corner
corner

Phys. Rev. D 15, 389–401 (1977)

Radiation damping and the expansion of the universe

Download: PDF (955 kB) Buy this article Export: BibTeX or EndNote (RIS)

P. C. Aichelburg and R. Beig
Institut für Theoretische Physik der Universität Wien, Wien, Austria

Received 22 July 1976; revised 27 September 1976; published in the issue dated 15 January 1977

An exactly soluble model consisting of a massless scalar field coupled to a harmonic oscillator considered previously in Minkowski space is generalized to spatially open Robertson-Walker cosmologies. It is shown that the dissipative behavior displayed by the system in Minkowski space when the total energy is finite is improved (weakened) by the expansion (contraction) of the universe. Further, we investigate the existence of solutions with purely retarded or purely advanced fields. We show that the system embedded in a universe which originates ("big bang") is similar to the open (external forces acting) system in Minkowski space, thus allowing for retarded but not advanced solutions.

© 1977 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.15.389
DOI:
10.1103/PhysRevD.15.389
PACS: