  We examine the binding energies of massive stripped-envelope core collapse
supernova (SECCSN) progenitors with the stellar evolution code MESA, and find
that the jittering jets explosion mechanism is preferred for explosions where
carbon-oxygen cores with masses of $>20 M_\odot$ collapse to leave a neutron
star (NS) remnant. We calculate the binding energy at core collapse under the
assumption that the remnant is a NS. Namely, stellar gas above mass coordinate
of $~1.5-2.5 M_\odot$ is ejected in the explosion. We find that the typical
binding energy of the ejecta of stripped-envelope progenitors with
carbon-oxygen core masses of $M_{CO} > 20 M_\odot$ is $E_{bind}>2 \times
10^{51} erg$. We claim that jets are most likely to explode such cores as
jet-driven explosion mechanisms can supply high energies to the explosion. We
apply our results to SN 2020qlb, which is a SECCSN with a claimed core mass of
$~30-50 M_\odot$, and conclude that the jittering jets explosion mechanism best
accounts for such an explosion that leaves a NS.
