Isentropic relations: Difference between revisions

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=== First law of thermodynamics ===
=== First law of thermodynamics ===


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{{NumEqn|<math>
{{NumEqn|<math>
de=Tds-pd\left(\frac{1}{\rho}\right)
de=Tds-pd\left(\frac{1}{\rho}\right)
</math>|eq-first-law-b}}
</math>|label=eq-first-law-b}}


Enthalpy is defined as: <math>h=e+p/\rho</math> and thus
Enthalpy is defined as: <math>h=e+p/\rho</math> and thus
Line 23: Line 31:
{{NumEqn|<math>
{{NumEqn|<math>
dh=de+pd\left(\frac{1}{\rho}\right)+\left(\frac{1}{\rho}\right)dp
dh=de+pd\left(\frac{1}{\rho}\right)+\left(\frac{1}{\rho}\right)dp
</math>|eq-dh}}
</math>|label=eq-dh}}


Eliminate <math>de</math> in {{EquationNote|eq-first-law-b}} using {{EquationNote|eq-dh}}
Eliminate <math>de</math> in {{EquationNote|label=eq-first-law-b}} using {{EquationNote|label=eq-dh}}


{{NumEqn|<math>
{{NumEqn|<math>
Line 39: Line 47:
{{NumEqn|<math>
{{NumEqn|<math>
ds=C_p\frac{dT}{T}-R\frac{dp}{p}
ds=C_p\frac{dT}{T}-R\frac{dp}{p}
</math>}}
</math>|label=eq-ds}}


Integrating Eqn. \ref{eq:ds} gives
Integrating {{EquationNote|eq-ds}} gives


{{NumEqn|<math>
{{NumEqn|<math>
s_2-s_1=\int_1^2 C_p\frac{dT}{T}-R\ln\left(\frac{p_2}{p_1}\right)
s_2-s_1=\int_1^2 C_p\frac{dT}{T}-R\ln\left(\frac{p_2}{p_1}\right)
</math>}}
</math>|label=eq-ds-b}}


For a calorically perfect gas, <math>C_p</math> is constant (not a function of temperature) and can be moved out from the integral and thus
For a calorically perfect gas, <math>C_p</math> is constant (not a function of temperature) and can be moved out from the integral and thus
Line 51: Line 59:
{{NumEqn|<math>
{{NumEqn|<math>
s_2-s_1=C_p\ln\left(\frac{T_2}{T_1}\right)-R\ln\left(\frac{p_2}{p_1}\right)
s_2-s_1=C_p\ln\left(\frac{T_2}{T_1}\right)-R\ln\left(\frac{p_2}{p_1}\right)
</math>}}
</math>|label=eq-ds-c}}


An alternative form of Eqn. \ref{eq:ds:c} is obtained by using <math>de=C_v dT</math> Eqn. \ref{eq:firstlaw:b}, which gives
An alternative form of {{EquationNote|label=eq-ds-c}} is obtained by using <math>de=C_v dT</math> in {{EquationNote|label=eq-first-law-b}}, which gives


{{NumEqn|<math>
{{NumEqn|<math>
s_2-s_1=\int_1^2 C_v\frac{dT}{T}-R\ln\left(\frac{\rho_2}{\rho_1}\right)
s_2-s_1=\int_1^2 C_v\frac{dT}{T}-R\ln\left(\frac{\rho_2}{\rho_1}\right)
</math>}}
</math>|label=eq-ds-d}}


Again, for a calorically perfect gas, we get
Again, for a calorically perfect gas, we get
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{{NumEqn|<math>
{{NumEqn|<math>
s_2-s_1=C_v\ln\left(\frac{T_2}{T_1}\right)-R\ln\left(\frac{\rho_2}{\rho_1}\right)
s_2-s_1=C_v\ln\left(\frac{T_2}{T_1}\right)-R\ln\left(\frac{\rho_2}{\rho_1}\right)
</math>}}
</math>|label=eq-ds-e}}


