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\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2015 (2015), No. 101, pp. 1--25.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu
\newline ftp ejde.math.txstate.edu}
\thanks{\copyright 2015 Texas State University - San Marcos.}
\vspace{9mm}}

\begin{document}
\title[\hfilneg EJDE-2015/101\hfil Pointwise estimates]
{Pointwise estimates for porous medium type equations with
low order terms and measure data}

\author[S. Sturm \hfil EJDE-2015/101\hfilneg]
{Stefan Sturm}

\address{Stefan Sturm \newline
Fachbereich Mathematik, Paris-Lodron-Universit\"at Salzburg,
5020 Salzburg, Austria}
\email{Stefan.Sturm@sbg.ac.at}

\thanks{Submitted January 13, 2015. Published April 15, 2015.}
\makeatletter
\@namedef{subjclassname@2010}{\textup{2010} Mathematics Subject Classification}
\makeatother
\subjclass[2010]{35K65, 35K20, 31B15}
\keywords{Porous medium equation; measure data; Riesz potential estimates; 
\hfill\break\indent degenerate
parabolic equations}

\begin{abstract}
  We study  a Cauchy-Dirichlet problem with homogeneous boundary conditions
  on the parabolic boundary of a space-time cylinder for degenerate porous
  medium type equations with low order terms and a non-negative, finite
  Radon measure on the right-hand side. The central objective is to acquire
  linear pointwise estimates for weak solutions in terms of Riesz potentials.
  Our main result, Theorem \ref{Hauptthm}, generalizes an estimate previously
  obtained by B\"ogelein, Duzaar and Gianazza \cite[Theorem 1.2]{BDG}),
  since the problem  and the structure conditions considered here, 
  are more universal.

\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\newtheorem{definition}[theorem]{Definition}
\allowdisplaybreaks


\section{Introduction and main result}

 In this introductory section, we determine the basic setting for our
further observations, describe the treated problem, specify some notation,
 mention the main conclusion and unveil the proof strategies.

\subsection{Setting} \label{KAP_1.1}
 In this section, we present the covered problem and explain the occurring
quantities, including some of their properties. Let $T > 0$ and
$E \subset \mathbb{R}^n$ be a bounded, open domain, where $n \geq 2$.
By $E_T:=E\times (0,T)$, we define a space-time cylinder, 
and write $\partial_\textup{par} E_T := (E\times\{0\}) 
\cup (\partial E\times [0,T))$ for its parabolic boundary.
Throughout this paper, we study a Cauchy-Dirichlet problem for porous
 medium type equations of the form
\begin{equation}  \label{PMG}
\begin{gathered}
\partial_t u - \operatorname{div}\big(\mathbf{A}(x,t,u,Du)\big)
 - \mathbf{B}(x,t,u,Du) = \mu \quad\text{in }E_T,\\
u=0 \quad\text{on }\partial_{\rm par} E_T,
\end{gathered}
\end{equation}
where $\mu$ is a non-negative Radon measure on $E_T$ with finite total
 mass $\mu(E_T)<\infty$.The vector fields
$\mathbf{A}: E_T \times \mathbb{R} \times \mathbb{R}^n \to \mathbb{R}^n$ and
$\mathbf{B}: E_T \times \mathbb{R} \times \mathbb{R}^n \to \mathbb{R}$ are assumed to be
measurable with respect to $(x,t) \in E_T$ for all $(u,\xi) \in \mathbb{R} \times \mathbb{R}^n$
and continuous with respect to $(u,\xi) \in \mathbb{R} \times \mathbb{R}^n$
for a.\,e.\ $(x,t) \in E_T$. Moreover, we require them to satisfy the
ellipticity condition
\begin{gather}
\mathbf{A}(x,t,u,\xi) \cdot \xi
 \geq C_0 m |u|^{m-1} |\xi|^2 - C^2 |u|^{m+1} \label{WEB1}\\
\intertext{as well as the two growth conditions}
|\mathbf{A}(x,t,u,\xi)| \leq C_1 m |u|^{m-1} |\xi| + C |u|^m, \label{WEB2}\\
|\mathbf{B}(x,t,u,\xi)| \leq Cm|u|^{m-1}|\xi| + C^2|u|^m \label{WEB3}
\end{gather}
for any $(x,t) \in E_T$, $u\in \mathbb{R}$ and $\xi \in \mathbb{R}^n$, where $C_0 > 0$, $C_1 > 0$
and $C \geq 0$ are fixed constants and $m > 1$, i.\,e.\ we are concerned
 with the degenerate case of the equation. Finally, in order to prove
the existence of very weak solutions (cf.\ \cite[Theorem 1.4 on page 3287]{BDG}),
 one requires the monotonicity assumption
\begin{equation*}
\big(\mathbf{A}(x,t,u,\xi_1) - \mathbf{A}(x,t,u,\xi_2)\big) \cdot
(\xi_1 - \xi_2) \geq C_0 |u|^{m-1} |\xi_1 - \xi_2|^2
\end{equation*}
to hold for any $u \in \mathbb{R}$, $\xi_1, \xi_2 \in \mathbb{R}^n$ and
a.\,e.\ $(x,t) \in E_T$. However, since our objective here is not
 an existence proof, we do not need to have any monotonicity condition
in the further course of this paper.
The prototype for equations treated in the sequel is given by the classical
porous medium equation
\begin{equation} \label{PME_einfach}
\partial_t u - \operatorname{div}\big(Du^m\big) = \mu \quad \text{in } E_T.
\end{equation}
This ends the passage on the fundamental requirements, and some comments
on the porous medium equation, its fields of utilization and the history
of the problem are to come up next.

\subsection{The porous medium equation}

There are lots of different applications in which one can portray the
underlying process using an equation of the above form. Besides considering
such an equation for the characterization of ground water problems, heat
radiation in plasmas, or spread of viscous fluids, one of the most important
examples is the modeling of an ideal gas flowing isoentropically in a homogeneous
 porous medium, e.\,g.\ soil or foam. The flow is controlled by the following
three physical laws, where for each one we like to give just a sketchy idea of
what the law signifies. \newline  Since we are guided from the concept
that the total amount of gas is conserved, i.\,e.\ the rate at which mass enters
some region of the medium is proportional to the rate at which mass leaves that
region (the constant of proportionality $\tilde\kappa \in (0,1)$ provides
information on the porosity of the medium), we postulate that the mass conservation
law $\tilde\kappa \partial_t \tilde\varrho + \operatorname{div}
 (\tilde\varrho \tilde{v}) =0$ holds, where $\tilde{v} \equiv \tilde{v} (x,t)$
is the velocity vector and $\tilde\varrho \equiv \tilde\varrho(x,t)$
is the density of the gas. Next, we may demand that also Darcy's diffusion law,
an empirically derived law describing the gas flow, applies to the situation,
meaning that $\tilde\nu \tilde{v} = -\tilde\mu D\tilde{p}$ is satisfied.
Here, $\tilde\nu \in \mathbb{R}^+$ denotes the viscosity of the gas, $\tilde\mu \in \mathbb{R}^+$
stands for the permeability of the medium, and $\tilde{p} \equiv \tilde{p}(x,t)$
is the pressure. At last, we ask the equation of state for ideal gases
$\tilde{p}=\tilde{p}_0 \tilde\varrho^\alpha$ to hold with constants
$\tilde{p}_0 \in \mathbb{R}^+$ and $\alpha \in [1,\infty)$. Combining these laws,
one can eliminate the quantities $\tilde{p}$ and $\tilde{v}$ from the equations,
which finally leads to the porous medium equation \eqref{PME_einfach} with
$\mu \equiv 0$, where in the physical context $m = 1+ \alpha \geq 2$, and
$u$ represents a scaled density. Therefore, it is completely natural to assume
$u \geq 0$ for our reflections.

Although from the physical background it seems instinctive to consider $m\geq 2$,
it is sufficient to impose $m>1$ as a condition on $m$, because the mathematical
theory makes no distinction between the exponents as long as they are larger
than $1$. More precisely, the modulus of ellipticity of the treated equation
is $|u|^{m-1}$. For $m>1$, it vanishes if $u$ becomes $0$, such that the
equation is degenerate on the set $\{ |u| = 0 \}$, whereas in the case that
$0<m<1$, the modulus of ellipticity $|u|^{m-1}$ tends to $\infty$ as
$|u| \to 0$, and the equation is singular on the set $\{ |u| = 0 \}$.
Throughout the paper, we will only look at the nonlinear, degenerate case,
in which $m>1$.

 Having in mind the physical intuition, we expect that the support
$\operatorname{supp} \big(\mathcal{B}_m(\cdot,t)\big)$ of the Barenblatt
fundamental solution, that is the (unique,
cf.\, \cite[Theorem 1 on page 175]{MPI})
very weak solution of the porous medium equation
$\partial_t u - \Delta u^m = \delta_{(0,0)}$ in $\mathbb{R}^n \times [0,\infty)$,
\begin{equation*}
\mathcal{B}_m(x,t) := \begin{cases}
t^{-\frac{n}{k}} \Big[ 1-b \big( |x| t^{-\frac{1}{k}} \big)^2
\Big]_+^{\frac{1}{m-1}} & \text{for } t>0, \\
0 & \text{for } t\leq 0
\end{cases}
\end{equation*}
is bounded for any fixed $t>0$ (here, $b = \frac{n(m-1)}{2nmk}$ and
 $k = n(m-1)+2$). This means that if we suppose that the gas solely occurs
in some bounded area at time $t=0$, the gas will have propagated after some
time $t>0$ only to a certain finite region, i.\,e.\ the gas propagates with
finite speed, which coincides with our imagination of $\mathcal{B}_m$ as
the distribution of the density of the gas (note that this mental image
is also in perfect accordance with the fact that the solution is radial in $x$,
in other words, the process does not prefer any specific direction). However,
this imagination fails in the case $m=1$, where the equation is nondegenerate
and \eqref{PME_einfach} passes into the well-known (linear) heat equation
$\partial_t u = \Delta u$, which characterizes the distribution of heat over
time not taking into account any exterior heat sources, and for which a rich
theory is available (cf.\,\cite{LSU}). The finite and infinite propagation speed,
respectively, is one of the most remarkable differences between the porous
medium equation with $m>1$ and the heat equation.

 As regards the regularity of solutions of the porous
medium type equation
$$
\partial_t u - \operatorname{div}\big(\mathbf{A}(x,t,u,Du)\big) -
\mathbf{B}(x,t,u,Du) = 0
$$
under the structure conditions \eqref{WEB1}-\eqref{WEB3}, the fact that locally
bounded solutions are locally H\"older continuous was established in \cite{BAF}.
In \cite{BGV}, local H\"older continuity is deduced from a Harnack inequality,
 and \cite{CAF} already contains the regularity result for the special case
of \eqref{PME_einfach} with $\mu \equiv 0$.

 Unlike in large parts of the literature existing so far, we examine a fairly
general version of the porous medium equation involving a Radon measure on the
right-hand side. In addition to diverse applications, such as the description
of explosions, Radon measures are equipped with their own mathematical charm,
 which is why it is worth studying the behavior of equations of the above form.
In order to get a more profound overview of the considered problem and the
associated results, we refer to \cite{ARO}, \cite{BGV}, \cite{VAZ} as well
as the list of references at the end of this article. At this point, we
finish our annotations concerning the classification of the treated problem.
The next subsection is devoted to settle some notations that we will employ
in the sequel.


\subsection{Notation} \label{KAP_NOT}

As to the notation, for a point $z\in\mathbb{R}^{n+1} \cong \mathbb{R}^n 
\times \mathbb{R}$, we always write $z=(x,t)$.As is customary, we denote
by $B_r(x_0) := \{ x \in \mathbb{R}^n : |x-x_0| < r \}$ the open ball in
$\mathbb{R}^n$ with center $x_0 \in \mathbb{R}^n$ and radius $r>0$, and we define
parabolic cylinders by $Q_{r,\theta}(z_0) := B_r(x_0) \times (t_0 - \theta, t_0)$,
 where $z_0 = (x_0,t_0) \in \mathbb{R}^{n+1}$, $\theta > 0$ and $r \in (0,R_0]$.
 Here, $R_0 > 0$ is an arbitrary upper bound for the radius $r$, which shall
be fixed for the rest of this report. What is more, for a cylinder
$Q \equiv Q_{r,\theta}(z_0)$, we use the abbreviation $2Q$ for the cylinder
$Q_{2r,4\theta}(z_0)$.

By $\{u > a\}$, we express the superlevel set $\{(x,t) \in E_T: u(x,t) > a \}$
where the function $u$ exceeds the level $a>0$, and we address the positive
part of $u$ as $u_+ := \max \{u,0\}$. We denote the weak spatial derivative
of the function $u$ by $Du = D_x u = (D_{x_1}u, D_{x_2}u, \dots, D_{x_n}u)$,
and $\partial_t = \frac{\partial}{\partial t}$ is the operator for the time
derivative. Finally, $\gamma\equiv\gamma(\cdot)$ stands for a constant
which may vary from line to line and depends only on the parameters presented behind.
 This completes our remarks on the notations, and we turn our attention towards
the central statement of this paper.

\subsection{Main result} \label{KAP_1.2}

 We now provide the principal theorem containing the linear pointwise
estimate \eqref{HauptBeh} for a weak solution of the Cauchy-Dirichlet
problem \eqref{PMG} in terms of the Riesz potential
 $\mathbf{I}_2^\mu (z_0, r, \theta)$, which will be introduced in
Definition \ref{RieszPot}. The proof of Theorem \ref{Hauptthm} will be
performed in Chapter \ref{KAP_4}.

\begin{theorem} \label{Hauptthm}
Let $u$ be a weak solution of the Cauchy-Dirichlet problem \eqref{PMG}
for the inhomogeneous porous medium type equation in the sense of
Definition \ref{DefSL} and $R_0 \in (0,\infty)$ be fixed. Suppose
that the structure conditions \eqref{WEB1}-\eqref{WEB3} are fulfilled.
 Then, for any $\lambda \in (0,\frac{1}{n}]$, almost every $z_0 \in E_T$
and every parabolic cylinder $Q_{r,\theta}(z_0) \Subset E_T$ with
$r \in (0,R_0]$ and $\theta > 0$, the linear potential estimate
\begin{equation} \label{HauptBeh}
u(z_0) \leq 5 \Big( \frac{r^2}{\theta} \Big)^{\frac{1}{m-1}}
+ \gamma \Big[ \frac{1}{r^{n+2}} \iint_{Q_{r,\theta}(z_0)} u^{m+\lambda}
\,d z \Big]^{\frac{1}{1+\lambda}} + \gamma \mathbf{I}_2^\mu (z_0, r, \theta)
\end{equation}
holds with a universal constant
$\gamma \equiv \gamma(n,C_0,C_1,C,m,\lambda, R_0)$.
\end{theorem}

 This estimate is optimal in the sense that the Barenblatt solution has exactly
the same behavior. Note that the bound depends on the Riesz potential in the
considered point $z_0$, hence, viewed in this light, it is very fine.
Having at hand the estimate, we ought to compare it with already existing results.

