Add to ORKGWe study the properties of rotating neutron stars within a generalized chiral SU(3)-flavor model. The influence of the rotation on the inner structure and the hyperon matter content of the star is discussed. We calculate the Kepler frequency and moments of inertia of the neutron star sequences. An estimate for the braking index of the associated pulsars is given
International audienceWith (nonbarotropic) equations of state valid even when the neutron, proton, a...
This paper gives an overview of the model of a neutron star with non-zero strangeness constructed wi...
International audienceWith (nonbarotropic) equations of state valid even when the neutron, proton, a...
The equations of state for neutron matter, strange and non-strange hadronic matter in the chiral SU(...
Context. The discovery of a 2M neutron star provided a robust constraint for the theory of exotic de...
Context. The discovery of a 2 M⊙ neutron star provided a robust constraint for the theory...
Context. The discovery of a 2 M⊙ neutron star provided a robust constraint for the theory...
In this paper, we use a three flavor non-local Nambu–Jona-Lasinio (NJL) model, an improved effective...
In this paper, we use a three flavor non-local Nambu–Jona-Lasinio (NJL) model, an improved effective...
honors thesisCollege of SciencePhysics and AstronomyYue ZhaoIn this work we examine the applications...
In this thesis a very comprehensive model of rotating neutron stars has been constructed, which is b...
honors thesisCollege of SciencePhysics and AstronomyYue ZhaoIn this work we examine the applications...
We construct models of rotating stars using the perturbative approach introduced by J. Hartle in 196...
In this paper, we present results from an investigation of the rotational properties of strange star...
International audienceWith (nonbarotropic) equations of state valid even when the neutron, proton, a...
International audienceWith (nonbarotropic) equations of state valid even when the neutron, proton, a...
This paper gives an overview of the model of a neutron star with non-zero strangeness constructed wi...
International audienceWith (nonbarotropic) equations of state valid even when the neutron, proton, a...
The equations of state for neutron matter, strange and non-strange hadronic matter in the chiral SU(...
Context. The discovery of a 2M neutron star provided a robust constraint for the theory of exotic de...
Context. The discovery of a 2 M⊙ neutron star provided a robust constraint for the theory...
Context. The discovery of a 2 M⊙ neutron star provided a robust constraint for the theory...
In this paper, we use a three flavor non-local Nambu–Jona-Lasinio (NJL) model, an improved effective...
In this paper, we use a three flavor non-local Nambu–Jona-Lasinio (NJL) model, an improved effective...
honors thesisCollege of SciencePhysics and AstronomyYue ZhaoIn this work we examine the applications...
In this thesis a very comprehensive model of rotating neutron stars has been constructed, which is b...
honors thesisCollege of SciencePhysics and AstronomyYue ZhaoIn this work we examine the applications...
We construct models of rotating stars using the perturbative approach introduced by J. Hartle in 196...
In this paper, we present results from an investigation of the rotational properties of strange star...
International audienceWith (nonbarotropic) equations of state valid even when the neutron, proton, a...
International audienceWith (nonbarotropic) equations of state valid even when the neutron, proton, a...
This paper gives an overview of the model of a neutron star with non-zero strangeness constructed wi...
International audienceWith (nonbarotropic) equations of state valid even when the neutron, proton, a...