Results 111 to 120 of about 129,239 (245)
Detecting the Hadron-Quark Phase Transition with Gravitational Waves
Universe, 2019 The long-awaited detection of a gravitational wave from the merger of a binary neutron star in August 2017 (GW170817) marks the beginning of the new field of multi-messenger gravitational wave astronomy.
Matthias Hanauske +9 more
doaj +1 more source
Zeitschrift f�r Physik A Atomic Nuclei, 1987 Generalized beta equilibrium involving nucleons, hyperons and isobars is examined for neutron star matter. The hyperons produce a considerable softening of the equation of state. It is shown that the observed masses of neutron stars can be used to settle a recent controversy concerning the nuclear compressibility.
openaire +2 more sources
The Black Hole Remnant of Black Hole-Neutron Star Coalescing Binaries
, 2013 We present a model for determining the dimensionless spin parameter and mass of the black hole remnant of black hole-neutron star mergers with parallel orbital angular momentum and initial black hole spin.
Pannarale, Francesco
core +2 more sources
NEUTRON RICH NUCLEI AND NEUTRON STARS [PDF]
Fission and Properties of Neutron-Rich Nuclei, 2013 The PREX experiment at Jefferson Laboratory measures the neutron radius of 208Pb with parity violating electron scattering in a way that is free from most strong interaction uncertainties. The 208Pb radius has important implications for neutron rich matter and the structure of neutron stars.
openaire +2 more sources
Band structure effects for dripped neutrons in neutron star crust
, 2004 The outer layers of a neutron star are supposed to be formed of a solid Coulomb lattice of neutron rich nuclei. At densities above neutron drip density (about one thousandth of nuclear saturation density), this lattice is immersed in a neutron fluid ...
Andreev +36 more
core +2 more sources
, 2012 6 pages, invited review, to appear in the proceedings of the ERPM conference, Zielona Gora, April ...
openaire +3 more sources
Properties and Dynamics of Neutron Stars and Proto-Neutron Stars
Universe, 2022 This Special Issue provides a comprehensive collection of papers that present modern theories to describe neutron star interiors and dynamics [...]
openaire +2 more sources
Ways to constrain neutron star equation of state models using relativistic disc lines
, 2011 Relativistic spectral lines from the accretion disc of a neutron star low-mass X-ray binary can be modelled to infer the disc inner edge radius. A small value of this radius tentatively implies that the disc terminates either at the neutron star hard ...
Akmal +45 more
core +1 more source
SOFT GAMMA REPEATERS AND ANOMALOUS X-RAY PULSARS BEYOND MAGNETARS
Odessa Astronomical Publications, 2016 The observational properties of Soft Gamma Repeaters and Anomalous X-ray Pulsars (SGR/AXP) indicate to necessity of the energy source different from a rotational energy of a neutron star.
G. S. Bisnovatyi-Kogan
doaj +1 more source
Hadron Masses in Medium and Neutron Star Properties
, 2005 We investigate the properties of the neutron star with relativistic mean field models. We incorporate in the quantum hadrodynamics and in the quark-meson coupling models a possible reduction of meson masses in nuclear matter.
Agakichiev +20 more
core +1 more source