The porous medium equation(PME for short)
appears in the description of different natural phenomena, and its theory and properties depart strongly from the heat equation, $ u_t = \Delta u $, it's most famous relative. There are kinds of physical applications where we can use this model, mainly to characterize process involving fluid flow, heat transfer or diffusion. For more knowledge, we recommend the book [1] to the reader.
Among typical nonlinear problems, the mathematical theory of PME is also based on a priori estimates. In 1979, Aronson and Bénilan obtained a celebrated second-order differential inequality of the form [2]
which applies to all positive smooth solutions of (1.1) defined on the whole Euclidean space on the condition that $ m > m_c : = 1-2/n $. The theory of PME on manifolds is rare. In 2008, Lu, Ni, Vázquez and Villani studied the PME on manifolds [3]. They got the following local Aronson-Bénilan estimate.
Theorem 1 (see [3]) Let $ u $ be a positive solution to PME (1.1), $ m>1 $ on the cylinder $ Q: = B({\mathcal O}, R)\times[0, T] $. Let $ v: = mu^{m - 1}/(m - 1) $ be the pressure and $ v^{R, T}_{\rm max}: = \mathop{\rm max}\limits_{{B(\mathcal O}, R)\times[0, T]}v $.
Assume that Ric $ \geq-(n-1)K^2 $ on $ B({\mathcal O}, R) $ for some $ K\geq 0 $. Then, for any $ \alpha > 1 $, we have that on $ Q': = B({\mathcal O}, R/2 ) \times[0, T] $
Here, $ a = \frac{n(m-1)}{n(m-1)+2} $, $ \widetilde{C_2(\alpha)} $, $ \widetilde{C_3(\alpha)} $ and $ \widetilde{C'_1(KR)} $ depend on $ m $ and $ n $.
Next, we will discuss PME with drifting Laplacian operator. Smooth metric measure spaces carry a similar operator to the Laplace-Beltrami operator $ \Delta $, the $ f $-Laplacian, which is also called drifting Laplacian or Witten-Laplacian, defined for a function $ u $ by $ \Delta_f u = \Delta u-g(\nabla f, \nabla u) = \Delta u-\langle{\nabla f, \nabla v}\rangle $. The N-Barkry-Emery Ricci tensor is defined by $ Ric^N_f = Ric+Hessf-\frac{1}{N}df\otimes df $. A natural question about smooth metric measure space is which of the results about the Ricci tensor and the Laplace-Beltrami operator can be extended to the N-Bakry-Emery Ricci tensor and $ f $-Laplacian. For example, In [3], Lu et al. derived some gradient estimates for the PME equation on Riemannian manifolds with Ricci curvature bounded from below:
where $ m> 1 $. In [4], Huang and Li got a better result in [3]. In [5], Huang and Li researched the following porous medium type equation,
on smooth metric measure space. Under the assumption that the N-dimensional Bakery-Emery Ricci curvature is bounded from below, Huang and Li obtained some gradient estimates that generalized the results in [3] and [5].
In this paper, we will follow closely [3] and derive local gradient estimates for positive bounded solutions of PME on Riemannian manifolds under general geometric flow. The general geometric flow equation where $ h_{i j} $ is a second-order symmetric tensor is as follows:
The idea is from the Ricci flow $ \frac{\partial g_{ij}}{\partial t} = -2R_{ij}, $ which was introduced by Hamilton [6] in 1982.
Then, we will get a similar result with drifting Laplacian operator on PME. Also, our idea comes from Huang and Ma in [7], who considered gradient estimate for the following parabolic equation
on smooth metric measure spaces. Inspired by the research of harmonic function and positive solution to linear heat flow on Riemannian manifolds, this paper extends corresponding gradient estimate from a fixed Riemannian metric to the case that the metric evolves by a general geometric flow.
Our first result states the gradient estimate of the pressure function $ v $.
