Journal ArticleDOI
The fourth-order symmetry energy of nuclear matter and symmetry energy coefficients of finite nuclei using extended semi-empirical mass formula
TLDR
An extended nuclear mass formula has been used by considering the bulk, surface and coulomb contributions to the nuclear mass as discussed by the authors, and the fourth-order symmetry energy coefficient asyclic.Abstract:
An extended nuclear mass formula has been used by considering the bulk, surface and coulomb contributions to the nuclear mass. In this mass formula, the fourth-order symmetry energy coefficient asy...read more
Citations
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Determination of the Equation of State of Dense Matter
TL;DR: In this article, the authors analyzed the flow of matter to extract pressures in excess of 1034 pascals, the highest recorded under laboratory-controlled conditions, using these analyses, they rule out strongly repulsive nuclear equations of state from relativistic mean field theory and weakly repulsive equations of states with phase transitions at densities less than three times that of stable nuclei, but not equation of state softened at higher densities because of a transformation to quark matter.
Surface Symmetry Energy
TL;DR: In this article, the authors show that the symmetry energy of symmetric nuclear matter can be accessed easily with the textbook mass-formula and a sample of nuclear masses, with a minimally modified formula along the lines of the droplet model.
Journal ArticleDOI
Study of the dependence of alpha decay half-life on the surface symmetry energy
S. Nejati,O. N. Ghodsi +1 more
TL;DR: In this article, the effect of the surface symmetry energy on the neutron skin thickness and division of it into the bulk and surface parts are investigated by determination of the symmetry energy co-existence.
References
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Journal ArticleDOI
Determination of the equation of state of dense matter.
TL;DR: This work analyzed the flow of matter to extract pressures in excess of 1034 pascals, the highest recorded under laboratory-controlled conditions, and ruled out strongly repulsive nuclear equations of state from relativistic mean field theory and weakly repulsive equation of state with phase transitions at densities less than three times that of stable nuclei.
Journal ArticleDOI
Recent Progress and New Challenges in Isospin Physics with Heavy-Ion Reactions
TL;DR: In this paper, the authors review the major progress achieved during the last decade in isospin physics with heavy ion reactions and discuss future challenges to the most important issues in this field.
Journal ArticleDOI
Equations of state for supernovae and compact stars
TL;DR: In this article, a review of the thermodynamic properties of matter at extreme densities, even exceeding nuclear matter density severely, is presented, where the composition of matter for such conditions, the resulting pressure, and the maximum mass of cold neutron stars are described.
Journal ArticleDOI
Isospin asymmetry in nuclei and neutron stars
TL;DR: In this article, the roles of isospin asymmetry in nuclei and neutron stars are investigated using a range of potential and field-theoretical models of nucleonic matter.
Journal ArticleDOI
Neutron radii in nuclei and the neutron equation of state
TL;DR: The root-mean-square radius for neutrons in nuclei is investigated in the Skyrme Hartree-Fock model and an important new constraint on the equation of state for neutron matter is placed.
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