In the framework of the non-relativistic Brueckner-Bethe-Goldstone theory, we derive a microscopic equation of state for asymmetric and $\beta$-stable matter containing $\Sigma^-$ and $\Lambda$ hyperons. We mainly study the effects of three-body forces (TBFs) among nucleons on the hyperon formation and the equation of state (EoS). We find that, when TBFs are included, the stellar core is almost equally populated by nucleons and hyperons. The resulting EoS, which turns out to be extremely soft, has been used in order to calculate the static structure of neutron stars. We obtain a value of the maximum mass of 1.26 solar masses (1 solar mass $M_o \simeq 1.99 \cdot 10^{33} g$). Stellar rotations increase this value by about 12%
We study the hadron-quark phase transition in the interior of neutron stars. For the hadronic sector...
The true nature and the internal constitution of the compact stars known as neutron stars (NSs) is o...
Recent progress in the understanding of the high density phase of neutron stars advances the view th...
In the framework of the non-relativistic Brueckner-Bethe-Goldstone theory, we derive a microscopic e...
In the framework of the Brueckner-Bethe-Goldstone theory, we determine a fully microscopic equation ...
In the framework of the Brueckner-Bethe-Goldstone theory, we determine a fully microscopic equation ...
We discuss the high-density nuclear equation of state within the Brueckner-Hartree-Fock approach. Pa...
We present results from Brueckner-Hartree-Fock calculatons for beta stable neutron star matter with ...
We calculate static properties of non-rotating neutron stars (NS's) using a microscopic equation of ...
We have developed a formalism for microscopic Brueckner-type calculations of dense nuclear matter th...
The Bethe-Brueckner-Goldstone many-body theory of the Nuclear Equation of State is reviewed in some ...
AbstractUsing the Dirac–Brueckner–Hartree–Fock approach, the properties of neutron-star matter inclu...
We determine the structure of neutron stars within a Brueckner-Hartree-Fock approach based on realis...
We adopt two- and three-body nuclear forces derived at the next-to-next-to-leading-order in the fram...
We adopt two- and three-body nuclear forces derived at the next-to-next-to-leading-order in the fram...
We study the hadron-quark phase transition in the interior of neutron stars. For the hadronic sector...
The true nature and the internal constitution of the compact stars known as neutron stars (NSs) is o...
Recent progress in the understanding of the high density phase of neutron stars advances the view th...
In the framework of the non-relativistic Brueckner-Bethe-Goldstone theory, we derive a microscopic e...
In the framework of the Brueckner-Bethe-Goldstone theory, we determine a fully microscopic equation ...
In the framework of the Brueckner-Bethe-Goldstone theory, we determine a fully microscopic equation ...
We discuss the high-density nuclear equation of state within the Brueckner-Hartree-Fock approach. Pa...
We present results from Brueckner-Hartree-Fock calculatons for beta stable neutron star matter with ...
We calculate static properties of non-rotating neutron stars (NS's) using a microscopic equation of ...
We have developed a formalism for microscopic Brueckner-type calculations of dense nuclear matter th...
The Bethe-Brueckner-Goldstone many-body theory of the Nuclear Equation of State is reviewed in some ...
AbstractUsing the Dirac–Brueckner–Hartree–Fock approach, the properties of neutron-star matter inclu...
We determine the structure of neutron stars within a Brueckner-Hartree-Fock approach based on realis...
We adopt two- and three-body nuclear forces derived at the next-to-next-to-leading-order in the fram...
We adopt two- and three-body nuclear forces derived at the next-to-next-to-leading-order in the fram...
We study the hadron-quark phase transition in the interior of neutron stars. For the hadronic sector...
The true nature and the internal constitution of the compact stars known as neutron stars (NSs) is o...
Recent progress in the understanding of the high density phase of neutron stars advances the view th...