Evolution of the cosmic horizons in a photon dominated universe (Ωr=1)
in proper (r) & comoving (R) distances; plot range: r&R=0..70, t=0..70
Gray dashed curves: worldlines of objects comoving with the Hubbleflow
The Hubbleradius rH & the particlehorizon rP coincide and grow with 2c
If H=67.15 at a=1, the age of this universe at a=1 would be t=7.280657
Other diagrams: pure matter (Ωm=1) and mixed component (Ω=1) universes
r(t)
r(t)
↑ r(t) / ↓ R(t)
R(t)
R(t)
«back Index: a, ȧ, ä, ã, â, H, Ḣ, Ḧ, rH, rE, rP, rL, Σr, Ω
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