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Existence and uniqueness for a nonlinear
parabolic/Hamilton-Jacobi coupled system describing the dynamics of dislocation densities
Hassan Ibrahim
To cite this version:
Hassan Ibrahim. Existence and uniqueness for a nonlinear parabolic/Hamilton-Jacobi coupled system
describing the dynamics of dislocation densities. 2007. �hal-00138531�
hal-00138531, version 1 - 26 Mar 2007
paraboli/Hamilton-Jaobi oupled system desribing
the dynamis of disloation densities
Hassan IBRAHIM
∗
Marh27, 2007
Abstrat
We study a mathematial model desribing the dynamis of disloation densities in rystals. This
model is expressed as a one-dimensional system of a paraboliequation and a rst order Hamilton-
Jaobiequationthatareoupledtogether. Weshowtheexisteneanduniquenessofavisositysolution
amongthoseassumingalower-boundontheirgradientforalltimeinludingtheinitialdata. Moreover,
weshowtheexisteneofavisositysolutionwhenwehavenosuh restritionontheinitialdata. We
alsostatearesultofexisteneanduniquenessofanentropysolutionofthesystemobtainedbyspatial
derivation. Theuniquenessofthisentropysolutionholdsinthelassofboundedfrombelowsolutions.
Inordertoprovetheseresults,weusearelationbetweensalaronservationlawsandHamilton-Jaobi
equations, mainlyto getsomegradientestimates. This studywill takeplaein
R
, andon abounded domainwithsuitableboundaryonditions.Resumé
Nous étudions unmodèle mathématique dérivant ladynamique de densités de disloations dans les
ristaux. Ce modèles'érit ommeunsystème 1Douplantune équationparaboliqueet uneéquation
deHamilton-Jaobidupremierordre.Onmontrel'existeneetl'uniitéd'unesolutiondevisositédans
lalassedesfontionsayantungradientminorépourtouttempsainsiqu'autempsinitial. Deplus,on
montre l'existened'unesolutionde visositésansette onditionsur ladonnéeinitiale. On présente
égalementun résultat d'existene et d'uniité pour une solutionentropiqued'un système obtenu par
dérivation spatiale. L'uniité deettesolutionentropiquealieu danslalassedessolutionsminorées.
Pourmontreresrésultats,onutiliseunerelationentrelesloisdeonservationsalaireetleséquations
deHamilton-Jaobi,prinipalementpourobtenirdesontrlesdugradient. Cetteétudealieu dans
R
etdansundomaineborné avedesonditionsauxbordsappropriées.
AMS Classiation: 70H20,35L65,49L25,54C70,74H20,74H25.
Key words: Hamilton-Jaobiequations, salaronservation laws,visositysolutions, entropy solu-
tions,dynamisofdisloationdensities.
∗
Cermis,EoledesPonts,ParisTeh,6et8avenueBlaisePasal,CitéDesartesChamps-sur-Marne,77455
Marne-la-ValléeCedex2,Frane
1.1 Physial motivation
A disloation is a defet, or irregularity within a rystal struture that an be observed by
eletron mirosopy. The theory was originally developed by Vito Volterra in 1905. Disloa-
tions area non-stationary phenomena and their motionis themain explanation of theplasti
deformation inmetallirystals (see[28 , 19℄for a reent and mathematial presentation).
Geometrially, eah disloation is haraterized by a physial quantity alled the Burgers
vetor, whih is responsible for its orientation and magnitude. Disloations are lassied as
being positive or negative due to the orientation of its Burgers vetor, and they an move in
ertainrystallographi diretions.
Startingfromthe motionofindividualdisloations, aontinuumdesriptionanbederived
by adopting a formulation of disloation dynamis in terms of appropriately dened disloa-
tion densities, namely the density of positive and negative disloations. In this paper we are
interested in the model desribed by Groma, Csikor and Zaiser [18℄, that sheads light on the
evolutionofthedynamisofthetwotypedensitiesofasystemofstraightparalleldisloations,
taking into onsideration the inuene of the short range disloation-disloation interations.
Themodelwasoriginally presentedin
R 2 × (0, T )
asfollows:
∂θ +
∂t + b · ∂
∂ r
θ +
(τ sc + τ ef f ) − AD b
(θ + + θ − ) · ∂
∂ r θ + − θ −
= 0,
∂θ −
∂t − b · ∂
∂ r
θ −
(τ sc + τ ef f ) − AD b
(θ + + θ − ) · ∂
∂ r θ + − θ −
= 0.
(1.1)
Where
T > 0
,r = (x, y)
represents the spatial variable,b
is the burger's vetor,θ + ( r , t)
and
θ − ( r , t)
denote the densities of the positive and negative disloations respetively. The quantityA
isdened by the formulaA = µ/[2π(1 − ν)]
, whereµ
is theshear modulus andν
is the Poisson ratio.
D
is a non-dimensional onstant. Stress elds are represented through the self-onsistent stressτ sc ( r , t)
, and the eetive stressτ ef f ( r , t)
.∂r ∂
denotes the gradientwithrespetto the oordinate vetor
r
. An earlier investigation of theontinuum desription of the dynamis of disloation densities has been done in [17℄. However, a major drawbakof these investigations is that the short range disloation-disloation orrelations have been
negleted and disloation-disloation interations were desribed only bythe long-range term
whih isthe self-onsistent stress eld. Moreover, forthe modeldesribed in[17℄,we refer the
reader to [11 , 12 ℄ for a one-dimensional mathematial and numerial study, and to [4℄ for a
two-dimensional existeneresult.
In our work,we are interestedina partiular setting of(1.1) where we make thefollowing
assumptions:
(a1) thequantities inequations (1.1) areindependent of
y
,(a2)
b = (1, 0)
,and theonstantsA
andD
aresetto be1
,(a3) theeetive stressis assumedto be zero.
Remark 1.1 (a1) gives that the self-onsistent stress
τ sc
is null; this is a onsequene of thedenitionof
τ sc
(see [18℄).Assumptions(a1)-(a2)-(a3)permitrewritingtheoriginalmodelasa
1D
probleminR × (0, T )
:
θ + t (x, t) −
θ + (x, t)
θ x + (x, t) − θ x − (x, t) θ + (x, t) + θ − (x, t)
x
= 0, θ − t (x, t) +
θ − (x, t)
θ x + (x, t) − θ x − (x, t) θ + (x, t) + θ − (x, t)
x
= 0.
