A new conformal heat flow of harmonic maps
Abstract.
We introduce and study a conformal heat flow of harmonic maps defined by an evolution equation for a pair consisting of a map and a conformal factor of metric on the two-dimensional domain. This flow is designed to postpone finite time singularity but does not get rid of possibility of bubble forming. We show that Struwe type global weak solution exists, which is smooth except at most finitely many points.
Key words and phrases:
harmonic maps, conformal heat flow, short time existence, global weak solution2020 Mathematics Subject Classification:
Primary 58E20, 53E99, 53C43; Secondary 35K581. Introduction
Consider a map from a compact Riemann surface with metric to a Riemannian manifold . Under the usual harmonic map heat flow, evolves to a map according to the evolution equation , where is the tension field with respect to the metric . In this paper we consider the generalization in which both the map and the metric evolve with satisfying the equations
(1a) | |||||
(1b) |
where are constants and is the energy density. We assume that the initial map and metric are smooth.
The first of these equations is the harmonic map heat flow, with varying metric . The second equation is designed to attenuate energy concentration. If the energy density become large in some region , then under the flow (1b), the metric is conformally enlarged; this increases the area of and decreases the energy density. This suggests that the system (1b) may be better behaved than the harmonic map heat flow, where energy concentration at points is an impediment to convergence.
Writing the metric for a real-valued function , equations (1b) are equivalent to the following equations for the pair :
(2a) | |||||
(2b) |
where and are with respect to the fixed metric , and where the initial conditions are , . In this form, the flow is more easily analyzed.
The main Theorem of this paper is the following.
Theorem 1.1.
(Existence of global weak solution) For any , a global weak solution of (2b) exists on which is smooth on except at most finitely many points.
There is a long history of harmonic maps and related fields. We could not list all such literatures but only few, including [1], [2], [3], [4], [5], [6], [7], [8], [9], [10], [11], [12] and therein. In terms of heat flow of harmonic maps, see for example [13], [14], [15], [16], [17], [18], [19], [20], [21], [22], [23], [24], [25] and therein. Note that usual heat flow can have finite time singularity, see Chang-Ding-Ye [26], Raphael-Schweyer [27], or more recently Dávila-Del Pino-Wei [28].
There are several directions to allow metric change along harmonic map heat flow. The most well-known direction is Teichmüller flow, where metric lies in Teichmüller space of constant curvature. Teichmüller flow is the gradient flow of the energy and hence reduce the energy in the fastest sense. For relevant literature, see for example Rupflin-Topping [29], Huxol-Rupflin-Topping [30] or Rupflin-Topping [31] and therein. Another direction is Ricci-harmonic map flow. This is a combination of harmonic map heat flow and Ricci flow of the metric. Surprisingly, this flow is more regular than both harmonic map heat flow and Ricci flow. See for example, Muller [32], Williams [33] or Buzano-Rupflin [34] among others. Recently in Huang-Tam [35], harmonic map heat flow together with evolution equation of metric is considered under time-dependent curvature restriction and smooth short time existence is obtained. Because we do not assume a priori curvature bounds of the domain, the result cannot be applied into our case.
The paper is organized as follows. In Section 2 we look at some preliminaries, including volume formula and its asymptotic limit if the map is steady solution, that is, harmonic. Next, in Section 3 we define Hilbert spaces and their closed subsets . So, from Section 3 we consider and . Then Section 4 defines the operator and shows their properties. Briefly, we can show that and and they satisfy twisted partial contraction properties, see Lemmas 4.3, 4.4, 4.7, and 4.8. In the last section 5 we define the operator on mapping into itself defined by . For small enough, is a contraction and hence we can prove short time existence.
Next we are working on types of singularity. Ultimately we will show that the solution is singular only when energy concentrates, similar with Struwe’s result. In Section 6 we show local estimate and obtain bounds for . This is used in Section 7 to show and higher estimate, which implies boundedness of . Finally in Section 8 we prove the main theorem 1.1.
1.1. Notation
Even though our equation is heat-type equation for varying metric, we use initial metric as default. So, all terms using metric use unless we specify the metric. For example, is calculated in terms of and is calculated in terms of . If the volume form is calculated in terms of metric , we denote it as . We also omit and if there is no confusion. We also use the simplifications , and . Also, the constant is universal and changed line by line.
