Results 11 to 20 of about 663,566 (334)
Strangeness and charm in QCD matter [PDF]
invited talk at Strangeness in Qaurk Matter 2004, Cape Town, Sep.
B. Kämpfer, Marcus Bluhm
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Strangeness in stellar matter [PDF]
A protoneutron star is formed immediately after the gravitational collapse of the core of a massive star. At birth, the hot and high density matter in such a star contains a large number of neutrinos trapped during collapse. Trapped neutrinos generally inhibit the presence of exotic matter -- hyperons, a kaon condensate, or quarks.
Madappa Prakash+3 more
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Confronting Strange Stars with Compact-Star Observations and New Physics
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
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Gravitational Waves from Strange Star Core–Crust Oscillation
According to the strange quark matter hypothesis, pulsars may actually be strange stars composed of self-bound strange quark matter. The normal matter crust of a strange star, unlike that of a normal neutron star, is supported by a strong electric field.
Ze-Cheng Zou+2 more
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Searching for strange quark matter objects among white dwarfs
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
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Bulk strong matter: the trinity
Our world is wonderful because of the normal but negligibly small baryonic part (i.e. atoms) although unknown dark matter and dark energy dominate the Universe.
Xiaoyu Lai, Chengjun Xia, Renxin Xu
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Sensitivity of KM3NeT/ARCA to a flux of nuclearites [PDF]
Over the past decades, theories have predicted the existence of heavy compact objects containing an extremely dense form of exotic matter named Strange Quark Matter (SQM).
Păun Alice+2 more
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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
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Strangeness and charm in nuclear matter [PDF]
The properties of strange ($K$, $\bar K$ and $\bar K^*$) and open-charm ($D$, $\bar D$ and $D^*$) mesons in dense matter are studied using a unitary approach in coupled channels for meson-baryon scattering. In the strangeness sector, the interaction with nucleons always comes through vector-meson exchange, which is evaluated by chiral and hidden gauge ...
Juan Nieves+9 more
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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
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