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Phys. Rev. Lett. 69, 3606–3609 (1992)

Entropy of a classical stochastic field and cosmological perturbations

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R. Brandenberger, V. Mukhanov, and T. Prokopec
Physics Department, Brown University, Providence, Rhode Island 02912
Institute of Theoretical Physics, Eidgenössische Technische Hochschule Hönggerberg, CH-8093 Zürich, Switzerland
Institute for Theoretical Physics, University of California, Santa Barbara, California 93106

Received 26 June 1992; published in the issue dated 21 December 1992

We propose a general definition of nonequilibrium entropy of a classical stochastic field. As an example of particular interest in cosmology we apply this definition to compute the entropy of density perturbations in an inflationary Universe. On the scales of structures in the Universe, the entropy of density perturbations dominates over the statistical fluctuations of the entropy of cosmic microwave photons, indicating the relevance of the entropy of density fluctuations for structure formation.

© 1992 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.69.3606
DOI:
10.1103/PhysRevLett.69.3606
PACS:
98.80.Cq, 04.20.Cv, 05.20.Gg