Generic 3-point Statistics with Tensor Modes in Light of Swampland and TCC
arXiv:2003.14066 · doi:10.1140/epjc/s10052-022-10869-x
Abstract
Recently proposed Swampland Criteria (SC) and Trans-Planckian Censorship Conjecture (TCC) together put stringent theoretical constraints on slow roll inflation, raising a question on future prospects of detection of Primordial Gravitational Waves (PGW). As it appears, the only option to relax the constraints is by considering Non Bunch Davies (NBD) initial states, that in turn brings back the observational relevance of PGW via its 2-point function. In this article we develop consistent 3-point statistics with tensor modes for all possible correlators (auto and mixed) for NBD initial states in the light of SC and TCC in a generic, model independent framework of Effective Field Theory of inflation. We also construct the templates of the corresponding nonlinearity parameters for different shapes of relevance and investigate if any of the 3-point correlators could be of interest for future CMB missions. Our analysis reveals that the prospects of detecting the tensor auto correlator are almost nil whereas the mixed correlators might be relevant for future CMB missions.
20 pages, 1 figure
References in corpus (7)
- The Effective Field Theory of Inflation
- Observational Signatures and Non-Gaussianities of General Single Field Inflation
- Planck 2018 results. IX. Constraints on primordial non-Gaussianity
- A Note on Calm Excited States of Inflation
- Tensor Non-Gaussianity Search: Current Status and Future Prospects
- The trans-Planckian censorship conjecture from the swampland distance conjecture
- Minimal cut-off vacuum state constraints from CMB bispectrum statistics
Cited by in corpus (3)
- Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme
- Stochastic gravitational wave background anisotropies from inflation with non-Bunch-Davies states
- Primordial magnetic non-Gaussianity with generic vacua and detection prospects in CMB spectral distortions