The novel numerical solutions for time-fractional Fornberg-Whitham equation by using fractional natural transform decomposition method

Aslı Alkan; Halil Anaç; Aslı Alkan; Halil Anaç

doi:10.3934/math.20241237

AIMS Mathematics

2024, Volume 9, Issue 9: 25333-25359. doi: 10.3934/math.20241237

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The novel numerical solutions for time-fractional Fornberg-Whitham equation by using fractional natural transform decomposition method

Aslı Alkan ¹,
Halil Anaç ^{2
,
,}

1.
Department of Mathematics, Faculty of Science, Fırat University, Elazığ 23119, Turkey
2.
Department of Computer Technologies, Torul Vocational School, Gumushane University, Gumushane 29802, Turkey

Received: 25 January 2024 Revised: 07 May 2024 Accepted: 20 May 2024 Published: 30 August 2024
MSC : 35C05, 35R11, 65R10

The time-fractional partial differential equations were solved by the fractional natural transform decomposition method. Fractional derivatives are Caputo sense. The Fornberg-Whitham equation is a generalization of the Korteweg-de Vries (KdV) equation, which describes the propagation of long waves in shallow water. It includes higher-order dispersion terms, making it applicable to a wider range of dispersive media the fractional natural transform decomposition method (FNTDM) was also used to examine applications, and the solutions obtained by this method have been compared to those obtained by the variational iteration method, fractional variational iteration method, and homotopy perturbation method. In addition, the MAPLE package drew graphs of the solutions of nonlinear time-fractional partial differential equations, taking into account physics. The method described in this study exhibited a notable degree of computational precision and straightforwardness when used to the analysis and resolution of intricate phenomena pertaining to fractional nonlinear partial differential equations within the domains of science and technology.

Keywords:

Citation: Aslı Alkan, Halil Anaç. The novel numerical solutions for time-fractional Fornberg-Whitham equation by using fractional natural transform decomposition method[J]. AIMS Mathematics, 2024, 9(9): 25333-25359. doi: 10.3934/math.20241237

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Abstract

1. Introduction

In this paper, we study the 2D steady compressible Prandtl equations in $\left\{ x > 0, y > 0 \right\}$ :

$\begin{align} \left\{\begin{aligned} &u\partial_{x}u+v\partial_{y}u-\frac{1}{\rho}\partial^{2}_{y}u = -\frac{\partial_{x}P(\rho)}{\rho},\\ &\partial_{x}(\rho u)+\partial_{y}(\rho v) = 0,\\ & u|_{x = 0} = u_{0}(y), \quad\lim\limits_{y\to \infty}u = U(x),\\ &u|_{y = 0} = v|_{y = 0} = 0, \end{aligned}\right. \end{align}$

(1.1)

where $(u, v)$ is velocity field, $\rho(x)$ and $U(x)$ are the traces at the boundary $\left\{y = 0\right\}$ of the density and the tangential velocity of the outer Euler flow. The states $\rho, U$ satisfy the Bernoulli law

$\begin{align} U\partial_{x}U+\frac{\partial_{x}P(\rho)}{\rho} = 0. \end{align}$

(1.2)

The pressure $P(\rho)$ is a strictly increasing function of $\rho$ with $0 < \rho_{0}\leq\rho \leq \rho_{1}$ for some positive constants $\rho_{0}$ and $\rho_{1}$ .

In this paper, we assume that the pressure satisfies the favorable pressure gradient $\partial_{x}P\leq0$ , which implies that

$\partial_{x}\rho\leq0.$

The boundary layer is a very important branch in fluid mechanics. Ludwig Prandtl ^[14] first proposed the related theory of the boundary layer in 1904. Since then, many scholars have devoted themselves to studying the mathematical theory of the boundary layer ^{[1,7,8,9,11,12,17,18,19,21,22,23,24,26,27]}. For more complex fluids, such as compressible fluids, one can refer to ^[19,20,28] and the references therein for more details. Here, for our purposes, we only list some relevant works.

There are three very natural problems about the steady boundary layer: (ⅰ) Boundary layer separation, (ⅱ) whether Oleinik's solutions are smooth up to the boundary for any $x > 0$ and (ⅲ) vanishing viscosity limit of the steady Navier-Stokes system. Next, we will introduce the relevant research progress in these three aspects. The separation of the boundary layer is one of the very important research contents in the boundary layer theory. ^[17]. The earliest mathematical theory in this regard was proposed by Caffarelli and E in an unpublished paper ^[25]. Their results show that the existence time $x^{*}$ of the solutions to the steady Prandtl equations in the sense of Oleinik is finite under the adverse pressure gradient. Moreover, the family $u_{\mu}(x, y) = \mu^{-\frac{1}{2}}u(x^{*}-\mu x, \mu^{\frac{1}{4}}y)$ is compact in $C^{0}(\mathbb{R}_{+}^{2})$ . Later, Dalibard and Masmoudi ^[4] proved the solution behaves near the separation as $\partial_{y} u(x, 0)\sim(x^{*}-x)^{\frac{1}{2}}$ for $x < x^{*}$ . Shen, Wang and Zhang ^[18] found that the solution near the separation point behaves like $\partial_{y} u(x, y)\sim(x^{*}-x)^{\frac{1}{4}}$ for $x < x^{*}$ . The above work further illustrates that the boundary layer separation is a very complex phenomenon. Recently, there were also some results about the steady compressible boundary layer separation ^[28]. The authors found that if the heat transfer in the boundary layer disappeared, then the singularity would be the same as that in the incompressible case. There is still relatively little mathematical theory on the separation of unsteady boundary layers. This is because back-flow and separation no longer occur simultaneously. When the boundary layer back-flow occurs, the characteristics of the boundary layer will continue to maintain for a period of time. Therefore, it is very important to study the back-flow point for further research on separation. Recently, Wang and Zhu ^[21] studied the back-flow problem of the two-dimensional unsteady boundary layer, which is a important work. It is very interesting to further establish the mathematical theory of the unsteady boundary layer separation.

Due to degenerate near the boundary, the high regularity of the solution of the boundary layer equation is a very difficult and meaningful work. In a local time $0 < x < x^{*}\ll 1$ , Guo and Iyer ^[6] studied the high regularity of of the Prandtl equations. Oleinik and Samokhin ^[13] studied the existence of solutions of steady Prandtl equations and Wang and Zhang ^[23] proved that Oleinik's solutions are smooth up to the boundary $y = 0$ for any $x > 0$ . The goal of this paper is to prove the global $C^{\infty}$ regularity of the two-dimensional steady compressible Prandtl equations. Recently, Wang and Zhang ^[24] found the explicit decay for general initial data with exponential decay by using the maximum principle.

In addition, in order to better understand the relevant background knowledge, we will introduce some other related work. As the viscosity goes to zero, the solutions of the three-dimensional evolutionary Navier-Stokes equations to the solutions of the Euler equations are an interesting problem. Beirão da Veiga and Crispo ^[2] proved that in the presence of flat boundaries convergence holds uniformly in time with respect to the initial data's norm. For the non-stationary Navier-Stokes equations in the 2D power cusp domain, the formal asymptotic expansion of the solution near the singular point is constructed and the constructed asymptotic decomposition is justified in ^[15,16] by Pileckas and Raciene.

Before introducing the main theorem, we introduce some preliminary knowledge. To use the von Mises transformation, we set

$\begin{align*} \tilde{u}(x,y) = \rho(x) u(x,y),\quad \tilde{v}(x,y) = \rho(x) v(x,y),\quad \tilde{u}_{0}(y) = \rho(0)u_{0}(y), \end{align*}$

then we find that $(\tilde{u}, \tilde{v})$ satisfies:

$\begin{align} \left\{\begin{aligned} &\tilde{u}\partial_{x}\tilde{u}+\tilde{v}\partial_{y}\tilde{u}-\partial^{2}_{y}\tilde{u}-\frac{\partial_{x}\rho}{\rho}\tilde{u}^{2} = -\rho \partial_{x}P(\rho),\\ &\partial_{x}\tilde{u}+\partial_{y}\tilde{v} = 0,\\ &\tilde{u}|_{x = 0} = \tilde{u}_{0}(y),\quad\lim\limits_{y\to \infty}\tilde{u} = \rho(x)U(x),\\ &\tilde{u}|_{y = 0} = \tilde{v}|_{y = 0} = 0. \end{aligned}\right. \end{align}$

(1.3)

By the von Mises transformation

$\begin{align} x = x, \quad \psi(x,y) = \int_{0}^{y}\tilde{u}(x,z)dz,\quad w = \tilde{u}^{2}, \end{align}$

(1.4)

$\begin{align} \begin{aligned} \partial_{x}\tilde{u} = \frac{\partial_{x}\omega}{2\sqrt{\omega}}+\frac{\partial_{\psi}\omega\partial_{x}\psi}{2\sqrt{\omega}}, \quad \partial_{y}\tilde{u} = \frac{\partial_{\psi}\omega}{2}, \quad \partial_{y}^{2}\tilde{u} = \frac{\sqrt{\omega}\partial_{\psi}^{2}\omega}{2}, \end{aligned} \end{align}$

(1.5)

and (1.3)–(1.5), we know that $w(x, \psi)$ satisfies:

$\begin{align} \partial_{x}w-\sqrt{w}\partial_{\psi}^{2}w-2\frac{\partial_{x}\rho}{\rho}w = -2\rho\partial_{x}P(\rho), \end{align}$

(1.6)

with

$\begin{align} w(x,0) = 0,\quad w(0,\psi) = w_{0}(\psi),\quad \lim\limits_{\psi\to+\infty}w = (\rho(x)U(x))^{2}. \end{align}$

(1.7)

In addition, we have

$\begin{align} 2\partial_{y}\tilde{u} = \partial_{\psi}w,\qquad2\partial_{y}^{2}\tilde{u} = \sqrt{w}\partial_{\psi}^{2}w. \end{align}$

(1.8)

In ^[5], Gong, Guo and Wang studied the existence of the solutions of system (1.1) by using the von Mises transformation and the maximal principle proposed by Oleinik and Samokhin in ^[13]. Specifically, they proved that:

Theorem 1.1. If the initial data $u_{0}$ satisfies the following conditions:

$\begin{align} \begin{aligned} &u\in C^{2,\alpha}_{b}([0,+\infty))(\alpha > 0),\quad u(0) = 0,\quad\partial_{y}u(0) > 0,\quad\partial_{y}u(y)\geq0\quad\mathit{\text{for}}\quad y\in[0,+\infty), \\ &\lim\limits_{y\to+\infty}u(y) = U(0) > 0,\quad\rho^{-1}(0)\partial_{y}^{2}u(y)-\rho^{-1}(0)\partial_{x}P(0) = O(y^{2}) \end{aligned} \end{align}$

(1.9)

and $\rho\in C^{2}([0, X_{0}])$ , then there exists $0 < X\leq X_{0}$ such that system (1.1) admits a solution $u\in C^{1}([0, X)\times \mathbb{R}_{+})$ . The solution has the following properties:

$(i)$ $u$ is continuous and bounded in $[0, X]\times \mathbb{R}_{+}$ ; $\partial_{y}u, \partial_{y}^{2}u$ are continuous and bounded in $[0, X)\times \mathbb{R}_{+}$ ; $v, \partial _{y}v, \partial_{x}u$ are locally bounded in $[0, X)\times \mathbb{R}_{+}$ .

$(ii)$ $u(x, y) > 0$ in $[0, X)\times \mathbb{R}_{+}$ and for any $\bar{x} < X$ , there exists $y_{0}, m > 0$ such that for all $(x, y)\in[0, \bar{x}]\times[0, y_{0}]$ ,

$\partial_{y}u(x,y )\geq m > 0.$

$(iii)$ if $\partial_{x}P\leq0(\partial_{x}\rho\leq0)$ , then

$X = +\infty.$

Remarks 1.2. $u\in C^{2, \alpha}_{b}([0, +\infty))(\alpha > 0)$ means that $u$ is Hölder continuity and bounded.

