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Cosmological Classicalization: Maintaining Unitarity under Relevant Deformations of the Einstein-Hilbert Action (1102.0313v2)

Published 1 Feb 2011 in hep-th, gr-qc, and hep-ph

Abstract: Generic relevant deformations of Einstein's gravity theory contain additional degrees of freedom that have a multi-facetted stabilization dynamics on curved spacetimes. We show that these relevant degrees of freedom are self-protected against unitarity violations by the formation of classical field lumps that eventually merge to a new background geometry. The transition is heralded by the massive decay of the original vacuum and evolves through a strong coupling regime. This process fits in the recently proposed classicalization mechanism and extends it further to free field dynamics on curved backgrounds.

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