21cmFirstCLASS I. Cosmological tool for $\Lambda$CDM and beyond
Jordan Flitter, Ely D. Kovetz

TL;DR
21cmFirstCLASS is a new computational tool that integrates cosmological and astrophysical modeling to analyze 21-cm signals across cosmic history, including non-linear models like scattering dark matter, enabling improved parameter constraints.
Contribution
It introduces 21cmFirstCLASS, a modified version of 21cmFAST that uses CLASS for consistent initial conditions and models inhomogeneities, allowing for comprehensive analysis of 21-cm signals and non-linear cosmologies.
Findings
Demonstrated how combined CMB and 21-cm data constrain parameters.
Provided self-consistent 21-cm power spectrum calculations with scattering dark matter.
Showcased the code's capability to analyze non-linear dark ages models.
Abstract
In this work we present 21cmFirstCLASS, a modified version of 21cmFAST, the most popular code in the literature for computing the anisotropies of the 21-cm signal. Our code uses the public cosmic microwave background (CMB) Boltzmann code CLASS, to establish consistent initial conditions at recombination for any set of cosmological parameters and evolves them throughout the dark ages, cosmic dawn, the epoch of heating and reionization. We account for inhomogeneity in the temperature and ionization fields throughout the evolution, crucial for a robust calculation of both the global 21-cm signal and its fluctuations. We demonstrate how future measurements of the CMB and the 21-cm signal can be combined and analyzed with 21cmFirstCLASS to obtain constraints on both cosmological and astrophysical parameters and examine degeneracies between them. As an example application, we show how…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Cosmology and Gravitation Theories · Scientific Research and Discoveries