This theorem shows that under the favorable pressure gradient, the solution is global-in- $x$ . However, if the pressure is an adverse pressure gradient, then boundary layer separation will occur. Xin and Zhang ^[26] studied the global existence of weak solutions of unsteady Prandtl equations under the favorable pressure gradient. For the unsteady compressible Prandtl equation, similar results are obtained in ^[3]. Recently, Xin, Zhang and Zhao ^[27] proposed a direct proof of the existence of global weak solutions of the Prandtl equation. The key content of this paper is that they have studied the uniqueness and regularity of weak solutions. This method can be applied to the compressible Prandtl equation.

Our main results are as follows:

Theorem 1.3. If $u$ is a solution for equation (1.1) in Theorem 1.1, assume $u_{0}$ satisfies the condition (1.9) and the known function $\rho$ and $\partial_{x}P$ are smooth. Then, there exists a constant $C > 0$ depending only on $\varepsilon, X, u_{0}, P(\rho), k, m$ such that for any $(x, y)\in[\varepsilon, X]\times[0, +\infty),$

$\begin{align*} |\partial_{x}^{k}\partial_{y}^{m}u(x,y)|\leq C, \end{align*}$

where $X, \varepsilon$ are positive constants with $\varepsilon < X$ and $m, k$ are any positive integers.

Remarks 1.4. Our methods may be used to other related models. There are similar results for the magnetohydrodynamics boundary layer and the thermal boundary layer. This work will be more difficult due to the influence of temperature and the magnetic field.

Due to the degeneracy near the boundary $\psi = 0$ , the proof of the main result is divided into two parts, Theorem 1.5 and Theorem 1.6. This is similar to the result of the incompressible boundary layer, despite the fluid being compressible and the degeneracy near the boundary. Different from the incompressible case ^[23], we have no divergence-free conditions, which will bring new terms. It is one of the difficulties in this paper to deal with these terms. Now, we will briefly introduce our proof framework. First, we prove the following theorem in the domain $[\varepsilon, X]\times[0, Y_{1}]$ for a small $Y_{1}$ . The key ingredients of proof is that we employ interior priori estimates and the maximum principle developed by Krylov ^[10].

Theorem 1.5. If $u$ is a solution for equation (1.1) in Theorem 1.1, assume $u_{0}$ satisfies the condition (1.9) and the known function $\rho$ and $\partial_{x}P$ are smooth. Then, there exists a small constant $Y_{1} > 0$ and a large constant $C > 0$ depending only on $\varepsilon, X, Y_{1}, u_{0}, P(\rho), k, m$ such that for any $(x, y)\in[\varepsilon, X]\times[0, Y_{1}],$

$\begin{align*} |\partial_{x}^{k}\partial_{y}^{m}u(x,y)|\leq C, \end{align*}$

where $X, \varepsilon$ are positive constants with $\varepsilon < X$ and $m, k$ are any positive integers.

Next, we prove the following theorem in the domain $[\varepsilon, X]\times[Y_{2}, +\infty)$ for a small positive constant $Y_{2}$ . The key of proof is that we prove (1.6) is a uniform parabolic equation in the domain $[\varepsilon, X]\times[Y_{2}, +\infty)$ in Section 4. Once we have (1.6) is a uniform parabolic equation, the global $C^{\infty}$ regularity of the solution is a direct result of interior Schauder estimates and classical parabolic regularity theory. The proof can be given similarly to the steady incompressible boundary layer. For the sake of simplicity of the paper, more details can be found in ^[23] and we omit it here.

Theorem 1.6. If $u$ is a solution for equation (1.1) in Theorem 1.1, assume $u_{0}$ satisfies the condition (1.9) and the known function $\rho$ and $\partial_{x}P$ are smooth. Then, there exists a constant $Y_{0} > 0$ such that for any constant $Y_{2}\in(0, Y_{0})$ , there exists a constant $C > 0$ depending only on $\varepsilon, X, Y_{2}, u_{0}, P(\rho), k, m$ such that for any $(x, y)\in[\varepsilon, X]\times[Y_{2}, +\infty),$

$\begin{align*} |\partial_{x}^{k}\partial_{y}^{m}u(x,y)|\leq C, \end{align*}$

where $X, \varepsilon$ are positive constants with $\varepsilon < X$ and $m, k$ are any positive integers.

Therefore, Theorem 1.3 can be directly proven by combining Theorem 1.5 with Theorem 1.6.

The organization of this paper is as follows. In Section 2, we study lower order and higher order regularity estimates. In Section 3, we prove Theorem 1.5 in the domain near $y = 0$ by transforming back to the original coordinates $(x, y)$ . In Section 4, we prove (1.6) is a uniform parabolic equation by using the maximum principle and we also prove the Theorem 1.3.

2. Lower order and higher order regularity estimates

2.1. Lower order regularity estimates

In this subsection, we study the lower order regularity estimates using the standard interior a priori estimates developed by Krylov ^[10].

Lemma 2.1. If $u$ is a solution for equation (1.1) in Theorem 1.1, assume $u_{0}$ satisfies the condition (1.9)and the known function $\rho$ and $\partial_{x}P$ are smooth. Assume $0 < \varepsilon < X$ , then there exists some positive constants $\delta_{1} > 0$ and $C$ independent of $\psi$ such that for any $(x, \psi)\in[\varepsilon, X]\times[0, \delta_{1}],$

$\begin{align*} |\partial_{x}w(x,\psi)|\leq C\psi. \end{align*}$

Proof. Due to Lemma 2.1 in ^[5] (or Theorem 2.1.14 in ^[13]), there exists $\delta_{1} > 0$ for any $(x, \psi)\in[0, X]\times[0, \delta_{1}]$ , such that for some $\alpha\in(0, \frac{1}{2})$ and positive constants $m, M$ (we assume $\delta_{1} < 1$ ),

$\begin{align} |\partial_{x}w|\leq C\psi^{\frac{1}{2}+\alpha},\quad 0 < m < \partial_{\psi}w < M,\quad m\psi < w < M\psi. \end{align}$

(2.1)

By (1.6), we obtain

$\begin{align*} \partial_{x} \partial_{x} w-\sqrt{w} \partial_{\psi}^{2} \partial_{x} w = \frac{\left(\partial_{x} w\right)^{2}}{2 w}+2 \frac{\rho\partial_{x}P \partial_{x}w }{2 w}+\frac{\partial_{x}\rho}{\rho}\partial_{x}w+2\partial_{x}\left(\frac{\partial_{x}\rho}{\rho}\right)w-2 \partial_{x}[\rho\partial_{x}P]. \end{align*}$

Take a smooth cutoff function $0 \leq \phi(x) \leq 1$ in $[0, X]$ such that

$\begin{align*} \phi(x) = 1, x \in [\varepsilon,X],\quad \phi(x) = 0, x \in[0,\frac{\varepsilon}{2}], \end{align*}$

then

$\begin{align*} \begin{aligned} \partial_{x}\left[\partial_{x} w \phi(x)\right]&-\sqrt{w} \partial_{\psi}^{2}\left[\partial_{x} w \phi(x)\right]\\ & = \frac{\left(\partial_{x} w\right)^{2}}{2 w} \phi(x)+2 \frac{\rho\partial_{x}P \partial_{x}w }{2 w}\phi(x)+\frac{\partial_{x}\rho}{\rho}\partial_{x}w\phi(x)\\ &+2\partial_{x}\left(\frac{\partial_{x}\rho}{\rho}\right)w\phi(x) -2 \partial_{x}(\rho\partial_{x}P)\phi(x)+\partial_{x} w \partial_{x} \phi(x) : = \mathcal{W}. \end{aligned} \end{align*}$

Combining with (2.1), we know

$\begin{align} |\mathcal{W}| \leq C \psi^{2 \alpha}+C \psi^{\alpha-\frac{1}{2}}+C\psi^{\alpha+\frac{1}{2}}+C\psi+C \leq C \psi^{\alpha-\frac{1}{2}}. \end{align}$

(2.2)

We take $\varphi(\psi) = \mu_{1} \psi-\mu_{2} \psi^{1+\beta}$ with constants $\mu_{1}, \mu_{2}$ , then by (2.1) and (2.2), we get

$\begin{align*} \begin{aligned} \partial_{x}\left[\partial_{x} w \phi(x)-\varphi\right]-\sqrt{w} \partial_{\psi}^{2}\left[\partial_{x} w \phi(x)-\varphi\right] & \leq|\mathcal{W}|-\mu_{2} \sqrt{w} \beta(1+\beta) \psi^{\beta-1} \\ & \leq C \psi^{\alpha-\frac{1}{2}}-\mu_{2} \sqrt{m} \beta(1+\beta) \psi^{\beta-\frac{1}{2}}. \end{aligned} \end{align*}$

By taking $\mu_{2}$ sufficiently large and $\alpha = \beta$ , for $(x, \psi)\in(0, X] \times\left(0, \delta_{1}\right)$ , we have

$\begin{align*} \partial_{x}\left[\partial_{x} w \phi(x)-\varphi\right]-\sqrt{w} \partial_{\psi}^{2}\left[\partial_{x} w \phi(x)-\varphi\right] < 0. \end{align*}$

For any $\psi\in\left[0, \delta_{1}\right]$ , let $\mu_{1} \geq \mu_{2}$ , and we have

$\begin{align*} \left(\partial_{x} w \phi-\varphi\right)(0, \psi) \leq 0 , \end{align*}$

and take $\mu_{1}$ large enough depending on $M, \delta_{1}, \mu_{2}$ such that

$\begin{align*} \left(\partial_{x} w \phi-\varphi\right)\left(x, \delta_{1}\right)\leq M \delta_{1}^{\frac{1}{2}+\alpha}-\mu_{1} \delta_{1}+\mu_{2} \delta_{1}^{1+\beta} \leq 0 . \end{align*}$

Since $w(x, 0) = 0$ , we know that for any $x\in[0, X]$ ,

$\begin{align*} \left(\partial_{x} w \phi-\varphi\right)(x, 0) = 0. \end{align*}$

By the maximum principle, it holds in $[0, X] \times[0, \delta_{1}]$ that

$\begin{align*} \left(\partial_{x} w \phi-\varphi\right)(x, \psi) \leq 0. \end{align*}$

Let $\delta_{1}$ be chosen suitably small, for $(x, \psi)\in[\varepsilon, X] \times[0, \delta_{1}]$ , and we obtain

$\begin{align*} \partial_{x} w(x, \psi) \leq \mu_{1} \psi-\mu_{2} \psi^{1+\beta} \leq \frac{\mu_{1}}{2} \psi. \end{align*}$

Considering $-\partial_{x} w \phi-\varphi$ , the result $-\partial_{x} w \leq \frac{\mu_{1}}{2} \psi$ in $[\varepsilon, X] \times[0, \delta_{1}]$ can be proved similarly. This completes the proof of the lemma.

