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Phenomenological quark-hadron equations of state with first-order phase transitions for astrophysical applications
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Phenomenological quark-hadron equations of state with first-order phase transitions for astrophysical applications
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In the current work an equation of state model with a first-order phase transition for astrophysical applications is presented. The model is based on a two-phase approach for quark-hadron phase transitions, which leads by construction to a first-order phase transition. The resulting model has already been successfully used in several astrophysical applications, such as cold neutron stars, core-collapse supernova explosions and binary neutron star mergers. Main goal of this work is to present the details of the model, discuss certain features and eventually publish it in a tabulated form for further use.
Forward citations
Cited by 2 Pith papers
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Strongly interacting matter with criticality induced by modified excluded volume in core-collapse supernova simulations
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$\Lambda$ hyperons in core-collapse supernovae: Equilibration and neutrino opacities
Lambda hyperons equilibrate rapidly in post-collapse proto-neutron stars through nonleptonic NN to N Lambda processes and enhance low-energy muon neutrino opacities beyond nucleonic contributions.
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