Reconstruction of Cosmological Initial Density Field with Observations from the Epoch of Reionization

Reconstruction of Cosmological Initial Density Field with Observations from the Epoch of Reionization

The initial density distribution provides a basis for understanding the complete evolution of cosmological density fluctuations. While reconstruction in our local Universe exploits the observations of galaxy surveys with large volumes, observations of high-redshift galaxies are performed with a smal...

Volledige beschrijving

Bibliografische gegevens
Hoofdauteurs: Meng Zhou, Yi Mao
Formaat: Artikel
Taal:English
Gepubliceerd in: IOP Publishing 2024-01-01
Reeks:The Astrophysical Journal
Onderwerpen:
Reionization
H I line emission
CO line emission
Initial conditions of the universe
Line intensities
Online toegang:https://doi.org/10.3847/1538-4357/ad2991

Internet

https://doi.org/10.3847/1538-4357/ad2991

Gelijkaardige items