
DIE HAUPTSÄCHLICHSTEN - THEORIEN DER GEOMETRIE - IN IHRER FRÜHEREN
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HEUTIGEN ENTWICKELUNG. - HISTORISCHE MONOGRAPHIE
FRITZ SCHÜTTE.
LEIPZIG, - VERLAG VON B. G. TEUBNER. - 1888.
Seiner teueren Mutter - als schwaches Unterpfand inniger Liebe
Vorwort. - ———
Inhaltsverzeichnis. - ———
Einleitung. - ———
I. Die Geometrie vor der Mitte des 19. Jahrhunderts. - ———
This work offers a concise yet thorough survey of the main strands of geometry as they stood in the late nineteenth century. Beginning with a look at the classical foundations, it moves through the evolution of plane curves, surface theory, and the emerging study of curvature, while highlighting the pivotal contributions that reshaped the field. The author also sketches the rise of non‑Euclidean ideas and the early attempts to extend geometric thinking into higher dimensions, providing clear explanations that bridge historical context with modern terminology.
Designed for students who have already passed the introductory stage, the book balances narrative overview with an extensive bibliography that invites deeper exploration. Its careful treatment of differential geometry and the algebraic side of transformations makes it a useful reference for anyone seeking to understand how today’s geometric concepts were forged. The scholarly tone remains approachable, keeping the focus on the development of ideas rather than on exhaustive technical detail.
Language
de
Duration
~4 hours (280K characters)
Publisher of text edition
Project Gutenberg
Credits
Produced by Joshua Hutchinson, Keith Edkins and the Online Distributed Proofreading Team at http://www.pgdp.net (This file was produced from images from the Cornell University Library: Historical Mathematics Monographs collection.)
Release date
2010-09-14
Rights
Public domain in the USA.
Subjects

1862–1954
Best known as a historian of mathematics, he helped make geometry’s long story readable for both scholars and general readers. His work linked rigorous mathematical research with a deep interest in how ideas develop over time.
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