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Cited article:

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The Boltzmann-radiation-hydrodynamics Simulations of Core-collapse Supernovae with Different Equations of State: The Role of Nuclear Composition and the Behavior of Neutrinos

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Asymmetric nuclear light clusters in supernova matter

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Influence of Density Dependence of Symmetry Energy in Hot and Dense Matter for Supernova Simulations

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Comparing Treatments of Weak Reactions with Nuclei in Simulations of Core-collapse Supernovae

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Radiation-Hydrodynamic Simulations of Core-collapse Supernovae with 6 Dimensional Boltzmann Neutrino Transport

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Towards a Unified Quark-Hadron-Matter Equation of State for Applications in Astrophysics and Heavy-Ion Collisions

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Composition of Nuclear Matter with Light Clusters and Bose–Einstein Condensation of $$\alpha $$ α Particles

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The State of Matter in Simulations of Core-Collapse supernovae—Reflections and Recent Developments

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