The book starts with stellar evolution and essential nuclear physics, gradually building to the complexities of the neutron star core. It presents the subject in three parts: the theoretical framework, observational constraints from X-ray telescopes and gravitational waves, and the implications of various EoS models on astrophysical phenomena like pulsar glitches. By integrating theoretical developments with cutting-edge observational data, Neutron Star Core provides a comprehensive overview for advanced students and researchers, fostering a critical understanding of these cosmic enigmas.
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