We discuss a model for the energy source of gamma-ray burst which is based on the "delayed conversion" of a metastable pure hadronic compact star ("neutron star") to a quark star (hybrid star or strange star)
We study the conversion of a neutron star to a strange star as a possible energy source for gamma-ra...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
We will follow the two-families scenario described in the accompanying paper, in which compact stars...
We describe a new model, proposed by Berezhiani et al. (2003), which is able to explain how a gamma-...
We explore some of the astrophysical consequences of the hadron-quark phase transition in compact st...
We report on a new model which is able to explain how a gamma-ray burst (GRB) can take place days or...
We propose a model to explain how a gamma-ray burst can take place days or years after a supernova e...
We propose a model to explain how a Gamma Rays Burst. can take place days or years after a supenova ...
There have been recently strong observational indications [1] about the possibility that some Gamma-...
We propose a model to explain how a gamma-ray burst can take place days or years after a supernova e...
We propose a model to explain how a Gamma Rays Burst can take place days or years after a supernova ...
The temporal structure of Gamma Ray Bursts can be interpreted assuming as a inner engine a neutron s...
We investigate the quark deconfinement phase transition in cold (T=0) and hot β-stable hadronic matt...
We study the consequences of the hadron-quark deconfinement phase transition in stellar compact obje...
We study the consequences of the hadron-quark deconfinement phase transition in stellar compact obje...
We study the conversion of a neutron star to a strange star as a possible energy source for gamma-ra...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
We will follow the two-families scenario described in the accompanying paper, in which compact stars...
We describe a new model, proposed by Berezhiani et al. (2003), which is able to explain how a gamma-...
We explore some of the astrophysical consequences of the hadron-quark phase transition in compact st...
We report on a new model which is able to explain how a gamma-ray burst (GRB) can take place days or...
We propose a model to explain how a gamma-ray burst can take place days or years after a supernova e...
We propose a model to explain how a Gamma Rays Burst. can take place days or years after a supenova ...
There have been recently strong observational indications [1] about the possibility that some Gamma-...
We propose a model to explain how a gamma-ray burst can take place days or years after a supernova e...
We propose a model to explain how a Gamma Rays Burst can take place days or years after a supernova ...
The temporal structure of Gamma Ray Bursts can be interpreted assuming as a inner engine a neutron s...
We investigate the quark deconfinement phase transition in cold (T=0) and hot β-stable hadronic matt...
We study the consequences of the hadron-quark deconfinement phase transition in stellar compact obje...
We study the consequences of the hadron-quark deconfinement phase transition in stellar compact obje...
We study the conversion of a neutron star to a strange star as a possible energy source for gamma-ra...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
We will follow the two-families scenario described in the accompanying paper, in which compact stars...
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