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| Main Author: | |
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| Format: | Preprint |
| Published: |
2023
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2305.09367 |
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Table of Contents:
- The Generalized Cosmological Time (GCT) framework interprets the observed time dilation in Type Ia supernovae (SNe Ia) as a manifestation of a generalized lapse function in the background metric, favoring a parameter value b \approx 0.04. However, precision spectroscopic measurements of the fine-structure constant αvia the alkali doublet (AD) and many-multiplet (MM) methods predominantly yield null results. In this work, I demonstrate that this discrepancy is not a sensitivity limitation but a fundamental physical consequence of distinguishing between global coordinate time and local proper time. By inverting the GCT scaling relations, I establish that spectroscopic data constrain the effective parameter to |b_{\text{local}}| \lesssim 10^{-5}, revealing a tension of three orders of magnitude against the background value. I resolve this by invoking the principle of environmental shielding. I argue that dense, virialized gas clouds maintain a static local metric that is dynamically decoupled from the background cosmological time flow, strictly analogous to the detachment of bound systems from the Hubble expansion. Consequently, atomic spectra probe a shielded local frame where physical constants remain invariant, whereas SNe Ia observations measure the accumulated geometric time dilation of photons traversing the expanding background. This framework reconciles the positive dilation signals in geometric probes with the stability of fundamental constants in local bound systems without modifying local physical laws.