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Supernovae are the most energetic stellar events and influence theinterstellar medium by their gasdynamics and energetics. By this, both alsoaffect the star formation positively and negatively. In this paper, we reviewthe development of the complexity of investigations aiming at understanding theinterchange between supernovae and their released hot gas with the star-formingmolecular clouds. Commencing from analytical studies the paper advances tonumerical models of supernova feedback from superbubble scales to galaxystructure. We also discuss parametrizations of star-formation andsupernova-energy transfer efficiencies. Since evolutionary models from theinterstellar medium to galaxies are numerous and apply multiple recipes ofthese parameters, only a representative selection of studies can be discussedhere.

Supernova Feedback on the Interstellar Medium and Star Formation