Data Matter
Definition
Data Matter is the dark matter of a universe: the data that never became physical. At the Physical Nova part of the data on the scaffold condenses into matter; the rest stays data, gaining mass at that moment by the Data–Matter Equivalence but never resolved into charged particles, so it gravitates and never touches light.
It is laid on the scaffold at the Data Nova as massless data and gains its mass at the Physical Nova, frozen there, so it thins with the expansion as a⁻³, as cold dark matter does. It has every observed property of dark matter: it gravitates (galaxy clusters, rotation curves), it neither emits nor absorbs light, it passes through itself without colliding (the Bullet Cluster), it is cold, and it forms the cosmic web before ordinary matter falls into it, the order the novas build in. The Proto Wells are its first wells, the seeds of the halos galaxies sit in. Over a universe's life it returns slowly along the Data Loop, within the limits the sky sets on decaying dark matter, and the space it leaves is the Null Vacuum. In our universe there is about 5.4 times as much of it as of ordinary matter (the Data Matter Ratio).
Formally, M◍ = N◍ · k_B · T↯ · ln(2) / c², where M◍ [𝕄] is the mass of a body of Data Matter, N◍ [∅] its unresolved bits, k_B [𝕄·𝕃²·𝕋⁻²·Θ⁻¹] the Boltzmann constant, T↯ [Θ] the temperature at the Physical Nova and c [𝕃·𝕋⁻¹] light speed: [𝕄] = [𝕄].
It connects to Data Matter Mass, Data Matter Ratio, Data Matter Return, Null Vacuum, Vacuum Pressure, Data–Matter Equivalence, Proto Well, Unresolved Computational Nodes and Data Loop.
Mathematical Expression
M◍ = N◍ · k_B · T↯ · ln(2) / c²
Technical Details
Category: Manuscript
Chapter: Chapter 3
Importance Level: