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Dy mo co


For understanding the evolution of complex chemical or physical systems a detailed knowledge of the fundamental interaction of the matter at an atomic or molecular level is required. Typical examples include technically important processes such as combustion, fusion plasmas or discharges. A more "remote" object of practical and scientific interest is the atmosphere of our earth. In this summer school we want to apply the knowledge on collision dynamics to fascinating objects which are "far away": it is intended to bring together theoreticians and experimentalists, physicists, chemists, and astronomers, observers and modellers in order to discuss the formation and disintegration of molecular structures under the extreme conditions prevailing in dense or diffuse interstellar clouds, star forming regions, circumstellar discs or other interesting regions in our universe.

Funding Scheme

SC - High Level Scientific Conference
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Herzl Street 2
76100 Rehovot