Properties of neutron stars with hyperons within a generalized relativistic approach
nucl-th, astro-ph.HE
Submitted: 2025-10-01
Updated: 2026-09-09
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Do hyperons exist in the interior of neutron stars ?
- Strangeness in Nuclei and Neutron Stars
- Neutron Stars and the Nuclear Equation of State
- Hyper-neutron stars from an ab initio calculation
- Shapiro delay measurement of a two solar mass neutron star
- The NANOGrav Nine-year Data Set: Mass and Geometric Measurements of Binary Millisecond Pulsars
- The NANOGrav 11-year Data Set: High-precision timing of 45 Millisecond Pulsars
- A Massive Pulsar in a Compact Relativistic Binary
- Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar
- Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GW170817: Measurements of Neutron Star Radii and Equation of State
- Properties of the binary neutron star merger GW170817
- Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models using Astrophysical Measurements
- Multi-physics constraints at different densities to probe nuclear symmetry energy in hyperonic neutron stars
- Bayesian inference of signatures of hyperons inside neutron stars
- A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
- PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
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