| Revista: | Revista mexicana de física |
| Base de datos: | PERIÓDICA |
| Número de sistema: | 000460655 |
| ISSN: | 0035-001X |
| Autors: | Escamilla Rivera, C1 |
| Institucions: | 1Universidad Nacional Autónoma de México, Instituto de Ciencias Nucleares, Cuidad de México. México |
| Any: | 2022 |
| Període: | Jul-Ago |
| Volum: | 68 |
| Número: | 4 |
| País: | México |
| Idioma: | Inglés |
| Tipo de documento: | Artículo |
| Enfoque: | Analítico, teórico |
| Resumen en inglés | We show that the gravitational waves measurements have raised the opportunity to measure H 0 with dark sirens to within 2σ, the accuracy required to resolve the Hubble-Lemaître tension. There are two principal reasons for our results: (1) upgrades to GW LIGO-Virgo transient catalogues GWTC-1 and GWTC-2 enhance their sensitive with only 10% of contamination fraction, and (2) new dark sirens should help to constrain our dynamical EoS. In conjunction, sensitivity upgrades and a new dark energy model will facilitate an accurate inference of the Hubble-Lemaître constant H 0 to better with an ±0.077 error in comparison to the LIGO dark siren with +14.0/-7.0, which would further solidify the role of dark sirens in late dark energy for precision cosmology in the future |
| Disciplines | Física y astronomía |
| Paraules clau: | Física, Ondas gravitacionales, Solución de energía oscura, Tensión Hubble-Lemaître |
| Keyword: | Physics, Gravitational waves, Dark energy solution, Hubble-Lemaitre tension |
| Text complet: | Texto completo (Ver HTML) Texto completo (Ver PDF) |
