Zingale's
Brown's
code
Iliadis' database
Herwig's
Meyer's
Other Stuff:
Contact:
my vitae,
vitae,
, and
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The tool in
snlite.tbz
generates simple radioactive decay models of late-time supernova light curves.
This tool was used in this
article and this
article on
SN 1987A.
The tool in
lc1a.tbz
generates simple supernova type 1a light curves. It is based on the
expressions in Arnett
1982
and Dado & Dar
2015
where the bolometric luminosity is given by
\begin{equation}
L_b(t) = \frac{1}{t_r^2} \exp \left ( \frac{-t^2}{2 \ t_r^2} \right ) \int_0^t t \ \exp \left ( \frac{-t^2}{2 \ t_r^2} \right ) \ {\dot E}(t) \ {\rm d}t
\ ,
\label{eq1}
\tag{1}
\end{equation}
where $t_r$ is the rise time
and ${\dot E}(t)$ is the energy deposition from
radioactive decay of $^{56}{\rm Ni}$ and $^{56}{\rm Co}$ and positron heating.
The tool's default set of parameters is aimed at
SN 1992bc:
for more on radioactive isotopes, peek at the
26Al and 60Fe,
44Ti, 60Co and 56Ni, and
other radioactivities.
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