Astrophysics with the laser interferometer space antenna
Abstract The Laser Interferometer Space Antenna (LISA) will be a transformative experiment
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
for gravitational wave astronomy, and, as such, it will offer unique opportunities to address …
The origins of massive black holes
M Volonteri, M Habouzit, M Colpi - Nature Reviews Physics, 2021 - nature.com
Massive black holes (MBHs) inhabit galactic centres, and power luminous quasars and
active galactic nuclei, sha** their cosmic environment with the energy they produce. The …
active galactic nuclei, sha** their cosmic environment with the energy they produce. The …
The NANOGrav 12.5 yr data set: search for an isotropic stochastic gravitational-wave background
Z Arzoumanian, PT Baker, H Blumer… - The Astrophysical …, 2020 - iopscience.iop.org
We search for an isotropic stochastic gravitational-wave background (GWB) in the 12.5 yr
pulsar-timing data set collected by the North American Nanohertz Observatory for …
pulsar-timing data set collected by the North American Nanohertz Observatory for …
Circumbinary accretion: From binary stars to massive binary black holes
We review recent works on the dynamics of circumbinary accretion, including time variability,
angular momentum transfer between the disk and the binary, and the secular evolution of …
angular momentum transfer between the disk and the binary, and the secular evolution of …
The NANOGrav 11-year data set: high-precision timing of 45 millisecond pulsars
Z Arzoumanian, A Brazier… - The Astrophysical …, 2018 - iopscience.iop.org
We present high-precision timing data over time spans of up to 11 years for 45 millisecond
pulsars observed as part of the North American Nanohertz Observatory for Gravitational …
pulsars observed as part of the North American Nanohertz Observatory for Gravitational …
Black holes, gravitational waves and fundamental physics: a roadmap
L Barack, V Cardoso, S Nissanke… - … and quantum gravity, 2019 - iopscience.iop.org
70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
Centre de Saclay, FR-91191 Gif-sur-Yvette, France
Orbital evolution of binaries in circumbinary discs
M Siwek, R Weinberger… - Monthly Notices of the …, 2023 - academic.oup.com
We present the to-date largest parameter space exploration of binaries in circumbinary discs
(CBDs), deriving orbital evolution prescriptions for eccentric, unequal mass binaries from our …
(CBDs), deriving orbital evolution prescriptions for eccentric, unequal mass binaries from our …
The MeerKAT pulsar timing array: First data release
We present the first 2.5 yr of data from the MeerKAT Pulsar Timing Array (MPTA), part of
MeerTime, a MeerKAT Large Survey Project. The MPTA aims to precisely measure pulse …
MeerTime, a MeerKAT Large Survey Project. The MPTA aims to precisely measure pulse …
Rapid and bright stellar-mass binary black hole mergers in active galactic nuclei
Abstract The Laser Interferometer Gravitational-wave Observatory (LIGO) found direct
evidence for double black hole binaries emitting gravitational waves. Galactic nuclei are …
evidence for double black hole binaries emitting gravitational waves. Galactic nuclei are …
Unveiling the gravitational universe at μ-Hz frequencies
We propose a space-based interferometer surveying the gravitational wave (GW) sky in the
milli-Hz to μ-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in …
milli-Hz to μ-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in …