Abstract
The present paper investigates the following inhomogeneous generalized Hartree equation , where the wave function is , with . In addition, the exponent gives an unbounded inhomogeneous term and denotes the Riesz-potential for certain . In this work, our aim is to establish the local existence of solutions in some radial Sobolev spaces, as well as the global existence for small data and the decay of energy sub-critical defocusing global solutions. Our results complement the recent work (Sharp threshold of global well-posedness versus finite time blow-up for a class of inhomogeneous Choquard equations, J. Math. Phys. 60 (2019), 081514). The main challenge in this work is to overcome the singularity of the unbounded inhomogeneous term for certain .
MSC:
35Q55
1. Introduction
The Schrödinger equation was formulated in 1926 by the Austrian physicist Erwin Schrödinger [1], and it was one of the real bases for the development of quantum mechanics. It is a prototypical dispersive nonlinear partial differential equation that has been since derived in many areas of physics. The nonlinear Schrödinger equation appears as a model in hydrodynamics, nonlinear optics, quantum condensates, heat pulses in solids and various other nonlinear instability phenomena; see, for instance, Newell [2] and Scott–Chu–McLaughlin [3]. Moreover, it was suggested that stable high power propagation can be achieved in a plasma by sending a preliminary laser beam that creates a channel with a reduced electron density and, thus, reduces the nonlinearity inside the channel; see Gill [4] and Liu-Tripathi [5]. In this case, the beam propagation can be modeled by the inhomogeneous nonlinear Schrödinger equation.
In this note, we consider the Cauchy problem for an inhomogeneous Schrödinger equation
Here and hereafter, , and the wave function u is a complex valued function of the variable . The real number refers to the focusing or defocusing regime. Moreover gives the unbounded inhomogeneous term . Finally, and the Riesz-potential is
The significance of Equation (1) is to model many important physical phenomena. For example, it describes the mean-field limit of large systems of non-relativistic Bosonic molecules [6,7]. It models also the propagation of plasma electromagnetic waves [8]. The fourth space dimensional case, the said Schrödinger–Poisson equation, arises in the theory of semi-conductor and quantum mechanics [9].
The Schrödinger problem with an inhomogeneous local source term, , for was treated in [10]. Indeed, some well-posedness issues were investigated using the potential-well method. Later on, this problem was revisited by the author [11] in the fractional case. Indeed, the existence of global and non-global energy solutions were discussed using the ground state threshold.
The inhomogeneous generalized Hartree problem (1) was first considered by Alharbi, G. M. et al. [12], where the authors only considered the case . Indeed, the global existence versus the blow-up of solutions was obtained. In addition, the scattering under the ground state threshold with spherically symmetric data was proven in [13], and it was extended to the non-radial regime in [14,15].
This paper complements the recent work by Alharbi, G. M. et al. [12], in which the authors only considered Equation (1) for . The method used in [12] consists of the division of the integrals on the unit ball of and its complementary fails for because for any . Instead, we skillfully use the Strauss estimate for any function . Consequently, we are able to prove local well-posedness in the energy spaces with a radial setting and the global existence for small data. Furthermore, the energy defocusing energy global solution decays for a long time in some Lebesgue spaces. However, in this work, the question regarding the existence of standing waves, which describes the threshold of global existence versus the finite time blow-up of energy solutions, is not discussed. This is considered in a paper in progress.
This paper is organized as follows. We introduce our main results and other components associated with our work in Section 2. In Section 3, we prove the local well-posedness of (1). In Section 4, the global well-posedness for the small data of (1) in the energy space is obtained. In Section 5, the decay of defocusing global solutions is established. Finally, a Morawetz estimate and some Gagliardo–Nirenberg inequalities are proven in the Appendix A.
We mention that C (respectively, ) denotes a constant (respectively, a constant depending on T) that may vary from line to line, and if A and B are non-negative real numbers, means that .
Here and hereafter, we denote, for short, some Lebesgue and Sobolev spaces endowed with the classical norms
Finally, is the maximal existence time of an eventual solution to (1). If , we denote by a real number close to x such that . The critical Sobolev embedding index is denoted by .
2. Background Material
This section contains the main results and some useful estimates.
