Home Groundstate for the Schrödinger-Poisson-Slater equation involving the Coulomb-Sobolev critical exponent
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Groundstate for the Schrödinger-Poisson-Slater equation involving the Coulomb-Sobolev critical exponent

  • Chunyu Lei , Jun Lei EMAIL logo and Hongmin Suo
Published/Copyright: March 22, 2023

Abstract

In this article, we study the existence of ground state solutions for the Schrödinger-Poisson-Slater type equation with the Coulomb-Sobolev critical growth:

Δ u + 1 4 π x u 2 u = u u + μ u p 2 u , in R 3 ,

where μ > 0 and 3 < p < 6 . With the help of the Nehari-Pohozaev method, we obtain a ground-state solution for the above equation by employing compactness arguments.

MSC 2010: 35J20; 35J61; 35B33

1 Introduction and main results

In this article, we study the following Schrödinger-Poisson-Slater equation:

(1.1) Δ u + 1 4 π x u 2 u = u u + μ u p 2 u , in R 3 ,

where μ > 0 and 3 < p < 6 . In equation (1.1), x 1 u 2 is known as the repulsive Coulomb potential, which makes the usual Sobolev space H 1 ( R 3 ) not to be a good framework for equation (1.1). In [14], the author introduced the following Coulomb-Sobolev space:

E v D 1 , 2 ( R 3 ) ; R 3 R 3 v ( x ) 2 v ( y ) 2 4 π x y d x d y < ,

the norm : E R for the space E is

v = R 3 v 2 d x + [ L ( v ) ] 1 2 1 2 ,

where

L ( v ) R 3 R 3 v ( x ) 2 v ( y ) 2 4 π x y d x d y

is the so-called Coulomb energy of the wave and has been studied, see, for instance, [13]. In [24], it was shown that E is a uniformly convex separable Banach space, and the embedding E L q ( R 3 ) is not compact for q [ 3 , 6 ] . Here, we call 6 and 3 the Sobolev critical exponent and the Coulomb Sobolev critical exponent, respectively.

Here, we recall the following Schrödinger-Poisson-Slater equation:

(1.2) Δ u + 1 4 π x u 2 u = μ u r 2 u , in R 3 .

From a physical standpoint, equation (1.2) appeared in various physical frameworks; the motivation in the study of problem (1.2) originates from the Slater approximation of the exchange term in the Hartree-Fock model, which we refer to in [26]. In this setting, r = 5 3 is an important exponent in (1.2). Of course, other exponents have been employed in various approximations, see [24] for more details related to these models and their variants.

In addition, Li et al. [12] considered the existence of infinitely many solutions for the fractional Kirchhoff-Schrödinger-Poisson system with critical or subcritical growth. We point out that the novelties of this article lie in the appearance of the possibly degenerate Kirchhoff function. Moreover, the nonlinear term is weak assumptions. Yao et al. [30] proved normalized solutions for the Choquard equations with 2 < r 2 N / N 2 by using new arguments, and they were also given some qualitative properties of the solutions with prescribed mass and of the associated Lagrange multipliers λ . In addition, the literature is the first to consider the normalized solutions for a nonlocal problem involving double critical exponents. By constraint variational method and quantitative deformation lemma, Ji et al. [10] studied the existence of the least energy sign-changing solutions for the Schrödinger-Poisson system. Moreover, there is no constraint for λ > 0 , and they showed that the energy of a sign-changing solution is strictly larger than twice of the ground state energy and studied the convergence property of the least energy sign-changing solutions as λ 0 . In [20,29], by the new variational approach, the authors proved the existence of solutions of the planar Schrödinger-Poisson systems. From the mathematical point of view, there is a series of analytical results on the Schrödinger-Poisson systems in the literature, see [1,8,9,11,15,18,19,2123,25,31] and so on. Especially, Ianni and Ruiz [9] focused on equation (1.2), and with the aid of the monotonicity trick, a positive ground state solution was obtained when 3 < r < 6 . Following the ideas in [27], Lei and Lei [11] considered the higher-dimensional version of the Schrödinger-Poisson-Slater equation (1.2). For example, we considered the following equation:

Δ u + ( x α N u 2 ) u = μ u r 2 u , in R N .

Under the assumption 2 ( α + 4 ) / ( 2 + α ) < r < 2 N / ( N 2 ) when N < 4 + α , or 2 N / ( N 2 ) < r < 2 ( α + 4 ) / ( 2 + α ) when N > 4 + α , they obtained a ground state solution of the Nehari-Pohozaev type.

