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eFTC-260501
The Schrodinger-Einstein-Bauer Geometric Effect and Total Energy in General Relativity |
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| Author: Y. Leblanc (eFieldTheory.COM) Email: AbstractIt is common knowledge that the spacetime metric is asymptotically flat at spatial infinity. It is false to believe however that the asymptotic spacetime is galilean. Although it describes the vacuum, its energy is generally not trivial when calculated in terms of orthogonal curvilinear coordinates and can actually diverge at infinity. This is the Schrodinger-Einstein-Bauer (SEB) geometric effect. It disappears however for the so-called normal vacuum, which is the Special Relativity vacuum in cartesian (galilean) coordinates. In the present work, we re-analyze the problem of the calculation of total energy in General Relativity for any systems in arbitrary curvilinear coordinates, and which takes into account the SEB effect and its physical consequences. Copyright © 2026 Yvan Leblanc. All rights reserved
PACS: 4.60.+n, 11.17.+y, 97.60.Lf Cite as: Leblanc, Y., "The Schrodinger-Einstein-Bauer Geometric Effect and Total Energy in General Relativity", Report no. eFTC-260501 (2026). http://www.efieldtheory.com/abs/?eFTC-260501; doi:10.13140/RG.2.2.12386.08648/1. |
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