Lie Symmetries of Non-Relativistic and Relativistic Motions

Abstract

We study the Lie symmetries of non-relativistic and relativistic higher order constant motions, in $d$ spatial dimensions, like constant acceleration, constant rate-of-change -of-acceleration (constant jerk), and so on. In the non-relativistic case, these symmetries contain the $z=\frac{2}{N}$ Galilean conformal transformations, where $N$ is the order of the differential equation that defines the constant motion. The dimension of this group grows with $N$. In the relativistic case the vanishing of the ($d+1$)-dimensional space-time relativistic acceleration, jerk, snap, ... , is equivalent, in each case, to the vanishing of a $d$-dimensional spatial vector. These vectors are the $d$-dimensional non-relativistic ones plus additional terms that guarantee the relativistic transformation properties of the corresponding $d+1$ dimensional vectors. In the case of acceleration there are no corrections, which implies that the Lie symmetries of zero acceleration motions are the same in the non-relativistic and relativistic cases. The number of Lie symmetries that are obtained in the relativistic case does not increase from the four-derivative order (zero relativistic snap) onwards. We also deduce a recurrence relation for the spatial vectors that in the relativistic case characterize the constant motions.

arXiv commentVersion accepted for publication in PRD. Some comments and references added

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Cited by in corpus (5)

• Geometry and BMS Lie algebras of spatially isotropic homogeneous spacetimes
• Integrability of geodesic motions in curved manifolds through non-local conserved charges
• Projective collineations of decomposable spacetimes generated by the Lie point symmetries of geodesic equations
• Hidden symmetries from distortions of the conformal structure
• Observers with constant proper acceleration, constant proper jerk, and beyond