The present article has been motivated by a seminal article by Liu et al. [19] who studied the existence of ground state solutions for the following Schrödinger-Poisson-Slater-type equation with critical growth:

(1.3) Δ u + u 2 1 4 π x u = μ u r 2 u + u 4 u , in R 3 ,

where μ > 0 . By combining a new perturbation method and the mountain pass theorem, when r ( 3 , 6 ) , they obtained the existence of positive ground state solutions. In particular, when r = 3 , they established the existence of radial solutions in radial space E rad by the constrained minimization method provided μ suitably large.

Based on the work of [19], we are also concerned with the existence of ground state solutions (which are not limited to be radial) of equation (1.1). To the best of our knowledge, we have not found any references involving the Coulomb-Sobolev critical growth.

Before stating our main result, it is well known that every solution to equation (1.1) is a critical point of the energy functional J : E R , which is given as follows:

J ( u ) = 1 2 R 3 u 2 d x + 1 4 L ( u ) 1 3 R 3 u 3 d x μ p R 3 u p d x .

Now, we introduce the following functionals and sets, respectively:

T ( u ) = R 3 u 2 d x ,

(1.4) = { u E \ { 0 } : I ( u ) = 0 } ,

where

I ( u ) = 3 2 1 2 R 3 u 2 d x + 1 4 L ( u ) 1 3 R 3 u 3 d x 2 p 3 2 p μ R 3 u p d x .

Now, our main results in this article can be stated as follows.

Theorem 1.1

Assume μ = 0 . Then, equation (1.1) has no nontrivial solutions.

Theorem 1.2

Let 3 < p < 6 and μ > 0 . Then, equation (1.1) has a positive ground state solution on .

Remark 1.1

  1. In [19], when r = 3 , in order to overcome the loss of compactness of the Sobolev embedding E L 3 ( R 3 ) , the authors worked on the radial space E rad to obtain a compactness result, namely, the embedding E rad L 3 ( R 3 ) is compact. In other words, r = 3 is no longer the Coulomb-Sobolev critical exponent in the radial space E rad .

    We recover Theorem 1.2 in [19] using the Nehari-Pohozaev manifold method instead of using a perturbation method and the mountain pass theorem. However, the most important and interesting point of our approach is that it handles a Schrödinger-Poisson-Slater equation with the Coulomb-Sobolev critical growth.

  2. The lack of compactness. A general tool that could be useful to overcome the lack of compactness is the Schwartz rearrangement map u u . The following properties are well known (see [11]):

    R 3 u 2 d x R 3 u 2 d x ;

    R 3 R 3 u ( x ) 2 u ( y ) 2 x y d x d y R 3 R 3 u ( x ) 2 u ( y ) 2 x y d x d y ;

    R 3 u p d x = R 3 u p d x , 1 p < + .

    For (1.1), however, if we use the Schwartz rearrangement technique, it is impossible to overcome the lack of compactness due to the nonlocal term.

  3. For (1.1), it is difficult to prove the boundedness of (PS) sequence of J . In the present article, we have opted to use the Nehari-Pohozaev manifold to avoid the difficulty.

2 Proof of Theorem 1.1

Assume that u is a nontrivial solution of (1.1), one has

T ( u ) + L ( u ) R 3 u 3 d x = 0 , 1 2 T ( u ) + 5 4 L ( u ) R 3 u 3 d x = 0 .

We deduce

(2.1) T ( u ) = 1 2 L ( u ) , L ( u ) = 2 3 R 3 u 3 d x , T ( u ) = 1 3 R 3 u 3 d x .

Noting that the function

ϕ u = R 3 u 2 4 π x y d x

solves the following equation:

(2.2) Δ ϕ u = u 2 , in R 3 .

Moreover,

R 3 ϕ 2 d x = R 3 ϕ u u 2 d x = R 3 R 3 u 2 ( x ) u 2 ( y ) 4 π x y d x d y = L ( u ) .

By (2.2), the Hölder inequality, and (2.1), there holds

R 3 u 3 d x R 3 ϕ u 2 d x 1 2 R 3 u 2 d x 1 2 = 2 3 R 3 u 3 d x 1 2 1 3 R 3 u 3 d x 1 2 = 2 3 R 3 u 3 d x ,

which implies that

1 2 3 ,

we arrive a contradiction, and hence u 0 . The proof is complete.

3 Proof of Theorem 1.2

First, we establish the following result.

Lemma 3.1

The functional J is unbounded from below.

