Can QPOs constrain Strange Matter?

Details Can QPOs constrain Strange Matter? Can QPOs constrain Strange Matter?

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.250o&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

Recent observations of 4U 1820-30 by RXTE have indicated a limiting QPO frequency of 1060 Hzs. If this is evidence for the marginally stable orbit of a neutron star it would correspond to a neutron star mass above the maximum mass for Strange Stars for most strange matter parameters. This would significantly constrain the parameter space for strange matter.

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