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CHAPTER 4. THERMODYNAMICS: THE FIRST LAW

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4-18<br />

Since H is a state function<br />

H(T ) 2<br />

aA + bB ! cC T 2<br />

H 9 H 9 8 H<br />

1 2 3<br />

aA + bB ! cC T 1<br />

H(T ) 1<br />

H(T ) = H + H + H(T ) + H .<br />

2 1 2 1 3<br />

For a reaction at constant pressure, the<br />

substance may be calculated from the relation<br />

H associated with changing the temperature of each<br />

T 2<br />

H ' n C P<br />

dT.<br />

T 1<br />

Therefore, T 1<br />

T 1<br />

T 2<br />

H(T 2) = H(T 1) + a C P<br />

(A)dT % b C P<br />

(B)dT % c C P<br />

(C)dT.<br />

T 2<br />

T 2<br />

T 1<br />

Over a restricted range of temperatures, the heat capacities may be treated as constants, in which case<br />

the above formula reduces to<br />

where<br />

H(T ) = H(T ) + C (T ! T ),<br />

2 1 P 2 1<br />

C j C P (i)<br />

P = cC P(C) ! aC P(A) ! bC P(B) = .<br />

iνi<br />

I. Work of adiabatic expansion<br />

The work associated with the expansion of a gas is given by<br />

V 2<br />

w ' !<br />

V 1<br />

P ex<br />

dV<br />

,<br />

and for the isothermal expansion of an ideal gas, we found<br />

a). w = !P V<br />

ex<br />

when P = constant<br />

ex

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