| _version_ | 1866902001982373888 |
|---|---|
| author | Mikheil, Rusishvili |
| author_facet | Mikheil, Rusishvili |
| contents | <p>VES 3.3: Emergent Cosmic Acceleration from Scrambling-Time Limited Spacetime Memory</p> <p>This repository contains the manuscript and theoretical framework for VES 3.3, a cosmological model that derives late-time cosmic acceleration from the holographic properties of the spacetime substrate.</p> <p>Unlike standard \LambdaCDM or phenomenological dark energy models, VES 3.3 eliminates ad-hoc parameters by grounding the dynamics of the universe in quantum information theory. The core of the framework is the identification of the spacetime relaxation time (\tau) with the Fast Scrambling Bound of the cosmological horizon.</p> <p>Key Theoretical Features:</p> <p>Microscopic Origin of Memory: The viscoelastic relaxation time is derived from first principles using the scrambling time of holographic degrees of freedom: \tau \sim H^{-1} \ln(S_{BH}).</p> <p>Causal Stability: By utilizing a Maxwell-Cattaneo memory kernel, the model ensures a ghost-free scalar sector and gradient stability (c_s^2 > 0) across all cosmic epochs.</p> <p>Holographic Trigger: Cosmic acceleration is shown to be a topological transition triggered when the bulk entanglement wedge saturates the Bekenstein-Hawking entropy bound at z \approx 1.</p> <p>Observational Predictions: VES 3.3 predicts a unique, frequency-dependent Lorentzian damping profile for gravitational waves in the LISA band (10^{-5} to 10^{-1} Hz), while remaining consistent with LIGO/Virgo observations (v_{gw} = c).</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18381211 |
| institution | Zenodo |
| language | eng |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Emergent Cosmic Acceleration from Scrambling-Time Limited Spacetime Memory ( VES 3.3 ) Mikheil, Rusishvili Hubble Tension Dark Energy Holography Quantum Information Gravitational Waves LISA Viscoelastic Spacetime <p>VES 3.3: Emergent Cosmic Acceleration from Scrambling-Time Limited Spacetime Memory</p> <p>This repository contains the manuscript and theoretical framework for VES 3.3, a cosmological model that derives late-time cosmic acceleration from the holographic properties of the spacetime substrate.</p> <p>Unlike standard \LambdaCDM or phenomenological dark energy models, VES 3.3 eliminates ad-hoc parameters by grounding the dynamics of the universe in quantum information theory. The core of the framework is the identification of the spacetime relaxation time (\tau) with the Fast Scrambling Bound of the cosmological horizon.</p> <p>Key Theoretical Features:</p> <p>Microscopic Origin of Memory: The viscoelastic relaxation time is derived from first principles using the scrambling time of holographic degrees of freedom: \tau \sim H^{-1} \ln(S_{BH}).</p> <p>Causal Stability: By utilizing a Maxwell-Cattaneo memory kernel, the model ensures a ghost-free scalar sector and gradient stability (c_s^2 > 0) across all cosmic epochs.</p> <p>Holographic Trigger: Cosmic acceleration is shown to be a topological transition triggered when the bulk entanglement wedge saturates the Bekenstein-Hawking entropy bound at z \approx 1.</p> <p>Observational Predictions: VES 3.3 predicts a unique, frequency-dependent Lorentzian damping profile for gravitational waves in the LISA band (10^{-5} to 10^{-1} Hz), while remaining consistent with LIGO/Virgo observations (v_{gw} = c).</p> |
| title | Emergent Cosmic Acceleration from Scrambling-Time Limited Spacetime Memory ( VES 3.3 ) |
| topic | Hubble Tension Dark Energy Holography Quantum Information Gravitational Waves LISA Viscoelastic Spacetime |
| url | https://doi.org/10.5281/zenodo.18381211 |