155 research outputs found
Astro-quark matter: a challenge facing astroparticle physics
Quark matter both in terrestrial experiment and in astrophysics is briefly
reviewed. Astrophysical quark matter could appear in the early Universe, in
compact stars, and as cosmic rays. Emphasis is put on quark star as the nature
of pulsars. Possible astrophysical implications of experiment-discovered sQGP
are also concisely discussed.Comment: 14 pages, 4 figures and 1 table; talk presented at CosPA2007
(International Symposium on Cosmology and Particle Astrophysics, Taipei, Nov.
13-15, 2007
Trinity of Strangeon Matter
Strangeon is proposed to be the constituent of bulk strong matter, as an
analogy of nucleon for an atomic nucleus. The nature of both nucleon matter (2
quark flavors, u and d) and strangeon matter (3 flavors, u, d and s) is
controlled by the strong-force, but the baryon number of the former is much
smaller than that of the latter, to be separated by a critical number of
. While micro nucleon matter (i.e., nuclei) is focused by
nuclear physicists, astrophysical/macro strangeon matter could be manifested in
the form of compact stars (strangeon star), cosmic rays (strangeon cosmic ray),
and even dark matter (strangeon dark matter). This trinity of strangeon matter
is explained, that may impact dramatically on today's physics.Comment: Xiamen-CUSTIPEN whorkshop on the EoS of dense matter (3-7 January
2019
PSR B1257+12: a quark star with planets?
A recent observation has shown that PSR B1257+12 could have quite small X-ray
emitting area, only about 2000 m, which is more than three orders smaller
than the canonical polar cap size. We suggest here that PSR B1257+12 could be a
low-mass quark star with radius of km and mass of M \simeq
3\times10^{-4}\msun. Such a low-mass quark star system may form in an
accretion induced collapse process or a collision process of two quark stars.Comment: 3 pages, 1figure, poster at the international conference
"Astrophysics of Compact Objects" (July 1-7, 2007, Huangshan, China
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