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      Transport properties of isospin asymmetric nuclear matter using the time-dependent Hartree-Fock method

      , ,
      Physical Review C
      American Physical Society (APS)

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          Most cited references92

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          The mean-field theory of nuclear structure and dynamics

          J. Negele (1982)
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            Is Open Access

            Determination of the Equation of State of Dense Matter

            , , (2002)
            Nuclear collisions can compress nuclear matter to densities achieved within neutron stars and within core-collapse supernovae. These dense states of matter exist momentarily before expanding. We analyzed the flow of matter to extract pressures in excess of 10^34 pascals, the highest recorded under laboratory-controlled conditions. Using these analyses, we rule out strongly repulsive nuclear equations of state from relativistic mean field theory and weakly repulsive equations of state with phase transitions at densities less than three times that of stable nuclei, but not equations of state softened at higher densities because of a transformation to quark matter.
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              Physics of Neutron Star Crusts

              The physics of neutron star crusts is vast, involving many different research fields, from nuclear and condensed matter physics to general relativity. This review summarizes the progress, which has been achieved over the last few years, in modeling neutron star crusts, both at the microscopic and macroscopic levels. The confrontation of these theoretical models with observations is also briefly discussed.
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                Author and article information

                Journal
                PRVCAN
                Physical Review C
                Phys. Rev. C
                American Physical Society (APS)
                2469-9985
                2469-9993
                August 2017
                August 30 2017
                : 96
                : 2
                Article
                10.1103/PhysRevC.96.024625
                37291b77-050d-4a4d-9064-a908f959f657
                © 2017

                https://link.aps.org/licenses/aps-default-license

                https://link.aps.org/licenses/aps-default-accepted-manuscript-license

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