Add to ORKGWe study the scenario that a newborn strange quark star cools to the quantum chromodynamics (QCD) phase transition temperature and converts to a neutron star, and we calculate the evolution of temperature and luminosity of the compact star. We argue that the conversion energy released can be of the order of 1053 erg. We also propose that a second neutrino burst will be emitted at the completion of this phase transition
We study the quark deconfinement phase transition in cold (T = 0) and hot beta-stable hadronic matte...
We study the quark deconfinement phase transition in cold (T = 0) and hot beta-stable hadronic matte...
AbstractWe study the quark deconfinement phase transition in hot β-stable hadronic matter. Assuming ...
We study the cooling behavior of an isolated strange-quark star, using an equation of state derived ...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
Context. A phase of strong interacting matter with deconfined quarks is expected in the core of a ma...
Context. A phase of strong interacting matter with deconfined quarks is expected in the core of a ma...
We investigate the quark deconfinement phase transition in cold (T=0) and hot β-stable hadronic matt...
Context. A phase of strong interacting matter with deconfined quarks is expected in the core of a ma...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
The possible role of a first order QCD phase transition at nonvanishing quark chemical potential and...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
The possible existence of two families of compact stars, neutron stars and quark stars, naturally le...
The possible existence of two families of compact stars, neutron stars and quark stars, naturally le...
We study the quark deconfinement phase transition in cold (T = 0) and hot beta-stable hadronic matte...
We study the quark deconfinement phase transition in cold (T = 0) and hot beta-stable hadronic matte...
AbstractWe study the quark deconfinement phase transition in hot β-stable hadronic matter. Assuming ...
We study the cooling behavior of an isolated strange-quark star, using an equation of state derived ...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
Context. A phase of strong interacting matter with deconfined quarks is expected in the core of a ma...
Context. A phase of strong interacting matter with deconfined quarks is expected in the core of a ma...
We investigate the quark deconfinement phase transition in cold (T=0) and hot β-stable hadronic matt...
Context. A phase of strong interacting matter with deconfined quarks is expected in the core of a ma...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
The possible role of a first order QCD phase transition at nonvanishing quark chemical potential and...
A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutr...
The possible existence of two families of compact stars, neutron stars and quark stars, naturally le...
The possible existence of two families of compact stars, neutron stars and quark stars, naturally le...
We study the quark deconfinement phase transition in cold (T = 0) and hot beta-stable hadronic matte...
We study the quark deconfinement phase transition in cold (T = 0) and hot beta-stable hadronic matte...
AbstractWe study the quark deconfinement phase transition in hot β-stable hadronic matter. Assuming ...