Hyperbolic Geometry in the Work of Johann Heinrich Lambert Athanase Papadopoulos, Guillaume Théret
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Download Report 2010-12
RESEARCH REPORt 2010—2012 MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science Cover: Aurora borealis paintings by William Crowder, National Geographic (1947). The International Geophysical Year (1957–8) transformed research on the aurora, one of nature’s most elusive and intensely beautiful phenomena. Aurorae became the center of interest for the big science of powerful rockets, complex satellites and large group efforts to understand the magnetic and charged particle environment of the earth. The auroral visoplot displayed here provided guidance for recording observations in a standardized form, translating the sublime aesthetics of pictorial depictions of aurorae into the mechanical aesthetics of numbers and symbols. Most of the portait photographs were taken by Skúli Sigurdsson RESEARCH REPORT 2010—2012 MAX-PLANCK-INSTITUT FÜR WISSENSCHAFTSGESCHICHTE Max Planck Institute for the History of Science Introduction The Max Planck Institute for the History of Science (MPIWG) is made up of three Departments, each administered by a Director, and several Independent Research Groups, each led for five years by an outstanding junior scholar. Since its foundation in 1994 the MPIWG has investigated fundamental questions of the history of knowl- edge from the Neolithic to the present. The focus has been on the history of the natu- ral sciences, but recent projects have also integrated the history of technology and the history of the human sciences into a more panoramic view of the history of knowl- edge. Of central interest is the emergence of basic categories of scientific thinking and practice as well as their transformation over time: examples include experiment, ob- servation, normalcy, space, evidence, biodiversity or force. -
James Clerk Maxwell
Conteúdo Páginas Henry Cavendish 1 Jacques Charles 2 James Clerk Maxwell 3 James Prescott Joule 5 James Watt 7 Jean-Léonard-Marie Poiseuille 8 Johann Heinrich Lambert 10 Johann Jakob Balmer 12 Johannes Robert Rydberg 13 John Strutt 14 Michael Faraday 16 Referências Fontes e Editores da Página 18 Fontes, Licenças e Editores da Imagem 19 Licenças das páginas Licença 20 Henry Cavendish 1 Henry Cavendish Referência : Ribeiro, D. (2014), WikiCiências, 5(09):0811 Autor: Daniel Ribeiro Editor: Eduardo Lage Henry Cavendish (1731 – 1810) foi um físico e químico que investigou isoladamente de acordo com a tradição de Sir Isaac Newton. Cavendish entrou no seminário em 1742 e frequentou a Universidade de Cambridge (1749 – 1753) sem se graduar em nenhum curso. Mesmo antes de ter herdado uma fortuna, a maior parte das suas despesas eram gastas em montagem experimental e livros. Em 1760, foi eleito Fellow da Royal Society e, em 1803, um dos dezoito associados estrangeiros do Institut de France. Entre outras investigações e descobertas de Cavendish, a maior ocorreu em 1781, quando compreendeu que a água é uma substância composta por hidrogénio e oxigénio, uma reformulação da opinião de há milénios de que a água é um elemento químico básico. O químico inglês John Warltire (1725/6 – 1810) realizou uma Figura 1 Henry Cavendish (1731 – 1810). experiência em que explodiu uma mistura de ar e hidrogénio, descobrindo que a massa dos gases residuais era menor do que a da mistura original. Ele atribuiu a perda de massa ao calor emitido na reação. Cavendish concluiu que algum erro substancial estava envolvido visto que não acreditava que, dentro da teoria do calórico, o calor tivesse massa suficiente, à escala em análise. -
4. Alexandrian Mathematics After Euclid — I I I