Lemma 2.2. If $u$ is a solution for equation (1.1) in Theorem 1.1, assume $u_{0}$ satisfies the condition (1.9) and the known function $\rho$ and $\partial_{x}P$ are smooth. Assume $0 < \varepsilon < X$ , then there exists some positive constants $\delta_{2} > 0$ and $C$ independent of $\psi$ such that for any $(x, \psi)\in[\varepsilon, X]\times[0, \delta_{2}],$

$\begin{align*} |\partial_{\psi} \partial_{x} w(x, \psi)| \leq C, \quad|\partial_{x}^{2} w(x, \psi)| \leq C \psi^{-\frac{1}{2}}, \quad|\partial_{\psi}^{2} \partial_{x} w(x, \psi)| \leq C \psi^{-1}. \end{align*}$

Proof. From Lemma 2.1, there exists $\delta_{1} > 0$ such that for any $(x, \psi)\in[\frac{\varepsilon}{2}, X] \times[0, \delta_{1}],$

$\begin{align*} |\partial_{x} w(x, \psi)| \leq C \psi. \end{align*}$

Let $\Psi_{0} = \min \{\frac{2}{3} \delta_{1}, \frac{\varepsilon}{2}\}$ , for any $(x_{0}, \psi_{0}) \in[\varepsilon, X] \times(0, \Psi_{0}]$ , and we denote

$\begin{align*} \Omega = \bigl\{(x,\psi)|x_{0}-\psi_{0}^{\frac{3}{2}} \leq x \leq x_{0},\frac{1}{2} \psi_{0} \leq \psi \leq \frac{3}{2} \psi_{0}\bigr\}. \end{align*}$

By the definition of $\Psi_{0}$ , we know $\Omega\subseteq[\frac{\varepsilon}{2}, X] \times[0, \delta_{1}]$ , then it holds in $\Omega$ that

$\begin{align} |\partial_{x} w| \leq C \psi. \end{align}$

(2.3)

The following transformation $f$ is defined:

$\begin{align*} \begin{aligned} \Omega \rightarrow \widetilde{\Omega}: = [-1,0]_{\tilde{x}} \times[-\frac{1}{2}, \frac{1}{2}]_{\tilde{\psi}}, \quad (x, \psi) \mapsto(\tilde{x}, \tilde{\psi}), \end{aligned} \end{align*}$

where $x-x_{0} = \psi_{0}^{\frac{3}{2}} \tilde{x}, \psi-\psi_{0} = \psi_{0} \tilde{\psi}$ .

Since $\partial_{\tilde{x}} = \psi_{0}^{\frac{3}{2}}\partial_{x}, \partial_{\tilde{\psi}} = \psi_{0} \partial_{\psi}$ , it holds in $\Omega$ that

$\begin{align*} \partial_{\tilde{x}}\left(\psi_{0}^{-1} w\right)-\psi_{0}^{-\frac{1}{2}} \sqrt{w} \partial_{\tilde{\psi}}^{2}\left(\psi_{0}^{-1} w\right)-2\frac{\partial_{\tilde{x}}\rho}{\rho}(\psi_{0}^{-1}w) = -2 \rho\partial_{\tilde{x}}P \psi_{0}^{-1} . \end{align*}$

Combining with (2.1), we get $0 < c \leq\psi_{0}^{-\frac{1}{2}} \sqrt{w} \leq C, |\psi_{0}^{-1} w| \leq C$ , and for any $\widetilde{z}_{1}, \widetilde{z}_{2} \in \widetilde{\Omega}$ ,

$\begin{align*} \begin{aligned} |\psi_{0}^{-\frac{1}{2}} \sqrt{w}(\tilde{z}_{1})-\psi_{0}^{-\frac{1}{2}} \sqrt{w}(\tilde{z}_{2})| = \psi_{0}^{-\frac{1}{2}} \frac{\left|w\left(\tilde{z}_{1}\right)-w\left(\tilde{z}_{2}\right)\right|}{\sqrt{w}\left(\tilde{z}_{1}\right)+\sqrt{w}\left(\tilde{z}_{2}\right)} \leq C \frac{\psi_{0}\left|\tilde{z}_{1}-\tilde{z}_{2}\right|}{\psi_{0}} = C\left|\tilde{z}_{1}-\tilde{z}_{2}\right|. \end{aligned} \end{align*}$

This means that for any $\alpha \in(0, 1)$ , we have

$\begin{align*} |\psi_{0}^{-\frac{1}{2}}\sqrt{w}|_{\mathcal{C}^{\alpha}(\widetilde{\Omega})} \leq C. \end{align*}$

Since $P$ and $\rho$ are smooth, we have

$\begin{align*} |\rho^{-1}\partial_{\tilde{x}}\rho|_{\mathcal{C}^{0,1}([-1,0]_{\tilde{x}})}+|\rho\partial_{\tilde{x}}P\psi_{0}^{-1}|_{\mathcal{C}^{0,1}([-1,0]_{\tilde{x}})} \leq C . \end{align*}$

By standard interior priori estimates (see Theorem 8.11.1 in ^[10] or Proposition 2.3 in ^[23]), we have

$\begin{align} | w \psi_{0}^{-1}|_{\mathcal{C}^{\alpha}([-\frac{1}{2}, 0]_{\tilde{x}} \times[-\frac{1}{4}, \frac{1}{4}]_{\tilde{\psi}})}+|\partial_{\tilde{\psi}}^{2} w \psi_{0}^{-1}|_{\mathcal{C}^{\alpha}([-\frac{1}{2}, 0]_{\tilde{x}} \times[-\frac{1}{4}, \frac{1}{4}]_{\tilde{\psi}})} \leq C. \end{align}$

(2.4)

Let $f: = \partial_{x} w \psi_{0}^{-1}$ , which satisfies

$\begin{align*} \partial_{\tilde{x}} f-\frac{\sqrt{w}}{\psi_{0}^{\frac{1}{2}}} \partial_{\tilde{\psi}}^{2} f-\frac{\partial_{\tilde{\psi}}^{2} w}{2 \sqrt{w} \psi_{0}^{\frac{1}{2}}} f-2\frac{\partial_{\tilde{x}}\rho}{\rho}f = -2 \partial_{x}[\rho\partial_{\tilde{x}}P] \psi_{0}^{-1}+2\partial_{x}\left(\frac{\partial_{\tilde{x}}\rho}{\rho}\right)(\psi_{0}^{-1}w) . \end{align*}$

By (2.3), we have $|f| \leq C$ in $\widetilde{\Omega}$ . Due to

$\begin{align*} \big|\psi_{0}^{\frac{1}{2}}w^{-\frac{1}{2}}(\tilde{z}_{1})-\psi_{0}^{\frac{1}{2}}w^{-\frac{1}{2}}(\tilde{z}_{2})\big| = \psi_{0}^{\frac{1}{2}} \frac{\left|\frac{w(\tilde{z}_{1})-w(\tilde{z}_{2})}{w(\tilde{z}_{1}) w(\tilde{z}_{2})}\right|}{w^{-\frac{1}{2}}(\tilde{z}_{1})+w^{-\frac{1}{2}}(\tilde{z}_{2})} \leq C\left|\tilde{z}_{1}-\tilde{z}_{2}\right|, \end{align*}$

we have

$\begin{align} \big|\psi_{0}^{\frac{1}{2}}w^{-\frac{1}{2}}\big|_{\mathcal{C}^{\alpha}(\widetilde{\Omega})} \leq C. \end{align}$

(2.5)

Since

$\frac{\partial_{\tilde{\psi}}^{2} w}{2 \sqrt{w} \psi_{0}^{\frac{1}{2}}} = \partial_{\tilde{\psi}}^{2} w \psi_{0}^{-1} \frac{\psi_{0}^{\frac{1}{2}}}{2 \sqrt{w}},$

which along with (2.4) and (2.5) gives

$\begin{align*} \bigg|\frac{\partial_{\tilde{\psi}}^{2} w}{2 \sqrt{w} \psi_{0}^{\frac{1}{2}}}\bigg|_{\mathcal{C}^{\alpha}([-\frac{1}{2}, 0]_{\tilde{x}} \times[-\frac{1}{4}, \frac{1}{4}]_{\tilde{\psi}})} \leq C . \end{align*}$

As before, by (2.4) and the density $\rho$ and $P$ are smooth, via the standard interior a priori estimates, it yield that

$\begin{align*} |\partial_{\tilde{x}} f|_{L^{\infty}([-\frac{1}{4}, 0]_{\tilde{x}} \times[-\frac{1}{8}, \frac{1}{8}]_{\tilde{\psi}})}+|\partial_{\tilde{\psi}} f|_{L^{\infty}([-\frac{1}{4}, 0]_{\tilde{x}} \times[-\frac{1}{8}, \frac{1}{8}]_{\tilde{\psi}})}+|\partial_{\tilde{\psi}}^{2} f|_{L^{\infty}([-\frac{1}{4}, 0]_{\tilde{x}} \times[-\frac{1}{8}, \frac{1}{8}]_{\tilde{\psi}})} \leq C . \end{align*}$

Therefore, we obtain

$\begin{align*} |\partial_{x}^{2} w\left(x_{0}, \psi_{0}\right)| \leq C \psi_{0}^{-\frac{1}{2}}, \quad|\partial_{\psi} \partial_{x} w\left(x_{0}, \psi_{0}\right)| \leq C, \quad|\partial_{\psi}^{2} \partial_{x} w\left(x_{0}, \psi_{0}\right)| \leq C \psi_{0}^{-1}. \end{align*}$

This completes the proof of the lemma.

2.2. Higher order regularity estimates

In this subsection, we study the higher order regularity estimates using the maximum principle. The two main results of this subsection are Lemma 2.3 and Lemma 2.7.

Lemma 2.3. If $u$ is a solution for equation (1.1) in Theorem 1.1, assume $u_{0}$ satisfies the condition (1.9) and the known function $\rho$ and $\partial_{x}P$ are smooth. Assume $0 < \varepsilon < X$ and $k \geq 2$ , then there exists some positive constants $\delta > 0$ and $C$ independent of $\psi$ such that for any $(x, \psi)\in[\varepsilon, X]\times[0, \delta],$

$\begin{align*} |\partial_{x}^{k} w| \leq C \psi, \quad|\partial_{\psi} \partial_{x}^{k} w| \leq C, \quad|\partial_{\psi}^{2} \partial_{x}^{k} w| \leq C \psi^{-1} . \end{align*}$

Proof. By Lemma 2.1 and Lemma 2.2, we may inductively assume that for $0 \leq j \leq k-1$ , there holds that in $\left[\frac{\varepsilon}{2}, X\right] \times\left[0, \delta_{3}\right]$ (assume $\delta_{3}\ll1$ ),

$\begin{align} |\partial_{\psi} \partial_{x}^{j} w| \leq C,\quad|\partial_{\psi}^{2} \partial_{x}^{j} w| \leq C \psi^{-1},\quad|\partial_{x}^{j} w| \leq C \psi,\quad|\partial_{x}^{j} \sqrt{w}| \leq C \psi^{\frac{1}{2}},\quad|\partial_{x}^{k} w| \leq C \psi^{-\frac{1}{2}}. \end{align}$

(2.6)

We will prove that there exists $\delta_{4} < \delta_{3}$ so that in $[\varepsilon, X] \times[0, \delta_{4}]$ ,

$\begin{align} |\partial_{\psi} \partial_{x}^{k} w| \leq C,\quad|\partial_{\psi}^{2} \partial_{x}^{k} w| \leq C \psi^{-1},\quad|\partial_{x}^{k} w| \leq C \psi,\quad|\partial_{x}^{k} \sqrt{w}| \leq C \psi^{\frac{1}{2}},\quad|\partial_{x}^{k+1} w| \leq C \psi^{-\frac{1}{2}}. \end{align}$

(2.7)

The above results are deduced from the following Lemma 2.4, Lemma 2.5 and Lemma 2.6.

Lemma 2.4. If $u$ is a solution for equation (1.1) in Theorem 1.1, assume $u_{0}$ satisfies the condition (1.9) and the known function $\rho$ and $\partial_{x}P$ are smooth. Assume that (2.6) holds, then there is a positive constant $M_{1}$ for any $(x, \psi)\in\left[\frac{7 \varepsilon}{8}, X\right] \times\left[0, \delta_{3}\right]$ and $0 < \beta \ll 1$ ,

$\begin{align*} |\partial_{x}^{k} w| < M_{1} \psi^{1-\beta}, \quad|\partial_{x}^{k} \sqrt{w}| \leq M_{1} \psi^{\frac{1}{2}-\beta}. \end{align*}$

Proof. Take a smooth cutoff function $0 \leq \phi(x) \leq 1$ in $[0, X]$ such that

$\begin{align*} \phi(x) = 1, x \in [\frac{7\varepsilon}{8},X],\quad \phi(x) = 0, x \in[0,\frac{5\varepsilon}{8}]. \end{align*}$

As in ^[23], fix any $h < \frac{\varepsilon}{8}$ . Set

$\Omega = \left\{(x,\psi)|0 < x\leq X, 0 < \psi < \delta_{3}\right\},$

and let

(ⅰ) $f = \frac{\partial_{x}^{k-1} w(x-h, \psi)-\partial_{x}^{k-1} w(x, \psi)}{-h} \phi+M \psi \ln \psi,$ $(x, \psi)\in[\frac{5 \varepsilon}{8}, X]\times [0, +\infty)$ ,

(ⅱ) $f = M \psi \ln \psi,$ $(x, \psi)\in[0, \frac{5 \varepsilon}{8})\times[\psi, +\infty),$

so we get $f(x, 0) = 0$ , $f(0, \psi) \leq 0$ . We know

$f\left(x, \delta_{3}\right) \leq C\left(\delta_{3}\right)^{-\frac{1}{2}}+M \delta_{3} \ln \delta_{3} \leq 0,$

where $M$ is large enough. Then, by choosing the appropriate $M$ , we know that the positive maximum of $f$ cannot be achieved in the interior. Finally, the lemma can be proven by the arbitrariness of $h$ .

