A MATHEMATICAL MODEL FOR CASE
HARDENING OF STEEL
ANTONIO FASANO
Dipartimento di Matematica, Universit�a degli Studi di Firenze,
Viale Morgagni 67/A, 50134 Firenze, Italyfasano@math-uni¯.it
DIETMAR HÖMBERG
Weierstrass Institute for Applied Analysis and Stochastics,
Mohrenstrasse 39, 10117 Berlin, Germany
LUCIA PANIZZI
Scuola Normale Superiore, Piazza dei Cavalieri 7
56126 Pisa, [email protected]
Received 18 April 2008Revised 5 January 2009
Communicated by N. Bellomo
A mathematical model for the case hardening of steel is presented. Carbon is dissolved in the
surface layer of a low-carbon steel part at a temperature su±cient to render the steel austenitic,followed by quenching to form a martensitic microstructure. The model consists of a nonlinear
evolution equation for the temperature, coupled with a nonlinear evolution equation for the
carbon concentration, both coupled with two ordinary di®erential equations to describe the
evolution of phase fractions. We investigate questions of existence and uniqueness of a solutionand ¯nally present some numerical simulations.
Keywords: Heat treatment; phase transitions; coupled PDE.
AMS Subject Classi¯cation: 35K60, 35R05, 82B26
1. Introduction
The goal of case hardening is to create a workpiece surface which is resistant to
external stresses and abrasion, while its case is still ductile in order to reduce fatigue
e®ects. The process will be explained in detail in the next section. It exploits the
solid�solid phase transitions occurring during thermal treatment of steel and
requires a certain amount of carbon in the layer to be hardened. Accordingly, the ¯rst
Mathematical Models and Methods in Applied SciencesVol. 19, No. 11 (2009) 2101�2126
#.c World Scienti¯c Publishing Company
DOI: 10.1142/S0218202509004054
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stage of case hardening is a carburization step during which the outer workpiece layer
is enriched by carbon. The second stage is a quenching step during which a hard and
wear resistant boundary layer is achieved. Sometimes, before quenching, a period of
slow di®usion is allowed. The goal of this paper is to derive and analyze a math-
ematical model capable to describe the complete process of case hardening. Con-
cerning case hardening there is mostly engineering literature available (see Refs. 15
and 16 and references therein). Carburization and quenching are usually considered
and studied separately. There are papers concerning only the carburization (see, for
example, Ref. 5) and others regarding the quenching of carburized steel (see Refs. 18
and 22). Generally, in all of the engineering papers, a lot of attention is spent to
determine the process and material parameters; nevertheless the question of ¯nding a
consistent and exhaustive database for all the parameters occurring in the whole
process seems to be still open. There is a vast literature, for instance, about the
di®usion coe±cient of carbon in iron, (see Ref. 23 and references therein), but much
less for the heat transfer coe±cient during quenching. Mathematical models for phase
transitions in steel and in their applications to heat treatments like induction
hardening have been developed and analyzed, e.g. in Refs. 7, 10, 11, 13 and 26. The
model for the phase fraction evolutions in the present paper follows the one proposed
in Ref. 10.
The main novelty of this paper is the derivation and analysis of a mathematical
model for the complete case hardening process accounting for the coupling of tem-
perature, phase transitions and carbon di®usion. This allows one to evaluate the
e®ect of additional di®usion of carbon prior to quenching, which could a®ect the ¯nal
result (see Ref. 24). Thus, from application point of view, a more accurate model
might lead to a more e±cient process guidance and reduced energy consumption.
The paper is organized as follows: in the next section we will derive the model. In
Sec. 3, we present notations and assumptions. In Secs. 4 and 5 we will prove the
existence and uniqueness of a weak solution. Section 6 is devoted to numerical
simulations; then, in Sec. 7, we collect our ¯nal considerations and remarks.
2. The Mathematical Model
To ¯x ideas we ¯rst give a sketch of the gas carburizing process. Nowadays high-
technology industry employs mostly low-carbon steels, with a carbon content around
0.2%. For this reason the enrichment of carbon in a super¯cial layer of the workpiece
may be necessary to make it resistant to fatigue. The source of carbon is a carbon-rich
furnace atmosphere produced from many gaseous components, through several
chemical reactions (see Ref. 24 for technical details). The workpiece is kept in the
furnace until the desired amount of carbon is di®used. After carburization the second
stage is quenching, a rapid coolingwhich can be performedby immersion in oil orwater.
In the boundary layer which has been enriched by carbon, the rapid cooling leads
to the growth of martensite eventually yielding the desired hard and wear resistant
layer or case, which explains why this heat treatment is called case hardening.
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The kinetics of the phase change can be brie°y described as follows. Depending on
temperature, two di®erent lattice structures can occur: a body-centered-cubic (b.c.c.)
and a face-centered-cubic (f.c.c.) lattice. Above a certain temperature As steel is in
the austenitic phase, a solid solution of carbon in f.c.c. iron. Below As this lattice is no
longer stable. But before the lattice can change its con¯guration to form a b.c.c.
structure, carbon atoms have to di®use, due to the higher solubility of carbon in the
f.c.c lattice. The result is pearlite, a lamellar aggregate of ferrite and cementite, soft
and ductile. Upon high cooling rate carbon has no time to di®use and is trapped,
forming a tetragonally distorted b.c.c. lattice, called martensite. Note that, depen-
ding on the cooling history and the carbon concentration, also two other phases,
ferrite and bainite, can occur.
The transformation diagrams of interest for the modelling of the phase fractions
evolution (see Eqs. (2.1a), (2.1b) below), during the cooling process, are called indeed
continuous cooling transformation (CCT) diagrams and describe the transformation
of austenite as a function of time for a continuously decreasing temperature. For
instance, in the left-hand side of Fig. 1, the CCT diagram for the steel AISI 1045 is
shown. In other words a sample is austenitized and then cooled at a predetermined
rate and the degree of transformation is measured, for example by dilatometry. The
start of transformation is de¯ned as the temperature at which 1% of the new
microstucture has formed. The transformation is completed when only 1% of the
original austenite is left.
In carburized steels the process is strongly in°uenced by the carbon content, which
varies from the carbon-enriched super¯cial layer to the core. Thus, it cannot be
described by only one continuous-cooling-transformation diagram. Figure 2 shows a
continuous cooling diagram describing, for a given austenitizing condition, the
transformation at all carbon levels in a carburized specimen. The cross sections for
¯xed carbon percentages give CCT diagrams of the type of the one plotted in Fig. 1
on the left. This ¯gure also shows that, with in¯nitely-slow cooling, the CCT diagram
Fig. 1. Equilibrium diagram of the system iron-carbon (right) as limit of the CCT-diagram with in¯nite
low cooling rate (taken from Ref. 13).
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is identical with the equilibrium diagram for the chemical composition of the steel. To
avoid unnecessary technicalities for the modelling, we assume that the cooling takes
place from the high temperature phase austenite with phase fraction a to two
di®erent product phases, pearlite with fraction p and martensite with fraction m. A
more elaborate model accounting for all the phases occurring during the heat
treatment of steel can be found in Ref. 13.
