Dibaryons in neutron stars

Details Dibaryons in neutron stars Dibaryons in neutron stars

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991stin...9129109o&link_type=abstract

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Physics

Baryons, Mass Transfer, Neutron Stars, Stellar Mass, Stellar Structure, Equations Of State, Gravitational Effects, Stability, Transport Properties

Scientific paper

The effects are studied of H-dibaryons on the structure of neutron stars. It was found that H particles could be present in neutron stars for a wide range of dibaryon masses. The appearance of dibaryons softens the equations of state, lowers the maximum neutron star mass, and affects the transport properties of dense matter. The parameter space is constrained for dibaryons by requiring that a 1.44 solar mass neutron star be gravitationally stable.

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