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 …
Challenges for ΛCDM: An update
L Perivolaropoulos, F Skara - New Astronomy Reviews, 2022 - Elsevier
A number of challenges to the standard Λ CDM model have been emerging during the past
few years as the accuracy of cosmological observations improves. In this review we discuss …
few years as the accuracy of cosmological observations improves. In this review we discuss …
A long time ago in a galaxy far, far away: A candidate z∼ 12 galaxy in early JWST CEERS imaging
We report the discovery of a candidate galaxy with a photo-z of z∼ 12 in the first epoch of
the James Webb Space Telescope (JWST) Cosmic Evolution Early Release Science …
the James Webb Space Telescope (JWST) Cosmic Evolution Early Release Science …
[HTML][HTML] The forward physics facility at the high-luminosity LHC
High energy collisions at the High-Luminosity Large Hadron Collider (LHC) produce a large
number of particles along the beam collision axis, outside of the acceptance of existing LHC …
number of particles along the beam collision axis, outside of the acceptance of existing LHC …
Primordial black holes
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Journals & Books Search RegisterSign in View PDF Download full book Search ScienceDirect …
Journals & Books Search RegisterSign in View PDF Download full book Search ScienceDirect …
[HTML][HTML] Observational evidence for primordial black holes: A positivist perspective
BJ Carr, S Clesse, J Garcia-Bellido, MRS Hawkins… - Physics Reports, 2024 - Elsevier
We review numerous arguments for primordial black holes (PBHs) based on observational
evidence from a variety of lensing, dynamical, accretion and gravitational-wave effects. This …
evidence from a variety of lensing, dynamical, accretion and gravitational-wave effects. This …
On the detection of a cosmic dawn signal in the radio background
The astrophysics of the cosmic dawn, when star formation commenced in the first collapsed
objects, is predicted to be revealed by spectral and spatial signatures in the cosmic radio …
objects, is predicted to be revealed by spectral and spatial signatures in the cosmic radio …
[HTML][HTML] Feebly-interacting particles: FIPs 2020 workshop report
With the establishment and maturation of the experimental programs searching for new
physics with sizeable couplings at the LHC, there is an increasing interest in the broader …
physics with sizeable couplings at the LHC, there is an increasing interest in the broader …
The forward physics facility: sites, experiments, and physics potential
LA Anchordoqui, A Ariga, T Ariga, W Bai, K Balazs… - Physics reports, 2022 - Elsevier
Abstract The Forward Physics Facility (FPF) is a proposal to create a cavern with the space
and infrastructure to support a suite of far-forward experiments at the Large Hadron Collider …
and infrastructure to support a suite of far-forward experiments at the Large Hadron Collider …
Wave dark matter
L Hui - Annual Review of Astronomy and Astrophysics, 2021 - annualreviews.org
We review the physics and phenomenology of wave dark matter: a bosonic dark matter
candidate lighter than about 30 eV. Such particles have a de Broglie wavelength exceeding …
candidate lighter than about 30 eV. Such particles have a de Broglie wavelength exceeding …