Assume that there exists a point

$p_{0} = (x_{0}, \psi_{0}) \in \Omega,$

such that

$f\left(p_{0}\right) = \max \limits_{\bar{\Omega}} f > 0.$

It is easy to know that

$x_{0} > \frac{5 \varepsilon}{8},\qquad \partial_{x}^{k-1} w(x_{0}-h, \psi_{0}) < \partial_{x}^{k-1} w(x_{0}, \psi_{0}).$

By (2.1), denote $\xi = \sqrt{m}$ , we have

$\begin{align} -\sqrt{w} \partial_{\psi}^{2}(M \psi \ln \psi) = -M \sqrt{w} \psi^{-1} \leq-\xi M \psi^{-\frac{1}{2}}. \end{align}$

(2.8)

By (1.6), a direct calculation gives

$\begin{align*} \begin{aligned} \partial_{x} \partial_{x}^{k-1} w-&\sqrt{w} \partial_{\psi}^{2} \partial_{x}^{k-1} w\\ & = -2 \partial_{x}^{k-1}(\rho\partial_{x}P)+\sum\limits_{m = 1}^{k-2} C_{k-1}^{m}\left(\partial_{x}^{k-1-m} \sqrt{w}\right) \partial_{\psi}^{2} \partial_{x}^{m} w+\left(\partial_{x}^{k-1} \sqrt{w}\right) \partial_{\psi}^{2} w \\ &\quad+2\sum\limits_{m = 0}^{k-1} C_{k-1}^{m}\partial_{x}^{k-1-m}\left(\frac{\partial_{x}\rho}{\rho}\right)\partial_{x}^{m}w\\ & = -2 \partial_{x}^{k-1}(\rho\partial_{x}P)+\sum\limits_{m = 1}^{k-2} C_{k-1}^{m}\left(\partial_{x}^{k-1-m} \sqrt{w}\right) \partial_{\psi}^{2} \partial_{x}^{m} w+\frac{\partial_{x}^{k-1} w}{2 \sqrt{w}} \frac{\partial_{x} w}{\sqrt{w}} \\ &\quad+\left(\frac{\partial_{x}^{k-1} w}{2 \sqrt{w}}\right) \frac{2\rho\partial_{x}P}{\sqrt{w}}-\left(\frac{\partial_{x}^{k-1} w}{2 \sqrt{w}}\right)\frac{2\frac{\partial_{x}\rho}{\rho}w}{\sqrt{w}}+2\sum\limits_{m = 0}^{k-1} C_{k-1}^{m}\partial_{x}^{k-1-m}\left(\frac{\partial_{x}\rho}{\rho}\right)\partial_{x}^{m}w\\ &\quad+ \sum\limits_{m = 0}^{k-2} C_{k-2}^{m} \partial_{\psi}^{2} w \partial_{x}^{m+1} w \partial_{x}^{k-2-m} \frac{1}{2 \sqrt{w}}\\ &: = \sum\limits_{i = 1}^{4}I_{i} \end{aligned} \end{align*}$

and

$\begin{align*} \begin{aligned} I_{1} & = -2 \partial_{x}^{k-1}(\rho\partial_{x}P)+\sum\limits_{m = 1}^{k-2} C_{k-1}^{m}\left(\partial_{x}^{k-1-m} \sqrt{w}\right) \partial_{\psi}^{2} \partial_{x}^{m} w+\frac{\partial_{x}^{k-1} w}{2 \sqrt{w}} \frac{\partial_{x} w}{\sqrt{w}}, \\ I_{2} & = \frac{\rho\partial_{x}P}{w}\partial_{x}^{k-1} w, \\ I_{3} & = -\frac{\partial_{x}\rho}{\rho}\partial_{x}^{k-1}w+2\sum\limits_{m = 0}^{k-1} C_{k-1}^{m}\partial_{x}^{k-1-m}\left(\frac{\partial_{x}\rho}{\rho}\right)\partial_{x}^{m}w,\\ I_{4}& = \sum\limits_{m = 0}^{k-2} C_{k-2}^{m} \partial_{\psi}^{2} w \partial_{x}^{m+1} w \partial_{x}^{k-2-m} \frac{1}{2 \sqrt{w}}. \end{aligned} \end{align*}$

For $x \geq \frac{5 \varepsilon}{8}$ , we consider the following equality

$\begin{align} \partial_{x} f_{1}-\sqrt{w\left(p_{1}\right)} \partial_{\psi}^{2} f_{1} = \frac{\sqrt{w(p_{1})}-\sqrt{w(p)}}{-h} \partial_{\psi}^{2} \partial_{x}^{k-1} w(p)+\sum\limits_{i = 1}^{4} \frac{1}{-h}\left(I_{i}\left(p_{1}\right)-I_{i}(p)\right), \end{align}$

(2.9)

where

$f_{1} = \frac{1}{-h}(\partial_{x}^{k-1} w\left(p_{1}\right)-\partial_{x}^{k-1} w(p)),$

with $p_{1} = (x-h, \psi), p = (x, \psi)$ .

For any $x \geq \frac{5 \varepsilon}{8}$ , by (2.6), it is easy to conclude that

$\begin{align} \begin{aligned} &\left|\frac{1}{-h}(\sqrt{w}(p_{1})-\sqrt{w}(p)) \partial_{\psi}^{2} \partial_{x}^{k-1} w(p)\right| \leq C \psi^{-\frac{1}{2}}, \\ &\left|\frac{1}{-h}(I_{1}(p_{1})-I_{1}(p))\right| \leq C \psi^{-\frac{1}{2}}, \\ &\left|\sum\limits_{i = 3}^{4}\frac{1}{-h}(I_{i}(p_{1})-I_{i }(p))\right| \leq C \psi^{-\frac{1}{2}}, \end{aligned} \end{align}$

(2.10)

where $C$ is dependent on the parameter $h$ .

Since

$\begin{align*} \frac{1}{-h}(I_{2}(p_{1})-I_{2}(p)) = f_{1} \cdot\big[\frac{\rho\partial_{x}P}{w} (p_{1})\big]+\partial_{x}^{k-1} w(p) \frac{1}{-h}\big[\frac{\rho\partial_{x}P}{w} (p_{1})-\frac{\rho\partial_{x}P}{w} (p)\big], \end{align*}$

combining with (2.6), $f_{1}(p_{0}) > 0$ and $\partial_{x}P\leq 0$ , it holds at $p = p_{0}$ that

$\begin{align} \frac{1}{-h}(I_{2}\left(p_{1}\right)-I_{2}(p_{0})) \leq C . \end{align}$

(2.11)

Summing up (2.10) and (2.11), we conclude that at $p = p_{0}$ ,

$\begin{align*} \partial_{x} f_{1}-\sqrt{w} \partial_{\psi}^{2} f_{1} \leq C_{0} \psi^{-\frac{1}{2}} . \end{align*}$

This along with (2.8) shows that for $x \geq \frac{5 \varepsilon}{8}$ , it holds at $p = p_{0}$ that

$\begin{align} \partial_{x} f-\sqrt{w} \partial_{\psi}^{2} f \leq C \psi^{-\frac{1}{2}}-\xi M \psi^{-\frac{1}{2}} . \end{align}$

(2.12)

By taking $M$ large enough, we have $\partial_{x} f\left(p_{0}\right)-\sqrt{w} \partial_{\psi}^{2} f\left(p_{0}\right) < 0$ . By the definition of $p_{0}$ , we obtain

$\begin{align*} \partial_{x} f\left(p_{0}\right)-\sqrt{w} \partial_{\psi}^{2} f\left(p_{0}\right) \geq 0, \end{align*}$

which leads to a contradiction. Therefore, for $M$ chosen as above and independent of $h$ , we have

$\max\limits _{\bar{\Omega}} f \leq 0.$

We can similarly prove that $\min _{\bar{\Omega}} f \geq 0$ by replacing $M \psi \ln \psi$ in $f$ with $-M \psi \ln \psi$ . By the arbitrariness of $h$ , for any $(x, \psi)\in(\frac{7\varepsilon}{8}, X] \times(0, \delta_{3}]$ we have

$\begin{align*} |\partial_{x}^{k} w| \leq-M \psi \ln \psi. \end{align*}$

Due to

$\begin{align} 2 \sqrt{w} \partial_{x}^{k} \sqrt{w}+\sum\limits_{m = 1}^{k-1} C_{k}^{m}(\partial_{x}^{m} \sqrt{w} \partial_{x}^{k-m} \sqrt{w}) = \partial_{x}^{k}(\sqrt{w} \sqrt{w}) = \partial_{x}^{k} w, \end{align}$

(2.13)

which along with (2.6) shows that in $(\frac{7}{8} \varepsilon, X] \times(0, \delta_{3}]$ ,

$\begin{align*} |\sqrt{w} \partial_{x}^{k} \sqrt{w}| \leq-C \psi \ln \psi . \end{align*}$

Lemma 2.5. If $u$ is a solution for equation (1.1) in Theorem 1.1, assume $u_{0}$ satisfies the condition (1.9) and the known function $\rho$ and $\partial_{x}P$ are smooth. Assume that (2.6) holds, then for any $(x, \psi)\in[\frac{15}{16} \varepsilon, X] \times[0, \delta_{3}]$ ,

$\begin{align*} |\partial_{x}^{k} w| \leq C \psi, \quad|\partial_{x}^{k} \sqrt{w}| \leq C \psi^{\frac{1}{2}} . \end{align*}$

Proof. Take a smooth cutoff function $\phi(x)$ so that

$\begin{align*} \phi(x) = 1, x \in [\frac{15\varepsilon}{16},X],\quad \phi(x) = 0, x \in[0,\frac{7\varepsilon}{8}]. \end{align*}$

Set

$f = \partial_{x}^{k} w \phi-\mu_{1} \psi+\mu_{2} \psi^{\frac{3}{2}-\beta}$

with constants $\mu_{1}, \mu_{2}$ . Let $\beta$ be small enough in Lemma 2.4. Then it holds in $[\frac{7 \varepsilon}{8}, X] \times[0, \delta_{3}]$ that

$\begin{align} |\partial_{x}^{k} w| \leq C \psi^{1-\beta}, \quad|\partial_{x}^{k} \sqrt{w}| \leq C \psi^{\frac{1}{2}-\beta}. \end{align}$

(2.14)

We denote

$\Omega = \left\{(x,\psi)|0 < x\leq X ,0 < \psi < \delta_{3}\right\}.$

As in ^[23], we have $f(x, 0) = 0$ , $f(0, \psi) \leq 0$ and $f(x, \delta_{3}) \leq 0$ by taking $\mu_{1}$ large depending on $\mu_{2}$ . We claim that the maximum of $f$ cannot be achieved in the interior.

