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Memory effect for generalized modes in pp-waves spacetime

F. L. Carneiro, H. P. de Carvalho, M. P. Lobo, L. A. Cabral

Abstract

The memory effect of test particles interacting with pp-wave Gaussian pulses is investigated for polarization modes beyond the standard quadrupolar $+$ and $\times$ states. Massive geodesic equations are solved numerically for several values of the multipolar index $m$, allowing the analysis of velocity and energy memory effects. In order to eliminate possible coordinate artifacts, the study is formulated in terms of the relative motion between two test particles. The results show that the relative kinetic energy variation exhibits a quartic dependence on the wave amplitude in the regime of low initial velocities. The coefficient of this scaling is found to depend on the multipolar structure of the wave, reflecting the spatial gradients associated with higher polarization modes. It is further shown that the energy memory effect is determined by the integrated tidal field, linking the permanent change in the relative kinetic energy to the history of the spacetime curvature carried by the wave.13

Memory effect for generalized modes in pp-waves spacetime

Abstract

The memory effect of test particles interacting with pp-wave Gaussian pulses is investigated for polarization modes beyond the standard quadrupolar and states. Massive geodesic equations are solved numerically for several values of the multipolar index , allowing the analysis of velocity and energy memory effects. In order to eliminate possible coordinate artifacts, the study is formulated in terms of the relative motion between two test particles. The results show that the relative kinetic energy variation exhibits a quartic dependence on the wave amplitude in the regime of low initial velocities. The coefficient of this scaling is found to depend on the multipolar structure of the wave, reflecting the spatial gradients associated with higher polarization modes. It is further shown that the energy memory effect is determined by the integrated tidal field, linking the permanent change in the relative kinetic energy to the history of the spacetime curvature carried by the wave.13

Paper Structure

This paper contains 12 sections, 62 equations, 9 figures.

Figures (9)

  • Figure 1: Deformation of a particle ring of radius $R=1$ caused by a pp-wave of mode $m=2$. The wave parameters are $A=1$ and $\Lambda=0.15$.
  • Figure 2: Out-of-plane deformation of a particle ring of radius $R=1$ caused by a pp-wave with $+$ polarization. The wave parameters are $A=1$ and $\Lambda=0.15$.
  • Figure 3: Classical kinetic energy \ref{['kinetic']} variation for a pp-wave with $+$ polarization.
  • Figure 4: Kinetic energy variation for the same particle displayed in Fig. \ref{['fig3']}b, but for another amplitude.
  • Figure 5: Deformation of a particle ring of radius $R=1$ caused by pp-waves of higher modes. The wave parameters are $A=1$ and $\Lambda=0.15$.
  • ...and 4 more figures