Part II

44. The Integrated Sachs-Wolfe Effect Does Not Require Decaying Gravitational Potentials

The late-time ISW effect, correlations between CMB temperature and large-scale structure, is conventionally used as evidence for dark-energy-driven accelerating expansion. BFUT Paper 12 addresses the same correlation through direct substrate temperature coupling with the matter density field, with simulated results matching the observed superstructure and supervoid signal amplitudes more closely than the standard model's own predicted amplitude, without requiring accelerating expansion as the mechanism [P12].

Source papers: P12

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