The E1 strength is systematically analyzed in very neutron-rich Sn nuclei, beyond $^{132}$Sn until $^{166}$Sn, within the Relativistic Quasiparticle Random Phase Approximation. The great neutron excess favors the appearance of a deformed ground state for $^{142−162}$Sn. The evolution of the low-lying strength in deformed nuclei is determined by the interplay of two factors, isospin asymmetry and deformation: while greater neutron excess increases the total low-lying strength, deformation hinders and spreads it. Very neutron rich deformed nuclei may not be as good candidates as stable spherical nuclei like $^{132}$Sn for the experimental study of low-lying E1 strength
The presence of some low-lying (pygmy) strength in the dipole spectrum, at excitation energy well be...
The Isovector Giant Dipole Resonance (IVGDR) is a collective nuclear excitation mode characterized b...
We present a study on the isoscalar quadrupole strength in tin nuclei, focusing mainly on the low-en...
The self-consistent random-phase approximation, based on the framework of relativistic energy densit...
By exploiting Coulomb dissociation of high-energy radioactive beams of the neutron-rich nuclei 129-1...
Among the many ways to describe and predict the behaviour of a nucleus, we find the nuclear equation...
In certain neutron-rich Te isotopes, a decrease in the energy of the first excited 2+ state is accom...
We have computed dipole strength distributions for nickel and tin isotopes within the Relativistic Q...
Among the many ways to describe and predict the behaviour of a nucleus, we find the nuclear equation...
Atomic nuclei with a few nucleons beyond shell closures are important in understanding the evolution...
The $\gamma$-ray strength functions (GSF) and nuclear level densities (NLD) below the neutron thresh...
The isovector spin-flip M1 strength function in the deformed heavy nuclei 156Gd and 238U is calculat...
The E1 strength function for 15 stable and unstable Sn even-even isotopes from A=100 to A=176 are ca...
The structure of deformed neutron-rich nuclei in the rare-earth region is of significant interest fo...
International audienceThe $\gamma$-ray strength functions (GSF) and nuclear level densities (NLD) be...
The presence of some low-lying (pygmy) strength in the dipole spectrum, at excitation energy well be...
The Isovector Giant Dipole Resonance (IVGDR) is a collective nuclear excitation mode characterized b...
We present a study on the isoscalar quadrupole strength in tin nuclei, focusing mainly on the low-en...
The self-consistent random-phase approximation, based on the framework of relativistic energy densit...
By exploiting Coulomb dissociation of high-energy radioactive beams of the neutron-rich nuclei 129-1...
Among the many ways to describe and predict the behaviour of a nucleus, we find the nuclear equation...
In certain neutron-rich Te isotopes, a decrease in the energy of the first excited 2+ state is accom...
We have computed dipole strength distributions for nickel and tin isotopes within the Relativistic Q...
Among the many ways to describe and predict the behaviour of a nucleus, we find the nuclear equation...
Atomic nuclei with a few nucleons beyond shell closures are important in understanding the evolution...
The $\gamma$-ray strength functions (GSF) and nuclear level densities (NLD) below the neutron thresh...
The isovector spin-flip M1 strength function in the deformed heavy nuclei 156Gd and 238U is calculat...
The E1 strength function for 15 stable and unstable Sn even-even isotopes from A=100 to A=176 are ca...
The structure of deformed neutron-rich nuclei in the rare-earth region is of significant interest fo...
International audienceThe $\gamma$-ray strength functions (GSF) and nuclear level densities (NLD) be...
The presence of some low-lying (pygmy) strength in the dipole spectrum, at excitation energy well be...
The Isovector Giant Dipole Resonance (IVGDR) is a collective nuclear excitation mode characterized b...
We present a study on the isoscalar quadrupole strength in tin nuclei, focusing mainly on the low-en...