[HTML][HTML] 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 …
[HTML][HTML] Cosmology with the laser interferometer space antenna
Abstract The Laser Interferometer Space Antenna (LISA) has two scientific objectives of
cosmological focus: to probe the expansion rate of the universe, and to understand …
cosmological focus: to probe the expansion rate of the universe, and to understand …
[HTML][HTML] The NANOGrav 15 yr data set: Constraints on supermassive black hole binaries from the gravitational-wave background
G Agazie, A Anumarlapudi, AM Archibald… - The Astrophysical …, 2023 - iopscience.iop.org
The NANOGrav 15 yr data set shows evidence for the presence of a low-frequency
gravitational-wave background (GWB). While many physical processes can source such low …
gravitational-wave background (GWB). While many physical processes can source such low …
[HTML][HTML] New horizons for fundamental physics with LISA
KG Arun, E Belgacem, R Benkel, L Bernard… - Living Reviews in …, 2022 - Springer
Abstract The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders
about the fundamental theory of nature at play in the extreme gravity regime, where the …
about the fundamental theory of nature at play in the extreme gravity regime, where the …
Gravitational waves from extreme-mass-ratio systems in astrophysical environments
We establish a generic, fully relativistic formalism to study gravitational-wave emission by
extreme-mass-ratio systems in spherically symmetric, nonvacuum black hole spacetimes …
extreme-mass-ratio systems in spherically symmetric, nonvacuum black hole spacetimes …
Gravitational waveforms for compact binaries from second-order self-force theory
We produce gravitational waveforms for nonspinning compact binaries undergoing a
quasicircular inspiral. Our approach is based on a two-timescale expansion of the Einstein …
quasicircular inspiral. Our approach is based on a two-timescale expansion of the Einstein …
[HTML][HTML] UNCOVER Spectroscopy Confirms the Surprising Ubiquity of Active Galactic Nuclei in Red Sources at z> 5
JE Greene, I Labbe, AD Goulding… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract The James Webb Space Telescope is revealing a new population of dust-reddened
broad-line active galactic nuclei (AGN) at redshifts z≳ 5. Here we present deep …
broad-line active galactic nuclei (AGN) at redshifts z≳ 5. Here we present deep …
Quasi-periodic eruptions from impacts between the secondary and a rigidly precessing accretion disc in an extreme mass-ratio inspiral system
A Franchini, M Bonetti, A Lupi, G Miniutti… - Astronomy & …, 2023 - aanda.org
X-ray quasi-periodic eruptions (QPEs) represent a recently discovered example of extreme
X-ray variability associated with supermassive black holes. These are high-amplitude bursts …
X-ray variability associated with supermassive black holes. These are high-amplitude bursts …
Probing accretion physics with gravitational waves
Gravitational-wave observations of extreme mass ratio inspirals (EMRIs) offer the
opportunity to probe the environments of active galactic nuclei (AGN) through the torques …
opportunity to probe the environments of active galactic nuclei (AGN) through the torques …
Observing GW190521-like binary black holes and their environment with LISA
Binaries of relatively massive black holes like GW190521 have been proposed to form in
dense gas environments, such as the disks of active galactic nuclei (AGNs), and they might …
dense gas environments, such as the disks of active galactic nuclei (AGNs), and they might …