15 May, 2026

Clarification

One shouldn't confuse 2 separate concepts:

The expansion rate Ht which:

  • was high in the early universe { high z } & is low today { z = 0 }
  • has changed over time; namely was decelerating in the past { high z } but is accelerating today { H0 }.

It’s like a car which was slowing down in the past but is currently speeding up!