The evolution of the phases p and m can be described by the following system:
_p ¼ ð1� p�mÞg1ð�; cÞ; ð2:1aÞ_m ¼ ½minfmð�; cÞ; 1� pg �m�þg2ð�; cÞ; ð2:1bÞ
pð0Þ ¼ 0; ð2:1cÞmð0Þ ¼ 0; ð2:1dÞ
where c is the concentration of carbon. Here the bracket ½ �þ denotes the positive part
function ½x�þ ¼ maxfx; 0g and the dot means the derivative with respect to t. While
the growth rate of pearlite _p is assumed to be proportional to the remaining austenite
fraction, the rate of martensite growth _m is zero if m exceeds either the non-pearlitic
fraction 1� p, or the threshold m depending on both temperature and carbon con-
centration. Indeed martensite is produced at temperatures less than a value Ms but
Fig. 2. Three-dimensional presentation of the transformation characteristic of a 14NiCr14 steel, for
continuous cooling, after austenization at 1023�K (Symbols: ZW bainite, M martensite, P pearlite, F
ferrite), (taken from Ref. 13).
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complete transformation to martensite can be obtained only below some other
temperature threshold Mf . Both these temperatures depend on the local value of
carbon concentration. The quantity mð�; cÞ represents the maximum attainable
value of martensite fraction and can be de¯ned as:
mð�; cÞ ¼0 � >MsðcÞ
1 � <MfðcÞ
(
and by interpolation for intermediate temperatures. Since there is no phase transition
from pearlite to martensite, the term minfmð�; cÞ; 1� pg represents the maximal
fraction of martensite that can be reached at time t. In Fig. 3, obtained from
experimental data (see Ref. 3), we can see how the functions Ms and Mf look like.
The functions g1 and g2 are positive given functions that can be identi¯ed from the
time-temperature-transformation diagrams described before. The process of carbon
di®usion is governed by the following nonlinear parabolic equation:
@c
@t� divðð1� p�mÞDð�; cÞrcÞ ¼ 0:
The factor ð1� p�mÞ in front of the di®usion coe±cientDð�; cÞ re°ects the fact thatenrichment with carbon only takes place in the austenite phase. The di®erence in
carbon potential between the surface and the workpiece provides the driving force for
carbon di®usion into the piece. The carbon potential of the furnace atmosphere must
be greater than the carbon potential of the surface of the workpiece for carburizing to
occur. Hence we have the following boundary condition:
�ð1� p�mÞDð�; cÞ @c@�
¼ �ðc� cpÞ;
where �, the mass transfer coe±cient, controls the rate at which carbon is absorbed
by the steel during carburizing and cp is the carbon concentration in the furnace,
0
200
0
Tra
nsfo
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ion
tem
pera
ture
Carbon content
Co
−200
400
0% martensite
~50%
~100%
Start of martensitetransformation
transformation
Start of martensite
End of martensite
Mass %1.60.4 0.8 1.2
Fig. 3. Level curves of function mð�; cÞ.
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usually named carbon potential of the gas. @c@� denotes the outward normal derivative.
The evolution of temperature during the entire process is described by the following
nonlinear problem
��ð�Þ @�@t
� divðkr�Þ ¼ �Lpð�Þ _pþ �Lmð�Þ _m;
�k@�
@�¼ hð�� ��Þ;
�ðx; 0Þ ¼ �0:
Here � is the mass density, � the speci¯c heat, k the heat conductivity of the material.
Lp and Lm denote latent heats of the austenite-pearlite and the austenite-martensite
phase changes, respectively. �� is the temperature of the coolant and �0ðxÞ is the
temperature at the beginning of the process. For simplicity � and k are taken
constant.
In the technical process, we have three di®erent time stages:
. Stage 1: carburization in a furnace, hence � 6¼ 0 and h ¼ 0.
. Stage 2: di®usion period, with � ¼ 0 and h 6¼ 0, serving as a linearized radiation
law.
. Stage 3: quenching with � ¼ 0 and h 6¼ 0.
From the mathematical point of view, without loss of generality, we will assume that
� and h are time-independent functions. Then, the mathematical result to be for-
mulated in the following section can be applied subsequently to the three process
stages, covering the complete case hardening process.
3. Assumptions and Main Result
Let � � R3 be an open bounded set with C 2-boundary @� and QT :¼ �� ð0;T Þ thecorresponding time cylinder. We use the following notations for function spaces:
. W 1;1ð0;T ;L1ð�ÞÞ ¼ fv 2 L1ð0;T ;L1ð�ÞÞ : vt 2 L1ð0;T ;L1ð�ÞÞg:
. W r;sp ðQT Þ ¼ Lpð0;T ;W r
p ð�ÞÞ \W sp ð0;T ;Lpð�ÞÞ.
For p ¼ 2 we write W r;sp ðQT Þ ¼ Hr;sðQT Þ.
. We denote by V the space H 1ð�Þ and by V � the space ðH 1ð�ÞÞ�.W ð0;T Þ ¼ fv 2 L2ð0;T ;V Þ : vt 2 L2ð0;T ;V �Þg, endowed with the norm
jjvjjWð0;T Þ ¼Z T
0
ðjjvðtÞjj2V þ jjv 0ðtÞjj 2V � Þdt� �1
2
:
Throughout the paper we will use the following assumptions:
(A1) � and k are positive constants.
(A2) � 2 CðRÞ and there exist positive constants �0; �1 such that 0 < �0 ��ð�Þ � �1. Lp;Lm 2 L1ðRÞ and they are Lipschitz-continuous.
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(A3) �� is a positive constant. h 2 L1ð@�Þ with hðxÞ 0 a.e. in @�. We assume that
�0 2 H 1ð�Þ and c0 2 L2ð�Þ.(A4) g1; g2 are Lipschitz-continuous in both variables, moreover there are positive
constants �1; �2 such that 0 � g1ð�; cÞ � �1; 0 � g2ð�; cÞ � �2; 8 �; c 2 R.
(A5) m is Lipschitz-continuous satisfying mð�; cÞ 2 ½0; 1� for every �; c 2 R.
(A6) Dð�; cÞ is Lipschitz in both arguments and there are constants �3; �4 such that
0 < �3 � Dð�; cÞ � �4; 8 �; c 2 R.
(A7) cp is a positive constant. � 2 L1ð@�Þ with � 0 a.e. in @�.
Summarizing the model equations of Sec. 2, we consider the following boundary value
problem:
��ð�Þ @�@t
� divðkr�Þ ¼ �Lpð�Þpt þ �Lmð�Þmt in QT ; ð3:1aÞ
@c
@t� divðð1� p�mÞDð�; cÞrcÞ ¼ 0 in QT ; ð3:1bÞ
pt ¼ ð1� p�mÞg1ð�; cÞ in QT ; ð3:1cÞmt ¼ ½minfmð�; cÞ; 1� pg �m�þg2ð�; cÞ in QT ; ð3:1dÞ
�k@�
@�¼ hð�� ��Þ on @�� ð0;T Þ; ð3:1eÞ
�ð1� p�mÞDð�; cÞ @c@�
¼ �ðc� cpÞ on @�� ð0;T Þ; ð3:1fÞ
�ðx; 0Þ ¼ �0 in �; ð3:1gÞcðx; 0Þ ¼ c0 in �; ð3:1hÞ
pð0Þ ¼ 0 in �; ð3:1iÞmð0Þ ¼ 0 in �: ð3:1jÞ
We are going to prove that, under the hypothesis above, the considered problem
has a weak solution.
