The first stars: formation, properties, and impact
RS Klessen, SCO Glover - Annual Review of Astronomy and …, 2023 - annualreviews.org
The first generation of stars, often called Population III (or Pop III), form from metal-free
primordial gas at redshifts z∼ 30 and below. They dominate the cosmic star-formation …
primordial gas at redshifts z∼ 30 and below. They dominate the cosmic star-formation …
Neutrino mass ordering from oscillations and beyond: 2018 status and future prospects
PF De Salas, S Gariazzo, O Mena… - Frontiers in Astronomy …, 2018 - frontiersin.org
The ordering of the neutrino masses is a crucial input for a deep understanding of flavor
physics, and its determination may provide the key to establish the relationship among the …
physics, and its determination may provide the key to establish the relationship among the …
Data analysis for precision 21 cm cosmology
A Liu, JR Shaw - Publications of the Astronomical Society of the …, 2020 - iopscience.iop.org
The redshifted 21 cm line is an emerging tool in cosmology, in principle permitting three-
dimensional surveys of our universe that reach unprecedentedly large volumes, previously …
dimensional surveys of our universe that reach unprecedentedly large volumes, previously …
HERA phase I limits on the cosmic 21 cm signal: constraints on astrophysics and cosmology during the epoch of reionization
Abstract Recently, the Hydrogen Epoch of Reionization Array (HERA) has produced the
experiment's first upper limits on the power spectrum of 21 cm fluctuations at z∼ 8 and 10 …
experiment's first upper limits on the power spectrum of 21 cm fluctuations at z∼ 8 and 10 …
Signature of excess radio background in the 21-cm global signal and power spectrum
A Fialkov, R Barkana - Monthly Notices of the Royal …, 2019 - academic.oup.com
The recent tentative detection by the Experiment to Detect the Global EoR Signature
(EDGES) low band of the hydrogen 21-cm line from cosmic dawn, if confirmed, is the first …
(EDGES) low band of the hydrogen 21-cm line from cosmic dawn, if confirmed, is the first …
[HTML][HTML] Snowmass2021 theory frontier white paper: Astrophysical and cosmological probes of dark matter
While astrophysical and cosmological probes provide a remarkably precise and consistent
picture of the quantity and general properties of dark matter, its fundamental nature remains …
picture of the quantity and general properties of dark matter, its fundamental nature remains …
21cmFAST v3: A Python-integrated C code forgenerating 3D realizations of the cosmic 21cm signal
This brief code paper presents a new Python-wrapped version of the popular 21cm
cosmology simulator, 21cmFAST. The new version, v3+, maintains the same core …
cosmology simulator, 21cmFAST. The new version, v3+, maintains the same core …
The redshifted 21 cm signal in the EDGES low-band spectrum
The EDGES collaboration reported an unexpectedly deep absorption in the radio
background at 78 MHz and interpreted the dip as the first detection of a redshifted 21 cm …
background at 78 MHz and interpreted the dip as the first detection of a redshifted 21 cm …
Tighter limits on dark matter explanations of the anomalous EDGES 21 cm signal
We investigate the hypothesis that Coulomb-type interactions between dark matter (DM) and
baryons explain the anomalously low 21 cm brightness-temperature minimum at redshift z∼ …
baryons explain the anomalously low 21 cm brightness-temperature minimum at redshift z∼ …
Sensitivities on nonspinning and spinning primordial black hole dark matter with global 21-cm troughs
AK Saha, R Laha - Physical Review D, 2022 - APS
Detection of the global 21 cm signal arising from neutral hydrogen can revolutionize our
understanding of the standard evolution of the Universe after recombination. In addition, it …
understanding of the standard evolution of the Universe after recombination. In addition, it …