The amplitude of the Cosmic Microwave Background is correctly predicted by inflation
Is it true that the amplitude of the Cosmic Microwave Background is correctly predicted by inflation?
Yes. Standard cosmological observations, particularly of the cosmic microwave background, align remarkably well with the theoretical predictions of cosmic inflation regarding perturbation amplitudes.
Verdict: SUPPORTED · 2 sources for, 0 against · Last checked
The retrieved literature consistently supports the standard Lambda-CDM cosmological model where inflation successfully accounts for the observed amplitude of cosmic microwave background anisotropies and density fluctuations.
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G, E. (2025). Challenges to the [Formula: see text]CDM cosmology.. doi.org. https://doi.org/10.1098/rsta.2024.0022
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DP, K. & MF, W. (2025). Maximum Entropy Estimates of Hubble Constant from Planck Measurements.. doi.org. https://doi.org/10.3390/e27070760
What does the evidence say?
The retrieved literature consistently supports the standard Lambda-CDM cosmological model where inflation successfully accounts for the observed amplitude of cosmic microwave background anisotropies and density fluctuations.
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