By (1.6), we have

$\begin{align*} \begin{aligned} \partial_{x} \partial_{x}^{k} w-&\sqrt{w} \partial_{\psi}^{2} \partial_{x}^{k} w\\ & = -2 \partial_{x}^{k}(\rho\partial_{x}P)+\sum\limits_{m = 0}^{k-1} C_{k}^{m}(\partial_{x}^{k-m} \sqrt{w}) \partial_{\psi}^{2} \partial_{x}^{m}w +2\sum\limits_{m = 0}^{k} C_{k}^{m}\partial_{x}^{k-m}\left(\frac{\partial_{x}\rho}{\rho}\right)\partial_{x}^{m}w, \end{aligned} \end{align*}$

and

$\begin{align*} \partial_{\psi}^{2} \partial_{x}^{m} w = \partial_{x}^{m} \partial_{\psi}^{2} w = \partial_{x}^{m}\left(\frac{\partial_{x} w}{\sqrt{w}}+\frac{2\rho\partial_{x}P}{\sqrt{w}}-\frac{2\partial_{x}\rho}{\rho}\sqrt{w} \right) . \end{align*}$

For any $x \geq \frac{7 \varepsilon}{8}$ , $0 \leq j \leq k-1$ and $0 \leq m \leq k-1$ , from (2.6) and (2.14), we get

$\begin{align*} |\partial_{x}^{j} w| \leq C \psi, \quad|\partial_{x}^{k} w| \leq C \psi^{1-\beta},\quad |\partial_{x}^{k-m} \sqrt{w}| \leq C \psi^{\frac{1}{2}-\beta}. \end{align*}$

Then let $\beta\ll\frac{1}{2}$ , for $0 \leq m \leq k-1$ and $x \geq \frac{7 \varepsilon}{8}$ , we obtain

$\begin{align*} |\partial_{\psi}^{2} \partial_{x}^{m} w| \leq C \psi^{\frac{1}{2}-\beta}+C \psi^{-\frac{1}{2}}+C \psi^{\frac{1}{2}-\beta}\leq C \psi^{-\frac{1}{2}}. \end{align*}$

Therefore, we conclude that for $x \geq \frac{7 \varepsilon}{8}$ ,

$\begin{align*} \partial_{x} \partial_{x}^{k} w-\sqrt{w} \partial_{\psi}^{2} \partial_{x}^{k} w \leq C+C \psi^{-\beta}+C\psi^{1-\beta}\leq C \psi^{-\beta}. \end{align*}$

By the above inequality and (2.1), it holds at $p = p_{0}$ that

$\begin{align*} \begin{aligned} \partial_{x} f-\sqrt{w} \partial_{\psi}^{2} f& = \partial_{x} \partial_{x}^{k} w-\sqrt{w} \partial_{\psi}^{2} \partial_{x}^{k} w+\partial_{x}^{k}w\partial_{x}\phi-\sqrt{w} \partial_{\psi}^{2}(-\mu_{1} \psi+\mu_{2} \psi^{\frac{3}{2}-\beta})\\& \leq C_{2} \psi^{-\beta}-\xi \mu_{2} \psi^{-\beta}, \end{aligned} \end{align*}$

where $\xi = \left(\frac{3}{2}-\beta\right)\left(\frac{1}{2}-\beta\right) \sqrt{m} > 0$ . Then we have $\partial_{x} f-\sqrt{w} \partial_{\psi}^{2} f < 0$ in $\Omega$ by taking $\mu_{2}$ large depending on $C_{2}$ . This means that the maximum of $f$ cannot be achieved in the interior. Therefore, we have

$\max \limits_{\bar{\Omega}} f \leq 0.$

In the same way, we can prove that

$\max\limits _{\bar{\Omega}}-\partial_{x}^{k} w \phi-\mu_{1} \psi+\mu_{2} \psi^{\frac{3}{2}-\beta} \leq 0.$

So, for any $(x, \psi)\in[\frac{15}{16} \varepsilon, X] \times[0, \delta_{3}]$ , we have

$\begin{align*} |\partial_{x}^{k} w| \leq \mu_{1} \psi-\mu_{2} \psi^{\frac{3}{2}-\beta} \leq \mu_{1} \psi. \end{align*}$

Combining with (2.6) and (2.13), it holds in $[\frac{15}{16} \varepsilon, X] \times[0, \delta_{3}]$ that

$\begin{align*} |\partial_{x}^{k} \sqrt{w}| \leq C \psi^{\frac{1}{2}}. \end{align*}$

This completes the proof of the lemma.

Lemma 2.6. If $u$ is a solution for equation (1.1) in Theorem 1.1, assume $u_{0}$ satisfies the condition (1.9) and the known function $\rho$ and $\partial_{x}P$ are smooth. Assume that (2.6) holds, then for any $(x, \psi)\in[\varepsilon, X] \times[0, \delta_{4}]$ ,

$\begin{align*} |\partial_{\psi} \partial_{x}^{k} w| \leq C, \quad|\partial_{\psi}^{2} \partial_{x}^{k} w| \leq C \psi^{-1}, \quad|\partial_{x}^{k+1} w| \leq C \psi^{-\frac{1}{2}}. \end{align*}$

Proof. By Lemma 2.5 and (2.6), for any $(x, \psi)\in[\frac{15}{16} \varepsilon, X] \times[0, \delta_{3}]$ ,

$\begin{align} |\partial_{x}^{j} w| \leq C \psi, \quad|\partial_{x}^{j} \sqrt{w}| \leq C \psi^{\frac{1}{2}},\quad 0 \leq j \leq k. \end{align}$

(2.15)

Set $\Psi_{0} = \min \{\frac{2}{3} \delta_{3}, \frac{\varepsilon}{16}\}$ , for $(x_{0}, \psi_{0}) \in[\varepsilon, X] \times(0, \Psi_{0}]$ , we denote

$\begin{align*} \Omega = \bigl\{(x,\psi)|x_{0}-\psi_{0}^{\frac{3}{2}} \leq x \leq x_{0},\frac{1}{2} \psi_{0} \leq \psi \leq \frac{3}{2} \psi_{0}\bigr\}. \end{align*}$

A direct calculation gives

$\begin{align*} \begin{aligned} \partial_{x} \partial_{x}^{k} w-\sqrt{w} \partial_{\psi}^{2} \partial_{x}^{k} w = &-2 \partial_{x}^{k}(\rho\partial_{x}P)+\partial_{x}^{k} \sqrt{w} \partial_{\psi}^{2} w+\sum\limits_{m = 1}^{k-2} C_{k}^{m}\left(\partial_{x}^{k-m} \sqrt{w}\right) \partial_{\psi}^{2} \partial_{x}^{m} w \\ &+C_{k}^{k-1} \frac{\partial_{x} w}{2 \sqrt{w}} \partial_{\psi}^{2} \partial_{x}^{k-1} w+2\sum\limits_{m = 0}^{k} C_{k}^{m}\partial_{x}^{k-m}\left(\frac{\partial_{x}\rho}{\rho}\right)\partial_{x}^{m}w. \end{aligned} \end{align*}$

By (1.6), we obtain

$\begin{align*} \begin{aligned} \partial_{\psi}^{2} \partial_{x}^{m} w & = \partial_{x}^{m} \partial_{\psi}^{2} w\\ & = \partial_{x}^{m}\left(\frac{\partial_{x} w}{\sqrt{w}}+\frac{2\rho\partial_{x}P}{\sqrt{w}}-2\frac{\partial_{x}\rho}{\rho}\sqrt{w}\right) \\ & = \frac{\partial_{x}^{m+1} w}{\sqrt{w}}+\sum\limits_{l = 1}^{m} C_{m}^{l} \partial_{x}^{m-l+1} w \partial_{x}^{l} \frac{1}{\sqrt{w}}+\partial_{x}^{m}\left(\frac{2\rho\partial_{x}P}{\sqrt{w}}\right)-\partial_{x}^{m}\left(2\frac{\partial_{x}\rho}{\rho}\sqrt{w}\right), \end{aligned} \end{align*}$

and

$\begin{align*} \partial_{x}^{k} \sqrt{w} = \partial_{x}^{k-1} \frac{\partial_{x} w}{2 \sqrt{w}} = \frac{\partial_{x}^{k} w}{2 \sqrt{w}}+\sum\limits_{l = 1}^{k-1} C_{k-1}^{l} \partial_{x}^{k-1-l+1} w \partial_{x}^{l} \frac{1}{2 \sqrt{w}}, \end{align*}$

then

$\begin{align*} \begin{aligned} \partial_{x} \partial_{x}^{k} w-&\sqrt{w} \partial_{\psi}^{2} \partial_{x}^{k} w\\ = &-2 \partial_{x}^{k}(\rho\partial_{x}P)+\sum\limits_{m = 1}^{k-2} C_{k}^{m} (\partial_{x}^{k-m} \sqrt{w}) \partial_{\psi}^{2} \partial_{x}^{m} w \\ &+\frac{\partial_{x}^{k} w}{2 \sqrt{w}} \partial_{\psi}^{2} w+\sum\limits_{l = 1}^{k-1} C_{k-1}^{l} \partial_{x}^{k-1-l+1} w\partial_{x}^{l} \left(\frac{1}{2 \sqrt{w}}\right) \partial_{\psi}^{2} w \\ &+C_{k}^{k-1} \frac{\partial_{x} w \partial_{x}^{k} w}{2 w}+2\sum\limits_{m = 0}^{k} C_{k}^{m}\partial_{x}^{k-m}\left(\frac{\partial_{x}\rho}{\rho}\right)\partial_{x}^{m}w\\ &+C_{k}^{k-1} \frac{\partial_{x} w}{2 \sqrt{w}}\left[\sum\limits_{l = 1}^{k-1} C_{k-1}^{l} \partial_{x}^{k-l} w \partial_{x}^{l} \frac{1}{\sqrt{w}}+\partial_{x}^{k-1}\left(\frac{2\rho\partial_{x}P}{\sqrt{w}} \right)-\partial_{x}^{k-1}\left(2\frac{\partial_{x}\rho}{\rho}\sqrt{w}\right)\right]. \end{aligned} \end{align*}$

The following transformation $f$ is defined:

where $x-x_{0} = \psi_{0}^{\frac{3}{2}} \tilde{x}, \psi-\psi_{0} = \psi_{0} \tilde{\psi}$ .

Let $f = \partial_{x}^{k} w \psi_{0}^{-1}$ , we get

$\begin{align*} \begin{aligned} \partial_{\tilde{x}} f-&\frac{\sqrt{w}}{\psi_{0}^{\frac{1}{2}}} \partial_{\tilde{\psi}}^{2} f-\frac{1}{2 \sqrt{w}} \partial_{\psi}^{2} w \psi_{0}^{\frac{3}{2}}f-\frac{\partial_{x} w}{2 w} \psi_{0}^{\frac{3}{2}} f\\ & = -2\psi_{0}^{\frac{1}{2}} \partial_{x}^{k}(\rho\partial_{x}P)+\psi_{0}^{\frac{1}{2}}\sum\limits_{m = 1}^{k-2} C_{k}^{m} (\partial_{x}^{k-m} \sqrt{w}) \partial_{\psi}^{2} \partial_{x}^{m} w \\ &\quad+\psi_{0}^{\frac{1}{2}}\sum\limits_{l = 1}^{k-1} C_{k-1}^{l} \partial_{x}^{k-l} w\left(\partial_{x}^{l} \frac{1}{2 \sqrt{w}}\right) \partial_{\psi}^{2} w \\ &\quad+2\psi_{0}^{\frac{1}{2}}\sum\limits_{m = 0}^{k} C_{k}^{m}\partial_{x}^{k-m}\left(\frac{\partial_{x}\rho}{\rho}\right)\partial_{x}^{m}w\\ &\quad+\psi_{0}^{\frac{1}{2}}\frac{\partial_{x} w}{2 \sqrt{w}}\left[\sum\limits_{l = 1}^{k-1} C_{k-1}^{l} \partial_{x}^{k-l} w \partial_{x}^{l} \frac{1}{\sqrt{w}}+\partial_{x}^{k-1}\left(\frac{2\rho\partial_{x}P}{\sqrt{w}} \right)-\partial_{x}^{k-1}\left(2\frac{\partial_{x}\rho}{\rho}\sqrt{w}\right)\right]\\ &: = F. \end{aligned} \end{align*}$

