Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvl..64..713b&link_type=abstract
Physical Review Letters (ISSN 0031-9007), vol. 64, Feb. 12, 1990, p. 713-716. Research supported by CONICET, Comision de Investi
Physics
32
Pulsars, Stellar Models, Equations Of State, Ground State, Hadrons, Low Pressure, Low Temperature, Quarks
Scientific paper
Deep modifications to the current strange-star structure can occur if strange matter is not stable all the way down to zero pressure. This would be the case, for example, if some stable particle is formed at relatively low pressure and/or temperature. It is shown that the inclusion of a likely specific candidate particle (quark alpha) in the strange-matter picture leads to stellar models that present more realistic behavior in the light of current pulsar understanding.
Benvenuto Omar G.
Horvath Jorge Ernesto
Vucetich Hector
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