2. Preliminaries
Before we show the main result, we record a few facts about solutions to the flow equations (2b).
2.1. Energy and Volume
First note that the 2-form is conformally invariant, and that the energy
(3) |
satisfies
(4) |
Thus for all .
Lemma 2.1.
The volume satisfies , and hence is finite for all .
Proof.
The second equation (2b) can be explicitly solved, yielding
(5) |
Consequently, the volume
(6) |
can be written as
(7) |
The lemma follows by noting that and integrating. ∎
2.2. Asymptotic behavior of steady solution
Now we consider steady solution.
Lemma 2.2.
Proof.
This means that, for solutions as in Lemma 2.2, the energy density converges as to the constant .
Hence the conformal heat flow forces the conformal factor and the energy density be distributed evenly.
Remark that, because the image does not change, this flow modifies the domain toward the space which is similar to the image with the similarity ratio .
3. Construction of Hilbert spaces
In this section we build Hilbert spaces and their closed subsets . For parabolic theory used here, see Mantegazza-Martinazzi [36], Evans [37] or Lieberman [38]. From now on, we consider the target manifold being isometrically embedded, .
3.1. Spaces , and
The set
is a Hilbert space with norm
As in Proposition 4.1 in [36],
and there is a constant such that
(8) |
Also, by standard parabolic theory (See, for example, [37]), implies , and
(9) |
This also implies that
(10) |
Next, denote
be another Hilbert space with norm
Note that in the notation of [36], and .
Now we define spaces for . The set
is a Hilbert space with norm
Similar to above, there is a constant such that
(11) |
and
(12) |
Also, by Sobolev embedding, we have
(13) |
Moreover, is continuous and there is a constant such that for all ,
(14) |
3.2. The ball and
Now we fix throughout the section and thereafter. Consider the operator . If , this operator is uniformly elliptic. So, Proposition 2.3 of [36] then says that the map is a linear isomorphism
Hence there is a constant such that for each and , there is a unique solution of the initial value problem
(15) |
with
(16) |
Because of (8), is a closed affine subspace of . Hence the ball
(19) |
is a closed subset of . Note that each satisfies
(20) |
Also let the ball
be a closed subset of . Obviously and . For simplicity, we denote and .
Now fix and define
(21) |
Choose small enough so that which implies . Also we assume .
4. Construction of operators
In this section we will construct operators and . First fix and . and are considered to be fixed throughout this section and after unless we mention any choice of them.
First we show a lemma that is needed in several places.
Lemma 4.1.
Fix . Then there is an such that for all , for each and ,
(22) |
Proof.
Next, consider .
Hence, by integrating, we have
if we choose small enough.
Finally, we will compute .
Hence,
if we choose small enough.
Combining all the estimates above, we get
which proves the lemma. ∎
4.1. The construction
Define an operator
by where is the unique solution of
(23) |
Lemma 4.2.
Fix . Then there is such that for all , restricts to an operator .
Proof.
We also can assume where depends only on the geometry of . Then the vector-valued function satisfies the pointwise bound . Fix and .
Now we estimate norm of
First, , so . Hence if we choose small enough, we have . Next, compute .
So, using Young’s inequality
we get, by (8), (9), (10), (12) and (20),
if we choose small enough. Finally,
and
if we choose small enough.
Therefore, if we choose small enough, we have . Noting that satisfies
The bounds (16) give
because satisfies (17).
Now by Lemma 4.1 with , , ,
This implies
Therefore . ∎
Lemma 4.3.
Fix and . Then there is an such that for all and for each ,
(24) |
Proof.
Set and for and subtracting, the function satisfies
Hence (15) gives a bound
(25) |
Next, we have
So, there is a constant with
Integrating and applying Holder’s inequality, (8), and (20) gives
if we choose small enough.
For , first note that
So, we get
Using (8), (9), (10), (12), (13), and using Young’s inequality, we can estimate it term by term.
Hence, using (20), if we choose small enough, we get
We obtain similar result for if we choose small enough:
Hence, we obtain that .
Finally, compute . As above, note that
So,
Similar with above, by (8), (9), (10), (12), (13) and (20),
if we choose small enough.
Combine all of them,
which proves the lemma. ∎
Lemma 4.4.
