Properties of strange-matter stars

Details Properties of strange-matter stars Properties of strange-matter stars

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994stin...9520873w&link_type=abstract

Presented at the International Conference Nuclei in the Cosmos, Gran Sasso, Italy, 8-13 Jul. 1994

Computer Science

Baryons, Iron Isotopes, Neutron Stars, Quarks, White Dwarf Stars, Amount, Hypotheses, Observation

Scientific paper

This paper deals with an investigation of the properties of hypothetical strange-matter stars, which are composed of u, d, s quark matter whose energy per baryon number lies below the one of Fe-56 (Witten's strange matter hypothesis). Observable quantities which allow to distinguish such objects from their 'conventional' counterparts, neutron stars and white dwarfs, are pointed out.

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