First substantial moves in the history of this field were achieved in
\cite[Theorem 4.1 on page 608]{KIL1} and
\cite[Theorem 1.6 on page 139]{KIL2}, where potential estimates were established
for the elliptic $p$-Laplacian equation. Beyond that, our conclusion generalizes
some previously obtained estimates for weak solutions of the porous medium equation.
To begin with, if $C=0$ in \eqref{WEB1} and \eqref{WEB2}, respectively,
and additionally $\mu \equiv 0$ and $\mathbf{B} \equiv 0$ in \eqref{PMG},
then our pointwise estimate \eqref{HauptBeh} reduces to the
$L^{\infty}_{\rm loc}$-bound for weak solutions of the porous
medium equation \cite[(1.6) on page 139]{AND}. If merely $C=0$ and
$\mathbf{B} \equiv 0$, we receive the result from
\cite[Theorem 1.2 on page 3285]{BDG}. Furthermore, for solutions
of \eqref{PME_einfach}, a similar bound was derived earlier in
\cite[Theorem 1.1 on page 260]{LIS}, but the estimate is weaker than ours
and the one from \cite{BDG}, since it comprises an extra term
\begin{equation*}
\gamma \sup_{t \in (t_0-\theta, t_0)} \frac{1}{\varrho^n}
\int_{B_{\varrho}(x_0)} u(x,t) \,d x
\end{equation*}
on the right-hand side. Thus, the sup-bound from \cite{AND} cannot be 
retrieved in the case $\mu \equiv 0$. Given the preceding observations, 
our potential estimate \eqref{HauptBeh} is natural, in the sense that 
it implies the known results from \cite{AND}, \cite{BDG} and \cite{LIS} 
in the mentioned special cases. 

 Moreover, when $m=1$ and
$\mu\not\equiv 0$, our result becomes a bound related to the potential estimate 
from \cite[Theorem 1.4 on page 1101]{DUM}, which is stronger than ours, 
however, the authors postulate that another continuity assumption holds. 
The only distinction in the outcome concerns the exponent $1+\lambda > 1$ 
in the integral
\begin{equation*}
\gamma \Big[ \frac{1}{r^{n+2}} \iint_{Q_{r,\theta}(z_0)} u^{1+\lambda} 
\,d z \Big]^{\frac{1}{1+\lambda}}.
\end{equation*}
Note that we are not allowed to pass to the limit $\lambda \searrow 0$, 
because the constant $\gamma$ blows up as $\lambda \searrow 0$.

 As demonstrated in \cite[Theorem 1.4 on page 3287]{BDG}, one can expect 
no more than very weak solutions to exist. For such solutions, the pointwise 
estimate \eqref{HauptBeh} follows for the case $\mathbf{B} \equiv 0$ 
by an approximation procedure (cf.\, \cite[Theorem 1.5 on page 3287]{BDG}). 
If actually $\mu \in L^\infty(E_T)$, one can prove the existence of 
weak solutions (cf.\ \cite[Theorem 3.1 on page 2739]{IVM}). 
In this report, we will not pick up the theory of very weak solutions, 
we merely speak of weak solutions instead, being conscious of the fact that 
the existence of such a solution is not guaranteed as long as we consider 
a general Radon measure $\mu$ without any further qualities.

Since, in contrast to \cite{BDG}, in our structure conditions 
(taken from \cite[Chapter 5 on page 33]{BGV}) there may additionally 
occur low order terms, we are allowed to explore even more extensive 
versions of the porous medium equation, for instance, equations with 
principal part
\begin{equation*}
\operatorname{div}\big(\mathbf{A}(x,t,u,Du)\big) 
= \sum_{i,j=1}^n D_{x_j} \Big(|u|^{m-1}a_{ij}(x,t) D_{x_i} u\Big) 
+ \sum_{j=1}^n D_{x_j} \Big( f(x,t) |u|^m \frac{D_{x_j} u}{|Du|}\Big),
\end{equation*}
where $f$ is a bounded, non-negative function, and the matrix 
$(a_{ij})_{1\leq i,j \leq n}$ is supposed to be measurable and locally 
positive definite in $E_T$ (cf.\ \cite[Section 5.2 on page 35]{BGV}).
 Next, we go a little bit into detail about the contents of the following 
text and outline the strategy of our argumentation.

\subsection{Contents and proof strategies} \label{KAP1.5}

 First of all, in Section \ref{KAP_schwLsg} we will
declare the concept of a weak solution of the Cauchy-Dirichlet problem
\eqref{PMG} for the inhomogeneous porous medium type equation.
 We will then define our notion of the localized parabolic
Riesz potential, which we require for writing down the pointwise estimate
 \eqref{HauptBeh}, and quote a parabolic Sobolev embedding, including
an associated Gagliardo-Nirenberg inequality \eqref{GNU}. After that,
we study three auxiliary functions $G_\lambda$, $V_\lambda$ and $W_\lambda$,
which will turn up in the proof of Theorem \ref{Hauptthm}.
Finally, we will prepare a mollification in time and on its basis develop
the regularized variant \eqref{REG} of the weak formulation \eqref{GleichungSL}.
\newline
In the third section, we will initially define
parabolic cylinders and then deduce the energy estimate \eqref{ENER}.
 To this end, we will insert a purpose-built testing function in
the regularized form \eqref{REG} and analyze all appearing terms by applying, 
inter alia, convergence results for the above mollification, standard estimates 
like H\"older's and Young's inequality, or the ellipticity and growth 
conditions \eqref{WEB1}-\eqref{WEB3}, pursuing the objective of gaining 
an inequality which enables us to properly bound $G_\lambda$, $DV_\lambda$ 
and $DW_\lambda$. The idea is to express these functions, which will show 
up in the computations of the proof of Theorem \ref{Hauptthm} in a natural way,
 by terms that one can reasonably cope with in the further course of the paper.

 The fourth paragraph is designated for the proof of the pointwise estimate
\eqref{HauptBeh} for weak solutions of the Cauchy-Dirichlet problem
\eqref{PMG} for the nonhomogeneous porous medium type equation in terms of
a Riesz potential. For the proof, we firstly define appropriate sequences of
cylinders $(Q_j)_{j \in \mathbb{N}_0}$ and parameters $(a_j)_{j \in \mathbb{N}_0}$ and
$(d_j)_{j \in \mathbb{N}_0}$ and record simple but beneficial tools for our upcoming
reflections. The matter of Chapter \ref{KAP_4.2} is to establish the recursive
bound \eqref{4.6} for $d_j$. To achieve this, we apply, among others, the
Gagliardo-Nirenberg inequality and the energy estimate \eqref{ENER} in its
version \eqref{4.10} with the previously designed cylinders $2Q_j$ and the
quantities $a_j$ and $d_j$. Here, the presence of the low order terms from
the structure conditions \eqref{WEB1}-\eqref{WEB3} causes extra difficulties,
since in principle we have to replace $|u|$ by $|u-a_{j -1}|$.
Eventually adding up \eqref{4.6} yields a convenient bound for $a_j$
and subsequently passing to the limit $j \to \infty$ results in the asserted
bound \eqref{HauptBeh} for $u(z_0)$, which ends the proof.


\section{Preliminaries} \label{KAP_2}

 In this section, we   characterize precisely the terms
 \textit{weak solution} and \textit{Riesz potential}. Moreover, 
we will state a parabolic Sobolev embedding, including a 
Gagliardo-Nirenberg inequality, and introduce some auxiliary functions, 
together with three lemmata concerning their properties.
 At last, we create a regularized version of the weak formulation of 
the Cauchy-Dirichlet problem for the porous medium type equation by 
means of a special time mollification.

\subsection{Weak solutions, Riesz potentials and a Sobolev embedding} 
\label{KAP_schwLsg}

This part deals with weak solutions, Riesz potentials, and a Sobolev embedding 
with a Gagliardo-Nirenberg inequality. To begin with, we declare the definition 
of a weak solution of the Cauchy-Dirichlet problem for the inhomogeneous 
porous medium type equation, remarking that our notion of a weak solution 
differs from the one used in \cite[Definition 1.1 on page 3284]{BDG}, 
where the regularity condition on $u^m$ is replaced by the assumption 
$u^\frac{m+1}{2} \in L^2\big((0,T); W^{1,2}_0(E)\big)$.

\begin{definition} \label{DefSL} \rm
A non-negative function $u : \overline{E_T} \to \mathbb{R}$ satisfying
$$
u \in C^0\big([0,T]; L^2(E)\big),\;
 u^m \in L^2\big((0,T); W^{1,2}_0(E)\big) \text{ and } 
u(\cdot,0)=0 \text{ in } E
$$
is termed a weak solution of the Cauchy-Dirichlet problem \eqref{PMG} 
for the inhomogeneous porous medium type equation if and only if the identity
\begin{equation} \label{GleichungSL}
\begin{aligned}
&\int_E u\varphi\Big|^T_0 \,d x + \iint_{E_T} 
[ -u\partial_t \varphi + \mathbf{A}(x,t,u,Du)\cdot D\varphi 
- \mathbf{B}(x,t,u,Du)\varphi ] \, dz \\
&= \iint_{E_T} \varphi \,d \mu
\end{aligned}
\end{equation}
holds  for any testing function $\varphi \in C^{\infty}(\overline{E_T})$ 
vanishing on $\partial E \times (0,T)$.
\end{definition}

 At this point, we have to give a meaning to the symbol $Du$ and become 
aware of the sense which it has to be understood in, because in 
Definition \ref{DefSL} we have imposed $Du^m \in L^2(E_T)$, among others, 
as a condition on $u$, hence, the existence of $Du$ cannot be assured. 
Formally, we set $$Du := \frac{1}{m} \chi_{\{u>0\}} u^{1-m} Du^m$$ and
like to interpret $Du$ in that way. On $\{ u > \sigma\}$, where $\sigma>0$, 
$Du$ indeed is the weak derivative of $u$, and we have 
$Du \in L^2(E_T \cap \{ u > \sigma \})$. In other words, whenever we will 
integrate over a superlevel set of the form $\{ u>\sigma \}$ with $\sigma > 0$, 
writing $Du$ under the integral sign is permissible and unproblematic 
(in the proofs of Theorem \ref{ENER_SATZ} and Theorem \ref{Hauptthm}, 
the parameter $a>0$ and the members $a_j > 0$ of the yet to be defined 
sequence $(a_j)_{j \in \mathbb{N}_0}$, respectively, will take on the role of $\sigma$). 
After that succinct discussion about the problems associated with $Du$, 
we get to the so-called localized parabolic Riesz potential.

\begin{definition} \label{RieszPot} \rm
For $\beta \in (0,n+2], z_0 \in E_T$ and $r,\theta > 0$ such that $Q_{r,\theta}(z_0) \Subset E_T$, we define the localized parabolic Riesz potential by
\begin{equation*}
\mathbf{I}_{\beta}^{\mu}(z_0,r,\theta) := \int_0^r \frac{\mu( Q_{\varrho, \varrho^2\theta/r^2} (z_0) )}{\varrho^{n+2-\beta}} \frac{d\varrho}{\varrho}.
\end{equation*}
\end{definition}

 Next, we cite a parabolic Sobolev embedding
(cf.\ \cite[Proposition 3.7 on page 7]{DIB}), which we will employ 
later many a time.

\begin{theorem} \label{GNU_SATZ}
Let $Q_{\varrho,\theta} (z_0)$ be a parabolic cylinder with $\varrho,\theta > 0$ 
and let \mbox{$1<p<\infty$} and $0<r<\infty$. Then, there exists a 
constant $\gamma \equiv \gamma(n,p,r)$ such that for every 
$$
u \in L^{\infty} \big((t_0-\theta,t_0);
 L^r(B_{\varrho}(x_0)) \big) \cap L^p \big((t_0-\theta,t_0);
 W^{1,p}(B_{\varrho}(x_0)) \big)
$$ 
there holds the Gagliardo-Nirenberg inequality
\begin{equation} \label{GNU}
\begin{aligned}
&\iint_{Q_{\varrho,\theta}(z_0)} |u|^q \,d z \\
&\leq \gamma 
\Big( \sup_{t \in (t_0-\theta, t_0)} \int_{B_{\varrho}(x_0) 
\times \{t\}} |u|^r \,d x \Big)^{p/n}
 \iint_{Q_{\varrho,\theta}(z_0)} \Big[ \Big| \frac{u}{\varrho} \Big|^p 
+ |Du|^p \Big] dz,
\end{aligned}
\end{equation}
where $q$ is given by $q = \frac{p(n+r)}{n}$.
\end{theorem}

Having specified the terms \textit{weak solution} and 
\textit{localized parabolic Riesz potential} and displayed the
 helpful Gagliardo-Nirenberg inequality, we hereby finish this section.