Proof

Let u E and u t = t u ( t b x ) , b = 1 / 2 , t > 0 . By the standard scaling, we have

R 3 u t 2 d x = t 3 2 R 3 u 2 d x , L ( u t ) = t 3 2 L ( u ) ,

and

R 3 u t 3 d x = t 3 2 R 3 u 3 d x , R 3 u t p d x = t p 3 2 R 3 u p d x .

Hence,

J ( u t ) = 1 2 R 3 u t 2 d x + 1 4 L ( u t ) 1 3 R 3 u t 3 d x μ p R 3 u t p d x = t 3 2 1 2 R 3 u 2 d x + 1 4 L ( u ) 1 3 R 3 u 3 d x μ t p 3 2 p R 3 u p d x .

Based on p > 3 , we see that J ( u t ) as t + .□

By calculations, we can easily obtain the following lemma.

Lemma 3.2

Let

f ( t ) = t 3 2 1 2 R 3 u 2 d x + 1 4 L ( u ) 1 3 R 3 u 3 d x μ t p 3 2 p R 3 u p d x

for t 0 and u . Then, f has a unique critical point, corresponding to its maximum.

Proof

For u , we have

1 2 R 3 u 2 d x + 1 4 L ( u ) 1 3 R 3 u 3 d x = 2 p 3 3 p μ R 3 u p d x > 0 .

Therefore,

f ( t ) 0 + as t 0 + , and f ( t ) as t + .

Noting f ( 0 ) = 0 , we see that f has a unique positive critical point. The proof of Lemma 3.2 is completed.□

Assume that u is a critical point of J . Write u t = t u ( t b x ) with b = 1 / 2 and t > 0 . Clearly, φ ( t ) J ( u t ) is positive for small t and tends to as t + . By Lemma 3.2, φ has a unique critical point that corresponds to its maximum. Since u is a critical point of J , the maximum of φ ( t ) should be achieved at t = 1 and φ ( 1 ) = 0 . Therefore, define the manifold as (1.4). Obviously, . Indeed, for given any v 0 , Lemma 3.2 shows that there exists t > 0 such that u t v . Moreover, the curve Γ = { u t } intersects the manifold and J Γ attains its maximum along Γ at the point u . If u is a mountain pass-type solution of problem (1.1), it is natural to look for the minima of J on . In addition, for any nontrivial critical point u of J , it is standard to prove the following Pohozaev identity:

P ( u ) = 1 2 R 3 u 2 d x + 5 4 L ( u ) R 3 u 3 d x 3 μ p R 3 u p d x = 0 .

It is clear that I ( u ) = J ( u ) , u b P ( u ) with b = 1 2 . Therefore, is called the Nehari-Pohozaev manifold here. If u is a nontrivial solution of (1.1), then u .

Moreover, we have the following result.

Lemma 3.3

is a C 1 -manifold and every critical point of J in is a critical point of J.

Proof

We proceed in three steps.

Step 1. We claim inf J > 0 and 0 .

Once u , then

1 2 R 3 u 2 d x + 1 4 L ( u ) 1 3 R 3 u 3 d x = 2 p 3 3 p μ R 3 u p d x ,

and so

(3.1) J ( u ) = 1 2 R 3 u 2 d x + 1 4 L ( u ) 1 3 R 3 u 3 d x 1 p μ R 3 u p d x = 2 p 3 3 p μ R 3 u p d x μ p R 3 u p d x = 2 p 6 3 p μ R 3 u p d x > 0 .

Moreover, we see that 0 .

Step 2. We claim that is a C 1 -manifold.

By the implicit function theorem, it only needs I ( u ) 0 for any u . We prove it by argument of contradiction. In particular, we suppose that I ( u ) = 0 for some u . Thus, in a weak sense, there holds

(3.2) Δ u + 1 4 π x u 2 u = u u + 2 p 3 3 μ u p 2 u .

Multiplying (3.2) by u and integrating, we have

(3.3) R 3 u 2 d x + L ( u ) R 3 u 3 d x 2 p 3 3 μ R 3 u p d x = 0 .

The Pohozaev identity corresponding to equation (3.2) is

(3.4) 1 2 R 3 u 2 d x + 5 4 L ( u ) R 3 u 3 d x 2 p 3 p μ R 3 u p d x = 0 .

It follows from p I ( u ) = 0 that

p R 3 u 2 d x + p 4 L ( u ) p R 3 u 3 d x 3 p 6 2 μ R 3 u p d x = 0 .

Multiplying (3.4) by 1 3 and applying I ( u ) = 0 , we obtain

R 3 u 2 d x = 1 2 L ( u ) .

