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Using the \textit{ab initio} symmetry-adapted no-core shell model, we computesum rules and response functions for light to medium-mass nuclei, starting frominteractions that are derived in the chiral effective field theory. Weinvestigate electromagnetic transitions of monopole, dipole and quadrupolenature for symmetric nuclei such as $^4$He, $^{16}$O, $^{20}$Ne and $^{40}$Ca.Furthermore, we study giant monopole resonance, which can provide informationon the incompressibility of symmetric nuclear matter.

Response functions and giant monopole resonances for light to medium-mass nuclei from the \textit{ab initio} symmetry-adapted no-core shell model