Observability of Sharp Phase Transitions in Neutron Stars
© 2019 Author(s). With central densities as high as 5-10 times the nuclear saturation density, neutron stars exhibit extreme conditions that cannot be observed elsewhere. They are ideal astrophysical laboratories for probing the composition and properties of cold, ultra-dense matter. We shall discuss taking into account currently available data from observation, how to reveal possible sharp phase transitions in dense neutron star cores.
Han, Sophia, "Observability of Sharp Phase Transitions in Neutron Stars" (2019). Physics & Astronomy Open Access Publications. 139.