=== Isentropic Relations ===
=== Isentropic Relations ===


Adiabatic and reversible processes, i.e., isentropic processes implies <math>ds=0</math> and thus Eqn. \ref{eq:ds:c} reduces to
Adiabatic and reversible processes, i.e., isentropic processes implies <math>ds=0</math> and thus {{EquationNote|label=eq-ds-c}} reduces to


<math display="block">
{{NumEqn|<math>
\frac{C_p}{R}\ln\left(\frac{T_2}{T_1}\right)=\ln\left(\frac{p_2}{p_1}\right)
\frac{C_p}{R}\ln\left(\frac{T_2}{T_1}\right)=\ln\left(\frac{p_2}{p_1}\right)
</math>
</math>}}


<math display="block">
<math display="block">
Line 81: Line 89:
</math>
</math>


<math display="block">
{{NumEqn|<math>
\frac{p_2}{p_1}=\left(\frac{T_2}{T_1}\right)^{\gamma/(\gamma-1)}
\frac{p_2}{p_1}=\left(\frac{T_2}{T_1}\right)^{\gamma/(\gamma-1)}
</math>
</math>|label=eq-isentropic-a}}


In the same way, Eqn. \ref{eq:ds:e} gives
In the same way, {{EquationNote|label=eq-ds-e}} gives


<math display="block">
{{NumEqn|<math>
\frac{\rho_2}{\rho_1}=\left(\frac{T_2}{T_1}\right)^{1/(\gamma-1)}
\frac{\rho_2}{\rho_1}=\left(\frac{T_2}{T_1}\right)^{1/(\gamma-1)}
</math>
</math>|label=eq-isentropic-b}}
 


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


<math display="block">
{{NumEqn|<math>
\frac{p_2}{p_1}=\left(\frac{\rho_2}{\rho_1}\right)^{\gamma}=\left(\frac{T_2}{T_1}\right)^{\gamma/(\gamma-1)}
\frac{p_2}{p_1}=\left(\frac{\rho_2}{\rho_1}\right)^{\gamma}=\left(\frac{T_2}{T_1}\right)^{\gamma/(\gamma-1)}
</math>
</math>}}

Latest revision as of 10:24, 1 April 2026

First law of thermodynamics

First law of thermodynamics:

de=δqδw(Eq. 1.10)

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

de=Tdspd(1ρ)(Eq. 1.11)

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

dh=de+pd(1ρ)+(1ρ)dp(Eq. 1.12)

Eliminate de in (Eq. 1.11) using (Eq. 1.12)

Tds=dhpd(1ρ)(1ρ)dp+pd(1ρ)(Eq. 1.13)
ds=dhTdpρT(Eq. 1.14)

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

ds=CpdTTRdpp(Eq. 1.15)

Integrating (Eq. 1.15) gives

s2s1=12CpdTTRln(p2p1)(Eq. 1.16)

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

s2s1=Cpln(T2T1)Rln(p2p1)(Eq. 1.17)

An alternative form of (Eq. 1.17) is obtained by using de=CvdT in (Eq. 1.11), which gives

s2s1=12CvdTTRln(ρ2ρ1)(Eq. 1.18)

Again, for a calorically perfect gas, we get

s2s1=Cvln(T2T1)Rln(ρ2ρ1)(Eq. 1.19)

Isentropic Relations

Adiabatic and reversible processes, i.e., isentropic processes implies ds=0 and thus (Eq. 1.17) reduces to

CpRln(T2T1)=ln(p2p1)(Eq. 1.20)

CpR=γγ1

γγ1ln(T2T1)=ln(p2p1)

p2p1=(T2T1)γ/(γ1)(Eq. 1.21)

In the same way, (Eq. 1.19) gives

ρ2ρ1=(T2T1)1/(γ1)(Eq. 1.22)


Eqn. (Eq. 1.21) and Eqn. (Eq. 1.22) constitutes the isentropic relations

p2p1=(ρ2ρ1)γ=(T2T1)γ/(γ1)(Eq. 1.23)