\subsection{Auxiliary functions}

In this part, we will introduce some mappings which will occur in the
third section in the energy estimate \eqref{ENER}. 
The assertions collected in the following lemmata will turn out to 
be useful in the proof of Theorem \ref{Hauptthm}. We start our 
reflections by announcing the auxiliary functions.

\begin{definition} \label{Hilfsfktn} \rm
For $\lambda \in (0,1)$ and $s \geq 0$, we define the functions 
$G_\lambda$, $V_\lambda$ and $W_\lambda$ by 
\begin{gather*}
G_\lambda(s) := \int_0^s \big[ 1- (1+\sigma)^{-\lambda} \big] \,d \sigma 
= s - \frac{1}{1-\lambda} \big[ (1+s)^{1-\lambda} -1 \big], \\
V_\lambda(s) := \int_0^s \sigma^{\frac{m-1}{2}} (1+\sigma)^{-\frac{1+\lambda}{2}} 
\,d \sigma,\\
W_\lambda(s) := \int_0^s (1+\sigma)^{-\frac{1+\lambda}{2}} \,d \sigma 
= \frac{2}{1-\lambda} \big[ (1+s)^{\frac{1-\lambda}{2}} -1 \big].
\end{gather*}
\end{definition}

 We now mention one lemma for each of those auxiliary functions containing 
some characteristics which are required afterwards. 
The corresponding proofs can be found in \cite[Section 2.3 on page 3291]{BDG}.

\begin{lemma}
For any $\varepsilon \in (0,1]$ and $s \geq 0$, there holds
\begin{equation} \label{L1}
s \leq \varepsilon + \gamma_\varepsilon G_\lambda(s)
\end{equation}
for a constant $\gamma_\varepsilon \equiv \frac{\gamma(\lambda)}{\varepsilon}$.
\end{lemma}

\begin{lemma} \label{L2}
For any $\varepsilon \in (0,1]$ and $s \geq 0$, there hold
\begin{gather} \label{L2a}
V_\lambda(s) \leq \frac{2}{m-\lambda} s^{\frac{m-\lambda}{2}},\\
 \label{L2b}
s^{m+\lambda} \leq \varepsilon^{1+\lambda}s^{m-1} 
+ \gamma_\varepsilon V_\lambda(s)^{\frac{2(m+\lambda)}{m-\lambda}},
\end{gather}
where the constant $\gamma_\varepsilon \equiv \gamma(m, \lambda, \varepsilon)$ 
blows up as $\varepsilon^{-(1+\lambda)\frac{m+\lambda}{m-\lambda}}$ 
in the limit $\varepsilon \searrow 0$.
\end{lemma}

\begin{lemma}
For any $\varepsilon \in (0,1]$ and $s \geq 0$, there hold
\begin{gather} \label{L3a}
W_\lambda(s) \leq \frac{2}{1-\lambda} s^{\frac{1-\lambda}{2}},\\
 \label{L3b}
s^{1+\lambda} \leq \varepsilon^{1+\lambda} 
+ \gamma_\varepsilon W_\lambda(s)^{\frac{2(1+\lambda)}{1-\lambda}},
\end{gather}
where the constant $\gamma_\varepsilon \equiv \gamma(\lambda, \varepsilon)$ 
blows up as $\varepsilon^{-\frac{(1+\lambda)^2}{1-\lambda}}$ 
in the limit $\varepsilon \searrow 0$.
\end{lemma}

 We conclude the segment about the auxiliary functions and their properties 
on this occasion and arrive at the passage that treats the time mollification.

\subsection{Regularization via time mollification}

In this subsection, we  write down the weak form \eqref{GleichungSL} 
in a regularized way with the aid of a particular mollification, 
because the weak formulation proves to be unsuitable for inserting 
the testing function $\varphi$ as defined in the proof of 
Theorem \ref{ENER_SATZ}. Basically, the trouble arises from the time 
derivative of $u$, which does not need to exist, but would appear when 
calculating $\partial_t \varphi$. Thus, the objective of this paragraph 
is to find a regularized version of \eqref{GleichungSL} where choosing 
the desired testing function in the proof of Theorem \ref{ENER_SATZ} 
is no longer an issue. At first, we describe what we mean by the mollification
 of a function.

\begin{definition} \label{GlatDef} \rm
For $v \in L^1(E_T)$, we define the mollification in time by
\begin{gather*}
\llbracket v \rrbracket_h (\cdot, t) 
:= \frac{1}{h} \int_0^t e^{\frac{s-t}{h}} v(\cdot, s) \,d s\\
\intertext{and its time reversed analogue by}
\llbracket v \rrbracket_{\overline{h}} (\cdot, t) 
:= \frac{1}{h} \int_t^T e^{\frac{t-s}{h}} v(\cdot, s) \,d s
\end{gather*}
for any $h \in (0,T]$ and $t \in [0,T]$.
\end{definition}

 Before establishing the regularized version \eqref{REG} of \eqref{GleichungSL},
 we like to provide in the next lemma various useful attributes of the 
mollification (cf.\, \cite[Lemma B.2 on page 261]{BDM}, 
\cite[Lemma 2.2 on page 417]{KIN}).

\begin{lemma} \label{GlatEig}
Let $p\geq 1$ and $v\in L^1(E_T)$. Then, the mollification 
$\llbracket v \rrbracket_h$ as introduced in Definition \ref{GlatDef}
has the following properties:
\begin{enumerate}
\item[(i)] If $v\in L^p(E_T)$, then also $\llbracket v \rrbracket_h \in L^p(E_T)$, 
and the convergence $\llbracket v \rrbracket_h \to v$ in $L^p(E_T)$ as
 $h \searrow 0$ holds. \label{GlatLemmaKonv1}

\item[(ii)] If $v \in L^p\big((0,T); W^{1,p}(E)\big)$, then also 
$\llbracket v \rrbracket_h \in L^p\big((0,T); W^{1,p}(E)\big)$, 
and the convergence $\llbracket v \rrbracket_h \to v$ in 
$L^p\big((0,T); W^{1,p}(E)\big)$ as $h \searrow 0$ holds.
Moreover, we have the componentwise identity 
$D\llbracket v \rrbracket_h = \llbracket Dv \rrbracket_h$. \label{GlatLemmaGleich}

\item[(iii)] If $v\in L^\infty\big((0,T); L^2(E)\big)$, then 
$\partial_t \llbracket v \rrbracket_h \in L^\infty\big((0,T);L^2(E)\big)$.

\item[(iv)] With analogous proofs, these properties hold for the time reversed 
mollification $\llbracket v \rrbracket_{\overline{h}}$ as well.
 \label{GlatLemmaAnalog}
\end{enumerate}
\end{lemma}

 After this overview of the most important features of the mollification,
 we can go a little bit more into detail about the regularized version \eqref{REG},
 which later on allows us to apply testing functions $\varphi$ whose time
 derivative does not necessarily have to exist. This is the essential benefit
 of the formulation exposed in the upcoming theorem and makes the mollification 
argument inevitable.

\begin{theorem} \label{REG_SATZ}
If $u$ is a weak solution of the Cauchy-Dirichlet problem \eqref{PMG}, 
then its time mollification $\llbracket u \rrbracket_h$ satisfies the 
regularized variant of the inhomogeneous porous medium type equation
\begin{equation} \label{REG}
\begin{aligned}
&\iint_{E_T} \big[ \partial_t \llbracket u \rrbracket_h \varphi
 + \llbracket \mathbf{A}(x,t,u,Du)\rrbracket_h \cdot D\varphi 
- \llbracket \mathbf{B}(x,t,u,Du) \rrbracket_h \varphi \big] \,d z\\
& = \iint_{E_T} \llbracket \varphi \rrbracket_{\overline{h}} \, \,d \mu
\end{aligned}
\end{equation}
for any testing function $\varphi \in L^2\big((0,T);W^{1,2}(E)\big) 
\cap L^{\infty}(E_T)$ with compact support in $E_T$.
\end{theorem}

\begin{proof}
Let $\varphi \in L^2\big((0,T);W^{1,2}(E)\big) \cap L^{\infty}(E_T)$ 
be an arbitrary testing function with compact support in $E_T$. 
To prove the identity \eqref{REG}, we insert 
$\llbracket \varphi \rrbracket_{\overline{h}}$ as a testing function in 
the weak form \eqref{GleichungSL}. In this context, we have to note 
that $\llbracket \varphi \rrbracket_{\overline{h}}$ is a valid testing 
function in \eqref{GleichungSL} by Lemma \ref{GlatEig} and a standard
approximation argument. Analyzing all involved terms (as performed in 
\cite[Chapter 2.4 on page 3293]{BDG}), one will easily receive the 
result \eqref{REG}.
\end{proof}

 Having at hand the terms \textit{weak solution} and \textit{Riesz potential}, 
the Sobolev embedding, the auxiliary functions, and the time regularized version 
of the weak formulation of the porous medium type equation, we finish this 
part so as to reach the next segment, which revolves around another tool, 
i.\,e.\ an energy estimate, for the proof of the pointwise estimate
 \eqref{HauptBeh}.

\section{Energy estimates} \label{KAP_3}

 In this section, we  deduce the energy estimate \eqref{ENER}, which 
we require in the proof of Theorem \ref{Hauptthm}. In view of this aim, 
we first of all present parabolic cylinders, which we will use in the 
course of the following observations. For this purpose, we recall the 
upper bound $R_0>0$ for the radius, which was determined at the beginning 
of Paragraph \ref{KAP_NOT}.

\begin{definition} \rm
For $a>0$, $\varrho \in (0,R_0]$ and $z_0 = (x_0,t_0) \in \mathbb{R}^{n+1}$, 
we define parabolic cylinders by 
\begin{equation*}
Q_\varrho^{(a)}(z_0) := B_\varrho(x_0) \times \Lambda_\varrho^{(a)}(t_0) 
:= B_\varrho(x_0) \times (t_0-a^{1-m}\varrho^2, t_0).
\end{equation*}
\end{definition}

 For the sake of simplicity, we omit the (fixed) point $z_0$ in our notation 
from now on; for instance, we will write $Q_\varrho^{(a)}$ or $B_\varrho$ 
instead of $Q_\varrho^{(a)}(z_0)$ and $B_\varrho(x_0)$, respectively. 
Next, we derive the energy estimate.

\begin{theorem} \label{ENER_SATZ}
Let $\lambda \in (0,1)$, $d>0$ and further suppose that $z_0 \in \mathbb{R}^{n+1}$, 
$a>0$ and $\varrho \in (0,R_0]$ are such that
 $Q_\varrho^{(a)}(z_0) \equiv Q_\varrho^{(a)} \subset E_T$. Then, for a weak 
solution $u$ of the Cauchy-Dirichlet problem \eqref{PMG}, the energy estimate
\begin{equation} \label{ENER}
\begin{aligned}
&\sup_{t \in \Lambda_{\varrho / 2}^{(a)}} \int_{B_{\varrho / 2}
 \times \{t\} \cap \{u>a\} } G_\lambda \Big( \frac{u-a}{d} \Big) \,d x  \\ 
&+ \iint_{Q_{\varrho / 2}^{(a)} \cap \{u>a\} } 
\Big[ d^{m-1}\Big|DV_\lambda \Big( \frac{u-a}{d} \Big)\Big|^2 + a^{m-1}\Big|
DW_\lambda \Big( \frac{u-a}{d} \Big)\Big|^2 \Big] dz \\
&\leq \frac{\gamma}{\varrho^2} \iint_{Q_\varrho^{(a)} \cap \{u>a\} } u^{m-1} 
\Big( 1+ \frac{u-a}{d} \Big)^{1+\lambda} \,d z 
+ \frac{\gamma}{d\varrho} \iint_{Q_\varrho^{(a)} \cap \{u>a\} } u^m \,d z  \\ 
&\quad + \frac{\gamma}{d^2} \iint_{Q_\varrho^{(a)} \cap \{u>a\} } 
\frac{u^{m+1}}{( 1+ \frac{u-a}{d})^{1+\lambda}} \,d z 
+ \frac{\gamma\mu \big(Q_\varrho^{(a)} \big)}{d}
\end{aligned}
\end{equation}
holds with a constant $\gamma \equiv \gamma(C_0, C_1, C, m, \lambda, R_0)$.
\end{theorem}

