E^2 =
m^2c^4 + p^2c^2
Ω(r)(z)/Ω(m)(z) =
Ω(r,0)(1+z)/Ω(m,0)
T =
1.4x10^10K/√t
E(typ) =
3MeV/√t
T(eq) =
10,000K
1x10^4K
t(eq) =
2x10^12s
for adiabatically-expanding universe
aT = const
a(dot)T + T(dot)a = 0
Y4 =
He/H+He
Ω(m)(z) =
Ω(m,0)(1+z)^3/E(z)^2
Ω(k)(z) =
Ω(k,0)(1+z)^2/E(z)^2
Ω(Λ)(z) =
Ω(Λ,0)/E(z)^2
T(dec) =
3000K