Submitted:
10 September 2025
Posted:
11 September 2025
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Abstract
Keywords:
1. Introduction
2. Theoretical Framework
3. Observational Evidence Across Four Plasma Systems
- Solar Wind (PSP): Magnetic switchbacks observed by Parker Solar Probe at 0.1–0.3 AU. Median pitch length = [2].
- Earth’s Magnetosheath (MMS): Turbulent eddies and current sheets in the post-shock region. Coherent structure scale = [3].
- Interstellar Medium (Voyager): Magnetic field correlation length beyond 120 AU. Scale = (assuming ) [4].
- Laboratory Plasma (LAPD): Alfvénic current sheets in the Large Plasma Device. Spacing = [5].

4. Discussion
- The ion inertial length is not arbitrary — it is the macroscopic projection of quantum information density.
- is measurable in classical systems — no quantum gravity experiment required.
- Plasma turbulence is not random — it is the classical shadow of quantum spacetime structure.
- AGN jets (if can be constrained, should be )
- Heliospheric boundary (IBEX/IMAP)
- Fusion plasmas (ITER, tokamaks)
5. Conclusion
References
- Yueshui Lin, Quantum Information Spacetime Theory: A Unified and Testable Framework for Quantum Gravity Based on the Physicalized Woodin Cardinal κ, August 2025. [CrossRef]
- M. Cuesta et al., Switchback Properties and Their Dependence on Solar Wind Parameters, ApJ 942, 112 (2023).
- T.-D. Phan et al., Magnetic reconnection and turbulence in the Earth’s magnetosheath, Nature Physics 17, 1163–1168 (2021).
- L. F. Burlaga et al., Magnetic field turbulence in the very local interstellar medium, ApJ 930, 115 (2022).
- S. Dorfman et al., Alfvén wave turbulence and magnetic intermittency in the Large Plasma Device, Physics of Plasmas 27, 052303 (2020).
- S. D. Bale et al., Parker Solar Probe observations of switchbacks in the young solar wind, Nature 598, 425–428 (2021).
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