The symmetry term in the standard semiempirical formula for binding energy has a volume character. However, as we demonstrate, the description of binding energies for light nuclei requires an inclusion of the surface symmetry energy in the binding-energy formula. The symmetry volume and surface energies combine in the formula like energies of two capacitors in parallel. A finite surface symmetry energy necessarily implies the existence of nuclear asymmetry skins, describable in terms of the ratio of symmetry energy volume parameter alpha to an analogous surface parameter beta. Using available binding energy and skin data, we constrain the parameter values, finding 27MeV< alpha < 32MeV and 10.0MeV< beta <12.5MeV. We demonstrate in the Thomas...
AbstractThe thermal evolution of the energies and free energies of a set of spherical and near-spher...
We study the bulk deformation properties of the Skyrme nuclear energy density functionals (EDFs). Fo...
Our current knowledge of the Equation of State of asymmetric nuclear matter around saturation densit...
Examination of symmetry energy is carried out on the basis of an elementary binding-energy formula. ...
Binding energy of isospin asymmetric nuclei can be accessed with minimally modified formula along th...
Thesis advisor: Kevin S. BedellWe investigate the structure of the equation of state of finite nucle...
International audienceProperties of the nuclear medium M Baldo and G F Burgio-Estimating the relevan...
We discuss to what extent information on ground-state properties of finite nuclei ( energies and rad...
In this talk, we will examine isoscaling, the exponential dependence of the isotope yield ratios on ...
We describe a relation between the symmetry energy coefficients csym(ρ) of nuclear matter and asym(A...
Excitation energies to isobaric states, that are analogs of ground states, are dominated by contribu...
Energy in nuclear matter is, in practice, completely characterized at different densities and asymme...
We study the bulk deformation properties of the Skyrme nuclear energy density functionals. Following...
27 pages, 18 figures, submitted to PRCInternational audienceThe problem of the determination of the ...
The role of isospin asymmetry in nuclei and neutron stars is discussed, with an emphasis on the dens...
AbstractThe thermal evolution of the energies and free energies of a set of spherical and near-spher...
We study the bulk deformation properties of the Skyrme nuclear energy density functionals (EDFs). Fo...
Our current knowledge of the Equation of State of asymmetric nuclear matter around saturation densit...
Examination of symmetry energy is carried out on the basis of an elementary binding-energy formula. ...
Binding energy of isospin asymmetric nuclei can be accessed with minimally modified formula along th...
Thesis advisor: Kevin S. BedellWe investigate the structure of the equation of state of finite nucle...
International audienceProperties of the nuclear medium M Baldo and G F Burgio-Estimating the relevan...
We discuss to what extent information on ground-state properties of finite nuclei ( energies and rad...
In this talk, we will examine isoscaling, the exponential dependence of the isotope yield ratios on ...
We describe a relation between the symmetry energy coefficients csym(ρ) of nuclear matter and asym(A...
Excitation energies to isobaric states, that are analogs of ground states, are dominated by contribu...
Energy in nuclear matter is, in practice, completely characterized at different densities and asymme...
We study the bulk deformation properties of the Skyrme nuclear energy density functionals. Following...
27 pages, 18 figures, submitted to PRCInternational audienceThe problem of the determination of the ...
The role of isospin asymmetry in nuclei and neutron stars is discussed, with an emphasis on the dens...
AbstractThe thermal evolution of the energies and free energies of a set of spherical and near-spher...
We study the bulk deformation properties of the Skyrme nuclear energy density functionals (EDFs). Fo...
Our current knowledge of the Equation of State of asymmetric nuclear matter around saturation densit...