Pith. sign in

REVIEW 3 cited by

Constraining Monodromy Inflation

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 1303.2616 v3 pith:KRZEF44K submitted 2013-03-11 astro-ph.CO hep-phhep-th

Hiranya Peiris , Richard Easther , Raphael Flauger This is my paper
classification astro-ph.COhep-phhep-th
keywords potentialangulardatainflationinflationarymodulatedmonodromynon-gaussianity
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We use cosmic microwave background (CMB) data from the 9-year WMAP release to derive constraints on monodromy inflation, which is characterized by a linear inflaton potential with a periodic modulation. We identify two possible periodic modulations that significantly improve the fit, but it is unclear whether this improvement is associated with a "signal" or with the scatter in the measured angular power spectrum. The unmodulated potential is mildly favored by standard model selection criteria. A modulated inflationary potential can generate substantial primordial non-Gaussianity, of a specific and characteristic form. For the best-fit parameters to the WMAP angular power spectrum, the corresponding non-Gaussianity might be detectable in upcoming CMB data, allowing nontrivial consistency checks on the predictions of a modulated inflationary potential.

Discussion (0). Sign in to comment.

Forward citations

Cited by 3 Pith papers

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

  1. Inverse-k Primordial Oscillations from a Symbolic Regression Search

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    Symbolic regression on Planck and Planck+ACT+SPT independently selects an inverse-k primordial oscillation cos(B/k)≈cos(4/k) that weakly outperforms linear and log templates.

  2. Searching for primordial features with radio surveys: synergy between the power spectrum and bispectrum

    astro-ph.CO 2026-06 unverdicted novelty 5.0 of 10

    Joint power spectrum and bispectrum analysis from future HI intensity mapping surveys improves constraints on primordial feature amplitudes by 30-40% and achieves percent-level precision on oscillation frequencies whe...

  3. Tightening constraints on primordial oscillations with latest ACT and SPT data

    astro-ph.CO 2025-07 conditional novelty 5.0 of 10

    Combining ACT DR6, SPT-3G D1, and Planck CMB data tightens the 95% upper limits on primordial oscillation amplitudes to about 0.029, with no significant signal.

Pith tools