Application of Arrhenius kinetic theory to viral eclipse: selection of bacteriophage phi X174 mutants

Analysis of the bacteriophage phi X174 eclipse period in terms of Arrhenius kinetic theory suggests the following hypothesis: mutants should exist with two concomitant physiological characteristics as their phenotype. These are an eclipse rate lower than that of the wild type at permissive temperatures for plaque formation and an eclipse rate too low at lower temperatures to permit plaque development. Thus, enrichment of a mutagenized virus population for mutants that fail to eclipse during a short period at permissive temperatures should yield eclipse mutants with the cold-sensitive (cs; nonpermissive temperature, 25 degrees C), and not the temperature-sensitive (ts; nonpermissive temperature, 42 degrees C), plaque phenotype. In several trials, the frequency of the cs phenotype in the population increased from less than 0.2% to between 2 and 4% after the enrichment step, whereas the frequency of the ts phenotype remained unchanged (less than 0.2%). Moreover, 80% of these cs mutants have eclipse rates that are 3- to 40-fold lower than that of the wild type at both 37 degrees C and 25 degrees C. The successful application of the Arrhenius theory to phi X eclipse may provide insights into the molecular mechanism whereby the phi X174 genome is delivered into the host cell. Since the eclipse kinetics of other nonenveloped viruses are similar to those of phi X174, kinetic theory may be broadly applicable in the selection and characterization of viral eclipse mutants.