Difference between revisions of "Meeting 20 April 2017"

Revision as of 17:40, 21 April 2017

PRESENTATIONS FROM THE MEETING

HOMEWORK FROM THE MEETING (from Thia's 4/21/17 email)

We agreed that the two WACS-focused groups would send suggested toy models of their systems that they would like to work on before the next meeting to Rolf, Tanja, and I for comment. This should be done in the next couple days so that we can iterate this back out quickly. All will work with a 10% radiator, 2.5 uAmps, 11.5 GeV beam for now.

In parallel, we all agreed that actual experiment benchmarking of the results, in particular the "interesting" differences we observed between codes, was important work to pursue.

Also, it seemed clear that the Hall D K_long effort was positively on track with what we did already - perhaps move to a rectangular toy model of the same thing with a beam aperture is all that's needed as a next step here.

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 * [https://wiki.jlab.org/cuawiki/images/0/0c/GN_HCPS_4_20_2017.pdf GEANT4 simulation (Gabi)]
+HOMEWORK FROM THE MEETING (from Thia's 4/21/17 email)
+* We agreed that the two WACS-focused groups would send suggested toy models of their systems that they would like to work on before the next meeting to Rolf, Tanja, and I for comment. This should be done in the next couple days so that we can iterate this back out quickly. All will work with a 10% radiator, 2.5 uAmps, 11.5 GeV beam for now.
+* In parallel, we all agreed that actual experiment benchmarking of the results, in particular the "interesting" differences we observed between codes, was important work to pursue.
+* Also, it seemed clear that the Hall D K_long effort was positively on track with what we did already - perhaps move to a rectangular toy model of the same thing with a beam aperture is all that's needed as a next step here.