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- W1601216389 abstract "In the present work we apply a quantum hadrodynamic effective model in the mean-field approximation to the description of neutron stars. We consider an adjustable derivative-coupling model and study the parameter influence on the dynamics of the system by analyzing the full range of values they can take. We establish a set of parameters that define a specific model that can describe phenomenological properties such as the effective nucleon mass at saturation as well as global static properties of neutron stars (mass and radius). If one uses observational data to fix the maximum mass for neutron stars by a specific model, we can predict the compression modulus of nuclear matter, which is found to be $K=257.2$ MeV." @default.
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- W1601216389 date "2008-06-20" @default.
- W1601216389 modified "2023-09-27" @default.
- W1601216389 title "Density dependent nuclear matter compressibility" @default.
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- W1601216389 doi "https://doi.org/10.1103/physrevc.77.065803" @default.
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