Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/99900
Title: From the crust to the core of neutron stars on a microscopic basis
Author: Baldo, M.
Burgio, G. F.
Centelles Aixalà, Mario
Sharma, B. K.
Viñas Gausí, Xavier
Keywords: Estels de neutrons
Astrofísica
Física nuclear
Neutron stars
Astrophysics
Nuclear physics
Issue Date: 2014
Publisher: Pleiades Publishing
Abstract: Within a microscopic approach the structure of Neutron Stars is usually studied by modelling the homogeneous nuclear matter of the core by a suitable Equation of State, based on a many-body theory, and the crust by a functional based on a more phenomenological approach. We present the first calculation of Neutron Star overall structure by adopting for the core an Equation of State derived from the Brueckner-Hartree-Fock theory and for the crust, including the pasta phase, an Energy Density Functional based on the same Equation of State, and which is able to describe accurately the binding energy of nuclei throughout the mass table. Comparison with other approaches is discussed. The relevance of the crust Equation of state for the Neutron Star radius is particularly emphasised.
Note: Versió postprint del document publicat a: http://dx.doi.org/10.1134/S1063778814080031
It is part of: Physics of Atomic Nuclei, 2014, vol. 77, num. 9, p. 1157-1165
Related resource: http://dx.doi.org/10.1134/S1063778814080031
URI: http://hdl.handle.net/2445/99900
ISSN: 1063-7788
Appears in Collections:Articles publicats en revistes (Física Quàntica i Astrofísica)

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