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 …

Quiescent and active galactic nuclei as factories of merging compact objects in the era of gravitational wave astronomy

M Arca Sedda, S Naoz, B Kocsis - Universe, 2023 - mdpi.com
Galactic nuclei harbouring a central supermassive black hole (SMBH), possibly surrounded
by a dense nuclear cluster (NC), represent extreme environments that house a complex …

Formation and evolution of compact-object binaries in AGN disks

H Tagawa, Z Haiman, B Kocsis - The Astrophysical Journal, 2020 - iopscience.iop.org
The astrophysical origin of gravitational wave (GW) events discovered by LIGO/VIRGO
remains an outstanding puzzle. In active galactic nuclei (AGNs), compact-object binaries …

Hints for a turnover at the snow line in the giant planet occurrence rate

RB Fernandes, GD Mulders, I Pascucci… - The Astrophysical …, 2019 - iopscience.iop.org
The orbital distribution of giant planets is crucial for understanding how terrestrial planets
form and predicting yields of exoplanet surveys. Here, we derive giant planets occurrence …

Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets

J Drazkowska, B Bitsch, M Lambrechts… - arXiv preprint arXiv …, 2022 - arxiv.org
Our understanding of planet formation has been rapidly evolving in recent years. The
classical planet formation theory, developed when the only known planetary system was our …

The New Generation Planetary Population Synthesis (NGPPS)-I. Bern global model of planet formation and evolution, model tests, and emerging planetary systems

A Emsenhuber, C Mordasini, R Burn, Y Alibert… - Astronomy & …, 2021 - aanda.org
Context. The explosion of observational data on exoplanets gives many constraints on
theoretical models of planet formation and evolution. Observational data probe very large …

Formation of planetary systems by pebble accretion and migration-How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

M Lambrechts, A Morbidelli, SA Jacobson… - Astronomy & …, 2019 - aanda.org
Super-Earths–planets with sizes between the Earth and Neptune–are found in tighter orbits
than that of the Earth around more than one third of main sequence stars. It has been …

Probing accretion physics with gravitational waves

L Speri, A Antonelli, L Sberna, S Babak, E Barausse… - Physical Review X, 2023 - APS
Gravitational-wave observations of extreme mass ratio inspirals (EMRIs) offer the
opportunity to probe the environments of active galactic nuclei (AGN) through the torques …

[图书][B] Astrophysics of planet formation

PJ Armitage - 2020 - books.google.com
" The study of planet formation has a long history. The idea that the Solar System formed
from a rotating disk of gas and dust-the Nebula Hypothesis-dates back to the writings of …

Formation of planetary systems by pebble accretion and migration: growth of gas giants

B Bitsch, A Izidoro, A Johansen, SN Raymond… - Astronomy & …, 2019 - aanda.org
Giant planets migrate though the protoplanetary disc as they grow their solid core and attract
their gaseous envelope. Previously, we have studied the growth and migration of an isolated …