Cosmic horizons: the maths
The same smooth ΛCDM universe as the Expanding-universe lab, drawn in conformal time so light travels at 45°. Tables of conformal time built by integration. Computed live.
Equations
- η(a) = ∫₀a da′ / (a′² H(a′))
- Conformal time: how far light can have travelled (in today's distances) by the time the universe had size a.
- particle horizon = c · η(1)
- The edge of the observable universe: the farthest matter whose light has had time to reach us.
- event horizon = c · [η(∞) − η(1)]
- The farthest galaxy a signal sent today can ever reach, because accelerating expansion carries the rest away.
Constants
| Ωm, ΩΛ, Ωr | 0.315, 0.685, 9.1 × 10⁻⁵ | Planck Collaboration (2020) |
| H₀ | 67.4 km/s/Mpc | Planck (2020) |
Worked examples ✓ checked on every change
| Observable universe (particle horizon), today | 46.1 billion ly | the integral above, done independently — about 46 billion light-years |
| Event horizon, today | 16.7 billion ly | the integral above — about 16.7 billion light-years |
What's simplified
- A perfectly smooth universe.
- Distances are 'proper distance today' (comoving).
Where it breaks
Only if the ΛCDM model does — for example if dark energy isn't constant.
Sources: T. M. Davis & C. H. Lineweaver, PASA 21, 97 (2004); Planck Collaboration (2020).