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