Fix and . Then there is an such that for all and for each ,
(26) |
4.2. The construction
Define an operator
by where is the unique solution of
(27) |
Lemma 4.5.
In the above definition, .
Proof.
From (27), we directly get
(28) |
So, and is trivially bounded if and . (Because , we have is pointwise uniformly bounded by .) Applying Cauchy-Schwarz, we obtain the pointwise bound
so
which is bounded if and .
In fact, we can show further.
Lemma 4.6.
Fix . Then there is such that for all , restricts to an operator .
Proof.
From previous calculation, we have
So, if we choose small enough, we get . Also, because and , we can make if we choose small. Finally,
so if we choose small enough, we get . This proves the lemma. ∎
Lemma 4.7.
Fix and . Then there is an such that for all and for each ,
(29) |
Proof.
Set . Then from (27), subtracting them gives
So,
if we choose small enough. Also,
if we choose small enough.
Next, compute .
So,
Integrating over gives
if we choose small enough.
Finally consider .
So,
if we choose small enough.
In summary, we get
which proves the lemma.
∎
Lemma 4.8.
Fix and . Then there is an such that for all and for each ,
(30) |
Proof.
Set . Subtracting them gives
Using , we have
so if we choose small enough, we have that .
Next, compute .
So,
Now we integrate over .
if we choose small enough.
Finally,
so
if we choose small enough.
In summary, we get
which proves the lemma.
∎
5. Existence of fixed point
Because and are Hilbert space, is also a Hilbert space and we can equip the norm
(31) |
Define an operator by
(32) |
Proposition 5.1.
Fix . Then there is an such that for all ,
-
(a)
restricts to an operator .
-
(b)
For each and ,
(33)
Proof.
Theorem 5.2.
(Short time existence for strong solution) There is such that there exists a smooth solution of (2b) on .
Proof.
The existence of solution comes from 5.1. The fact can be easily shown using nearest point projection, see for example [24]. Moreover, the operator is uniformly parabolic, so for any , by standard parabolic theory. This implies
for any .
Next, by direct computation from (2b), we have
hence
which implies for any . Now taking in the equation (2a) to get
which implies
for any .
Finally, from Sobolev embedding, we have for some . This implies where is parabolic Hölder space of exponent . Now by Schauder estimate and standard bootstrapping argument, we conclude that is smooth, so is. ∎
6. Local estimate
To get global weak solution, we will follow Struwe’s idea: Run the flow until singularity occurs. Then take weak limit as new initial condition, run the flow again. Keep going this process and we will have only finitely many singularities due to finiteness of the energy. Because our flow is coupled, we need to re-establish the whole process with and . And this requires some condition on , which can be interpreted as the sensitiveness of the conformal evolution of the metric with respect to high energy density. Let be a constant only depending on the embedding such that where is the Riemannian curvature tensor of . And from now on, assume .
6.1. Energy estimate
Now we establish local energy estimate. Fix and let be a cut-off function supported on such that on , and .
Proposition 6.1.
Proof.
Lemma 6.2.
Furthermore, assume
Then we have
(36) | ||||
(37) |
Proof.
6.2. Estimate for
The next step is to get estimate for derivative of , which will lead to the control of itself. For the future purpose, here we introduce more general version of it. For now, we need .
Proposition 6.3.
Proof.
By taking time-derivative to (2a), we have
Taking inner product with and integrating gives
Now we have
On the other hand, LHS becomes
All together, we have
By the choice of , the last term is negative for all . Hence,
by Gronwall’s inequality. ∎
Lemma 6.4.
Proof.
Corollary 6.5.
Under the same assumption as above, we also have
(43) | ||||
(44) |
Proof.
From the equation (38) with , we can integrate from to .
Hence, we have
The other inequality is similar. ∎
6.3. Higher estimate for time derivatives
In this subsection we will get estimate for . We first build up -version of Equation 34.
Proposition 6.6.
For solutions of (2b) and for , we have
(45) | ||||
Proof.
First note that for any , . Also, for simplicity, denote . Multiplying to (2a) gives
Multiplying for and integrating gives
Now
This completes the proof. ∎
Now we will show the desired estimate.
Proposition 6.7.
Note that depends on .
Proof.
For simplicity, denote , . Also, denote for any number appeared in computations. Suppose be a cut-off function supported on and on and . Also, let be a cut-off function supported on and on and . Let and .
