Results 91 to 100 of about 129,239 (245)
Neutron-Star Radius from a Population of Binary Neutron Star Mergers [PDF]
Physical Review Letters, 2018 9 pages and 7 ...
Bose, Sukanta +4 more
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Bound Debris Expulsion from Neutron Star Merger Remnants
The Astrophysical Journal, 2023 Many studies have found that neutron star mergers leave a fraction of the stars’ mass in bound orbits surrounding the resulting massive neutron star or black hole. This mass is a site of r -process nucleosynthesis and can generate a wind that contributes
Yossef Zenati +6 more
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, 2007 We study the effect of the neutron star spin -- kick velocity alignment observed in young radio pulsars on the coalescence rate of binary neutron stars. Two scenarios of the neutron star formation are considered: when the kick is always present and when ...
A. G. Kuranov +9 more
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The Oblate Schwarzschild Approximation for Light Curves of Rapidly Rotating Neutron Stars [PDF]
, 2007 We present a simple method for including the oblateness of a rapidly rotating neutron star when fitting X-ray light curves. In previous work we showed that the oblateness induced by rotation at frequencies above 300 Hz produces a geometric effect which ...
Braga, John +3 more
core +2 more sources
European Physical Journal C: Particles and FieldsRecent discovery of a compact binary coalescence through GW230529 by LIGO has indicated the merger event of a compact object of mass between $$2.5{-}4.5~M_{\odot }$$ 2.5 - 4.5 M ⊙ with a neutron star of mass between $$1.2{-}2.0~M_{\odot }$$ 1.2 - 2.0 M ⊙
Mayukh Bandyopadhyay
doaj +1 more source
, 2007 We use a post-Newtonian diagnostic tool to examine numerically generated quasiequilibrium initial data sets for non-spinning double neutron star and neutron star-black hole binary systems.
Clifford M. Will +6 more
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On the masses of neutron stars
Astronomy & Astrophysics, 1995 5 pages of compressed, uuencoded postscript (text+figure). Accepted for publication in A&A.
van Kerkwijk, M.H. +2 more
openaire +4 more sources
Role of strangeness to the neutron star mass and cooling
EPJ Web of Conferences, 2018 Neutron star provides unique environments for the investigation of the physics of extreme dense matter beyond normal nuclear saturation density. In such high density environments, hadrons with strange quarks are expected to play very important role in ...
Lee Chang-Hwan +3 more
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Constraints on Microscopic and Phenomenological Equations of State of Dense Matter from GW170817
Universe, 2019 We discuss the constraints on the equation of state (EOS) of neutron star matter obtained by the data analysis of the neutron star-neutron star merger in the event GW170807.
Domenico Logoteta, Ignazio Bombaci
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Constraints on the Symmetry Energy Using the Mass-Radius Relation of Neutron Stars
, 2014 The nuclear symmetry energy is intimately connected with nuclear astrophysics. This contribution focuses on the estimation of the symmetry energy from experiment and how it is related to the structure of neutron stars.
Lattimer, James M., Steiner, Andrew W.
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