Moderator: Simon Foreman
Presentation materials (upload).
4:30pm-4:40pm - George M. Fuller - High precision neutrino decoupling calculations
4:45pm-4:55pm - Evan Grohs - Neutrinos in BBN
5:00pm-5:45pm - Neutrino physics discussion panel: Kev Abazajian, George M. Fuller, Evan Grohs, Joel Meyers
Guiding discussion questions:
What are the new opportunities for neutrino physics presented by CMB in HD, as compared to say Simons Observatory?
Would CMB in HD observations be expected to help to break or circumvent optical depth degeneracy with neutrino mass?
Are m_nu, N_eff, and Y_p the most relevant neutrino physics related observables as we push to a new regime of observation?
How will constraints from Super-CHIME on Neff compare to CMB constraints?
5:50pm-6:00pm - Joel Meyers - Summary of Workshop