| Speaker | Ernst Rehm, Argonne National Laboratory, Physics Division |
|---|---|
| Date | Thursday, July 15, 2010, 7:30 PM |
| Location | Pavillon RJA Levesque, salle 104 |
Abstract
The 12C(α,γ)16O reaction is one of the most important reactions in stellar nucleosynthesis and, for that reason, has sometimes been called ‘the holy grail’ of nuclear astrophysics. I will give a brief status report on earlier measurements and then discuss a new approach, which will utilize a superheated droplet detector and the free electron laser at Duke University.
Refreshments will be served at café et biscuits à 15h00.

