A pedagogical extension of QHD mean-field neutron-star models to exotic particles, reporting that a scanned SU(3) parameter αV can give hyperonic maximum masses near 2.2 solar masses.
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An Undergraduate Approach to the Quantum Hadrodynamics and the Physics of Neutron Stars Part II: Neutron Stars' Exotic Content
A pedagogical extension of QHD mean-field neutron-star models to exotic particles, reporting that a scanned SU(3) parameter αV can give hyperonic maximum masses near 2.2 solar masses.