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Physical Environment of Accreting Neutron Stars
Published 2016-01-01“…Neutron stars (NSs) powered by accretion, which are known as accretion-powered NSs, always are located in binary systems and manifest themselves as X-ray sources. …”
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Analyzing the speed of sound in neutron star with machine learning
Published 2024-12-01“…It has a negative trough beyond the maximal central densities of neutron stars. The change in sign of the trace anomaly hints towards a near-conformal matter at the centre of neutron stars, which may not necessarily be conformal quark matter.…”
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Tidal Reconstruction of Neutron Star Mergers from Their Late Inspiral
Published 2025-01-01Subjects: Get full text
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GRB 130603B: No Compelling Evidence for Neutron Star Merger
Published 2015-01-01“…Moreover, SHB plus a kilonova can be produced also by the collapse of a compact star (neutron star, strange star, or quark star) to a more compact object due to cooling, loss of angular momentum, or mass accretion.…”
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Analysis of the Conformally Flat Approximation for Binary Neutron Star Initial Conditions
Published 2017-01-01“…The spatially conformally flat approximation (CFA) is a viable method to deduce initial conditions for the subsequent evolution of binary neutron stars employing the full Einstein equations. …”
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GR-Athena++: General-relativistic Magnetohydrodynamics Simulations of Neutron Star Spacetimes
Published 2025-01-01Subjects: Get full text
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Influence of Effective Nucleon Mass on Equation of State for Supernova Simulations and Neutron Stars
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Constraining the equation of state in neutron-star cores via the long-ringdown signal
Published 2025-02-01“…Abstract Multimessenger signals from binary neutron star (BNS) mergers are promising tools to infer the properties of nuclear matter at densities inaccessible to laboratory experiments. …”
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Neutron stars in extended scalar-Gauss–Bonnet gravity: the richness of the solution spectrum
Published 2024-12-01“…Abstract Neutron stars are natural laboratories for testing gravity in the strong field regime. …”
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Nucleonic Direct Urca Processes and Cooling of the Massive Neutron Star by Antikaon Condensations
Published 2020-01-01“…Nucleonic direct Urca processes and cooling of the massive neutron stars are studied by considering antikaon condensations. …”
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On Possible Reduction of Equilibrium Radius of a Neutron Star Influenced by Superstrong Magnetic Field
Published 2012-01-01“…Based on this, it is shown that, in superstrong magnetic field, equilibrium radius of a neutron star is approximately several times smaller than without the field influence. …”
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PSR J1947−1120: A New Huntsman Millisecond Pulsar Binary
Published 2025-01-01Subjects: “…Neutron stars…”
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Novel features of asymmetric nuclear matter from terrestrial experiments and astrophysical observations of neutron stars
Published 2025-02-01Subjects: Get full text
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Long-term Evolution of Sco X-1: Implications for the Current Spin Frequency and Ellipticity of the Neutron Star
Published 2025-01-01Subjects: Get full text
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Continuous Gravitational Waves from Thermal Mountains on Accreting Neutron Stars: Effect of the Nuclear Pasta Phase
Published 2025-01-01Subjects: “…Neutron stars…”
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X-ray pulsed light curves of highly compact neutron stars as probes of scalar–tensor theories of gravity
Published 2024-12-01“…Abstract The strong gravitational potential of neutron stars (NSs) makes them ideal astrophysical objects for testing extreme gravity phenomena. …”
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Intersections of ultracold atomic polarons and nuclear clusters: how is a chart of nuclides modified in dilute neutron matter?
Published 2024-02-01Subjects: Get full text
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Giant Hall Waves Launched by Superconducting Phase Transition in Pulsars
Published 2025-01-01Subjects: Get full text
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The Timing and Spectral Properties of the 2022 Outburst of SGR J1935+2154 Observed with NICER
Published 2025-01-01Subjects: “…Neutron stars…”
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A Universal Break in Energy Functions of Three Hyperactive Repeating Fast Radio Bursts
Published 2025-01-01Subjects: Get full text
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