Gravitational Memory: an approximate description
Plane gravitational waves play a role both in relativistic and in non-relativisitic physics, highlighted by two different mass parameters. The large-distance behaviour of a sandwich gravitational wave can be approximated by a continuous but not necessarily smooth profile, providing us with a simplified description of particle motion. Our model is consistent with the Carroll symmetry. Our strategy is illustrated by the Pöschl-Teller profile. The limitations of the sandwich approximation are discussed.