关于马达瓦及其对 $π$ 的马达瓦-莱布尼兹数列的修正项

V. N. Krishnachandran
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引用次数: 0

摘要

本文旨在达到两个目的:其一,根据现代历史学术研究,介绍喀拉拉邦天文学和数学学派的创始人桑伽玛-摩挲达瓦(Sangamagr\=ama M\adhava)的生平;其二,对归功于摩挲达瓦的三个神秘的修正术语进行批判性研究,以便在使用摩挲达瓦-莱布尼兹数列计算$\pi$值时获得更精确的值;其三,对摩挲达瓦的三个神秘的修正术语进行批判性研究,以便在使用摩挲达瓦-莱布尼兹数列计算$\pi$值时获得更精确的值;其四,对摩挲达瓦的三个神秘的修正术语进行批判性研究。为了第二个目的,我们收集了描述这些校正术语的原始梵文诗句、它们的英译本以及它们在现代符号中的表述。我们还对喀拉拉邦使用这些修正术语的理由进行了严格审查。这方面的总体结论是,即使修正项给出了高精度的$\pi$ 值近似值,喀拉拉邦作者提出的理由也不足以说服现代数学学术界。作者通过提出更高阶的修正项对 M\adhava 的结果进行了扩展,这些修正项比 M\adhava 提出的修正项对 $\pi$ 产生了更好的近似值。作者还讨论了 M\=adhava 和他的弟子们利用 M\=adhava 的修正项从基本的 M\=adhava-Leibniz 序列得到的 $/pi$ 的各种无穷序列表示。此外,还介绍了一些使用作者开发的更好的修正项的此类序列表示。本文还讨论了关于 M\=adhavam 可能最初是如何得出修正项的各种猜想。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On Mādhava and his correction terms for the Mādhava-Leibniz series for $π$
This paper is intended to serve two purposes: one, to present an account of the life of Sangamagr\=ama M\=adhava, the founder of the Kerala school of astronomy and mathematics which flourished during the 15th - 18th centuries, based on modern historical scholarship and two, to present a critical study of the three enigmatic correction terms, attributed to M\=adhava, for obtaining more accurate values of $\pi$ while computing its value using the M\=adhava-Leibniz series. For the second purpose, we have collected together the original Sanskrit verses describing the correction terms, their English translations and their presentations in modern notations. The Kerala rationale for these correction terms are also critically examined. The general conclusion in this regard is that, even though the correction terms give high precision approximations to the value of $\pi$, the rationale presented by Kerala authors is not strong enough to convince modern mathematical scholarship. The author has extended M\=adhava's results by presenting higher order correction terms which yield better approximations to $\pi$ than the correction terms attributed to M\=adhava. The various infinite series representations of $\pi$ obtained by M\=adhava and his disciples from the basic M\=adhava-Leibniz series using M\=adhava's correction terms are also discussed. A few more such series representations using the better correction terms developed by the author are also presented. The various conjectures regarding how M\=adhava might have originally arrived at the correction terms are also discussed in the paper.
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