Pith. sign in

REVIEW 1 cited by

Non-Gaussian perturbations in hybrid inflation

Not yet reviewed by Pith; the record is open.

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 hep-ph/0405103 v2 pith:FPQ5RUWM submitted 2004-05-12 hep-ph astro-ph

classification hep-phastro-ph
keywords sigmahybridinflationperturbationsnon-gaussianitiesapplycaseconsider
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

We consider second order inflationary perturbations in the case of two scalar fields, $\sigma$ and the inflaton $\phi$. We derive an expression for the non-Gaussianity of perturbations and apply the results to hybrid inflation. We isolate the contributions due to $\sigma$ and evaluate the resulting terms to show that $\sigma$-induced non-Gaussianities dominate over inflaton-induced non-Gaussianities when $m^2_{\sigma} \gtrsim \eta H^2$, where $\eta$ is the slow-roll parameter. This may provide a useful test of hybrid inflation in forthcoming CMB experiments.

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