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Visinelli,Natural Warm Inflation,JCAP09(2011) 013 [1107.3523]

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it

citation-role summary

background 1

citation-polarity summary

fields

hep-ph 2 gr-qc 1

years

2026 1 2025 2

verdicts

UNVERDICTED 3

roles

background 1

polarities

background 1

representative citing papers

Warm Inflation with Pseudo-scalar Couplings

hep-ph · 2025-05-12 · unverdicted · novelty 7.0

Warm inflation models with pseudo-scalar couplings require inclusion of induced chemical potentials that make the thermal friction-fluctuation relation model-dependent rather than universal.

Natural Metric-Affine Inflation: Reloaded

gr-qc · 2026-05-22 · unverdicted · novelty 5.0

Combining periodic non-minimal couplings to the Nieh-Yan term and Ricci scalar in metric-affine gravity makes natural inflation viable for sub-Planckian periodicity scales.

Axions as Dark Matter, Dark Energy, and Dark Radiation

hep-ph · 2025-09-21 · unverdicted · novelty 2.0

A mini-review of axion phenomenology showing how light bosons can account for dark matter, drive cosmic acceleration, or contribute to relativistic backgrounds in the early and late Universe.

citing papers explorer

Showing 3 of 3 citing papers.

  • Warm Inflation with Pseudo-scalar Couplings hep-ph · 2025-05-12 · unverdicted · none · ref 11

    Warm inflation models with pseudo-scalar couplings require inclusion of induced chemical potentials that make the thermal friction-fluctuation relation model-dependent rather than universal.

  • Natural Metric-Affine Inflation: Reloaded gr-qc · 2026-05-22 · unverdicted · none · ref 10

    Combining periodic non-minimal couplings to the Nieh-Yan term and Ricci scalar in metric-affine gravity makes natural inflation viable for sub-Planckian periodicity scales.

  • Axions as Dark Matter, Dark Energy, and Dark Radiation hep-ph · 2025-09-21 · unverdicted · none · ref 46

    A mini-review of axion phenomenology showing how light bosons can account for dark matter, drive cosmic acceleration, or contribute to relativistic backgrounds in the early and late Universe.