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.
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Research Article| July 17 2019
Observability of sharp phase transitions in neutron stars
AIP Conf. Proc. 2127, 020006 (2019)
Sophia Han; Observability of sharp phase transitions in neutron stars. AIP Conf. Proc. 17 July 2019; 2127 (1): 020006. https://doi.org/10.1063/1.5117796
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