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arXiv · 1301.2438

Unified description of dense matter in neutron stars and magnetars

N. Chamel·R. L. Pavlov·L. M. Mihailov·Ch. J. Velchev·Zh. K. Stoyanov·Y. D. Mutafchieva·M. D. Ivanovich·A. F. Fantina·J. M. Pearson·S. Goriely
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Abstract

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.

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N. Chamel, R. L. Pavlov, L. M. Mihailov, Ch. J. Velchev, Zh. K. Stoyanov, Y. D. Mutafchieva, M. D. Ivanovich, A. F. Fantina, J. M. Pearson, S. Goriely. 2013-01-11. Unified description of dense matter in neutron stars and magnetars. https://doi.org/10.1017/s1743921312024118

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