Excursion into Quantum Gravity via Inflation
arXiv:1403.5100 · doi:10.1016/j.physletb.2014.08.022
Abstract
The discovery of B-modes, and their effect on the fit to inflationary parameters, opens a window to explore quantum gravity. In this paper we adopt an effective theory approach to study quantum gravity effects in inflation. We apply this approach to chaotic and inflation, and find that BICEP2 constrains these new operators to values which are consistent with the effective theory approach. This result opens the possibility to study quantum gravity in a systematic fashion, including its effect on Higgs inflation and other Starobisnky-like models.
10 pages, 3 figures
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Cited by in corpus (10)
- Embedding inflation into the Standard Model - more evidence for classical scale invariance
- Resurrecting Quadratic Inflation in No-Scale Supergravity in Light of BICEP2
- Saving Natural Inflation
- Reconstructing inflationary potential from BICEP2 and running of tensor modes
- BICEP2, the Higgs Mass and the SUSY-breaking Scale
- Theoretical bounds on dark matter masses
- Hidden Sector and Gravity
- A possible solution to the Hubble tension from quantum gravity
- Curvaton and quantum gravity effect on the tensor to scalar ratio of the chaotic inflation
- Implications of Quantum Gravity for Dark Matter