Sneutrino Inflation with $\alpha$-attractors

Andrei Linde; Diederik Roest; Renata Kallosh; Timm Wrase

Sneutrino Inflation with $\alpha$-attractors

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 1607.08854 v2 pith:4GRIFDSH submitted 2016-07-29 hep-th astro-ph.COgr-qchep-ph

Renata Kallosh , Andrei Linde , Diederik Roest , Timm Wrase This is my paper

classification hep-thastro-ph.COgr-qchep-ph

keywords alphaattractorsinflationsneutrinoconsistencycosmologicaldataembedding

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

abstract

Sneutrino inflation employs the fermionic partners of the inflaton and stabilizer field as right-handed neutrinos to realize the seesaw mechanism for light neutrino masses. We show that one can improve the latest version of this scenario and its consistency with the Planck data by embedding it in the theory of cosmological $\alpha$-attractors.

Discussion (0). Sign in 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

Post-inflationary enhancement of adiabatic perturbations in modular cosmology
astro-ph.CO 2025-07 conditional novelty 6.0 of 10

In modular inflation models, entropic perturbations frozen during inflation are converted into curvature perturbations after inflation, producing an enhanced power spectrum while preserving the spectral index ns.

Pith tools