Isentropic relations: Difference between revisions

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<td style="float: center; border: 1px solid blue"><math>de=\delta q - \delta w</math></td>
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<td style="float: right; border: 1px solid blue">(Eq. 1)</td>
<td style="width: 5em; padding-right: 0.5em; text-align: right; vertical-align:middle; border: 1px solid blue">(Eq. 1)</td>
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Revision as of 07:54, 27 March 2026


First law of thermodynamics

First law of thermodynamics:

de=δq−δw (Eq. 1)
de=δq−δw
(Eq. 1)

de=δq−δw

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

de=Tds−pd(1ρ)

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

dh=de+pd(1ρ)+(1ρ)dp

Eliminate $de$ in Eqn. \ref{eq:firstlaw:b} using Eqn. \ref{eq:dh}

Tds=dh−pd(1ρ)−(1ρ)dp+pd(1ρ)

ds=dhT−dpρT

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

ds=CpdTT−Rdpp

Integrating Eqn. \ref{eq:ds} gives

s2−s1=∫12CpdTT−Rln⁡(p2p1)

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)

An alternative form of Eqn. \ref{eq:ds:c} is obtained by using de=CvdT Eqn. \ref{eq:firstlaw:b}, which gives

s2−s1=∫12CvdTT−Rln⁡(ρ2ρ1)

Again, for a calorically perfect gas, we get

s2−s1=Cvln⁡(T2T1)−Rln⁡(ρ2ρ1)

Isentropic Relations

Adiabatic and reversible processes, i.e., isentropic processes implies ds=0 and thus Eqn. \ref{eq:ds:c} reduces to

CpRln⁡(T2T1)=ln⁡(p2p1)

CpR=γγ−1

γγ−1ln⁡(T2T1)=ln⁡(p2p1)⇒

p2p1=(T2T1)γ/(γ−1)

In the same way, Eqn. \ref{eq:ds:e} gives

ρ2ρ1=(T2T1)1/(γ−1)

Eqn. \ref{eq:isentropic:a} and Eqn. \ref{eq:isentropic:b} constitutes the isentropic relations

p2p1=(ρ2ρ1)γ=(T2T1)γ/(γ−1)