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Limits on $\boldmath n {\bar n}$ oscillations from nuclear stability

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arxiv hep-ph/9907334 v2 pith:L675MPAA submitted 1999-07-13 hep-ph nucl-th

classification hep-phnucl-th
keywords nuclearlimitgammaloweroscillationstabilitytimetimes
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abstract

The relationship between the lower limit on the nuclear stability lifetime as derived from the non disappearance of `stable` nuclei ($T_{d}~\gtrsim~5.4~\times~10^{31}$ yr), and the lower limit thus implied on the oscillation time $(\tau_{n \bar n})$ of a possibly underlying neutron-antineutron oscillation process, is clarified by studying the time evolution of the nuclear decay within a simple model which respects unitarity. The order-of-magnitude result $\tau_{n \bar n} \approx 2 (T_{d}/\Gamma_{\bar n})^{1/2} > 2 \times 10^{8}$ sec, where $\Gamma_{\bar n}$ is a typical $\bar n$ nuclear annihilation width, agrees as expected with the limit on $\tau_{n \bar n}$ established by several detailed nuclear physics calculations, but sharply disagreeing by 15 orders of magnitude with a claim published recently in Phys. Rev. CRAP.

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

  1. Overdamping of Neutron-Mirror-Neutron Transitions in Neutron Stars

    hep-ph 2026-03 conditional novelty 6.5 of 10

    Collisional decoherence overdamps n–n′ transitions in neutron stars, yielding Γ ≈ 4ε²/M ≪ oscillation rates and a mirror admixture suppressed by ~4ε²/M² at all times.

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