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Hartle-Hawking No-Boundary vs Vilenkin's Tunneling from Nothing
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Hartle-Hawking No-Boundary Speculative | Vilenkin's Tunneling from Nothing Speculative | |
|---|---|---|
| Proposed | 1983 | 1982 |
| Key figures | James Hartle, Stephen Hawking | Alexander Vilenkin |
| In one sentence | The universe has no temporal boundary at the beginning. In Euclidean time, the universe is a smooth four-dimensional surface with no edge, like asking what is south of the South Pole. | Vilenkin proposed in 1982 that the universe quantum-tunneled into existence from a state with no space, no time, no fields, literal nothing. |
| Predictions |
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| Where it breaks |
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| Key unresolved problem | The instability problem: a careful redo of the math by Feldbrugge, Lehners, and Turok suggests the no-boundary proposal predicts runaway, ever-growing fluctuations, which would mean an unstable universe rather than the smooth one we see. | The laws-from-nothing problem: the quantum tunneling that creates the universe still needs quantum laws and a space of possible states to work in, so the proposal has not truly started from nothing. |
| Reader vote | 0% · 0 votes | 100% · 2 votes |
Hartle-Hawking No-Boundary
1983 · Speculative
Vilenkin's Tunneling from Nothing
1982 · Speculative
Proposed
1983
1982
Key figures
James Hartle, Stephen Hawking
Alexander Vilenkin
In one sentence
The universe has no temporal boundary at the beginning. In Euclidean time, the universe is a smooth four-dimensional surface with no edge, like asking what is south of the South Pole.
Vilenkin proposed in 1982 that the universe quantum-tunneled into existence from a state with no space, no time, no fields, literal nothing.
Predictions
- No initial [[singularity]]
- Universe wavefunction smooth at a = 0
- Predicts a specific spectrum of cosmological perturbations
- [[Inflation]] begins naturally with high probability after tunneling
- Universe is initially small, closed, and de Sitter-like
- No contracting phase before the Bang
Where it breaks
- Feldbrugge, Lehners, Turok (2017) argue the proposal predicts an unstable universe
- Direction of "outgoing" vs "incoming" mode is contested
- A more careful mathematical analysis of the path integral suggests deeper problems, hinting the proposal may predict unstable outcomes (see Go Deeper)
- Maldacena (2024) re-examines the no-boundary proposal and finds it predicts spatial curvature in conflict with observations, and is non-normalizable for landscape-like potentials.
- Ivo, Li & Maldacena (2024) show that once you account for the regions of space we cannot observe, the mathematics of the no-boundary state leads to physically unrealistic predictions, sharpening the case against the original proposal.
- Krauss: still requires quantum laws, so not really nothing
- Hawking & Bousso (1995): catastrophic particle production
- Penrose: ignores Weyl curvature hypothesis
Key unresolved problem
The instability problem: a careful redo of the math by Feldbrugge, Lehners, and Turok suggests the no-boundary proposal predicts runaway, ever-growing fluctuations, which would mean an unstable universe rather than the smooth one we see.
The laws-from-nothing problem: the quantum tunneling that creates the universe still needs quantum laws and a space of possible states to work in, so the proposal has not truly started from nothing.
Reader vote
0% · 0 votes
100% · 2 votes