Isospin asymmetry in nuclei and neutron stars

  title={Isospin asymmetry in nuclei and neutron stars},
  author={Andrew W. Steiner and Madappa Prakash and James M. Lattimer and Paul J. Ellis},
  journal={Physics Reports},
Prior Probability Distributions of Neutron Star Crust Models
To make best use of multifaceted astronomical and nuclear data sets, probability distributions of neutron star models that can be used to propagate errors consistently from one domain to another are
A survey of the parameter space of the compressible liquid drop model as applied to the neutron star inner crust
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Two-fluid models of superfluid neutron star cores
Both relativistic and non-relativistic two-fluid models of neutron star cores are constructed, using the constrained variational formalism developed by Brandon Carter and co-workers. We consider a
Bayesian Inference of the Symmetry Energy of Superdense Neutron-rich Matter from Future Radius Measurements of Massive Neutron Stars
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Innermost Stable Circular Orbits Around Rotating Compact Stars
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Constraining the surface properties of effective Skyrme interactions
The purpose of this study is threefold: first, to identify a scheme for the determination of the surface energy coefficient a_surf that offers the best compromise between robustness, precision, and
Suggested formulas for half-life time of unstable nuclei: Effect of the isospin asymmetry
Using the available data of half-life time of unstable nuclei given that the number of protons is greater than the number of neutrons, an elaboration was made on the dependence of half-life time of
Equation of State of Neutron-Rich Matter in $d$-Dimensions
Nuclear systems under constraints, with high degrees of symmetries and/or collectivities may be considered as moving effectively in spaces with reduced spatial dimensions. We first derive analytical


Nuclear equation of state
We present a discussion of the equation of state of cold nuclear matter predicted by our recently completed Thomas-Fermi model. The equation is in the form of a three-term polynomial in the cube root
Interaction of photons with /sup 208/Pb and neighboring isotopes at energies below the neutron emission threshold
Average elastic photon scattering cross sections were measured for /sup 209/Bi, /sup 208/Pb, /sup 207/Pb, /sup 206/Pb, Tl and Hg at excitation energies between 4.5 MeV and the neutron emission