Geodesic
Particle production near the cosmological singularity
Teoretičeskaâ i matematičeskaâ fizika, Tome 42 (1980) no. 1, pp. 23-36 Cet article a éte moissonné depuis la source Math-Net.Ru

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The method of definition of positive-frequency functions with the help of the causal propagator is applied to the calculation of particle production amplitude in the Robertson–Walker space-time with the flat space slice and in the Casner space-time. The propagator is defined as the Green's function with the minimal divergencies on the “Euclidean section” of the space-time. It is shown that the massless conformal invariant particles are produced in the Robertson–Walker space-time with the scale factor $a(t)=t^\lambda$, $\lambda<1$. It is demonstrated that the conformal transformation method gives the same prediction provided that the global properties of the space-time are taken into consideration. Due to catastrophical character of the particle production, Universe with the true singularity and the expansion law $a(t)=t^\lambda$, $\lambda<1$, turns out to be unstable. 
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     title = {Particle production near the cosmological singularity},
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O. Yu. Karmanov; M. B. Menskii. Particle production near the cosmological singularity. Teoretičeskaâ i matematičeskaâ fizika, Tome 42 (1980) no. 1, pp. 23-36. http://geodesic.mathdoc.fr/item/TMF_1980_42_1_a2/

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