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The dipole of the galaxy bispectrum

Research output: Contribution to journalArticle

The bispectrum will play an important role in future galaxy surveys. On large scales it is a key probe for measuring primordial non-Gaussianity which can help differentiate between different inflationary models and other theories of the early universe. On these scales a variety of relativistic effects come into play once the galaxy number-count fluctuation is projected onto our past lightcone. We show for the first time that the leading relativistic correction from these distortions in the galaxy bispectrum generates a significant dipole, mainly from relativistic redshift space distortions. The amplitude of the dipole can be more than 10% of the monopole even on equality scales. Such a dipole is absent in the Newtonian approximation to the redshift space bispectrum, so it offers a clear signature of relativistic effects on cosmological scales in large scale structure.
Original languageEnglish
Pages (from-to)L101-L104
JournalMonthly Notices of the Royal Astronomical Society
Volume486
Issue number1
Early online date6 May 2019
DOIs
Publication statusPublished - Jun 2019

Documents

  • The dipole of the galaxy bispectrum AAM

    Rights statement: This is a pre-copyedited, author-produced PDF of an article accepted for publication in MNRAS following peer review. The version of record Chris Clarkson, Eline M de Weerd, Sheean Jolicoeur, Roy Maartens, Obinna Umeh, The dipole of the galaxy bispectrum, Monthly Notices of the Royal Astronomical Society: Letters, slz066 is available online at: https://doi.org/10.1093/mnrasl/slz066.

    Accepted author manuscript (Post-print), 779 KB, PDF document

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