Although very weakly interacting, neutrinos are produced copiously in
the early universe and may play a crucial role in establishing the con
tents and structure of the universe and its subsequent evolution. Afte
r reviewing the physics which influences the production and survival o
f neutrinos--massive as well as massless--in the early universe, I wil
l outline their effects on primordial nucleosynthesis and on the dynam
ics and large scale structure of the universe. The complementary natur
e of the Astro-Particle Physics Connection will be emphasized with par
ticular attention paid to the ''17 keV neutrino'', light neutrinos as
hot dark matter and constraints on the mass and lifetime of the tau-ne
utrino.