Theorem 3.1. (Existence of a weak solution) Assume (A1)�(A7), then there exists
a weak solution ð�; c; p;mÞ to problem (3.1a)�(3.1j) such that � 2 H 2;1ðQT Þ,c 2 W ð0;T Þ; p;m 2 W 1;1ð0;T ;L1ð�ÞÞ.
With slightly stronger assumptions on the data, we can also prove uniqueness.
Theorem 3.2. (Uniqueness) Suppose that (A1)�(A7) are satis¯ed. Assume
moreover that � is constant, D ¼ Dð�Þ;h; � 2 W 15 ð@�Þ; �0; c0 2 W 2
5 ð�Þ. Then the
solution to (3.1a)�(3.1j) is unique.
Remark 3.1. The regularity assumptions on the boundary and initial values in the
uniqueness theorem could be weakened; to avoid unnecessary technicalities we
assumed �� and cp to be constants, but they could in fact be functions of space and
time.
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4. Proof of Theorem 3.1
The proof is carried out using a nested ¯xed point argument. We divide the proof in
three steps. The ¯rst is a preliminary lemma concerning the ODE system (3.1c)�(3.1d) only, for � and c prescribed. The second step is the coupling of the ODE system
and the temperature equation, which gives a solution p;m; � depending on c and the
third is the further coupling with the equation for c.
We begin with considering the initial value problem
zt ¼ fðz; �; cÞ in QT ; ð4:1aÞ
zð0Þ ¼ 0 in �; ð4:1bÞ
where z ¼ ðp;mÞT and f ¼ ðf1; f2ÞT denotes the right-hand side of (3.1c) and (3.1d).
Lemma 4.1. Under the assumptions (A4), (A5) the following statements are valid:
(a) For every �; c 2 L2ðQT Þ problems (4.1a)–(4.1b) has a unique solution z such that
p 0;m 0 and
jjjzjjjW 1;1ð0;T ;L1ð�ÞÞ � M
for a constant M independent of � and c. Moreover, there exists a constant cTsuch that
0 � pðx; tÞ þmðx; tÞ � cT < 1 for a:e: ðx; tÞ in QT :
(b) There are constants M1;M2 > 0 such that for every �1; �2; c1; c2 2 LpðQT Þ, foralmost all t 2 ð0;T Þ and all p 2 we have
jjjz1ðtÞ � z2ðtÞjjjpW 1;pð�Þ � M1
Z t
0
jj�1 � �2 jjpLpð�ÞdsþM2
Z t
0
jjc1 � c2 jjpLpð�Þds;
ð4:2Þ
where pi;mi is the solution corresponding to ð�i; ciÞ and j � j is the Euclidean
norm in R2.
Proof of Lemma 4.1. In order to prove (a) it is convenient to rewrite problem
(4.1a)�(4.1b) as:
zt ¼ F ðz; tÞ in ð0;T Þ ð4:3aÞ
zð0Þ ¼ 0 ð4:3bÞ
with F ðz; �Þ ¼ fðz; �ð�Þ; cð�ÞÞ.First of all we are going to show that the hypothesis of the existence Car-
ath�eodory's theorem are satis¯ed:
(i) t 7! F ðz; tÞ is measurable on ð0;T Þ for each z 2 ½0; 1� � ½0; 1�;
z 7! F ðz; tÞ is continuous on ½0; 1� � ½0; 1� for almost all t 2 ð0;T Þ:
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These conditions follow from the de¯nition of F as a consequence of the
measurability of � and c on ð0;T Þ and of the fact that g1ð�; cÞ; g2ð�; cÞ are
Lipschitz-continuous in both variables.
(ii) Using assumptions (A4), (A5) we have
jF1ðz; tÞj � j1� p�mjg1ð�; cÞ � �1 on ½0; 1� � ½0; 1� � ð0;T Þ;jF2ðz; tÞj � jm �mjg2ð�; cÞ � �2 on ½0; 1� � ½0; 1� � ð0;T Þ:
According to Carath�eodory's theorem (cf. e.g. p. 1044 of Ref. 27) (4.3a)–(4.3b)
has a solution on some time interval ð0;TþÞ.
Next we are going to show that the solution is unique. To this end we have to
prove that there holds
jF ðz1; tÞ � F ðz2; tÞj � Ljz1 � z2j 8 ðz1; tÞ; ðz1; tÞ 2 ½0; 1� � ½0; 1� � ð0;T Þ: ð4:4Þ
Indeed, according to the de¯nition of F:
jF ðz1; tÞ � F ðz2; tÞj2 ¼ jð1� p1 �m1Þg1ðtÞ � ð1� p2 �m2Þg1ðtÞj2
þ j½minfmðtÞ; 1� p1g �m1�þg2ðtÞ
� ½minfmðtÞ; 1� p2g �m2�þg2ðtÞj2:
Thanks to the boundedness of g1 and g2, we obtain
jð1� p1 �m1Þg1ðtÞ � ð1� p2 �m2Þg1ðtÞj � �1ðjp1 � p2j þ jm2 �m1jÞ
and
j½minfmðtÞ; 1� p1g �m1�þg2ðtÞ � ½minfmðtÞ; 1� p2g �m2�þg2ðtÞj
� �2jminfmðtÞ; 1� p1g �m1 �minfmðtÞ; 1� p2g þm2j:
We shall now distinguish some cases.
If either minfmðtÞ; 1� pig ¼ 1� pi or minfmðtÞ; 1� pig ¼ mðtÞ, for i ¼ 1; 2,
(4.4) immediately follows.
If minfmðtÞ; 1� p1g ¼ 1� p1 and minfmðtÞ; 1� p2g ¼ mðtÞ (the same holds for
inverted indices), we have
�2jminfmðtÞ; 1� p1g �m1 �minfmðtÞ; 1� p2g þm2j
� �2ðjm1 �m2j þ j1� p1 �mðtÞjÞ � �2 jm1 �m2j þ jp1 � p2jð Þ: ð4:5Þ
Thus, there exists a positive constant L such that
jF ðz1; tÞ � F ðz2; tÞj � Ljz1 � z2j:
Hence we have proved uniqueness of z on ð0;TþÞ:Now, we de¯ne T� as the maximal time such that the solution to (4.3a,b) exists and
Z < 1� � on ð0;T�Þ, where Z ¼ pþm.
The last step in order to prove point (a) of the lemma is to show that for any T > 0
there exists an � such that jZj � 1� � in ½0;T �.
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This will be done by means of a classical comparison criterium for ODE (see for
instance Ref. 17, Chap. I, Prop. 3.1).
