Abstract
We review the properties of the parametric coupling model and analyze its results when considering neutron star observations and heavy-ion collision experiments, specially those concerning the isospin characteristics of symmetric and asymmetric nuclear matter. By the end of the analysis, we are able to constrain the free parameters to a very small range of acceptable values.
| Original language | English |
|---|---|
| Pages (from-to) | 1463-1468 |
| Number of pages | 6 |
| Journal | International Journal of Modern Physics D |
| Volume | 19 |
| Issue number | 8-10 |
| DOIs | |
| State | Published - Aug 2010 |
Keywords
- equation of state
- Heavy-ion collision
- isospin
- neutron star
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