⚛️ nuclear theory
Hadron-quark phase transitions along proto-neutron-star evolution
This paper investigates the evolution of proto-hybrid stars by deriving hot hybrid equations of state under various charge conservation and neutrino trapping conditions, revealing that the early stages of a hybrid star's life critically influence its maximum gravitational mass in later stages.
Original paper licensed under CC BY 4.0 (http://creativecommons.org/licenses/by/4.0/). This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer
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