If strange quark matter is the true ground state of matter, it must have lower energy than nuclear matter. Simultaneously, two-flavor quark matter must have higher energy than nuclear matter, for otherwise the latter would convert to the former. We show, using an effective chiral Lagrangian, that the existence of a new lower energy ground state for two-flavor quark matter, the pion condensate, shrinks the window allowing strange quark matter to be the ground state of matter and sets new limits on the current strange quark mass
We calculate strange star properties, using large N_c approximation with built-in chiral symmetry re...
Properties of dense quark matter in and out of chemical equilibrium arestudied within the SU(3) Namb...
Abstract. Strange quark matter is studied in the framework of the Chromodielectric model (CDM), and ...
Kurkela A, Romatschke P, Vuorinen A. Cold quark matter. Phys. Rev. D. 2010;81(10): 105021.We perform...
We discuss the possible existence of absolutely stable strange quark matter within three different t...
We discuss the possible existence of absolutely stable strange quark matter within three different t...
We discuss the possible existence of absolutely stable strange quark matter within three different t...
We discuss the possible existence of absolutely stable strange quark matter within three different t...
We construct a model for dense matter based on low-density nuclear matter properties that exhibits a...
We examine, in the chiral limit where the up and down quark masses are vanishingly small, the stabil...
We examine, in the chiral limit where the up and down quark masses are vanishingly small, the stabil...
Strange quark matter in beta equilibrium at high densities is studied in a quark confinement model. ...
We improve our recently proposed unified description for strange quark matter (SQM) objects, in the ...
Some recent developments concerning the role of strange quark matter for astrophysical systems and t...
The existence of quark states with more than three quarks is allowed in QCD. The stability of such q...
We calculate strange star properties, using large N_c approximation with built-in chiral symmetry re...
Properties of dense quark matter in and out of chemical equilibrium arestudied within the SU(3) Namb...
Abstract. Strange quark matter is studied in the framework of the Chromodielectric model (CDM), and ...
Kurkela A, Romatschke P, Vuorinen A. Cold quark matter. Phys. Rev. D. 2010;81(10): 105021.We perform...
We discuss the possible existence of absolutely stable strange quark matter within three different t...
We discuss the possible existence of absolutely stable strange quark matter within three different t...
We discuss the possible existence of absolutely stable strange quark matter within three different t...
We discuss the possible existence of absolutely stable strange quark matter within three different t...
We construct a model for dense matter based on low-density nuclear matter properties that exhibits a...
We examine, in the chiral limit where the up and down quark masses are vanishingly small, the stabil...
We examine, in the chiral limit where the up and down quark masses are vanishingly small, the stabil...
Strange quark matter in beta equilibrium at high densities is studied in a quark confinement model. ...
We improve our recently proposed unified description for strange quark matter (SQM) objects, in the ...
Some recent developments concerning the role of strange quark matter for astrophysical systems and t...
The existence of quark states with more than three quarks is allowed in QCD. The stability of such q...
We calculate strange star properties, using large N_c approximation with built-in chiral symmetry re...
Properties of dense quark matter in and out of chemical equilibrium arestudied within the SU(3) Namb...
Abstract. Strange quark matter is studied in the framework of the Chromodielectric model (CDM), and ...