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Daniel D'Orazio edited untitled.tex
over 9 years ago
Commit id: 82be4b53a60179aecdc76457e4c1b66ed98ecac7
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For an ideal gas
\begin{align}
d\epsilon &= \frac{R}{\gamma -1}dT \\
PdV &= -\left(\gamma -1\right)\epsilon \frac{d \rho}{\rho} = RT
\frac{d \rho}{\rho}
\end{align}
Then
\begin{equation}
dQ = \frac{R}{\gamma -1}dT - RT \frac{d \rho}{\rho}
\end{equation}
Let's also introduce the enthalpy $h$ in the limit that the number of particles in the system is constant,
\begin{equation}
dh = TdS + VdP = TdS + \frac{dP}{\rho}
\end{equation}
and also the Gibbs free energy $G$ in the same paticle conserving limit
\begin{equation}
dG = SdT + \frac{dP}{\rho}
\end{equation}
In the adiabatic limit $TdS = dQ =0$ and $dh = \frac{dP}{\rho}$. So for an adiabatic ideal gas
\begin{equation}
\int{\frac{dP}{\rho}} = h
\end{equation}