Pith. sign in

REVIEW 6 cited by

A Vacuum Accumulation Solution to the Strong CP Problem

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-th/0510053 v1 pith:BGRGGZS2 submitted 2005-10-06 hep-th

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

We suggest a solution to the strong CP problem in which there are no axions involved. The superselection rule of the \theta-vacua is dynamically lifted in such a way that an infinite number of vacua are accumulated within the phenomenologically acceptable range of \theta < 10^{-9}, whereas only a measure-zero set of vacua remains outside of this interval. The general prediction is the existence of membranes to which the standard model gauge fields are coupled. These branes may be light enough for being produced at the particle accelerators in form of the resonances with a characteristic membrane spectrum.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 6 Pith papers

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

  1. CMB Birefringence from Vacuum Interfaces

    hep-th 2026-05 unverdicted novelty 7.0 of 10

    CMB polarization rotation emerges as a Pancharatnam phase localized at dark sector vacuum interfaces, independent of redshift, frequency, and the presence of light axions.

  2. Boiling After the Dust Settles: Constraining First-Order Phase Transitions During Dark Energy Domination

    hep-ph 2025-09 conditional novelty 7.0 of 10

    CMB anisotropies from stochastic bubble nucleation constrain late-time phase transitions to release less than ~1% of dark energy when β/H⋆≲25, much tighter than Hubble-budget limits.

  3. Discretely Evanescent Dark Energy

    hep-th 2025-06 conditional novelty 6.0 of 10

    Dark energy is proposed to be the vacuum energy of a hidden QCD-like sector, set by a topological phase, which decays in discrete membrane-nucleation steps and may vanish within roughly the current age of the universe.

  4. Solving the strong CP problem in string-inspired theories with modular invariance

    hep-ph 2025-05 conditional novelty 6.0 of 10

    Modular invariance can suppress the QCD theta angle to zero in string-inspired supersymmetric models with positive modular weights and non-trivial gauge kinetic functions, while the CKM phase stays large.

  5. A Quantal Theory of Restoration of Strong CP Symmetry

    hep-ph 2025-05 unverdicted novelty 6.0 of 10

    A mechanism is proposed where the CP violating phase relaxes in discrete steps via nucleation of membranes that discharge the magnetic dual of a 4-form flux, with bubbles colliding and percolating near the chiral symm...

  6. Electromagnetic Couplings of Dark Domain Walls

    hep-th 2026-02 reject novelty 4.0 of 10

    A Chern–Simons coupling between photons and a dark 3-form is claimed to rotate CMB polarization by ~10^-3 rad when light crosses dark domain walls, but the derivation has boundary-condition errors and the signal is fi...

Pith tools