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The reversible Frank model is capable of amplifying the initial smallstatistical deviations from the idealized racemic composition. This temporaryamplification can be interpreted as a chiral excursion in a dynamic phasespace. It is well known that if the system is open to matter and energyexchange, a permanently chiral state can be reached asymptotically, while thefinal state is necessarily racemic if the system is closed. In this work, wecombine phase space analysis, stability analysis and numerical simulations tostudy the initial chiral excursions and determine how they depend on whetherthe system is open, semi-open or closed.

Temporary mirror symmetry breaking and chiral excursions in open and closed systems