Theoretical bounds on the tensor-to-scalar ratio in the cosmic microwave background

Abstract

Tensor modes in the cosmic microwave background are one of the most robust signatures of inflation. We derive theoretical bounds on the tensor fraction, as a generalization of the well-known Lyth bound. Under reasonable assumptions, the new bounds are at least two orders of magnitude stronger than the original one. We comment on a previously derived generalization, the so-called Efstathiou-Mack relationship. We also derive a new absolute upper bound on tensors using de Sitter entropy bounds.

4 pages, 1 figure. Minor typos corrected and Figure problem fixed. Abstract and title updated. Matches published version in PRD

References in corpus (3)

• CMBPol Mission Concept Study: Probing Inflation with CMB Polarization
• A Microscopic Limit on Gravitational Waves from D-brane Inflation
• The Volume of the Universe after Inflation and de Sitter Entropy

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