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Partial regularity of stable solutions to the fractional Geľfand-Liouville equation

  • Ali Hyder and Wen Yang EMAIL logo
Published/Copyright: May 22, 2021

Abstract

We analyze stable weak solutions to the fractional Geľfand problem

(Δ)su=euinΩRn.

We prove that the dimension of the singular set is at most n − 10s.

MSC 2010: 35B65; 35J60; 35R11

1 Introduction

Let Ω be an open subset of ℝn. We consider the following fractional Geľfand equation

(Δ)su=euin ΩRn,n1, (1.1)

where s ∈ (0, 1), and u satisfies

euLloc1(Ω)anduLs(Rn).

Here the space Ls(ℝn) is defined by

Ls(Rn):=uLloc1:uLs(Rn)<,uLs(Rn):=Rn|u(x)|1+|x|n+2sdx<.

The non-local operator (−δ)s is defined by

(Δ)sφ(x)=cn,sP.V.Rnφ(x)φ(y)|xy|n+2sdy,

with cn,s:=22s1πn/2Γ(n+2s2)|Γ(s)| being a normalizing constant.

We are interested in the classical question of regularity of solutions to (1.1). More precisely, we aim at studying the partial regularity of stable weak solutions of (1.1). By a weak solution we mean that u satisfies (1.1) in the sense of distribution, that is

Rnu(Δ)sϕdx=Ωeuϕdx,ϕCc(Ω).

We recall that a solution u to (1.1) is said to be a stable weak solution if us(Ω) and

cn,s2RnRn(ϕ(x)ϕ(y))2|xy|n+2sdxdyRneuϕ2dx,ϕCc(Ω), (1.2)

where the function space s(Ω) is defined by

H˙s(Ω):=uLloc2(Ω)ΩΩ|u(x)u(y)|2|xy|n+2sdxdy<+.

For equation (1.1) in the whole space ℝn, the study on the classification of stable solutions and finite Morse index solutions has attracted a lot of attentions in recent decades. In the classical case, that is s = 1, Farina [11] and Dancer - Farina [3] established non-existence of stable solutions to (1.1) for 2 ≤ n ≤ 9 and non-existence of finite Morse index solutions to (1.1) for 3 ≤ n ≤ 9. A counterpart issue for equation (1.1) in a bounded domain is to analyze the extremal solutions. Let us first recall the definition of extremal solutions. Given a bounded smooth domain Ω ⊂ ℝn, consider the following problem

Δu+λf(u)=0inΩ,u=0onΩ, (1.3)

where f : ℝ → ℝ is C1, non-negative, nondreceasing and superlinear at infinity. Then there exists a constant λ* > 0 such that for each λ ∈ [0, λ*) there exists a minimal classical solution uλ(x), and for λ > λ* there exists no solution, even in the weak sense, see [9, Proposition 3.3.1]. The family (uλ)0<λ<λ* is monotone increasing with respect to the parameter λ, and the pointwise limit uλ* := limλλ*uλ is a weak stable solution to (1.3). The solution uλ* is called the extremal solution. When f(u) is the exponential nonlinearity, it is proved that if dimension n ≤ 9, the extremal solution is always smooth, see [9, Theorem 4.2.1]. For more general nonlinearity f(u), very recently, Cabré et al. [2] showed that the extremal solutions are regular when n ≤ 9. The restriction on the dimension n < 10 is sharp in the sense that there are singular weak stable solutions for n ≥ 10, for example u(x) = log2(n − 2) − 2log∣x∣ provides a weak stable solution which is not regular.

As there are singular stable weak solutions in dimension n ≥ 10, a natural question is to understand the partial regularity of stable solutions for n ≥ 10. In the classical case with exponential nonlinearity, the partial regularity result has been studied by Wang [21, 22], and he proved that the Hausdorff dimension of the singular set for weak stable solutions is at most n − 10. In dimension n = 3, Da Lio [5] showed that the dimension of singular set for stationary solution can be at most 1. We refer the readers to [7, 10] for the results on the extremal solutions of Liouville system and [4] on the stable solutions of biharmonic Liouville equation.

Let us also mention that the partial regularity of solutions for Lane-Emden equation, that is, the nonlinearity is given by f(u) = up, has been studied in various settings, e.g., estimating the singular set of stable solutions and stationary solutions, see e.g. [6, 9, 16, 17, 20].

