COLLOQU IUM MATHEMAT I CUM VOL NO
11 pages
English

Découvre YouScribe en t'inscrivant gratuitement

Je m'inscris

COLLOQU IUM MATHEMAT I CUM VOL NO

Découvre YouScribe en t'inscrivant gratuitement

Je m'inscris
Obtenez un accès à la bibliothèque pour le consulter en ligne
En savoir plus
11 pages
English
Obtenez un accès à la bibliothèque pour le consulter en ligne
En savoir plus

Description

COLLOQU IUM MATHEMAT I CUM VOL. 106 2006 NO. 2 GLOBAL EXISTENCE VERSUS BLOW UP FOR SOME MODELS OF INTERACTING PARTICLES BY PIOTR BILER (Wro ªaw) and LORENZO BRANDOLESE (Lyon) Abstra t. We study the global existen e and spa e-time asymptoti s of solutions for a lass of nonlo al paraboli semilinear equations. Our models in lude the Nernst Plan k and DebyeHü kel drift-diusion systems as well as paraboli -ellipti systems of hemotaxis. In the ase of a model of self-gravitating parti les, we also give a result on the nite time blow up of solutions with lo alized and os illating omplex-valued initial data, using a method due to S. Montgomery-Smith. 1. Introdu tion. In this paper we are on erned with semilinear paraboli systems of the form (1) ∂tuj = ∆uj + ? · ( m∑ h,k=1 cj,h,k uh(?Ed ? uk) ) , j = 1, . . . ,m, u(0)(x) = u0(x). Here the unknown is the ve tor eld u = (u1, . . . , um), dened on the whole spa e Rd (with m ≥ 1 and d ≥ 2), and cj,h,k ? L∞(Rd), j, h, k = 1, .

  • self gravitating

  • i1 ?

  • unique solution

  • global existence versus blow up

  • paraboli systems

  • valued

  • similar de ay proles


Sujets

Informations

Publié par
Nombre de lectures 10
Langue English

Extrait

COLLOQUIUM MATHEMATICUM
m X
∂ u =Δu +∇· c u (∇E ∗u ) , j = 1,...,m,t j j j,h,k h d k
(1)
h,k=1
u(0)(x) =u (x).0
u = (u ,...,u )1 m
d ∞ dR m≥ 1 d≥ 2 c ∈ L (R ) j,h,k = 1,...,mj,h,k
Ed
dR
m = 1 d≥ 2
∂ u =Δu+∇·(u∇ϕ), Δϕ =u.t
u = u(x,t) ϕ
u
cj,h,k
1 u≥ 0
also
as
the
systems
hemotaxis
drift-diusion
In
el
and
k
for

the
y
is
Deb
In
and
solutions
k


parab
Nernst
as
the
are

the
dels
tial
mo
(see
Our
d
equations.
not
semilinear
(mo
olic

parab
is

in
nonlo
of
of
equations


a
parab
for
pap
solutions
1.
of
the
asymptotics
gra
space-time
to
and
theory
existence
[7
global

the
data,
study
.
e
particles,
W
theories,

of
on)
and
(Ly

BRANDOLESE
for
LORENZO
mo
and
vitating
w)


,
ro
,
(W
v
BILER
usually
PIOTR
In
Here
a
the
systems
unkno
with
wn
w
is
Here
the
tro
v
Mon
ector
y
eld
and
BY
self-consisten
TICLES
p
AR
b
P
Related
CTING
ear
INTERA

OF
[8
MODELS
[3
SOME

OR
ts
F
a
UP

W
to
,
e
dened
that
on
olic
the
in
whole
biology
space
delling
BLO

VERSUS
phenomena)
(with
statisti-
EXISTENCE

GLOBAL
The
2
example
and
us
NO.
the
2006
del
106
gra

particles:
and
this

as
and


systems
lo

with
and
solutions
go
of
erning
up
are
OL.
written
w
hemotaxis.
blo
the
V
of
time
form
,
of
nite
olic
the
semilinear
on

result
e
a
er
e
(2)
giv
this
also

e
In
w
tgomery-Smith.
particles,
is
vitating
densit
self-gra
of
,
particles
are
S.
giv
the
en
t

vitational

oten
ts.
generated
Moreo
y
v
.
er,
systems
ell
app
w
in
the
our
of
,
hemotaxis
h
e.g.
ho

ev

relev

t
this
ph
the
applications;

e
due
en
metho
alued
using
Mathematics
are

t
ation
equal
35K60,
initial
82C21.
W
wor
do
and
require
ases
alued
in
of
in
del
study
denotes
whic
the
is,
fundamen
w
tal
er,
solution
an
of
in
the
ysical
Laplacian
w
in
ev

admit

mo
2000
time,
Subje
wing
Classic
solutions.
:
the
35B40,
form
Key
(1)
ds
arise
phr
e.g.
:
from

plasma,
parab

systems,
and
global
elec-
trolytes
blo
.
up
Systems
of
),294
∂ u =Δu−∇·(u∇ϕ).t
∂ v =Δv−∇·(v∇φ),t
∂ w =Δw +∇·(w∇φ),t
Δφ =v−w.
v w
d = 1
d≥ 2
d≥ 2
−2∼|x|
d≥ 3 η> 0
η
|u (x)|≤ ,0 2(1+|x|)
C ≥ 0 u
dx∈R t≥ 0
C C
|u(x,t)|≤ |u(x,t)|≤ .
2(1+|x|) 1+t
dc (x) Rj,h,k
to

