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)

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