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 [2014/06/01 20:46] long |
culinary_services [2014/06/02 17:50] long |
||
---|---|---|---|
Line 1: | Line 1: | ||
- | We are Culinary Services. | + | We are Culinary Services. \\ |
+ | \\ | ||
Who ordered the extra side of <sup>44</sup>Ti? | Who ordered the extra side of <sup>44</sup>Ti? | ||
**GROUP MEMBERS**\\ | **GROUP MEMBERS**\\ | ||
- | Alex Long\\ | + | Alex Long (parameters)\\ |
- | McKenzie Warren\\ | + | MacKenzie Warren (code)\\ |
- | Nathan Parzuchowski\\ | + | Nathan Parzuchowski (analysis)\\ |
**TOPIC** \\ | **TOPIC** \\ | ||
- | Early Carbon production (Helium burning) in **very** massive Pop III stars, and ensuing CNO cycle. | + | 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 []. | ||
+ | |||
+ | **REFERENCES** \\ | ||
+ | [[http://iopscience.iop.org/0067-0049/191/1/66|Trends in 44Ti and 56Ni from Core-Collapse Supernovae]] |