In the nonlocal case, Duong - Nguyen [8] studied stable solutions and proved that Eq. (1.1) has no regular stable solution for n < 10s. Later, the authors of this paper gave the following optimal condition on n, s

n2s,or n>2s and Γ(n2)Γ(1+s)Γ(n2s2)>Γ2(n+2s4)Γ2(n2s4), (1.4)

for which Eq. (1.1) has no stable solutions in the whole space ℝn, see [14]. In addition, the authors also showed that weak stable solutions are smooth, whenever n < 10s. While for the case of extremal solutions, Ros-Oton - Serra [18] proved that the extremal solutions are regular for n < 10s. In a subsequent paper, under certain symmetry assumptions on the domain, Ros-Oton [19] proved regularity of extremal solutions (for the case of exponential nonlinearity) up to the optimal dimension, that is, n and s satisfy (1.4). His arguments are based on the fact that, due to the symmetry assumptions on the domain, the extremal solution can have at most one singular point. For the recent developments on the regularity of extremal solutions for nonlocal systems we refer to [12] and the references therein.

Definition 1.1

A point x0Ω is said to be a singular point for a solution u to (1.1) if u is not bounded in any small neighborhood of x0. The singular set 𝓢 is the collection of all singular points.

It follows from the above definition that the singular set 𝓢 is closed in Ω. Moreover, by standard regularity theory one gets that u is regular in Ω ∖ 𝓢.

Our main result is the following:

Theorem 1.1

Let u be a stable weak solution of (1.1). Then the Hausdorff dimension of the singular set 𝓢 is at most n − 10s.

The dimension estimate n − 10s is optimal in the limit s ↑ 1 as there are singular weak stable solutions for s = 1. However, due to the regularity results of Ros-Oton [19] for extremal solutions, one would expect that the Hausdorff dimension of the singular set would be at most nn*(s), where n*(s) > 10s is implicitly defined by the second condition in (1.4) with equality. This remains as an open question.

To prove Theorem 1.1 we follow the approach of Wang [21, 22] for the classical case. More precisely, Wang considered the energy

F(u,x0,r):=r2nBr(x0)eudx. (1.5)

Then he showed that there exists ε0 > 0 (independent of u, x0, r) such that if 𝓕(u, x0, r) ≤ ε0 then u is regular in a small neighborhood of x0. This, and the fact that eu is in Llocp for every p < 5, thanks to Farina’s estimate [11], imply that the Hausdorff dimension of the singular set is at most n − 10.

Contrary to the above energy (1.5), in our case we shall consider the following energy involving interior and boundary quantities

E(u,x0,r):=r2snBr(x0)eudx+r4sn2Brn+1(x0)R+n+1t12seu¯dxdt,

where u is the Caffarelli-Silvestre extension of u in R+n+1 , i.e.,

u¯(X)=RnP(X,y)u(y)dy,X=(x,t)Rn×(0,+),

where

P(X,y)=dn,st2s|(xy,t)|n+2s,

and dn,s > 0 is a normalizing constant such that nP(X,y)dy = 1, see [1]. The function u satisfies

div(t12su¯)=0inR+n+1,limt0t12stu¯=κs(Δ)su=κseu,inΩ,

where κs=Γ(1s)22s1Γ(s). As in the classical case, the Farina type estimate for the nonlocal case also imply that if u is a stable weak solution then eu Llocp for every p < 5, see Lemma 2.1. Due to this integrability restrictions we have the dimension estimate n − 10s in Theorem 1.1. Let us also emphasize here that the stability condition will be used only to obtain the Farina type estimate in Lemma 2.1 and to get uniform bounds in the space Ls(ℝn) for a family of rescaled solutions in Lemma 2.3.

It is important to note that each term in the energy 𝓔(u, x0, r) controls the other one in a suitable way. More precisely, due to the stability hypothesis, the second term controls the L2 norm of eu, see (2.2), whereas, by Jensen’s inequality, the second term is controlled by the first one, see Lemma 3.1. This interplay turned out to be very crucial in proving energy decay estimate (see Proposition 3.4 and Lemma 3.5 for precise statements), that is, if 𝓔(u, x0, r) ≤ ε0 for some sufficiently small ε0 > 0 then there exists θ ∈ (0, 1) such that 𝓔(u, x0,θr) ≤ 12 𝓔(u, x0, r).