Multiplying (3.3) by 1 p and using I ( u ) = 0 again, we have

p 2 2 R 3 u 2 d x + p 4 4 L ( u ) = p 3 3 R 3 u 3 d x .

Applying the relation R 3 u 2 d x = 1 2 L ( u ) to the above equation, we obtain

L ( u ) = 2 3 R 3 u 3 d x .

Finally, taking L ( u ) = 2 3 R 3 u 3 d x and R 3 u 2 d x = 1 2 L ( u ) into (3.4), we obtain

R 3 u p d x = 0 .

This a contradiction. Thus, is a C 1 -manifold.

Step 3. We claim that every critical point of J on is a critical point of J in E .

Assume that u is a critical point of J on , there exists a Lagrange multiplier λ such that J ( u ) = λ I ( u ) . It can be written, in a weak sense, as follows:

Δ u + 1 4 π x u 2 u u u μ u p 2 u = λ Δ u + 1 4 π x u 2 u u u 2 p 3 3 μ u p 2 u .

That is,

(3.5) ( 1 λ ) Δ u + ( 1 λ ) 1 4 π x u 2 u = ( 1 λ ) u u + 1 2 p 3 3 λ μ u p 2 u .

We see that λ 1 , it remains now to prove that λ = 0 . Denote

= R 3 u 3 d x , C = μ R 3 u p d x .

We can establish the following equations:

(3.6) 1 2 T ( u ) + 1 4 L ( u ) 1 3 2 p 3 3 p C = 0 , T ( u ) + L ( u ) 1 1 λ 1 2 p 3 3 λ C = 0 , 1 2 T ( u ) + 5 4 L ( u ) 3 p 1 1 λ 1 2 p 3 3 λ C = 0 ,

where the second equation follows by multiplying (3.5) by u and integrating, and the third equality is the Pohozaev identity corresponding to equation (3.5).

It follows from the first and the third equations in (3.6) that

(3.7) L ( u ) = 2 3 + 3 p 1 1 λ 1 2 p 3 3 λ 2 p 3 3 p C .

Applying the the first and the second equations in (3.6), we have

1 4 L ( u ) = 1 2 ( 1 λ ) 1 2 p 3 3 λ 2 p 3 3 p C + 1 6 .

In particular,

(3.8) L ( u ) = 2 1 λ 1 2 p 3 3 λ 8 p 12 3 p C + 2 3 .

It follows from (3.7) and (3.8) that

3 p 1 1 λ 1 2 p 3 3 λ 2 p 3 3 p C = 2 1 λ 1 2 p 3 3 λ 8 p 12 3 p C .

That is,

(3.9) 3 p 1 1 λ 1 2 p 3 3 λ 2 p 3 3 p 2 1 λ 1 2 p 3 3 λ + 8 p 12 3 p C = 0 .

Noting that

3 p 1 1 λ 1 2 p 3 3 λ 2 p 3 3 p 2 1 λ 1 2 p 3 3 λ + 8 p 12 3 p = 1 1 λ 1 2 p 3 3 λ 3 p 2 + 2 p 3 p = 2 p 3 p 1 1 1 λ 1 2 p 3 3 λ = 2 p 3 p 1 3 ( 2 p 3 ) λ 3 ( 1 λ ) = 2 p 3 p ( 2 p 6 ) λ 3 ( 1 λ ) ,

we obtain

2 p 3 p ( 2 p 6 ) λ 3 ( 1 λ ) C = 0 .

Since p > 3 , we have

λ 0 .

Therefore, we obtain J ( u ) = 0 , i.e., u is a critical point of J . The proof is complete.□

Let us define : E R as follows:

( u ) R 3 u 2 d x + R 3 R 3 u ( x ) 2 u ( y ) 2 4 π x y d x d y .

Lemma 3.4

Let { u n } be a minimizing sequence of J. Then, { u n } is a bounded ( PS ) inf J sequence for J. Then, up to a subsequence { u n } , still denoted itself, a number k N { 0 } , and a finite sequence

( v 0 , v 1 , , v k ) E , v i 0 , f o r i > 0

of critical points problem (1.1) and k sequences { ξ n 1 } , , { ξ n k } R 3 , such that as n + ,

(3.10) u n v 0 i = 1 k v ( ξ n i ) 0 ,

ξ n i + , ξ n i ξ n j + , i j ,

J ( v 0 ) + i = 1 k J ( v i ) = inf J .

