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NSR database version of May 6, 2024.

Search: Author = M.Shelley

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2021SH16      Phys.Rev. C 103, 035807 (2021)

M.Shelley, A.Pastore

Systematic analysis of inner crust composition using the extended Thomas-Fermi approximation with pairing correlations

NUCLEAR STRUCTURE Z=16-60; calculated energy per particle, proton fraction, pressure in the inner crust of neutron stars. Used extended Thomas-Fermi method with shell (Strutinsky integral) and pairing corrections to calculate number of protons and equation of state (EoS), as a function of baryonic density, for Skyrme interactions with a range of pure neutron matter (PNM) properties.

doi: 10.1103/PhysRevC.103.035807
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2017PA23      J.Phys.(London) G44, 94003 (2017)

A.Pastore, M.Shelley, S.Baroni, C.A.Diget

A new statistical method for the structure of the inner crust of neutron stars

doi: 10.1088/1361-6471/aa8207
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