Pith. sign in

REVIEW 1 cited by

Scalar dark matter production from the inflaton

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 2309.08305 v1 pith:YJ474HK3 submitted 2023-09-15 hep-ph astro-ph.COhep-th

classification hep-phastro-ph.COhep-th
keywords darkmatterproductioninflatonisocurvaturescalaranalyticalcandidate
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

A curved space-time is known to act as a source for particle production in environments where gravity plays a significant role. We explore this effect in a minimal setup of cosmic inflation on the production of a scalar dark matter candidate during and after the inflationary stage of the universe. We consider the production of dark matter via direct coupling to the inflaton field or from pure gravitational interactions. Cosmological constraints from structure formation and dark matter isocurvature perturbations are discussed. A new analytical expression for the isocurvature power spectrum is provided.

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

  1. Gravitational Waves from Spectator Scalar Fields

    hep-ph 2025-06 conditional novelty 4.0 of 10

    Heavy spectator scalar fields with masses near the inflationary Hubble scale generate a gravitational wave background observable across pulsar timing arrays, LISA, and ground-based interferometers, with constraints re...

Pith tools