Proof

Step 1. Let { u n } be a minimizing sequence of J in , i.e., J ( u n ) inf J as n . We claim that { u n } is a (PS) sequence of J . In fact, by the Ekeland variational principle (see Theorem 8.5 in [28]), there exists { λ n } R such that

J ( u n ) inf J ,

J ( u n ) λ n I ( u n ) 0 as n .

Then,

Δ u n + 1 4 π x u n 2 u n u n u n μ u n p 2 u n = λ n Δ u n + 1 4 π x u n 2 u n u n u n 2 p 3 3 μ u n p 2 u n + o ( 1 ) .

In particular,

( 1 λ n ) Δ u n + ( 1 λ n ) 1 4 π x u n 2 u n = ( 1 λ n ) u n u n + 1 2 p 3 3 λ n μ u n p 2 u n + o ( 1 ) .

We also have ( λ n 0 )

1 2 T ( u n ) + 1 4 L ( u n ) 1 3 R 3 u n 3 d x 2 p 3 3 p μ R 3 u n p d x = 0 , T ( u n ) + L ( u n ) R 3 u n 3 d x 1 1 λ n 1 2 p 3 3 λ n μ R 3 u n p d x = o ( 1 ) , 1 2 T ( u n ) + 5 4 L ( u n ) R 3 u n 3 d x 3 p 1 1 λ n 1 2 p 3 3 λ n μ R 3 u n p d x = o ( 1 ) .

It is similar to the Step 3 in Lemma 3.3 that

lim n λ n = 0 .

Thus, we obtain that { u n } is (PS) sequence of J . In particular,

(3.11) J ( u n ) inf J , J ( u n ) 0 as n .

It follows from J ( u n ) 0 and I ( u n ) = 0 that

(3.12) P ( u n ) 0 as n .

By (3.1), there holds

(3.13) 2 p 6 3 p μ R 3 u n p d x inf J ( n ) ,

and so we obtain that R 3 u n p d x is bounded.

Step 2. We claim that { u n } is bounded in E .

In fact, by P ( u n ) = o ( 1 ) , u , and (3.13), we deduce that when n ,

(3.14) 1 2 u n 2 2 + 1 4 L ( u n ) 1 3 u n 3 3 = 2 p 3 3 p μ R 3 u n p d x = 2 p 3 2 p 6 inf J + o ( 1 ) , 1 2 u n 2 2 + 5 4 L ( u n ) u n 3 3 = 3 p μ R 3 u n p d x = 9 2 p 6 inf J + o ( 1 ) .

Now, for each u E \ { 0 } , define

γ ( t ) t 1 u ( t 1 2 x ) , t > 0 .

By a simple computation,

(3.15) γ ( t ) 2 = t 3 2 R 3 u 2 d x + t 3 4 [ L ( u ) ] 1 2 .

It follows from (3.15) that lim t 0 + γ ( t ) 2 = + and lim t + γ ( t ) 2 = 0 . Therefore, for any u E \ { 0 } , there exists a unique T u > 0 such that

(3.16) γ ( T u ) ( x ) 2 = T u 1 u ( T u 1 2 x ) 2 = 1 .

This and (3.15) lead to

(3.17) T u + as u + .

Next, we prove that u n is bounded by contradiction argument. We suppose that there exists a subsequence of u n denoted by itself such that u n + as n . Then, by (3.16) and (3.17), there exists T n T u n such that

(3.18) v n = 1 and T n + ( n ) .

Here, { v n } E is defined by v n ( x ) T n 1 u n ( T n 1 2 x ) . By (3.14),

T n 3 2 1 2 v n 2 2 + 1 4 L ( v n ) 1 3 v n 3 3 = 2 p 3 2 p 6 inf J + o ( 1 ) , T n 3 2 1 2 v n 2 2 + 5 4 L ( v n ) v n 3 3 = 9 2 p 6 inf J + o ( 1 ) .

Once T n + , then we infer

1 2 v n 2 2 + 1 4 L ( v n ) 1 3 v n 3 3 = o ( 1 ) , 1 2 v n 2 2 + 5 4 L ( v n ) v n 3 3 = o ( 1 ) .

This yields

v n 2 2 = 1 2 L ( v n ) + o ( 1 ) , L ( v n ) = 2 3 v n 3 3 + o ( 1 ) .

Now, by (3.18), we obtain

1 = v n 2 = v n 2 2 + [ L ( v n ) ] 1 2 = 1 2 L ( v n ) + [ L ( v n ) ] 1 2 + o ( 1 ) .

We solve the above equation as follows:

L ( v n ) = 4 2 3 + o ( 1 ) .