(1.2)
We onsideran integratedform of(1.2) and we let:
ρ ± x = θ ± , θ = θ + + θ − , ρ = ρ + − ρ −
andκ = ρ + + ρ − ,
(1.3)in order to obtain, for speial values of the onstants of integration, the following system of
PDEsinterms of
ρ
andκ
:( κ t κ x = ρ t ρ x
inQ T = R × (0, T ), κ(x, 0) = κ 0 (x)
inR ,
(1.4)
and
(
ρ t = ρ xx
inQ T , ρ(x, 0) = ρ 0 (x)
inR ,
(1.5)
where
T > 0
isa xedonstant. Enough regularityontheinitialdatawillbegiveninordertoimpose thephysiallyrelevant ondition,
κ 0 x ≥ | ρ 0 x | .
(1.6)This ondition is natural: it indiates nothing but thepositivity of the disloation densities
θ ± (x, 0)
atthe initial time(see(1.3)).1.2 Main results
In this paper, we show the existene and uniqueness of a visosity solution
κ
of (1.4) in thelassofallLipshitzontinuousvisositysolutions having speialbounded frombelow spatial
gradients. However, we show the existene of aLipshitz ontinuousvisosity solution of (1.4)
when this restrition is relaxed. A relation between salar onservation laws and Hamilton-
Jaobi equations will be exploited to get almost all our gradient ontrols of
κ
. This relation,that will be made preise later, will also lead to a result of existene and uniqueness of a
bounded entropy solutionof the following equation:
θ t = ρ x ρ xx
θ
x
in
Q T , θ(x, 0) = θ 0 (x)
inR ,
(1.7)
whih is dedued formally by taking a spatial derivation of (1.4). The uniqueness of this
entropy solution is always restrited to the lass of bounded entropy solutions witha speial
lower-bound.
Let
Lip( R )
denotes:Lip( R ) = { f : R 7→ R ; f
is aLipshitz ontinuousfuntion} .
We prove the following theorems:
Let
T > 0
. Takeκ 0 ∈ Lip( R )
andρ 0 ∈ C 0 ∞ ( R )
as initial data that satisfy:κ 0 x ≥ p
(ρ 0 x ) 2 + ǫ 2
a.e. inR ,
(1.8)for some onstant
ǫ > 0
. Then, given the solutionρ
of (1.5), there exists a visosity solutionκ ∈ Lip( ¯ Q T )
of (1.4), unique among the visosity solutions satisfying:κ x ≥ p
ρ 2 x + ǫ 2
a.e. inQ ¯ T .
Theorem 1.3 (Existene and uniquenessof an entropy solution)
Let
T > 0
. Takeθ 0 ∈ L ∞ ( R )
andρ 0 ∈ C 0 ∞ ( R )
suh that,θ 0 ≥ p
(ρ 0 x ) 2 + ǫ 2
a.e. inR ,
for some onstant
ǫ > 0
. Then, there exists an entropy solutionθ ∈ L ∞ ( ¯ Q T )
of (1.7), uniqueamong the entropy solutions satisfying:
θ ≥ p
ρ 2 x + ǫ 2
a.e. inQ ¯ T .
Moreover, we have
θ = κ x
, whereκ
isthe solution given by Theorem 1.2.The notion of visosity solutions and entropy solutions will be realled inSetion 2. We now
relate these results to our one-dimensional problem(1.2). Remarking that
ρ x = θ + − θ −
andκ x = θ + + θ −
,wehave asa onsequene:Corollary 1.4 (Existene and uniqueness for problem (1.2))
Let
T > 0
. Letθ 0 +
andθ 0 −
be two given funtions representingthe initial positive and negative disloation densities respetively. If the followingonditions are satised:(1)
θ + 0 − θ 0 − ∈ C 0 ∞ ( R ),
(2)
θ + 0
,θ 0 − ∈ L ∞ ( R )
,togetherwith,
θ + 0 + θ − 0 ≥ q
(θ + 0 − θ − 0 ) 2 + ǫ 2
a.e. inR ,
thenthere existsasolution
(θ + , θ − ) ∈ (L ∞ (Q T )) 2
tothesystem(1.2),inthesenseofTheorems1.2and 1.3,unique among those satisfying:
θ + + θ − ≥ p
(θ + − θ − ) 2 + ǫ 2
a.e. inQ ¯ T .
Remark 1.5 Conditions (1)and (2)are suient requirements for the ompatibility withthe
regularity of
ρ 0
andκ 0
previously stated.Theorem 1.6 (Existene of a visosity solution, ase
ǫ = 0
)Let
T > 0
,κ 0 ∈ Lip( R )
andρ 0 ∈ C 0 ∞ ( R )
. If the ondition (1.6) is satised a.e. inR
, then there exists a visosity solutionκ ∈ Lip( ¯ Q T )
of (1.4) satisfying:κ x ≥ | ρ x |
a.e. inQ ¯ T .
(1.9)Remark 1.7 Inthelimitasewhere
ǫ = 0
,weremarkthathaving(1.9)wasintuitivelyexpeted due tothe positivity of the disloation densitiesθ +
andθ −
. Thisreets in somewaythe well-posedness of the model(1.2) of the dynamis ofdisloation densities. We also remark that our
result of existene of a solution of (1.4)under (1.9)still holds if we startwith
κ 0 x = ρ 0 x = 0
onsomeintervalof thereal line. In otherwords, we an imaginethat we startwiththeprobability
of the formationof no disloation zones.
Problem with boundary onditions.
We onsider one again problem(1.4), similar results to thatannouned above will be shown
ona bounded intervalof thereal linewithDirihlet boundaryonditions(see Setion 5). This
problemorresponds physiallyto thestudy of thedynamis of disloation densitiesina part
ofa materialwiththegeometry of aslab (see [18℄).
