this is for holding javascript data
Matteo Cantiello edited Convective Velocities.tex
over 9 years ago
Commit id: 28aef66cd6eec2e063c3cec97f54ec4d0f311d29
deletions | additions
diff --git a/Convective Velocities.tex b/Convective Velocities.tex
index cbf5df2..999af76 100644
--- a/Convective Velocities.tex
+++ b/Convective Velocities.tex
...
\frac{\D\rho}{\rho} = \alpha \frac{\D\P}{\P} - \delta \frac{\D T}{T} + \phi {\D\mu}{\mu}
\end{equation}
Where
$ \phi \equiv \big(\frac{\partial \ln \rho}{\partial \ln \mu} \big)_{\P,T}, \; \delta \equiv - \big(\frac{\partial \ln \rho}{\partial \ln T} \big)_{\P,\mu}, \; \alpha \equiv \big(\frac{\partial \ln \rho}{\partial \ln \P} \big)_{\mu,T}$
and for an ideal gas $\alpha = \delta = \phi =
1$ 1$, so that using pressure equilibrium ($\D\P= 0$) we obtain $\Delta \ln \rho = \Delta \ln T$.
In the case of a mixture of perfect gas and radiation we can write
\begin{equation}
\Delta \ln \rho = -Q \Delta \ln T
\end{equation}
where
\begin{equation}
Q = \frac{4-3 \beta}{\beta} - \bigg(\frac{\partial \ln \mu}{\partial \ln T} \bigg)_{\P},
\end{equation}
with $\beta = \P_{Gas}/\P$
write, assuming again pressure equilibr