Senikoğlu, Yorgo2024-07-122024-07-1220230001-77011572-953210.1007/s10714-023-03089-52-s2.0-85148702386https://doi.org/10.1007/s10714-023-03089-5https://hdl.handle.net/20.500.12415/7225Gravitational pulse waves are defined as step functions at the boundaries. In this setting, linearized Rarita-Schwinger equations are precisely solved in Rosen coordinates. It is found that the gravitino's energy-momentum varies with the sandwich wave's shape. The gravitino's energy density will decrease as it crosses the sandwich wave at the test field level since the background won't change.eninfo:eu-repo/semantics/openAccessSupergravityGravitational WavesExact SolutionsArticle2Q155WOS:000934589000001N/A