Nuclear matter and neutron-star properties calculated with the Skyrme interaction

By J. Stone, J. Miller, R. Koncewicz, P. Stevenson, M. Strayer. 2003

189 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/c8832fa85627c3aba33b2c79d09c99c312c0a3a4

How researchers see this paper

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In Astronomy and Astrophysics

1. J. Lattimer
2. Bao-An Li
3. Jun Xu
4. A. Steiner
5. Lie-Wen Chen
6. E. Brown
7. Hong-ru Ma
8. G. Fiorella Burgio

In Geophysics

1. J. Lattimer
2. A. Steiner
3. Bao-An Li
4. Jun Xu
5. Y. Lim
6. A. Watts

In Nuclear and High Energy Physics

1. Bao-An Li
2. Jun Xu
3. J. Lattimer
4. Lie-Wen Chen
5. Hong-ru Ma
6. A. Steiner
7. G. Fiorella Burgio
8. Nai-Bo Zhang

Citations in the corpus

• NUCLEAR CONSTRAINTS ON PROPERTIES OF NEUTRON STAR CRUSTS (2009, background): “…for these 51 Skyrme forces are available from numerous references (Brack et al. 1985; Friedrich & Reinhard 1986; Brown 1998; Chabanat et al. 1997; Stone et al. 2003; Stone & Reinhard 2007; Chen et al. 2005b; Steiner & Li 2005b; Samyn et al. 2002, 2003, 2004, 2005; Goriely et al. 2003, 2005,…”
• THE EQUATION OF STATE FROM OBSERVED MASSES AND RADII OF NEUTRON STARS (2010, methodology): “These Skyrme models were selected in Steiner & Watts (2009) because they are a representative setof the recommended models from Stone et al. (2003) which have symmetry energies which do not become negativ at high density.”