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Stability Properties of the Starobinsky Cosmological Model

U. Kasper·S. Kluske·M. Rainer·S. Reuter·H. -J. Schmidt
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Abstract

We discuss the instabilities appearing in the cosmological model with a quasi de Sitter phase following from a fourth-order gravity theory. Both the classical equation as well as the quantization in form of a Wheeler - De Witt equation are conformally related to the analogous model with Einstein's theory of gravity with a minimally coupled scalar field. Results are: 1. In the non-tachyonic case, classical fourth-order gravity is not more unstable than Einstein's theory itself. 2. The well-known classically valid conformal relation is also (at least for some typical cases) valid on the level of the corresponding Wheeler - De Witt equations, which turns out to be a non-trivial statement. (to appear in: Proc. Sem. Relativistic Astrophysics Potsdam 1994, Ed .: J. Mücket)

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U. Kasper, S. Kluske, M. Rainer, S. Reuter, H. -J. Schmidt. 1994-10-21. Stability Properties of the Starobinsky Cosmological Model. https://arxiv.org/abs/gr-qc/9410030

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