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| Main Authors: | , |
|---|---|
| Format: | Recurso digital |
| Language: | English |
| Published: |
Zenodo
2025
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| Subjects: | |
| Online Access: | https://doi.org/10.5281/zenodo.14986857 |
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Table of Contents:
- <p>In the framework of the Emerging Quantum Fields and Adaptive Gravity Theory (CCEGA), gravity and time are not fundamental entities but rather emergent properties of the quantum field and spacetime curvature . In this work, we extend the concept of emergent gravity to time, proposing that its flow dynamically adapts to and the quantum state of .</p> <p> </p> <p>Furthermore, we explore how this formulation modifies black hole structure and Hawking radiation, leading to the concept of an adaptive quantum horizon, where the Schwarzschild radius and Hawking temperature are corrected by terms dependent on . This suggests the possible existence of black hole remnants, in contrast to the complete evaporation predicted by General Relativity.</p> <p> </p> <p>The model predicts observable effects, such as:</p> <p> </p> <p>Deviations in gravitational redshift, measurable in high-curvature environments.</p> <p> </p> <p>Corrections in CMB fluctuations, due to the emergent quantization of time in the early universe.</p> <p> </p> <p>Modified gravitational waves observed in LIGO/VIRGO, with possible quantum echoes.</p> <p> </p> <p>Altered photon ring structure in the Event Horizon Telescope (EHT), due to the smooth transition of the quantum horizon.</p> <p> </p> <p> </p> <p>These results open the door to future investigations into the relationship between emergent time, black hole structure, and quantum cosmology, establishing a unified framework for the interaction between quantum mechanics and gravity.</p>