Nobutoshi Yasutake

Hyperon mixing and universal many-body repulsion in neutron stars

A multi-Pomeron exchange potential (MPP) is proposed as a model for the universal many-body repulsion in baryonic systems on the basis of the extended soft core (ESC) baryon-baryon interaction. The strength of the MPP is determined by analyzing the nucleus-nucleus scattering with the

Finite-size effects at the hadron-quark transition and heavy hybrid stars

G

Multi-Pomeron repulsion and the neutron-star mass

-matrix folding model. The interaction in

Signatures of hadron-quark mixed phase in gravitational waves

\ensuremath{\Lambda}N

Hyperon-mixed neutron star with universal many-body repulsion

channels is shown to reproduce well the experimental

Asymmetric neutrino emission from magnetized proto-neutron star matter including hyperons in relativistic mean field theory

\ensuremath{\Lambda}

Lepton effects on the protoneutron stars with the hadron-quark mixed phase in the Nambu-Jona-Lasinio model

binding energies. The equation of state (EoS) in neutron matter with hyperon mixing is obtained including the MPP contribution, and mass-radius relations of neutron stars are derived. It is shown that the maximum mass can be larger than the observed one,

Rapid spin deceleration of magnetized protoneutron stars via asymmetric neutrino emission

2{M}_{\ensuremath{\bigodot}}

Relativistic hybrid stars with super-strong toroidal magnetic fields: An evolutionary track with QCD phase transition

, even in the case of including hyperon mixing on the basis of model parameters determined by terrestrial experiments.

Hot hadron-quark mixed phase including hyperons

We study the role of finite-size effects at the hadron-quark phase transition in a new hybrid equation of state constructed from an ab initio Bruckner