Z ¼ pþm satis¯es, on ½0;T�Þ:
_ZðtÞ ¼ ð1� ZðtÞÞg1ðtÞ þ ½minfmðtÞ; 1� pðtÞg �mðtÞ�þg2ðtÞ
� gðt;ZðtÞÞ :¼ ð1� ZðtÞÞðg1ðtÞ þ g2ðtÞÞ;
Zð0Þ ¼ 0:
Now, if we consider on ½0;T � the auxiliary problem:
V:ðtÞ ¼ ð1� V ðtÞÞðg1ðtÞ þ g2ðtÞÞ ¼ gðt;V ðtÞÞ;
V ð0Þ ¼ 0;
the solution is given by
V ðtÞ ¼ 1� e�R t
0ðg1þg2ÞðsÞds 8 t 2 ½0;T �
and we immediately have that there exists a constant CT > 0 such that:
0 � V ðtÞ � CT < 1 on ½0;T Þ:
Notice that gðt;V ðtÞÞ ¼ ð1� V ðtÞÞðg1ðtÞ þ g2ðtÞÞ is Lipschitz-continuous on ½0;T Þwith respect to V.
Thus, choosing � ¼ 1� CT , we have
ZðtÞ � V ðtÞ � 1� � on ½0;T �:
Since T� was chosen maximally such that ZðtÞ � 1� � on ½0;T��, it follows that
T� T .
(b) Let us consider again the equation zt ¼ fðz; �; cÞ. Let zi be the solution to
(4.1a)�(4.1b), corresponding to �i; ci; i ¼ 1; 2. Denoting z ¼ z1 � z2, subtracting the
equations and taking the scalar product with the function jzjp�2z, we obtain:
1
p
Z�
jzðtÞjpdx ¼Z t
0
Z�
ðfðz1; �1; c1Þ � fðz1; �2; c2ÞÞ � zjzjp�2dxds: ð4:6Þ
Invoking (A4), f is Lipschitz-continuous in all variables, thus, proceeding from (4.6),
the conclusion follows through standard application of Young's inequality and
Gronwall lemma. The proof is thus complete.
Next, we de¯ne
Bð�; cÞ :¼ �Lpð�Þ _pþ �Lmð�Þ _m; ð4:7Þ
where ðp;mÞ depends on �; c as characterized by the previous lemma.
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Lemma 4.2. Suppose that (A2), (A4) hold. Then the operator B de¯ned by (4.7) has
the following properties
(a) There exists a constant �B independent of �, c such that, for all � 2 L2ðQT Þ; c 2L2ðQT Þ there holds
jjBð�; cÞjjL1ðQT Þ � �B:
(b) Given c 2 L2ðQT Þ, let �k � L2ðQT Þ be any sequence converging strongly in
L2ðQT Þ to � 2 L2ðQT Þ. Then for every p 2 ½1;1Þ, we have
Bð�k; cÞ ! Bð�; cÞ strongly in LpðQT Þ: ð4:8Þ
(c) There are constants K1;K2 > 0 such that for all �1; �2; c1; c2 2 L2ðQT Þ and for
almost all x 2 � and every t 2 ð0;T ÞZ t
0
jBð�1ðx; sÞ; c1ðx; sÞÞ � Bð�2ðx; sÞ; c2ðx; sÞÞj2ds
� K1
Z t
0
j�1ðx; sÞ � �2ðx; sÞj2 dsþK2
Z t
0
jc1ðx; sÞ � c2ðx; sÞj2ds:
Proof of Lemma 4.2. (a) follows directly from assumptions (A2), (A4), (A5) and
Lemma 4.1(a).
(b) We have
_p�;c ¼ ð1� p�mÞg1ð�; cÞ; ð4:9Þ_m�;c ¼ ½minfmð�; cÞ; 1� pg �m�þg2ð�; cÞ: ð4:10Þ
Let x 2 �nN, with N � � of zero measure and consider z ¼ ðp;mÞ. By Lemma
4.1(a), jjz�kjjW 1;1ð0;T ;L1ð�ÞÞ � M 8 k, thus jjz�kjjW 1;pð0;T ;L1ð�ÞÞ � M 8 k; 8 p <1. Thus,
there exists a subsequence, f�k 0 g, and some z such that
z�k 0 ðx; �Þ ! zðx; �Þ weakly-star in W 1;1ð0;T Þ; for a:e: x 2 �:
Thus, we have
_z�k 0 ðx; �Þ ! z:ðx; �Þ weakly in Lpð0;T Þ 8 p <1; for a:e: x 2 �: ð4:11Þ
z� 0kðx; �Þ ! zðx; �Þ strongly in C½0;T �; for a:e: x 2 �: ð4:12Þ
Since the solution to (4.3a)�(4.3b) is unique we have zðx; �Þ ¼ z�ðx; �Þ and the con-
vergence holds for the whole sequence, hence we can conclude that z�kðx; tÞ ! z�ðx; tÞpointwise in Q. Since �k ! � strongly in L2ðQT Þ, using assumption (A4), possibly
extracting a subsequence, we have
�Lpð�k 0 Þ _p�k 0 ;c þ �Lmð�k 0 Þ _m�k 0 ;c ! �Lpð�Þ _p� þ �Lmð�Þ _m� a:e: in QT : ð4:13Þ
But, applying Lebesgue theorem, we get
Bð�k 0 ; cÞ ! Bð�; cÞ strongly in LpðQT Þ:Since the limit does not depend on the extracted subsequence the convergence holds
for the whole sequence f�kg, hence we obtain (4.8).
(c) follows directly from assumption (A2) and Lemma 4.1(b).
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Lemma 4.3. Let c 2 L2ð0;T ;L2ð�ÞÞ. Then there exists a unique �ðcÞ 2 H 2;1ðQT Þand a unique zðcÞ ¼ ðpðcÞ; mðcÞÞ 2 W 1;1ð0; T ; L1ð�ÞÞ �W 1;1ð0;T ; L1ð�ÞÞ,satisfying
��ð�Þ @�@t
� divðkr�Þ ¼ Bð�; cÞ in QT ; ð4:14aÞ
�k@�
@�¼ hð�� ��Þ on @�� ð0;T Þ; ð4:14bÞ
�ðx; 0Þ ¼ �0 in �; ð4:14cÞzt ¼ fðz; �; cÞ in QT ; ð4:14dÞ
zð0Þ ¼ 0 in �; ð4:14eÞ
where f is de¯ned as in (4.1a). Moreover, there exist �1; �2 > 0 such that
jj�1 � �2 jj2L 2ð0;t;L 2ð�ÞÞ � �1
Z t
0
jjc1 � c2 jj 2L2ð0;s;L 2ð�ÞÞds ð4:15Þ
and
jjjz1 � z2jjj2L 2ð0;t;L 2ð�ÞÞ � �2
Z t
0
jjc1 � c2 jj2L 2ð0;s;L 2ð�ÞÞds; ð4:16Þ
where ð�i; ciÞ is the solution corresponding to ci; i ¼ 1; 2.
Proof of Lemma 4.3. Existence. We introduce the operator
P : L2ðQT Þ ! L2ðQT Þ;
� ¼ P �;
by demanding � to be the solution of the linear parabolic problem
��ð�Þ @�@t
� k4� ¼ Bð�; cÞ in QT ; ð4:17aÞ
�k@�
@�¼ hð�� ��Þ on @�� ð0;T Þ; ð4:17bÞ
�ðx; 0Þ ¼ �0 in �: ð4:17cÞ
According to classical results about parabolic equations, problems (4.17a)�(4.17c)
has a unique strong solution � 2 H 2;1ðQT Þ (see, for instance, Ref. 19), therefore the
operator P is well-de¯ned.
