Results 21 to 30 of about 113,434 (277)

Confronting Strange Stars with Compact-Star Observations and New Physics

open access: yesUniverse, 2023
Strange stars ought to exist in the universe according to the strange quark matter hypothesis, which states that matter made of roughly equal numbers of up, down, and strange quarks could be the true ground state of baryonic matter rather than ordinary ...
Shuhua Yang   +3 more
doaj   +1 more source

The Ω− and the strange quark mass [PDF]

open access: yesNuclear Physics B - Proceedings Supplements, 2005
Three pages, proceedings of the Lattice-04 symposium. (Corrected typographical errors)
Davies, C., Toussaint, Doug
openaire   +3 more sources

Role of Quark Matter and Color Superconductivity in the Structure and Tidal Deformability of Strange Dwarfs

open access: yesUniverse, 2023
In 1995, Glendenning, Kettner and Weber postulated the existence of a new class of compact stars resembling white dwarfs but containing a small strange quark-matter core surrounded by hadronic layers attaining much higher densities than those found in ...
Loïc Perot, Nicolas Chamel
doaj   +1 more source

Centrality dependence of multistrangeness production in high-energy heavy-ion collisions [PDF]

open access: yesEPJ Web of Conferences, 2022
We compare the experimental data on yields of protons, strange Λ′s, and multistrange baryons (Ξ, Ω), and antibaryons production on nuclear targets, and the experimental ratios of multistrange to strange antibaryon production, at the energy region from ...
Arakelyan Gevorg H.   +2 more
doaj   +1 more source

Quark Matter May Not Be Strange [PDF]

open access: yesPhysical Review Letters, 2018
If quark matter is energetically favored over nuclear matter at zero temperature and pressure then it has long been expected to take the form of strange quark matter (SQM), with comparable amounts of $u$, $d$, $s$ quarks. The possibility of quark matter with only $u$, $d$ quarks ($ud$QM) is usually dismissed because of the observed stability of ...
Holdom, Bob, Ren, Jing, Zhang, Chen
openaire   +4 more sources

Light- and strange-quark mass dependence of the ρ(770) meson revisited

open access: yesJournal of High Energy Physics, 2020
Recent lattice data on ππ-scattering phase shifts in the vector-isovector channel, pseudoscalar meson masses and decay constants for strange-quark masses smaller or equal to the physical value allow us to study the strangeness dependence of these ...
R. Molina, J. Ruiz de Elvira
doaj   +1 more source

Strange Quarks and Lattice QCD [PDF]

open access: yesFew-Body Systems, 2012
The last few years have seen a dramatic improvement in our knowledge of the strange form factors of the nucleon. With regard to the vector from factors the level of agreement between theory and experiment gives us considerable confidence in our ability to calculate with non-perturbative QCD.
Thomas, A., Shanahan, P., Young, R.
openaire   +4 more sources

The crystallography of strange quark matter [PDF]

open access: yesJournal of Physics G: Nuclear and Particle Physics, 2006
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

Searching for strange quark planets

open access: yesThe Sixteenth Marcel Grossmann Meeting, 2023
Strange quark matter (SQM) may be the true ground state of matter. According to this SQM hypothesis, the observed neutron stars actually should all be strange quark stars. But distinguishing between neutron stars and strange quark stars by means of obser- vations is extremely difficult.
Wang, Xu, Huang, Yong-Feng, Li, Bing
openaire   +2 more sources

Strange Quark Star (SQS) in Tolman IV potential with density dependent B-parameter and charge

open access: yesEuropean Physical Journal C: Particles and Fields, 2022
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

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