Neutron star merger remnants
S Bernuzzi - General Relativity and Gravitation, 2020 - Springer
Binary neutron star mergers observations are a unique way to constrain fundamental
physics and astrophysics at the extreme. The interpretation of gravitational-wave events and …
physics and astrophysics at the extreme. The interpretation of gravitational-wave events and …
Black-hole binaries, gravitational waves, and numerical relativity
J Centrella, JG Baker, BJ Kelly, JR van Meter - Reviews of Modern Physics, 2010 - APS
Understanding the predictions of general relativity for the dynamical interactions of two black
holes has been a long-standing unsolved problem in theoretical physics. Black-hole …
holes has been a long-standing unsolved problem in theoretical physics. Black-hole …
Binary neutron star mergers: mass ejection, electromagnetic counterparts, and nucleosynthesis
D Radice, A Perego, K Hotokezaka… - The Astrophysical …, 2018 - iopscience.iop.org
We present a systematic numerical relativity study of the mass ejection and the associated
electromagnetic transients and nucleosynthesis from binary neutron star (NS) mergers. We …
electromagnetic transients and nucleosynthesis from binary neutron star (NS) mergers. We …
The SXS Collaboration catalog of binary black hole simulations
Accurate models of gravitational waves from merging black holes are necessary for
detectors to observe as many events as possible while extracting the maximum science …
detectors to observe as many events as possible while extracting the maximum science …
Improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
We improve the accuracy of the effective-one-body (EOB) waveforms that were employed
during the first observing run of Advanced LIGO for binaries of spinning, nonprecessing …
during the first observing run of Advanced LIGO for binaries of spinning, nonprecessing …
Setting the cornerstone for a family of models for gravitational waves from compact binaries: The dominant harmonic for nonprecessing quasicircular black holes
In this paper we present imrphenomxas, a thorough overhaul of the imrphenomd [S. Husa,
Phys. Rev. D 93, 044006 (2016) PRVDAQ 2470-0010 10.1103/PhysRevD. 93.044006; S …
Phys. Rev. D 93, 044006 (2016) PRVDAQ 2470-0010 10.1103/PhysRevD. 93.044006; S …
Numerical relativity simulations of the neutron star merger GW170817: long-term remnant evolutions, winds, remnant disks, and nucleosynthesis
V Nedora, S Bernuzzi, D Radice… - The Astrophysical …, 2021 - iopscience.iop.org
We present a systematic numerical relativity study of the dynamical ejecta, winds, and
nucleosynthesis in neutron star (NS) merger remnants. Binaries with the chirp mass …
nucleosynthesis in neutron star (NS) merger remnants. Binaries with the chirp mass …
Science with the space-based interferometer eLISA: Supermassive black hole binaries
We compare the science capabilities of different eLISA mission designs, including four-link
(two-arm) and six-link (three-arm) configurations with different arm lengths, low-frequency …
(two-arm) and six-link (three-arm) configurations with different arm lengths, low-frequency …
Strong-field scattering of two spinning black holes: Numerical relativity versus post-Minkowskian gravity
Highly accurate models of the gravitational wave signal from coalescing compact binaries
are built by completing analytical computations of the binary dynamics with nonperturbative …
are built by completing analytical computations of the binary dynamics with nonperturbative …
The Einstein Toolkit: a community computational infrastructure for relativistic astrophysics
Abstract We describe the Einstein Toolkit, a community-driven, freely accessible
computational infrastructure intended for use in numerical relativity, relativistic astrophysics …
computational infrastructure intended for use in numerical relativity, relativistic astrophysics …