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We develop a new equation of state (EoS) table involving thermal (anti)kaons,Bose-Einstein condensate of $K^{-}$ mesons and $\Lambda$-hyperons forcore-collapse supernova and neutron star merger simulations. This EoS table isbased on a finite temperature density-dependent relativistic hadron fieldtheory where baryon-baryon interaction is mediated by scalar $\sigma$, vector$\omega$ and $\rho$ mesons, using the parameter set DD2 for nucleons. Therepulsive hyperon-hyperon interaction is mediated by an additional strange$\phi$ meson. The EoS for the $K^-$ condensed matter is also calculated withinthe framework of relativistic mean field model, whereas the low-density,inhomogeneous matter is calculated in the extended Nuclear StatisticalEquilibrium model (NSE). The EoS table is generated for a wide range of valuesof three parameters - baryon density ($10^{-12}$ to $\sim$ 1 fm$^{-3}$),positive charge fraction(0.01 to 0.60) and temperature(0.1 to 158.48 MeV).

Equation of State table with hyperon and antikaon for supernova and neutron star merger