Riemann Integration in the Euclidean Space

Fuente: arXiv
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Auteur principal: Segun, Akerele Olofin
Format: Preprint
Publié: 2024
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author Segun, Akerele Olofin
author_facet Segun, Akerele Olofin
contents The so-called Riemann sums have their origin in the efforts of Greek mathematicians to find the center of gravity or the volume of a solid body. These researches led to the method of exhaustion, discovered by Archimedes and described using modern ideas by MacLaurin in his \textit{Treatise of Fluxions} in 1742. At this times the sums were only a practical method for computing an area under a curve, and the existence of this area was considered geometrically obvious. The method of exhaustion consists in almost covering the space enclosed by the curve with $n$ geometric objects with well-known areas such as rectangles or triangles, and finding the limit (though this topic was very blurry at these early times) when $n$ increases. One of its most remarkable application is squaring the area $\mathcal{A}$ enclosed by a parabola and a line.
format Preprint
id arxiv_https___arxiv_org_abs_2403_19703
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Riemann Integration in the Euclidean Space
Segun, Akerele Olofin
History and Overview
The so-called Riemann sums have their origin in the efforts of Greek mathematicians to find the center of gravity or the volume of a solid body. These researches led to the method of exhaustion, discovered by Archimedes and described using modern ideas by MacLaurin in his \textit{Treatise of Fluxions} in 1742. At this times the sums were only a practical method for computing an area under a curve, and the existence of this area was considered geometrically obvious. The method of exhaustion consists in almost covering the space enclosed by the curve with $n$ geometric objects with well-known areas such as rectangles or triangles, and finding the limit (though this topic was very blurry at these early times) when $n$ increases. One of its most remarkable application is squaring the area $\mathcal{A}$ enclosed by a parabola and a line.
title Riemann Integration in the Euclidean Space
topic History and Overview
url https://arxiv.org/abs/2403.19703