Moreover, thanks to Lemma 4.2(a), there exists a constant M > 0, independent of
�, such that:
jj�jjH 2;1ðQT Þ � M : ð4:18Þ
We shall now show the continuity of the operator P.
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Let ð�nÞ � L2ðQT Þ with �n ! � strongly in L2ðQT Þ. De¯ning �n ¼ P �n, in view of
(4.18), jj�n jjH 2;1ðQT Þ � M. Thus, we can ¯nd a subsequence �n 0 such that
�n 0 ! � weakly in H 2;1ðQT Þ; strongly in L2ðQT Þ; ð4:19aÞ�n 0 ! � a:e: in QT : ð4:19bÞ
Testing Eq. (4.17a), written for the index n 0, by 2 L2ð0; t;H 1ð�ÞÞ, we getZ t
0
Z�
��ð�n 0 Þ�n 0;s dx dsþ k
Z t
0
Z�
r�n 0rdx ds
þZ t
0
Z@�
hðÞð�n 0 � ��Þ d ds�Z t
0
Z�
Bð�n 0 ; cÞdx ds ¼ 0: ð4:20Þ
By means of (4.19a)�(4.19b) we can pass to the limit in the last three terms of (4.20).
We can break the ¯rst term in to two terms
�
Z t
0
Z�
�ð�n 0 Þ�n 0;sdx ds ¼ �
Z t
0
Z�
�ð�n 0 Þð�n 0;s � �sÞ dx dsþ �
Z t
0
Z�
�ð�n 0 Þ�s dxds:
Thanks to the continuity of �, we have that
�ð�n 0 Þ! �ð�Þ a:e: in QT
thus, using Lebesgue theorem, ��ð�n 0 Þ! ��ð�Þ strongly inL2ðQT Þwhile �n 0;s ! �sweakly in L2ðQT Þ. Thus,
R t
0
R��ð�n 0 Þð�n 0;s � �sÞ dx ds ! 0 and
�
Z t
0
Z�
�ð�n 0 Þ�n 0;s dx ds ! �
Z t
0
Z�
�ð�Þ�s dx ds:
Hence we have obtained
�
Z t
0
Z�
�ð�Þ�sdx dsþ k
Z t
0
Z�
r�r dx ds
þZ t
0
Z@�
hðÞð�� ��Þ d ds �Z t
0
Z�
Bð�; cÞdx ds ¼ 0:
As the solution to the parabolic problem (4.17a)�(4.17c) is unique, we have
� ¼ P � a:e: in QT
and, since the limit does not depend on the extracted subsequence, it follows that
P �n ! P �
weakly in H 2;1ðQT Þ and strongly in L2ðQT Þ.Now, let
K :¼ fu 2 L2ðQT Þ : jjujjH 2;1ðQT Þ � Mg:
K is non-empty, convex, closed and relatively compact subset of L2ðQT Þ and F :
K � L2ðQT Þ ! K is a continuous mapping. By Schauder ¯xed point theorem, there
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exists a ¯xed point of the mapping F, i.e. there exists a weak solution � 2 H 2;1ðQT Þ to(3.1a), (3.1e) and (3.1g).
Uniqueness and stability. Let
Jð�Þ :¼Z �
0
��ð�Þd�: ð4:21Þ
Integration of (3.1a) with respect to time leads toZ t
0
Bð�; cÞðx; sÞds ¼ Jð�ðx; tÞÞ � Jð�0ðxÞÞ � k�
Z t
0
�ðx; sÞds: ð4:22Þ
Now, let �1; �2 2 H 2;1ðQT Þ be solutions to (3.1a), (3.1e) and (3.1g) corresponding to
c1; c2 respectively. Inserting these solutions into (4.22), subtracting both equations,
and testing by � :¼ �1 � �2, we ¯ndZ t
0
Z�
Z s
0
Bð�1ðx; �Þ; c1ðx; �ÞÞ � Bð�2ðx; �Þ; c2ðx; �ÞÞd�� �
�ðx; sÞdx ds
¼Z t
0
Z�
½Jð�1ðx; sÞÞ � Jð�2ðx; sÞÞ��ðx; sÞdx ds
þ k
Z t
0
Z�
rZ s
0
�ðx; �Þd�� �
r�ðx; sÞdx ds
þZ t
0
Z@�
Z s
0
hðÞ�ð; �Þd�� �
�ð; sÞd ds: ð4:23Þ
Concerning the last term we can see thatZ t
0
Z@�
Z s
0
hðÞ�ð; �Þd�� �
�ð; sÞd ds
¼Z t
0
Z@�
hðÞZ s
0
�ð; �Þ d�� �
�ð; sÞd ds
¼ 1
2
Z t
0
Z@�
hðÞ d
ds
Z s
0
�ð; �Þd�� �2
d ds
¼ 1
2
Z@�
hðÞZ t
0
�ð; sÞds� �2
d:
Thus, from (4.23) we getZ t
0
Z�
Z s
0
Bð�1ðx; �Þ; c1ðx; �ÞÞ �Bð�2ðx; �Þ; c2ðx; �ÞÞðx; �Þd�� �
�ðx; sÞdx ds
��
Z t
0
Z�
�2ðx; sÞdx dsþ k
2
Z�
rZ t
0
�ðx; sÞds����
����2
dx
þ 1
2
Z@�
hðÞZ t
0
�ð; sÞds� �2
d ��
Z t
0
Z�
�2ðx; sÞdx ds:
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Using H€older's and Young's inequalities and Lemma 4.1 it follows thatZ t
0
Z�
Z s
0
Bð�1ðx; �Þ; c1ðx; �ÞÞ � Bð�2ðx; �Þ; c2ðx; �ÞÞd�� �
�ðx; sÞdx ds����
����� 1
4
Z t
0
Z�
Z s
0
Bð�1ðx; �Þ; c1ðx; �ÞÞ � Bð�2ðx; �Þ; c2ðx; �ÞÞd�� �2
dx ds
þ
Z t
0
jj�ð�; sÞjj2L 2ð�Þ ds
� T
4
Z t
0
Z�
Z s
0
K1j�1ðx; �Þ � �2ðx; �Þj2 þ K2jc1ðx; �Þ � c2ðx; �Þj2� �
d�dx ds
þ
Z t
0
jj�ð�; sÞjj2L 2ð�Þ ds
� CT
4
Z t
0
jj�jj2L 2ð0;s;L 2ð�ÞÞdsþCT
4
Z t
0
jjcjj 2L2ð0;s;L2ð�ÞÞ ds
þ
Z t
0
jj�ð�; sÞjj2L 2ð�Þ ds:
Thus, we have
��
Z t
0
Z�
�2ðx; sÞdx ds � CT
4
Z t
0
jj�jj 2L2ð0;s;L 2ð�ÞÞds
þ CT
4
Z t
0
jjcjj 2L2ð0;s;L 2ð�ÞÞ dsþ
Z t
0
jj�ð�; sÞjj2L 2ð�Þ ds:
Choosing > 0 such that ��� > 0 we have:
jj�jj2L 2ð0;t;L 2ð�ÞÞ � �
Z t
0
jj�jj2L 2ð0;s;L 2ð�ÞÞds þ �
Z t
0
jjcjj2L 2ð0;s;L 2ð�ÞÞds
with constants �; � > 0.