Main Theorem 1 Let $ g(t) $ be a solution to the general geometric flow on a Riemannian manifold $ M^n(n\geq2) $ for $ t $ in some time interval $ [0, T] $. Let $ M $ be complete under the initial metric $ g(0) $. Let $ u $ be a positive smooth solution to PME (1.1), $ m>1 $ on the cylinder $ Q: = B({\mathcal{O}}, R)\times[0, T] $. Note $ v: = \frac{m}{m-1}u^{m-1} $ is the pressure, and write $ v^{R, T}_{{\rm max}}: = \mathop{{\rm max}}\limits_{B({\mathcal O}, R)\times[0, T]}v $ and $ v^{R, T}_{\rm min}: = \mathop{\rm min}\limits_{B({\mathcal O}, R)\times[0, T]}v $.
Assume that $ -(n-1)K_0^2\leq Ric $, $ -(n-1)K_1^2\leq h \leq(n-1)K_2^2 $, $ |\nabla h|\leq K_3 $ on $ B({\mathcal O}, R) $ for some $ K_0, K_1, K_2, K_3\geq 0 $. Then, for any $ \alpha>1 $, we have that on $ Q': = B({\mathcal O}, \frac{R}{2})\times[0, T] $,
$ C_{i} $ is a constant depending on $ m, \ n, \ a, \ \alpha, \ K_0, \ K_1, \ K_2, \ K_3, \ K_4, \ R. $
Remark When $ h = -2Ric $, (1.6) is the Ricci flow equation. In this case our results reduce to [8]. Note that for Ricci flow the assumption $ |\nabla Ric|\leq K_3 $ is not needed because of the contracted second Bianchi identity [[9], section 4].
As an application, we get the following result.
Corollary 1.1 $ v $ is the pressure, then for any $ x_1 $, $ x_2 $ $ \in B({\mathcal O}, R/6) $ and any $ \alpha>1 $,
where $ \gamma (s) $ is a smooth curve connected $ x_1 $ and $ x_2 $ with $ \gamma (t_1) = x_1 $ and $ \gamma (t_2) = x_2 $, $ |\gamma'(s)|_s $ is the length of the vector $ \gamma'(s) $ at time $ s $.
We extend the Laplacian operator to the drifting Laplacian operator, and we can get similar gradient estimate.
Main Theorem 2 Let $ (M^n, g, dv) $ be a smooth metric measure space. Suppose that $ u $ is a positive solution to (1.5). If $ |\nabla f|\leq c_0 $, $ |\nabla^2 v|\leq c_1 $, $ Ric^N_f(B_p(2R))\geq-k_0 $, $ -k_1\leq h\leq k_2 $, $ |\nabla h|\leq k_3 $. Here, $ k_0, k_1, k_2, k_3 \geq 0 $, then on the ball $ B_p(R) $ we have
where $ c_2, c_3, c_4 $ are constants depending on $ a, \ c_0, \ c_1, \ \alpha, \ m, \ n, \ H, \ R, \ T $, and
Corollary 2.1 Let $ (M^n, g, dv) $ be a smooth metric measure space with $ |\nabla f|\leq c_0 $, $ |\nabla^2 v|\leq c_1 $, $ Ric^N_f\geq -k_0 $, $ -k_1\leq h\leq k_2 $, $ |\nabla h|\leq k_3 $. Here, $ k_0, k_1, k_2, k_3 \geq0 $ suppose that $ (M^n, g) $ is a complete non-compact Riemannian manifold and $ u $ is a positive solution to (1.5), then
where $ c_{i} $ is a constant depending on $ a, \ \alpha, \ m, \ n, \ S, \ T $, and $ S = \mathop{sup}\limits_{M^n\times [0, T]}(m-1)v, \alpha(t) = e^{2Sk_0t}. $
Remark When $ g $ is independent of $ t $, our results reduce to [10].
Note that the pressure $ v: = \frac{m}{(m-1)}u^{m-1} $ satisfies
Assuming that $ u>0 $, we introduce the quantities $ y = \frac{|\nabla v|^2}{v} $, $ z = \frac{v_t}{v} $ and the differential operator: $ L: = \partial _{ t }-(m-1)v \Delta. $ Let $ F_\alpha: = \alpha z-y. $ From equation (2.1) we know
First, let us calculate a formula for $ L(F_\alpha) $.
