Kirezli, Pınar2023-04-202023-04-2020221029-8479https://doi.org/10.1007/JHEP08(2022)003https://hdl.handle.net/20.500.11776/10958Algebraic classification of higher dimensional, shear-free, twist-free, expanding (or non-expanding) spacetime is studied with the limit of D -> infinity. Similar to classification of any arbitrary dimension D > 4, this spacetime is Type I(b) or more special, according to our calculations. However, thanks to the method of taking the limit of dimension D -> infinity, the relevant Weyl scalars become much simpler. Without solving field equations, by determining obligatory conditions to the components of Weyl scalar vanish, the spacetime is classified Type I(a), Type II(a-b-c-d), Type III(a-b), Type N and Type O for primary Weyl aligned null direciton (WAND), and Type I-i, Type IIi, Type IIIi, and Type D(a-b-c-d) for secondary WAND.en10.1007/JHEP08(2022)003info:eu-repo/semantics/openAccessClassical Theories Of GravityLarge Extra DimensionsSpacesArticle8Q1WOS:0008362714000122-s2.0-85135248457Q2