CosmoReionMC: a package for estimating cosmological and astrophysical parameters using CMB, Lyman-α absorption, and global 21 cm data. Issue 2 (11th August 2021)

• Record Type: Journal Article
• Authors: Chatterjee, Atrideb; Choudhury, Tirthankar Roy; Mitra, Sourav
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 507:Issue 2(2021)
• Page Start: 2405
• Page End: 2422
• Publication Date: 2021-08-11
• Subjects: stars: Population III -- intergalactic medium -- dark ages, reionization, first stars -- cosmology: theory; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stab2316
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We present a Markov Chain Monte Carlo (MCMC)-based parameter estimation package, CosmoReionMC, to jointly constrain cosmological parameters of the Lambda cold dark matter (ΛCDM) model and the astrophysical parameters related to hydrogen reionization. The package is based on a previously developed physically motivated semi-analytical model for reionization, a similar semi-analytical model for computing the global 21 cm signal during the cosmic dawn and using an appropriately modified version of the publicly available camb for computing the CMB anisotropies. These calculations are then coupled to an MCMC ensemble sampler emcee to compute the posterior distributions of the model parameter. The model has 12 free parameters in total: five cosmological and seven related to the stellar populations. We constrain the parameters by matching the theoretical predictions with CMB data from Planck, observations related to the quasar absorption spectra, and, for the first time, the global 21 cm signal from EDGES. We find that incorporating the quasar spectra data in the analysis tightens the bounds on the electron scattering optical depth τ and consequently the normalization As of the primordial matter power spectrum (or equivalently σ8 ). Furthermore, when we include the EDGES data in the analysis, we find that an early population of metal-free stars with efficient radio emission is necessary to match the absorption amplitude. The CosmoReionMC package should have interesting future applications, e.g. probing non-standard extensions to the ΛCDM model.