Lemma 2.1
Proof Recall that $ \frac{\partial}{\partial t}\Gamma^k_{ij} = g^{kl}(\nabla_ih_{jl}+\nabla_jh_{il}-\nabla_lh_{ij}). $ Thus,
Lemma 2.2 Let $ g(t) $ be a solution to the geometric flow on a Riemannian manifold $ M^n(n\geq2) $ for t in some time interval $ [0, T] $. Let $ M $ be complete under the initial metric $ g(0) $. Let u be a positive smooth solution to (1.1) on manifold $ (M^n, g(t)) $ for some $ m>0 $, and let $ v: = \frac{m}{m-1}u^{m-1} $ be the pressure. Then we have
Proof Calculate directly by using the Lemma 2.1.
Proposition 2.1 Let $ u $ and $ v $ be as in Lemma 2.2. Then
Proof The following formula is helpful in the calculation:
Using (2.6) and Lemma 2.2 we have
These give that
Using the formula
we have
Hence we obtain
Note the fourth to eighth terms in the above equation, they can be rewritten as
This completes the proof.
Then, we prove a local estimate for PME on complete manifolds under general geometric flow. We use the technique of Li and Yau [11] and some calculation of Lu, Ni, Vázquez and Villani in [3]. Denote by $ B({\mathcal O}, R) $ the ball of radius $ R>0 $ and centered $ \mathcal{O} $ in $ (M^n, g(t)) $, and denote by $ r(x, t) $ the distance function from $ \mathcal{O} $ to $ x $ with metric $ g(t) $.
Proof of the Main Theorem 1
(i) Since bounded $ h $ tensor implies that $ g(t) $ is uniform equivalence to the initial metric $ g(0) $[[12], Corollary 6.11], that is $ e^{-2K_1T}g(0)\leq g(t)\leq e^{2K_2T}g(0). $ By definition, we know that $ (M, g(t)) $ is also complete for $ t\in[0, T] $. Inspired by the choice of cutoff function in the proof of Theorem3.1 in [10], we let $ \eta(x, t): = \theta(r(x, t)/R) $ be cutoff function, where $ \theta(s) $ is a smooth monotone function which satisfies $ \theta(s)\equiv1 $ for $ 0\leq s\leq1/2 $, $ \theta(s)\equiv0 $ for $ s\geq 1 $, and $ ({\theta'})^2/\theta \leq40 $, and $ \theta''\geq-40\theta\geq-40 $. On $ B({\mathcal O}, R) $, using the Laplacian comparison theorem, one can easily get
and
(ii) After the preparation in (i), now we apply $ L $ to $ t\eta(-F_\alpha) $ and use the maximum principle to obtain our estimates. If $ t\eta(-F_\alpha)\leq0 $ on $ Q $, then the main theorem 1 is trivial. So we assume max$ _{(x, t)\in Q}t\eta(-F_\alpha)>0 $. Suppose $ t\eta(-F_\alpha) $ achieves its maximum at $ (x_0, t_0) $. Then we have $ t_0>0 $ and
at $ (x_0, t_0) $. From now on, all calculations are at $ (x_0, t_0) $.
By the evolution formula of geodesic length under geometric flow(see [13]), we calculate
where $ \gamma_{t_0} $ is the geodesic connecting $ x $ and $ \mathcal{O} $ under the metric $ g(t_0) $, $ S $ is the unit tangent vector to $ \gamma_{t_0} $ and $ ds $ is the element of arc length.
Denote $ C_1: = 40((n-1)(1+K_0R)+1) $, $ C_2: = \sqrt{40}(n-1)K_1^2 $, $ \widetilde{y}: = \eta y = \eta|\nabla v|^2/v $ and $ \widetilde{z}: = \eta z = \eta\frac{v_t}{v} $. Combining (2.5) with the above estimates of $ \eta $, we have
Here, we have used Proposition 2.1. Using the following inequality, (2.10) and (2.11)
Using Young's inequality,
and attention our assumption of $ h $,
On the other hand,
We get
Now write $ C_3: = 80+C_1 $ and
Also note that
and write $ a: = \frac{n(m-1)}{1+n(m-1)} $, we get
Using
then the above quadratical inequality (2.12) on $ (\widetilde{y}-\alpha\widetilde{z}) $ reduces to
Here, $ C_8: = \alpha^2(m-1)((n-1)(K_1^2+K_2^2))^2+\frac{9}{2}nK_3^2\alpha^2(m-1)^2 $. This implies that
Proof of the Corollary 1.1 Direct calculation implies
The result follows from the observation that $ \gamma(s) $ lies completely inside $ B({\mathcal{O}}, \frac{R}{2}) $ at any time in $ [0, T] $ (since bounded tensor $ h $ implies that $ g(t) $ is uniform equivalence to the initial metric $ g(0) $) and the estimate in the main theorem 1.