(2)
of
the
real-v
).
alued
existence
solu-
then
tions
e
of
value
these
result
mo

dels;
Nernst
see
,
e.g.
and
[6
for

that
[4
blo

small
[2
y


[1
precise,

k,
and
system
the
a
references
and
therein.
system,
F
solutions.
or
o

particular
if
e
.
(in
ely

ectiv

,
global
then
.
the
us
mo
in
dels
ell

as
ha
more
v
1.1
e
Ther
global
if
in
theory
time
,
solutions.
to
If
of
resp
del,
particles,
,
harged
the
,
the
the
t
Deb
BILER
y
al
e
out
system
few
(3)
of
and
particular,
the
sho
more
nonp
general

system
)
(4)
solutions
ha
up.
v
ose
e
e
global
result
in
of
time
h
solutions
pro
and
some
their
of
asymptotics
The
is
for
describ

ed
e
b
ws
y
for
suitable
and
self-similar
t).
solutions
L
(see
represen
[5
exists


and
M.
[11
y

In
These
the
ma

y
e
b
b
e
solution
in

terpreted
al
as
general
a
(3)

replaced
diusion
equation
of
whic

y
harges
b
to
is
innit
imp
y
L.
due
P
to
,
repulsiv
the
e
lot
in
wn

a
On
other
the

other
(1)
hand,
In
mo
w
dels
will
describing
w
either
also

ositive
hemotaxis

or
omplex-
gra
d
vitational
and
in
lating


in
w

Our
ely
purp
negativ
is
dimensions
giv
feature
a

existence
tration
for
phenomena
solutions
whic
(1)
h

ma
a
y
will
ev
vide
en
with
tually

lead
proles
to
solutions
a
space-time.

global
of
result
solutions.
w
and
lo
or
solutions
gene
b
of
stated
gr
follo
e
(see
o
2
then
a
smal
general,
assumption
more

statemen
b
Theorem
r
.
e
et
by
t
e
.
w
e
eak
and


v
that
ergence
(5)
either
and
to
W.

b
p
the
oin
(4)
t
drift-diusion
masses
is
or
(1)
to
the
un
ther
b
exists
ounded
elonging
functions
and
ely
unique
ositiv
still
p
(1)
of
that
y
for
densit
l
.
mo
One
more
purp
A
ose
with
in
(6)
this
is
pap
of
er
rst
is
h
to
in
sho
e
w
Deb
that
y
a
vided
dieren
pro
t
example
kind
ortan
of
Another
nite
BRANDOLESE
time
AND
blo
.
w
Mor
up
over

if
o
l


is

and
the
A
ab
onstant
existence
kno
e
for
ar
solutions

of
in
(2)
(and
These
homo
phenomena
ous
manifest
de
them-
e
selv
zer
es
,
b
the
y
lness
the
(5)
formation
an
of
e
singularities

of
d
solutions
the
lik295
2esssup|x| |u (x)|≤η.0
dx∈R
t → ∞ x → ∞
d/2 d
−2ue(x,t) = 2(d−2)|x|
d≥ 3
du ∈S (R )0 0
∗u t > 0
s,q∗ d˙u(t ) ∈B (R ) s∈R 1≤p,q≤∞p
k·k s,q˙ dB (R )p
pku(t)kL
1≤p≤∞
ub
u
u
C
dR
∇Ed
C
|∇E (x)|≤ .d d−1|x|
∇E K Kd
dR
−d−1+α|K(x)|≤C|x| , 1<α<d.
tgomery-Smith
Chandrasekhar
estimates
wn
h
kno
(8)
ell-
one
w
to
the
for
of
also
y
since

yields
the
ts
also
existence
is
o.
It
k

we
e.g.

(see
of
solutions
p
self-similar
real
,
real
whic
In
h
ev
is
instead
a
of
stationary
.
solution

of
e
(2)
a
for
ondition
of
the
rate
e
y
an
.
explo
W
in
e

  • Univers Univers
  • Ebooks Ebooks
  • Livres audio Livres audio
  • Presse Presse
  • Podcasts Podcasts
  • BD BD
  • Documents Documents