Classification of multidimensional inflationary models
S. Mignemi, H.-J. Schmidt

TL;DR
This paper classifies constant curvature spacetimes in various signatures and dimensions, providing an algorithm to identify inflationary de Sitter models within multidimensional cosmology.
Contribution
It introduces a classification scheme for multi-warped product spacetimes and offers a practical algorithm to recognize inflationary de Sitter metrics.
Findings
Classified constant curvature spaces for various dimensions and signatures.
Identified specific counts of representations for D=2 and D=3.
Developed an algorithm to distinguish inflationary de Sitter spacetimes.
Abstract
We define under which circumstances two multi-warped product spacetimes can be considered equivalent and then we classify the spaces of constant curvature in the Euclidean and Lorentzian signature. For dimension D=2, we get essentially twelve representations, for D=3 exactly eighteen. More general, for every even D, 5D+2 cases exist, whereas for every odd D, 5D+3 cases exist. For every D, exactly one half of them has the Euclidean signature. Our definition is well suited for the discussion of multidimensional cosmological models, and our results give a simple algorithm to decide whether a given metric represents the inflationary de Sitter spacetime (in unusual coordinates) or not.
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