Astrophysics with the laser interferometer space antenna
P Amaro-Seoane, J Andrews, M Arca Sedda… - Living Reviews in …, 2023 - Springer
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 quest for dual and binary supermassive black holes: A multi-messenger view
A De Rosa, C Vignali, T Bogdanović, PR Capelo… - New Astronomy …, 2019 - Elsevier
The quest for binary and dual supermassive black holes (SMBHs) at the dawn of the multi-
messenger era is compelling. Detecting dual active galactic nuclei (AGN)–active SMBHs at …
messenger era is compelling. Detecting dual active galactic nuclei (AGN)–active SMBHs at …
The second data release from the European Pulsar Timing Array: V. Implications for massive black holes, dark matter and the early Universe
J Antoniadis, P Arumugam, S Arumugam… - arXiv preprint arXiv …, 2023 - arxiv.org
The European Pulsar Timing Array (EPTA) and Indian Pulsar Timing Array (InPTA)
collaborations have measured a low-frequency common signal in the combination of their …
collaborations have measured a low-frequency common signal in the combination of their …
Science with the space-based interferometer LISA. V. Extreme mass-ratio inspirals
The space-based Laser Interferometer Space Antenna (LISA) will be able to observe the
gravitational-wave signals from systems comprised of a massive black hole and a stellar …
gravitational-wave signals from systems comprised of a massive black hole and a stellar …
The second data release from the European Pulsar Timing Array-IV. Implications for massive black holes, dark matter, and the early Universe
J Antoniadis, P Arumugam, S Arumugam… - Astronomy & …, 2024 - aanda.org
The European Pulsar Timing Array (EPTA) and Indian Pulsar Timing Array (InPTA)
collaborations have measured a low-frequency common signal in the combination of their …
collaborations have measured a low-frequency common signal in the combination of their …
Post-Newtonian evolution of massive black hole triplets in galactic nuclei–IV. Implications for LISA
Coalescing massive black hole binaries (MBHBs) of, forming in the aftermath of galaxy
mergers, are primary targets of the space mission LISA, the Laser Interferometer Space …
mergers, are primary targets of the space mission LISA, the Laser Interferometer Space …
Massive binary black holes in galactic nuclei and their path to coalescence
M Colpi - Space Science Reviews, 2014 - Springer
Massive binary black holes (10 5 M⊙–10 9 M⊙) form at the centre of galaxies that
experience a merger episode. They are expected to coalesce into a larger black hole …
experience a merger episode. They are expected to coalesce into a larger black hole …
The final-parsec problem in the collisionless limit
E Vasiliev, F Antonini, D Merritt - The Astrophysical Journal, 2015 - iopscience.iop.org
ABSTRACT A binary supermassive black hole loses energy via ejection of stars in a galactic
nucleus, until emission of gravitational waves becomes strong enough to induce rapid …
nucleus, until emission of gravitational waves becomes strong enough to induce rapid …
Eccentricity evolution of massive black hole binaries from formation to coalescence
A Gualandris, FM Khan, E Bortolas… - Monthly Notices of …, 2022 - academic.oup.com
Coalescing supermassive black hole binaries (BHBs) are expected to be the loudest
sources of gravitational waves (GWs) in the Universe. Detection rates for ground or space …
sources of gravitational waves (GWs) in the Universe. Detection rates for ground or space …
Supermassive black hole binary evolution in axisymmetric galaxies: the final parsec problem is not a problem
FM Khan, K Holley-Bockelmann… - The Astrophysical …, 2013 - iopscience.iop.org
During a galaxy merger, the supermassive black hole (SMBH) in each galaxy is thought to
sink to the center of the potential and form an SMBH binary; this binary can eject stars via …
sink to the center of the potential and form an SMBH binary; this binary can eject stars via …