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Paper detail

Unified description of dense matter in neutron stars and magnetars

We have recently developed a set of equations of state based on the nuclear energy density functional theory providing a unified description of the different regions constituting the interior of neutron stars and magnetars. The nuclear functionals, which were constructed from generalized Skyrme effective nucleon-nucleon interactions, yield not only an excellent fit to essentially all experimental atomic mass data but were also constrained to reproduce the neutron-matter equation of state as obtained from realistic many-body calculations.

preprint2013arXivOpen access
N. ChamelR. L. PavlovL. M. MihailovCh. J. VelchevZh. K. StoyanovY. D. MutafchievaM. D. IvanovichA. F. FantinaJ. M. PearsonS. Goriely
astro-ph.HEnucl-th
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Open access10 authors2 topics
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N. ChamelR. L. PavlovL. M. MihailovCh. J. VelchevZh. K. StoyanovY. D. MutafchievaM. D. IvanovichA. F. FantinaJ. M. PearsonS. Goriely

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