pith. sign in

CP Conservation in the Presence of Instantons,

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

4 Pith papers citing it

years

2026 4

verdicts

UNVERDICTED 4

representative citing papers

A Near-Cutoff Waveguide Haloscope for sub-meV Dark Matter

hep-ph · 2026-05-15 · unverdicted · novelty 7.0

A novel waveguide haloscope concept using near-cutoff slow-wave response for sub-meV bosonic dark matter, projecting dark photon sensitivity of ε≈2.1×10^{-15} at 0.1 meV.

Searching for axions with quantum interferometry

hep-ph · 2026-04-14 · unverdicted · novelty 6.0

Axion-photon coupling imprints measurable Aharonov-Bohm and Berry phases in superconducting circuits and interferometers, projecting sensitivity to g_aγγ ~ 7.8e-14 GeV^{-1} at m_a ~ 1e-10 eV.

Gravitational Waves from Matter Perturbations of Spectator Scalar Fields

hep-ph · 2026-04-06 · unverdicted · novelty 5.0

A spectator scalar field with strong portal coupling to the inflaton sources a stochastic gravitational wave background reaching Ω_GW h² ∼ 10^{-11} at frequencies 10^7-10^8 Hz for benchmark parameters σ/λ ≃ 10^4 and T_reh = 2×10^{14} GeV.

citing papers explorer

Showing 4 of 4 citing papers.

  • A Near-Cutoff Waveguide Haloscope for sub-meV Dark Matter hep-ph · 2026-05-15 · unverdicted · none · ref 9

    A novel waveguide haloscope concept using near-cutoff slow-wave response for sub-meV bosonic dark matter, projecting dark photon sensitivity of ε≈2.1×10^{-15} at 0.1 meV.

  • RadioAxion results on the search for axion dark matter under Gran Sasso hep-ex · 2026-02-20 · unverdicted · none · ref 10

    The RadioAxion experiment at Gran Sasso found no evidence for axion dark matter induced periodic modulations in 241Am decays and derived constraints on the axion decay constant for masses from 10^{-21} to 10^{-9} eV.

  • Searching for axions with quantum interferometry hep-ph · 2026-04-14 · unverdicted · none · ref 3

    Axion-photon coupling imprints measurable Aharonov-Bohm and Berry phases in superconducting circuits and interferometers, projecting sensitivity to g_aγγ ~ 7.8e-14 GeV^{-1} at m_a ~ 1e-10 eV.

  • Gravitational Waves from Matter Perturbations of Spectator Scalar Fields hep-ph · 2026-04-06 · unverdicted · none · ref 22

    A spectator scalar field with strong portal coupling to the inflaton sources a stochastic gravitational wave background reaching Ω_GW h² ∼ 10^{-11} at frequencies 10^7-10^8 Hz for benchmark parameters σ/λ ≃ 10^4 and T_reh = 2×10^{14} GeV.