4. Alexandrian mathematics after Euclid — I I I Due to the length of this unit , it has been split into three parts . This is the final part , and it deals with other Greek mathematicians and scientists from the period . The previously described works or Archimedes and Apollonius represent the deepest and most original discoveries in Greek geometry that have been passed down to us over the ages (there were probably others that did not survive) , and indeed they pushed the classical methods to their limits . More powerful tools would be needed to make further advances , and these were not developed until the 17 th century . Much of the subsequent activity in ancient Greek mathematics was more directed towards developing the trigonometry and spherical geometry needed for observational astronomy and studying questions of an arithmetic nature . At the beginning of this period there was also a resurgence of activity in astronomy and its related mathematics which continued the tradition of Babylonian mathematics in the Seleucid Empire ( c. 300 B.C.E. – 63 B.C.E) , and although there must have been some interaction , its precise extent is unclear . Eratosthenes of Cyrene Eratosthenes (276 – 197 B.C.E.) probably comes as close as anyone from this period to reaching the levels attained by Euclid , Archimedes and Apollonius . He is probably best known for applying geometric and trigonometric ideas to estimate the diameter of the earth to a fairly high degree of accuracy ; this work is summarized on pages 186 – 188 of Burton . Within mathematics itself , his main achievement was to give a systematic method for finding all primes which is known as the sieve of Eratosthenes. -
The Astronomical Work of Carl Friedrich Gauss
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector HISTORIA MATHEMATICA 5 (1978), 167-181 THE ASTRONOMICALWORK OF CARL FRIEDRICH GAUSS(17774855) BY ERIC G, FORBES, UNIVERSITY OF EDINBURGH, EDINBURGH EH8 9JY This paper was presented on 3 June 1977 at the Royal Society of Canada's Gauss Symposium at the Ontario Science Centre in Toronto [lj. SUMMARIES Gauss's interest in astronomy dates from his student-days in Gattingen, and was stimulated by his reading of Franz Xavier von Zach's Monatliche Correspondenz... where he first read about Giuseppe Piazzi's discovery of the minor planet Ceres on 1 January 1801. He quickly produced a theory of orbital motion which enabled that faint star-like object to be rediscovered by von Zach and others after it emerged from the rays of the Sun. Von Zach continued to supply him with the observations of contemporary European astronomers from which he was able to improve his theory to such an extent that he could detect the effects of planetary perturbations in distorting the orbit from an elliptical form. To cope with the complexities which these introduced into the calculations of Ceres and more especially the other minor planet Pallas, discovered by Wilhelm Olbers in 1802, Gauss developed a new and more rigorous numerical approach by making use of his mathematical theory of interpolation and his method of least-squares analysis, which was embodied in his famous Theoria motus of 1809. His laborious researches on the theory of Pallas's motion, in whi::h he enlisted the help of several former students, provided the framework of a new mathematical formu- lation of the problem whose solution can now be easily effected thanks to modern computational techniques. -
Thermodynamic Temperature
Thermodynamic temperature Thermodynamic temperature is the absolute measure 1 Overview of temperature and is one of the principal parameters of thermodynamics. Temperature is a measure of the random submicroscopic Thermodynamic temperature is defined by the third law motions and vibrations of the particle constituents of of thermodynamics in which the theoretically lowest tem- matter. These motions comprise the internal energy of perature is the null or zero point. At this point, absolute a substance. More specifically, the thermodynamic tem- zero, the particle constituents of matter have minimal perature of any bulk quantity of matter is the measure motion and can become no colder.[1][2] In the quantum- of the average kinetic energy per classical (i.e., non- mechanical description, matter at absolute zero is in its quantum) degree of freedom of its constituent particles. ground state, which is its state of lowest energy. Thermo- “Translational motions” are almost always in the classical dynamic temperature is often also called absolute tem- regime. Translational motions are ordinary, whole-body perature, for two reasons: one, proposed by Kelvin, that movements in three-dimensional space in which particles it does not depend on the properties of a particular mate- move about and exchange energy in collisions. Figure 1 rial; two that it refers to an absolute zero according to the below shows translational motion in gases; Figure 4 be- properties of the ideal gas. low shows translational motion in solids. Thermodynamic temperature’s null point, absolute zero, is the temperature The International System of Units specifies a particular at which the particle constituents of matter are as close as scale for thermodynamic temperature. -
