Pith. sign in

REVIEW 1 cited by

Chaotic inflation in supergravity and cosmic string production

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 1303.4435 v1 pith:3ZHOE4Z2 submitted 2013-03-18 hep-th astro-ph.COgr-qchep-ph

Andrei Linde This is my paper · ORCID
classification hep-thastro-ph.COgr-qchep-ph
keywords chaoticcosmicinflationstringsupergravityanisotropybasiccontribution
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We describe a simple model of chaotic inflation in supergravity where one can easily tune not only the basic cosmological parameters such as n_{s}, r, and f_NL, but also a possible (subdominant) cosmic string contribution to the CMB anisotropy.

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. Gravitational waves from metastable cosmic strings in the delayed scaling scenario

    astro-ph.CO 2025-01 conditional novelty 5.0 of 10

    Metastable cosmic strings with delayed scaling can explain the PTA gravitational wave background with tension up to Gmu ~ 3e-5 while evading LVK bounds, producing a plateau and an f^-1/3 tail detectable by future inte...

Pith tools