The Deep Orbit Parallax of Gravitational Lensing in the Context of Space-based Telescopes

Abstract: This paper proposes anchoring the isospin axis within astrophysical data reduction processes using multi-wavelength and multispectral observations. Drawing from the foundations of Zermelo–Fraenkel and Von Neumann–Bernays–Gödel set theories, the time series of black hole dynamics can be reconstructed based on local nuclear particle behaviors—an alternative to conventional atomic clock-based relativistic timekeeping. This framework enables the derivation of more objective models of celestial dynamics, including possible dark energy evidence inferred from black hole and white hole oscillations. The meta-theoretical nature of this work is complemented by white hole data analyses, enhancing cosmological theory with particle-based representations of mechanical sources in an open universe—contrasting the closed Big Bang model. Built upon the measurable hypothesis from Conformal Cyclic Cosmology, this study utilizes analytical geometry and orbital frequency modulations in space-based telescopes to link parallax phenomena with gravitational lensing effects.