Pith. sign in

REVIEW 4 cited by

UV Freeze-in in Starobinsky 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 2006.02442 v2 pith:ZJKTW2SO submitted 2020-06-03 hep-ph astro-ph.COgr-qc

classification hep-phastro-ph.COgr-qc
keywords darkmatterabundancedecayeffectivefreeze-ininflationinflaton
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

In the Starobinsky model of inflation, the observed dark matter abundance can be produced from the direct decay of the inflaton field only in a very narrow spectrum of close-to-conformal scalar fields and spinors of mass $\sim 10^7$ GeV. This spectrum can be, however, significantly broadened in the presence of effective non-renormalizable interactions between the dark and the visible sectors. In particular, we show that UV freeze-in can efficiently generate the right dark matter abundance for a large range of masses spanning from the keV to the PeV scale and arbitrary spin, without significantly altering the heating dynamics. We also consider the contribution of effective interactions to the inflaton decay into dark matter.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 4 Pith papers

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

  1. Tunnelling out of Starobinsky inflation: Raising the spectral tilt

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

    A first-order phase-transition exit from a displaced Starobinsky branch truncates ~12 e-folds, shifting the spectral tilt from n_s≈0.965 to ≈0.973 at r≈2×10⁻³.

  2. Dark Matter Ultraviolet Freeze-in in General Reheating Scenarios

    hep-ph 2025-01 accept novelty 6.0 of 10

    The paper derives analytic dark matter freeze-in yields for arbitrary power-law reheating histories and maps the gravitational production parameter space.

  3. The Goldstone Awakens: Unimodular dark energy in scale-invariant $R^2$ gravity

    astro-ph.CO 2026-07 conditional novelty 5.0 of 10

    In a scale-invariant R² + unimodular-gravity model, the Goldstone boson of scale symmetry becomes thawing dark energy, with its equation of state fixed by the same coupling that sets the inflationary spectral tilt.

  4. Starobinsky Inflation and the Latest CMB Data: A Subtle Tension?

    astro-ph.CO 2025-11 conditional novelty 4.0 of 10

    When implemented directly in CLASS, Starobinsky inflation remains consistent with Planck+ACT+BAO data at the 2σ level, but the inferred e-fold range sits above the reheating-motivated window, and a fitted R³ correctio...

Pith tools