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Yamamoto, K., Tada, M., Kishimoto, Y., Shibata, M., Kominato, K., Ooishi, T., Yamada, S., Saida, T., Funahashi, H., Masaike, A. and Matsuki, S. (2010) The Rydberg-Atom-Cavity Axion Search.
https://arxiv.org/abs/hep-ph/0101200

has been cited by the following article:

• TITLE: Cosmological and Tokamak Signatures of GW and Gravitons

  AUTHORS: Andrew W. Beckwith, Fangyu Li, Gary V. Stephenson

  KEYWORDS: Torsion, Entanglement, Initial GW Frequencies, HUP (Heisenberg Uncertainty Principle), Black Holes

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.12 No.4, October 21, 2026

  ABSTRACT: First, we consider the cosmological geometry of toroidal space, as given in earlier papers. Secondly, we explore how to simulate this toroidal geometry and the emissions thereof using Tokamak GW experimental signatures, albeit in a scaled-down manner. Thirdly, we explore the sensitivity of a HFGW (High Frequency Gravitational Wave) detection device, as given by Pro. Fangyu Li of Chongqing University, and the detection of Tokamak plasma-created GW (Gravitational wave) strain values as low as 10−26 in lieu of GW (Gravitational wave) frequencies as high as 60 GHz (60 Gigahertz). This paper is intended to be a preliminary planning document as to how to extend the design concepts given in ITER and other advanced Tokamak generators as to GW (Gravitational wave) development. Appendix A in particular allows foundational issues as to Tokamak detection to be built up as a way to enrich engagement in the basics of GW detection and Gravitons.