group2
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group2 [2014/06/10 17:55] bartl |
group2 [2014/06/13 08:49] (current) bartl |
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| * Varying $\Lambda_{QCD}$ | * Varying $\Lambda_{QCD}$ | ||
| * Neutron magnetic moment | * Neutron magnetic moment | ||
| - | * ... | + | * Variations in gravitational constant |
| + | |||
| + | ==== Results ==== | ||
| + | For our results, please refer to our {{::bsmbbn-presentation.pdf|final presentation}} | ||
| ==== Logbook ==== | ==== Logbook ==== | ||
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| * started figuring out how the proton-neutron mass splitting and the deuteron properties depend on our input parameters | * started figuring out how the proton-neutron mass splitting and the deuteron properties depend on our input parameters | ||
| * fixed several bugs in the code, continued familiarizing ourselves with Fortran and the BBN code | * fixed several bugs in the code, continued familiarizing ourselves with Fortran and the BBN code | ||
| + | |||
| + | === Wednesday, June 11 === | ||
| + | * produced plots of BBN abundance as function of grav. constant | ||
| + | * tried to calculate and fit the $p(n,\gamma)d$ rate to use as input; partially succeeded | ||
| + | |||
| + | === Thursday, June 12 === | ||
| + | * produced data and plots for BBN abundance as function of $\Lambda_{QCD}$ and $\mu_n$ | ||
| + | * also looked at the individual effects of $\Lambda_{QCD}$ on the actual inputs to the BBN calculation (neutron-proton mass splitting, neutron life time, deuteron energy, $p(n,\gamma)d$ rate) and identified the life time effect as the main effect driving the change in the <sup>4</sup>He abundance. | ||
| + | * created {{::bsmbbn-presentation.pdf|final presentation}} | ||
group2.1402437347.txt.gz · Last modified: 2014/06/10 17:55 by bartl
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