In the CEJSN scenario, the accretion disk can entrain up to ~0.01-0.03 M_sun of neutron star crust material via Kelvin-Helmholtz mixing, enhancing the r-process yield.
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Mixing neutron star material into the jets in the common envelope jets supernova r-process scenario
In the CEJSN scenario, the accretion disk can entrain up to ~0.01-0.03 M_sun of neutron star crust material via Kelvin-Helmholtz mixing, enhancing the r-process yield.