arXiv · 1705.05834
On the Inflationary Perturbations of Massive Higher-Spin Fields
Abstract
Cosmological perturbations of massive higher-spin fields are generated during inflation, but they decay on scales larger than the Hubble radius as a consequence of the Higuchi bound. By introducing suitable couplings to the inflaton field, we show that one can obtain statistical correlators of massive higher-spin fields which remain constant or decay very slowly outside the Hubble radius. This opens up the possibility of new observational signatures from inflation.
Explore related subjects
Keep this discovery
Alex Kehagias, Antonio Riotto. 2017-05-16. On the Inflationary Perturbations of Massive Higher-Spin Fields. https://doi.org/10.1088/1475-7516%2F2017%2F07%2F046
Cite the original work for its findings. Save a collection to share your selection of sources.