Add to ORKGIf strange matter is formed in the interior of a neutron star, it will convert the entire neutron star into a strange star. The proposed mechanisms are reviewed for strange matter seeding and the possible strange matter contamination of neutron star progenitors. The conversion process that follows seeding and the recent calculations of the conversion timescale are discussed
We discuss the role of strangeness on the internal constitution and structural properties of neutron...
It is shown that protostrange stars can be convective, and there are two possible scenarios for turb...
We study the effect of a magnetic field on the strage quark matter and apply to strange star. We fou...
It is generally agreed on that the tremendous densities reached in the centers of neutron stars prov...
We propose that some neutron stars in low-mass x-ray binaries can accrete sufficient mass to undergo...
We address the production of strangelets inside neutron stars by means of high-energy neutrino inter...
At greater than nuclear densities, matter may convert into a mixture of nucleons, hyperons, dibaryon...
Creation of strange quark stars through strong interaction deconfinement is studied based on modern ...
A protoneutron star is formed immediately after the gravitational collapse of the core of a massive ...
The conversion of neutron matter into strange matter in a neutron star occurs through the non-lepton...
The conversion of neutron matter to strange matter in a neutron star have been studied as a two step...
The possible existence of deconfined matter in the cores of neutron stars has been studied for over ...
We consider the general conditions of quark droplet formation in high-density neutron matter. The gr...
We study the conversion of a neutron star to a strange star as a possible energy source for gamma-ra...
The properties of strange quark matter and strange hadronic matter and their finite counterparts (st...
We discuss the role of strangeness on the internal constitution and structural properties of neutron...
It is shown that protostrange stars can be convective, and there are two possible scenarios for turb...
We study the effect of a magnetic field on the strage quark matter and apply to strange star. We fou...
It is generally agreed on that the tremendous densities reached in the centers of neutron stars prov...
We propose that some neutron stars in low-mass x-ray binaries can accrete sufficient mass to undergo...
We address the production of strangelets inside neutron stars by means of high-energy neutrino inter...
At greater than nuclear densities, matter may convert into a mixture of nucleons, hyperons, dibaryon...
Creation of strange quark stars through strong interaction deconfinement is studied based on modern ...
A protoneutron star is formed immediately after the gravitational collapse of the core of a massive ...
The conversion of neutron matter into strange matter in a neutron star occurs through the non-lepton...
The conversion of neutron matter to strange matter in a neutron star have been studied as a two step...
The possible existence of deconfined matter in the cores of neutron stars has been studied for over ...
We consider the general conditions of quark droplet formation in high-density neutron matter. The gr...
We study the conversion of a neutron star to a strange star as a possible energy source for gamma-ra...
The properties of strange quark matter and strange hadronic matter and their finite counterparts (st...
We discuss the role of strangeness on the internal constitution and structural properties of neutron...
It is shown that protostrange stars can be convective, and there are two possible scenarios for turb...
We study the effect of a magnetic field on the strage quark matter and apply to strange star. We fou...