Future prospects on constraining neutrino cosmology with the Ali CMB
  Polarization Telescope
  We forecast the constraints on the parameters of neutrino physics with the
constructions of Cosmic Microwave Background (CMB) temperature, E-mode
polarization and lensing spectra for the ground-based Ali Cosmic Microwave
Background Polarization Telescope (AliCPT). To implement the forecast
calculations, we perform numerical simulations which show that AliCPT would
yield the result $\sigma (N_{\mathrm{eff}})=0.42$ and $\sigma (M_{\nu})=0.18$
for the first year observation. Moreover, we investigate how the instrumental
parameters, such as noise level, full width at half maxima (FWHM), and sky
coverage can affect the constraints on these two parameters. Our forecasting
results find that a large aperture telescope with a large sky survey strategy
would significant improve the current constraints.