1.3 Organization of the paper
The paper isorganized asfollows. In Setion 2, we start bystating the denitionof visosity
and entropy solutions withsome of their properties. In Setion 3, we prove the existeneand
uniqueness of a visosity solution to an approximated problem of (1.4), namely Proposition
3.1, and we move on, giving additional properties of our approximated solution (Proposition
3.2) and onsequently proving Theorems 1.2 and 1.3. In Setion 4, we present the proof of
Theorem 1.6. Setion 5 is devoted to the study of problem (1.4) on a bounded domain with
suitableboundaryonditions. Finally,Setion6isanappendixontainingaskethoftheproof
to thelassial omparison priniple of salar onservationlaws adapted to our equation with
lowregularity.
2 Notations and Preliminaries
We rst x some notations. If
Ω
is an open subset ofR n
,k
is a positive integer, we denoteby
C k (Ω)
the spae of all real valuedk
times ontinuously dierentiable funtions.C 0 k (Ω)
isthe subspae of
C k (Ω)
onsisting offuntion of ompat support inΩ
,andC b k (Ω) = C k (Ω) ∩ W k,∞ (Ω)
whereW k,∞ (Ω)
is dened below. Furthermore, letU C(Ω)
andLip(Ω)
denote thespaes of uniformlyontinuous funtionsand Lipshitzontinuousfuntions on
Ω
respetively.Thesobolevspae
W m,p (Ω)
withm ≥ 1
an integer andp : 1 ≤ p ≤ ∞
a real,isdened byW n,p (Ω) =
u ∈ L p (Ω)
∀ α
with| α | ≤ n ∃ f α ∈ L p (Ω)
suh thatZ
Ω
uD α φ = ( − 1) |α|
Z
Ω
f α φ ∀ φ ∈ C 0 ∞ (Ω)
,
where we denote
D α u = f α
. Thisspae equippedwiththenorm|| u || W n,p = X
0≤|α|≤n
|| D α u || L p
isa Banah spae. Inwhat follows,
T > 0
. A mapm : [0, ∞ ) 7→ [0, ∞ )
that satisfy• m
isontinuous andnon-dereasing;• lim
x→0 + m(x) = 0
;• m(a + b) ≤ m(a) + m(b)
fora, b ≥ 0
;issaidto be amodulus, and
U C x (Ω × [0, T ])
denotes thespae ofthoseu ∈ C(Ω × [0, T ])
forwhih thereis amodulus
m
andr > 0
suhthat| u(x, t) − u(y, t) | ≤ m( | x − y | )
forx, y ∈ Ω, | x − y | ≤ r
andt ∈ [0, T ].
We will dealwithtwo typesofequations:
1. Hamilton-Jaobi equation:
( u t + F(x, t, u x ) = 0
inQ T , u(x, 0) = u 0 (x)
inR ,
(2.1)
2. Salar onservation laws:
( v t + (F (x, t, v)) x = 0
inQ T , v(x, 0) = v 0 (x)
inR ,
(2.2)
where
F : R × [0, T ] × R → R (x, t, u) 7→ F (x, t, u)
isalledtheHamiltonian intheHamilton-Jaobiequations and theuxfuntion inthesalar
onservationlaws. Wewillagreeontheontinuityofthisfuntion,whileadditionalandspei
regularitywill be givenwhen itis needed.
Remark 2.1 We will use the funtion
F
as a notation for the Hamiltonian/ux funtion.Although
F
might dier from oneequation toanother, it will be laried in all whatfollows.Remark 2.2 The major part of this work onerns a Hamiltonian/ux funtion of a speial
form,namely:
F (x, t, u) = g(x, t)f (u),
(2.3)where suh forms often arise in problems of physial interest inluding tra ow [31℄ and
two-phase ow inporous media [16℄.
We start by dening the notion of visosity solution to Hamilton-Jaobi equations (2.1),
andentropysolutiontosalaronservationlaws(2.2)withauxfuntiongivenbyRemark2.2,
aswellassomeresultsaboutexistene,uniqueness,andregularitypropertiesofthesesolutions.
We will end bya lassial relation between these two problems. Theseresults will be needed
throughout this paper, preisereferenes for theproofswillbe mentioned later on.
2.1 Visosity solution: denition and properties
Denition 2.3 ([10℄, Visosity solution: non-stationary ase)
1) A funtion
u ∈ C(Q T ; R )
is a visosity sub-solution ofu t + F (x, t, u x ) = 0
inQ T ,
(2.4)if for every
φ ∈ C 1 (Q T )
, wheneveru − φ
attains a loal maximum at(x 0 , t 0 ) ∈ Q T
, thenφ t (x 0 , t 0 ) + F (x 0 , t 0 , φ x (x 0 , t 0 )) ≤ 0.
2) A funtion
u ∈ C(Q T ; R )
is a visosity super-solution of (2.4) if for everyφ ∈ C 1 (Q T )
,whenever
u − φ
attains a loal minimum at(x 0 , t 0 ) ∈ Q T
, thenφ t (x 0 , t 0 ) + F (x 0 , t 0 , φ x (x 0 , t 0 )) ≥ 0.
3) A funtion
u ∈ C(Q T ; R )
is a visosity solution of (2.4) if it is both a visosity sub- andsuper-solutionof (2.4).
4) A funtion
u ∈ C( ¯ Q T ; R )
is a visosity solution of the initial value problem (2.1) ifu
is avisosity solutionof (2.4) and
u(x, 0) = u 0 (x)
inR
.It is worth mentioning here that if a visosity solution of a Hamilton-Jaobi equation is dif-
ferentiable at a ertain point, then it solves the equation there (see [10 , Corollary I.6℄). An
equivalent denition depending on the sub- and super-dierential of a ontinuous funtion is
now presented. Thisdenition will be usedfor the demonstration of Proposition 2.10. Letus
reall thatthe sub-and the super-dierential of a ontinuous funtion
u ∈ C( R n × (0, T ))
, atapoint
(x, t) ∈ R n × (0, T )
, aredened asthelosed onvex sets:D 1,− u(x, t) = n
(p, α) ∈ R n × R : lim inf
(y,s)→(x,t)
u(y, s) − u(x, t) − (p · (y − x) + α · (s − t))
| y − x | + | s − t | ≥ 0 o ,
and
D 1,+ u(x, t) = n
(p, α) ∈ R n × R : lim sup
(y,s)→(x,t)
u(y, s) − u(x, t) − (p · (y − x) + α · (s − t))
| y − x | + | s − t | ≤ 0 o ,
respetively.
