In this paper, we prove the global well-posedness of the 2-D magnetic Prandtl model in the mixed Prandtl/Hartmann regime when the initial data is a small perturbation of the Hartmann layer in Sobolev space.
In this paper, we consider a 2-D magnetic Prandtl model in :
where denotes the velocity field and b denotes the tangential magnetic field. This model is derived from the incompressible MHD system under a transverse magnetic field on the boundary for the parameters of the system in the mixed Prandtl/Hartmann regime. See [8] for a formal derivation.
Thanks to the boundary conditions and , we get
Substituting it into (1.1), we obtain a Prandtl type equation with an extra damping term :
The damping term in the system is induced by the combined effect of the magnetic diffusivity and transversal magnetic field. This term should have no effect on the local behavior of the solution. So, it seems not difficult to generalize the following well-posedness results for the classical Prandtl system to the system (1.2).
Local well-posedness in Sobolev space for monotonic data [1,3,13,14];
Local well-posedness for analytic data [12,16,20];
Ill-posedness in Sobolev space and local well-posedness in Gevrey class for a class of non-monotonic data [4,6,7,11];
Global existence of weak solution for monotonic data [18].
Moreover, E and Engquist proved that the analytic solution can blow up in a finite time [5]. See [10] for the extension to van Dommelen–Shen type singularity. However, the damping term should play an important role for the long time behaviour of the solution.
In a recent work [20], Zhang and the fouth author proved the long time well-posedness of the classical Prandtl equation with small analytic initial data. More precisely, if the initial data and , then the lifespan of the solution is greater than . In [9], Ignatova and Vicol obtained a larger lifespan with small analytical data of size , whose analytical width as .
With the damping term and , Ren and Zhang proved the global well-posedness of the system (1.2) for small analytic data and finite time blowup for a class of large analytic data [15]. When , Xie and Yang proved the global stability of the Hartmann layer for analytic perturbations [17]. The Hartmann layer derived from the incompressible MHD equations in the Hartmann regime(see [8]) is just a steady solution of the system (1.2).
When the initial data is a small perturbation of the Hartmann layer, it is still monotonic in y variable so that the system is locally well-posed in Sobolev space. Then an important question is:
Whether the system is globally well-posed in Sobolev space in the case when the initial data is near the Hartmann layer.
For the classical Prandtl system, when the initial data is close to a monotonic shear flow, Xu and Zhang [19] proved a long time existence result in Sobolev space. However, it remains open whether one can obtain an explicit life span of the solution when the data is a small perturbation of a monotonic shear flow in Sobolev space in the sprit of the results in [9,20] for small analytic data.
For analytic perturbation, the key point for global result is to show that the analytic band cannot deteriorate to zero. Due to the damping term , the authors in [17] control the analytic band globally. For Sobolev perturbation, the problem becomes highly nontrivial. More precisely, we study the global stability of the Hartmann layer . Without lose of generality, we take and introduce the perturbation , which satisfies
To obtain the well-posedness in Sobolev space, we need to introduce a good unknown as in [1,13] defined by
Then w satisfies
where are some nonlinear terms (see Section 3). To prove the global well-posedness, we encounter two main difficulties:
Unlike the system (1.2), the new system (1.4) for good unknown w has no obvious damping mechanism;
Although for any , it decays exponentially to zero as so that the good unknown w becomes degenerate at . For this, we have to give a global in time control for the behavior of .
In fact, these also explain why the question of giving an explicit life span for the classical Prandtl system is still open. To overcome these difficulties, our proof introduces the following three key ingredients:
The exponential point-wise decay estimate inyvariable for the lower order derivatives of the velocity such as . A key observation is that the decay rate in y does not slow down as the time evolves due to the damping term. This fact is crucial for resovling the second difficulty. The proof of the point-wise bounds relies on the high order energy bounds.
High order energy estimate without the derivative loss inxvariable. For this, we introduce a good unknown w and use the paralinearized method in order to avoid using the Nash–Moser iteration as in [1]. More importantly, we reveal the damping mechanism hidden in the new system (1.4).
High order energy estimates inyvariable. We still use the velocity equation. Here we don’t need to take care of the derivative loss in x variable, since we only take one order derivative in x variable.
To state our result, we introduce the following weighted Sobolev space. For , the space consists of all functions satisfying
where with a positive weight function.
Now our main result is stated as follows.
Assume thatwithsatisfiesThen there existssuch that for any, the magnetic Prandtl model (
1.2
) has a unique global in time solution. Moreover, there holds that for any,
Exponential pointwise decay estimates
In this section, we derive the exponential pointwise decay estimates in the y variable. To this end, we introduce
Then satisfies
where . We define
Letbe a smooth solution of (
1.3
) onwith the initial datasatisfyingThen there exists a constantindependent of T so that for any,where
Let us first give the following pointwise estimates of F.
