Based on a recently proposed reinterpretation of gravitational wave memory
that builds up on the definition of gravitational waves pioneered by Isaacson,
we provide a unifying framework to derive both ordinary and null memory from a
single well-defined equation at leading order in the asymptotic expansion. This
allows us to formulate a memory equation that is valid for any unbound
asymptotic energy-flux that preserves local Lorentz invariance. Using Horndeski
gravity as a concrete example metric theory with an additional potentially
massive scalar degree of freedom in the gravitational sector, the general
memory formula is put into practice by presenting the first account of the
memory correction sourced by the emission of massive field waves. Throughout
the work, physical degrees of freedom are identified by constructing manifestly
gauge invariant perturbation variables within an SVT decomposition on top of
the asymptotic Minkowski background, which will in particular prove useful in
future studies of gravitational wave memory within vector tensor theories.

Unifying Framework for Gravitational Wave Memory

Based on a recently proposed reinterpretation of gravitational wave memory, we have developed a unifying framework to derive both ordinary and null memory from a single equation at leading order in the asymptotic expansion. This framework allows us to formulate a memory equation that is valid for any unbound asymptotic energy-flux, while preserving local Lorentz invariance.

Memory Correction in Horndeski Gravity

To demonstrate the practical application of the general memory formula, we have utilized Horndeski gravity as a concrete example metric theory. Horndeski gravity includes an additional potentially massive scalar degree of freedom in the gravitational sector. We present the first account of the memory correction sourced by the emission of massive field waves within this theory.

Identification of Physical Degrees of Freedom

To ensure reliable and accurate analysis, we have identified physical degrees of freedom by constructing manifestly gauge invariant perturbation variables within an SVT decomposition on top of the asymptotic Minkowski background. This approach will prove particularly useful in future studies of gravitational wave memory within vector tensor theories.

Future Roadmap: Challenges and Opportunities

  1. Expanding Memory Equation Application: The derived memory equation can be further applied to various metric theories beyond Horndeski gravity. Researchers can explore its applicability in different contexts to gain a deeper understanding of gravitational wave memory.
  2. Investigation of Massive Field Waves: The memory correction sourced by the emission of massive field waves opens up new opportunities for studying the effects of massive particles in gravitational wave memory. Future research can focus on the properties, behavior, and potential observable consequences of these waves.
  3. Generalizing to Vector Tensor Theories: The identification of physical degrees of freedom and the SVT decomposition approach provide a solid foundation for exploring gravitational wave memory within vector tensor theories. Researchers can utilize these techniques to investigate the features and implications of memory in these theories.
  4. Verification and Experimental Confirmation: Experimental validation of the derived memory equation and the effects of massive field waves will be crucial for confirming the theoretical predictions. Collaborations between theoretical physicists and experimentalists are required to design and conduct experiments that can detect and measure gravitational wave memory accurately.
  5. Enhancing Memory Detection Techniques: As our understanding of gravitational wave memory evolves, there is a need for continually improving detection techniques to capture memory effects effectively. Researchers can focus on developing new technologies, data analysis methods, and observational strategies to enhance the sensitivity and resolution of memory measurements.

Overall, the reinterpretation of gravitational wave memory and the development of a unifying framework provide a solid foundation for future advancements in this field. By expanding the application of the memory equation, investigating massive field waves, exploring vector tensor theories, verifying theoretical predictions through experiments, and enhancing detection techniques, researchers can unlock exciting new insights into gravitational wave memory.

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