Spherical Trigonometry Through the Ages
School of Mathematics and Statistics Newcastle University MMath Mathematics Report Spherical Trigonometry Through the Ages Author: Supervisor: Lauren Roberts Dr. Andrew Fletcher May 1, 2015 Contents 1 Introduction 1 2 Geometry on the Sphere Part I 4 2.1 Cross-sections and Measurements . .4 2.2 Triangles on the Sphere . .7 2.2.1 What is the Largest Possible Spherical Triangle? . .7 2.2.2 The Sum of Spherical Angles . .9 3 Menelaus of Alexandria 12 3.1 Menelaus' Theorem . 13 3.2 Astronomy and the Menelaus Configuration: The Celestial Sphere . 16 4 Medieval Islamic Mathematics 18 4.1 The Rule of Four Quantities . 18 4.2 Finding the Qibla . 20 4.3 The Spherical Law of Sines . 22 5 Right-Angled Triangles 25 5.1 Pythagoras' Theorem on the Sphere . 25 5.2 The Spherical Law of Cosines . 27 6 Geometry on the Sphere Part II 30 6.1 Areas of Spherical Polygons . 30 6.2 Euler's Polyhedral Formula . 33 7 Quaternions 35 7.1 Some Useful Properties . 35 7.1.1 The Quaternion Product . 36 7.1.2 The Complex Conjugate and Inverse Quaternions . 36 1 CONTENTS 2 7.2 Rotation Sequences . 37 7.2.1 3-Dimensional Representation . 39 7.3 Deriving the Spherical Law of Sines . 39 8 Conclusions 42 Bibliography 44 Abstract The art of applying trigonometry to triangles constructed on the surface of the sphere is the branch of mathematics known as spherical trigonometry. It allows new theorems relating the sides and angles of spherical triangles to be derived. The history and development of spherical trigonometry throughout the ages is discussed. -
OH Absorption Spectroscopy to Investigate Light
OH Absorption Spectroscopy to Investigate Light- Load HCCI Combustion by Sean J. Younger A thesis submitted in partial fulfillment of the requirements for a degree of Master of Science (Mechanical Engineering) at the University of Wisconsin – Madison 2005 Approved: ____________________________ Jaal B. Ghandhi Professor – Mechanical Engineering University of Wisconsin – Madison Date: ________________________ i Abstract Absorption spectroscopy of the OH molecule was used to examine the light-load limit of the HCCI combustion process. Optical results were compared to cylinder pressure and emissions data, with a focus on the transition from low to high engine-out CO emissions. The goal of the work was to experimentally verify a low-load emissions limit to practical HCCI combustion that has been predicted by detailed kinetic simulations. Two diluent mixtures were used along with 100% air to create intake charges with varying specific heats in order to highlight the temperature dependence of OH formation. Peak OH concentration data show a correlation with temperature, which agrees with theory. In general, OH absorption decreased monotonically with the mass of fuel injected per cycle for all diluent cases. The absorption spectra, which were taken with 400 µs time resolution (~1.8 CAD at 600 RPM) show that OH forms during the second- stage heat release and remains in the cylinder well into the expansion stroke. Spectral resolution did not allow a temperature measurement from absorption, so temperature was measured separately. Emissions data showed low exhaust CO concentrations at high fuel rates, and higher CO concentrations at low fueling rates. Qualitatively, the detection limit for OH coincided with the onset of increased engine-out CO emissions and the transition from strong to weak second stage heat release. -
John Wallis (1616–1703), Oxford's Savilian Professor