Hence,

v n 2 2 = 2 3 + o ( 1 ) , R 3 v n 3 d x = 3 ( 2 3 ) + o ( 1 ) .

Since { v n } is bounded in E , we may assume that v n v weakly in E . In view of J ( u n ) 0 as n , we have

R 3 u n φ d x + R 3 R 3 u n ( x ) 2 u n ( y ) φ ( y ) 4 π x y d x d y R 3 u n u n φ d x μ R 3 u n p 2 u n φ d x = o ( 1 )

for φ C 0 ( R 3 ) . That is,

R 3 v n φ d x + R 3 R 3 v n ( x ) 2 v n ( y ) φ ( y ) 4 π x y d x d y R 3 v n v n φ d x T n p 3 μ R 3 v n p 2 v n φ d x = o ( 1 ) .

Then, we deduce that

R 3 v φ d x + R 3 R 3 v ( x ) 2 v ( y ) φ ( y ) 4 π x y d x d y R 3 v v φ d x lim n T n p 3 μ R 3 v n p 2 v n φ d x = 0

for φ C 0 ( R 3 ) . If

lim n T n p 3 R 3 v n p 2 v n φ d x = 0 ,

then one has

R 3 v φ d x + R 3 R 3 v ( x ) 2 v ( y ) φ ( y ) 4 π x y d x d y R 3 v v φ d x = 0

for φ C 0 ( R 3 ) . This implies that v is a nontrivial solution of the equation

(3.19) Δ v + 1 4 π x v 2 v = v v .

This is impossible because problem (3.19) has no nontrivial solutions by Theorem 1.1. Therefore, taking the test function φ = v n , we have

lim n T n p 3 R 3 v n p d x 0 .

This yields

0 lim n T n p 3 R 3 v n p d x = lim n T n 3 2 T n p 3 2 R 3 v n p d x = lim n T n 3 2 R 3 u n p d x = lim n T n 3 2 3 p 2 p 6 inf J ,

which implies that

lim n T n 3 2 0 ,

resulting in a contradiction, and hence { u n } is bounded in E .

Step 3. Since { u n } is bounded in E , we can find a subsequence of u n denoted by itself such that u n v 0 weakly in E when n . It follows from J ( u n ) 0 ( n ) that

R 3 v 0 φ d x + R 3 R 3 v 0 ( x ) 2 v 0 ( y ) φ ( y ) 4 π x y d x d y R 3 v 0 v 0 φ d x μ R 3 v 0 p 2 v 0 φ d x = 0

for φ C 0 ( R 3 ) . Then, v 0 is a critical point for J . Thereby,

J ( v 0 ) , v 0 = 0 and P ( v 0 ) = 0 .

Denote u n 1 u n v 0 , then u n 1 0 in E when n . By the Brézis-Lieb lemma (cf. [5]), we have

(3.20) R 3 u n 1 3 d x = R 3 u n 3 d x R 3 v 0 3 d x + o ( 1 ) ,

(3.21) R 3 u n 1 2 d x = R 3 u n 2 d x R 3 v 0 2 d x + o ( 1 ) ,

(3.22) R 3 u n 1 p d x = R 3 u n p d x R 3 v 0 p d x + o ( 1 ) ,

and

(3.23) L ( u n 1 ) = L ( u n ) L ( v 0 ) + o ( 1 ) ,

when n . Hence, from the above information, we obtain

(3.24) J ( u n 1 ) = J ( u n ) J ( v 0 ) + o ( 1 ) inf J J ( v 0 ) , J ( u n 1 ) 0 ,

and

P ( u n ) = 1 2 R 3 u n 2 d x + 5 4 L ( u n ) R 3 u n 3 d x 3 p μ R 3 u n p d x = 1 2 R 3 u n 1 2 d x + 5 4 L ( u n 1 ) R 3 u n 1 3 d x 3 p μ R 3 u n 1 p d x + 1 2 R 3 v 0 2 d x + 5 4 L ( v 0 ) R 3 v 0 3 d x 3 p μ R 3 v 0 p d x + o ( 1 ) = 1 2 R 3 u n 1 2 d x + 5 4 L ( u n 1 ) R 3 u n 1 3 d x 3 p μ R 3 u n 1 p d x + o ( 1 ) ,

when n . In view of (3.12), we have

(3.25) P ( u n 1 ) = 1 2 R 3 u n 1 2 d x + 5 4 L ( u n 1 ) R 3 u n 1 3 d x 3 p μ R 3 u n 1 p d x = o ( 1 ) .