We remark that the energy estimate does not seem to work if we only consider one of the two terms in 𝓔(u, x0, r). For instance, on one hand, if we only consider the first term (as in the local case), then we lack a Harnack type inequality for non-negative fractional sub-harmonic functions. However, in the fractional case, we do have a Harnack type inequality involving the extension function, see Lemma 3.3. This suggests to consider the second term in the definition of the energy. On the other hand, if we only consider the second term in the energy, then the L1 norm of v (as defined in ℝef{def-barv}) is of the order E due to the fact that there is a sacrifice in the power of ε when we use Hölder inequality, which is not good enough (compare (3.5) and (3.7)) to prove the energy decay estimate in Proposition 3.4.

The article is organized as follows: In section 2 we list some preliminary results, including the conclusions presented in our previous work [14] and some known results that would be used in the current article. In section 3, we give the proof of Theorem 1.1.

Notations

  1. represent points in R+n+1 = ℝn × [0, ∞) and ℝn = R+n+1 .

  2. the ball centered at x with radius r in ℝn, Br := Br(0).

  3. the ball centered at x with radius r in Rn+1,Brn+1:=Brn+1(0).

  4. the intersection of Brn+1 (x) and R+n+1 , i.e., Brn+1(x)R+n+1,Dr:=Dr(0).

  5. represents the non-negative part of u, i.e., u+ = max(u, 0).

  6. a generic positive constant which may change from line to line.

2 Preliminary results

In this section we present several results that will be used in next section. First, we extend the stability condition in the fractional setting. Notice that u is well-defined as uLs(ℝn). Moreover, t12s2u¯Lloc2(Ω×[0,)) whenever us(Ω). We recall from [14] that the stability condition (1.2) can be generalized to the extended function u. Precisely, if u is stable in Ω then

R+n+1t12s|Φ|2dxdtκsRneuϕ2dx, (2.1)

for every ΦCc(R+n+1¯) satisfying ϕ():=Φ(,0)Cc(Ω). The following Farina type estimate has been proven in [14, Lemma 3.4]:

Lemma 2.1

([14]). Let us(Ω) be a weak stable solution to (1.1). Given a function Φ be of the form Φ(x, t) = ϕ(x)η(t) for some ϕ Cc (Ω) and η = 1 in a small neighborhood of the origin, for every α ∈ (0, 2) we have

(2α)κsRne(1+2α)uϕ2dx2R+n+1t12se2αu¯|Φ|2dxdt12R+n+1e2αu¯[t12sΦ2]dxdt. (2.2)

Though the following regularity result on Morrey’s space is well-known, we give a proof for convenience. We recall that a function f is in the Morrey’s space Mp(Ω) if fL1(Ω), and it satisfies

ΩBr(x0)|f|dxCrn(11p)for every Br(x0)Rn.

The norm ∥fMp(Ω) is defined to be the infimum of constants C > 0 for which the above inequality holds.

Lemma 2.2

Let fMn2sδ(B3) for some δ > 0. We set

Rsf(x):=B11|xy|n2s|f(y)|dy.

Then we have

RsfL(B1)C(n,s,δ)fMn2sδ(B3).

Proof

We set

F(r)=Br(x)|f(y)|dy.

Then

Rsf(x)B21|y|n2s|f(xy)|dy=02ρ2snF(ρ)dρ,xB1, (2.3)

where ρ = ∣y∣. We can derive from (2.3) and integration by parts that

|Rsf|02ρ2snF(ρ)dρ=22snF(2)+(n2s)02ρ2sn1F(ρ)dρfMn2sδ(B3)22sn2n+δ2s+(n2s)fMn2sδ(B2)02ρδ1dρCfMn2sδ(B3).

Thus we finish the proof.□

For any x0B1, we set

uλ(x):=u(x0+λx)+2slogλ. (2.4)

The following lemma is crucial for the proof of Lemma 3.5.

Lemma 2.3

Let u be a stable solution to (1.1) with Ω = B1. Let uλ be defined as in (2.4) for somex0∣ < 1 and 0<λ<(1|x0|)1+n2s. Then

u+λLs(Rn)C(1+u+Ls(Rn)),

for some C > 0 independent of u.

Proof

It is easy to see that uλ is a stable solution to (1.1) on BR with R:=1λ(1|x0|). Hence, by (2.1)

BρeuλdxCρn2sfor 0<ρR2.

This would imply that

BR/2u+λ(x)1+|x|n+2sdxBR/2euλ(x)1+|x|n+2sdxC.

As λ < 1 we get

u+λ(x)<u+(x0+λx).

