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...
Kaydedildi:
| Asıl Yazarlar: | , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
De Gruyter
2026-06-01
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| Seri Bilgileri: | Open Astronomy |
| Konular: | |
| Online Erişim: | https://doi.org/10.1515/astro-2025-0022 |
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