If

u n 1 0 in E ( n ) ,

we are done. Indeed, by the Coulomb-Sobolev inequality:

R 3 u n 1 q d x C u n 1 2 5 q 12 3 [ L ( u n 1 ) ] 6 q 6

for 3 q 6 . Thus,

R 3 u n 1 3 d x 0 , R 3 u n 1 p d x 0 , as n .

By (3.1), we have

J ( v 0 ) = inf J > 0 , [ u n ] [ v 0 ] ( n ) .

Observe that in this case v 0 0 and v 0 .

If

u n 1 0 in E ( n ) .

Recall (3.11) and that v 0 is a solution, then, when n ,

J ( u n ) , u n = [ u n ] R 3 u n 3 d x μ R 3 u n p d x 0 = [ v 0 ] R 3 v 0 3 d x μ R 3 v 0 p d x .

Next, the argument is divided into two cases as follows:

C a s e 1 . lim n R 3 u n p d x = R 3 v 0 p d x ; C a s e 2 . lim n R 3 u n p d x R 3 v 0 p d x .

In Case 1, when n , it follows from (3.25) that

(3.26) 1 2 R 3 u n 1 2 d x + 5 4 L ( u n 1 ) R 3 u n 1 3 d x = o ( 1 ) .

In addition, by (3.11) and (3.20)–(3.23), we see that as n ,

R 3 u n 1 2 d x + R 3 v 0 2 d x + L ( u n 1 ) + L ( v 0 ) R 3 u n 1 3 d x R 3 v 0 3 d x μ R 3 v 0 p d x = o ( 1 ) .

The equality combined with J ( v 0 ) , v 0 = 0 gives that

(3.27) R 3 u n 1 2 d x + L ( u n 1 ) R 3 u n 1 3 d x = o ( 1 ) ( n ) .

It follows from (3.26) and (3.27) that

L ( u n 1 ) = 2 R 3 u n 1 2 d x + o ( 1 ) ( n ) .

Hence, we obtain

inf u = J ( u n ) + o ( 1 ) = 1 2 R 3 u n 2 d x + 1 4 L ( u n ) 1 3 R 3 u n 3 d x 1 p μ R 3 u n p d x + o ( 1 ) = 1 2 R 3 u n 1 2 d x + 1 2 R 3 v 0 2 d x + 1 4 L ( u n 1 ) + 1 4 L ( v 0 ) 1 3 R 3 u n 1 3 d x 1 3 R 3 v 0 3 d x μ p R n v 0 p d x + o ( 1 ) = 1 2 R 3 u n 1 2 d x + 1 4 L ( u n 1 ) 1 3 R 3 u n 1 3 d x + J ( v 0 ) + o ( 1 ) = 1 6 R 3 u n 1 2 d x 1 12 L ( u n 1 ) + J ( v 0 ) + o ( 1 ) = J ( v 0 ) + o ( 1 ) .

When n , we have

J ( v 0 ) = inf J > 0 .

This implies that

v 0 0 .

Since v 0 is a solution of (1.1), thus

J ( v 0 ) , v 0 = 0 and P ( v 0 ) = 0 .

This combining v 0 0 implies

v 0 .

Moreover, by the strong maximum principle, v 0 is a positive ground state solution of (1.1), and Theorem 1.2 is proved.

In Case 2, since E L l o c p ( R 3 ) ( 3 < p < 6 ) is compact, there exist δ 1 > 0 and { ξ n 1 } R 3 such that

(3.28) B 1 u n 1 ( x + ξ n 1 ) p d x δ 1 > 0 .

This and (3.28) lead to ξ n 1 + ( n ) .

Step 4. Define v n 1 u n 1 ( + ξ n 1 ) . Obviously, it is a bounded (PS) sequence at level inf u J J ( v 0 ) (recall (3.24)). Up to a subsequence, we may assume that

u n 1 v 1 in E ( n ) ,

and v 1 is a solution of (1.1), By (3.28) we also have that v 1 0 and

v 1 .

Define

u n 2 u n 1 v 1 ( ξ n 1 ) .

Then,

u n 2 0 in E ( n ) .

Arguing as in Step 3 and taking into account (3.24), we obtain that when n ,

(3.29) R 3 u n 2 p d x = R 3 u n p d x R 3 v 0 p d x R 3 v 1 p d x + o ( 1 ) , J ( u n 2 ) = J ( u n 1 ) J ( v 1 ) = J ( u n ) J ( v 0 ) J ( v 1 ) + o ( 1 ) , J ( u n 2 ) 0 , P ( u n 2 ) 0 .