From the proof of Lemma 2.2 and Lemma 2.6, we know that in $\widetilde{\Omega}$ for $\alpha \in(0, 1)$ ,

$\begin{align*} |f|\leq C, \quad 0 < c \leq \psi_{0}^{-\frac{1}{2}}\sqrt{w} \leq C, \quad|\psi_{0}^{-\frac{1}{2}}\sqrt{w}|_{\mathcal{C}^{\alpha}(\widetilde{\Omega})} \leq C . \end{align*}$

By (2.6), (2.15) and the equality

$\begin{align*} \begin{aligned} \partial_{\psi}\left(\partial_{\psi}^{2} \partial_{x}^{m} w\right) = & \frac{\partial_{\psi} \partial_{x}^{m+1} w}{\sqrt{w}}-\frac{\partial_{\psi} w \partial_{x}^{m+1} w}{2(\sqrt{w})^{3}}+\sum\limits_{l = 1}^{m} C_{m}^{l} \partial_{x}^{m-l+1} \partial_{\psi} w \partial_{x}^{l} \frac{1}{\sqrt{w}} \\ &+\sum\limits_{l = 1}^{m} C_{m}^{l} \partial_{x}^{m-l+1} w \partial_{x}^{l} \frac{\partial_{\psi} w}{-2(\sqrt{w})^{3}}+\partial_{x}^{m}\left(\frac{\rho\partial_{x}P\partial_{\psi} w}{-(\sqrt{w})^{3}} \right)-\partial_{x}^{m}\left(\frac{\partial_{x}\rho}{\rho}\frac{\partial_{\psi}w}{\sqrt{w}}\right), \end{aligned} \end{align*}$

we can conclude that for $j \leq k-1$ and $m \leq k-2$ ,

$\begin{align*} \big|\nabla_{\tilde{x}, \tilde{\psi}} \partial_{x}^{j} \sqrt{w}\big| \leq C \psi_{0}^{\frac{1}{2}}, \quad\big|\nabla_{\tilde{x}, \tilde{\psi}} \partial_{x}^{j}\big(\frac{1}{\sqrt{w}}\big)\big| \leq C \psi_{0}^{-\frac{1}{2}}, \quad\big|\nabla_{\tilde{x}, \tilde{\psi}} \partial_{\psi}^{2} \partial_{x}^{m} w\big | \leq C \psi_{0}^{-\frac{1}{2}}. \end{align*}$

Combining (2.4) with (2.5), we can obtain

$\begin{align*} |\frac{1}{2 \sqrt{w}} \partial_{\psi}^{2} w \psi_{0}^{\frac{3}{2}}+\frac{\partial_{x} w}{2 w} \psi_{0}^{\frac{3}{2}}|_{\mathcal{C}^{\alpha}(\widetilde{\Omega})}+|F|_{\mathcal{C}^{\alpha}(\widetilde{\Omega})} \leq C . \end{align*}$

By the standard interior priori estimates, we obtain

Therefore, this means that

$\begin{align*} |\partial_{x}^{k+1} w\left(x_{0}, \psi_{0}\right)| \leq C \psi_{0}^{-\frac{1}{2}}, \quad|\partial_{\psi} \partial_{x}^{k} w\left(x_{0}, \psi_{0}\right)| \leq C, \quad|\partial_{\psi}^{2} \partial_{x}^{k} w\left(x_{0}, \psi_{0}\right)| \leq C \psi_{0}^{-1} . \end{align*}$

Since $\left(x_{0}, \psi_{0}\right)$ is arbitrary, this completes the proof of the lemma.

Lemma 2.7. If $u$ is a solution for equation (1.1) in Theorem 1.1, assume $u_{0}$ satisfies the condition (1.9) and the known function $\rho$ and $\partial_{x}P$ are smooth. Assume $0 < \varepsilon < X$ and integer $m, k \geq 0$ , then there exists a positive constant $\delta > 0$ such that for any $(x, \psi)\in[\varepsilon, X]\times[0, \delta],$

$\begin{align} |\partial_{\psi}^{m} \partial_{x}^{k} w| \leq C \psi^{1-m}. \end{align}$

(2.16)

Proof. From Lemma 2.1, (2.1), Lemma 2.2 and Lemma 2.3, a direct calculation can prove that

$\begin{align*} \big|\partial_{x}^{k} \frac{1}{\sqrt{w}}\big| \leq C \psi^{-\frac{1}{2}}, \quad\big|\partial_{x}^{k} \partial_{\psi} \frac{1}{\sqrt{w}}\big| \leq C \psi^{-\frac{3}{2}}, \quad\big|\partial_{x}^{k} \partial_{\psi}^{2} \frac{1}{\sqrt{w}}\big| \leq C \psi^{-\frac{5}{2}} , \end{align*}$

and (2.16) holds for $m = 0, 1, 2$ . Then for $0 \leq m \leq j$ with $j \geq 1$ , we inductively assume that

$\begin{align} |\partial_{\psi}^{m} \partial_{x}^{k} w| \leq C \psi^{1-m},\quad \big|\partial_{x}^{k} \partial_{\psi}^{m} \frac{1}{\sqrt{w}}\big| \leq C \psi^{-\frac{1}{2}-m}. \end{align}$

(2.17)

In the next part, we will prove that (2.17) still holds for $m = j+1$ .

By (1.6), we obtain

$\begin{align*} \begin{aligned} \partial_{\psi}^{j+1} \partial_{x}^{k} w & = \partial_{\psi}^{j-1} \partial_{x}^{k} \partial_{\psi}^{2} w\\& = \partial_{x}^{k} \partial_{\psi}^{j-1}\left(\frac{\partial_{x} w}{\sqrt{w}}+\frac{2\rho\partial_{x}P}{\sqrt{w}} -2\frac{\partial_{x}\rho}{\rho}\frac{w}{\sqrt{w}}\right) \\ & = \partial_{x}^{k}\left(\sum\limits_{i = 0}^{j-1} C_{j-1}^{i} \partial_{\psi}^{j-1-i} \partial_{x} w \partial_{\psi}^{i} \frac{1}{\sqrt{w}}+2 \rho\partial_{x}P \partial_{\psi}^{j-1} \frac{1}{\sqrt{w}}-2\frac{\partial_{x}\rho}{\rho} \sum\limits_{i = 0}^{j-1} C_{j-1}^{i} \partial_{\psi}^{j-1-i} w \partial_{\psi}^{i} \frac{1}{\sqrt{w}}\right). \end{aligned} \end{align*}$

Combining with (2.17), we get

$\begin{align} |\partial_{\psi}^{j+1} \partial_{x}^{k} w| \leq C \psi^{\frac{3}{2}-j}+ C \psi^{\frac{1}{2}-j}+ C \psi^{\frac{3}{2}-j}\leq C \psi^{\frac{1}{2}-j} . \end{align}$

(2.18)

By straight calculations, we get

$\begin{align*} \begin{aligned} 0& = \partial_{x}^{k} \partial_{\psi}^{j+1}\bigg(\frac{1}{\sqrt{w}} \frac{1}{\sqrt{w}} w\bigg) \\ & = \partial_{x}^{k}\bigg[2 \sqrt{w} \partial_{\psi}^{j+1} \frac{1}{\sqrt{w}}+\sum\limits_{i = 1}^{j} \sum\limits_{l = 0}^{j+1-i} C_{j+1}^{i} C_{j+1-i}^{l}\left(\partial_{\psi}^{i} \frac{1}{\sqrt{w}}\right)\left(\partial_{\psi}^{l} \frac{1}{\sqrt{w}}\right) \partial_{\psi}^{j+1-l-i} w\\ &\qquad\qquad\qquad\qquad\qquad\qquad\qquad\qquad\quad +\sum\limits_{l = 0}^{j} C_{j+1}^{l} \frac{1}{\sqrt{w}}\left(\partial_{\psi}^{l} \frac{1}{\sqrt{w}}\right) \partial_{\psi}^{j+1-l} w\bigg]. \end{aligned} \end{align*}$

Combining the above equality with (2.17), we can conclude that

$\begin{align*} \big|\partial_{x}^{k} \partial_{\psi}^{j+1} \frac{1}{\sqrt{w}}\big| \leq C \psi^{-\frac{3}{2}-j}. \end{align*}$

This completes the proof of the lemma.

3. Proof of Theorem 1.5

In this section, we will prove the regularity of the solution $u$ in the domain

$\left\{(x,\psi)|\varepsilon\leq x\leq X, 0\leq y \leq Y_{1}\right\}.$

Proof of Theorem 1.5:

Proof. For the convenience of proof, we denote

$\begin{align*} (\tilde{x}, \psi) = \left(x, \int_{0}^{y} \tilde{u} d y\right) . \end{align*}$

A direct calculation gives (see P13 in ^[23])

$\begin{align*} \begin{aligned} \partial_{y} = \sqrt{w} \partial_{\psi}, \quad \partial_{x} = \partial_{\tilde{x}}+\partial_{x} \psi(x, y) \partial_{\psi}, \quad \partial_{x} \psi = \frac{1}{2} \sqrt{w} \int_{0}^{\psi} w^{-\frac{3}{2}} \partial_{\tilde{x}} w d \psi . \end{aligned} \end{align*}$

By (2.1) and Lemma 2.3, we have $|\partial_{x} \psi| \leq C \psi$ . Due to $\partial_{y} = \sqrt{w} \partial_{\psi}$ , we obtain

$\begin{align*} \begin{aligned} \partial_{x}^{k} 2 \partial_{y} \tilde{u} & = \left(\partial_{\tilde{x}}+\partial_{x} \psi \partial_{\psi}\right)^{k} \partial_{\psi} w, \\ \partial_{x}^{k} 2 \partial_{y}^{2} \tilde{u} & = \left(\partial_{\tilde{x}}+\partial_{x} \psi \partial_{\psi}\right)^{k}\left(\partial_{\tilde{x}} w+2 \rho\partial_{x}P-2\frac{\partial_{x}\rho}{\rho}w\right) \\ & = \left(\partial_{\tilde{x}}+\partial_{x} \psi \partial_{\psi}\right)^{k}\left(\partial_{\tilde{x}} w\right)+2 \partial_{\tilde{x}}^{k}(\rho\partial_{x}P)-2\left(\frac{\partial_{x}\rho}{\rho}\right)(\partial_{\tilde{x}}+\partial_{x} \psi \partial_{\psi})^{k}w-2\partial_{\tilde{x}}^{k}\left(\frac{\partial_{x}\rho}{\rho}\right)w. \end{aligned} \end{align*}$

By $|\partial_{x} \psi| \leq C \psi$ and Lemma 2.7, we obtain that Theorem 1.5 holds for $m = 0, 1, 2,$

$\begin{align} |\partial_{x}^{k} \partial_{y} \tilde{u}|+|\partial_{x}^{k} \partial_{y}^{2} \tilde{u}| \leq C . \end{align}$

(3.1)

We inductively assume that for any integer $k$ and $m \geq 1$ ,

$\begin{align} |\partial_{x}^{k} \partial_{y}^{j}\tilde{u}| \leq C, \quad j \leq m . \end{align}$

(3.2)

A direct calculation gives

$\begin{align*} \begin{aligned} &\partial_{x}^{k} \partial_{y}^{m+1} \tilde{u} \\ & = \partial_{x}^{k} \partial_{y}^{m-1} \partial_{y}^{2} \tilde{u}\\ & = \partial_{x}^{k} \partial_{y}^{m-1}\left(\tilde{u} \partial_{x} \tilde{u}-\partial_{y}\tilde{u} \int_{0}^{y}\partial_{x} \tilde{u}d y-\frac{\partial_{x}\rho}{\rho}\tilde{u}^{2}\right) \\ & = \partial_{x}^{k}\bigg(\sum\limits_{i = 0}^{m-1} C_{m-1}^{i} \partial_{y}^{m-1-i}\tilde{u}\partial_{y}^{i} \partial_{x} \tilde{u}-\sum\limits_{i = 0}^{m-2} C_{m-1}^{i+1} \partial_{y}^{m-1-i}\tilde{u} \partial_{y}^{i} \partial_{x} \tilde{u}-\partial_{y}^{m}\tilde{u} \int_{0}^{y}\partial_{x} \tilde{u}d y-\frac{\partial_{x}\rho}{\rho}\partial_{y}^{m-1}\tilde{u}^{2}\bigg), \end{aligned} \end{align*}$

and we can deduce from (3.1) and (3.2) that

$\begin{align*} |\partial_{x}^{k} \partial_{y}^{j} \tilde{u}| \leq C, \quad j \leq m+1 .\quad \Rightarrow \quad |\partial_{x}^{k} \partial_{y}^{j} u| \leq C, \quad j \leq m+1. \end{align*}$

This completes the proof of the theorem.

