Self-gravitating strange dark matter halos around galaxies [PDF]
A new family of nonrelativistic, Newtonian, non-quantum equilibrium configurations describing galactic halos is introduced, by considering strange quark matter conglomerates with masses larger than about 8 GeV as new possible components of the dark ...
M. Merafina+4 more
semanticscholar +1 more source
Quark stars with 2.6 $$M_\odot $$ M ⊙ in a non-minimal geometry-matter coupling theory of gravity
This work analyses the hydrostatic equilibrium configurations of strange stars in a non-minimal geometry-matter coupling (GMC) theory of gravity. Those stars are made of strange quark matter, whose distribution is governed by the MIT equation of state ...
G. A. Carvalho+4 more
doaj +1 more source
Axion Emission from Strange Matter in Core-Collapse SNe. [PDF]
The duration of the neutrino burst from the supernova event SN 1987A is known to be sensitive to exotic sources of cooling, such as axions radiated from the dense and hot hadronic matter thought to constitute the inner core of the supernova.
Maël Cavan-Piton+4 more
semanticscholar +1 more source
Relativistic heavy ion collisions offer the possibility to produce exotic metastable states of nuclear matter containing (roughly) equal number of strangeness compared to the content in baryon number. The reasoning of both their stability and existence, the possible distillation of strangeness necessary for their formation and the chances for their ...
Juergen Schaffner-Bielich+1 more
openaire +4 more sources
The crystallography of strange quark matter [PDF]
Cold three-flavor quark matter at large (but not asymptotically large) densities may exist as a crystalline color superconductor. We explore this possibility by calculating the gap parameter Delta and free energy Omega(Delta) for possible crystal structures within a Ginzburg-Landau approximation, evaluating Omega(Delta) to order Delta^6.
Rishi Sharma+3 more
openaire +3 more sources
Strange Matter: a state before black hole [PDF]
Normal baryonic matter inside an evolved massive star can be intensely compressed by gravity after a supernova. General relativity predicts formation of a black hole if the core material is compressed into a singularity, but the real state of such ...
R. Xu, Yanjun Guo
semanticscholar +1 more source
Study of anisotropic strange stars in f(R,T) gravity: An embedding approach under the simplest linear functional of the matter-geometry coupling [PDF]
The present work is focused on the investigation of the existence of compact structures describing anisotropic matter distributions within the framework of modified gravity theories, specifically f(R,$\mathcal{T}$) gravity theory.
S. Maurya+4 more
semanticscholar +1 more source
Strange matter and strange stars in a thermodynamically self-consistent perturbation model with running coupling and running strange quark mass [PDF]
A quark model with running coupling and running strange quark mass, which is thermodynamically self-consistent at both high and lower densities, is presented and applied to study properties of strange quark matter and structure of compact stars.
Jia Xu+4 more
semanticscholar +1 more source
Energy Dependence of Strangeness Production in Heavyion Collision [PDF]
An experimental overview of the energy dependence of strangeness production is presented. The strange hadrons are considered a good probe to study the QCD matter created in relativistic nucleus-nucleus collisions.
Nasim Md
doaj +1 more source
Strange Quark Star (SQS) in Tolman IV potential with density dependent B-parameter and charge
In this paper, the solutions of Einstein–Maxwell Field Equations for relativistic strange quark star in Tolman-IV potential considering MIT bag model EoS $$p=\frac{1}{3}(\rho -4B)$$ p = 1 3 ( ρ - 4 B ) of interior matter in presence of charge in higher ...
K. B. Goswami+3 more
doaj +1 more source