riemannian geometry in English

noun
1
a form of differential non-Euclidean geometry developed by Riemann, used to describe curved space. It provided Einstein with a mathematical basis for his general theory of relativity.
His interests had turned away from affine and projective differential geometry and turned towards Riemannian geometry .

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1. In 1880 he became a lecturer of mathematics at the University of Padua where he dealt with Riemannian geometry and differential quadratic forms.

2. In particular, when M is a (pseudo-)Riemannian manifold and ∇ is the Levi-Civita connection, then the affine geodesic are the usual geodesics of Riemannian geometry and are the locally distance minimizing curves.