Equations of state for supernovae and compact stars
M Oertel, M Hempel, T Klähn, S Typel - Reviews of Modern Physics, 2017 - APS
A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …
Origin of the heaviest elements: The rapid neutron-capture process
JJ Cowan, C Sneden, JE Lawler, A Aprahamian… - Reviews of Modern …, 2021 - APS
The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …
A kilonova following a long-duration gamma-ray burst at 350 Mpc
Gamma-ray bursts (GRBs) are divided into two populations,; long GRBs that derive from the
core collapse of massive stars (for example, ref.) and short GRBs that form in the merger of …
core collapse of massive stars (for example, ref.) and short GRBs that form in the merger of …
GW170817: Measurements of neutron star radii and equation of state
BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley… - Physical review …, 2018 - APS
On 17 August 2017, the LIGO and Virgo observatories made the first direct detection of
gravitational waves from the coalescence of a neutron star binary system. The detection of …
gravitational waves from the coalescence of a neutron star binary system. The detection of …
Illuminating gravitational waves: A concordant picture of photons from a neutron star merger
Merging neutron stars offer an excellent laboratory for simultaneously studying strong-field
gravity and matter in extreme environments. We establish the physical association of an …
gravity and matter in extreme environments. We establish the physical association of an …
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
GW170817: joint constraint on the neutron star equation of state from multimessenger observations
Gravitational waves detected from the binary neutron star (NS) merger GW170817
constrained the NS equation of state by placing an upper bound on certain parameters …
constrained the NS equation of state by placing an upper bound on certain parameters …
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 …
Kilonovae
BD Metzger - Living reviews in relativity, 2017 - Springer
The mergers of double neutron star (NS–NS) and black hole (BH)–NS binaries are
promising gravitational wave (GW) sources for Advanced LIGO and future GW detectors. The …
promising gravitational wave (GW) sources for Advanced LIGO and future GW detectors. The …
GW170817, general relativistic magnetohydrodynamic simulations, and the neutron star maximum mass
Recent numerical simulations in general relativistic magnetohydrodynamics (GRMHD)
provide useful constraints for the interpretation of the GW170817 discovery. Combining the …
provide useful constraints for the interpretation of the GW170817 discovery. Combining the …