Finite size effects in neutron star and nuclear matter simulations

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In this work we study molecular dynamics simulations of symmetric nuclear and neutron star matter using a semi-classical nucleon interaction model. Our aim is to gain insight on the nature of the so-called "finite size effects", unavoidable in this kind of simulations, and to understand wh...

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Detalles Bibliográficos
Autor principal: Dorso, Claudio Oscar
Publicado: 2015
Materias:
Finite size effects
Molecular dynamics simulations
Nuclear astrophysics
Nuclear matter phase transition
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03759474_v933_n_p306_GimenezMolinelli
http://hdl.handle.net/20.500.12110/paper_03759474_v933_n_p306_GimenezMolinelli
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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