\begin{proof}
Let $u$ be a weak solution of \eqref{PMG} in the sense of Definition \ref{DefSL}. 
In the regularized form \eqref{REG}, we choose the testing function 
$\varphi := \eta^2 \zeta v$, where $v$ is given by
\begin{equation*}
v := g(u) := 1- \Big( 1+ \frac{(u-a)_+}{d} \Big)^{-\lambda},
\end{equation*}
$\eta \in C_0^1(B_\varrho(x_0), [0,1])$ is a function with $\eta \equiv 1$ 
on $B_{\varrho / 2}(x_0)$ and $|D\eta| \leq \frac{4}{\varrho}$, and
$\zeta \in W_0^{1,\infty}(\mathbb{R}, [0,1])$ fulfills
\begin{equation*}
\zeta(t) := \begin{cases} 
0 & \text{for } t \in (-\infty, t_0-a^{1-m}\varrho^2) \cup [\tau,\infty), \\ 
\frac{4a^{m-1}}{3\varrho^2} \big(t-(t_0-a^{1-m}\varrho^2) \big) 
 & \text{for } t \in [t_0-a^{1-m}\varrho^2, t_0-a^{1-m}(\frac{\varrho}{2})^2), \\ 
1 & \text{for } t \in [t_0-a^{1-m}(\frac{\varrho}{2})^2, \tau-\varepsilon), \\ 
\frac{1}{\varepsilon} (\tau-t) & \text{for } t \in [\tau-\varepsilon, \tau) 
\end{cases}
\end{equation*}
for a fixed $\tau \in \Lambda_{\varrho / 2}^{(a)}$ and $\varepsilon > 0$. 
To avoid an overburdened notation, we employ the abbreviations
\begin{gather*}
Q^+ := Q_\varrho^{(a)}(z_0) \cap \{u>a\} 
= \big(B_\varrho(x_0) \times (t_0-a^{1-m}\varrho^2, t_0) \big) \cap \{u>a\},\\
B^+(t) := B_\varrho(x_0) \cap \{u(\cdot, t) >a\}.
\end{gather*}
Since $u$ is a weak solution of \eqref{PMG}, by Theorem \ref{REG_SATZ} the 
identity \eqref{REG} holds, which we now insert the above concrete
testing function $\varphi$ in. Using the shortcuts
\begin{align}
 \textup{I}^{(1)} &:= \iint_{E_T} \partial_t \llbracket u
 \rrbracket_h \varphi \,d z, \label{I1} \\
 \textup{II}^{(1)} &:= \iint_{E_T} \llbracket \mathbf{A}(x,t,u,Du)\rrbracket_h
 \cdot D\varphi \,d z, \label{II1} \\
 \textup{III}^{(1)} &:= \iint_{E_T} \llbracket \mathbf{B}(x,t,u,Du)
 \rrbracket_h \varphi \,d z, \label{III1}\\
\textup{IV}^{(1)} &:= \iint_{E_T} \llbracket \varphi
\rrbracket_{\overline{h}} \, \,d \mu, \label{IV1}
\end{align}
we obtain the equation
\begin{equation} \label{I1II1III1IV1}
 \textup{I}^{(1)} +  \textup{II}^{(1)}
-  \textup{III}^{(1)} - \textup{IV}^{(1)} = 0.
\end{equation}
In the following, we will separately estimate the terms \eqref{I1}-\eqref{IV1}, 
starting with \eqref{I1}. As $g$ is increasing, the identity 
$\partial_t \llbracket u \rrbracket_h = -\frac{1}{h}(\llbracket u \rrbracket_h-u)$ 
implies
\begin{equation*}
\partial_t \llbracket u \rrbracket_h \big(g(u) - g(\llbracket u \rrbracket_h)\big) 
= \frac{1}{h} \big(\llbracket u \rrbracket_h-u\big) \big(g(\llbracket u \rrbracket_h)
-g(u) \big) \geq 0
\end{equation*}
which yields
\begin{equation} \label{AbschI1}
\begin{aligned}
 \textup{I}^{(1)}
&= \iint_{E_T} \partial_t \llbracket u \rrbracket_h \varphi \,d z  \\ 
&\geq \iint_{Q^+} \eta^2\zeta \partial_t \llbracket u \rrbracket_h 
 g(\llbracket u \rrbracket_h) \,d z  \\ 
& = \iint_{Q^+} \eta^2\zeta \frac{\partial}{\partial t} 
 \Big[ \int_a^{\llbracket u \rrbracket_h} g(\sigma) \,d \sigma \Big] \, dz  \\ 
&= - \iint_{Q^+} \eta^2 \partial_t \zeta \int_a^{\llbracket u \rrbracket_h} 
g(\sigma) \,d \sigma \,d z  \\ 
&= -\frac{4a^{m-1}}{3\varrho^2} \int_{t_0-a^{1-m}\varrho^2}^{t_0-a^{1-m}
(\varrho / 2)^2} \int_{B^+(t)} \eta^2 \int_a^{\llbracket u \rrbracket_h}
 g(\sigma) \,d \sigma \,d x \,d t  \\ 
&\quad+ \frac{1}{\varepsilon} \int_{\tau-\varepsilon}^\tau \int_{B^+(t)} \eta^2 
\int_a^{\llbracket u \rrbracket_h} g(\sigma) \,d \sigma \,d x \,d t  \\ 
&=:  \textup{I}^{(2)}(h) +  \textup{II}^{(2)}(h,\varepsilon).
\end{aligned}
\end{equation}
First, we consider $ \textup{II}^{(2)}(h,\varepsilon)$.
Passing to the limits $\varepsilon \searrow 0$ and $h \searrow 0$, by the 
Lebesgue differentiation theorem we receive
\begin{equation} \label{AbschII2}
\begin{aligned}
\lim_{h \searrow 0} \lim_{\varepsilon \searrow 0} 
 \textup{II}^{(2)}(h,\varepsilon)
&= \lim_{h \searrow 0} \lim_{\varepsilon \searrow 0}\, 
-\hspace{-3.9mm}\int_{\tau-\varepsilon}^\tau \int_{B^+(t)} \eta^2 
\int_a^{\llbracket u \rrbracket_h(x,t)} g(\sigma) \,d \sigma \,d x \,d t  \\ 
&= \lim_{h \searrow 0} \int_{B^+(\tau)} \eta^2 
\int_a^{\llbracket u \rrbracket_h(x,\tau)} 
\Big[ 1- \Big( 1+ \frac{\sigma-a}{d} \Big)^{-\lambda} \Big] d \sigma \,d x  \\ 
&= d \int_{B^+(\tau)} \eta^2 \Big[ \frac{u-a}{d} - \frac{1}{1-\lambda} 
\Big( \Big( 1+ \frac{u-a}{d} \Big)^{1-\lambda} -1 \Big) \Big] dx  \\ 
&= d \int_{B^+(\tau)} \eta^2 G_\lambda \Big( \frac{u-a}{d} \Big) \,d x
\end{aligned}
\end{equation}
for a.\,e.\ $\tau \in \Lambda_{\varrho / 2}^{(a)}$, where we have exploited the 
$L^2$-convergence $\llbracket u \rrbracket_h \to u$ as $h \searrow 0$ 
(cf.\ Lemma \ref{GlatEig}). Next, we let $h \searrow 0$ also in the term
$ \textup{I}^{(2)}(h)$ which results in
\begin{equation} \label{AbschI2}
\begin{aligned}
\lim_{h \searrow 0} |  \textup{I}^{(2)}(h) |
&\leq \frac{4d}{3\varrho^2} \int_{t_0-a^{1-m}\varrho^2}^{t_0} 
\int_{B^+(t)} \eta^2 a^{m-1} \frac{u-a}{d} \,d x \,d t  \\ 
&\leq \frac{4d}{3\varrho^2} \int_{t_0-a^{1-m}\varrho^2}^{t_0} 
\int_{B^+(t)} u^{m-1} \Big( 1+ \frac{u-a}{d} \Big)^{1+\lambda} \,d x \,d t.
\end{aligned}
\end{equation}
To get this, we have used the inequality $g(\sigma) \leq 1$ for $\sigma \geq a$, 
enlarged the domain of integration, and in the last step estimated $\eta \leq 1$, 
$a \leq u$ and 
\[
\frac{u-a}{d} \leq 1+\frac{u-a}{d} \leq \Big(1+ \frac{u-a}{d}\Big)^{1+\lambda}
\]
 on the domain of integration. Inserting \eqref{AbschII2} and \eqref{AbschI2} 
in \eqref{AbschI1}, we can record as an interim conclusion the lower bound
\begin{equation} \label{ZWFaz1}
\begin{aligned}
\lim_{h \searrow 0} \lim_{\varepsilon \searrow 0}  \textup{I}^{(1)}
&\geq d \int_{B^+(\tau)} \eta^2 G_\lambda \Big( \frac{u-a}{d} \Big) \,d x\\
&\quad - \frac{4d}{3\varrho^2} \int_{t_0-a^{1-m}\varrho^2}^{t_0} 
\int_{B^+(t)} u^{m-1} \Big( 1+ \frac{u-a}{d} \Big)^{1+\lambda} \,d x \,d t
\end{aligned}
\end{equation}
for $ \textup{I}^{(1)}$, which holds for a.\,e.\
$\tau \in \Lambda_{\varrho / 2}^{(a)}$. In the following, we deal with the 
term $ \textup{II}^{(1)}$. Again building the limits
$\varepsilon \searrow 0$ and $h \searrow 0$, we find
\begin{equation} \label{AbschII1}
\begin{aligned}
\lim_{h \searrow 0} \lim_{\varepsilon \searrow 0}  \textup{II}^{(1)}
&= \iint_{Q^+} \mathbf{A}(x,t,u,Du) \cdot D\varphi \,d z  \\ 
&= \iint_{Q^+} \eta^2\zeta \mathbf{A}(x,t,u,Du) \cdot Dv \,d z \\
&\quad + 2 \iint_{Q^+} \eta\zeta v \mathbf{A}(x,t,u,Du) \cdot D\eta \,d z  \\ 
&=:  \textup{I}^{(3)} +  \textup{II}^{(3)}.
\end{aligned}
\end{equation}
Before turning towards the term $ \textup{II}^{(3)}$, we treat
the term $ \textup{I}^{(3)}$. Having in mind the ellipticity
condition \eqref{WEB1}, we compute for the latter
\begin{equation} \label{AbschI3}
\begin{aligned}
 \textup{I}^{(3)}
&= \frac{\lambda}{d} \iint_{Q^+} \eta^2\zeta 
\Big( 1+ \frac{u-a}{d} \Big)^{-1-\lambda} \mathbf{A}(x,t,u,Du) \cdot Du \,d z  \\ 
&\geq \frac{\lambda C_0 m}{d} \iint_{Q^+} \eta^2\zeta
 \frac{u^{m-1} |Du|^2}{(1+ \frac{u-a}{d})^{1+\lambda}} \,d z 
- \frac{\lambda C^2}{d} \iint_{Q^+} \frac{u^{m+1}}{(1+ \frac{u-a}{d})^{1+\lambda}} 
\,d z.
\end{aligned}
\end{equation}
For the other term, we exploit in turn the fact that $v \leq 1$, the growth 
condition \eqref{WEB2}, the bounds $|D\eta| \leq \frac{4}{\varrho}$ and 
$\eta\zeta \leq 1$, Young's inequality, and $\zeta \leq 1$ to conclude that
\begin{equation} \label{AbschII3}
\begin{aligned}
| \textup{II}^{(3)}|
&\leq 2 \iint_{Q^+} \eta\zeta v |\mathbf{A}(x,t,u,Du)| |D\eta| \,d z  \\ 
&\leq \frac{8C_1 m}{\varrho} \iint_{Q^+} \eta\zeta u^{m-1} |Du| \,d z 
 + \frac{8C}{\varrho} \iint_{Q^+} u^m \,d z  \\ 
&\leq \frac{\lambda C_0 m}{2d} \iint_{Q^+} \eta^2\zeta 
 \frac{u^{m-1}|Du|^2 }{(1+ \frac{u-a}{d})^{1+\lambda}} \,d z \\
&\quad + \frac{64m C_1^2 d}{2\lambda C_0 \varrho^2} \iint_{Q^+} u^{m-1} 
\Big( 1+ \frac{u-a}{d} \Big)^{1+\lambda} \,d z  
 + \frac{8C}{\varrho} \iint_{Q^+} u^m \,d z.
\end{aligned}
\end{equation}
Combining \eqref{AbschI3} and \eqref{AbschII3} with \eqref{AbschII1} leads us 
to the estimate
\begin{equation} \label{ZWFaz2}
\begin{aligned}
&\lim_{h \searrow 0} \lim_{\varepsilon \searrow 0}  \textup{II}^{(1)}\\
 &\geq \frac{\lambda C_0 m}{2d} \iint_{Q^+} \eta^2\zeta 
\frac{u^{m-1}|Du|^2 }{(1+ \frac{u-a}{d})^{1+\lambda}} \,d z
 - \frac{\lambda C^2}{d} \iint_{Q^+} \frac{u^{m+1}}{(1+ \frac{u-a}{d})^{1+\lambda}} 
\,d z  \\ 
&\quad- \frac{32m C_1^2 d}{\lambda C_0 \varrho^2} \iint_{Q^+} u^{m-1} 
\Big( 1+ \frac{u-a}{d} \Big)^{1+\lambda} \,d z - \frac{8C}{\varrho} 
\iint_{Q^+} u^m \,d z
\end{aligned}
\end{equation}
as an outcome of our thoughts on the term $ \textup{II}^{(1)}$.
We now give our attention to the third summand of \eqref{I1II1III1IV1}, 
initially letting $\varepsilon \searrow 0$ and $h \searrow 0$ and subsequently 
using $v\leq 1$, the growth condition \eqref{WEB3}, the fact that 
$\eta^2\zeta \leq 1$, and finally Young's inequality to obtain
\begin{equation} \label{ZWFaz3}
\begin{aligned}
&|\lim_{h \searrow 0} \lim_{\varepsilon \searrow 0}  \textup{III}^{(1)}| \\
&\leq \iint_{Q^+} \eta^2\zeta v |\mathbf{B}(x,t,u,Du)| \,d z  \\ 
&\leq Cm \iint_{Q^+} \eta^2\zeta u^{m-1} |Du| \,d z + C^2 \iint_{Q^+} u^m \,d z  \\ 
&\leq \frac{\lambda C_0 m}{4d} \iint_{Q^+} \eta^2 \zeta 
 \frac{u^{m-1}|Du|^2}{(1+ \frac{u-a}{d})^{1+\lambda}} \,d z\\
&\quad  + \frac{dmC^2}{\lambda C_0} \iint_{Q^+} u^{m-1} 
 \Big( 1+ \frac{u-a}{d} \Big)^{1+\lambda} \,d z  
 + C^2 \iint_{Q^+} u^m \,d z.
\end{aligned}
\end{equation}
It remains to estimate the term $\textup{IV}^{(1)}$.
Passing to the limits first and then applying Lemma \ref{GlatEig} and
$\varphi \leq 1$, we have
\begin{equation} \label{ZWFaz4}
\lim_{h \searrow 0} \lim_{\varepsilon \searrow 0} \textup{IV}^{(1)}
 = \lim_{h \searrow 0} \iint_{Q^+} \llbracket \varphi \rrbracket_{\overline{h}} \,
 \,d \mu = \iint_{Q^+} \varphi \,d \mu \leq \mu(Q^+).
\end{equation}
This completes the evaluations of the terms appearing in \eqref{I1II1III1IV1}, 
and we can insert the results \eqref{ZWFaz1} and \eqref{ZWFaz2}-\eqref{ZWFaz4} 
there. 
Noting that the inclusions $Q^+ \supset Q_\ast$ 
(where $Q_\ast := B_{\varrho /2} \times (t_0-a^{1-m}
(\tfrac{\varrho}{2})^2, \tau) \cap \{ u > a \}$) and 
$B^+(\tau) \supset B_{\varrho /2} \cap \{ u(\cdot,\tau) > a \}$ hold, 
(\ref{I1II1III1IV1}) gives 
\begin{equation} \label{ENER_ZW1}
\begin{aligned}
&\int_{B_{\varrho /2} \times \{\tau\} \cap \{ u > a \}} \eta^2 G_\lambda 
\Big( \frac{u-a}{d} \Big) \,d x + \frac{\lambda C_0 m}{4d^2} 
\iint_{Q_\ast} \eta^2\zeta \frac{u^{m-1}|Du|^2 }{(1+ \frac{u-a}{d})^{1+\lambda}} 
\,d z  \\ 
&\leq \Big( \frac{4}{3\varrho^2} + \frac{32m C_1^2}{\lambda C_0 \varrho^2} 
 + \frac{mC^2}{\lambda C_0}\Big) \iint_{Q^+} u^{m-1} 
 \Big( 1+ \frac{u-a}{d} \Big)^{1+\lambda} \,d z  \\ 
&\quad + \frac{1}{d} \Big( \frac{8C}{\varrho} + C^2 \Big) 
 \iint_{Q^+} u^m \,d z + \frac{\lambda C^2}{d^2} 
 \iint_{Q^+} \frac{u^{m+1}}{(1+ \frac{u-a}{d})^{1+\lambda}} \,d z 
 + \frac{\mu(Q^+)}{d}
\end{aligned}
\end{equation}
for a.\,e.\ $\tau \in \Lambda_{\varrho /2}^{(a)}$. Since $\eta \equiv 1$ 
on $B_{\varrho /2}$ and $\zeta \equiv 1$ on 
$(t_0-a^{1-m} (\frac{\varrho}{2})^2, \tau)$, by respectively taking the 
supremum over all $\tau \in \Lambda_{\varrho / 2}^{(a)}$ we infer from 
\eqref{ENER_ZW1} that both
\begin{gather*}
\sup_{t \in \Lambda_{\varrho / 2}^{(a)}} \int_{B_{\varrho /2} 
\times \{t\} \cap \{ u > a \}} G_\lambda \Big( \frac{u-a}{d} \Big) \,d x,\\
\frac{\lambda C_0 m}{4d^2} \iint_{Q_{\varrho /2}^{(a)} \cap \{ u > a \}} 
 \frac{u^{m-1}|Du|^2 }{(1+ \frac{u-a}{d})^{1+\lambda}} \,d z
\end{gather*}
can be bounded by the right-hand side of \eqref{ENER_ZW1} which easily leads us to
\begin{equation} \label{ENER_ZW3}
\begin{aligned}
&\sup_{t \in \Lambda_{\varrho / 2}^{(a)}} \int_{B_{\varrho / 2} \times \{t\} 
 \cap \{u>a\}} G_\lambda \Big( \frac{u-a}{d} \Big) \,d x 
 + \frac{\lambda}{d^2} \iint_{Q_{\varrho /2}^{(a)} \cap \{u>a\}} 
 \frac{u^{m-1}|Du|^2 }{(1+ \frac{u-a}{d})^{1+\lambda}} \,d z  \\ 
&\leq \frac{\gamma}{\varrho^2} \iint_{Q_\varrho^{(a)} \cap \{u>a\}} u^{m-1} 
\Big( 1+ \frac{u-a}{d} \Big)^{1+\lambda} \,d z + \frac{\gamma}{d\varrho} 
\iint_{Q_\varrho^{(a)} \cap \{u>a\}} u^m \,d z  \\ 
&\quad + \frac{\gamma}{d^2} \iint_{Q_\varrho^{(a)} \cap \{u>a\}} 
 \frac{u^{m+1}}{(1+ \frac{u-a}{d})^{1+\lambda}} \,d z
  + \frac{\gamma\mu\big(Q_\varrho^{(a)}\big)}{d}
\end{aligned}
\end{equation}
with a constant $\gamma \equiv \gamma(C_0,C_1,C,m,\lambda,R_0)$. 
On the set $Q_{\varrho /2}^{(a)} \cap \{u>a\}$, we have
\begin{equation*}
DV_\lambda \Big(\frac{u-a}{d} \Big) 
= \Big(\frac{u-a}{d} \Big)^{\frac{m-1}{2}} \Big(1+ \frac{u-a}{d} \Big)
^{-\frac{1+\lambda}{2}}\, \frac{Du}{d},
\end{equation*}
 on the other hand, there holds
\begin{equation*}
DW_\lambda \Big(\frac{u-a}{d} \Big) 
= \Big(1+ \frac{u-a}{d} \Big)^{-\frac{1+\lambda}{2}}\, \frac{Du}{d}
\end{equation*}
which together yields
\begin{align*}
&d^{m-1} \Big| DV_\lambda \Big(\frac{u-a}{d} \Big) \Big|^2 
+ a^{m-1} \Big| DW_\lambda \Big(\frac{u-a}{d} \Big) \Big|^2 \\
&= \frac{|Du|^2}{d^2} \Big(1+ \frac{u-a}{d} \Big)^{-(1+\lambda)}\, 
\big[(u-a)^{m-1} + a^{m-1}\big] \\ 
&\leq \frac{|Du|^2}{d^2} \Big(1+ \frac{u-a}{d} \Big)^{-(1+\lambda)}\, 2 u^{m-1}.
\end{align*}
Hence, we are allowed to rewrite \eqref{ENER_ZW3} in the form
\begin{equation} \label{ENER_ZW4}
\begin{aligned}
&\sup_{t \in \Lambda_{\varrho / 2}^{(a)}} \int_{B_{\varrho / 2} 
\times \{t\} \cap \{u>a\}} G_\lambda \Big( \frac{u-a}{d} \Big) \,d x  \\ 
&+ \frac{\lambda}{2} \iint_{Q_{\varrho /2}^{(a)} \cap \{u>a\}} 
\Big[ d^{m-1} \Big| DV_\lambda \Big(\frac{u-a}{d} \Big) \Big|^2 
+ a^{m-1} \Big| DW_\lambda \Big(\frac{u-a}{d} \Big) \Big|^2 \Big] dz  \\ 
&\leq \frac{\gamma}{\varrho^2} \iint_{Q_\varrho^{(a)} \cap \{u>a\}} u^{m-1} 
\Big( 1+ \frac{u-a}{d} \Big)^{1+\lambda} \,d z 
+ \frac{\gamma}{d\varrho} \iint_{Q_\varrho^{(a)} \cap \{u>a\}} u^m \,d z  \\ 
&\quad + \frac{\gamma}{d^2} \iint_{Q_\varrho^{(a)} \cap \{u>a\}} 
\frac{u^{m+1}}{(1+ \frac{u-a}{d})^{1+\lambda}} \,d z
 + \frac{\gamma\mu\big(Q_\varrho^{(a)}\big)}{d}.
\end{aligned}
\end{equation}
As $\lambda \in (0,1)$, the inequality \eqref{ENER_ZW4} remains true if we
 multiply the term involving the supremum by $\frac{\lambda}{2}$. 
After that, the assertion \eqref{ENER} eventually results from dividing 
the whole inequality by $\frac{\lambda}{2}$. 
\end{proof}