Hence, applying Gronwall lemma, we ¯nd a constant C1 such that
jj�1 � �2 jj2L 2ð0;t;L 2ð�ÞÞ � C1
Z t
0
jjc1ðsÞ � c2ðsÞjj2L 2ð0;s;L 2ð�ÞÞds: ð4:24Þ
Inequality (4.16) follows immediately from Lemma 4.1(b) and estimate (4.15).
The proof of Lemma 4.3 is thus complete.
Now, we are in a position to prove Theorem 3.1.
Let us denote
�ð�; cÞ :¼ ð1� p�mÞDð�; cÞ:
We note that, in view of (A6) and Lemma 4.1(b), � is Lipschitz-continuous with
respect to � and c.
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We de¯ne an operator
T : L2ðQT Þ ! L2ðQT Þ;
T c ¼ c;ð4:25Þ
by demanding c to be the solution of the parabolic problem
@c
@t� divð�crcÞ ¼ 0 in QT ; ð4:26aÞ
��c@c
@�¼ �ðc� cpÞ on @�� ð0;T Þ; ð4:26bÞ
cðx; 0Þ ¼ c0 in �; ð4:26cÞ
where �c ¼ ð1� pc �mcÞDð�c; cÞ; ð�c; pc;mcÞ being the solution to (3.1a), (3.1c) and
(3.1d) with respect to given c. Denoting
aðc; ; tÞ :¼Z�
�crcr dxþZ@�
� c d;
hfðtÞ; i :¼Z@�
�cp d; 2 H 1ð�Þ;
we have that problem (4.26a)�(4.26c) is equivalent to the following. We seek a
function c such that, for all 2 H 1ð�Þ and a.e. in t 2 ð0;T Þd
dtcðtÞ;
� �þ aðcðtÞ; ; tÞ ¼ hfðtÞ; i; ð4:27aÞ
cð0Þ ¼ c0; ð4:27bÞc 2 W ð0;T Þ; ð4:27cÞ
where h ; i denotes the duality between H 1ð�Þ and ðH 1ð�ÞÞ�.In view of (A3), (A6), (A7), admits a unique solution c (cf. Ref. 27, Prop. 30.10).
Moreover, there exists a constant M independent of c, such that
jjcjjWð0;T Þ � M : ð4:28Þ
To derive the continuity of the operator T , let fcng � L2ð0;T ;L2ð�ÞÞ, with cn ! c
strongly in L2ðQT Þ. De¯ning cn ¼ T cn, thanks to (4.28), we have jjcn jjWð0;T Þ � M .
Thus, there exists a subsequence fcn 0 g such that
cn 0 ! c weakly in W ð0;T Þ: ð4:29Þ
We test (4.26a) by
�ðx; tÞ ¼ ðtÞðxÞ with 2 C 1½0;T �; ðT Þ ¼ 0; 2 H 1ð�Þ: ð4:30Þ
Denoting T cn 0 :¼ cn 0 , we haveZ T
0
Z�
cn 0;s�dx dsþZ T
0
Z�
�cn 0 rcn 0r�dx dsþZ T
0
Z@�
�ðcn 0 � cpÞ�d ds ¼ 0: ð4:31Þ
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Concerning the ¯rst term in (4.31) we haveZ T
0
Z�
cn 0;s � dx ds ¼ �Z�
cn 0 ðx; 0Þ�ðx; 0Þdx�Z T
0
Z�
cn 0 �s dx ds:
Now, Z�
cn 0 ðx; 0Þ�ðx; 0Þdx ¼Z�
c0 �ðx; 0Þdx;
and, by virtue of (4.29),Z T
0
Z�
cn 0 �s dx ds !Z T
0
Z�
c�s dx ds a:e: in QT :
The second term can be rearranged asZ T
0
Z�
�cn 0 rcn 0r�dx ds
¼Z T
0
Z�
�cn 0 ðrcn 0 � rcÞr� dx dsþZ T
0
Z�
�cn 0 rcr�dx ds:
Since � is continuous and bounded as a function of c, possibly extracting a sub-
sequence, we obtain: �cn 0 ðx; tÞ ! �cðx; tÞ a.e. in QT , therefore �cn 0 ðx; tÞr� !�cðx; tÞr� pointwise, moreover �cn 0 ðx; tÞr� is bounded in L2 thus, using Lebesgue
theorem, we have
�cn 0 r� ! �cr� strongly in L2ðQT Þ:
Moreover, ðrcn 0 � rcÞ ! 0 weakly in L2ðQT Þ because of (4.29), thus we obtainZ T
0
Z�
�cn 0 rcn 0r� dx ds !Z T
0
Z�
�crcr� dx ds:
Applying the trace theorem, the last term in (4.31) converges too.
Thus, we can pass to the limit in (4.31) obtaining
� ð0ÞZ�
c0 ðxÞdx�Z T
0
Z�
c s dx ds
þZ T
0
Z�
�crcr dx dsþZ T
0
Z@�
�ðc� cpÞ d ds ¼ 0: ð4:32Þ
ConsequentlyZ T
0
Z�
cs dxþZ�
�crcr dxþZ@�
�ðc� cpÞd� �
ds ¼ 0:
The above is true for ; satisfying (4.32). Therefore (4.32) gives, a.e. in t 2 ð0;T Þ
d
dtcðtÞ;
� �þ aðt; cðtÞ; Þ ¼ hF ðtÞ; i 8 2 H 1ð�Þ:
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Since the solution of (4.26a)�(4.26c) is unique, we can conclude
T c ¼ c;
and, since the limit does not depend on the extracted subsequence, it follows that
T cn ! T c ð4:33Þ
weakly in W ð0;T Þ and strongly in L2ðQT Þ.Now, let
K :¼ fv 2 L2ðQT Þ : jjvjjWð0;T Þ � Mg:
K is convex and compact in L2ðQT Þ and F : K � L2ðQT Þ ! K is a continuous
mapping. By the Schauder ¯xed point theorem the proof is concluded.
5. Proof of Theorem 3.2
We commence with the following regularity result:
Lemma 5.1. Under the assumptions of Theorem 3.2, the solutions �, c to the
initial�boundary value problems related to Eqs. (3.1a)�(3.1b) are in W 2;15 ðQT Þ.
Proof. Since we proved the existence of at least one solution for the initial-boundary
value problems related to Eqs. (3.1a), (3.1b), we can now follow the approach
developed by Griepentrog, in Refs. 8 and 9 about linear parabolic equations with
nonsmooth bounded coe±cients, in order to improve the regularity of the solutions
under consideration.
The coe±cients and the right-hand sides of the equations are indeed functions in
L1ðQT Þ and the coe±cients in the boundary conditions too.
