Maximal Acceleration Is Nonrotating
Don N. Page (Canadian Institute for Advanced Research, Theoretical, Physics Institute, University of Alberta, Edmonton, Canada)

TL;DR
This paper investigates special congruences of worldlines in stationary axisymmetric spacetimes, defining locally extremal acceleration conditions and deriving explicit formulas, with applications to Kerr-Newman and astrophysical objects.
Contribution
It introduces the concept of Nonrotating Acceleration Worldlines (NAW) and related congruences, providing explicit formulas and analyzing their properties in various gravitational fields.
Findings
Formulas for SCALE properties in Kerr-Newman spacetime
SCAM is counter-rotating in weak-field limit
Applications to stars and Solar System gravitational fields
Abstract
In a stationary axisymmetric spacetime, the angular velocity of a stationary observer that Fermi-Walker transports its acceleration vector is also the angular velocity that locally extremizes the magnitude of the acceleration of such an observer, and conversely if the spacetime is also symmetric under reversing both t and phi together. Thus a congruence of Nonrotating Acceleration Worldlines (NAW) is equivalent to a Stationary Congruence Accelerating Locally Extremely (SCALE). These congruences are defined completely locally, unlike the case of Zero Angular Momentum Observers (ZAMOs), which requires knowledge around a symmetry axis. The SCALE subcase of a Stationary Congruence Accelerating Maximally (SCAM) is made up of stationary worldlines that may be considered to be locally most nearly at rest in a stationary axisymmetric gravitational field. Formulas for the angular velocity and…
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