It holds that
A direct calculation shows that
and
By Sobolev embedding and the interpolation, we have
Then we infer that
A simple calculation yields
Then we have
This proves the second inequality. □
Using the assumption and , we get by integration by parts that
It follows from Lemma 2.2 that
In a similar way, we have
and
Thus, we have
A direct calculation gives
Here we use the fact with C independent of a. Thus, we infer from Lemma 2.2 that
Similarly, we have
In summary, we conclude the proof of the proposition. □
High order energy estimate in x variable
In this section, we assume that
where is a constant determined later. We introduce a weight and denote by C a constant independent of T and .
Paralinearization and good unknown
Due to the derivative loss induced by the term , we cannot make the energy estimate to the equation (1.3) directly. Motivated by [1,13], we need to introduce a good unknown. To avoid the Nash–Moser iteration, we will use the paralinearized method.
Using Bony’s decomposition (A.1), we get
where
Notice that there is no derivative loss for the terms in f. We denote
To eliminate the trouble term , we introduce a good unknown w defined by
A direct calculation shows that
where and are given by
Using the equation (1.2), we find
where . Then we have
Then we can write as
where
Therefore, . Thanks to , we can rewrite (3.4) as
Relationship between w and u
The following facts could be deduced from the definitions of .
It holds that for any,
The following lemma states the relation between and . For this, we will use the following formulas:
There existsso that if, then we haveHereare constants independent of.
By (3.7), we write
Here we used the fact that . Then by Lemma A.1, Lemma 3.1 and Young’s inequality, we get
Thanks to (3.1), taking ε small enough, we can deduce that
Using (3.8), we get by Lemma A.1 and Lemma 3.1 that
which along with (3.1) and (3.9) implies
This completes the proof of the lemma. □
Energy estimates
Let w be a smooth solution of (
3.4
). There existsso that if, then for any,
We first present the estimates of the source terms .
It holds that for any,
By Lemma A.1 and Lemma 3.1, we get
By Lemma A.1 and Lemma 3.1 again, we have
Similarly, we have
By Lemma A.2 and Lemma 3.1, we have
Summing up the estimates of , we get by Lemma 3.2 that
Similarly, we have
This finished the proof of the lemma. □
Taking the inner product between (3.6) and w, we obtain
Thanks to , we get by integration by parts that
and
This shows that
A simple calculation gives
From Lemma A.1 and Lemma A.2, we deduce that for ,
Summing up, we conclude by Lemma 3.4 that
which gives our result by taking ε small enough so that . □
High order energy estimate in y variable
In Proposition 3.3, we just present the high order derivative estimates of the solution in the x variable. To close the energy estimate, we need to derive the high order derivative estimates in the y variable. For this part, we don’t need to use the monotonicity. Again we make the assumption (3.1).
Letbe a smooth solution of (
1.3
) in. It holds that for any,Here C is a constant independent of.
The proof is split into three steps.
Step 1. estimate.
Taking inner product between (1.3) and , we obtain
First of all, we get by integration by parts that
By integration by parts again and , we get
It is easy to see that
This shows that
Thus, we deduce that
Step 2. estimate
We get by taking to (1.3) that
Taking inner product between (4.2) and , we obtain
Due to , we get by integration by parts that
By integration by parts again and , we get
and
Thus, we deduce that
Step 3. estimate
We first take to (1.3) to obtain
Then we take inner product with to obtain
We get by integration by parts and using that
Using , we get by integration by parts that
Similarly, we have
Thus, we deduce that
Summing up (4.1)–(4.5), we conclude that
This completes the proof. □
The proof of the local well-posedness of the system (1.2) is almost the same as the classical Prandtl system. So, we just use the bootstrap argument to prove that the local solution can be continued to a global one. To this end, we introduce the energy functional
Let us first assume that for any ,
where the constants are determined later, and with given by Lemma 3.2 and Proposition 3.3 respectively.
By Proposition 2.1, (5.1) and (5.2), we have
Taking , we deduce that for any ,
By Proposition 3.3, we have
which along with Lemma 3.2 implies
By Proposition 4.1, we have
Using (5.1) and (5.2), we can take ε small enough(if necessary) so that
which gives
It follows from (5.4) and (5.5) that
Note that here C is independent of . So, we can take so that
Now, (5.3) and (5.6) ensure that maximal existence time of the solution and there hold (5.1) and (5.2) for any .
Footnotes
Paraproduct
We introduce the paraproduct decomposition in R. Choose two smooth functions and , which satisfy
and for any ,
Then we define
The Bony’s paraproduct is defined by
Then we have the following Bony’s decomposition
where the remainder term is defined by
Let us recall the classical paraproduct estimate and paraproduct calculus in Sobolev space [2]. We denote by the usual Sobolev spaces.
Acknowledgements
Z. Zhang is partially supported by NSF of China under Grant 11425103.
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