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In this fifth paper of the series, we use the parametrized, sphericallysymmetric explosion method PUSH to investigate the impact of eight differentnuclear equations of state (EOS). We present and discuss the explosionproperties and the detailed nucleosynthesis yields, and predict the remnant(neutron star or black hole) for all our simulations. For this, we perform twosets of simulations. One, a complete study of non-rotating stars from 11 to 40M$_{\odot}$ at three different metallicities using the SFHo EOS. And two, asuite of simulations for four progenitors (16 M$_{\odot}$ at threemetallicities and 25 M$_{\odot}$ at solar metallicity) for eight differentnuclear EOS. We compare our predicted explosion energies and yields to observedsupernovae and to the metal-poor star HD~84937. We find EOS-dependentdifferences in the explosion properties and the nucleosynthesis yields.However, when comparing to observations, these differences are not large enoughto rule out any EOS considered in this work.

astrophysical journal/the astrophysical journal

PUSHing core-collapse supernovae to explosions in spherical symmetry V:  Equation of state dependency of explosion properties, nucleosynthesis yields,  and compact remnants