2025/02/20 by Hui Tong, Serdar Elhatisari, Tong, Hui +3 · 4 citations
Engineering · Physics and Astronomy · #FOS: Physical sciences #Geophysics and Sensor Technology #Nuclear Theory (nucl-th) #Pulsars and Gravitational Waves Research
paper · doi:10.48550/arxiv.2502.14435
openalex publication_date 2025/02/20 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The equation of state (EoS) of neutron matter plays a decisive role to understand the neutron star properties and the gravitational waves from neutron star mergers. At sufficient densities, the appearance of hyperons generally softens the EoS, leading to a reduction in the maximum mass of neutron stars well below the observed values of about 2 solar masses. Even though repulsive three-body forces are known to solve this so-called ``hyperon puzzle'', so far performing ab initio calculations with a substantial number of hyperons for neutron star properties has remained elusive. Starting from the newly developed auxiliary field quantum Monte Carlo algorithm to simulate hyper-neutron matter (HNM) without any sign oscillations, we derive three distinct EoSs by employing the state-of-the-art Nuclear Lattice Effective Field Theory. We include NΛ, ΛΛ two-body forces, NNΛ, and NΛΛ three-body forces. Consequently, we determine essential astrophysical quantities such as the neutron star mass, radius, tidal deformability, and the universal I-Love-Q relation. The maximum mass, radius and tidal deformability of a 1.4M_\odot neutron star are predicted to be 2.17(1)(1)~M_\odot, R1.4M\odot=13.10(1)(7)~km, and Λ1.4M_\odot=597(5)(18), respectively, based on our most realistic EoS. These predictions are in good agreement with the latest astrophysical constraints derived from observations of massive neutron stars, gravitational waves, and joint mass-radius measurements. Also, for the first time in ab initio calculations, we investigate both non-rotating and rotating neutron star configurations. The results indicate that the impact of rotational dynamics on the maximum mass is small, regardless of whether hyperons are present in the EoS or not.