 The energy estimate \eqref{ENER} is now at our disposal, and we end this 
paragraph. Moreover, we have finished the preparations for the proof of 
Theorem \ref{Hauptthm}, which permits us to head for this central statement.


\section{Proof of Theorem \ref{Hauptthm}} \label{KAP_4}

 We arrive at the core of this report. The instruments developed in the previous
 two sections enable us to explicitly prove the pointwise estimate \eqref{HauptBeh}
for weak solutions of the Cauchy-Dirichlet problem \eqref{PMG} for the 
nonhomogeneous porous medium type equation.

\begin{proof}
We will proceed as described in Section \ref{KAP1.5}.

\subsection{Choice of parameters} \label{KAP_4.1}

In this segment, we will provide cylinders and parameters which later on 
will turn out to be suitable, when inserted in the energy estimate \eqref{ENER}. 
Therefore, we have to mention the quantities $\mathbf{K}_j$ and
$\mathbf{k}_j$ that will show up in a natural way in the proof, which 
is why we will additionally detect some of their features in this passage. 
What is more, we will outline several expedient relations between functions, 
cylinders etc. that will emerge in the further course of the proof. 

 Let $\lambda \in (0, \frac{1}{n}]$ and $Q_{r,\theta}(z_0) \Subset E_T$, 
where $r \in (0,R_0]$ and $\theta > 0$. As before, we omit the center $z_0$ 
in our notation. For $j \in \mathbb{N}_0$, we define sequences of radii 
$$
r_j := \frac{r}{2^j},
$$ 
parameters 
$$
\theta_j := \frac{\theta}{2^{2j}},
$$ 
and cylinders 
$$
Q_j := B_j \times \Lambda_j := B_{r_j} \times (t_0 - a_j^{1-m} r_j^2, t_0),
$$ 
where the quantities $a_j$ will be chosen inductively below. We set 
$$
a_0 := \Big( \frac{r^2}{\theta} \Big)^{\frac{1}{m-1}}
$$ 
and assume for $j \geq 0$ that $a_0, \dots, a_j$ have already been specified. 
For the purpose of selecting $a_{j+1}$, we first define
\begin{equation*}
\mathbf{K}_j(a) := \frac{1}{r_j^{n+2}} \iint_{Q_j \cap \{u>a_j\} } u^{m-1} 
\Big( \frac{u-a_j}{a-a_j} \Big)^{1+\lambda} \,d z
\end{equation*}
for $a>a_j$ and observe the convergence $\mathbf{K}_j(a) \to 0$ as $a \to \infty$. 
Let $\kappa \in (0,1)$ be a fixed parameter which we will determine later. 
Then we choose
\begin{equation} \label{DEFaj+1A}
a_{j+1} := \big[1+2^{-(j+2)} \big] a_j
\end{equation}
if
\begin{equation} \label{DEFaj+1ABed}
\mathbf{K}_j\left([1+2^{-(j+2)}] a_j\right) \leq \kappa
\end{equation}
holds, and
\begin{equation} \label{DEFaj+1B}
a_{j+1} := \sup\big\{ a \in \big([1+2^{-(j+2)}] a_j, \infty \big) : 
\mathbf{K}_j(a) > \kappa \big\},
\end{equation}
provided that we have
\begin{equation*}
\mathbf{K}_j\big([1+2^{-(j+2)}] a_j\big) > \kappa.
\end{equation*}
When $a_{j+1}$ is defined as in \eqref{DEFaj+1B}, there hold
\begin{equation} \label{KjaJ+1=kappa}
\mathbf{K}_j(a_{j+1}) = \kappa
\end{equation}
and $a_{j+1} > \big[1+ 2^{-(j+2)}\big] a_j$, because the mapping 
$\mathbf{K}_j: (a_j,\infty) \to \mathbb{R}$ is continuous and decreasing. 
In both cases, \eqref{DEFaj+1A} and \eqref{DEFaj+1B}, we set 
$d_j := a_{j+1}-a_j$ for $j \in \mathbb{N}_0$ and define 
$$
\mathbf{k}_j := \mathbf{K}_j(a_{j+1}),
$$
which satisfies
\begin{equation} \label{Absch_kj}
\mathbf{k}_j = \frac{1}{r_j^{n+2}} \iint_{Q_j \cap \{u>a_j\} } u^{m-1} 
\Big( \frac{u-a_j}{d_j} \Big)^{1+\lambda} \,d z \leq \kappa
\end{equation}
for any $j \in \mathbb{N}_0$, since we have \eqref{DEFaj+1ABed} if $a_{j+1}$ 
is defined via \eqref{DEFaj+1A}, and, in the case that $a_{j+1}$ 
is given by \eqref{DEFaj+1B}, there even holds equality in \eqref{Absch_kj} 
by \eqref{KjaJ+1=kappa}. In order to be enabled to replace $u$ 
by $u-a_{j-1}$ later in the proof, we need the estimation
\begin{equation} \label{u->u-aj-1}
u \leq 2^{j+2} (u-a_{j-1})
\end{equation}
for any $j \in \mathbb{N}$ on the set $\{ u>a_j \}$, which we briefly establish 
in the following. Both if $a_j$ is defined as in \eqref{DEFaj+1A} and if $a_j$ 
is stated in \eqref{DEFaj+1B}, there holds 
$a_j \geq \big[1+ 2^{-(j+1)}\big] a_{j-1}$, or equivalently, 
$a_j-a_{j-1} \geq 2^{-(j+1)} a_{j-1}$. This leads us to the estimate
\begin{equation} \label{AbschInBeh3}
\frac{a_j}{a_j-a_{j-1}} = 1 + \frac{a_{j-1}}{a_j-a_{j-1}} \leq 2^{j+2}.
\end{equation}

On $\{u>a_j\}$, we compute $\big(1-\tfrac{a_{j-1}}{a_j}\big) u = u - a_{j-1} 
+ \tfrac{a_{j-1}}{a_j} (a_j-u) \leq u - a_{j-1}$, and using the inequality 
\eqref{AbschInBeh3}, we obtain
 $u \leq \tfrac{a_j}{a_j - a_{j-1}} (u-a_{j-1}) \leq 2^{j+2} (u-a_{j-1})$.
We terminate this paragraph with two statements regarding the previously 
initiated cylinders. To begin with, due to the fact that $2r_{j+1} = r_j$ 
and $a_{j+1} > a_j$, we infer the inclusion
\begin{equation} \label{ZylAbsch}
2Q_{j+1} \subset Q_j
\end{equation}
for any $j \in \mathbb{N}_0$, and, furthermore, we have
\begin{equation} \label{Zyl2Absch}
Q_j \subset Q_{r_j, \theta_j}
\end{equation}
for any $j \in \mathbb{N}_0$, since $a_j \geq a_0 = (r^2 / \theta)^{\frac{1}{m-1}}$ 
and thus $a_j^{1-m} r_j^2 \leq \frac{\theta}{r^2} r_j^2 = \theta_j$ holds.

\subsection{Recursive bounds for $\boldsymbol{d_j}$} 
\label{KAP_4.2}

Having prepared the sequences $(Q_j)_{j\in\mathbb{N}_0}$, $(a_j)_{j\in\mathbb{N}_0}$ and
 $(d_j)_{j\in\mathbb{N}_0}$, we arrive at this section whose objective is to show that 
the inequality
\begin{equation} \label{4.6}
d_j \leq \frac{1}{2} d_{j-1} + 2^{-(j+2)} a_j 
+ \frac{\gamma\mu (2Q_{r_j, \theta_j})}{r_j^n}
\end{equation}
is valid for any $j \in \mathbb{N}$, where $\gamma \equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0)$ 
is a constant. We will roughly proceed as follows: After various introductory 
comments, we will apply the energy estimate \eqref{ENER} with the concrete 
cylinders and parameters from Chapter \ref{KAP_4.1} and modify the outcome 
until we reach the assertion \eqref{4.10}. Next, we estimate by the right-hand 
side of \eqref{4.13} the terms $ \textup{I}^{(5)}$ and
$ \textup{II}^{(5)}$ which will occur in a natural way in \eqref{4.11}.
 To achieve this, we will repeatedly avail ourselves to the 
Gagliardo-Nirenberg inequality \eqref{GNU} and the energy estimate in its 
version \eqref{4.10}. Then, immediately after rewriting \eqref{4.13} 
in the more convenient form \eqref{HausVomNikoUMG} and a simple case analysis, 
the conclusion \eqref{4.6} ensues. 

