Gravitational Memory Effects as a Possible Contributor to Dark Matter

This paper explores a theoretical idea in which certain gravitational effects may mimic the presence of unseen mass in the universe. In this framework, matter that moves or changes configuration could leave behind temporary gravitational signatures, potentially contributing to phenomena usually attributed to dark matter in galaxies and larger cosmic structures. The mechanism is speculative and intended as a conceptual exploration, offering a new perspective on how gravitational memory or delayed interactions might influence cosmic dynamics. This work provides a foundation for further discussion, modeling, and potential observational tests within the astrophysics and cosmology communities.