Cosmic microwave background (CMB) temperature and polarization anisotropies from Planck have estimated a lower value of the optical depth to reionization (τ) compared to WMAP. A significant period in the reionization history would then fall within 6
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http://dx.doi.org/10.1103/PhysRevLett.125.071301 DOI Listing Publication Analysis
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August 2024
Department of Physics, Graduate School of Science, Nagoya University, Nagoya, Japan.
The Cosmic Gems arc is among the brightest and highly magnified galaxies observed at redshift z ≈ 10.2 (ref. ).
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Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK.
The hydrogen 21-cm signal is predicted to be the richest probe of the young Universe, including those 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.
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National Astronomical Observatory of Japan.
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Paris Centre for Cosmological Physics, Université de Paris, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France; Institute for Advanced Study & Physics Department, Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, Hong Kong; Physics Department and Lawrence Berkeley National Laboratory, University of California, Berkeley, California 94720, USA; and Energetic Cosmos Laboratory, Nazarbayev University, Astana, Kazakhstan.
Cosmic microwave background (CMB) temperature and polarization anisotropies from Planck have estimated a lower value of the optical depth to reionization (τ) compared to WMAP. A significant period in the reionization history would then fall within 6
Astrophys J
February 2020
JHU Department of Physics and Astronomy, 3701 San Martin Drive, Baltimore MD, 21218, USA.
We explore the fundamental limits to which reionization histories can be constrained using only large-scale cosmic microwave background (CMB) anisotropy measurements. The redshift distribution of the fractional ionization () affects the angular distribution of CMB polarization. We project constraints on the reionization history of the universe using low-noise full-sky temperature and E-mode measurements of the CMB.
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