 We start our considerations by excluding certain trivial cases. 
According to \eqref{Absch_kj}, we have $\mathbf{k}_j \leq \kappa$ for 
any $j \in \mathbb{N}_0$. If $\mathbf{k}_j < \kappa$ holds, $a_{j+1}$ is defined
 via \eqref{DEFaj+1A}, meaning that we have $a_{j+1} = [1+2^{-(j+2)}] a_j$,
 which is equivalent to $d_j = 2^{-(j+2)}a_j$, so that \eqref{4.6} is
 obviously satisfied. Consequently, let
\begin{equation} \label{k_j=kappa}
\mathbf{k}_j = \kappa
\end{equation}
from now on. Moreover, we can assume without loss of generality that
\begin{equation} \label{dj>dj-1}
d_j > \frac{1}{2} d_{j-1}
\end{equation}
holds, since otherwise we would have $d_j \leq \frac{1}{2} d_{j-1}$ 
which again instantly implies \eqref{4.6}. Before approaching the proof 
of the bound \eqref{4.6}, we shall establish some helpful estimates 
which we will frequently require later on. For one thing, we have
\begin{equation} \label{4.7}
1 = \frac{a_j - a_{j-1}}{d_{j-1}} \leq \frac{u - a_{j-1}}{d_{j-1}}
\end{equation}
on the set $2Q_j \cap \{u>a_j\}$, for another thing, the inequality
\begin{equation} \label{4.8}
\frac{u - a_j}{d_j} \leq \frac{u - a_{j-1}}{d_j} 
\leq 2 \frac{u - a_{j-1}}{d_{j-1}}
\end{equation}
holds on $2Q_j \cap \{u>a_j\}$ by the fact that $a_j > a_{j-1}$ 
and the assumption \eqref{dj>dj-1} from above. Beyond that, we use 
the observation \eqref{4.7} and the identity $\frac{1}{r_j} = \frac{2}{r_{j-1}}$, 
extend the domain of integration (note that $a_j > a_{j-1}$ and 
$2Q_j \subset Q_{j-1}$ by \eqref{ZylAbsch}), and finally consult the 
property \eqref{Absch_kj} of $\mathbf{k}_{j-1}$ to obtain
\begin{equation} \label{4.9}
\begin{aligned}
&\frac{1}{r_j^{n+2}} \iint_{Q_j \cap \{u>a_j\} } u^{m-1} \,d z \\
&\leq \frac{1}{r_j^{n+2}} \iint_{2Q_j \cap \{u>a_j\} } u^{m-1} \,d z  \\ 
&\leq \frac{1}{r_j^{n+2}} \iint_{2Q_j \cap \{u>a_j\} } u^{m-1} 
\Big( \frac{u-a_{j-1}}{d_{j-1}} \Big)^{1+\lambda} \,d z  \\ 
&\leq \frac{2^{n+2}}{r_{j-1}^{n+2}} \iint_{Q_{j-1} \cap \{u>a_{j-1}\} } u^{m-1} 
\Big( \frac{u-a_{j-1}}{d_{j-1}} \Big)^{1+\lambda} \,d z  \\ 
&= 2^{n+2} \mathbf{k}_{j-1} \leq 2^{n+2}\kappa.
\end{aligned}
\end{equation}
This completes the preliminary thoughts of this section, and we now devote 
ourselves to the energy estimate with the concrete quantities from 
Section \ref{KAP_4.1}. To this end, we fix $\lambda \in (0, \frac{1}{n}]$ 
and apply \eqref{ENER} with the cylinder $2Q_j$ in lieu of $Q_\varrho^{(a)}$, 
also replacing the parameters $(a,d)$ from Theorem \ref{ENER_SATZ} by
 $(a_j, d_j)$. This yields
\begin{equation} \label{HausVomNiko}
\begin{aligned}
&\sup_{t \in \Lambda_j} \int_{B_j \times \{t\} \cap \{u>a_j\} } 
G_\lambda \Big( \frac{u-a_j}{d_j} \Big) \,d x  \\ 
&+ \iint_{Q_j \cap \{u>a_j\} } \Big[ d_j^{m-1}\Big|DV_\lambda 
\Big( \frac{u-a_j}{d_j} \Big)\Big|^2 + a_j^{m-1}\Big|DW_\lambda 
\Big( \frac{u-a_j}{d_j} \Big)\Big|^2 \Big] \,d z  \\ 
&\leq \frac{\gamma}{r_j^2} \iint_{2Q_j \cap \{u>a_j\} } u^{m-1} 
 \Big( 1+ \frac{u-a_j}{d_j} \Big)^{1+\lambda} \,d z 
 + \frac{\gamma}{d_j r_j} \iint_{2Q_j \cap \{u>a_j\} } u^m \,d z  \\
 &\quad + \frac{\gamma}{d_j^2} \iint_{2Q_j \cap \{u>a_j\} } 
\frac{u^{m+1}}{ (1+ \frac{u-a_j}{d_j})^{1+\lambda}} \,d z
 + \frac{\gamma\mu (2Q_j)}{d_j}  \\ 
&=:  \textup{I}^{(4)} +  \textup{II}^{(4)}
+  \textup{III}^{(4)} + \frac{\gamma\mu ( 2Q_j )}{d_j}.
\end{aligned}
\end{equation}
In turn, we examine the terms $ \textup{I}^{(4)}$,
$ \textup{II}^{(4)}$ and $ \textup{III}^{(4)}$, starting
with $ \textup{I}^{(4)}$. With the aid of the inequalities
\eqref{4.7} and \eqref{4.8} in the first and \eqref{4.9} in the second step, 
respectively, we compute
\begin{equation} \label{AbschI4}
 \textup{I}^{(4)}
\leq \gamma \frac{1}{r_j^2} \iint_{2Q_j \cap \{u>a_j\} } u^{m-1} 
\Big( \frac{u-a_{j-1}}{d_{j-1}} \Big)^{1+\lambda} \,d z \leq \gamma r_j^n\kappa
\end{equation}
for a constant $\gamma \equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0)$. 
Estimating $u$ via \eqref{u->u-aj-1} and successively using the assumption 
\eqref{dj>dj-1}, the fact that $2^j = \frac{r}{r_j} \leq \frac{R_0}{r_j}$, 
the observation \eqref{4.7}, and ultimately the inequality \eqref{4.9}, we find
\begin{equation} \label{AbschII4}
\begin{aligned}
 \textup{II}^{(4)}
&= \frac{\gamma}{d_j r_j} \iint_{2Q_j \cap \{u>a_j\} } u^{m-1}u \, \,d z \\
&\leq \gamma \frac{2^j}{r_j} \iint_{2Q_j \cap \{u>a_j\} } u^{m-1} 
 \frac{u-a_{j-1}}{d_j} \,d z  \\ 
&\leq  \gamma \frac{1}{r_j^2} \iint_{2Q_j \cap \{u>a_j\} } u^{m-1} 
\Big( \frac{u-a_{j-1}}{d_{j-1}} \Big)^{1+\lambda} \,d z 
\leq \gamma r_j^n\kappa
\end{aligned}
\end{equation}
for the second term. Before discussing the term $ \textup{III}^{(4)}$,
we convince ourselves that on the domain of integration, there holds
\begin{equation} \label{VorüberFürIII4}
\begin{aligned}
\frac{u}{1+\frac{u-a_j}{d_j}} 
&\leq 2^{j+2} \frac{(u-a_{j-1})d_j}{d_j+u-a_j}
 = 2^{j+2} \Big[ \frac{(u-a_j)d_j}{d_j+u-a_j} 
+ \frac{(a_j-a_{j-1})d_j}{d_j+u-a_j} \Big]  \\ 
&\leq 2^{j+2} (d_j + d_{j-1}) \leq 12 \cdot 2^j d_j \leq 12R_0 \frac{d_j}{r_j},
\end{aligned}
\end{equation}
where we have deployed the result \eqref{u->u-aj-1}, the fact that $d_j \geq 0$ 
and $u-a_j \geq 0$ hold true, and the assumption \eqref{dj>dj-1}. 
Initially decreasing the denominator of the fraction in 
$ \textup{III}^{(4)}$ and subsequently consulting \eqref{VorüberFürIII4}
and the bound for $ \textup{II}^{(4)}$ from \eqref{AbschII4},
we are enabled to establish the estimate
\begin{equation} \label{AbschIII4}
\begin{aligned}
 \textup{III}^{(4)}
&\leq \frac{\gamma}{d_j^2} \iint_{2Q_j \cap \{u>a_j\} } u^m 
\frac{u}{ 1+ \frac{u-a_j}{d_j} } \,d z \\
&\leq \frac{\gamma}{d_jr_j} \iint_{2Q_j \cap \{u>a_j\} } u^m \,d z 
\leq \gamma r_j^n\kappa.
\end{aligned}
\end{equation}
We insert the outcomes \eqref{AbschI4}, \eqref{AbschII4} and \eqref{AbschIII4} 
in \eqref{HausVomNiko} to obtain the energy estimate
\begin{equation} \label{4.10}
\begin{aligned}
&\sup_{t \in \Lambda_j} \int_{B_j \times \{t\} \cap \{u>a_j\} } G_\lambda 
\Big( \frac{u-a_j}{d_j} \Big) \,d x  \\
 &+ \iint_{Q_j \cap \{u>a_j\} } \Big[ d_j^{m-1}\Big|DV_\lambda 
\Big( \frac{u-a_j}{d_j} \Big)\Big|^2 + a_j^{m-1}\Big|DW_\lambda 
\Big( \frac{u-a_j}{d_j} \Big)\Big|^2 \Big] \,d z  \\ 
&\leq \gamma \big[ r_j^n\kappa + \frac{\mu(2Q_j)}{d_j} \big]
\end{aligned}
\end{equation}
for a constant $\gamma \equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0)$. 

