Results 141 to 150 of about 112,699 (275)
Nuclear Physics A, 1995 Abstract Several experiments are using heavy ion collisions as a means of creating and studying strange quark matter in the laboratory. I will describe why I think it is important and interesting to look for strange quark matter, and discuss the physics addressed by the experiments that have been designed to look for it in high energy heavy ion ...
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Importance of Nonperturbative QCD Parameters for Bottom Mesons
Advances in High Energy Physics, 2014 The importance of nonperturbative quantum chromodynamics (QCD) parameters is discussed in context to the predicting power for bottom meson masses and isospin splitting.
A. Upadhyay, M. Batra
doaj +1 more source
Strange quark stars - A review [PDF]
arXiv, 2002 A pedagogical overview of strange quark matter and strange stars is presented. After a historical notation of the research and an introduction to quark matter, a major part is devoted to the physics and astrophysics of strange stars, with attention being paid to the possible ways by which neutron stars and strange stars can be distinguished in ...
arxiv
Stranger still: Kaon loops and strange quark matrix elements of the nucleon [PDF]
, 1994 M. J. Musolf, Matthias Burkardt
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The NJL model and strange-quark matter [PDF]
Europhysics Letters (EPL), 2003 8 pages, 2 figures, reference added, typos corrected, version to appear in Europhys ...
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Searching for a dark matter particle with anti-protonic atoms. [PDF]
Eur Phys J C Part Fields, 2023 Doser M, Farrar G, Kornakov G.
europepmc +1 more source
Energy Properties of Strange Quark Matter Studied in Constituent Quark Model [PDF]
, 1994 Mitsuru Ishii +2 more
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Exploring S-wave threshold effects in QCD: A heavy-light approach
Physics Letters B, 2020 QCD exhibits complex dynamics near S-wave two-body thresholds. For light mesons, we see this in the failure of quark models to explain the f0(500) and K0⁎(700) masses. For charmonium, an unexpected X(3872) state appears at the open charm threshold.
Estia Eichten, Ciaran Hughes
doaj
Erratum: Surface tension of strange-quark matter in the early Universe [PDF]
, 1991 M. S. Berger
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Strange stars: Which is the ground stage of QCD at finite baryon number [PDF]
`High Energy Phenomenology' eds. M. A. Perez & R. Huerta (World
Scientific), 1992, p. 347 - 356, 1996 Witten's conjecture about strange quark matter (`Strange Matter') being the ground state of QCD at finite baryon number is presented and stars made of strange matter (`Strange Stars') are compared to neutron stars. The only observable way in which a strange star differs from a neutron star is in its early thermal history and a detailed study of strange
arxiv