Results 11 to 20 of about 2,490,142 (296)

Medium modification of strange hadronic resonances at SIS, RHIC and LHC energies [PDF]

open access: yesEPJ Web of Conferences, 2018
The properties of strange pseudoscalar and vectors mesons as well as strange baryon resonances in dense matter are reviewed. Some open questions on the properties of strange hadrons in medium are addressed, such as the experimental signatures of inmedium
Tolos Laura
doaj   +2 more sources

Strange matter prospects within the string-flip model [PDF]

open access: yesEPJ Web of Conferences, 2018
In this contribution we extend the recently developed two-flavor quark-matter string-flip model by including strange quarks. We discuss implications for compact stars.
Bastian Niels-Uwe F.   +6 more
doaj   +4 more sources

Strange-Matter Stars [PDF]

open access: yes, 1994
This paper gives an overview of the properties of all possible equilibrium sequences of compact strange-matter stars with nuclear crusts, which range from strange stars to strange dwarfs. In contrast to their non-strange counterparts--neutron stars and white dwarfs--their properties are determined by two (rather than one) parameters, the central star ...
Weber, F.   +3 more
openaire   +2 more sources

HADES Overview [PDF]

open access: yesEPJ Web of Conferences, 2022
In March 2019 the HADES experiment recorded 14 billion Ag+Ag collisions at √SNN = 2.55 GeV$\sqrt {{S_{{\rm{NN}}}}} = 2\.55\,{\rm{GeV}}$SNN=2.55 GeV as a part of the FAIR phase-0 physics program.
Spies Simon
doaj   +1 more source

Strange quark matter and proto-strange stars in an equivaparticle model [PDF]

open access: yes, 2021
The properties of strange quark matter and the structures of (proto-)strange stars are studied within the framework of an equivparticle model, where a new quark mass scaling and self-consistent thermodynamic treatment are adopted.
Xia, C. J.   +5 more
core   +1 more source

Quark stars with 2.6 $$M_\odot $$ M ⊙ in a non-minimal geometry-matter coupling theory of gravity

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

Theory progress at Strange Quark Matter 2021 [PDF]

open access: yesEPJ Web of Conferences, 2022
I review recent theory progress reported at the 19th International Conference on Strangeness in Quark Matter (SQM), and discuss open questions to be addressed by the coming editions of SQM.
Schenke Björn
doaj   +1 more source

Strange hadronic matter

open access: yesPhysical Review Letters, 1993
We have studied the composition, stability, and production mechanisms of strange hadronic matter. By applying the RMF model to systems of nucleons, Λ’s, Σ’s, and Ξ’s, stable systems with hyperon lifetimes and charge to mass ratio close to zero are obtained. In this extended model, purely hyperonic matter consisting of lambda’s and cascades is predicted.
Schaffner, Jürgen   +4 more
openaire   +2 more sources

Strange matter

open access: yesInternational Journal of Modern Physics A
Pulsar-like objects are extremely compact, with an average density that exceeds nuclear saturation density, where the fundamental strong interaction plays an essential role, particularly in the low-energy regime. The internal structures and properties of those objects are profoundly connected to phenomena such as supernova explosions, gamma-ray bursts (
Chengjun Xia, Xiaoyu Lai, Renxin Xu
openaire   +3 more sources

Boiling of strange-quark matter [PDF]

open access: yesPhysical Review D, 1991
Boiling of strange-quark matter is studied assuming baryon chemical equilibrium between a quark phase described by the bag model, and a hadron phase described by Walecka's mean-field theory. Boiling of quark nuggets at high temperatures is shown to be much less efficient than previously believed. Thus quark nuggets with large baryon numbers may survive
, Madsen, , Olesen
openaire   +2 more sources

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