Isentropic relations

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First law of thermodynamics

First law of thermodynamics:

de=δq−δw(Eq. 1.6)

For a reversible process: δw=pd(1/ρ) and δq=Tds

de=Tds−pd(1ρ)(Eq. 1.7)

Enthalpy is defined as: h=e+p/ρ and thus

dh=de+pd(1ρ)+(1ρ)dp(Eq. 1.8)

Eliminate de in (Eq. 1.7) using (Eq. 1.8)

Tds=dh−pd(1ρ)−(1ρ)dp+pd(1ρ)(Eq. 1.9)
ds=dhT−dpρT(Eq. 1.10)

Using dh=CpT and the equation of state p=ρRT, we get

ds=CpdTT−Rdpp(Eq. 1.11)

Integrating (Eq. 1.11) gives

s2−s1=∫12CpdTT−Rln⁡(p2p1)(Eq. 1.12)

For a calorically perfect gas, Cp is constant (not a function of temperature) and can be moved out from the integral and thus

s2−s1=Cpln⁡(T2T1)−Rln⁡(p2p1)(Eq. 1.13)

An alternative form of (Eq. 1.13) is obtained by using de=CvdT in (Eq. 1.7), which gives

s2−s1=∫12CvdTT−Rln⁡(ρ2ρ1)(Eq. 1.14)

Again, for a calorically perfect gas, we get

s2−s1=Cvln⁡(T2T1)−Rln⁡(ρ2ρ1)(Eq. 1.15)

Isentropic Relations

Adiabatic and reversible processes, i.e., isentropic processes implies ds=0 and thus (Eq. 1.13) reduces to

CpRln⁡(T2T1)=ln⁡(p2p1)(Eq. 1.16)

CpR=γγ−1

γγ−1ln⁡(T2T1)=ln⁡(p2p1)⇒

p2p1=(T2T1)γ/(γ−1)(Eq. 1.17)

In the same way, (Eq. 1.15) gives

ρ2ρ1=(T2T1)1/(γ−1)(Eq. 1.18)


Eqn. (Eq. 1.17) and Eqn. (Eq. 1.18) constitutes the isentropic relations

p2p1=(ρ2ρ1)γ=(T2T1)γ/(γ−1)(Eq. 1.19)