A comparison of Bayesian and frequentist confidence intervals in the presence of a late Universe degeneracy
Abstract Hubble tension is a problem in one-dimensional (1D) posteriors, since local $$H_0$$ H 0 determinations are only sensitive to a single parameter. Projected 1D posteriors for $$\Lambda $$ Λ CDM cosmological parameters become more non-Gaussian with increasing effective redshift when the model...
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| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
SpringerOpen
2025-02-01
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| Series: | European Physical Journal C: Particles and Fields |
| Online Access: | https://doi.org/10.1140/epjc/s10052-024-13727-0 |
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