Luminosity evolution of strange dwarf stars

Details Luminosity evolution of strange dwarf stars Luminosity evolution of strange dwarf stars

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phrvd..53..635b&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 53, Issue 2, 15 January 1996, pp.635-638

Physics

4

Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Quark-Gluon Plasma, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

We study the evolution of strange dwarf stars of 0.4, 0.55, and 0.8 Msolar in the range of luminosities attributed to white dwarf stars. It is shown that, if the density at the base of the normal matter envelope is slightly lower than the density at which the onset of neutron drip occurs, these objects will have an evolution observationally indistinguishable from that corresponding to normal white dwarfs. This result is independent of the chemical composition of the high density, normal matter layers. However, strange dwarfs should behave very differently from white dwarfs in mass exchanging close binary systems.

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