Moreover, the initial conditions are Lipschitz-continuous functions and we can
apply Th. 3.4 and Th. 6.8 of Ref. 8 and Th. 6.1 of Ref. 9, whence we obtain that � and
c are in Cð�QT Þ.It follows that the right-hand sides of the ODEs (3.1c)�(3.1d) are continuous
functions, therefore the corresponding solutions are continuously di®erentiable.
Thus, the PDEs (3.1a)�(3.1b) have continuous coe±cients and we can apply
a classical result of Ladyzenskaja (Ref. 19, Th. 9.1, p. 341) which yields: �, c 2W 2;1
5 ðQT Þ.
Lemma 5.2. Assuming that � is constant, we have that, for every c1; c2 2 L2ðQT Þ,there exists a constant M > 0 such that, for the corresponding �1; �2, it holds:
jj�1 � �2 jj2H 2;1ðQT Þ � M jjc1 � c2 jj 2L2ðQT Þ: ð5:1Þ
Proof. We consider the heat equation of our system:
���t ¼ k��þ �Lppt þ �Lmmt: ð5:2Þ
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We write (5.2) for �1; c1; p1;m1 and �2; c2; p2;m2. Subtracting and denoting as usual
� ¼ �1 � �2, we see that the di®erence satis¯es the following system:
���t � k�� ¼ �ðLpð�1Þp1;t � Lpð�2Þp2;tÞ þ �ðLmð�1Þm1;t � Lmð�2Þm2;tÞ ¼: f;
�k@�
@�¼ h�;
�ðx; 0Þ ¼ 0:
Applying again standard parabolic theory (cf. Ref. 21 Th. 6.2, Chap. 6), we know
that there exists a positive constant K such that we can estimate the norm of the
solution as follows:
jj�jjH 2;1ðQT Þ � KjjfjjL2ðQT Þ:
Now we can estimate the term jjfjjL 2ðQT Þ, by means of Lemma 4.1(b) and assumptions
(A2), as:
jj�ðLpð�1Þp1;t � Lpð�2Þp2;tÞ þ �ðLmð�1Þm1;t � Lmð�2Þm2;tÞjjL 2ðQT Þ
� K1jj�1 � �2 jjL 2ðQT Þ þK2jjc1 � c2 jjL2ðQT Þ;
with K1;K2 positive constants. Now, using Lemma 4.3, we can estimate the term
jj�1 � �2 jjL 2ðQT Þ and therewith ¯nish the proof.
Lemma 5.3. Let u 2 L1ð0;T ;L2ð�ÞÞ \ L2ð0;T ;H 1ð�ÞÞ, then there holds
Z T
0
jjuðtÞjj 10=3L10=3ð�Þ
dt �Z T
0
jjuðtÞjj2L 6ð�Þ
dt
� �jjujj4=3
L1ð0;T ;L 2ð�ÞÞ:
Proof. Owing to Riesz' convexity theorem (cf. Ref. 27, A113), we have
jjujjLrð�Þ � jjujj1��Lq1 ð�Þ
jjujj�Lq2 ð�Þ
;
for all u 2 Lq1ð�Þ \ Lq2ð�Þ with 1 � q1; q2 <1; 0 < � < 1, and 1r ¼ 1��
q1þ �
q2.
Invoking the continuous embedding H 1ð�Þ � L6ð�Þ, the assertion follows by
de¯ning q1 ¼ 6; q2 ¼ 2; � ¼ 25, and r ¼ 10
3 .
We are now in a position to prove Theorem 3.2. We write Eq. (3.1b) for c1 and c2,
subtract, integrate over QT and test by c1 � c2. In the sequel we will use the following
notations: c ¼ c1 � c2; � ¼ �1 � �2; p ¼ p1 � p2; m ¼ m1 �m2. We have
1
2
Z�
c2ðtÞdxþZ t
0
Z�
ðð1� p1 �m1ÞDð�1Þrc1 � ð1� p2 �m2ÞDð�2Þrc2Þrc dx ds
þZ t
0
Z@�
�c2d ds ¼ 0:
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Now,
Z t
0
Z�
ðð1� p1 �m1ÞDð�1Þrc1 � ð1� p2 �m2ÞDð�2Þrc2Þrc dx ds
¼Z t
0
Z�
ð1� p1 �m1ÞDð�1Þjrcj2dx ds�Z t
0
Z�
ðpþmÞDð�1Þrc2rc dx ds
þZ t
0
Z�
ð1� p2 �m2ÞðDð�1Þ �Dð�2ÞÞrc2rc dx ds: ð5:3Þ
Denoting, in the sequel, by Ki generic positive constants independent of � and c, we
obtain
1
2
Z�
c2ðtÞdxþK1
Z t
0
jjrcjj 2L2ð�Þdx ds
�Z t
0
Z�
jpþmjjDð�1Þjjrc2jjrcj dx ds
þZ t
0
Z�
j1� p2 �m2jjDð�1Þ �Dð�2Þjjrc2jjrcj dx ds: ð5:4Þ
By means of Lemma 5.1, we know that c2 2 W 2;15 ðQT Þ. According to Amann (cf.
Ref. 2, Th. 1.1), we have the embedding W 2;15 ðQT Þ ,! Cð½0;T �;W 1
5 ð�ÞÞ.Thus, we can estimate the ¯rst term in the right-hand side of (5.4) as:
Z t
0
Z�
jpþmjjDð�1Þjjrc2jjrcj dx ds
�Z t
0
jjpþmjjL 10=3ð�Þjjrc2 jjL 5ð�ÞjjDð�1ÞjjL1ð�ÞjjrcjjL 2ð�Þds
� K1
4
Z t
0
jjrcjj2L 2ð�Þdsþ4K2
K1
Z t
0
jjpþmjj2L 10=3ð�Þds: ð5:5Þ
Moreover, thanks to Lemma 4.1(b), we get
Z t
0
jjpþmjj2L 10=3ð�Þds ¼Z t
0
Z�
jpþmj10=3dx� 3=5
ds
� K3
Z t
0
Z s
0
Z�
�10=3
dx d�
� 3=5ds
þK4
Z t
0
Z s
0
Z�
c10=3
dx d�
� 3=5ds: ð5:6Þ
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Now, we apply Lemma 5.3, Young's inequality and the embedding H 1ð�Þ ,! L6ð�Þto the right-hand side of (5.6), obtainingZ t
0
Z s
0
Z�
�10=3
dx d�
� 3=5ds �
Z t
0
Z s
0
K5jj�jj2H 1ð�Þd�
� 3=5jj�jj 4=5L1ð0;s;L 2ð�ÞÞds
� 3K5
5
Z t
0
Z s
0
jj�jj2H 1ð�Þd� ds þ 2
5
Z t
0
jj�jj 2L1ð0;s;L 2ð�ÞÞds:
ð5:7Þ
Analogously, it holdsZ t
0
Z s
0
Z�
c10=3
dx d�
� 3=5ds � 3K5
5
Z t
0
Z s
0
jjcjj 2H 1ð�Þd� dsþ2
5
Z t
0
jjcjj2L1ð0;s;L 2ð�ÞÞds:
ð5:8Þ
Regarding the second term on the right-hand side of (5.4), using Lemma 4.1,
assumption (A6) and Young's inequality again, we haveZ t
0
Z�
j1� p2 �m2jjDð�1Þ �Dð�2Þjjrc2jjrcj dx ds
� jjrc2 jjL1ð0;t;L3ð�ÞÞ
Z t
0
jj�jjL 6ð�ÞjjrcjjL 2ð�Þds
� K6
Z t
0
jj�jj2H 1ð�Þds þ K1
4
Z t
0
jjrcjj2L 2ð�Þds: ð5:9Þ
Using (5.4) to (5.9), we ¯nd that
min1
2;K1
2
�Z�
c2ðtÞdxþZ t
0
jjrcjj2L 2ð�Þds
� K7
Z t
0
jj�jj 2H 1ð�ÞdsþZ t
0
jj�jj2L1ð0;s;L 2ð�ÞÞds
� �þ 3K5
5
Z t
0
Z s
0
jj�jj2H 1ð�Þd� ds
þ K8
Z t
0
Z s
0
jjcjj2H 1ð�Þd�dsþZ t
0
jjcjj 2L1ð0;s;L2ð�ÞÞds
� �: ð5:10Þ
Thanks to the embedding W 2;12 ðQT Þ ,! Cð½0;T �;W 1
2 ð�ÞÞ (see Ref. 2, Th. 1.1) and
Lemma 5.2, we obtain for the ¯rst term in the right-hand side of (5.10):Z t
0
jj�ðsÞjj 2H 1ð�Þds �Z t
0
jj�jj 2L1ð0;s;H 1ð�ÞÞds
� K9
Z t
0
jj�jjH 2;1Qs
ds
�Z t
0
K10
Z s
0
jjcjj 2L2ð�Þd� ds: ð5:11Þ
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Analogous estimates hold for the other terms involving �. Thus we end up with
jjcðtÞjj 2L2ð�Þ þZ t
0
jjrcjj 2L2ð�Þds
� K11
Z t
0
jjcjj2L1ð0;s;L 2ð�ÞÞdsþK12
Z t
0
Z s
0
