Among the many ways to describe and predict the behaviour of a nucleus, we find the nuclear equation of state (EoS). This expression aims to account for the properties of nuclear matter from common run-off-the-mill nuclei, such as those found in nature, to neutron stars and nuclei far from stability synthesized in laboratories. Around the density nuclear matter would assume if it were infinite and constituted in equal parts by neutrons and protons, the nuclear equation of state can be expanded in a Taylor series: the first terms of this series define the behaviour of the equation of state. Of particular interest is the second order term, known as the symmetry energy. Because it is not experimentally accessible, though, a direct measurement...
Inelastic scattering cross sections to individual bound excited states of 104 Sn were measured at 15...
Atomic nuclei with a few nucleons beyond shell closures are important in understanding the evolution...
Heavy atomic nuclei are thought to have proton and neutron radial distributions which have differen...
Among the many ways to describe and predict the behaviour of a nucleus, we find the nuclear equation...
Among the many ways to describe and predict the behaviour of a nucleus, we find the nuclear equation...
The E1 strength distribution in Ni68 has been investigated using Coulomb excitation in inverse kinem...
The Isovector Giant Dipole Resonance (IVGDR) is a collective nuclear excitation mode characterized b...
We have computed dipole strength distributions for nickel and tin isotopes within the Relativistic Q...
The electric dipole is an important property of heavy nuclei. Precise information on the electric di...
The present thesis reports on the systematics of the electric dipole response in stable even mass ti...
Inelastic scattering cross sections to individual bound excited states of Sn-104 were measured at 15...
We examine a method to determine the neutron-skin thickness of nuclei using data on the charge-excha...
The $\gamma$-ray strength functions (GSF) and nuclear level densities (NLD) below the neutron thresh...
Inelastic scattering cross sections to individual bound excited states of 104 Sn were measured at 15...
Atomic nuclei with a few nucleons beyond shell closures are important in understanding the evolution...
Heavy atomic nuclei are thought to have proton and neutron radial distributions which have differen...
Among the many ways to describe and predict the behaviour of a nucleus, we find the nuclear equation...
Among the many ways to describe and predict the behaviour of a nucleus, we find the nuclear equation...
The E1 strength distribution in Ni68 has been investigated using Coulomb excitation in inverse kinem...
The Isovector Giant Dipole Resonance (IVGDR) is a collective nuclear excitation mode characterized b...
We have computed dipole strength distributions for nickel and tin isotopes within the Relativistic Q...
The electric dipole is an important property of heavy nuclei. Precise information on the electric di...
The present thesis reports on the systematics of the electric dipole response in stable even mass ti...
Inelastic scattering cross sections to individual bound excited states of Sn-104 were measured at 15...
We examine a method to determine the neutron-skin thickness of nuclei using data on the charge-excha...
The $\gamma$-ray strength functions (GSF) and nuclear level densities (NLD) below the neutron thresh...
Inelastic scattering cross sections to individual bound excited states of 104 Sn were measured at 15...
Atomic nuclei with a few nucleons beyond shell closures are important in understanding the evolution...
Heavy atomic nuclei are thought to have proton and neutron radial distributions which have differen...