Thermal Stiffness of Warm Nuclear-Matter and Super-Nova Explosions by Shock Heating

Physical review letters（1980）

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摘要

The thermal stiffness derived from a realistic equation of state lies just in the range necessary for mass ejection in the collapse of the cores of heavy stars.Received 9 January 1980DOI:https://doi.org/10.1103/PhysRevLett.44.832©1980 American Physical Society

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