Therefore, changing the variable x0 + λ xy we obtain

BR/2cu+λ(x)1+|x|n+2sdxλn{|y|2}{|x0y|12Rλ}+|y|>2u+(y)1+|x0y|λn+2sdyCλnRn+2s|y|2u+(y)dy+Cλ2s|y|>2u+(y)|y|n+2sdyCu+Ls(Rn).

We conclude the lemma.□

3 Proof of Theorem 1.1

We start with the following refinement version of [14, Lemma 3.3]:

Lemma 3.1

Let eαuL1(B1). Then t1−2seαu Lloc1 (B1 × [0, ∞)). Moreover,

  1. there exists δ = δ(n, s) > 0 and C = C(n, s,∥u+Ls(ℝn)) > 0 such that

    t12seαu¯L1(D1/2)CeαuL1(B1)+eαuL1(B1)δ,
  2. for every δ0 > 0 small there exists r0 = r0(n, s,δ0) > 0 small such that

    0r0B1/2t12seαu¯dxdtCeαuL1(B1)+eαuL1(B1)1δ0.

Proof

For X = (x, t) ∈ D1/2 we have

u¯(x,t)Cu+Ls(Rn)+B1u(y)P(X,y)dy=C+B1g(x,t)u(y)P(X,y)g(x,t)dy,

where

1>g(x,t):=B1P(X,y)dyδ, (3.1)

for some positive constant δ depending on n and s only. The last inequality easily follows from

limt0B1P(X,y)dy=1.

Therefore, by Jensen’s inequality

B1/2eαu¯(x,t)dxCB1/2B1eαg(x,t)u(y)P(X,y)dydxCB1maxeαu(y),eαδu(y)B1/2P(X,y)dxdyCB1eδαu(y)+B1eαu(y)dyCeαuL1(B1)+eαuL1(B1)δ,

where the last inequality follows from Hölder inequality. Integrating the above inequality with respect to t on the interval [0,12] we obtain i).

To to prove ii), we notice that for a given δ0 > 0 small we can choose r0 > 0 sufficiently small such that (3.1) holds with δ = 1−δ0 for every xB1/2 and 0 < tr0. Then ii) follows in a similar way.□

Up to a translation and dilation of the domain Ω, we can simply assume that B1Ω. For fixed 0 < r < 1 we decompose

u¯=v¯+w¯,

where

v¯(x,t):=C(n,s)Br1(|xy|2+t2)n2s2eu(y)dy,xRn, (3.2)

where C(n, s) > 0 is a dimensional constant such that

limt0t12stv¯=κseuon Br.

Then w satisfies

div(t12sw¯)=0inR+n+1,limt0t12stw¯=0inBr. (3.3)

Notice that w is continuous up to the boundary Br.

Now we prove some elementary properties of the functions v and w.

Lemma 3.2

Setting v := v(x, 0) we have

t12s2v¯L2(Dr)+vL2(Br)CeuL1(Br)γeuL2(Br)1γ,0<r1,

for some γ ∈ (0, 1) and C > 0 independent of u.

Proof

The function v can be written as a convolution, and in fact,

vχBr(ΓχB2r)(euχBr),Γ(x):=C(n,s)|x|n2s,

where χA denotes the characteristic function of the set A. On the one hand, by Young’s inequality, we obtain

vLp(Br)ΓLq(B2r)euL2(Br), (3.4)

where p, q verify the following conditions

1+1p=1q+12,1<q<nn2s.

On the other hand, it is easy to see that

vL1(Br)ΓL1(B2r)euL1(Br). (3.5)

Therefore, together with the interpolation inequality

vL2(Br)vL1(Br)γvLp(Br)1γ,

with γ, p satisfying

12=γ+1γp,0<γ<1,

we obtain

vL2(Br)CeuL1(Br)γeuL2(Br)1γ,r(0,1].

Here we choose p slightly bigger than 2 in (3.4), and use the fact that the Lq and L1 norms of Γ are uniformly bounded in Br if r stays bounded. The lemma follows as v(x, t) ≤ v(x).□

Lemma 3.3

Setting w = w(x0, 0) we have for every 0 < ρ < R := (r − ∣x0∣)

csew(x0)ρ2sn2Dρ(x0)t12sew¯dxdtR2sn2DR(x0)t12seu¯dxdt,x0Br,

where

cs=D1t12sdxdt.

