Free neutrons survive r-process freeze-out in fast ejecta of neutron star mergers and their beta-decay heating produces a visible early kilonova precursor for mass fractions above ~0.05.
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A minimally decoupled anisotropic strange star model with MIT bag EOS and g(r)=sin(Psi r^2) reproduces observed pulsar masses up to 2.28 solar masses with radii 11.3-12.9 km while satisfying stability.
citing papers explorer
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Nucleosynthesis in the fast ejecta of a neutron star merger
Free neutrons survive r-process freeze-out in fast ejecta of neutron star mergers and their beta-decay heating produces a visible early kilonova precursor for mass fractions above ~0.05.
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Probing geometrically perturbed strange stars with minimal decoupling using millisecond pulsar timing observations
A minimally decoupled anisotropic strange star model with MIT bag EOS and g(r)=sin(Psi r^2) reproduces observed pulsar masses up to 2.28 solar masses with radii 11.3-12.9 km while satisfying stability.