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Abstract
Using the consistency relation in Fourier space, we derive the observed galaxy bispectrum from single-field inflation 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 effective non-Gaussianity due to general relativistic lightcone effects that could mimic a primordial non-Gaussian signal.
Original language | English |
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Article number | 050 |
Number of pages | 20 |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2018 |
Issue number | 07 |
DOIs | |
Publication status | Published - 23 Jul 2018 |
Keywords
- astro-ph.CO
- gr-qc
- hep-th
- RCUK
- STFC
- ST/N000668/1
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Data availability statement for 'The observed galaxy bispectrum from single-field inflation in the squeezed limit'.
Koyama, K. (Creator), Umeh, O. (Creator), Maartens, R. (Creator) & Bertacca, D. (Creator), University of Portsmouth, 23 Jul 2018
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Space telescope to test Einstein's theories about gravity
19/09/18 → 5/10/18
1 item of Media coverage, 1 Media contribution
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