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EnglishBy a careful implementation of gauge transformations involving long-wavelength modes, we show that a variety of effects involving squeezed bispectrum configurations, for which one Fourier mode is much shorter than the other two, cannot be gauged away, except for the unphysical exactly infinite-wavelength (k = 0) limit. Our result applies, in particular, to the Maldacena consistency relation for single-field inflation, yielding a local non-Gaussianity strength f_NLlocal = −(5/12)(nS − 1) (with nS the primordial spectral index of NL scalar perturbations), and to the f_NLGR = −5/3 term, appearing in the dark matter bispectrum and in the halo bias, as a consequence of the general relativistic non-linear evolution of matter perturbations. Such effects are therefore physical and observable in principle by future high-sensitivity experiments.
| Titolo: | Resilience of long modes in cosmological observables | |
| Autori: | ||
| Data di pubblicazione: | 2021 | |
| Rivista: | ||
| Handle: | http://hdl.handle.net/11697/155300 | |
| Appare nelle tipologie: | 1.1 Articolo in rivista |
File in questo prodotto:
| File | Descrizione | Tipologia | Licenza | |
|---|---|---|---|---|
| paper.pdf | preprint | Documento in Pre-print |  | Open Access Visualizza/Apri |
http://hdl.handle.net/11697/155300
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