Generalizing the Hubble constant determination including curvature and dynamical dark energy
We determine the Hubble constant H 0 using two calibrator samples of type Ia supernovae (SNe Ia). We extend the well-consolidated procedure involving cosmographic series by including spatial curvature and we also utilize a different approach based on the Bézier interpolation curve accounting for the...
Furkejuvvon:
| Váldodahkkit: | , |
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| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
De Gruyter
2026-06-01
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| Ráidu: | Open Astronomy |
| Fáttát: | |
| Liŋkkat: | https://doi.org/10.1515/astro-2025-0022 |
| Fáddágilkorat: |
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