The explicit energy dependence of the single particle self-energy (dispersive effects), due to short range correlations, is included in the treatment of neutron matter superfluidity. The method can be applied in general to strong interacting fermion systems, and it is expected to be valid whenever the pairing gap is substantially smaller than the Fermi kinetic energy. The results for neutron matter show that dispersive effects are strong in the density region near the gap closure
Ultracold atomic gases and low-density neutron matter are unique in that they exhibit pairing gaps c...
Nuclear superfludity in exotic nuclei close to the drip lines and in the inner crust matter of neutr...
The $^1S_0$ pairing in neutron matter has been investigated in presence of realistic two-- and three...
Pairing gaps in neutron matter need to be computed in a wide range of densities to address open ques...
The superfluidity of neutron matter in the channel $^1 S_0$ is studied by taking into account the ef...
Nucleon pairing is studied with specific considerations directed toward the possible influence on ne...
Effects of medium polarization are studied for $^1S_0$ pairing in neutron and nuclear matter. The sc...
We discuss superfluidity in neutron matter, with particular attention to induced interactions and to...
The inner crust of a neutron star is a superfluid and inhomogeneous system, consisting of a lattice ...
The inner crust of a neutron star is a superfluid and inhomogeneous system, consisting of a lattice ...
none3siBackground: An accurate description of nuclear pairing gaps is extremely important for unders...
We compute singlet pairing gaps and critical temperatures in pure neutron matter with different many...
We compute singlet pairing gaps and critical temperatures in pure neutron matter with different many...
Some aspects of the superfluidity in nuclear matter and neutron matter are numerically investigated ...
We report on recent work on the equation of state and pairing gap of neutron matter and cold atomic ...
Ultracold atomic gases and low-density neutron matter are unique in that they exhibit pairing gaps c...
Nuclear superfludity in exotic nuclei close to the drip lines and in the inner crust matter of neutr...
The $^1S_0$ pairing in neutron matter has been investigated in presence of realistic two-- and three...
Pairing gaps in neutron matter need to be computed in a wide range of densities to address open ques...
The superfluidity of neutron matter in the channel $^1 S_0$ is studied by taking into account the ef...
Nucleon pairing is studied with specific considerations directed toward the possible influence on ne...
Effects of medium polarization are studied for $^1S_0$ pairing in neutron and nuclear matter. The sc...
We discuss superfluidity in neutron matter, with particular attention to induced interactions and to...
The inner crust of a neutron star is a superfluid and inhomogeneous system, consisting of a lattice ...
The inner crust of a neutron star is a superfluid and inhomogeneous system, consisting of a lattice ...
none3siBackground: An accurate description of nuclear pairing gaps is extremely important for unders...
We compute singlet pairing gaps and critical temperatures in pure neutron matter with different many...
We compute singlet pairing gaps and critical temperatures in pure neutron matter with different many...
Some aspects of the superfluidity in nuclear matter and neutron matter are numerically investigated ...
We report on recent work on the equation of state and pairing gap of neutron matter and cold atomic ...
Ultracold atomic gases and low-density neutron matter are unique in that they exhibit pairing gaps c...
Nuclear superfludity in exotic nuclei close to the drip lines and in the inner crust matter of neutr...
The $^1S_0$ pairing in neutron matter has been investigated in presence of realistic two-- and three...