Quantum Fluctuations, Decoherence of the Mean Field, and Structure Formation in the Early Universe

Details Quantum Fluctuations, Decoherence of the Mean Field, and Structure Formation in the Early Universe Quantum Fluctuations, Decoherence of the Mean Field, and Structure Formation in the Early Universe

1995-05-24

arxiv.org/abs/gr-qc/9505046v1

Phys.Rev.D52:6770-6788,1995

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

35 pages, latex, 0 figures

Scientific paper

10.1103/PhysRevD.52.6770

We examine from first principles one of the basic assumptions of modern quantum theories of structure formation in the early universe, i.e., the conditions upon which fluctuations of a quantum field may transmute into classical stochastic perturbations, which grew into galaxies. Our earlier works have discussed the quantum origin of noise in stochastic inflation and quantum fluctuations as measured by particle creation in semiclassical gravity. Here we focus on decoherence and the relation of quantum and classical fluctuations. Instead of using the rather ad hoc splitting of a quantum field into long and short wavelength parts, the latter providing the noise which decoheres the former, we treat a nonlinear theory and examine the decoherence of a quantum mean field by its own quantum fluctuations, or that of other fields it interacts with. This is an example of `dynamical decoherence' where an effective open quantum system decoheres through its own dynamics. The model we use to discuss fluctuation generation has the inflation field coupled to the graviton field. We show that when the quantum to classical transition is properly treated, with due consideration of the relation of decoherence, noise, fluctuation and dissipation, the amplitude of density contrast predicted falls in the acceptable range without requiring a fine tuning of the coupling constant of the inflation field ($\lambda$). The conventional treatment which requires an unnaturally small $\lambda \approx 10^{-12}$ stems from a basic flaw in naively identifying classical perturbations with quantum fluctuations.

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