 Since we have reduced the situation to the case in which \eqref{k_j=kappa} holds, 
we can now proceed as follows:
\begin{equation} \label{4.11}
\begin{aligned}
\kappa = \mathbf{k}_j 
&= \frac{1}{r_j^{n+2}} \iint_{Q_j \cap \{u>a_j\} } \big[(u-a_j)+a_j\big]^{m-1} 
\Big( \frac{u-a_j}{d_j} \Big)^{1+\lambda} \,d z  \\ 
&\leq \frac{\gamma d_j^{m-1}}{r_j^{n+2}} \iint_{Q_j \cap \{u>a_j\} } 
 \Big( \frac{u-a_j}{d_j} \Big)^{m+\lambda} \,d z \\
&\quad + \frac{\gamma a_j^{m-1}}{r_j^{n+2}}
  \iint_{Q_j \cap \{u>a_j\} } \Big( \frac{u-a_j}{d_j} \Big)^{1+\lambda} \,d z  \\
&=:  \textup{I}^{(5)} +  \textup{II}^{(5)}
\end{aligned}
\end{equation}
for a constant $\gamma \equiv \gamma(m)$. In the sequel, we first consider 
$ \textup{I}^{(5)}$ and then $ \textup{II}^{(5)}$.
For the former, we have
\begin{align*}
 \textup{I}^{(5)}
 &\leq \frac{\gamma d_j^{m-1}}{r_j^{n+2}} 
\Big[ \varepsilon^{1+\lambda} \iint_{Q_j \cap \{u>a_j\} } 
\Big( \frac{u-a_j}{d_j} \Big)^{m-1} \,d z \\
&\quad + \gamma_\varepsilon \iint_{Q_j \cap \{u>a_j\} } 
\Big( V_\lambda \Big( \frac{u-a_j}{d_j} \Big) \Big)^{\frac{2(m+\lambda)}{m-\lambda}} 
\, dz \Big]  \\ 
&\leq \gamma \varepsilon^{1+\lambda} \frac{1}{r_j^{n+2}} 
\iint_{Q_j \cap \{u>a_j\} } u^{m-1} \,d z \\
&\quad + \frac{\gamma_\varepsilon d_j^{m-1}}{r_j^{n+2}} 
\iint_{Q_j \cap \{u>a_j\} } \Big( V_\lambda \Big( \frac{u-a_j}{d_j} \Big) 
\Big)^{\frac{2(m+\lambda)}{m-\lambda}} \, dz  \\
 &\leq \gamma\varepsilon^{1+\lambda}\kappa 
 + \frac{\gamma_\varepsilon d_j^{m-1}}{r_j^{n+2}} \iint_{Q_j} 
\Big( V_\lambda \Big( \frac{(u-a_j)_+}{d_j} \Big) \Big)
 ^{\frac{2(m+\lambda)}{m-\lambda}} dz
\end{align*}
for constants $\gamma\equiv\gamma(n,m)$ and 
$\gamma_\varepsilon \equiv \gamma(m,\lambda,\varepsilon)$, 
using the inequality \eqref{L2b} from Lemma \ref{L2} for some 
$\varepsilon \in (0,1)$ to be chosen later and \eqref{4.9} as well as noting
 that $V_\lambda(0) = 0$ holds. Next, we apply the Gagliardo-Nirenberg 
inequality with $p=2$, $q=\frac{2(m+\lambda)}{m-\lambda}$ and 
$r=\frac{2\lambda n}{m-\lambda}$ to receive
\begin{equation} \label{AbschI6II6III6}
\begin{aligned}
 \textup{I}^{(5)}
&\leq \gamma\varepsilon^{1+\lambda}\kappa + \gamma_\varepsilon 
\Big[ \sup_{t \in \Lambda_j} \frac{1}{r_j^n} \int_{B_j \times \{t\}} 
\Big| V_\lambda \Big( \frac{(u-a_j)_+}{d_j} \Big) 
 \Big|^{\frac{2\lambda n}{m-\lambda}} \, dx \Big]^{2/n}  \\
&\quad\times \frac{d_j^{m-1}}{r_j^n} \iint_{Q_j} 
\Big[ \frac{1}{r_j^2} \Big| V_\lambda \Big( \frac{(u-a_j)_+}{d_j} \Big) \Big|^2
 + \Big| DV_\lambda\Big( \frac{(u-a_j)_+}{d_j} \Big) \Big|^2 \Big] dz  \\
 &=: \gamma\varepsilon^{1+\lambda}\kappa 
+ \gamma_\varepsilon  \textup{I}^{(6)}
\big( \textup{II}^{(6)} +  \textup{III}^{(6)}\big)
\end{aligned}
\end{equation}
for constants $\gamma\equiv\gamma(n,m)$ and
 $\gamma_\varepsilon \equiv \gamma(n,m,\lambda,\varepsilon)$. 
At this point, we shall take a brief snapshot of the progress of the proof. 
We have begun to work on the expression $ \textup{I}^{(5)}$,
where further terms $ \textup{I}^{(6)}$, $ \textup{II}^{(6)}$
and $ \textup{III}^{(6)}$, which are to be discussed in what follows,
arose in \eqref{AbschI6II6III6}. Our next goal is to estimate these terms, 
before we cope with $ \textup{II}^{(5)}$ from \eqref{4.11}.
 We continue the proof by looking at the term $ \textup{I}^{(6)}$.
 With the help of inequality \eqref{L2a}, H\"older's inequality, the 
statement \eqref{L1} for some fixed $\varepsilon_1 \in (0,1)$ to be chosen later, 
and the energy estimate \eqref{4.10}, we deduce
\begin{equation} \label{AbschI6}
\begin{aligned}
 \textup{I}^{(6)}
&= \Big[ \sup_{t \in \Lambda_j} \frac{1}{r_j^n} \int_{B_j 
\times \{t\} \cap \{u>a_j\}} \Big| V_\lambda 
\Big( \frac{u-a_j}{d_j} \Big) \Big|^{\frac{2\lambda n}{m-\lambda}} \,d x 
\Big]^{2/n}  \\
&\leq \gamma \Big[ \sup_{t \in \Lambda_j} \frac{1}{r_j^n} \int_{B_j 
\times \{t\} \cap \{u>a_j\}} \Big( \frac{u-a_j}{d_j} \Big)^{\lambda n} \,d x 
\Big]^{2/n}  \\
&\leq \gamma \Big[ \sup_{t \in \Lambda_j} \frac{1}{r_j^n} 
\int_{B_j \times \{t\} \cap \{u>a_j\}} \frac{u-a_j}{d_j} \,d x \Big]^{2\lambda}  \\ 
&\leq \gamma\varepsilon_1^{2\lambda} + \gamma\varepsilon_1^{-2\lambda} 
\Big[ \sup_{t \in \Lambda_j} \frac{1}{r_j^n} \int_{B_j \times \{t\} 
\cap \{u>a_j\}} G_\lambda \Big( \frac{u-a_j}{d_j} \Big) \,d x \Big]^{2\lambda}  \\ 
&\leq \gamma\varepsilon_1^{2\lambda} + \gamma\varepsilon_1^{-2\lambda} 
\Big[ \kappa + \frac{\mu(2Q_j)}{d_jr_j^n} \Big]^{2\lambda}
\end{aligned}
\end{equation}
for a constant $\gamma\equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0)$. 
This completes our thoughts on the term $ \textup{I}^{(6)}$,
and we now turn towards $ \textup{II}^{(6)}$ by applying the
inequality \eqref{L2a}, enlarging the domain of integration, and using the 
fact that $u-a_j \leq u$ and \eqref{4.8}. Additionally enlarging the exponent 
from $1-\lambda$ to $1+\lambda$ (note that \eqref{4.7} holds) and
 exploiting \eqref{4.9}, we obtain
\begin{equation} \label{AbschII6}
\begin{aligned}
 \textup{II}^{(6)}
&= \frac{d_j^{m-1}}{r_j^{n+2}} \iint_{Q_j \cap \{u>a_j\}} 
\Big| V_\lambda \Big( \frac{u-a_j}{d_j} \Big) \Big|^2 \,d z  \\ 
&\leq \frac{\gamma d_j^{m-1}}{r_j^{n+2}} \iint_{Q_j \cap \{u>a_j\}} 
\Big( \frac{u-a_j}{d_j} \Big)^{m-\lambda} \,d z  \\ 
&\leq \frac{\gamma}{r_j^{n+2}} \iint_{2Q_j \cap \{u>a_j\}} u^{m-1} 
\Big( \frac{u-a_j}{d_j} \Big)^{1-\lambda} \,d z  \\ 
&\leq \frac{\gamma}{r_j^{n+2}} \iint_{2Q_j \cap \{u>a_j\}} u^{m-1} 
\Big( \frac{u-a_{j-1}}{d_{j-1}} \Big)^{1-\lambda} \,d z  \\ 
&\leq \frac{\gamma}{r_j^{n+2}} \iint_{2Q_j \cap \{u>a_j\}} u^{m-1} 
\Big( \frac{u-a_{j-1}}{d_{j-1}} \Big)^{1+\lambda} \,d z \leq \gamma\kappa
\end{aligned}
\end{equation}
for a constant $\gamma\equiv \gamma(n,m,\lambda)$. Studying the term 
$ \textup{III}^{(6)}$, we find
\begin{equation} \label{AbschIII6}
 \textup{III}^{(6)}
= \frac{d_j^{m-1}}{r_j^n} \iint_{Q_j 
\cap \{u>a_j\}} \Big| DV_\lambda\Big( \frac{u-a_j}{d_j} \Big) \Big|^2 \,d z 
\leq \gamma \Big[ \kappa + \frac{\mu(2Q_j)}{d_jr_j^n} \Big]
\end{equation}
for a constant $\gamma\equiv\gamma(n,C_0,C_1,C,m,\lambda,R_0)$, where we made 
use of \eqref{4.10}. We insert the results \eqref{AbschI6}, \eqref{AbschII6} 
and \eqref{AbschIII6} in \eqref{AbschI6II6III6} and gain
\begin{equation} \label{AbschI5}
 \textup{I}^{(5)}
\leq \gamma\varepsilon^{1+\lambda}\kappa + \gamma_\varepsilon 
\Big[ \varepsilon_1^{2\lambda} + \varepsilon_1^{-2\lambda} 
\Big( \kappa + \frac{\mu(2Q_j)}{d_jr_j^n} \Big)^{2\lambda} \Big] 
\Big[ \kappa + \frac{\mu(2Q_j)}{d_jr_j^n} \Big]
\end{equation}
for constants $\gamma \equiv \gamma(n,m)$ and 
$\gamma_\varepsilon \equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0,\varepsilon)$, 
which qualifies us to put aside the considerations of the first summand 
from \eqref{4.11} to address ourselves to some illustrations of 
$ \textup{II}^{(5)}$. For the term $ \textup{II}^{(5)}$,
we involve in turn the inequalities \eqref{L3b} and $a_j^{m-1} \leq u^{m-1}$ 
(the latter holds on the domain of integration), the fact that $W_\lambda(0) = 0$, 
and \eqref{4.9} to derive the estimate
\begin{align*}
\textup{II}^{(5)}
&\leq \frac{\gamma \varepsilon^{1+\lambda}}{r_j^{n+2}} \iint_{Q_j 
 \cap \{u>a_j\} } a_j^{m-1} \,d z \\
&\quad + \frac{\gamma_\varepsilon a_j^{m-1}}{r_j^{n+2}}
  \iint_{Q_j \cap \{u>a_j\} } \Big( W_\lambda 
 \Big( \frac{u-a_j}{d_j} \Big) \Big)^{\frac{2(1+\lambda)}{1-\lambda}} \, dz \\
&\leq \gamma \varepsilon^{1+\lambda} \frac{1}{r_j^{n+2}} \iint_{Q_j 
 \cap \{u>a_j\} } u^{m-1} \,d z \\
&\quad + \frac{\gamma_\varepsilon a_j^{m-1}}{r_j^{n+2}} 
 \iint_{Q_j} \Big( W_\lambda \Big( \frac{(u-a_j)_+}{d_j} \Big) 
 \Big)^{\frac{2(1+\lambda)}{1-\lambda}} dz \\ 
&\leq \gamma \varepsilon^{1+\lambda} \kappa 
+ \frac{\gamma_\varepsilon a_j^{m-1}}{r_j^{n+2}} \iint_{Q_j} 
 \Big( W_\lambda \Big( \frac{(u-a_j)_+}{d_j} \Big) 
 \Big)^{\frac{2(1+\lambda)}{1-\lambda}} dz
\end{align*}
for constants $\gamma\equiv \gamma(n,m)$ and 
$\gamma_\varepsilon \equiv \gamma(m,\lambda,\varepsilon)$. 
Once again applying the Gagliardo-Nirenberg inequality from Theorem 
\ref{GNU_SATZ}, this time for the choices $p=2$, $q=\frac{2(1+\lambda)}{1-\lambda}$ 
and $r=\frac{2\lambda n}{1-\lambda}$, we acquire
\begin{equation} \label{AbschI7II7III7}
\begin{aligned}
\textup{II}^{(5)}
&\leq \gamma \varepsilon^{1+\lambda} \kappa + \gamma_\varepsilon 
\Big[ \sup_{t \in \Lambda_j} \frac{1}{r_j^n} \int_{B_j \times \{t\}} 
\Big| W_\lambda \Big( \frac{(u-a_j)_+}{d_j} \Big) \Big|
 ^{\frac{2\lambda n}{1-\lambda}} dx \Big]^{2/n}  \\
&\quad\times \frac{a_j^{m-1}}{r_j^n} \iint_{Q_j} 
\Big[ \frac{1}{r_j^2} \Big| W_\lambda \Big( \frac{(u-a_j)_+}{d_j} \Big) \Big|^2 
+ \Big| DW_\lambda \Big( \frac{(u-a_j)_+}{d_j} \Big) \Big|^2 \Big] dz  \\ 
&=: \gamma \varepsilon^{1+\lambda} \kappa + \gamma_\varepsilon 
 \textup{I}^{(7)} (  \textup{II}^{(7)}
+  \textup{III}^{(7)} )
\end{aligned}
\end{equation}
for constants $\gamma\equiv \gamma(n,m)$ and 
$\gamma_\varepsilon \equiv \gamma(n,m,\lambda,\varepsilon)$. 
Analogous to the approach in \eqref{AbschI6II6III6}, we have to develop 
in the following some appropriate bounds for the terms 
$ \textup{I}^{(7)}$, $ \textup{II}^{(7)}$ and
$ \textup{III}^{(7)}$ as well. Fortunately, the former two can by
little moves be reduced to the terms $ \textup{I}^{(6)}$ and
$ \textup{II}^{(6)}$, with the result that we are enabled to employ
the inequalities \eqref{AbschI6} and \eqref{AbschII6}, respectively,
 which we have already deduced. For the term $ \textup{III}^{(7)}$,
the same argumentation as the one used for $ \textup{III}^{(6)}$ is
operating effectively. After this synoptic view of the further proof strategy, 
we commence the evaluation of $ \textup{I}^{(7)}$. Consulting \eqref{L3a}
and the accomplishments for $ \textup{I}^{(6)}$ from above
(cf.\,\eqref{AbschI6}), we find
\begin{equation} \label{AbschI7}
\begin{aligned}
 \textup{I}^{(7)}
 &= \Big[ \sup_{t \in \Lambda_j} \frac{1}{r_j^n} 
\int_{B_j \times \{t\} \cap \{u>a_j\}} \Big| W_\lambda 
\Big( \frac{u-a_j}{d_j} \Big) \Big|^{\frac{2\lambda n}{1-\lambda}} \,d x 
\Big]^{2/n}  \\
&\leq \gamma \Big[ \sup_{t \in \Lambda_j} \frac{1}{r_j^n} 
\int_{B_j \times \{t\} \cap \{u>a_j\}} \Big( \frac{u-a_j}{d_j} \Big)^{\lambda n} 
\,d x \Big]^{2/n}  \\ 
&\leq \gamma\varepsilon_1^{2\lambda} + \gamma\varepsilon_1^{-2\lambda} 
\Big[ \kappa + \frac{\mu(2Q_j)}{d_jr_j^n} \Big]^{2\lambda}
\end{aligned}
\end{equation}
for a constant $\gamma\equiv\gamma(n,C_0,C_1,C,m,\lambda,R_0)$. 
To deal with the term $ \textup{II}^{(7)}$, we also exploit
the inequality \eqref{L3a}, replace $a_j$ by $u$, and exert the observations 
for $ \textup{II}^{(6)}$ from \eqref{AbschII6} to obtain
\begin{equation} \label{AbschII7}
\begin{aligned}
 \textup{II}^{(7)}
&= \frac{a_j^{m-1}}{r_j^{n+2}} 
\iint_{Q_j \cap \{u>a_j\} } \Big| W_\lambda \Big( \frac{u-a_j}{d_j} \Big) 
\Big|^2 \,d z \\
&\leq \frac{\gamma}{r_j^{n+2}} 
\iint_{Q_j \cap \{u>a_j\} } a_j^{m-1} \Big( \frac{u-a_j}{d_j} \Big)^{1-\lambda} 
\,d z  \\
 &\leq \frac{\gamma}{r_j^{n+2}} \iint_{Q_j \cap \{u>a_j\} } u^{m-1} 
\Big( \frac{u-a_j}{d_j} \Big)^{1-\lambda} \,d z \leq \gamma\kappa
\end{aligned}
\end{equation}
for a constant $\gamma\equiv \gamma(n,\lambda)$. Eventually, working with 
the same arguments as in \eqref{AbschIII6}, we get the estimate
\begin{equation} \label{AbschIII7}
 \textup{III}^{(7)}
= \frac{a_j^{m-1}}{r_j^n} \iint_{Q_j \cap \{u>a_j\} } 
\Big| DW_\lambda \Big( \frac{u-a_j}{d_j} \Big) \Big|^2 \,d z 
\leq \gamma \Big[ \kappa + \frac{\mu(2Q_j)}{d_jr_j^n} \Big]
\end{equation}
for a constant $\gamma\equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0)$. 
We insert \eqref{AbschI7}-\eqref{AbschIII7} in \eqref{AbschI7II7III7} 
to find that
\begin{equation} \label{AbschII5}
 \textup{II}^{(5)}
\leq \gamma\varepsilon^{1+\lambda}\kappa + \gamma_\varepsilon 
\Big[ \varepsilon_1^{2\lambda} + \varepsilon_1^{-2\lambda} 
\Big( \kappa + \frac{\mu(2Q_j)}{d_jr_j^n} \Big)^{2\lambda} \Big] 
\Big[ \kappa + \frac{\mu(2Q_j)}{d_jr_j^n} \Big]
\end{equation}
holds for constants $\gamma\equiv \gamma(n,m)$ and 
$\gamma_\varepsilon\equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0,\varepsilon)$, 
in other words, $ \textup{II}^{(5)}$ can be bounded by the right-hand
side of \eqref{AbschI5} as well. This closes our calculations for the
 term $ \textup{II}^{(5)}$, and we join both the estimates
\eqref{AbschI5} and \eqref{AbschII5}. Afterwards, we will specify the 
parameters $\varepsilon$, $\varepsilon_1$ and $\kappa$. By means of a case analysis, 
the desired recursive bound \eqref{4.6} for $d_j$ finally becomes apparent. 
Embedding the estimates \eqref{AbschI5} and \eqref{AbschII5} for 
$ \textup{I}^{(5)}$ and $ \textup{II}^{(5)}$ in \eqref{4.11} yields
\begin{equation} \label{4.13}
\kappa \leq \gamma\varepsilon^{1+\lambda}\kappa + \gamma_\varepsilon 
\Big[ \varepsilon_1^{2\lambda} + \varepsilon_1^{-2\lambda} 
\Big( \kappa + \frac{\mu(2Q_j)}{d_jr_j^n} \Big)^{2\lambda} \Big] 
\Big[ \kappa + \frac{\mu(2Q_j)}{d_jr_j^n} \Big]
\end{equation}
for constants $\gamma\equiv \gamma(n,m)$ and 
$\gamma_\varepsilon\equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0,\varepsilon)$. 
Before deciding on the values of the quantities 
$\varepsilon,\varepsilon_1,\kappa \in (0,1)$, we shall detect an alternative 
representation for \eqref{4.13}. If $\kappa \leq \frac{\mu(2Q_j)}{d_jr_j^n}$ 
holds, we conclude
\begin{equation*}
\kappa \leq \gamma\varepsilon^{1+\lambda}\kappa + \gamma_\varepsilon 
\Big[ \varepsilon_1^{2\lambda} + \varepsilon_1^{-2\lambda} 
\Big( 2\frac{\mu(2Q_j)}{d_jr_j^n} \Big)^{2\lambda} \Big] 
\Big[ 2\frac{\mu(2Q_j)}{d_jr_j^n} \Big],
\end{equation*}
whereas in the case that $\kappa > \frac{\mu(2Q_j)}{d_jr_j^n}$ is valid, 
one can infer
\begin{equation*}
\kappa \leq \gamma\varepsilon^{1+\lambda}\kappa 
+ \gamma_\varepsilon \big[ \varepsilon_1^{2\lambda} 
+ \varepsilon_1^{-2\lambda} ( 2\kappa )^{2\lambda} \big] 
\big[ 2\kappa \big].
\end{equation*}
We note that $\varepsilon_1^{2\lambda} \leq \varepsilon_1^{-2\lambda}$ 
to find that in any case, by adding the right-hand sides of the last 
two inequalities, \eqref{4.13} implies
\begin{equation} \label{4.13til}
\kappa \leq \big( \gamma\varepsilon^{1+\lambda} 
+ \gamma_\varepsilon \varepsilon_1^{2\lambda} 
+ \gamma_\varepsilon \varepsilon_1^{-2\lambda} \kappa^{2\lambda} \big) \kappa 
+ \gamma_\varepsilon \varepsilon_1^{-2\lambda} 
\Big[ \frac{\mu(2Q_j)}{d_jr_j^n} + \Big( \frac{\mu(2Q_j)}{d_jr_j^n} 
\Big)^{1+2\lambda} \Big].
\end{equation}
We now determine the still available parameters $\varepsilon$, $\varepsilon_1$ 
and $\kappa$ as follows: First, we choose $\varepsilon$ such that 
$\gamma\varepsilon^{1+\lambda} = \frac{1}{6}$, then $\varepsilon_1$ such that
 $\gamma_\varepsilon \varepsilon_1^{2\lambda} = \frac{1}{6}$, and finally 
$\kappa$ to satisfy $\gamma_\varepsilon \varepsilon_1^{-2\lambda} \kappa^{2\lambda} 
= \frac{1}{6}$, where one can easily verify that all three quantities actually 
lie within the demanded interval $(0,1)$. Besides, $\varepsilon$, $\varepsilon_1$ 
and $\kappa$ only depend on $n$, $C_0$, $C_1$, $C$, $m$, $\lambda$ and $R_0$. 
That way, the preceding inequality \eqref{4.13til} evolves into
\begin{equation} \label{HausVomNikoUMG}
\kappa \leq \gamma \Big[ \frac{\mu(2Q_j)}{d_jr_j^n} 
+ \Big( \frac{\mu(2Q_j)}{d_jr_j^n} \Big)^{1+2\lambda} \Big]
\end{equation}
for a constant $\gamma\equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0)$. 
With the aid of a case analysis, the inequality \eqref{4.6} will relatively 
quickly come out of \eqref{HausVomNikoUMG}. 
Indeed, if there holds $\alpha := \mu(2Q_j)/(d_jr_j^n) \leq 1$, we have 
$\alpha^{1+2\lambda} \leq \alpha$, and, consequently, one can infer
\begin{equation} \label{SchrankeFürDJ1}
d_j \leq \gamma \frac{\mu(2Q_j)}{r_j^n}
\end{equation}
from \eqref{HausVomNikoUMG}, since $\kappa$, just like $\gamma$, solely 
depends on $n$, $C_0$, $C_1$, $C$, $m$, $\lambda$ and $R_0$. 
If otherwise $\alpha > 1$ holds, we have $\alpha \leq \alpha^{1+2\lambda}$, 
and \eqref{HausVomNikoUMG} likewise yields \eqref{SchrankeFürDJ1}. 
In both cases, this leads to
\begin{equation*}
d_j \leq 2\gamma \frac{\mu(2Q_j)}{r_j^n} 
\leq \frac{\gamma\mu(2Q_{r_j,\theta_j})}{r_j^n},
\end{equation*}
where we have used \eqref{Zyl2Absch}. Eventually, the claim \eqref{4.6} 
ensues from this estimate. We hereby terminate this passage on the recursive
bound for $d_j$ and move on to the last subsection to establish the proposition 
\eqref{HauptBeh}.