Denition 2.4 (Equivalent denition of visosity solution)
1) Afuntion
u ∈ C( R n × (0, T ))
is a visosity super-solution of (2.1)if andonly if,for every(x, t) ∈ R n × (0, T )
:∀ (p, α) ∈ D 1,− u(x, t), α + F(x, t, p) ≥ 0.
(2.5)2) A funtion
u ∈ C( R n × (0, T ))
is a visosity sub-solution of (2.1) if and only if, for every(x, t) ∈ R n × (0, T )
:∀ (p, α) ∈ D 1,+ u(x, t), α + F(x, t, p) ≤ 0.
(2.6)Thisdenitionismoreloal,foritpermitsveriationthatagivenexpliitfuntionisavisosity
solution in a more lassial way, i.e. using the derivative alulus. A similar denition, that
will be usedlater, ould be given inthe stationaryase. Let
Ω ⊂ R n
be anopen domain,and onsiderthe PDEF(x, u(x), ∇ u(x)) = 0, ∀ x ∈ Ω,
(2.7)where
F : Ω × R × R n 7→ R
isa ontinuousmapping.A ontinuous funtion
u : Ω 7→ R
is a visosity sub-solution of the PDE (2.7) if for any ontinuously dierentiable funtionφ : Ω 7→ R
and any loal maximumx 0 ∈ Ω
ofu − φ
, onehas
F(x 0 , u(x 0 ), ∇ φ(x 0 )) ≤ 0.
Similarly,if at any loal minimum point
x 0 ∈ Ω
ofu − φ
, one hasF(x 0 , u(x 0 ), ∇ φ(x 0 )) ≥ 0,
then
u
isa visositysuper-solution. Finally, ifu
isboth a visosity sub-solution anda visosity super-solution,thenu
isalled a visosity solution.Infat,this denitionisusedforinterpreting solutions of(1.4) inthevisositysense. Further-
more,we saythat
u
isa visositysolution of theDirihlet problem (2.7) withu = ζ ∈ C(∂Ω)
if:
(1)
u ∈ C( ¯ Ω)
,(2)
u
isa visositysolutionof (2.7) inΩ
,(3)
u = ζ
on∂Ω
.For abetter understandingof thevisosityinterpretationofboundaryonditionsof Hamilton-
Jaobi equations,we refer the readerto [2 , Setion 4.2℄.
Now, we will proeedbygiving themain results onerningvisositysolutions of (2.1). In
order to have existeneand uniqueness, the Hamiltonian
F
will be restritedbythefollowingonditions :
( F0 ) F ∈ C( R × [0, T ] × R )
;( F1 )
for eahR > 0
there is a onstantC R
suh that for all(x, t, p)
,(y, t, q) ∈ R × [0, T ] × [ − R, R],
| F (x, t, p) − F (y, t, q) | ≤ C R ( | p − q | + | x − y | );
( F2 )
there isa onstantC F
suh thatfor all(t, p) ∈ [0, T ] × R
and allx, y ∈ R ,
| F (x, t, p) − F (y, t, p) | ≤ C F | x − y | (1 + | p | ).
We usethese onditions towrite downsome results onvisositysolutions.
Theorem 2.6 (Comparison, [9, Theorem 1℄)
Let
F
satisfy( F0 )
-( F1 )
-( F2 )
. Ifu
,u ¯ ∈ U C x ( ¯ Q T )
are two visosity sub- and super-solution of the Hamilton-Jaobiequation (2.1) respetively, withu(x, 0) ≤ u(x, ¯ 0)
inR ,
then
u ≤ u ¯
inQ ¯ T
.Theorem 2.7 (Existene, [9, Theorem 1℄)
Let
F
satisfy( F0 )
-( F1 )
-( F2 )
. Ifu 0 ∈ U C( R )
,then(2.1)hasavisositysolutionu ∈ U C x ( ¯ Q T )
.Remark 2.8 The omparison theorem stated above gives the uniqueness of the visosity so-
lution.
F (x, t, u) = g(x, t)f (u),
the following onditions:
( V0 ) f ∈ C b 1 ( R ; R ), ( V1 ) g ∈ C b ( ¯ Q T ; R ), ( V2 ) g x ∈ L ∞ ( ¯ Q T )
,imply
( F0 )
-( F1 )
-( F2 )
togetherwith the boundedness of the Hamiltonian.The next proposition reets the behavior of visosity solutions under additional regularity
assumptionson
u 0
andF
.Proposition 2.10 (Additional regularity of the visosity solution)
Let
F = gf
satisfy( V0 )
-( V1 )
-( V2 )
. Ifu 0 ∈ Lip( R )
andu ∈ U C x ( ¯ Q T )
isthe unique visositysolutionof (2.1), then
u ∈ Lip( ¯ Q T )
.Proof. Consider the funtion
u ε
dened onR × [0, T ]
by:u ε (x, t) = sup
y∈R
u(y, t) − e kt | x − y | 2 2ε
.
By [20,Theorem 3℄, thefuntion
u
satises,| u(x, t) | ≤ c ∗ ( | x | + 1)
for(x, t) ∈ R × [0, T ],
where
c
andc ∗
are two positive onstants. Therefore,u
is a sublinear funtion for everytime
t ∈ [0, T ]
. The funtionu ε
is dened via a supremum whih is attained beause of thesublinearityofthefuntion
u
(aquadratifuntionalwaysontrolalinearone);thesupremuman be ahievedat several points; let
x ε
beone of them,sowe anwriteu ε (x, t) = u(x ε , t) − e kt | x − x ε | 2
2ε .
We aregoingto prove thatfor
(p, α) ∈ R × R
,we have:(p, α) ∈ D 1,+ u ε (x, t) ⇒
p, α + ke kt | x − x ε | 2 2ε
∈ D 1,+ u(x ε , t).
(2.8)Sine
(p, α) ∈ D 1,+ u ε (x, t)
,thenwe an writefor(y, s) ∼ (x, t)
that,L = u ε (y, s) ≤ u ε (x, t) + α(s − t) + p(y − x) + o( | s − t | + | y − x | ) = R,
(2.9)where theleftside
L
of(2.9) satises,L ≥ u(z, s) − e ks | z − y | 2
2ε , z ∈ R ,
(2.10)and theright side
R
of(2.9) satises,R ≤ u(x ε , t) − e kt | x − x ε | 2
2ε + α(s − t) + p(y − x) + o( | s − t | + | y − x | ).
