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| Main Author: | |
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| Format: | Recurso digital |
| Language: | English |
| Published: |
Zenodo
2026
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| Subjects: | |
| Online Access: | https://doi.org/10.5281/zenodo.19999876 |
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Table of Contents:
- <p class="MsoNormal">This paper introduces the theory of Metric Topological Relaxation (MTR). We propose that black holes (BHs) function as topological "sinks" where localized standing waves of space-time (quanta of matter) undergo a process of smoothing into a non-localized vacuum state. By applying the Lagrangian formalism to this relaxation process, we analytically derive the cosmological coupling coefficient k ≈ 3. This result provides a theoretical foundation for recent observational data (Farrah et al., 2023) suggesting that black holes are the astrophysical source of dark energy.</p>