Abstract
Changes of hadronic properties in dense nuclear matter as predicted by theory have usually been investigated by means of relativistic heavy‐ion reactions. In this talk I show that observable consequences of such changes can also be seen in more elementary reactions on nuclei. Particular emphasis is put on a discussion of photonuclear reactions; examples are the dilepton production at ≈ 1 GeV and the hadron production in nuclei at 10 – 20 GeV photon energies. The observable effects are expected to be as large as in relativistic heavy‐ion collisions and can be more directly related to the underlying hadronic changes.
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