(2.11)Choose
z
suh thatz − y = x ε − x
,thenz = x ε + (y − x) ∼ x ε ,
siney ∼ x.
(2.12)Combining (2.9),(2.10), (2.11) and(2.12) together, we get
u(x ε + (y − x), s) − e ks | x − x ε | 2
2ε ≤
u(x ε , t) − e kt | x − x ε | 2
2ε + α(s − t) + p(z − x ε ) + o( | s − t | + | z − x ε | ),
and hene,
u(z, s) ≤ u(x ε , t) + (e ks − e kt ) | x − x ε | 2 2ε
+α(s − t) + p(z − x ε ) + o( | s − t | + | z − x ε | ).
(2.13)We have
(e ks − e kt ) | x − x ε | 2
2ε = ke kt | x − x ε | 2
2ε (s − t) + o( | s − t | ),
thenusing inequality(2.13), we get
u(z, s) ≤ u(x ε , t) +
α + ke kt | x − x ε | 2 2ε
(s − t)
+p(z − x ε ) + o( | s − t | + | z − x ε | ),
whih provesthat
α + ke kt | x − x ε | 2 2ε , p
∈ D 1,+ u(x ε , t),
and henestatement (2.8) is true. Sine
u
isavisositysub-solution of(2.1), we haveα + ke kt | x − x ε | 2
2ε + F(x ε , t, p) ≤ 0.
We useondition
( F1 )
withp = q
,to getα + ke kt | x − x ε | 2
2ε + F (x, t, p) ≤ F(x, t, p) − F (x ε , t, p),
≤ C | x − x ε | ,
therefore,
α + F(x, t, p) ≤ C | x − x ε | − ke kt | x − x ε | 2 2ε ,
≤ Cr ε − k r ε 2 2ε ,
≤ sup
r>0
Cr − kr 2 2ε
,
where
r ε = | x − x ε | .
At themaximum¯ r
,wehaveC = k¯ ε r
. Byhoosingk = C 2 2
,we getα + F (x, t, p) ≤ ε.
This inequality shows that
v ε = u ε − εt
is a visosity sub-solution of (2.1) withv ε (x, 0) = u ε (x, 0)
. By the omparison priniple,we havev ε (x, t) − u(x, t) ≤ sup
x∈R
(v ε (x, 0) − u 0 (x)),
≤ sup
x∈R
(u ε (x, 0) − u 0 (x)),
≤ sup
x∈R
sup
y∈R
u 0 (y) − | x − y | 2 2ε
− u 0 (x)
! ,
≤ sup
x,y∈R
γ | x − y | − | x − y | 2 2ε
,
≤ sup
r≥0
γr − r 2 2ε
= γ 2 ε 2 ,
where
γ
is the Lipshitz onstant of the funtionu 0
, andr = | x − y |
. This altogether showsthe following inequalityfor
x, y ∈ R
:u(y, t) − e kt | x − y | 2
2ε ≤ u ε (x, t) ≤ u(x, t) + εt + γ 2 ε
2 .
(2.14)Remarkherethat
k
isa xed; previously hosenonstant. Inequality(2.14) yields:u(y, t) − u(x, t) ≤ e kt | x − y | 2
2ε +
t + γ 2
2
ε = ζ/ε + βε,
(2.15)where
ζ = e kt |x−y| 2 2
andβ =
t + γ 2 2
. We minimizeinequality(2.15) over
ε
to obtain,u(y, t) − u(x, t) ≤ 2 p
ζβ,
≤ e kt 2 √ 2
r t + γ 2
2 | x − y | .
Sinethis inequality holds
∀ x, y ∈ R
,exhangingx
withy
yields,| u(x, t) − u(y, t) | ≤ C(F, u 0 ) | x − y | ∀ x, y ∈ R
andt ∈ [0, T ].
Thisshows thatthefuntion
u
isLipshitz ontinuousinx
,uniformlyintimet
. To prove theLipshitz ontinuity in time, we mainly use the result of [20 , Theorem 3℄) with the fat that
u t = − F (x, t, u x )
,andthe boundedness oftheHamiltonian.2
Remark 2.11 It is worth mentioning that the spae Lipshitz onstant of the funtion
u
de-pendson
C
,whereC
appearsin( F1 )
forp = q
,andonthe Lipshitzonstantγ
ofthefuntionu 0
. While the time Lipshitzonstant depends on the bound of the Hamiltonian.Denition 2.12 (Entropy sub-/super-solution)
Let
F (x, t, v) = g(x, t)f (v)
withg, g x ∈ L ∞ loc (Q T ; R )
andf ∈ C 1 ( R ; R )
. A funtionv ∈ L ∞ (Q T ; R )
is an entropy sub-solution of (2.2) with bounded initial datav 0 ∈ L ∞ ( R )
if itsatises:
Z
Q T
h η i (v(x, t))φ t (x, t) + Φ(v(x, t))g(x, t)φ x (x, t)+
h(v(x, t))g x (x, t)φ(x, t) i dxdt +
Z
R
η i (v 0 (x))φ(x, 0)dx ≥ 0,
(2.16)
∀ φ ∈ C 0 1 ( R × [0, T ); R + )
, for any non-dereasing onvex funtionη i ∈ C 1 ( R ; R )
,Φ ∈ C 1 ( R ; R )
suh that:
Φ ′ = f ′ η i ′ ,
andh = Φ − f η ′ i .
