This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision Next revision Both sides next revision | ||
culinary_services [2014/06/02 17:40] long |
culinary_services [2014/06/02 17:52] long |
||
---|---|---|---|
Line 12: | Line 12: | ||
Sensitivity studied of <sup>44</sup>Ti production in in core-collapse supernova environments. | Sensitivity studied of <sup>44</sup>Ti production in in core-collapse supernova environments. | ||
- | + | **Recipe** \\ | |
+ | Starting with a set parameter space of peak temperatures [T<sub>9</sub> = 4 - 7] and densities [$\rho$ = 10<sup>5</sup> - 10<sup>7</sup> g/cm<sup>3</sup>]. | ||
**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]] |