NASA NTRS · 19910019795
Dibaryons in neutron stars
Abstract
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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Olinto, Angela V., Haensel, Pawel, Frieman, Joshua A.. 1991-06-01. Dibaryons in neutron stars. https://ntrs.nasa.gov/citations/19910019795
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