A NNALES DE L ’I. H. P., SECTION A
S EBASTIANO G IAMBÒ
Incompressible heat-conducting relativistic fluid
Annales de l’I. H. P., section A, tome 31, n
o1 (1979), p. 73-76
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73
Incompressible heat-conducting
relativistic fluid (*)
Sebastiano
GIAMBÒ
Istituto di Matematica dell’Università, Universita di Messina, 98100 Messina, Italia
Vol. XXXI, n° 1, 1979. Physique théorique.
ABSTRACT. - We consider a
heat-conducting
relativistic fluid in thecase extreme in which the
incompressibility
conditions hold. We deducesome
important
consequences after we have written the fieldequations
ina
simple particular
formby introducing
two four-vectors which determine thecomplete
field.1. INTRODUCTION
Let us consider a
perfect heat-conducting
relativistic fluid.By
follo-wing [1 ],
the fieldequations
can be written :where is the energy tensor, r the proper material
density (number
ofparticles),
p the pressure,f
the index of thefluid,
p the proper energydensity :
p = T and S are the proper temperature of the fluid and its properspecific
entropy, ga~ is the metric tensor(with signature
+, 2014,(*) This work was supported by the G. N. F. M. of C. N. R. (Italy).
Annales de l’Institut Henri Poincaré-Section A-Vol. XXXI, 0020-2339/1979/l/:)t4,00/
CGauthier-Villars
74 S. GIAMBO
-, -), ~
theunitary four-velocity :
=1,
q" the heat flux vector.Together
with theequations (1)
we consider thefollowing
heatequation [2] ]
which
automatically implies
= 0.At first we observe
that, differently
from the Boillat’s results[3] ] (on
account of the different scheme
used),
the system(1)-(2)
remainshyperbolic
also when the characteristic velocities
21 and 03BB2
areequal.
In fact if
21
==~2,
we have[2] ]
and in
general
we findAll the discontinuities are determined in terms of 5~ and 5T which are
completely
free. It follows that the waveis double.
Here U =
u03B103C603B1,
G =g03B103B203C603B103C603B2, 03C603B1
=~03C6 ~x03B1, 03C6(x03B1) bein g the solutions of
the wave equation.
2 INCOMPRESSIBLE FLUID
[4]
For an
incompressible fluid 03BB21 = 03BB22
= 1 andequation (3) gives
which, taking
account ofequations (1), permits
to write the heatequation
as :while the stream lines system becomes
The
equation (7), by
virtue ofequation (8),
can be rewritten asAnnales de l’Institut Henri Poincaré-Section A
Finally
thecontinuity equation
may be written
3 . THE TWO FIELD FOUR-VECTORS v03B1 AND w03B1 At this stage let us introduce the two four vectors
It is
immediately
seen that all the field variables are known in terms ofV and w". In fact we have :After
this,
if we putthe field
equations
for anincompressible
fluid may besimply
written as4. DISCONTINUITIES
The discontinuities are
immediately
evaluable.By setting
the
equations ( 15) gives :
Vol. XXXI, n° 1-1979.
76 S. GIAMBO
By contracting
theequations (172)
and(174)
with andtaking
intoaccount
equation (173),
we haveIf G ~
0,
fromequation (19)
we find0,
so thatequation (174) gives
We have two
possibilities
and
In the case
(b),
fromequations (17) and (18)
we conclude that~w~ == ~v~
= 0and we have not discontinuities.
This
excluded,
the(a)
holds and fromequations (17)-(19)
we deduce thefollowing
fourindependent equations
for theeight
components ofbv~
and
There are four
degree
offreedom,
so that the wave V == 0(which
corres-ponds
to the material waves ~ =0)
hasmultiplicity
four.Finally
whenG ==
0,
we havewhere k and h are
arbitrary parameters and,
ofcourse, 5 Vex
can begiven
in terms of and
ACKNOWLEDGMENTS
The author is
grateful
to Prof. A. Lichnerowicz for this comments onan earlier version of this paper.
REFERENCES
[1] A. GRECO and S. GIAMBO, Rend. Ac. Naz. Lincei, t. 60, 1976, p. 815.
[2] S. GIAMBÒ, Ann. Inst. H. Poincaré, 27 A, 1977, p. 185.
[2] S. GIAMBÒ, Ann. Inst. H. Poincaré, 27 A, 1977, p. 185; S. GIAMBÒ, C. R. Acad.
Sc. Paris, 284 A, 1977, p. 93.
[3] G. BOILLAT, Lett. Nuovo Cimento, t. 10, 1974, p. 352.
[4] A. LICHNEROWICZ, Relativistic Hydrodynamics and Magnetohydrodynamics, Benia-
min Inc., New York, Amsterdam, 1967.
(Manuscrit reçu le 21 1979)
Annales de l’Institut Henri Poincare-Section A