Pith. sign in

REVIEW 1 cited by

General formula for the running of local fNL

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1210.1851 v2 pith:4FKEYLZT submitted 2012-10-05 astro-ph.CO gr-qchep-phhep-th

Christian T. Byrnes , Jinn-Ouk Gong This is my paper · ORCID
classification astro-ph.COgr-qchep-phhep-th
keywords dependencescalefieldmetricmulti-fieldspaceadditionallowing
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We compute the scale dependence of fNL for models of multi-field inflation, allowing for an arbitrary field space metric. We show that, in addition to multi-field effects and self interactions, the curved field space metric provides another source of scale dependence, which arises from the field-space Riemann curvature tensor and its derivatives. The scale dependence may be detectable within the near future if the amplitude of fNL is not too far from the current observational bounds.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Origin of ultra-light fields during inflation and their suppressed non-Gaussianity

    hep-th 2019-08 conditional novelty 6.0 of 10

    A scaling symmetry in a class of two-field inflation models naturally produces a massless isocurvature field whose self-interactions are suppressed, making primordial non-Gaussianity slow-roll suppressed but with a sq...

Pith tools