First stars, chemical evolution, cosmology
What are the major recent accomplishments?
What are the specific compelling open questions? (Unexplained observations, problems in theoretical modeling, etc)
How can one address these open questions? What are the high impact nuclear experiments, observations, theoretical studies that need to be done?
What kinds of experiments, theoretical work, and observations are needed?
In which direction should this area evolve in light of expected new observational, theoretical, and experimental capabilities?
How does this subfield intersect with other subfields? (For example, is there work needed in other subfields to move this subfield forward)
Working group program
Talks (8-10 minutes, addressing questions, first hour of working group)
Discussion (interspersed with talks)
Extended discussion about questions. See this link
for a Google Doc summarizing the discussion (which may be updated over time) or this link
for a pdf version (which will likely not be up-to-date).
wiki/first_stars_chemical_evolution_cosmology_fields_o_shea.txt · Last modified: 2013/01/10 17:47 (external edit)