Hawking's Singularity Theorem
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A Hawking's Singularity Theorem is a singularity theorem that proves the existence of singularities in cosmological spacetimes under expansion conditions and energy constraints.
- AKA: Hawking Singularity Theorem, Cosmological Singularity Theorem, Big Bang Singularity Theorem.
- Context:
- It can typically prove Big Bang Singularities in expanding universes.
- It can typically apply Time-Reverse Arguments to cosmological evolution.
- It can typically require Energy Conditions for matter content.
- It can typically assume Cosmological Homogeneity at large scales.
- It can often complement Penrose's Singularity Theorem for black holes.
- It can often utilize Raychaudhuri Equation in geometric analysis.
- It can often inspire Quantum Cosmology through initial singularity problems.
- It can range from being a Classical Hawking's Singularity Theorem to being a Quantum-Modified Hawking's Singularity Theorem, depending on its theoretical framework.
- It can range from being a Strong Hawking's Singularity Theorem to being a Weak Hawking's Singularity Theorem, depending on its assumption strength.
- It can range from being a Past Hawking's Singularity Theorem to being a Future Hawking's Singularity Theorem, depending on its temporal direction.
- It can range from being a Isotropic Hawking's Singularity Theorem to being an Anisotropic Hawking's Singularity Theorem, depending on its symmetry assumptions.
- ...
- Example:
- Related Cosmological Theorems, such as:
- Applications, such as:
- ...
- Counter-Example:
- Penrose's Singularity Theorem, which focuses on gravitational collapse rather than cosmological expansion.
- No-Boundary Proposal, which avoids initial singularity through quantum effects.
- See: Singularity Theorem, Penrose's Singularity Theorem, General Relativity Theory, Cosmology, Big Bang Theory, Einstein's Field Equations, Energy Condition.