4. Proof of Theorem 1.3 and 1.6

In this section, we prove our main theorem. The key point is to prove that (1.6) is a uniform parabolic equation. The proof is based on the classical parabolic maximum principle. The specific proof details are as follows.

Proof. By (1.2) and $\partial_{x}P \leq 0$ , we obtain

$\begin{align*} C \geq U^{2}(x) = U^{2}(0)-2 \int_{0}^{x} \frac{\partial_{x}P(\rho)}{\rho} d x \geq U^{2}(0). \end{align*}$

By (1.7) and $w$ increasing in $\psi$ (see below), we know that there exists some positive constants $\Psi$ and $C_{0}$ such that for any $(x, \psi)\in[0, X] \times[\Psi, +\infty),$

$\begin{align} w \geq C_{0}U^{2}(0). \end{align}$

(4.1)

From Theorem 1.1, we know that there exists positive constants $y_{0}, M, m$ such that for any $(x, \psi)\in[0, X] \times[0, y_{0}]$ (we can take $y_{0}$ to be small enough),

$\begin{align} M \geq \partial_{y} \tilde{u}(x, y) \geq m . \end{align}$

(4.2)

The fact that $\psi\sim y^{2}$ is near the boundary $y = 0$ (see Remark 4.1 in ^[23]), for some small positive constant $0 < \kappa < 1$ , we get

$\begin{align} \frac{\kappa}{2} y_{0}^{2} \leq \psi \leq \kappa y_{0}^{2} \Rightarrow \sigma y_{0} \leq y \leq \frac{y_{0}}{2}, \end{align}$

(4.3)

for some constant $\sigma > 0$ depends on $\kappa, m, M$ .

We denote

$\begin{align*} \Omega = \bigl\{(x,\psi)|0\leq x\leq X,\frac{\kappa}{2} y_{0}^{2}\leq \psi\leq +\infty\bigr\}. \end{align*}$

By (4.2) and (4.3), we get $\tilde{u}(x, \sigma y_{0}) \geq m \sigma y_{0}$ , then for any $x\in[0, X]$ , we have

$\begin{align} w(x, \frac{\kappa}{2} y_{0}^{2}) \geq m^{2} \sigma^{2} y_{0}^{2}. \end{align}$

(4.4)

Since the initial data $u_{0}$ satisfies the condition (1.9) and $w = \tilde{u}^{2}$ , we know $w(0, \psi) > 0$ for $\psi > 0$ and there exists a positive constant $\zeta$ , such that for $\psi \in[\frac{\kappa}{2} y_{0}^{2}, \Psi]$ ,

$\begin{align} w(0, \psi) > \zeta. \end{align}$

(4.5)

Then, we only consider

$\begin{align*} \Omega_{1} = \bigl\{(x, \psi)|0\leq x\leq X, \frac{\kappa}{2} y_{0}^{2}\leq\psi\leq \Psi\bigr\}. \end{align*}$

We denote $H(x, \psi): = e^{-\lambda x}\partial_{\psi}w(x, \psi)$ , which satisfies the following system in the region $\Omega_{0} = \left\{(x, \psi)|0\leq x < X, 0 < \psi < +\infty\right\}$ :

$\begin{align} \left\{\begin{aligned} &\partial_{x}H-\frac{\partial_{\psi}w}{2\sqrt{w}}\partial_{\psi}H-\sqrt{w}\partial_{\psi}^{2}H+(\lambda-2\frac{\partial_{x}\rho}{\rho})H = 0,\\ &H|_{x = 0} = \partial_{\psi}w_{0}(\psi),\quad H|_{\psi = 0} = 2e^{-\lambda x}\partial_{y}\tilde{u}|_{y = 0},\quad H|_{\psi = +\infty} = 0. \end{aligned}\right. \end{align}$

(4.6)

Then, we choose $\lambda$ properly large such that $\lambda-2\frac{\partial_{x}\rho}{\rho}\geq 0$ . Due to

$\begin{align*} H|_{x = 0} = \partial_{\psi}w_{0}(\psi)\geq0,\quad H|_{\psi = 0} = 2e^{-\lambda x}\partial_{y}\tilde{u}|_{y = 0} > 0,\quad H|_{\psi = +\infty} = 0, \end{align*}$

it follows that

$\begin{align*} H(x,\psi) = e^{-\lambda x}F(x,\psi) = e^{-\lambda x}\partial_{\psi}w\geq0,\quad (x, \psi)\in[0,X^{*})\times\mathbb{R}_{+}, \end{align*}$

which means $\partial_{\psi}w\geq0$ in $[0, X)\times\mathbb{R}_{+}$ . Hence, $w$ is increasing in $\psi$ . Therefore, we know that there exists a positive constant $\lambda\geq m^{2} \sigma^{2} y_{0}^{2}$ such that for any $x\in[0, X],$

$\begin{align} w(x, \Psi) \geq \lambda. \end{align}$

(4.7)

By (1.6), for any $\varepsilon > 0$ , we know $W: = w+\varepsilon x$ satisfies the following system in $\Omega_{1}:$

$\begin{align*} \left\{\begin{aligned} &\partial_{x}W-\sqrt{w}\partial_{\psi}^{2}W-2\frac{\partial_{x}\rho}{\rho}W = \mathcal{F},\\ &W|_{x = 0} = W_{0} > \zeta,\quad W|_{\psi = \frac{\kappa}{2}y^{2}_{0}} = W_{1}\geq m^{2}\sigma^{2}y^{2}_{0},\quad W|_{\psi = \Psi} = W_{2}\geq \lambda, \end{aligned}\right. \end{align*}$

where

$\begin{align*} \mathcal{F} = -2\rho\partial_{x}P+\varepsilon-2\varepsilon x \frac{\partial_{x}\rho}{\rho}. \end{align*}$

Since $\partial_{x}P\leq0$ , we know the diffusive term $\mathcal{F} > 0.$ Therefore, the minimum cannot be reached inside $\Omega_{1}$ . Set

$\begin{align*} \eta_{0} = \min\left\{W_{0}, W_{1}, W_{2}\right\}, \end{align*}$

then by the maximum principle, we obtain $W = w+\varepsilon x\geq \eta_{0}$ . Let $\varepsilon \rightarrow 0$ , we have $w \geq \eta_{0}$ in $\Omega_{1}$ . Then we denote

$\begin{align*} \eta = \min\left\{\eta_{0}, C_{0}U^{2}(0)\right\} > 0, \end{align*}$

combining with (4.1), we have $w\geq\eta$ in $\Omega$ . Therefore, there exists some positive constant $c$ such that $c\leq w$ in $\Omega$ . From Theorem 1.1, we have $w \leq C$ in $\Omega$ . In sum, there exists positive constants $c, C$ such that $c \leq w \leq C$ in $\Omega$ . This further means that

$\begin{align} 0 < \sqrt{c}\leq\sqrt{w}\leq\sqrt{C}, \end{align}$

(4.8)

where $C$ depends on $X$ . Therefore, we prove (1.6) is a uniform parabolic equation. Furthermore, by Theorem 1.1, we know $\partial_{y}\tilde{u}, \partial_{y}^{2}\tilde{u}$ are continuous and bounded in $[0, X)\times \mathbb{R}_{+}$ . Combining $\rho$ , $\partial_{x}P$ are smooth, (4.8) with

$\begin{align*} 2\partial_{y}\tilde{u} = \partial_{\psi}w,\quad 2\partial_{y}^{2}\tilde{u} = \sqrt{w}\partial_{\psi}^{2}w = \partial_{x}w-2\frac{\partial_{x}\rho}{\rho}w+2\rho\partial_{x}P(\rho), \end{align*}$

we obtain

$\begin{align*} \|\sqrt{w}\|_{\mathcal{C}^{\alpha}(\Omega)}\leq C. \end{align*}$

Once we have the above conclusion, the proof of Theorem 1.6 can be given in a similar fashion to ^[23]. Here, we provide a brief explanation for the reader's convenience. More details can be found in ^[23].

Step 1: For any $(x_{1}, \psi_{1})\in[\varepsilon, X]\times[ \kappa y_{0}^{2}, +\infty)$ , we denote

$\begin{align*} \Omega_{x_{1}, \psi_{1}} = \bigl\{(x, \psi)|x_{1}-\frac{\varepsilon}{2}\leq x\leq x_{1}, \psi_{1}-\frac{\kappa}{2} y_{0}^{2}\leq\psi\leq \psi_{1}+\frac{\kappa}{2} y_{0}^{2}\bigr\}. \end{align*}$

Step 2: Note that the known function $\rho$ , $\partial_{x}P$ is smooth, we can repeat interior Schauder estimates in $\Omega_{x_{1}, \psi_{1}}$ to achieve uniform estimates independent of choice of $(x_{1}, \psi_{1})$ for any order derivatives of $w$ . Since the width and the length of $\Omega_{x_{1}, \psi_{1}}$ are constants and the estimates employed are independent of $(x_{1}, \psi_{1})$ , restricting the estimates to the point $(x_{1}, \psi_{1})$ , we can get for any $m < +\infty, |\nabla^{m}w(x_{1}, \psi)|\leq C_{X, m, y_{0}, \varepsilon}$ .

Step 3: Since $(x_{1}, \psi_{1})$ is arbitrary, we have for any $m < +\infty, |\nabla^{m}w(x_{1}, \psi)|\leq C_{X, m, y_{0}, \varepsilon}$ in $[\varepsilon, X]\times[ \kappa y_{0}^{2}, +\infty)$ . Then, as in Section 3, we can prove Theorem 1.6.

Finally, Theorem 1.3 is proven by combining Theorem 1.5 and Theorem 1.6.

Use of AI tools declaration

The authors declare they have not used Artificial Intelligence (AI) tools in the creation of this article.

Acknowledgments

The research of Zou was supported by the Fundamental Research Funds for the Central Universities (Grant No. 202261101).

Conflict of interest

The authors declare there is no conflict of interest.

