notation by setting $ \gamma: = \gamma_{N, k} $. Since

    $ g(r)=2r[1+2kNγ(k+1)2kR2k(R2r2)k]
    $
    (7.17)

    elementary calculus shows that there is a unique $ \bar{r} \in (0, R) $ such that

    $ g(ˉr)=0,  g(r)>0 for r(0,ˉr)  and g(r)<0 for r(ˉr,R).
    $
    (7.18)

    Hence we just need to show that $ g(\bar{r}) \leq 0 $. From (7.17), the critical value $ \bar{r} $ in (7.18) satisfies the relations

    $ γ2kR2k(R2ˉr2)k=N+2kN(k+1)andˉr2=(1δ)R2  with δ:=2[N+2kN(k+1)1γ]1/k,
    $

    and hence

    $ g(ˉr)=R2(2kN+δ(N+2k)kN(k+1))0
    $

    provided that

    $ \delta = 2 \left[ \frac{N + 2k}{N(k+1)} \frac{1}{\gamma} \right]^{1/k} \leq \frac{2(k+1)}{N + 2k} \ \ \Longleftrightarrow \ \ \gamma \geq \gamma_{N,k} = \frac{1}{N} \left( \frac{N + 2k}{k + 1} \right)^{k+1} . $

    The authors wish to thank an anonymous referee for the careful reading and suggestions which led to improvement of the original manuscript.

    Payne is partially supported by the Gruppo Nazionale per l'Analisi Matematica, la Probabilità e le loro Applicazioni (GNAMPA) of the Istituto Nazionale di Alta Matematica (INdAM) and the projects: GNAMPA 2017 "Viscosity solution methods for fully nonlinear degenerate elliptic equations", GNAMPA 2018 "Costanti critiche e problemi asintotici per equazioni completamente non lineari" e GNAMPA 2019 "Problemi differenziali per operatori fully nonlinear fortemente degeneri".

    The authors declare no conflict of interest.

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