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The equation of state (EOS) of neutron-rich nuclear matter is not only important for nuclear physics but also crucial for many phenomena and processes in astrophysics and cosmology (Refs. [1, 2]) for a recent review. Heavy-ion reactions induced by neu-
The equation of state (EOS) of neutron-rich nuclear matter is not only important for nuclear physics but also crucial for many phenomena and processes in astrophysics and cosmology (Refs. [1, 2]) for a recent review. Heavy-ion reactions induced by neu-