References

[1]	R. Hilfer, Applications of fractional calculus in physics, World Scientific, 2000.
[2]	A. A. Kilbas, H. M. Srivastava, J. J. Trujillo, Theory and applications of fractional differential equations, Elsevier, 2006.
[3]	K. S. Miller, B. Ross, An introduction to the fractional calculus and fractional differential equations, New York: Wiley, 1993.
[4]	K. Oldham, J. Spanier, The fractional calculus theory and applications of differentiation and integration to arbitrary order, Elsevier, 1974.
[5]	I. Podlubny, Fractional differential equations, Elsevier, 1998.
[6]	R. Abu-Gdairi, M. Al-Smadi, G. Gumah, An expansion iterative technique for handling fractional differential equations using fractional power series scheme, J. Math. Stat., 11 (2015), 29.
[7]	D. Baleanu, A. K. Golmankhaneh, A. K. Golmankhaneh, M. C. Baleanu, Fractional electromagnetic equations using fractional forms, Int. J. Theor. Phys., 48 (2009), 3114–3123. https://doi.org/10.1007/s10773-009-0109-8 doi: 10.1007/s10773-009-0109-8
[8]	D. Baleanu, A. Jajarmi, M. Hajipour, On the nonlinear dynamical systems within the generalized fractional derivatives with Mittag-Leffler kernel, Nonlinear Dyn., 94 (2018), 397–414. https://doi.org/10.1007/s11071-018-4367-y doi: 10.1007/s11071-018-4367-y
[9]	D. Baleanu, J. H. Asad, A. Jajarmi, New aspects of the motion of a particle in a circular cavity, In: Proceedings of the Romanian Academy, 19 (2018), 361–367.
[10]	D. Baleanu, A. Jajarmi, E. Bonyah, M. Hajipour, New aspects of poor nutrition in the life cycle within the fractional calculus, Adv. Differ. Equ., 2018 (2018), 1–14. https://doi.org/10.1186/s13662-018-1684-x doi: 10.1186/s13662-018-1684-x
[11]	A. Jajarmi, D. Baleanu, Suboptimal control of fractional-order dynamic systems with delay argument, J. Vib. Control, 24 (2018), 2430–2446. https://doi.org/10.1177/1077546316687936 doi: 10.1177/1077546316687936
[12]	A. Jajarmi, D. Baleanu, A new fractional analysis on the interaction of HIV with CD4⁺ T-cells, Chaos Solitons Fract., 113 (2018), 221–229. https://doi.org/10.1016/j.chaos.2018.06.009 doi: 10.1016/j.chaos.2018.06.009
[13]	M. Klimek, Fractional sequential mechanics–models with symmetric fractional derivative, Czech. J. Phys., 51 (2001), 1348–1354. https://doi.org/10.1023/A: 1013378221617
[14]	N. Laskin, Fractional quantum mechanics, Phys. Rev. E, 62 (2000), 3135. https://doi.org/10.1103/PhysRevE.62.3135 doi: 10.1103/PhysRevE.62.3135
[15]	F. Mainardi, Fractional calculus and waves in linear viscoelasticity: an introduction to mathematical models, Singapore: World Scientific, 2010.
[16]	A. Secer, S. Altun, A new operational matrix of fractional derivatives to solve systems of fractional differential equations via Legendre wavelets, Mathematics, 6 (2018), 1–16. https://doi.org/10.3390/math6110238 doi: 10.3390/math6110238
[17]	S. M. El-Sayed, D. Kaya, Exact and numerical traveling wave solutions of Whitham-Broer-Kaup equations, Appl. Math. Comput., 167 (2005), 1339–1349. https://doi.org/10.1016/j.amc.2004.08.012 doi: 10.1016/j.amc.2004.08.012
[18]	A. M. Wazwaz, A reliable modification of Adomian decomposition method, Appl. Math. Comput., 102 (1999), 77–86. https://doi.org/10.1016/S0096-3003(98)10024-3 doi: 10.1016/S0096-3003(98)10024-3
[19]	J. H. He, Homotopy perturbation technique, Comput. Methods Appl. Mech. Eng., 178 (1999), 257–262. https://doi.org/10.1016/S0045-7825(99)00018-3 doi: 10.1016/S0045-7825(99)00018-3
[20]	J. H. He, Homotopy perturbation method: a new nonlinear analytical technique, Appl. Math. Comput., 135 (2003), 73–79. https://doi.org/10.1016/S0096-3003(01)00312-5 doi: 10.1016/S0096-3003(01)00312-5
[21]	J. H. He, Homotopy perturbation method for solving boundary value problems, Phys. Lett. A, 350 (2006), 87–88. https://doi.org/10.1016/j.physleta.2005.10.005 doi: 10.1016/j.physleta.2005.10.005
[22]	Ş. Yüzbaşı, A numerical method for solving second-order linear partial differential equations under Dirichlet, Neumann and Robin boundary conditions, Int. J. Comput. Methods., 14 (2017), 1750015. https://doi.org/10.1142/S0219876217500153 doi: 10.1142/S0219876217500153
[23]	Ş. Yüzbaşı, A collocation approach for solving two-dimensional second-order linear hyperbolic equations, Appl. Math. Comput., 338 (2018), 101–114. https://doi.org/10.1016/j.amc.2018.05.053 doi: 10.1016/j.amc.2018.05.053
[24]	Ş. Yüzbaşı, G. Yıldırım, A collocation method to solve the parabolic-type partial integro-differential equations via Pell-Lucas polynomials, Appl. Math. Comput., 421 (2022), 126956. https://doi.org/10.1016/j.amc.2022.126956 doi: 10.1016/j.amc.2022.126956
[25]	M. Merdan, H. Anac, T. Kesemen, The new Sumudu transform iterative method for studying the random component time-fractional Klein-Gordon equation, Sigma, 10 (2019), 343–354.
[26]	K. Wang, S. Liu, A new Sumudu transform iterative method for time-fractional Cauchy reaction-diffusion equation, SpringerPlus, 5 (2016), 1–20. https://doi.org/10.1186/s40064-016-2426-8 doi: 10.1186/s40064-016-2426-8
[27]	F. Ayaz, Applications of differential transform method to differential-algebraic equations, Appl. Math. Comput., 152 (2004), 649–657. https://doi.org/10.1016/S0096-3003(03)00581-2 doi: 10.1016/S0096-3003(03)00581-2
[28]	F. Kangalgil, F. Ayaz, Solitary wave solutions for the KdV and mKdV equations by differential transform method, Chaos Solitons Fract., 41 (2009), 464–472. https://doi.org/10.1016/j.chaos.2008.02.009 doi: 10.1016/j.chaos.2008.02.009
[29]	M. Merdan, A. Gökdoğan, A. Yıldırım, S. T. Mohyud-Din, Numerical simulation of fractional Fornberg-Whitham equation by differential transformation method, Abstr. Appl. Anal., 2012 (2012), 965367. https://doi.org/10.1155/2012/965367 doi: 10.1155/2012/965367
[30]	J. H. He, Variational iteration method–a kind of non-linear analytical technique: some examples, Int. J. Non-Linear. Mech., 34 (1999), 699–708. https://doi.org/10.1016/S0020-7462(98)00048-1 doi: 10.1016/S0020-7462(98)00048-1
[31]	G. W. Leibniz, Letter from Hanover, Germany to G.F.A. L'Hospital, September 30, 1695, In: Mathematische Schriften 1849, reprinted 1962,301–302.
[32]	P. K. Gupta, M. Singh, Homotopy perturbation method for fractional Fornberg-Whitham equation, Comput. Math. Appl., 61 (2011), 250–254. https://doi.org/10.1016/j.camwa.2010.10.045 doi: 10.1016/j.camwa.2010.10.045
[33]	S. Momani, Z. Odibat, A. Alawneh, Variational iteration method for solving the space‐ and time‐fractional KdV equation, Numer. Methods Partial Differ. Equ., 24 (2008), 262–271. https://doi.org/10.1002/num.20247 doi: 10.1002/num.20247
[34]	M. Merdan, On the solutions of nonlinear fractional Klein-Gordon equation with modified Riemann-Liouville derivative, Appl. Math. Comput., 242 (2014), 877–888. https://doi.org/10.1016/j.amc.2014.06.013 doi: 10.1016/j.amc.2014.06.013
[35]	Z. H. Khan, W. A. Khan, N-transform properties and applications, NUST J. Eng. Sci., 1 (2008), 127–133.
[36]	F. B. M. Belgacem, R. Silambarasan, Maxwell's equations solutions by means of the natural transform, Math. Eng. Sci. Aerosp, 3 (2012), 313–323.
[37]	F. B. M. Belgacem, R. Silambarasan, Theory of natural transform, Math. Eng. Sci. Aerosp, 3 (2012), 99–124.
[38]	M. S. Rawashdeh, S. Maitama, Solving coupled system of nonlinear PDE's using the natural decomposition method, Int. J. Pure Appl. Math., 92 (2014), 757–776. https://doi.org/10.12732/ijpam.v92i5.10 doi: 10.12732/ijpam.v92i5.10
[39]	M. S. Rawashdeh, S. Maitama, Solving nonlinear ordinary differential equations using the NDM, J. Appl. Anal. Comput., 5 (2015), 77–88. https://doi.org/10.11948/2015007 doi: 10.11948/2015007
[40]	M. S. Rawashdeh, S. Maitama, Solving PDEs using the natural decomposition method, Nonlinear Stud., 23 (2016), 63–72.
[41]	M. Rawashdeh, S. Maitama, Finding exact solutions of nonlinear PDEs using the natural decomposition method, Math. Methods Appl. Sci., 40 (2017), 223–236. https://doi.org/10.1002/mma.3984 doi: 10.1002/mma.3984
[42]	H. M. Baskonus, H. Bulut, Y. Pandir, The natural transform decomposition method for linear and nonlinear partial differential equations, Math. Eng. Sci. Aerosp, 5 (2014), 111–126.
[43]	M. S. Rawashdeh, The fractional natural decomposition method: theories and applications, Math. Methods Appl. Sci., 40 (2017), 2362–2376. https://doi.org/10.1002/mma.4144 doi: 10.1002/mma.4144
[44]	W. Gao, P. Veeresha, D. G. Prakasha, H. M. Baskonus, New numerical simulation for fractional Benney-Lin equation arising in falling film problems using two novel techniques, Numer. Methods Partial Differ. Equ., 37 (2021), 210–243. https://doi.org/10.1002/num.22526 doi: 10.1002/num.22526
[45]	G. M. Mittag-Leffler, Sur la nouvelle function Eα(x), C. R. Acad. Sci. Paris, 137 (1903), 554–558.
[46]	K. Shah, H. Khalil, R. A. Khan, Analytical solutions of fractional order diffusion equations by natural transform method, Iran. J. Sci. Technol. Trans. A Sci., 42 (2018), 1479–1490. https://doi.org/10.1007/s40995-016-0136-2 doi: 10.1007/s40995-016-0136-2
[47]	A. K. Golmankhaneh, A. K. Golmankhaneh, D. Baleanu, On nonlinear fractional Klein-Gordon equation, Signal Process., 91 (2011), 446–451. https://doi.org/10.1016/j.sigpro.2010.04.016 doi: 10.1016/j.sigpro.2010.04.016
[48]	J. Liouville, Memoire sur quelques questions de geometries et de mecanique, et sur un nouveau genre de calcul pour resoundre ces questions, J. École. Polytech., 13 (1832), 1–69.
[49]	B. Ross, A brief history and exposition of the fundamental theory of fractional calculus. In: Fractional calculus and its applications, Berlin, Heidelberg: Springer, 1975, 1–36. https://doi.org/10.1007/BFb0067096
[50]	R. Hilfer, Y. Luchko, Desiderata for fractional derivatives and integrals, Mathematics, 7 (2019), 1–5. https://doi.org/10.3390/math7020149 doi: 10.3390/math7020149
[51]	D. Baleanu, A. Fernandez, On fractional operators and their classifications, Mathematics, 7 (2019), 1–10. https://doi.org/10.3390/math7090830 doi: 10.3390/math7090830
[52]	M. D. Ortigueira, J. A. T. Machado, What is a fractional derivative? J. Comput. Phys., 293 (2015), 4–13. https://doi.org/10.1016/j.jcp.2014.07.019 doi: 10.1016/j.jcp.2014.07.019
[53]	M. Caputo, M. Fabrizio, On the notion of fractional derivative and applications to the hysteresis phenomena, Meccanica, 52 (2017), 3043–3052. https://doi.org//10.1007/s11012-017-0652-y doi: 10.1007/s11012-017-0652-y
[54]	D. Z. Zhao, M. K. Luo, Representations of acting processes and memory effects: general fractional derivative and its application to theory of heat conduction with finite wave speeds, Appl. Math. Comput., 346 (2019), 531–544. https://doi.org/10.1016/j.amc.2018.10.037 doi: 10.1016/j.amc.2018.10.037

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