Results 31 to 40 of about 301,890 (253)
Strange quark matter in a chiral SU(3) quark mean field model [PDF]
Phys.Rev. C67 (2003) 015210, 2002 We apply the chiral SU(3) quark mean field model to investigate strange quark matter. The stability of strange quark matter with different strangeness fraction is studied. The interaction between quarks and vector mesons destabilizes the strange quark matter.
arxiv +1 more source
Quark, pion and axial condensates in three-flavor finite isospin chiral perturbation theory
European Physical Journal C: Particles and Fields, 2021 We calculate the light-quark condensate, the strange-quark condensate, the pion condensate, and the axial condensate in three-flavor chiral perturbation theory ( $$\chi $$ χ PT) in the presence of an isospin chemical potential at next-to-leading order at
Prabal Adhikari +2 more
doaj +1 more source
Searching for strange quark matter objects among white dwarfs
Physics Letters B, 2022 The ground state of matter may be strange quark matter (SQM), not hadronic matter. A whole sequence of SQM objects, ranging from strange quark stars and strange quark dwarfs to strange quark planets, can stably exist according to this SQM hypothesis.
Abdusattar Kurban +3 more
doaj
On the estimation of the strange quark mass from the experimental data on the light baryon octet
Âderna Fìzika ta Energetika, 2018 Simple relations connecting the strange quark mass to the splittings of the light hyperon masses were obtained on the basis of the phenomenological quark model compatible with the present-day theory of strong interactions, i.e.
V. A. Babenko, N. M. Petrov
doaj +1 more source
Strangeness, Charm and Beauty in Quark Matter: SQM 2007 Experimental Overview [PDF]
J.Phys.G35:044055,2008, 2007 This paper aims at providing an experimental overview of the Strangeness in Quark Matter 2007 ...
arxiv +1 more source
Dark matter admixed strange quark stars in the Starobinsky model [PDF]
, 2018 We compute the mass-to-radius profiles for dark matter admixed strange quark stars in the Starobinsky model of modified gravity. For quark matter we assume the MIT bag model, while self-interacting dark matter inside the star is modelled as a Bose ...
I. Lopes, G. Panotopoulos
semanticscholar +1 more source
Spin and Flavor Strange Quark Content of the Nucleon [PDF]
Phys.Rev.D78:014001,2008, 2008 Several spin and flavor dependent parameters characterizing the strangeness content of the nucleon have been calculated in the chiral constituent quark model with configuration mixing (\chiCQM_{config}) which is known to provide a satisfactory explanation of the ``proton spin crisis'' and related issues.
arxiv +1 more source
Strange Quark Matter in Stars: A General Overview [PDF]
J.Phys. G31 (2005) S651-S658, 2004 The physics of strange quark matter in the core of compact stars and recent compact star data is reviewed. Emphasis is put on the possible existence of a third family of strange quark stars.
arxiv +1 more source
Strange Quark Magnetic Moment of the Nucleon at the Physical Point. [PDF]
Physical Review Letters, 2016 We report a lattice QCD calculation of the strange quark contribution to the nucleon's magnetic moment and charge radius. This analysis presents the first direct determination of strange electromagnetic form factors including at the physical pion mass ...
R. Sufian +5 more
semanticscholar +1 more source
Electrically charged strange quark stars with a non-linear equation-of-state
The European Physical Journal C, 2019 The properties of electrically charged strange quark stars are investigated. We assume a non-linear equation-of-state, and we obtain numerical solutions to the structure equations.
G. Panotopoulos, Á. Rincón
semanticscholar +1 more source