Order reduction in semiclassical cosmology

Details Order reduction in semiclassical cosmology Order reduction in semiclassical cosmology

1999-01-29

arxiv.org/abs/astro-ph/9901416v1

Phys.Rev.D59:083504,1999

Astronomy and Astrophysics

Astrophysics

to be published in Phys.Rev.D vol. 59, 6 pages with 2 figures

Scientific paper

10.1103/PhysRevD.59.083504

We investigate the Robertson-Walker cosmology with Lagrangian $R+\alpha_1\hbar R^2+\alpha_2\hbar R^{\mu\nu}R_{\mu\nu} +L_{rad}$ where $L_{rad}$ means classical source with traceless energy-momentum tensor. We weaken the self-consistence condition (L. Parker, J. Z. Simon, Phys. Rev. {D47}(1993),{1339}). Quantum corrections are expressed as contributions to the effective equation of state. We show that the empty space-time is stable within the class of radiation-filled expanding universes with no order reduction of the field equations.

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