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arXiv · 2308.03796

Superluminal Transformations in Spacetimes of Definite Metric

Kent A. Peacock
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Abstract

This paper reviews and extends an approach to superluminal kinematics set forth by R. Sutherland and J. Shepanski in 1986. This theory is characterized by a spacetime with positive definite metric, a Lorentz factor of the form $1/\sqrt{β^2 - 1}$, and real-valued proper times and proper lengths for superluminal reference frames.

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Kent A. Peacock. 2023-08-04. Superluminal Transformations in Spacetimes of Definite Metric. https://arxiv.org/abs/2308.03796

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