Proof

We prove the lemma only for x0 = 0. From (3.3) we have that

div(t12sew¯)=t12sew¯|w¯|20in R+n+1,limt0t12stew¯=0in Br.

Therefore, for 0 < ρ < r

0Dρdiv(t12sew¯(x,t))dxdt=DρBρt12sνew¯(x,t)dσ(X)=ρn+12sρD1B1t12sew¯(ρx,ρt)dσ.

This implies that ρ2sn−1 DρBρ t1−2sewdσ is monotone increasing with respect to ρ. As a consequence, we have that ρ2sn−2Dρ t1−2sewdxdt is increasing in ρ. Hence, using that w < u and w is continuous up to the boundary Br, where the former conclusion follows from the fact that v > 0, we get

csew¯(0)ρ2sn2Dρt12sew¯dxdtρ2sn2Dρt12seu¯dxdt.

It completes the proof.□

We now prove the following energy decay estimate for 𝓔(u, x0, r). For simplicity, we write 𝓔(u, x0, r) by 𝓔(x0, r), and consider x0 = 0 and r = 1 in the following proposition.

Proposition 3.4

Let u be a stable solution to (1.1) with Ω = B1 for some uLs(ℝn). Then there exists ε0 ∈ (0, 1) and θ ∈ (0, 1) depending only on n, s andu+Ls(ℝn) such that if

ε:=E(0,1)=B1eudx+D1t12seu¯dxdtε0

then

E(0,θ)12E(0,1).

Proof

It follows from (2.2) that

B1/2e2udxCD1t12seu¯dxdtCε. (3.6)

Then writing u = v+w, where v is given by (3.2) with r = 12 , we get from Lemma 3.2 that

vL2(B1/2)+t12s2v¯L2(D1/2)Cε1+γ2. (3.7)

We shall give estimation on 𝓔(0, r) for suitable r. Using Lemma 3.1 one can find r1 = r1(n, s,γ) ∈ (0, 12 ) such that for every 0 < rr1

Drt12se2u¯(x,t)dxdtCε1γ2,

where C > 0 depends on n, s and ∥u+Ls(ℝn). Together with (3.6), (3.7) and Hölder inequality

Brveudx+Drt12sv¯eu¯dxdtCε1+γ4.

This in turn implies that

r4sn2Dr{v¯1}t12seu¯dxdtCr4sn2ε1+γ4.

Moreover, by Lemma 3.3

r4sn2Dr{v¯1}t12seu¯dxdtCr4sn2Drt12sew¯dxdtCr2sε.

Combining the above two estimates

r4sn2Drt12seu¯dxdtC(r2sε+r4sn2ε1+γ4).

In a similar way, by Lemma 3.3 we can also obtain,

r2snBreudxCr2snBr{v1}ewdx+r2snBr{v1}veudxCr2snrnD1t12seu¯dxdt+Cr2snε1+γ4C(r2sε+r2snε1+γ4).

Thus, for 0 < rr1,

E(0,r)C(r2sε+r4sn2ε1+γ4),

for some C = C(n, s,∥u+Ls(ℝn)) > 0, where we used s < 1 and r1 12 .

Finally, we first choose θ > 0 small enough such that Cθ2s=14, and then choose ε0 > 0 small such that Cθ4sn2ε0γ4=14. Then for εε0 we obtain

E(0,θ)12ε=12E(0,1).

Hence, we finish the proof.□

Though the proof of the following lemma is quite standard, thanks to Proposition 3.4 and Lemma 2.3, for completeness we give a sketch of the proof.

Lemma 3.5

Let uLs(ℝn) be a stable solution to (1.1) with Ω = B1. Then there exists ε̂0 > 0 depending only on n, s andu+Ls(ℝn) such that if

0<E(u,0,1)ε^0,

then u is continuous in B1/6.

Proof

For x0B12 and 0<λλ0:=22n2s we set

uλ(x)=u(x0+λx)+2slogλ.

Then by Lemma 2.3 we see that

u+λLs(Rn)C1for every x0B12,0<λλ0,

for some C1 > 0 independent of x0B12 and 0 < λλ0. Therefore, by Proposition 3.4, we can find ε0 > 0 and θ ∈ (0, 1) (depending only on n, s and C1) such that

E(uλ,0,1)ε0E(uλ,0,θ)12E(uλ,0,1). (3.8)

It follows from the definition of the energy 𝓔 that

E(uλ,0,1)=E(u,x0,λ),E(u,x0,λ0)C(λ0)E(u,0,1).

