On the effect of high order empirical parameters on the nuclear equation of state
arXiv:1807.01729 · doi:10.1103/PhysRevC.99.025806
Abstract
A quantitative knowledge of the nuclear Equation of State (EoS) requires an accurate estimation of the uncertainties on the EoS parameters and their mutual correlations. Such correlations are empirically observed in a large set of EoS models by different authors, but they are not always fully understood. We show that some of these correlations can be interpreted from basic physical constraints imposed on a simple Taylor expansion of the binding energy around saturation density. In particular, we investigate the correlations among the following empirical parameters: the symmetry energy , the slope and curvature of the symmetry energy and , and the curvature and skewness of the binding energy in symmetric matter and . The uncertainties on these correlations is estimated through analytical modelling as well as a meta-modelling analysis of the EoS subject to physical constraints. We show that a huge dispersion of the correlations among low order empirical parameters is induced by the unknown higher order empirical parameters, such as (second order) and and (third order). We also propose an explanation of the reason why is weakly constrained by present experimental data. We conclude that selective observables on high order parameters, such as and , should be better determined before the present uncertainties on the EoS can be further reduced.
References in corpus (14)
- Relativistic Nuclear Energy Density Functionals: adjusting parameters to binding energies
- Relativistic Mean-Field Hadronic Models under Nuclear Matter Constraints
- A critical examination of constraints on the equation of state of dense matter obtained from GW170817
- Constraints on the Symmetry Energy Using the Mass-Radius Relation of Neutron Stars
- The Giant Dipole Resonance as a quantitative constraint on the symmetry energy
- Core-crust transition in neutron stars: predictivity of density developments
- Neutron skin thickness in droplet model with surface width dependence: indications of softness of the nuclear symmetry energy
- Incompressibility of neutron-rich matter
- Uncertainty Quantification for Nuclear Density Functional Theory and Information Content of New Measurements
- Origin of the neutron skin thickness of 208Pb in nuclear mean-field models
- Interdependence of different symmetry energy elements
- Constraints on the symmetry energy from observational probes of the neutron star crust
- Universal correlations in the nuclear symmetry energy, slope parameter, and curvature
- Moving Beyond Chi-Squared in Nuclei and Neutron Stars
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