The Equation of State of Nuclear Matter: From Finite Nuclei to Neutron Stars
<i>Background.</i> We investigate possible correlations between neutron star observables and properties of atomic nuclei. In particular, we explore how the tidal deformability of a 1.4 solar mass neutron star, <inline-formula><math display="inline"><semantics><msub><mi>M</mi><mrow><mn>1.4</mn></mrow...
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| Hoofdauteurs: | , |
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| Formaat: | Artigo |
| Taal: | Inglês |
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MDPI AG
2020-08-01
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| Reeks: | Universe |
| Onderwerpen: | |
| Online toegang: | https://www.mdpi.com/2218-1997/6/8/119 |
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