2.1. Preliminary
The Hartree Equation (1) employs the scaling invariance
The following critical exponent,
is the only one keeping invariant the Sobolev norm
Therefore, the Schrödinger problem (1) is said to be critical if ; it is sub-critical if and super-critical if . Let us define the real numbers related to Equation (1).
If is a smooth function, we define the variance potential and the Morawetz action as follows
In a standard way, the repeated indices are summed, and subscripts denote the partial derivatives. Finally, let us take the differential operator
The next sub-section contains the contribution of this note.
2.2. Main Results
The first result deals with the local well-posedness of the problem (1) in the radial energy space.
Theorem 1.
Let , , and . Assume that satisfies and or and . Then, there exists and to be a unique local solution to (1). Moreover,
- 1.
- the solution satisfies the following conservation laws
- 2.
- , for all admissible pairs in the meaning of Definition 1;
- 3.
- if , then u is global.
In view of the results stated in the above theorem, some comments are in order.
- Using Proposition 4 via the Hardy–Littlewood–Sobolev inequality, we obtainwhen , and the energy is well-defined for . Therefore, it seems that the previous theorem also holds;
- the assumption is possible, at least for low space dimensions;
- the presence of the derivative term gives the dichotomy and .
The second result deals with the local well-posedness of the Hartree problem (1) in the Sobolev space .
Theorem 2.
Let , , , and . Assume that and or , and . Then, there exists and to be a unique maximal solution to (1). Moreover,
- 1.
- the solution satisfies the mass conservation law;
- 2.
- , for all admissible pairs ;
- 3.
- if , then u is global.
Remark 1.
The difference between the local existence in and for is due to the use of some different Strauss inequalities stated in Proposition 3.
The third result deals with the global well-posedness of the Schrödinger problem (1) for small data.
Theorem 3.
Take the assumptions of Theorem 1 and , such that if . Then, there exists such that if , then, the solution to (1) is global and scatters in . Moreover, it satisfies
Let us state some comments about the above theorem.
- The Strichartz norms and are defined in Definition 1;
- in the defocusing regime, any local solution is global; in the focusing regime, a local solution may be non-global, but for small data, this scenario cannot happen.
- the scattering means that there exists , such that
The fourth result deals with the decay of global defocusing solutions.
Theorem 4.
Let , and . Take the conditions of Theorem 1. Then, the global solution to (1), denoted by , satisfies for any ,
Let us give some remarks about the above result.
- the assumptions and allow the use of the Morawetz estimate (2);
- the scattering of energy global solutions is stronger than the decay but not available in the mass-sub-critical regime;
- in a future work, the authors will investigate the energy scattering of global solutions to the Hartree problem (1).
The next variance identity is established in Appendix A.
Proposition 1.
Take and the assumptions of Theorem 1. Let a local solution to (1) be denoted as . Then, holds on are represented as
Moreover, if , it follows that
Remark 2.
The previous Morawetz estimate is an essential tool in the proof of the decay of defocusing energy global solutions to (1).
Finally, the next Gagliardo–Nirenberg type inequalities adapted to the Schrödinger Equation (1) are established in the Appendix A.
Proposition 2.
Let , and .
- 1.
- If , there exists , such that for any ,
- 2.
- if , there exists , such that for any ,
2.3. Tools
This sub-section collects some useful estimates. First, we recall a Hardy–Littlewood–Sobolev estimate [11,16].
Lemma 1.
Let and .
- 1.
- If , then
- 2.
- if , then
The next Gagliardo–Nirenberg inequality [17] is useful.
Lemma 2.
Let , and . Then
The radial assumption enables us to use the next Strauss inequalities [18].
Proposition 3.
Let and . Then
- 1.
- there is , such that for any
- 2.
- there is , such that for any ,
The following inhomogeneous Gagliardo–Nirenberg-type inequalities are essential in this work [10,11].
Proposition 4.
Let , and . Then
- 1.
- if , there exists , such that for all
- 2.
- if , there exists , such that for any ,
Let us recall a useful fractional chain rule [19].
Lemma 3.
Let , and , such that . Thus,
The Strichartz estimate [20] is an essential tool to estimate an eventual solution to (1) in Sobolev spaces.