(2.17)Anentropy super-solutionof (2.2)isdened by replaingin(2.16)
η i
withη d
; anon-inreasing onvex funtion. An entropy solution isdened asbeing both entropy sub- and super-solution.In other words, it veries (2.16) for any onvexfuntion
η ∈ C 1 ( R ; R )
.A well knowharaterization of theentropysolution isthat:
Proposition 2.13 A funtion
v ∈ L ∞ (Q T )
is an entropy sub-solution of (2.2) if and onlyif∀ k ∈ R
,φ ∈ C 0 1 ( R × [0, T ); R + )
, onehas:Z
Q T
h (v(x, t) − k) + φ t (x, t) +
sgn+ (v(x, t) − k)(f (v(x, t)) − f (k))g(x, t)φ x (x, t) −
sgn
+ (v(x, t) − k)f (k)g x (x, t)φ(x, t) i dxdt +
Z
R
(v 0 (x) − k) + φ(x, 0)dx ≥ 0,
(2.18)Where
a ± = 1 2 ( | a | ± a)
and sgn± (x) = 1 2 (
sgn(x) ± 1)
. An entropy super-solution of (2.2) is dened replaing in (2.18)( · ) +
,sgn+
by( · ) −
, sgn−
.This haraterization an be dedued from (2.16), by using regularizations of the funtion
( · − k) +
. Also(2.16)maybeobtainedfrom(2.18) byapproximatinganynon-dereasingonvex funtionη i ∈ C 1 ( R ; R )
by a sequene of funtions of the form:η i (n) ( · ) = P n
1 β i (n) ( · − k i (n) ) +
,with
β i (n) ≥ 0
.Entropy solution was rst introdued by Kru
z ˇ
kov [22 ℄ as the only physially admissiblesolution among all weak (distributional) solutions to salar onservation laws. These weak
solutions lak the fat of being unique for it is easy to onstrut multiple weak solutions to
Cauhyproblems (2.2),see [25 ℄.
Ournextdenitiononerns lassialsub-/super-solutionto salaronservationlaws. This
kindof solutions areshown tobe entropy solutions,for thedetails seelemma 3.3.
Denition 2.14 (Classial solutionto salar onservation laws)
Let
F (x, t, v) = g(x, t)f (v)
withg, g x ∈ L ∞ loc (Q T ; R )
andf ∈ C 1 ( R ; R )
. A funtionv ∈ W 1,∞ (Q T )
is said tobe a lassial sub-solution of (2.2)withv 0 (x) = v(x, 0)
if it satisesv t (x, t) + (F (x, t, v(x, t))) x ≤ 0
a.e. inQ T .
(2.19)Classialsuper-solutionsare dened byreplaing
≤
with≥
in(2.19), andlassialsolutionsare dened to be both lassial sub- andsuper-solutions.
Theorem 2.15 (Kru
z ˇ
kov's Existene Theorem)Let
F
,v 0
be given by Denition 2.12, andthe following onditions hold:( E0 ) f ∈ C b 1 ( R ), ( E1 ) g, g x ∈ C b ( ¯ Q T ), ( E2 ) g xx ∈ C( ¯ Q T )
,then there exists an entropy solution
v ∈ L ∞ (Q T )
of (2.2).In fat, Kru
ˇ z
kov'sonditions for existene were given for a general ux funtion [22 , Setion4℄. However, in Subsetion 5.4 of the same paper, a weak version of these onditions, that
an be easily heked in the ase
F (x, t, v) = g(x, t)f (v)
and( E0 )
-( E1 )
-( E2 )
, is presented.Furthermore, uniquenessfollows fromthe following omparison priniple.
Theorem 2.16 (Comparison Priniple)
Let
F
be given by Denition 2.12withf
satisfying(E0), andg
satises,( E3 ) g ∈ W 1,∞ ( ¯ Q T ).
Let
u(x, t)
,v(x, t) ∈ L ∞ (Q T )
be two entropy sub-/super-solutions of (2.2) with initial datau 0
,v 0 ∈ L ∞ ( R )
. Suppose that,u 0 (x) ≤ v 0 (x)
a.e. inR ,
then
u(x, t) ≤ v(x, t)
a.e. inQ ¯ T .
Proof. See Setion 6,Appendix.
2
It is worth notiing that in[22 ℄, theproof of the existene of entropy solutions of (2.2) is
made througha paraboli regularization of (2.2) and passingto the limit,with respet to the
L 1
onvergene onompats, ina onvenient spae.At this stage,we are ready to present a relation thatsometimes hold between salar on-
servationlaws and Hamilton-Jaobiequations inone-dimensional spae.
2.3 Entropy-Visosity relation
Formally, by dierentiating (2.1) with respet to
x
and deningv = u x
, we see that (2.1) isequivalent to thesalaronservation law(2.2)with
v 0 = u 0 x
andthesameF
. Thisequivaleneof the two problems has been exploited in order to translate some numerial methods for
hyperboli onservation laws to methods for Hamilton-Jaobi equations. Moreover, several
proofsweregivenintheonedimensionalase. Theusualproofofthisrelationdependsstrongly
on the known results about existene and uniqueness of the solutions of the two problems
together withthe onvergene of the visosity method (see [8, 23, 27℄). Another proof of this
proof ould alsobe found in[21℄ using the front traking method. The ase ofa Hamiltonian
of the form (2.3) is also treated even when
g(x, t)
is allowed to be disontinuous inthe(x, t)
planealong anite numberof (possiblyinterseted) urves, see[29 ℄.
In our work, the above stated relation will be suessfully used to get some gradient es-
timates of
κ
. Although several approahes were given to establish this onnetion, we willpresent for the reader's onveniene, a proof similar to that given in [8 , Theorem 2.2℄. For
every Hamiltionian/ux funtion
F = gf
andeveryu 0 ∈ Lip( R )
,letEV = { ( V0 ), ( V1 ), ( V2 ), ( E0 ), ( E1 ), ( E2 ), ( E3 ) } ,
inother words,
EV =
The setof allonditions on
f
andg
ensuring theexistene anduniquenessof aLipshitz ontinuousvisosity
solution
u ∈ Lip( ¯ Q T )
of (2.1),and of anentropysolution
v ∈ L ∞ (Q T )
of (2.2),withv 0 = u 0 x ∈ L ∞ ( R )
.Theorem 2.17 (A link between visosity and entropy solutions)
Let
F = gf
withg ∈ C 2 ( ¯ Q T )
,u 0 ∈ Lip( R )
andEV
satised. Then,v = u x
a.e. inQ T .
Sketh of the proof. Let
ε > 0
andδ > 0
. We start the prove by making a paraboliregularization of equation (2.1) and a smooth regularization of
u 0
and we solve the followingparaboli equation:
( u ε,δ t + F (x, t, u ε,δ x ) = ǫu ε,δ xx
inR × (0, T ), u ε,δ (x, 0) = u 0,δ (x)
inR .
