Strangeness in strongly interacting matter [PDF]
18 pages, 7 figures, uses iopams.sty; Invited opening talk at the 6th International Conference on Strange Quarks in Matter 2001 (SQM2001),Frankfurt, Germany, 25-29 Sep 2001; revised and accepted version for publication in Journal of Physics ...
Carsten Greiner
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Search for Strange Quark Matter and Nuclearites on Board the International Space Station (SQM-ISS): A Future Detector to Search for Massive, Non-Relativistic Objects in Space [PDF]
SQM-ISS is a detector that will search from the International Space Station for massive particles possibly present among the cosmic rays. Among them, we mention strange quark matter, Q-Balls, lumps of fermionic exotic compact stars, Primordial Black ...
Massimo Bianchi+21 more
doaj +2 more sources
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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Strange stars within bosonic and fermionic admixed dark matter [PDF]
In this work, we study dark matter (DM) admixed strange quark stars exploring the different possibilities about the nature of the DM and their effects on the macroscopic properties of strange stars, such as maximum masses, radii, as well the ...
L. Lopes, H. C. Das
semanticscholar +1 more source
Strange magnetars admixed with fermionic dark matter [PDF]
We discuss strange stars admixed with fermionic dark matter in the presence of a strong magnetic field using the two-fluid Tolman-Oppenheimer-Volkov equations.
O. Ferreira, E. Fraga
semanticscholar +1 more source
Compact star merger events with stars composed of interacting strange quark matter [PDF]
We investigate the properties of stars participating in double compact star merger events considering interacting model of stable strange quark matter.
Anil Kumar, V. Thapa, M. Sinha
semanticscholar +1 more source
Vector dark boson mediated feeble interaction between fermionic dark matter and strange quark matter in quark stars [PDF]
We study the structural properties like the gravitational mass, radius and tidal deformability of dark matter (DM) admixed strange quark stars (SQSs).
Debashree Sen, Atanu Guha
semanticscholar +1 more source
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
openaire +5 more sources
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
doaj +1 more source
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
doaj +1 more source