Consequently, if we choose 0<ε^0<ε0C(λ0), then from (3.8) we get

E(u,x0,λ0θ)=E(uλ0,0,θ)12E(uλ0,0,1)=12E(u,x0,λ0)12ε0.

By an iteration argument one obtains

E(u,x0,λ0θk)12kE(u,x0,λ0)ε02k,k=1,2,3,.

In particular, setting α:=log2logθ>0 we get

E(u,x0,r)CrαE(u,0,1)for every x0B12and0<r14,

which gives

Br(x)eu(y)dyCrn2s+αfor every xB12and0<r14. (3.9)

Now we decompose u = u1+u2, with

u1(x)=c(n,s)B1/31|xy|n2seu(y)dy,xRn,

where c(n, s) is chosen such that

c(n,s)(Δ)s1|xy|n2s=δ(xy).

By (3.9) and Lemma 2.2 we conclude that u1 is bounded in B1/3. While u2 satisfies (−Δ)s u2 = 0 in B1/3, and it implies that u2 is smooth in B1/6. As a consequence, we get that u is continuous in B1/6.□

We recall that if u is stable in Ω, then eu Llocp (Ω) for every p ∈ [1, 5) by Lemma 2.1. Consequently, the small energy regularity results can be stated as follows:

Lemma 3.6

For every 1 ≤ p < 5 there exists εp > 0 depending only on n, s anduLs(ℝn) such that if

B1epudxεp,

then u is continuous on B1/12.

Proof

By Hölder inequality we get that

B1eudxCεp1p.

Hence, by Lemma 3.1

D1/2t12seu¯dxdtCεpδp,

for some δ > 0. This shows that

E(0,12)Cεpδp.

Then by Lemma 3.5 we get that u is continuous in B1/12 provided Cεpδ/p is sufficiently small.□

Proof

Proof of Theorem 1.1. The problem (1.1) is invariant under the rescaling

uλ(x):=u(x0+λx)+2slogλ.

Therefore, if

r2psnBr(x0)epudxεp,

for some p ∈ [1, 5), then u is continuous in Br/12(x0), thanks to Lemma 3.6. Thus, if x0 ∈ 𝓢 (𝓢 is the singular set) we see that for every r > 0 small

r2psnBr(x0)epudx>εp.

Hence, by the well-known Besicovitch covering theorem we have that the Hausdorff dimension of 𝓢 is at most n − 2ps with p ∈ [1,5), see for instance [15, Lemma 1.3.5, Lemma 2.1.1] or [13, Proposition 9.21]. Hence, we conclude that the Hausdorff dimension of 𝓢 is at most n − 10s and it completes the proof.□

Acknowledgement

The first author is supported by the SNSF Grant No. P400P2-183866. The second author is partially supported by NSFC No.11801550 and NSFC No.11871470. We are grateful to the anonymous referees for many insightful remarks and valuable suggestions.

  1. Conflicts of interest: The authors declare that they have no conflict of interest.

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Received: 2020-11-24
Accepted: 2021-03-09
Published Online: 2021-05-22

© 2021 Ali Hyder and Wen Yang, published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

