Astro 2020 Science White Paper: Fundamental Cosmology in the Dark Ages with 21-cm Line Fluctuations

Early-Universe constraints on dark matter-baryon scattering and their implications for a global 21 cm signal

Original

T. R. Slatyer and C.-L. Wu · 1903

Earlier work this paper cites.

Measuring the Small-Scale Power Spectrum of Cosmic Density Fluctuations through 21 cm Tomography Prior to the Epoch of Structure Formation

A. Loeb and M. Zaldarriaga · 2004

Earlier work this paper cites.

21cm angular-power spectrum from the dark ages

A. Lewis and A. Challinor · 2007

Earlier work this paper cites.

How accurately can 21 cm tomography constrain cosmology?

Y. Mao, M. Tegmark, M. McQuinn, M. Zaldarriaga, and O. Zahn · 2008

Earlier work this paper cites.

Inflation and the scale dependent spectral index: prospects and strategies

P. Adshead, R. Easther, J. Pritchard, and A. Loeb · 2011

Earlier work this paper cites.

Towards a complete treatment of the cosmological recombination problem

J. Chluba and R. M. Thomas · 2011

Earlier work this paper cites.

21 cm cosmology in the 21st century

J. R. Pritchard and A. Loeb · 2012

Earlier work this paper cites.

Population III Star Formation in Large Cosmological Volumes. I. Halo Temporal and Physical Environment

B. D. Crosby, B. W. O’Shea, B. D. Smith, M. J. Turk, and O. Hahn · 2013

Earlier work this paper cites.

Primordial non-gaussianity from the bispectrum of 21-cm fluctuations in the dark ages

J. B. Muñoz, Y. Ali-Haïmoud, and M. Kamionkowski · 2015

Earlier work this paper cites.

Heating of baryons due to scattering with dark matter during the dark ages

J. B. Muñoz, E. D. Kovetz, and Y. Ali-Haïmoud · 2015

Earlier work this paper cites.

The future of primordial features with 21 cm tomography

X. Chen, P. D. Meerburg, and M. Münchmeyer · 2016

Earlier work this paper cites.

21cmSense: Calculating the sensitivity of 21cm experiments to the EoR power spectrum, Sep 2016

J. Pober · 2016

Cited alongside, same era.

Violation of statistical isotropy and homogeneity in the 21-cm power spectrum

M. Shiraishi, J. B. Muñoz, M. Kamionkowski, and A. Raccanelli · 2016

Cited alongside, same era.

Possible interaction between baryons and dark-matter particles revealed by the first stars

R. Barkana · 2018

Cited alongside, same era.

Severely Constraining Dark-Matter Interpretations of the 21-cm Anomaly

A. Berlin, D. Hooper, G. Krnjaic, and S. D. McDermott · 2018

Cited alongside, same era.

An absorption profile centred at 78 megahertz in the sky-averaged spectrum

J. D. Bowman, A. E. E. Rogers, R. A. Monsalve, T. J. Mozdzen, and N. Mahesh · 2018

Cited alongside, same era.

Reconstructing the Inflationary Landscape with Cosmological Data

Tighter limits on dark matter explanations of the anomalous EDGES 21 cm signal

E. D. Kovetz, V. Poulin, V. Gluscevic, K. K. Boddy, R. Barkana, and M. Kamionkowski · 2018

Later among the works it cites.

The 21cm Absorption Line and Axion Quark Nugget Dark Matter Model

Original

K. Lawson and A. R. Zhitnitsky · 2018

Later among the works it cites.

Axion-photon conversion and effects on 21 cm observation

T. Moroi, K. Nakayama, and Y. Tang · 2018

Later among the works it cites.

21-cm Fluctuations from Charged Dark Matter

J. B. Muñoz, C. Dvorkin, and A. Loeb · 2018

Later among the works it cites.

A small amount of mini-charged dark matter could cool the baryons in the early Universe

J. B. Muñoz and A. Loeb · 2018

Later among the works it cites.

Dark Cosmology: Investigating Dark Matter & Exotic Physics in the Dark Ages using the Redshifted 21-cm Global Spectrum