Vacuum Pressure

Vacuum Pressure is the dark energy of a universe: the outward push of the Null Vacuum, whose pressure is the negative of its energy density. However space grows, a vacuum stays the same vacuum and keeps the same energy in every cubic metre, so for energy to be conserved its pressure must be the negative of its density; in general relativity pressure gravitates, and negative pressure gravitates outward, so the expansion speeds up. Because every place in a universe was inside its Pulsecore at the pin head, the Null Vacuum is everywhere at once and the push acts everywhere, not from a centre. It is fed by returning Data Matter (Vacuum Feeding), so it is smallest early and grows late, and its equation of state evolves, as Part 9.1 predicts. Formally, p⦵ = −ρ⦵ · c², where p⦵ [𝕄·𝕃⁻¹·𝕋⁻²] is the pressure of the Null Vacuum, ρ⦵ [𝕄·𝕃⁻³] its density and c [𝕃·𝕋⁻¹] light speed: [𝕄·𝕃⁻¹·𝕋⁻²] = [𝕄·𝕃⁻¹·𝕋⁻²]. The equation of state is w = −1. It connects to Null Vacuum, Acceleration Equation, Cosmological Constant of the Null Vacuum, Level Λ Law, Vacuum Feeding and Global Recursion Tension Imbalance.

Category: Manuscript

Chapter: Chapter 3

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