The observed galaxy bispectrum from single-field inflation in the squeezed limit
dc.contributor.author | Koyama, Kazuya | |
dc.contributor.author | Umeh, Obinna | |
dc.contributor.author | Maartens, Roy | |
dc.contributor.author | Bertacca, Daniele | |
dc.date.accessioned | 2018-09-04T13:52:29Z | |
dc.date.available | 2018-09-04T13:52:29Z | |
dc.date.issued | 2018 | |
dc.description.abstract | Using the consistency relation in Fourier space, we derive the observed galaxy bispectrum from single- eld in ation in the squeezed limit, in which one of the three modes has a wavelength much longer than the other two. This provides a non-trivial check of the full computation of the bispectrum based on second-order cosmological perturbation theory in this limit. We show that gauge modes need to be carefully removed in the second-order cosmological perturbations in order to calculate the observed galaxy bispectrum in the squeezed limit. We then give an estimate of the e ective non- Gaussianity due to general-relativistic lightcone e ects that could mimic a primordial non-Gaussian signal. | en_US |
dc.identifier.citation | Koyama, K. et al. (2018). The observed galaxy bispectrum from single- eld in ation in the squeezed limit. Journal of Cosmology and Astroparticle Physics, 20180: 050 | en_US |
dc.identifier.issn | 1475-7516 | |
dc.identifier.uri | http://dx.doi.org/10.1088/1475-7516/2018/07/050 | |
dc.identifier.uri | http://hdl.handle.net/10566/4016 | |
dc.language.iso | en | en_US |
dc.privacy.showsubmitter | FALSE | |
dc.publisher | IOP Publishing | en_US |
dc.rights | This is a pre-print version of the article published online at: http://dx.doi.org/10.1088/1475-7516/2018/07/050 | |
dc.status.ispeerreviewed | TRUE | |
dc.subject | Fourier space | en_US |
dc.subject | Galaxy | en_US |
dc.subject | Galaxy bispectrum | en_US |
dc.subject | Single-fi eld inflation | en_US |
dc.title | The observed galaxy bispectrum from single-field inflation in the squeezed limit | en_US |
dc.type | Article | en_US |