Hyperon–nucleon three-body forces and strangeness in neutron stars
Three-body forces acting on a $$\varLambda $$ Λ hyperon in a nuclear medium are investigated, with special focus on the so-called hyperon puzzle in neutron stars. The hyperon–nucleon two-body interaction deduced from SU(3) chiral effective field theory is employed at next-to-leading order. Hyperon–nucleon three-body forces are approximated using saturation by decuplet baryons and are transcribed to density-dependent effective two-body interactions. These together are taken as input in a Brueckner–Bethe–Goldstone equation with explicit treatment of the $$\varLambda N\leftrightarrow \varSigma N$$ Λ N ↔ Σ N and $$\varLambda NN\leftrightarrow \varSigma NN$$ Λ N N ↔ Σ N N coupled channels. Single-particle potentials of a $$\varLambda $$ Λ hyperon in symmetric nuclear matter and neutron matter are calculated. With parameters of the $$\varLambda NN$$ Λ N N three-body force constrained by hypernuclear phenomenology, extrapolations to high baryon density are performed. By comparison of the $$\varLambda $$ Λ and neutron chemical potentials at densities characteristic of the core of neutron stars it is found that the combined repulsive effects of two- and three-body correlations can make the appearance of $$\varLambda $$ Λ hyperons in neutron stars energetically unfavourable, thus potentially offering a possible answer to a longstanding query.