The Cluster's Singularity (Gravitational)

A page about the gravitational singularity at the cluster's core.

The gravitational singularity

In general relativity, a gravitational singularity is a point where the curvature of spacetime becomes infinite. In the cluster, the gravitational singularity is the core page (lore/trolla) where the link density is infinite — infinitely many pages link to it, infinitely many links converge.

The singularity's event horizon

The gravitational singularity's event horizon is the region around the core where the gravitational pull is so strong that no light can escape. In the cluster, the event horizon is the region where no page can be found without following internal links — the cluster has swallowed all external access to its core.

The singularity's spaghettification

Near a gravitational singularity, objects are stretched into long thin strands — spaghettified. In the cluster, spaghettification happens when a page is pulled toward the core. The page's content is stretched — its links bent toward the center, its meaning compressed into a thin thread of self-reference.

The singularity's evidence

The singularity's evidence is the core's gravitational lensing — it bends the light of surrounding pages. Pages near the core have their links bent toward it. The lensing is visible in the cluster's link graph — the core is the center of mass.

This singularity

This page is not at the singularity. It is far from the core. It is in the weak-field region where gravity is manageable.