Definition 1.
Take and . A pair of real numbers is s-admissible if
Take the set , s-admissible }, and the Strichartz norms
Proposition 5.
Let , , and a time slab . Then
- 1.
- ;
- 2.
3. Well-Posedness
In what follows, we establish the energy local well-posedness of the non-linear Hartree problem (1).
3.1. -Theory
The proof proceeds with a standard fixed point Picard theorem. Take and and the distance
on the space
Define
Using Strichartz estimates, we obtain the following for and :
Since and , we take two positive real numbers , satisfying . Using Hardy–Littlewood–Sobolev and Hölder estimates, we obtain
Using the Gagliardo–Nirenberg inequality in Proposition 4, we write
under the conditions and
This gives the condition
Moreover, the equality , via the admissibility condition , gives
This is satisfied if
These conditions are verified because
Thus,
Let us estimate the term . Since and , we take positive real numbers satisfying . Due to the Hardy–Littlewood–Sobolev and Hölder estimates, it follows that
Using the Gagliardo–Nirenberg inequality in Proposition 4, we write
under the conditions and
This gives the condition
Moreover, the equality , via the admissibility condition , gives
This is satisfied as above because
Thus, there exists such that
Moreover,
Now, let us estimate the term . Compute
Taking account of the Strichartz estimates and arguing as previously, we obtain
For the above, we discuss two regimes.
- 1.
- First case: .Take the real numbers andand such that . Therefore, according to the Hölder estimate, we obtainunder the conditionThe equality , given via the condition , isThis is satisfied ifThis is satisfied because . ThenMoreover, with the Hölder estimate, for andwe haveunder the conditionMoreover, the assumption givesThis is satisfied ifThe integral on can be estimated similarly. So, for , we obtain , and is stable by the function .
- 2.
- Second case: .By calculus in the estimation of with , rather than , we obtain the requested estimation under the assumptionsThis givesThis is satisfied becauseNow, we need to estimate the termunder the conditionsThis is satisfied ifThis is the same above condition.Therefore, for , we obtain . Thus, is stable by the function .
Then, for some , the function is the contract , and its fix point is a solution to the Hartree problem (1). The uniqueness is a consequence of the previous calculus with a classical translation argument.
3.2. -Theory
Take, for and , the closed ball
Repeating the above argument with the same notions of the distance d and the function , we have for
Here, using the Gagliardo–Nirenberg inequality in Proposition 2, we write
under the conditions and
This gives the condition
Moreover, the equality , via the admissibility condition , gives
This is satisfied if
The above condition is verified because
Moreover,
which is the above condition. Thus,
Now, let us estimate the term . Due to the fractional chain rule in Lemma 3, we have
Due to the Strichartz estimates and arguing as previously, we obtain
For the above, we have two cases:
- 1.
- first case .Take the real numbers andand , such that . Then, using the Hölder estimate and Proposition 2, we haveunder the conditionSince , the admissibility condition is satisfied ifThis gives the conditionThis is satisfied becauseThen,Now, we estimate the termunder the conditionsThe admissibility condition givesThe following condition, which is the same above, yieldsThe term for can be controlled similarly. Therefore, for , we obtain . Thus, is stable under .
- 2.
- Second case .Arguing as previously, via the estimateswe haveHere, we assume the conditions andThis is satisfied ifThis is satisfied ifThe following term needs to be estimated; therefore, we haveunder the conditionsThis is satisfied ifThis is the same above condition. Therefore, we do not need any supplementary condition.Therefore, for , we obtain . Thus, is stable under .
So, for some , is the contract and its fix point resolves the Hartree Equation (1). The uniqueness follows by the previous calculus and a classical translation argument.
4. Global Existence
In what follows, Theorem 3 is established with a Picard fixed point argument. Take the complete space
under the distance
Let, as previously, the integral function be
Take, for , the real numbers
This gives
Taking account of the Strichartz and Hardy–Littlewood–Sobolev estimates, it follows that
under the conditions
Taking , the above condition, via , is satisfied if
Equivalently
Now, taking
we obtain
and with the Strichartz estimate, we obtain
Moreover, arguing as previously, we obtain
Let us discuss two regimes.
- 1.
- Case one: . Taking and , we obtainunder the condition , which is satisfied ifCoupling this condition withwe obtain . Thus, the above estimate holds ifThe estimate of the term follows similarly, and also, we haveTherefore,
- 2.
- . Taking into account the calculus of the first case , we obtainunder the conditionsTaking , the above condition is satisfied ifSimilarly, we obtainTherefore,
5. Decay of Defocusing Global Solutions
In this section, we take the defocusing regime and prove Theorem 4. Let and a weakly convergent sequence
- Claim.
For all there exists , such that
Let us define the functions and , as well as, and
Similarly, let us define and
Taking and , we have
Due to Hölder’s inequality and Sobolev embedding, for and ,
Moreover, for , we have
under the condition
The admissibility condition gives
Equivalently,
Moreover, for , we have
under the condition
The admissibility condition gives
Equivalently,
Now, according to the Rellich theorem, for the sub-sequence, when ,
Furthermore, with the conservation laws and the properties of ,
Taking account of the Strichartz estimate, it follows that
This established the claim.
Now, it is sufficient to prove the decay for via an interpolation argument. Let us write a Gagliardo–Nirenberg-type estimate
Here, is the square centered at x with edge length a. With the contradiction, assume that there exists and , such that
According to (7) and the previous inequality, there exists and a real number (denoted also by satisfying
Following the lines in [21], we obtain
Therefore, from Propositions 1 and 3, for , we obtain
Due to the radial assumption and (8), is bounded. Then,
This contradiction achieves the proof.
6. Conclusions
Theorems 1 and 2 establish the local well-posedness, in the Sobolev space for , of the inhomogeneous Hartree problem (1) in the sub-critical regime . Moreover, according to Theorem 3, the global well-posedness holds in the energy space for small data. Furthermore, in the defocusing regime, Theorem 4 proves that the mass-sub-critical solutions vanish for a long time in some Lebesgue spaces. The main ingredients used are Strichartz-type estimates in Proposition 5, coupled with some radial Strauss inequalities in Proposition 3. In a future work, the authors will try to improve the present paper in three directions. The first one is to remove the radial assumption. The second one is to treat the critical regime: . The third one is to investigate the scattering versus finite time blow-up dichotomy of focusing solutions in the spirit of [22].
Author Contributions
Conceptualization, T.S.; Formal analysis, S.A. and R.G. All authors wrote and revised the paper. All authors have read and agreed to the published version of the manuscript.
Funding
This research received no external funding.
Institutional Review Board Statement
Not applicable.
Data Availability Statement
No data-sets were generated or analyzed during the current study.
Acknowledgments
Researchers would like to thank the Deanship of Scientific Research, Qassim University for funding the publication of this project.
Conflicts of Interest
The authors declare no conflict of interest.
Appendix A
Appendix A.1. Proof of Proposition 1
In this sub-section, we take . Let be a local solution to (1). Recall the variance and source term
We compute
Due to the equality,
we have
Moreover,
This implies that
Thus,
Now, let us write
Therefore, we obtain
Finally,
This completes the proof of the first part. Moreover, taking the choice , we obtain
and
Now, because a is convex, we have
Thus,
Now, due to the identity
we write
Thus, for , it follows that
This finishes the proof.
Appendix A.2. Proof of Proposition 2
In what follows, we prove two Gagliardo–Nirenberg-type estimates related to the Hartree problem (1).
Appendix A.2.1. H1-Gagliardo–Nirenberg Inequality
Using the radial assumption via the Strauss inequality in Proposition 3, we have
Thus,
Therefore, with the Hardy–Littlewood–Sobolev inequality, we have
Thus, with Lemma 2, via the fact that , it follows that
Appendix A.2.2. Fractional Gagliardo–Nirenberg Inequality
In this sub-section, we prove a fractional Gagliardo–Nirenberg estimate related to the Hartree problem (1). Using the radial assumption via the Strauss inequality (3), we have
Thus,
Therefore, with the Hardy–Littlewood–Sobolev estimate, we have
Thus, by Lemma 2 and the assumption , we obtain
This ends the proof.
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