Articles in the same Issue

  1. Editorial
  2. Editorial to Volume 10 of ANA
  3. Regular Articles
  4. Convergence Results for Elliptic Variational-Hemivariational Inequalities
  5. Weak and stationary solutions to a Cahn–Hilliard–Brinkman model with singular potentials and source terms
  6. Single peaked traveling wave solutions to a generalized μ-Novikov Equation
  7. Constant sign and nodal solutions for superlinear (p, q)–equations with indefinite potential and a concave boundary term
  8. On isolated singularities of Kirchhoff equations
  9. On the existence of periodic oscillations for pendulum-type equations
  10. Multiplicity of concentrating solutions for a class of magnetic Schrödinger-Poisson type equation
  11. Nehari-type ground state solutions for a Choquard equation with doubly critical exponents
  12. Gradient estimate of a variable power for nonlinear elliptic equations with Orlicz growth
  13. The structure of 𝓐-free measures revisited
  14. Solvability of an infinite system of integral equations on the real half-axis
  15. Positive Solutions for Resonant (p, q)-equations with convection
  16. Concentration behavior of semiclassical solutions for Hamiltonian elliptic system
  17. Global existence and finite time blowup for a nonlocal semilinear pseudo-parabolic equation
  18. On variational nonlinear equations with monotone operators
  19. Existence results for nonlinear degenerate elliptic equations with lower order terms
  20. Blow-up criteria and instability of normalized standing waves for the fractional Schrödinger-Choquard equation
  21. Ground states and multiple solutions for Hamiltonian elliptic system with gradient term
  22. Positivity of solutions to the Cauchy problem for linear and semilinear biharmonic heat equations
  23. Convex solutions of Monge-Ampère equations and systems: Existence, uniqueness and asymptotic behavior
  24. Multiple solutions for critical Choquard-Kirchhoff type equations
  25. Regularity for sub-elliptic systems with VMO-coefficients in the Heisenberg group: the sub-quadratic structure case
  26. Inducing strong convergence of trajectories in dynamical systems associated to monotone inclusions with composite structure
  27. A posteriori analysis of the spectral element discretization of a non linear heat equation
  28. Liouville property of fractional Lane-Emden equation in general unbounded domain
  29. Large data existence theory for three-dimensional unsteady flows of rate-type viscoelastic fluids with stress diffusion
  30. On some classes of generalized Schrödinger equations
  31. Variational formulations of steady rotational equatorial waves
  32. On a class of critical elliptic systems in ℝ4
  33. Exponential stability of the nonlinear Schrödinger equation with locally distributed damping on compact Riemannian manifold
  34. On a degenerate hyperbolic problem for the 3-D steady full Euler equations with axial-symmetry
  35. Existence, multiplicity and nonexistence results for Kirchhoff type equations
  36. Combined effects of Choquard and singular nonlinearities in fractional Kirchhoff problems
  37. Convergence analysis for double phase obstacle problems with multivalued convection term
  38. Multiple solutions for weighted Kirchhoff equations involving critical Hardy-Sobolev exponent
  39. Boundary value problems associated with singular strongly nonlinear equations with functional terms
  40. Global solvability in a three-dimensional Keller-Segel-Stokes system involving arbitrary superlinear logistic degradation
  41. Multiplicity and concentration behaviour of solutions for a fractional Choquard equation with critical growth
  42. Concentration results for a magnetic Schrödinger-Poisson system with critical growth
  43. Periodic solutions for a differential inclusion problem involving the p(t)-Laplacian
  44. The concentration-compactness principles for Ws,p(·,·)(ℝN) and application
  45. Regularity for commutators of the local multilinear fractional maximal operators
  46. An improvement to the John-Nirenberg inequality for functions in critical Sobolev spaces
  47. Local versus nonlocal elliptic equations: short-long range field interactions
  48. Analysis of a diffusive host-pathogen model with standard incidence and distinct dispersal rates
  49. Blowing-up solutions of the time-fractional dispersive equations
  50. Fixed point of some Markov operator of Frobenius-Perron type generated by a random family of point-transformations in ℝd
  51. Non-stationary Navier–Stokes equations in 2D power cusp domain
  52. Non-stationary Navier–Stokes equations in 2D power cusp domain
  53. Nontrivial solutions to the p-harmonic equation with nonlinearity asymptotic to |t|p–2t at infinity
  54. Iterative methods for monotone nonexpansive mappings in uniformly convex spaces
  55. Optimality of Serrin type extension criteria to the Navier-Stokes equations
  56. Fractional Hardy-Sobolev equations with nonhomogeneous terms
  57. New class of sixth-order nonhomogeneous p(x)-Kirchhoff problems with sign-changing weight functions
  58. On the set of positive solutions for resonant Robin (p, q)-equations
  59. Solving Composite Fixed Point Problems with Block Updates
  60. Lions-type theorem of the p-Laplacian and applications
  61. Half-space Gaussian symmetrization: applications to semilinear elliptic problems
  62. Positive radial symmetric solutions for a class of elliptic problems with critical exponent and -1 growth
  63. Global well-posedness of the full compressible Hall-MHD equations
  64. Σ-Shaped Bifurcation Curves
  65. On the critical behavior for inhomogeneous wave inequalities with Hardy potential in an exterior domain
  66. On singular quasilinear elliptic equations with data measures
  67. On the sub–diffusion fractional initial value problem with time variable order
  68. Partial regularity of stable solutions to the fractional Geľfand-Liouville equation
  69. Ground state solutions for a class of fractional Schrodinger-Poisson system with critical growth and vanishing potentials
  70. Initial boundary value problems for the three-dimensional compressible elastic Navier-Stokes-Poisson equations
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