The proof consists of several steps, increasing power of .
Step 1. Estimate for .
Step 2. Estimate for .
Step 3. Estimate for and .
From (38) with , we can integrate from to .
Note that . Now, from (48), (49), and (50), we have
So, we have
(51) |
Similarly,
(52) |
Step 4. Estimate for .
Step 5. Estimate for .
Remark 6.8.
We can keep going on to get bounds for for any . However, these bounds blow up to infinity as .
7. and gradient estimate
In this section we will get estimate and gradient estimate for the solution of (2a). For simplicity, denote and . First observe the following.
Lemma 7.1.
Let be a solution of (2b). For and for any ,
(55) |
Proof.
Note that
So, multiplying and integrating over gives
by Young’s inequality with weight . Hence, by integrating, we obtain the result. ∎
Lemma 7.2.
Let be any smooth function and let be a cut-off function. Then for any and , we have
(56) |
Proof.
Let be such that . By Sobolev embedding,
∎
Next, we will show estimate.
Proposition 7.3.
Let are solutions of (2b). Then there exists such that the following holds:
Assume that
Then for , we have
(57) |
where
Proof.
Suppose be a cut-off function supported on and on and . Also, let be a cut-off function supported on and on and . Let .
Without loss of generality, assume . Then we have, by Poincare,
From the equation , multiplying and arranging terms gives
By the estimate, we have
(58) |
where the constant only depends on and .
Now applying Lemma 7.2 with , gives
On the other hand, applying Lemma 7.2 with , gives
All together, we have
Let . Then the above equation becomes
So, if is small enough so that , then by Gronwall’s inequality, we have
This completes the proof. ∎
From Sobolev embedding, we now have, for ,
(59) |
for any .
Now we will show gradient estimate. This can be achieved by obtaining better estimate than , say .
Proposition 7.4.
Assume the same as in 7.3. In addition, we assume that
Then for , we have
(60) |
where
In particular,
(61) |
Proof.
By Equation 59, we have uniform bound for for any . Now from equation (58), we have
Now let and . Then we have, using (55) and Equation 59,
Applying Equation 59 completes the proof. ∎
8. Global weak solution
In this section, we will prove the main theorem 1.1.
Lemma 8.1.
There exists such that if be a smooth solution of (2b) on and
(62) |
then Hölder norms of and their derivatives are all bounded by constants only depending on .
Proof.
By the sup bound of , we have and
Hence the operator is uniformly parabolic on .
Similar in proof of Theorem 5.2, we conclude the desired estimate. ∎
Proof.
(Proof of Theorem 1.1) First consider is smooth. By Theorem 5.2, there exists a smooth solution in for some . Let be the maximal existence time. If then we obtain global solution which is smooth everywhere. So suppose .
If we have for any and , then by above lemma Hölder norms of and their derivatives are all bounded, hence can be extended beyond the time . This contradicts with maximality of . So there should be a point such that
Since the total energy is finite, there are at most finitely many such points . Then by above lemma, we get smooth solution on . If we denote and as the weak limit of and as , then converges to strongly in .
Next, denote and consider the flow (2b) with initial map and initial metric . As above, there is a smooth solution on . From these we can set up a smooth solution on which is smooth except . Iterate this process to obtain global solution with exception points, which are at most finitely many because the total energy is finite.
∎
9. Finite time singularity
As the conformal heat flow is developed to postpone the finite time singularity, it is expected to have no finite time singularity. In this section we will discuss few remarks about finite time singularity.
Recall the following
Lemma 9.1.
([23]) There exist a compact target manifold , a smooth map and such that every smooth map homotopic to fails to be harmonic. If furthermore , then
Together with energy decreasing property of harmonic map heat flow , the above lemma implies that no heat flow starting with initial map homotopic to above can be smooth after the time .
This argument can be avoided in conformal heat flow. From (4), we have
So, if is large, can be smaller than even if .
The proof of the above lemma relies on no-neck property of approximate harmonic map with . And the assumption is essential in the no-neck property as there is a counter example of Parker without the assumption. The conformal heat flow makes the tension field converge to zero with different scale. Hence the information about the converging scale of the tension field will play an important role in the property of the flow.
Acknowledgement
The author would like to thanks Armin Schikorra and Thomas Parker for valuable comments and advice.
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