jjrcjj2L2ð�Þd� ds
þK13
Z t
0
Z s
0
jjcjj2L2ð�Þd� ds 8 t 2 ½0;T �: ð5:12Þ
Taking the essential supremum over ½0; t� for some t 2 ½0;T � in the previous
inequality, we obtain
jjcðtÞjj 2L1ð0;tL 2ð�ÞÞ þZ t
0
jjrcjj2L 2ð�Þ
� K11
Z t
0
jjcjj2L1ð0;s;L 2ð�ÞÞdsþK12
Z t
0
Z s
0
jjrcjj2L 2ð�Þd� ds
þK13
Z t
0
Z s
0
jjcjj2L 2ð�Þd� ds: ð5:13Þ
SinceR t
0
R s
0jjcjj2L 2ð�Þd� ds � T
R t
0jjcjj 2L1ð0;s;L 2ð�ÞÞds, we can apply the Gronwall lemma
and conclude the proof of Theorem 3.2.
The following table contains the parameters involved in the complete process.
6. Numerical Results
In this section we present some numerical simulations to demonstrate the e®ect of gas
carburizing on a sample workpiece. The simulations are based on our model (3.1a)�(3.1j). As a sample con¯guration, we consider the cross section of a cylinder of radius
50mm. Note that our initial temperature is chosen above the austenitization tem-
perature such that we may assume it to be homogeneously austenitic. Material
parameters are taken from the data tables for the low-carbon steel AISI 4130. The
interval time ð0;T Þ of the whole process is divided as ð0;Tc� [ ½Tc;T Þ, where Tc
denotes the ending time of carburization.
For the process parameters we refer to Table 1. The expression for Dð�; cÞ is takenfrom Ref. 24, the value of h is taken from Ref. 15. For the function g1 we took the data
of Ref. 6, cf. Fig. 4. g2 has been taken constant as in Ref. 13, which has been found
su±cient to describe the kinetics of the phase transition. The main coupling e®ect is
through the carbon dependent start and end temperature of the martensite for-
mation, MsðcÞ and MfðcÞ respectively, which have been identi¯ed from Fig. 3. The
simulations were performed with Femlab, a software based on the ¯nite element
method.
Figure 5 is a view of a sector of the sample con¯guration that we considered, after
carburizing for about eight hours.
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0 100 200 300 400 500 600 700 800 9000
0.02
0.04
0.06
0.08
0.1
0.12
0.14
0.16
0.18
0.2
Temperature, oC
g 1(θ)
Fig. 4. Plot of the transformation function g1, depending on the temperature �.
Table 1. Process parameters.
Value Unit Value Unit
� 7800 kg=m3 �0 1150 K
� 385 J=kg K c0 0.25 weight %
Lp 77,000 J=kg cp 1.2 weight %
Lm 82,000 J=kg �� 300 K
� ðif t � T1Þ 6e-5 m=s � ðif T1 < t � T Þ 0 m=sh ðif t � T1Þ 0 W=m2K h ðif T1 < t � T Þ 10,000 W=m2KD 0:47 expð�1:6c� ð37000� 6600cÞ=ð1:987T ÞÞ1e� 4 m2=s
k 35 W=mK
Fig. 5. Snapshot of the simulation at time t ¼ 30;120 s (after 30,000 seconds carburizing and 120 seconds
quenching) showing the carburizing e®ect. In the right column carbon percentage is indicated.
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As already mentioned in the Introduction the process consists of at least two
stages: ¯rst, the workpiece is immersed in a carbon-rich atmosphere furnace (the
so-called carburizing); secondly, quenching is performed, through which austenite is
transformed into the hard phase martensite m, where the temperature gradient is
high and into pearlite p where the temperature gradient is lower. In other words, the
hardening occurs close to the boundary, while in the core the softer phase pearlite is
formed. The e®ect of time and temperature on total case depth (which is usually
speci¯ed as the layer at carbon content 0.4%) is shown in Fig. 6.
In Fig. 7 we can observe the distribution of phase fractions at the end of a cycle of
carburizing and quenching.
In the same ¯gure we can see how the formation of martensite depends on the
carbon concentration, in accordance with the graphic of Fig. 3 of the ¯rst section.
Indeed, as we can see in Fig. 3, the martensite terminal temperature is well below
zero, because of the residual austenite at room temperature which cannot be trans-
formed into martensite, thus 100% of martensite is not achieved; in Fig. 7, derived
from our simulations, the maximum of the martensite phase fraction is about 65%.
The maximum of the martensite fraction is not achieved on the surface, but at the
total case depth, i.e. where the carbon concentration corresponds to 0.4%.
Fig. 6. Plot of total case depth vs. carburizing time at four selected temperatures. Graph based on data in
table.
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7. Concluding Remarks
In this paper we have studied a mathematical model of case hardening, including the
coupling between carbon di®usion equation, temperature evolution and phase tran-
sitions. From mathematical point of view, we have proved existence and uniqueness
of a solution. First numerical results con¯rm qualitative agreement with experiments.
A more detailed comparison requires more precise data. To this end a cooperation
with some engineering institutes has been started. The results will be published in a
forthcoming paper.
From a practical point of view, a reduction of energy consumption and of process
time as well as increasing the process stability are of great interest. Therefore the
development of an optimal control strategy is under study.
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