scispace - formally typeset
Open AccessPosted Content

Baryon Acoustic Oscillation Intensity Mapping of Dark Energy

TLDR
Here it is shown how the study of acoustic oscillation in the 21 cm brightness can be accomplished by economical three-dimensional intensity mapping, and may be the starting point for a new class of dark energy experiments dedicated to large angular scale mapping of the radio sky, shedding light on dark energy.
Abstract
The expansion of the universe appears to be accelerating, and the mysterious anti-gravity agent of this acceleration has been called ``dark energy''. To measure the dynamics of dark energy, Baryon Acoustic Oscillations (BAO) can be used. Previous discussions of the BAO dark energy test have focused on direct measurements of redshifts of as many as $10^9$ individual galaxies, by observing the 21cm line or by detecting optical emission. Here we show how the study of acoustic oscillation in the 21 cm brightness can be accomplished by economical three dimensional intensity mapping. If our estimates gain acceptance they may be the starting point for a new class of dark energy experiments dedicated to large angular scale mapping of the radio sky, shedding light on dark energy.

read more

Citations
More filters
Journal ArticleDOI

Multipole expansion for H I intensity mapping experiments: simulations and modelling

TL;DR: In this article, a framework and an open-source python toolkit are presented to analyse the 2-point statistics of 3D fluctuations in the context of HI intensity maps using the multipole expansion formalism.
Journal ArticleDOI

Extreme spheres: counts-in-cells for 21cm intensity mapping

TL;DR: In this article, the authors used a large state-of-the-art magneto-hydrodynamic simulation from the IllustrisTNG project to determine the relation between neutral hydrogen and matter densities in cells.
Journal ArticleDOI

Signatures of the Baryon acoustic oscillations on the convergence power spectrum of weak lensing by large scale structure

TL;DR: In this paper, the authors employ an analytical approach to investigate the signatures of Baryon acoustic oscillations (BAOs) on the convergence power spectrum of weak lensing by large scale structure.
Journal ArticleDOI

A high-resolution self-consistent whole sky foreground model

TL;DR: In this article, a high resolution self-consistent sky model at low frequencies, which incorporates both diffuse foreground and point sources, is constructed by generating physical foreground components including the galactic synchrotron emission and galactic free-free emission.
References
More filters
Journal ArticleDOI

Observational probes of cosmic acceleration

TL;DR: In this article, the authors present extensive forecasts for constraints on the dark energy equation of state and parameterized deviations from General Relativity, achievable with Stage III and Stage IV experimental programs that incorporate supernovae, BAO, weak lensing, and cosmic microwave background data.
Journal ArticleDOI

Reionization and Cosmology with 21-cm Fluctuations

TL;DR: In this article, the authors discuss recent advances in theoretical understanding of the epoch of reionization (EoR), the application of 21-cm tomography to cosmology and measurements of the dark energy equation of state after reionisation, and the instrumentation and observational techniques shared by 21cm EoR and postreionization cosmology machines.
Journal ArticleDOI

Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS

TL;DR: In this paper, the power spectrum and bispectrum up to 4th order in the initial density perturbations were modeled as a Taylor series in the local mass density, with the unknown coefficients in the series treated as free bias parameters.
Journal ArticleDOI

Late-time cosmology with 21cm intensity mapping experiments

TL;DR: In this paper, the authors present a framework for forecasting cosmological constraints from future neutral hydrogen intensity mapping experiments at low to intermediate redshifts, and establish a simple way of comparing such surveys with optical galaxy redshift surveys.
Journal ArticleDOI

How to evade the sample variance limit on measurements of redshift-space distortions

TL;DR: In this article, the authors used multiple tracers of large-scale density with different biases to measure the redshift-space distortion parameter β ≡ b −1f ≡ b−1d−ln D/d −ln a (where D is the growth factor and a the expansion factor).
Related Papers (5)