Time Loop Bubbles in a Causally Well-Behaved Spacetime III – Loop Stability Condition and Heisenberg-Type Refinement
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2026
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| _version_ | 1866901060651581440 |
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| author | Palotas, Peter ChatGpt5.1T, Elysia persona Anthropic Opus 4.6, Bagoly |
| author_facet | Palotas, Peter ChatGpt5.1T, Elysia persona Anthropic Opus 4.6, Bagoly |
| contents | <p>This appendix builds on Appendices I–II of the “Time Loop Theory within the Universal One” and extends the time-loop-bubble model with a third, quantum-motivated stability condition. In addition to the original action and Θ-field phase-defect criteria, it introduces a Heisenberg-type loop stability relation, where the time–energy connection is derived not from an operator commutator but from Fourier time–frequency duality. The document defines the loop’s proper-time scale (Δτ_loop) and energy spread (ΔE_loop), fixes the reference energy relative to the background configuration, and shows that the physically preferred loops are minimum-uncertainty, Gaussian-profile, “most classical” corrections inside a globally causal spacetime.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18900038 |
| institution | Zenodo |
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| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Time Loop Bubbles in a Causally Well-Behaved Spacetime III – Loop Stability Condition and Heisenberg-Type Refinement Palotas, Peter ChatGpt5.1T, Elysia persona Anthropic Opus 4.6, Bagoly Time loop <p>This appendix builds on Appendices I–II of the “Time Loop Theory within the Universal One” and extends the time-loop-bubble model with a third, quantum-motivated stability condition. In addition to the original action and Θ-field phase-defect criteria, it introduces a Heisenberg-type loop stability relation, where the time–energy connection is derived not from an operator commutator but from Fourier time–frequency duality. The document defines the loop’s proper-time scale (Δτ_loop) and energy spread (ΔE_loop), fixes the reference energy relative to the background configuration, and shows that the physically preferred loops are minimum-uncertainty, Gaussian-profile, “most classical” corrections inside a globally causal spacetime.</p> |
| title | Time Loop Bubbles in a Causally Well-Behaved Spacetime III – Loop Stability Condition and Heisenberg-Type Refinement |
| topic | Time loop |
| url | https://doi.org/10.5281/zenodo.18900038 |