John Wallis (1616–1703), Oxford’s Savilian Professor of Geometry from 1649 to 1703, was the most influential English mathematician before the rise of Isaac Newton. His most important works were his Arithmetic of Infinitesimals and his treatise on Conic Sections, both published in the 1650s. It was through studying the former that Newton came to discover his version of the binomial theorem. Wallis’s last great mathematical work A Treatise of Algebra was published in his seventieth year. John Wallis Wallis’ time-line “In the year 1649 I removed to 1616 Born in Ashford, Kent Oxford, being then Publick 1632–40 Studied at Emmanuel College, Professor of Geometry, of the Cambridge Foundation of Sr. Henry Savile. 1640 Ordained a priest in the And Mathematicks which Church of England had before been a pleasing 1642 Started deciphering secret codes diversion, was now to be for Oliver Cromwell’s intelligence my serious Study.” service during the English Civil Wars John Wallis 1647 Inspired by William Oughtred’s Clavis Mathematicae (Key to Mathematics) which considerably extended his mathematical knowledge 1648 Initiated mathematical correspondence with continental scholars (Hevelius, van Schooten, etc.) 1649 Appointed Savilian Professor of Geometry at Oxford 31 October: Inaugural lecture 1655–56 Arithmetica Infinitorum (The Arithmetic of Infinitesimals) and De Sectionibus Conicis (On Conic Sections) 1658 Elected Oxford University Archivist 1663 11 July: Lecture on Euclid’s parallel postulate 1655–79 Disputes with Thomas Hobbes 1685 Treatise of Algebra 1693–99 Opera Mathematica 1701 Appointed England’s first official decipherer (alongside his grandson William Blencowe) 1703 Died in Oxford John Wallis (1616–1703) Savilian Professor During the English Civil Wars John Wallis was appointed Savilian Professor of Geometry in 1649. -
Org: Tom Archibald (SFU), Craig Fraser (Toronto) And/Et Menolly Lysne (Toronto
History and Philosophy of Mathematics Histoire et philosophie des math´ematiques (Org: Tom Archibald (SFU), Craig Fraser (Toronto) and/et Menolly Lysne (Toronto)) TOM ARCHIBALD, Simon Fraser University Galois and the Galois Theory of Differential Equations It took decades before the French mathematician Evariste´ Galois became the national and international mathematical icon that is now familiar. However, we shall show that this was well-established by the 1880s, and that competition to become the true heir to Galois’ thought was fierce in the context of establishing a “Galois theory” of differential equations. At the time, Picard, Vessiot, Drach and others display competing views of the essential character of Galois’ achievement. In this paper we assess these contrasting views, comparing them to the image of the mid-19th century and to that today. DAVID BELLHOUSE, University of Western Ontario Mathematicians in the British Financial Revolution of the Eighteenth Century Some modern historians of science have argued that during the eighteenth century practicing mathematicians had little or no impact on the pricing of life contingent products that were sold in the marketplace, although the same mathematicians wrote several books on the fair pricing of these products. For the first two-thirds of the eighteenth century, the major life contingent product was the life annuity. Annuities were sold both on the open market for privately financed schemes and through the government to finance the national debt. Through the use of several examples, it is shown that that there was a diffuse, but perhaps not very large, group of mathematicians active in the annuity and insurance marketplace during the eighteenth century. -
Bibliography