(2.20)
For thesakeofsimpliity,wewilldenote
u ε,δ
byw
andu 0,δ
byw 0
. Notethattherstequationof(2.20) an beviewed asthe heatequationwitha soure term
F
. Thus, we have:( w t − εw xx = F[w](x, t)
inQ T ,
w(x, 0) = w 0
inR ,
(2.21)
with
F [w](x, t) = F(x, t, w x (x, t))
. From the lassial theory of heat equations, sineF[w] ∈ L p loc (Q T )
andw 0 ∈ W loc 1,p ( R )
, thereexistsa unique solutionw
of(2.21) suh thatw ∈ W p 2,1 (Ω) ∀ Ω ⊂⊂ Q T
and1 < p < ∞ .
Here the spae
W p 2,1 (Ω)
,p ≥ 1
is the Banah spae onsisting of all funtionsw ∈ L p (Ω)
having generalized derivatives of the form
w t
andw xx
inL p (Ω)
. For more details, see [24,Theorem 9.1℄. We also notie that the spae
W p 2,1 (Ω)
is ontinuously injeted in the Hölder spaeC α,α/2 (Ω)
forα = 2 − 3 p
andp > 3 2
, see [24℄. We use now a bootstrap argument toinreasetheregularityof
w
,takingineahstage,the newregularityofF [w]
andtheregularityof
w 0
. Finally, we get thatw ∈ C 3,1 ( R × [0, T ))
(three times ontinuously dierentiable inL p
-estimatesoftheheatequation,see[24,3℄,itfollowstheuniformboundofu ε,δ
inW loc 1,p (Q T )
,for
p > 2
. Therefore,we getasδ → 0
andε → 0
that:u ε,δ → u
inC( R × [0, T )),
with
u(x, 0) = u 0
. We now make use ofthe stabilitytheorem, [2 , Théorème 2.3℄, twieon theequation(2.20) togetthatthelimit
u
istheuniquevisositysolution of(2.1). Hene, wehavefor any
φ ∈ C 0 ∞ (Q T )
ε→0, δ→0 lim Z T
0
Z
R
u ε,δ x φ dx dt = − lim
ε→0, δ→0
Z T 0
Z
R
u ε,δ φ x dx dt
= −
Z T
0
Z
R
uφ x dx dt = Z T
0
Z
R
u x φ dx dt.
Theappearaneof
u x
followssineu ∈ Lip( ¯ Q T )
. Moreover,asa regularsolution, thefuntionv ε,δ = u ε,δ x
solvesthe derived problem( v ε,δ t + (F (x, t, v ε,δ )) x = ǫv ε,δ xx
inR × (0, T ), v ε,δ (x, 0) = u 0,δ x (x)
inR ,
(2.22)
and,aordingto[22 ,Theorem4℄,thesequene
v ε,δ
onvergeinL loc 1 ( ¯ Q T )
,asε → 0
andδ → 0
,to theentropysolution
v
of(2.2). Then, for anyφ ∈ C 0 ∞ (Q T )
,ε→0 lim δ→0
Z T 0
Z
R
v ε,δ φ dx dt = Z T
0
Z
R
vφ dx dt.
Consequently,
Z T 0
Z
R
u x φ dx dt = Z T
0
Z
R
vφ dx dt,
and
u x = v
a.e. inQ T
.2
Remark 2.18 The onverse ofthe previous theoremholdsunder ertain assumptions(see [21,
7℄).
Remark 2.19 In the multidimensional ase this one-to-one orrespondene no longer exists,
instead the gradient
v = ∇ u
satises formally a non-strit hyperboli system of onservation laws (see [27,23 ℄).Throughout Setions 3 and 4,
ρ
will always be the solution of the heat equation (1.5). Thepropertiesofthesolutionoftheheatequationwithsuharegularinitialdatawillbefrequently
used, we referthe reader to [3,13℄ fordetails.
3 The approximate problem
In this setion, we approximate (1.4) and we pose a more restritive ondition (see ondition
(1.8)) on the gradient of the initial data than of the physialy relevent one (1.6). We prove
thereaderwillnotie at theend ofthissetionthatthis restritiveonditionis satisedforall
time, and this what anels the approximation in the struture of (1.4) and returns it to its
original one. Finaly we present the proof ofTheorem 1.3.
For every
a > 0
, we build up an approximation funtionf a ∈ C b 1 ( R )
of the funtion1 x
dened by:
f a (x) =
1
x
ifx ≥ a,
2a − x
a 2 + a 2 (x − a) 2
otherwise.(3.1)
Proposition 3.1 For any
a > 0
, letf a
be dened by (3.1) andH ∈ C 1 ( R )
be a salar-valued funtion. IfF a (x, t, u) = − H(ρ x (x, t))ρ xx (x, t)f a (u)
(3.2)and
κ 0 ∈ Lip( R )
, then the Hamilton-Jaobi equation( κ t + F a (x, t, κ x ) = 0
inQ T , κ(x, 0) = κ 0 (x)
inR ,
(3.3)
has a unique visosity solution
κ ∈ Lip( ¯ Q T )
.Proof. The proof is easily onluded from Theorems 2.6, 2.7 and Proposition 2.10, after
heking that the onditions
( V0 )
-( V1 )
-( V2 )
aresatised withg(x, t) = − H(ρ x (x, t))ρ xx (x, t).
(3.4)Theondition
( V0 )
istrivial,whilefor( V1 )
,wejustusethefatthatH
isboundedonompatsandthefatthat
| ρ x (x, t) | ≤ || ρ 0 x || L ∞ (R)
inQ ¯ T
. Fortheondition( V2 )
,theregularityofρ
andH
permits toompute thespatial derivative ofg
inQ ¯ T
,thus we have:g x = − (H ′ (ρ x )ρ 2 xx + H(ρ x )ρ xxx ).
