Elucidating cosmological model dependence with $$H_0$$ H 0
Abstract We observe that the errors on the Hubble constant $$H_0$$ H 0 , a universal parameter in any FLRW cosmology, can be larger in specific cosmological models than Gaussian processes (GP) data reconstruction. We comment on the prior mean function and trace the smaller GP errors to stronger corr...
| Hlavní autoři: | , |
|---|---|
| Médium: | Článek |
| Jazyk: | English |
| Vydáno: |
SpringerOpen
2021-10-01
|
| Edice: | European Physical Journal C: Particles and Fields |
| On-line přístup: | https://doi.org/10.1140/epjc/s10052-021-09708-2 |