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We consider a possible crystalline equation of state (EOS) that follows fromnucleons that are chiral solitons with deep relativistic quark bound states. Inthis model conventional quark matter does not occur till a high densitythreshold at which the quark bound states in the nucleons get compressed andmerge with the continuum. Once the barrier at this threshold is overcome,roughly when, $n_B \sim 1/fm^3$, we expect the crystalline nuclear matter tomake a sudden transition into quark matter when the EOS becomes soft through adecompression. The sudden increase in density triggers a collapse releasinglarge amount of gravitational potential energy that can generate a sphericaloutburst (or kilonova) of ejected matter.

Probing spherical outbursts of neutron star mergers from an equation of state with composite nucleons