\subsection{Potential estimates}

In this segment, we resort to the property \eqref{4.6} of $d_j$ to deduce 
the alleged inequality \eqref{HauptBeh}. More precisely, we will add 
up \eqref{4.6} which gives us the bound \eqref{al<=4a1} for the members 
of the sequence $(a_j)_{j \in \mathbb{N}_0}$. Appropriately estimating in 
\eqref{al<=4a1} both $a_1$ and the involved sum (the latter in terms of 
a Riesz potential), subsequently passing to the limit $j \to \infty$, and 
additionally employing a short argument which allows to associate $u(z_0)$ 
with the limit $a_\infty$, we obtain the assertion of Theorem \ref{Hauptthm}. 

 Summing up the result \eqref{4.6} proved in Section \ref{KAP_4.2}, we receive
\begin{equation} \label{DiffALA1}
\begin{aligned}
a_\ell-a_1 
&= \sum_{j=1}^{\ell-1} d_j \leq \frac{1}{2} \sum_{j=1}^{\ell-1} d_{j-1} 
 + \sum_{j=1}^{\ell-1} 2^{-(j+2)} a_j 
 + \gamma \sum_{j=1}^{\ell-1} \frac{\mu(2Q_{r_j,\theta_j})}{r_j^n} \\
&\leq \frac{3}{4} a_\ell + \gamma \sum_{j=1}^\ell 
 \frac{\mu(2Q_{r_j,\theta_j})}{r_j^n}
\end{aligned}
\end{equation}
for any $\ell\geq 2$, where we have worked with the estimates 
(note that $(a_j)_{j \in \mathbb{N}_0}$ is an increasing sequence)
\begin{gather*}
\sum_{j=1}^{\ell-1} d_{j-1} = a_{\ell-1} - a_0 \leq a_{\ell-1} \leq a_\ell,\\
\sum_{j=1}^{\ell-1} 2^{-(j+2)} a_j \leq \frac{a_\ell}{4} \sum_{j=1}^{\ell-1} 2^{-j} \leq \frac{a_\ell}{4}.
\end{gather*}
The inequality \eqref{DiffALA1} connotes
\begin{equation} \label{al<=4a1}
a_\ell \leq 4a_1 + \gamma \sum_{j=1}^\ell \frac{\mu(2Q_{r_j,\theta_j})}{r_j^n}
\end{equation}
for any $\ell\geq 2$. In the following, we are interested in a bound 
for the parameter $a_1$, which is why we recall its definition. 
If $\mathbf{K}_0 (\frac{5}{4}a_0) \leq \kappa$, we have set 
$a_1= \frac{5}{4}a_0$, hence, \eqref{al<=4a1} gives
\begin{equation} \label{AbschAL1}
a_\ell \leq 5 \Big( \frac{r^2}{\theta} \Big)^{\frac{1}{m-1}} 
+ \gamma \sum_{j=1}^\ell \frac{\mu(2Q_{r_j,\theta_j})}{r_j^n},
\end{equation}
whereas in the case that $\mathbf{K}_0 (\frac{5}{4}a_0) > \kappa$ holds, 
the equation \eqref{KjaJ+1=kappa} for $j=0$ reads as
\begin{equation*}
\frac{1}{r^{n+2}} \iint_{Q_0 \cap \{u>a_0\} } u^{m-1} 
\Big( \frac{u-a_0}{a_1-a_0} \Big)^{1+\lambda} \,d z = \kappa.
\end{equation*}
We multiply both sides by $\frac{(a_1-a_0)^{1+\lambda}}{\kappa}$ 
and subsequently raise them to the power $\frac{1}{1+\lambda}$ to acquire
\begin{align*}
a_1 &= a_0 + \Big[ \frac{1}{\kappa r^{n+2}} \iint_{Q_0 \cap \{u>a_0\} } 
 u^{m-1} (u-a_0)^{1+\lambda} \,d z \Big]^{\frac{1}{1+\lambda}} \\ 
&\leq \Big( \frac{r^2}{\theta} \Big)^{\frac{1}{m-1}} 
 + \Big[ \frac{1}{\kappa r^{n+2}} \iint_{Q_{r,\theta}} u^{m+\lambda} \,d z 
 \Big]^{\frac{1}{1+\lambda}},
\end{align*}
where in the second step we have replaced $u-a_0$ by $u$ and enlarged the 
domain of integration via \eqref{Zyl2Absch}. Inserting this in 
\eqref{al<=4a1}, we find
\begin{equation} \label{AbschAL2}
a_\ell \leq 4 \Big( \frac{r^2}{\theta} \Big)^{\frac{1}{m-1}} 
+ 4 \Big[ \frac{1}{\kappa r^{n+2}} \iint_{Q_{r,\theta}} u^{m+\lambda} \,d 
z \Big]^{\frac{1}{1+\lambda}} 
+ \gamma \sum_{j=1}^\ell \frac{\mu(2Q_{r_j,\theta_j})}{r_j^n}.
\end{equation}
Thus, regardless of whether $\mathbf{K}_0 (\frac{5}{4}a_0) \leq \kappa$ 
or not, we derive
\begin{equation} \label{4.14tiltil}
a_\ell \leq 5 \Big( \frac{r^2}{\theta} \Big)^{\frac{1}{m-1}} 
+ \gamma \Big[ \frac{1}{r^{n+2}} \iint_{Q_{r,\theta}} u^{m+\lambda} \,d z 
\Big]^{\frac{1}{1+\lambda}} + \gamma \sum_{j=1}^\infty 
\frac{\mu(2Q_{r_j,\theta_j})}{r_j^n}
\end{equation}
for a constant $\gamma\equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0)$ 
from \eqref{AbschAL1} and \eqref{AbschAL2}. Next, we estimate the series 
in \eqref{4.14tiltil} by a Riesz potential. For this purpose, we set 
$r_{-1} := 2r$ and compute
\begin{align*}
\sum_{j=1}^\infty \frac{\mu(2Q_{r_j,\theta_j})}{r_j^n} 
&= \sum_{j=1}^\infty \frac{1}{r_{j-2}-r_{j-1}} \int_{r_{j-1}}^{r_{j-2}}
 \frac{\mu (Q_{r_{j-1},r_{j-1}^2 \theta / r^2})}{r_j^n} \,d \varrho \\ 
&\leq 2^{2n} \sum_{j=1}^\infty \int_{r_{j-1}}^{r_{j-2}} 
 \frac{\mu (Q_{\varrho, \varrho^2 \theta / r^2})}{r_{j-2}^n (r_{j-2}-r_{j-1})} 
 \,d \varrho \\ 
&\leq 2^{2n+1} \sum_{j=1}^\infty \int_{r_{j-1}}^{r_{j-2}} 
 \frac{\mu (Q_{\varrho, \varrho^2 \theta / r^2})}{\varrho^n\varrho} \,d \varrho \\ 
&= 2^{2n+1} \int_0^{2r} \frac{\mu (Q_{\varrho, \varrho^2 \theta / r^2})}{\varrho^n} 
 \frac{d\varrho}{\varrho} \\ 
&= 2^{2n+1} \mathbf{I}_2^\mu \left( z_0,2r,4\theta \right),
\end{align*}
which, inserted in \eqref{4.14tiltil}, yields the inequality
\begin{align*}
a_\ell 
&\leq 5 \Big( \frac{r^2}{\theta} \Big)^{\frac{1}{m-1}} + \gamma 
\Big[ \frac{1}{r^{n+2}} \iint_{Q_{r,\theta}} u^{m+\lambda} \,d z 
\Big]^{\frac{1}{1+\lambda}} + \gamma \mathbf{I}_2^\mu 
\left( z_0,2r,4\theta \right) \\ &\leq 5 \Big( \frac{(2r)^2}{4\theta} 
\Big)^{\frac{1}{m-1}} + \gamma \Big[ \frac{1}{(2r)^{n+2}} 
\iint_{Q_{2r,4\theta}} u^{m+\lambda} \,d z \Big]^{\frac{1}{1+\lambda}}
 + \gamma \mathbf{I}_2^\mu \left( z_0,2r,4\theta \right).
\end{align*}
Substituting $2r$ by $r$ and $4\theta$ by $\theta$, this implies in particular that
\begin{equation} \label{AbschAInfty}
\begin{aligned}
a_\infty := \lim_{j\to\infty} a_j 
&\leq 5 
\Big( \frac{r^2}{\theta} \Big)^{\frac{1}{m-1}} + \gamma 
\Big[ \frac{1}{r^{n+2}} \iint_{Q_{r,\theta}} u^{m+\lambda} \,d z 
\Big]^{\frac{1}{1+\lambda}} \\
&\quad + \gamma \mathbf{I}_2^\mu \left( z_0,r,\theta \right) 
< \infty
\end{aligned}
\end{equation}
for a constant $\gamma\equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0)$.
 By the definition of $d_j$ $(=a_j-a_{j-1})$, we infer the convergence 
$d_j \to 0$ as $j \to \infty$. Now, let $z_0$ be a Lebesgue point of $u$. 
Defining for short \mbox{$\omega_n := \mathcal{H}^{n-1}(\mathcal{S}^{n-1})$}, 
we then have
\begin{align*}
0&\leq \Big( \frac{u(z_0)}{a_\infty} \Big)^{m-1} \big(u(z_0)
-a_\infty \big)_+^{1+\lambda} \\
&= \lim_{j\to\infty} -\!\!-\hspace{-6.6mm}\iint_{Q_j} 
\Big( \frac{u}{a_j} \Big)^{m-1} \big(u-a_j \big)_+^{1+\lambda} \,d z \\ 
&= \lim_{j\to\infty} \frac{n d_j^{1+\lambda}}{\omega_n} \frac{1}{r_j^{n+2}} 
\iint_{Q_j \cap \{u>a_j\}} u^{m-1} \Big( \frac{u-a_j}{d_j} \Big)^{1+\lambda} \,d z \\
 &\leq \frac{n \kappa}{\omega_n} \lim_{j\to\infty} d_j^{1+\lambda} = 0
\end{align*}
by the inequality \eqref{Absch_kj} and the limit $d_j \to 0$ as $j\to\infty$, 
which we have just established above. Hence, $u(z_0) - a_\infty \leq 0$ 
necessarily holds. Taking into account the estimate \eqref{AbschAInfty}, 
this leads us to
\begin{equation*}
u(z_0) \leq a_\infty \leq 5 \Big( \frac{r^2}{\theta} \Big)^{\frac{1}{m-1}} 
+ \gamma \Big[ \frac{1}{r^{n+2}} \iint_{Q_{r,\theta}} u^{m+\lambda} \,d z 
\Big]^{\frac{1}{1+\lambda}} + \gamma \mathbf{I}_2^\mu \left( z_0,r,\theta \right)
\end{equation*}
for any Lebesgue point $z_0$ of $u$ with a constant 
$\gamma\equiv \gamma(n,C_0,C_1,C,m,\lambda,R_0)$ which proves the assertion 
of Theorem \ref{Hauptthm}. 
\end{proof}

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\end{document}
