Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences
, 2021 We report the observation of gravitational waves from two compact binary coalescences in LIGO’s and Virgo’s third observing run with properties consistent with neutron star–black hole (NSBH) binaries.
The Ligo Scientific Collaboration +499 more
semanticscholar +1 more source
Experimental Challenge to Heavy Element Synthesis under Explosive Burning on Neutron Stars [PDF]
EPJ Web of Conferences, 2020 Binary stellar systems that involve a neutron star or two neutron stars make interesting phenomena, X-ray bursts and kilo-novae, respectively, which involve explosive burning either in the proton-rich environment or in the neutron-rich environment. These
Kubono Shigeru
doaj +1 more source
Nuclear Physics with Gravitational Waves from Neutron Stars Disrupted by Black Holes
The Astrophysical Journal Letters, 2023 Gravitational waves from neutron star–black hole (NSBH) mergers that undergo tidal disruption provide a potential avenue to study the equation of state of neutron stars and hence the behavior of matter at its most extreme densities.
Teagan A. Clarke +3 more
doaj +1 more source
Inferring the dense nuclear matter equation of state with neutron star tides [PDF]
EPJ Web of Conferences, 2022 During the late stages of a neutron star binary inspiral finite-size effects come into play, with the tidal deformability of the supranuclear density matter leaving an imprint on the gravitational-wave signal.
Pnigouras Pantelis +2 more
doaj +1 more source
PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter [PDF]
Astrophysical Journal, 2019 Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear physicists because their attributes can be used to determine the properties of the dense matter in their cores.
M. Miller +22 more
semanticscholar +1 more source
PROTO-NEUTRON AND NEUTRON STARS [PDF]
Astronomy and Relativistic Astrophysics, 2010 Prepared for International Workshop on Astronomy and Relativistic Astrophysics (IWARA 2007), Joao Pessoa, Brazil, 3-6 Oct ...
Horst Stoecker +2 more
openaire +3 more sources
Semi-empirical relation to understand matter properties at neutron star interiors
European Physical Journal C: Particles and Fields, 2022 The occurrence of quark matter at the center of neutron stars is still in debate. This study defines some semi-empirical parameters that try to quantify the presence and the amount of quark matter at star interiors.
Ritam Mallick +2 more
doaj +1 more source
Thermodynamics of Hot Neutron Stars and Universal Relations
Universe, 2022 Over the last few years, the detection of gravitational waves from binary neutron star systems has rekindled our hopes for a deeper understanding of the unknown nature of ultradense matter.
Pavlos Laskos-Patkos +3 more
doaj +1 more source
Neutron-star tidal deformability and equation-of-state constraints [PDF]
General Relativity and Gravitation, 2020 Despite their long history and astrophysical importance, some of the key properties of neutron stars are still uncertain. The extreme conditions encountered in their interiors, involving matter of uncertain composition at extreme density and isospin ...
K. Chatziioannou
semanticscholar +1 more source
Coalescence of black hole–neutron star binaries [PDF]
Living Reviews in Relativity, 2021 We review the current status of general relativistic studies for coalescences of black hole–neutron star binaries. First, high-precision computations of black hole–neutron star binaries in quasiequilibrium circular orbits are summarized, focusing on the ...
K. Kyutoku, M. Shibata, K. Taniguchi
semanticscholar +1 more source