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Fuentes-Mart´ ın, M

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

3 Pith papers citing it

citation-role summary

background 2

citation-polarity summary

fields

hep-ph 3

years

2026 3

verdicts

UNVERDICTED 3

roles

background 2

polarities

background 2

representative citing papers

The KSVZ Atlas: A Unified SMEFT-ALP Framework

hep-ph · 2026-06-10 · unverdicted · novelty 6.0

A matching framework from arbitrary KSVZ UV completions to SMEFT and ALP EFT yields robust operator bounds from global fits that often dominate direct ALP searches except when mass mixing occurs.

The structure of multi-axion solutions to the strong CP problem

hep-ph · 2026-05-07 · unverdicted · novelty 6.0 · 2 refs

Multi-axion solutions to the strong CP problem produce varied mass-coupling patterns set by PQ symmetry breaking structure and QCD-EM anomaly alignment, summarized by a general sum rule for N-axion systems.

How well can the QCD axion hide?

hep-ph · 2026-04-09 · unverdicted · novelty 6.0

Multi-axion models relax the E/N bound on QCD axion photon coupling and allow subdominant dark matter contribution, but an axion-like particle is typically visible to next-generation experiments.

citing papers explorer

Showing 3 of 3 citing papers.

  • The KSVZ Atlas: A Unified SMEFT-ALP Framework hep-ph · 2026-06-10 · unverdicted · none · ref 17

    A matching framework from arbitrary KSVZ UV completions to SMEFT and ALP EFT yields robust operator bounds from global fits that often dominate direct ALP searches except when mass mixing occurs.

  • The structure of multi-axion solutions to the strong CP problem hep-ph · 2026-05-07 · unverdicted · none · ref 61 · 2 links

    Multi-axion solutions to the strong CP problem produce varied mass-coupling patterns set by PQ symmetry breaking structure and QCD-EM anomaly alignment, summarized by a general sum rule for N-axion systems.

  • How well can the QCD axion hide? hep-ph · 2026-04-09 · unverdicted · none · ref 23

    Multi-axion models relax the E/N bound on QCD axion photon coupling and allow subdominant dark matter contribution, but an axion-like particle is typically visible to next-generation experiments.