Bibliography A. Aaboe, Episodes from the Early History of Mathematics (Random House, New York, 1964) A.D. Aczel, Fermat’s Last Theorem: Unlocking the Secret of an Ancient Mathematical Problem (Four Walls Eight Windows, New York, 1996) D. Adamson, Blaise Pascal: Mathematician, Physicist, and Thinker About God (St. Martin’s Press, New York, 1995) R.P. Agarwal, H. Agarwal, S.K. Sen, Birth, Growth and Computation of Pi to ten trillion digits. Adv. Differ. Equat. 2013, 100 (2013) A.A. Al-Daffa’, The Muslim Contribution to Mathematics (Humanities Press, Atlantic Highlands, 1977) A.A. Al-Daffa’, J.J. Stroyls, Studies in the Exact Sciences in Medieval Islam (Wiley, New York, 1984) E.J. Aiton, Leibniz: A Biography (A. Hilger, Bristol, Boston, 1984) R.E. Allen, Greek Philosophy: Thales to Aristotle (The Free Press, New York, 1966) G.J. Allman, Greek Geometry from Thales to Euclid (Arno Press, New York, 1976) E.N. da C. Andrade, Sir Issac Newton, His Life and Work (Doubleday & Co., New York, 1954) W.S. Anglin, Mathematics: A Concise History and Philosophy (Springer, New York, 1994) W.S. Anglin, The Queen of Mathematics (Kluwer, Dordrecht, 1995) H.D. Anthony, Sir Isaac Newton (Abelard-Schuman, New York, 1960) H.G. Apostle, Aristotle’s Philosophy of Mathematics (The University of Chicago Press, Chicago, 1952) R.C. Archibald, Outline of the history of mathematics.Am. Math. Monthly 56 (1949) B. Artmann, Euclid: The Creation of Mathematics (Springer, New York, 1999) C.N. Srinivasa Ayyangar, The History of Ancient Indian Mathematics (World Press Private Ltd., Calcutta, 1967) A.K. Bag, Mathematics in Ancient and Medieval India (Chaukhambha Orientalia, Varanasi, 1979) W.W.R. -
Johann Lambert's Scientific Tool Kit
Johann Lambert’s Scientific Tool Kit. Maarten Bullynck To cite this version: Maarten Bullynck. Johann Lambert’s Scientific Tool Kit.: Exemplified by the Measurement of Humidity. Science in Context, Cambridge University Press (CUP), 2010, 23 (1), pp.65-89. 10.1017/S026988970999024X. halshs-00663305 HAL Id: halshs-00663305 https://halshs.archives-ouvertes.fr/halshs-00663305 Submitted on 26 Jan 2012 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Maarten Bullynck Université Paris 8 Vincennes à St.-Denis Département d'Histoire / Mathématiques & Histoire des Sciences 2 rue de la Liberté, 93526 Saint-Denis Adress: Krijgslaan 57, 9000 Gent, Belgium Email: [email protected] Telephone: 0032-484 634495 Title of the paper: J.H. Lambert’s Scientific Tool Kit. (Exemplified by Lambert’s Measurement of Humidity, 1769–1772) Abstract: J.H. Lambert (1728-1777) developed a very detailed theory of science and experiment. Using Lambert's hygrometric studies, this article provides an introduction into Lambert's theory and its practice. Of special interest in Lambert's theory are a well-founded theory on the emergence and definition of concepts and his neat neat eye for heuristics that should ultimately lead up to a mathematization of physical phenomena. -
Two Heirs to the Great Chain of Being
TWO HEIRS TO THE GREAT CHAIN OF BEING Two heirs to the great chain of being B. B. Mandelbrot Think of the satiric poetry of Jonathan Swift (1667-1745) and the writings of Immanuel Kant (1724- 1804) before he achieved fame. How would it be that both contributed to the revolution that shook mathematics in the years 1875-1922 and then ----- through fractal geometry ----- reaches diverse natural sciences? The question, at first foolish, improves upon acquaintance ----- as this sketch hopes to demonstrate. It also turns out to bear most directly on the great mystery of the practical usefulness of mathematics, or ----- using the grand phrase by Eugene Wigner (1902-1995) ----- of the unreasonable effectiveness of mathematics in the natural sciences. Stated in the grandest terms, the question deals with the seemingly necessary and unavoidable relations between the purest thought and the most real reality. Thanks to fractal geometry, the mathematical tools of natural science (that is, to use the classic words of Galileo Galilei (1 - ) its ‘‘geometrical alphabet),’’ are now being extended in the most unexpected directions. This expansion challenges us to reflect again on the overall nature of the ‘‘foreign relations’’ of mathematics with the various sciences. A hundred-odd years ago mathematics veered abruptly towards unprecedented and deepening abstraction. For example, it was shown by explicit counterexamples that a continuous function may fail to have a derivative. Soon after, geometric constructions whose successive steps were familiar and individually innocuous were combined by Cantor (1845-1918), Peano (1858-1932), and Koch (1870-1924) to generate patterns that seemed on the contrary totally without precedent.