If u n 2 0 ( n ) in E , we are done. In fact, when n , u n 1 v 1 ( ξ n 1 ) in E . As in Step 3, we can obtain that v 1 is a nontrivial solution of (1.1) with J ( v 1 ) = inf u J > 0 .

If u n 2 0 ( n ) in E . Similarly, if u n 2 0 ( n ) in L p ( R 3 ) , we are done and J ( v 1 ) = inf u J > 0 . If u n 2 0 ( n ) in L p ( R 3 ) , we may assume the existence of { ξ n 2 } R 3 such that

B 1 u n 2 ( x + ξ n 2 ) p d x δ 2 for some δ 2 > 0 .

Since

u n 2 0 and u n 2 ( + ξ n 1 ) 0 in E ( n ) ,

we deduce that when n ,

ξ n 2 + , ξ n 2 ξ n 1 + .

Therefore, up to a subsequence, we may assume that

u n 2 ( + ξ n 2 ) v 2 ( ) in E ( n ) ,

and v 2 is a nontrivial solution of (1.1). We now define

u n 3 u n 2 v 2 ( ξ n 2 ) .

Iterating the above procedure, we construct sequences { u n j } j and { ξ n j } j in the following way:

u n j + 1 u n j v j ( ξ n j ) ,

(3.30) R 3 u n j p d x = R 3 u n p d x i = 0 j 1 R 3 v i p d x + o ( 1 ) ( n ) ,

(3.31) J ( u n j ) = J ( u n ) i = 0 j 1 J ( v i ) + o ( 1 ) ( n ) ,

J ( v i ) = 0 , for i 0 .

Since v i for i 1 , this combining (3.13) yields

μ R 3 v i p d x 3 p 2 p 6 inf J .

Noting that

μ R 3 u n p d x = 3 p 2 p 6 inf J + o ( 1 )

is bounded, which implies that the iteration in (3.30) must stop by at most finite steps. In particular, there exists some positive integer k such that u n k 0 ( n ) in E . The proof is finished.□

Proof of Theorem 1.2

By (3.31), we obtain

(3.32) i = 0 k J ( v i ) = inf J .

Since v i ( i = 1 , , k ) is a solution of equation (1.1), we have J ( v i ) = 0 and P ( v i ) = 0 for i = 0 , 1 , , k .

For v 0 , it follows from J ( v 0 ) = 0 and P ( v 0 ) = 0 that

I ( v 0 ) = J ( v 0 ) , v 0 1 2 P ( v 0 ) = 0 .

Therefore, there holds

J ( v 0 ) = 1 2 R 3 v 0 2 d x + 1 4 L ( v 0 ) 1 3 R 3 v 0 3 d x μ p R 3 v 0 p d x 1 2 R 3 v 0 2 d x + 1 4 L ( v 0 ) 1 3 R 3 v 0 3 d x 2 p 3 3 p μ R 3 v 0 p d x = 2 p 3 3 p μ R 3 v 0 p d x 1 p μ R 3 v 0 p d x = 2 p 6 3 p μ R 3 v 0 p d x 0 .

For i 1 , since v i , thus J ( v i ) inf J for i = 1 , , k . Applying J ( v i ) inf J to (3.32), we obtain that there are two possibilities: either v 0 0 and k = 0 , or v 0 = 0 and k = 1 . In the first case, u n ( + ξ n 1 ) v 0 ( ) ( n ) in E (by (3.10)) and v 0 is a ground state solution of (1.1) (by Step 3 in Lemma 3.3) with J ( v 0 ) = inf J (by (3.32)). In the latter case, u n ( + ξ n 1 ) v 1 ( ) in E as n (by (3.10)) and v 1 is a positive ground state solution of equation (1.1) with J ( v 1 ) = inf J (by (3.32)). The proof is ended.□

Acknowledgements

The authors thank the anonymous referees for their valuable comments and nice suggestions to improve the results.

  1. Funding information: Chunyu Lei is supported by the Science and Technology Foundation of Guizhou Province (No. ZK[2022]199); the Natural Science Research Project of Department of Education of Guizhou Province (Grant No. QJJ2022015, QJJ2022047).

  2. Author contributions: The authors contributed equally in this article.

  3. Conflict of interest: The authors declare that there is no conflict of interest in this article.

  4. Data availability statement: No data were used to support this study.

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Received: 2022-09-18
Revised: 2023-01-01
Accepted: 2023-01-24
Published Online: 2023-03-22

© 2023 the author(s), published by De Gruyter

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

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