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culinary_services [2014/06/03 17:04] parzuchowski |
culinary_services [2014/06/03 18:43] long |
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\end{equation} | \end{equation} | ||
- | which **obviously** leads to: | + | Where $\tau$ is some static free-fall timescale. |
+ | This **obviously** leads to: | ||
\begin{equation} | \begin{equation} | ||
T(t) = T_0 exp(-t/3\tau) \hspace{1cm} \rho (t) = \rho_0 exp(-t/\tau) | T(t) = T_0 exp(-t/3\tau) \hspace{1cm} \rho (t) = \rho_0 exp(-t/\tau) | ||
\end{equation} | \end{equation} | ||
- | where $T_0$ and $\rho_0$ are the peak temperatures and densities in the supernova. | + | where $T_0$ and $\rho_0$ are the peak temperature and density in the supernova. |
- | + | ||
- | + | ||
+ | Then you run the code, and it doesn't work. | ||
**REFERENCES** \\ | **REFERENCES** \\ | ||
- | [[http://iopscience.iop.org/0067-0049/191/1/66|Trends in 44Ti and 56Ni from Core-Collapse Supernovae]] | + | [[http://iopscience.iop.org/0067-0049/191/1/66|Trends in 44Ti and 56Ni from Core-Collapse Supernovae]]\\ |
+ | [[http://iopscience.iop.org/0004-637X/504/1/500|Nuclear Reactions Governing the Nucleosynthesis of 44Ti]] |