Pith. sign in

REVIEW 19 cited by

Completing Natural 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 hep-ph/0409138 v1 pith:NLHMJRW5 submitted 2004-09-12 hep-ph astro-phhep-th

classification hep-phastro-phhep-th
keywords axionscaleeffectivelargesymmetryanomalousaxionsgroups
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

If the inflaton is a pseudo-scalar axion, the axion shift symmetry can protect the flatness of its potential from too large radiative corrections. This possibility, known as natural inflation, requires an axion scale which is greater than the (reduced) Planck scale. It is unclear whether such a high value is compatible with an effective field theoretical description, and if the global axionic symmetry survives quantum gravity effects. We propose a mechanism which provides an effective large axion scale, although the original one is sub-Planckian. The mechanism is based on the presence of two axions, with a potential provided by two anomalous gauge groups. The effective large axion scale is due to an almost exact symmetry between the couplings of the axions to the anomalous groups. We also comment on a possible implementation in heterotic string theory.

Discussion (0). Sign in to comment.

Forward citations

Cited by 19 Pith papers

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

  1. Extra-dimensional Origins of Chemical Potentials at the Cosmological Collider

    hep-ph 2026-07 conditional novelty 7.0 of 10

    A rolling 5D gauge-field inflaton acts as an extra-dimensional electric field, creating charged and neutral KK particles far heavier than H and yielding observable oscillatory signatures.

  2. Natural Phantom Crossing from Axion-WIMP Interactions

    hep-ph 2026-07 conditional novelty 6.0 of 10

    A Z_N-symmetric WIMP sector stores the initial axion value in its relic distribution and later generates a finite-density axion potential, producing an apparent late-time phantom crossing without ghosts.

  3. One Feature, Three Clocks: Phase-Locked Gravitational Waves, Primordial Black Holes, and Non-Gaussianity from Periodic Warm Inflation

    astro-ph.CO 2026-06 unverdicted novelty 6.0 of 10

    Periodic warm inflation imprints one log-periodic feature on the curvature spectrum that saturates asteroid-mass PBHs, generates dual-band GW backgrounds, and offsets the bispectrum phase by a quarter cycle fixed by s...

  4. Pseudo-Nambu-Goldstone inflation with $Z_N$ symmetric waterfall fields

    hep-ph 2026-05 unverdicted novelty 6.0 of 10

    Hybrid inflation model with Z_N-symmetric waterfall fields cancels quadratic radiative corrections for any N and logarithmic ones for N>2, yielding a stable inflaton potential and domain-wall-free reheating via Higgs-...

  5. Constraints on High-Frequency Gravitational Waves from Graviton-Photon Conversion in the M87 Galaxy

    hep-ph 2026-04 conditional novelty 6.0 of 10

    Graviton–photon conversion in M87's magnetic field sets h_c and Ωgw h² limits 1–5 orders of magnitude tighter than Milky Way-based bounds across 10^10–10^27 Hz.

  6. Axion-photon conversion in stochastic magnetic fields

    hep-ph 2025-12 accept novelty 6.0 of 10

    Axion-photon conversion in random Gaussian magnetic fields fixes the expectation values and variances of photon Stokes parameters, including a circular-polarization signal from helical fields.

  7. Axion USR Inflation

    astro-ph.CO 2025-07 conditional novelty 6.0 of 10

    In axion inflation with an intermediate ultra-slow-roll phase, the instability parameter collapses at the start of USR, terminating gauge production and yielding a two-peak power spectrum with P_R ∝ k^m, m>4.

  8. Coupled quintessence from an axion dark sector

    astro-ph.CO 2026-08 conditional novelty 5.0 of 10

    A coupled two-axion dark sector reproduces the apparent phantom-crossing dark energy hinted at by DESI and fits CMB, BAO, and Type Ia supernova data as well as LambdaCDM.

  9. Corrections to inflationary models induced by non-minimal coupling between scalar field and curvature

    gr-qc 2026-07 conditional novelty 5.0 of 10

    Power-law non-minimal coupling F=(H/λ)^{2n} deforms inflationary potentials, shifts r and n_S while preserving n_T=-r/8 and GR-like reheating, enabling r(1-n_S) classification of models against Planck/ACT data.

  10. Natural Metric-Affine Inflation: Reloaded

    gr-qc 2026-05 unverdicted novelty 5.0 of 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.

  11. Sharpening the Supersymmetric Axion Weak Gravity Conjecture

    hep-th 2026-05 unverdicted novelty 5.0 of 10

    The paper verifies the bound fS/|n| ≤ (π/(2 κ_d)) sqrt((d-1)/(d-2)) for axion instantons and sharpens it to fS/|n| ≤ (1/κ_4) sqrt(7/2) for supersymmetric 4d instantons using three approaches in the string landscape.

  12. Dimming of Photon Ring due to Photon-Axion Conversion around Kerr Black Holes

    gr-qc 2026-05 unverdicted novelty 5.0 of 10

    Photon-axion conversion near Kerr black holes produces dimming of photon spectral luminosity that increases with black hole spin, magnetic field strength, and photon-axion coupling, most efficiently at high frequencies.

  13. New Particles at the Z-Pole: Tera-Z factories as discovery and precision machines

    hep-ph 2025-11 unverdicted novelty 5.0 of 10

    Tera-Z factories can produce millions of heavy neutral leptons and billions of axion-like particles under optimistic assumptions, turning them into exotics factories for discovery and detailed study.

  14. ACT-ing on inflation: Implications of non Bunch-Davies initial condition and reheating on single-field slow roll models

    astro-ph.CO 2025-05 unverdicted novelty 5.0 of 10

    Non-Bunch-Davies initial conditions substantially improve the fit of various single-field slow-roll inflation models to updated n_s-r constraints from ACT DR6 combined with Planck, DESI, and BICEP/Keck data.

  15. A multi-axion model of inflation and dark matter

    hep-ph 2026-07 reject novelty 4.0 of 10

    A 300-mode Kaluza-Klein axion tower is proposed as a unified inflaton and dark-matter sector, but the lightest state's quoted lifetime contradicts the paper's own decay-rate formula.

  16. What to do with a Ricci-flat Calabi--Yau metric?

    hep-th 2026-05 unverdicted novelty 3.0 of 10

    Numerical Ricci-flat Calabi–Yau metrics turn string compactifications from topological existence statements into computable geometries, unlocking normalized couplings, spectra, and metric-level tests of mirror symmetry.

  17. Noncanonical Approaches To Inflation

    gr-qc 2019-06 unverdicted novelty 3.0 of 10

    A review thesis covering Mukhanov parametrization, general scalar-tensor theories, and new slow-roll techniques for canonical and noncanonical inflation observables.

  18. Rich Phenomenology from Simple Ingredients: A Review of Confining Dark Sectors

    hep-ph 2026-06 unverdicted novelty 2.0 of 10

    Review of confining dark sectors summarizing dark matter candidates, abundance mechanisms, discovery channels, and applications to the abundance similarity puzzle.

  19. The landscape of QCD axion models

    hep-ph 2020-03 unverdicted novelty 2.0 of 10

    Review classifies QCD axion models extending the standard mass-coupling window and updates bounds from cosmology, astrophysics, and experiments.

Pith tools