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time interval t is simply R b
a
tf dx. We now have the following mathematical
expression for our basic energy balance:
t.q.a; t/ q.b; t// C Z b
a
tf dx D Z b
a
% @e
@t t dx :
(7.21)
The mathematical similarity with the mass conservation equation (7.14) is striking;
only a factor % differs due to a slightly different definition of q. Using integration by
parts “backward” on the left-hand side transforms this difference to an integral over
Œa; b:
Z b
a
@x dx C Z b
a
tf dx D Z b
a
@q
% @e
@t t dx :
Collecting the integrals yields
% @e
@x f dx D 0:
Z b
@t C @q
a
For this equation to hold for an arbitrary interval Œa; b, the integrand must vanish, a
requirement that leads to the PDE
% @e
@t C @q
@x f D 0:
(7.22)
We have two unknown functions, e.x; t/ and q.x; t/, and thus we need an addi-
tional equation. Observe also that the temperature , which is the quantity we want to
compute, does not yet enter our model. However, we will relate both e and q to the
temperature T .
In thermodynamics there is a class of relations called equations of state .One
such relation reads e D e.T; V /, relating internal energy e to temperature T and
density % D 1=V (V is referred to as volume). By the chain rule, we have
ˇ ˇ ˇ ˇ V
ˇ ˇ ˇ ˇ T
@e
@t D @e
@T
@t C @e
@V
@t
:
@T
@V
The first coefficient .@e=@T / V
is called the specific heat capacity at constant
volume , denoted by c v ,
ˇ ˇ ˇ ˇ V
c v @e
@T
:
The heat capacity will in general vary with T and V ( D 1=%), but taking it as a
constant is reasonable in many applications. We will do so here. One can find tables
in the literature with the constant values of c v for many substances.
The other term, .@e=@V / T , can, by the second law of thermodynamics, be shown
to be proportional to the derivative of T with respect to V (or %). The term models
temperature effects due to compressibility and volume expansion. These effects are
often small and can be neglected. We will therefore set .@e=@V / T D 0.
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