Background Cosmology Flashcards
Friedmann equation
(a dot / a)^2 = 8 pi G rho/3 - kc^2/a^2
H^2/H_0^2=
Omega_r(1+z)^4 + Omega_m(1+z)^3+Omega_k*(1+z)^2 + Omega_lambda
density with w’s
rho = rho_0*a^(-3(1+w))
scale factor with w’s
a = a_0*t^(2/(3(1+w))
w’s
rad: 1/3
matter: 0
curvature: -1/3, k=-1
lambda: w=-1
Horizon
r = integrate from 0 to t over c/a dt
Inflation scale factor
a ~ exp(t/T)
Radiation scale factor
a ~t^(1/2)
Matter scale factor
a ~ t^(2/3)
Dark energy scale factor
a~exp(t)
FLRW metric
ds^2=cdt^2 - a^2[dr^2/(1-kr^2)+ r^2(dtheta^2+sin(theta)^2 dphi^2)]
density as function of H
rho=3H^2/(8piG) = 1/(6pi(1+w)^2 G t^2)
Horizon as function of z
r = integrate from 0 to z over c/H dz
Luminosity distance in flat universe
d_L=r(1+z)
Angular distance in flat universe
d_A = r/(1+z)