Stochastic Stabilization of the Cosmic Microwave Background Radiation

Details Stochastic Stabilization of the Cosmic Microwave Background Radiation Stochastic Stabilization of the Cosmic Microwave Background Radiation

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1851d&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

Photon trajectories in models of the Universe that have constant negative spatial curvature are exponentially unstable. We demonstrate that they can be stabilized by additional random fluctuations in the curvature. The mechanism is analogous to the one responsible for stabilizing the stochastic Kapitsa pendulum. We discuss the consequences for the cosmic microwave background fluctuations.

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