Gravitational wave memory: further examples
P. -M. Zhang, Q. -L. Zhao, M. Elbistan, P. A. Horvathy
TL;DR
The paper investigates gravitational wave memory by analyzing geodesics in a four-dimensional Brinkmann metric with memory profile $\mathcal{A}(U)$, comparing velocity memory ($VM$) and displacement memory ($DM$) across several profiles. It demonstrates that Gaussian and Pöschl–Teller profiles yield $DM$ in the attractive sector but not in the repulsive sector, while the $|U|^{-4}$ profile produces $DM$ in the attractive transverse direction with no $DM$ in the repulsive direction unless the trajectory is trivially zero; the flyby derivatives can yield $DM$ or $DM-2$ depending on gluing, and a double-square potential enables parameter-tuned $DM$ (e.g., $h a = m\pi + \pi/4$). The results refine Zel'dovich–Polnarev’s claim by showing that pure displacement memory is achievable only for specific wave parameters, whereas broader profiles can yield mixed memory (including $DM-2$). Overall, the work connects early expectations with concrete analytic and approximate solutions, clarifying how memory signatures depend on profile shape, gluing choices, and derivative order of the profile $\mathcal{A}(U)$.$
Abstract
Ehlers and Kundt [1] argued in favor of the velocity effect: particles initally at rest hit by a burst of gravitational waves should fly apart with constant velocity after the wave has passed. Zel'dovich and Polnarev [2] suggested instead that waves generated by flyby would be merely displaced. Their prediction is confirmed provided the wave parameters take some particular values.