Theuniform bound ofthe spatialderivatives,up tothethirdorder, of thesolution oftheheat
equation, and the boundedness of
H ′
onompats givesimmediately( V2 )
.2
Inthefollowingproposition, weshowalower-boundestimateforthegradientof
κ
obtainedin Proposition 3.1. It is worth mentioning that a result of lower-bound gradient estimates
for rst-order Hamilton-Jaobi equations ould be found in[26, Theorem 4.2℄. However, this
resultholdsforHamiltonians
F (x, t, u)
thatareonvexintheu
-variable,usingonlythevisositytheorytehniques. Thisisnottheasehere, andinordertoobtainour lower-bound estimates,
we need to usethe visosity/entropy theorytehniques. Inpartiular,wehave thefollowing:
Proposition 3.2 Let
G ∈ C 3 ( R ; R )
satisfyingthe followingonditions:(G1)
G(x) ≥ G(0) > 0
,(G2)
G ′′ ≥ 0.
H = GG ′
and0 < a ≤ G(0).
If
κ 0
satises:κ 0 x (x) ≥ G(ρ 0 x (x)),
a.e. inR ,
then the solution
κ
obtained fromProposition 3.1satises:κ x (x, t) ≥ G(ρ x (x, t))
a.e. inQ ¯ T .
(3.5)Inorder to proveProposition 3.2, we rstshow that
G(ρ x )
is anentropysub-solution of( ω t + (F (x, t, ω)) x = 0
inQ T , ω(x, 0) = ω 0 (x)
inR ,
(3.6)
with
w 0 = G(ρ 0 x )
andF
isthe sameasin(3.2). Before going further,we willpause to prove alemmawhih makesiteasierto reahour goal.
Lemma 3.3 (Classial sub-solutions are entropy sub-solutions)
Let
v ∈ W 1,∞ (Q T )
bea lassial sub-solutionof(2.2)withv 0 (x) = v(x, 0)
,thenv
isan entropysub-solution.
Proof. Let
η i
,Φ
,h
andφ
begiven byDenition2.12. Multiplyinginequality(2.19) byη i ′ (v)φ
doesnot hange its sign. Hene, afterdeveloping, we have:
η i ′ (v)v t φ + η ′ i (v)g x f (v)φ + η ′ i (v)gf ′ (v)v x φ ≤ 0,
a.e. inQ T ,
(3.7)andsine
v
isLipshitzontinuous,weusethehain-ruleformulatogetherwith(2.17)torewrite(3.7) as:
(η i (v)) t φ + g x f (v)η i ′ (v)φ + g(Φ(v)) x φ ≤ 0,
a.e. inQ T .
(3.8)Uponintegrating(3.8) over
Q T
and transferringderivativeswithrespettot
andx
tothetestfuntion,we obtain:
Z
Q T
h
η i (v(x, t))φ t (x, t) + Φ(v(x, t))g(x, t)φ x (x, t)+
h(v(x, t))g x (x, t)φ(x, t) i dxdt +
Z
R
η i (v 0 (x))φ(x, 0)dx ≥ 0,
(3.9)whih endsthe proof.
2
Following same arguments, lassialsuper-solutions are shownto entropysuper-solutions. We
return now to the funtion
G(ρ x )
and we areready to show thatit is indeed an entropysub-solutionof (3.6). In partiular,we have thefollowing:
Lemma 3.4 The funtion
G(ρ x )
dened onQ T
isa lassial sub-solution of (3.6)with initial dataG(ρ 0 x )
, hene an entropy sub-solution.Proof of Lemma 3.4. First, it is easily seen that
G(ρ x ) ∈ W 1,∞ (Q T )
. Dene the salarvaluedquantity
B
onQ T
by:B (x, t) = ∂ t (G(ρ x (x, t))) + ∂ x (F (x, t, G(ρ x (x, t)))).
Sine
0 < a ≤ G(0)
, we use(G1) to getf a (G(ρ x )) = 1/G(ρ x )
and we observe that,B = G ′ (ρ x )ρ xt − ∂ x
H(ρ x )ρ xx G(ρ x )
= G ′ (ρ x )ρ xxx − G(ρ x )[H ′ (ρ x )ρ 2 xx + H(ρ x )ρ xxx ] − (G ′ (ρ x )ρ 2 xx H(ρ x )) G 2 (ρ x )
!
= G(ρ x )ρ xxx (G(ρ x )G ′ (ρ x ) − H(ρ x )) − ρ 2 xx (H ′ (ρ x )G(ρ x ) − H(ρ x )G ′ (ρ x )) G 2 (ρ x )
= − ρ 2 xx G ′′ (ρ x ).
The ondition (G2) gives immediately that
B ≤ 0
. This proves thatG(ρ x )
is a lassial sub-solutionof equation(3.6) and henean entropysub-solution.
2
Proof of Proposition 3.2. From the denition of
H
and the properties ofρ
, it is easy tohek that
g ∈ C 2 ( ¯ Q T )
and thatEV
is fully satised. Hene, we are in the framework ofTheorem2.17with
u 0 = κ 0
. Thistheoremgivesthatκ x
istheunique entropysolutionof(3.6)with
w 0 = κ 0 x
. Moreover, by the previous lemma,G(ρ x )
is an entropy sub-solution of (3.6).Sine
κ 0 x ≥ G(ρ 0 x ),
a.e. inR ,
we an applythe Comparison Theorem 2.16to getthedesiredresult.
2
It is worth notable here that we do not know how to obtain the lower-bound on the spatial
gradient
κ x
using thevisosity framework diretly. However, for thease ofthe upper-bound, we an doso(see Remark4.1). Atthis stage,xsomeǫ > 0
,and letG ǫ (x) = p
x 2 + ǫ 2
anda = G ǫ (0) = ǫ.
It islear that
G ǫ (x)
satisestheonditions (G1)-(G2) withH ǫ (x) = x,
and theHamiltonian
F
from (3.2) takesnowthefollowing shape:F ǫ (x, t, u) = − ρ x (x, t)ρ xx (x, t)f ǫ (u).
(3.10)Moreover,wehavethefollowingorollarywhihisisanimmediateonsequeneofPropositions
3.1and 3.2.
Corollary 3.5 There existsa unique visosity solution
κ ∈ Lip( ¯ Q T )
of( κ t + F ǫ (x, t, κ x ) = 0
inQ T ,
κ(x, 0) = κ 0 ∈ Lip( R )
inR ,
(3.11)