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GENERAL RELATIVITY / QUANTUM FRONTIER / COSMOLOGY

Black Holes, Horizons & Cosmological Time

Black holes test temporal geometry locally and regionally. Cosmology asks how temporal structure behaves across the history, boundaries, and possible future of the universe.

Black Holes & Cosmology

Black Holes as Temporal Laboratories

Time Dilation

Different worldlines near strong gravity accumulate different proper times. This enables future-directed differential aging, not automatic travel to the past.

Horizons

An event horizon is a causal boundary, not a material surface or established portal.

Rotation

Kerr geometry produces frame dragging, ergospheres, rotational-energy access, and difficult inner-horizon physics.

Cosmological Temporal Structure

Cosmic Time

A natural large-scale parameter in homogeneous cosmological models, not Newtonian absolute time.

Low-Entropy Past

The early universe’s smooth gravitational state is central to explaining the arrow of time.

Horizons & Deep Time

Accelerated expansion can isolate regions permanently and constrain any long-lived civilization.

Beginnings & Endings

The Big Bang is the boundary of classical extrapolation; bounces, cycles, heat death, vacuum decay, and other futures remain model-dependent.

Claim boundary: black holes are extreme spacetime structures and powerful research environments. They are not infinite energy sources or automatic time machines.