In this paper, we will establish the lower bound for the blow-up time of the solution to the following problems:
Here $ a>0 $, $ m>1 $, $ p\geq 0 $ and $ q\geq 0 $, $ \Omega\subset \mathbb{R}^n\; (n\geq 3) $ is a smooth bounded domain, $ \nu $ is the outward norm vector. The initial data $ u_{0}(x) $ is a continuous nonnegative function and satisfies the compatible conditions. In [3], LI and XIE proved that the solution to (1.1) exists globally if $ p+q< m $ or $ p+q = m $ and $ a $ is sufficiently small, while the solution will blow-up in finite time if $ p+q> m $ and the initial data $ u_{0}(x) $ is sufficiently large.
The direct motivation of this paper comes from the papers [1] and [2]. In [1], the authors estimated the lower bounds for the blow-up time of solution to (1.1) subject to Dirichlet boundary condition and Neumann boundary condition in 3-dimension space. In [2], the authors only established the lower bounds for the blow-up time of the solution to (1.1) subject to Dirichlet boundary condition with smooth bounded $ \Omega\subset \mathbb{R}^n $ and $ n\geq 3 $. Naturally, we hope to obtain the lower bound for the blow-up time of the solution to $ (1.1) $ subject to Dirichlet boundary condition and Neumann boundary condition with smooth bounded $ \Omega\subset \mathbb{R}^n $ and $ n\geq 3 $. Inspired by Payne-Schaefer's idea and following the AN and SONG's methods in [4], we will use a delicate application of general Sobolev inequality to deal with both (1.1) subject to Neumann boundary condition and (1.1) subject to Dirichlet boundary condition. There are many results about the estimates of the lower bounds for blow-up time of the solution to parabolic equation. We can refer to [5-13] and the references therein to get more information.
Our main result in this paper can be stated as follows:
Theorem 1.1 Assume that $ u $ is the blow-up solution of $ (1.1) $, which will blow-up at time $ t = t^{\ast} $. Then the lower bound for the blow-up time of the solution is
where $ \phi(t) = \int_{\Omega}u^{nk}\mathrm{d}x, \; \phi(0) = \int_{\Omega}u_{0}^{nk}\mathrm{d}x, $ with $ n\geq3 $, $ k>\max\{\frac{p+q-m}{2}, \frac{1}{n}\} $, and $ M $, $ C_1 $, $ C_2 $ are given by the following section.
We will give the details to proof of Theorem $ 1.1 $ in the next section.
In this section, using a delicate application of general Sobolev inequality, we will establish the lower bound for the blow-up time of the solution to (1.1).
Proof of Theorem 1.1. Define
with $ n\geq3 $, $ k>\max\{\frac{p+q-m}{2}, \frac{1}{n}\} $.
Using Green formula, we have
Using Hölder inequality to the last term in the right of $ (2.2) $, we get
where $ |\Omega| $ denotes the measure of $ \Omega $.We denote that $ C(\Omega) $ is the best constant in general Sobolev's inequality
for any $ w\in H^{1}(\Omega) $.
In convenience, we denote
Then using Hölder inequality and Young's inequality, we have
Here $ \varepsilon $ will be chosen later, while
Using general Sobolev's inequality and Young's inequality to the last term in the right of $ (2.4) $, we get
By Young's inequality to the last term in the right of $ (2.5) $, we get
Substituting $ (2.6) $ into $ (2.5) $, we obtain
Substituting $ (2.7) $ into $ (2.4) $, we have
Substituting $ (2.8) $ into $ (2.3) $, we get
Now we can choose
to make the coefficient of $ \int_{\Omega}|\nabla u^{\frac{nk+m-1}{2}}|^2\mathrm{d}x $ vanishes. Then we have
where
Integrating (2.9), we have
with
By the analysis above, we can get the proof of Theorem 1.1.