Speaker
Description
We construct the equation of state of hypernuclear matter and study the structure of neutron stars employing
a chiral hyperon-nucleon interaction of the Julich–Bonn group tuned to femtoscopic ¨ Λp data of the ALICE Collaboration, and ΛΛ and ΞN interactions determined from lattice QCD calculations by the HAL QCD Collaboration that
reproduce the femtoscopic ΛΛ and Ξ
− p data. We employ the ab-initio microscopic Brueckner–Hartree–Fock theory
extended to the strange baryon sector. A special focus is put on the uncertainties of the hyperon interactions and how
they are effectively propagated to the composition, equation of state, mass-radius relation and tidal deformability of
neutron stars. To such end, we consider the uncertainty due to the experimental error of the femtoscopic Λp data used
to fix the chiral hyperon-nucleon interaction and the theoretical uncertainty, estimated from the residual cut-off dependence of this interaction. We find that the final maximum mass of a neutron star with hyperons is in the range 1.3 − 1.4
M⊙, in agreement with previous works. The hyperon puzzle, therefore, remains still an open issue if only two-body
hyperon-nucleon and hyperon-hyperon interactions are considered. Predictions for the tidal deformability of neutron
stars with hyperons are found to be in agreement with the observational constraints from the gravitational wave event
GW170817 in the mass range 1.1 − 1.3 M⊙.
