Abstract
The galaxy bispectrum on scales around and above the equality scale receives contributions from relativistic effects. Some of these arise from lightcone deformation effects, which come from local and line-of-sight integrated contributions. Here we calculate the local contributions from the generated vector and tensor background which is formed as scalar modes couple and enter the horizon. We show that these modes are sub-dominant when compared with other relativistic contributions.
Original language | English |
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Article number | 004 |
Pages (from-to) | 1-17 |
Number of pages | 17 |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2019 |
Issue number | 03 |
DOIs | |
Publication status | Published - 1 Mar 2019 |
Keywords
- astro-ph.CO
- gr-qc
- RCUK
- STFC
- ST/P000592/1
- ST/N000668/1
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Jolicoeur, S. (Creator), Allahyari, A. (Creator), Clarkson, C. (Creator), Larena, J. (Creator), Umeh, O. (Creator) & Maartens, R. (Creator), IOP Publishing, 1 Mar 2019
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