To prove the main theorem 2, we need some lemmas as well. Note
Suppose that $ u $ is a positive solution to (2.13). Let $ v = \frac{m}{m-1}u^{m-1} $. Direct calculation shows that
Since $ v\not = 0 $, then (2.14) is equivalent to
Let $ L = \partial_t-(m-1)v\Delta_f $ and $ F = \frac{|\nabla v|^2}{v}-\alpha\frac{v_t}{v} $. We have the following lemmas.
Lemma 2.3 Suppose that $ u $ is a poistive solution to (2.13). Then
Proof Direct calculation shows that
Therefore, we get
By (2.15) and Lemma 2.1, we have
According to (2.18), (2.19), (2.20), and (2.21). We conclude that
On the other hand, by (2.14) we get
Direct calculation shows that
According to (2.23) and (2.24), we obtain
According to [[14], [15]], we have
By (2.25) and (2.26), we conclude that (2.17) is true.
Lemma 2.4 The function $ F $ satisfies the following equation:
Proof For the reader's convenience, we give the details of the proof of Lemma 2.4. By (2.16) and (2.17), we have
By the definition of F, we have
According to (2.15) we get
Using (2.15) again, we arrive at
Putting (2.29), (2.30) and (2.31) into (2.28), we conclude that (2.27) is true.
Proof of the Main Theorem 2 We consider $ F $ in the geodesic ball $ B_p(2R) $, which is centered at $ p $ with radius $ 2R $, where $ \alpha = e^{2Hk_0t} $. Since $ Ric^N_f(B_p(2R))\geq-k_0 $, by (2.27) and definition of $ H $ and $ a: = \frac{(n+N)(m-1)}{(n+N)(m-1)+2} $, we have
Since $ L(\alpha^{-1}F) = (\alpha^{-1})'F+\alpha^{-1}L(F) $ and $ \alpha' = 2Hk_0\alpha $, then
By (2.15) and definition of $ F $, we get
Putting (2.33) into (2.32), we obtain
Attention the definition of $ h, |\nabla f| $, the following reality and the Young's inequality,
we have,
where we have used $ -ax^2+bx\leq b^2/4a $ to the first term in the second inequality.
Write $ c_2: = (m-1)c_0(k_1+k_2)H+\frac{9}{4}n(m-1)k_3^2H+\frac{a\alpha(2(\alpha-1)(k_1+k_2)+2\alpha)^2}{4(\alpha-1)((\alpha-1)+a)}+2(m-1)(k_1+k_2)c_1 $, we have
According to (2.4) and (2.5) in [7], we can construct a cut-off function $ \phi $ such that $ 0\leq\phi\leq1 $, sup$ (\phi) \subset B_p(2R) $, $ \phi|_{B_p(R)} = 1 $ and
where $ C $ is a constant depending only on n. Set $ G = t\phi\alpha^{-1}F $. Assume that $ G $ achieves its maximum at the point $ (x_0, s) \in B_p(2R) \times [0, T] $ and assume $ G(x_0, s)\geq 0 $. By the maximum principle, we have
at the point ($ x_0, s $), and
Multiplying both sides of (2.36) by $ s\phi $, and using $ -ax^2+bx\leq b^2/4a $, we get
Write $ c_3: = \frac{1+a(\alpha-1)}{a\alpha} $, $ c_4: = \frac{a\alpha^2m^2H}{2(m-1)(\alpha-1)(1-a)}\frac{C}{R^2}+H\frac{C}{R^2}(1+R\sqrt{k_0})+2H\frac{C}{R^2}+\frac{1}{T} $. The above inequality becomes
We can get
Hence, for all $ x \in B_p(R) $, it holds that
Thus, the proof of the main theorem 2 is completed. Letting $ R \rightarrow \infty $, $ c_4 \rightarrow \frac{1}{T} $, we get the result of Corollary 1.2.