Strange, quark, and metastable neutron stars

Details Strange, quark, and metastable neutron stars Strange, quark, and metastable neutron stars

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pzetf..46....5k&link_type=abstract

Pis'ma v Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0370-274X), vol. 46, July 10, 1987, p. 5-8. In Russian.

Statistics

Computation

5

Metastable State, Neutron Stars, Quarks, Computational Astrophysics, Pulsars

Scientific paper

Limits on the coupling energy of stable strange quark matter are obtained. The observational consequences of the possible existence of strange, quark, and metastable neutron stars are examined; and the possibility of the Bose condensation of dibaryons in dense nuclear matter is considered. It is shown that the characteristic pulsar age changes as a result of the conversion of a metastable neutron star into a quark or strange star.

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