Cosmic mysteries and the hydrogen 21-cm line: bridging the gap with lunar observations

Abstract

The hydrogen 21-cm signal is predicted to be the richest probe of the young Universe including eras known as the cosmic Dark Ages, the Cosmic Dawn when the first star and black hole formed, and the Epoch of Reionization. This signal holds the key to deciphering processes that take place at the early stages of cosmic history. In this opinion piece, we discuss the potential scientific merit of lunar observations of the 21-cm signal and their advantages over more affordable terrestrial efforts. The moon is a prime location for radio cosmology which will enable precision observations of the low-frequency radio sky. The uniqueness of such observations is that they will provide an unparalleled opportunity to test cosmology and the nature of dark matter using the Dark Ages 21-cm signal. No less enticing is the opportunity to obtain a much clearer picture of Cosmic Dawn than what is achievable from the ground, which will allow us to probe properties of the first stars and black holes.

15 pages, 3 figures, accepted for publication in Philosophical Transactions A

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Cited by in corpus (4)

• Exploiting synergies between JWST and cosmic 21-cm observations to uncover star formation in the early Universe
• Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization
• Radiometer Calibration using Machine Learning
• ECHO21: a tool for modelling global 21-cm signal from dark ages to reionization