The Early Drama of the Hyperbolic Functions
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Section 6.7 Hyperbolic Functions 3
Section 6.7 Difference Equations to Hyperbolic Functions Differential Equations The final class of functions we will consider are the hyperbolic functions. In a sense these functions are not new to us since they may all be expressed in terms of the exponential function and its inverse, the natural logarithm function. However, we will see that they have many interesting and useful properties. Definition For any real number x, the hyperbolic sine of x, denoted sinh(x), is defined by 1 sinh(x) = (ex − e−x) (6.7.1) 2 and the hyperbolic cosine of x, denoted cosh(x), is defined by 1 cosh(x) = (ex + e−x). (6.7.2) 2 Note that, for any real number t, 1 1 cosh2(t) − sinh2(t) = (et + e−t)2 − (et − e−t)2 4 4 1 1 = (e2t + 2ete−t + e−2t) − (e2t − 2ete−t + e−2t) 4 4 1 = (2 + 2) 4 = 1. Thus we have the useful identity cosh2(t) − sinh2(t) = 1 (6.7.3) for any real number t. Put another way, (cosh(t), sinh(t)) is a point on the hyperbola x2 −y2 = 1. Hence we see an analogy between the hyperbolic cosine and sine functions and the cosine and sine functions: Whereas (cos(t), sin(t)) is a point on the circle x2 + y2 = 1, (cosh(t), sinh(t)) is a point on the hyperbola x2 − y2 = 1. In fact, the cosine and sine functions are sometimes referred to as the circular cosine and sine functions. We shall see many more similarities between the hyperbolic trigonometric functions and their circular counterparts as we proceed with our discussion. -
“An Introduction to Hyperbolic Functions in Elementary Calculus” Jerome Rosenthal, Broward Community College, Pompano Beach, FL 33063
“An Introduction to Hyperbolic Functions in Elementary Calculus” Jerome Rosenthal, Broward Community College, Pompano Beach, FL 33063 Mathematics Teacher, April 1986, Volume 79, Number 4, pp. 298–300. Mathematics Teacher is a publication of the National Council of Teachers of Mathematics (NCTM). The primary purpose of the National Council of Teachers of Mathematics is to provide vision and leadership in the improvement of the teaching and learning of mathematics. For more information on membership in the NCTM, call or write: NCTM Headquarters Office 1906 Association Drive Reston, Virginia 20191-9988 Phone: (703) 620-9840 Fax: (703) 476-2970 Internet: http://www.nctm.org E-mail: [email protected] Article reprint with permission from Mathematics Teacher, copyright April 1986 by the National Council of Teachers of Mathematics. All rights reserved. he customary introduction to hyperbolic functions mentions that the combinations T s1y2dseu 1 e2ud and s1y2dseu 2 e2ud occur with sufficient frequency to warrant special names. These functions are analogous, respectively, to cos u and sin u. This article attempts to give a geometric justification for cosh and sinh, comparable to the functions of sin and cos as applied to the unit circle. This article describes a means of identifying cosh u 5 s1y2dseu 1 e2ud and sinh u 5 s1y2dseu 2 e2ud with the coordinates of a point sx, yd on a comparable “unit hyperbola,” x2 2 y2 5 1. The functions cosh u and sinh u are the basic hyperbolic functions, and their relationship to the so-called unit hyperbola is our present concern. The basic hyperbolic functions should be presented to the student with some rationale. -
Inverse Hyperbolic Functions
INVERSE HYPERBOLIC FUNCTIONS We will recall that the function eex − − x sinh x = 2 is a 1 to 1 mapping.ie one value of x maps onto one value of sinhx. This implies that the inverse function exists. y =⇔=sinhxx sinh−1 y The function f(x)=sinhx clearly involves the exponential function. We will now find the inverse function in its logarithmic form. LET y = sinh−1 x x = sinh y THEN eey − − y x = 2 (BY DEFINITION) SOME ALGEBRAIC MANIPULATION GIVES yy− 2xe=− e MULTIPLYING BOTH SIDES BY e y yy2 21xe= e − RE-ARRANGING TO CREATE A QUADRATIC IN e y 2 yy 02=−exe −1 APPLYING THE QUADRATIC FORMULA 24xx± 2 + 4 e y = 2 22xx± 2 + 1 e y = 2 y 2 exx= ±+1 SINCE y e >0 WE MUST ONLY CONSIDER THE ADDITION. y 2 exx= ++1 TAKING LOGARITHMS OF BOTH SIDES yxx=++ln2 1 { } IN CONCLUSION −12 sinhxxx=++ ln 1 { } THIS IS CALLED THE LOGARITHMIC FORM OF THE INVERSE FUNCTION. The graph of the inverse function is of course a reflection in the line y=x. THE INVERSE OF COSHX The function eex + − x fx()== cosh x 2 Is of course not a one to one function. (observe the graph of the function earlier). In order to have an inverse the DOMAIN of the function is restricted. eexx+ − fx()== cosh x , x≥ 0 2 This is a one to one mapping with RANGE [1, ∞] . We find the inverse function in logarithmic form in a similar way. y = cosh −1 x x = cosh y provided y ≥ 0 eeyy+ − xy==cosh 2 2xe=+yy e− 02=−+exeyy− 2 yy 02=−exe +1 USING QUADRATIC FORMULA −24xx±−2 4 e y = 2 y 2 exx=± −1 TAKING LOGS yxx=±−ln2 1 { } yxx=+−ln2 1 is one possible expression { } APPROPRIATE IF THE DOMAIN OF THE ORIGINAL FUNCTION HAD BEEN RESTRICTED AS EXPLAINED ABOVE. -
Volta, the Istituto Nazionale and Scientific Communication in Early Nineteenth-Century Italy*
Luigi Pepe Volta, the Istituto Nazionale and Scientific Communication in Early Nineteenth-Century Italy* In a famous paper published in Isis in 1969, Maurice Crosland posed the question as to which was the first international scientific congress. Historians of science commonly established it as the Karlsruhe Congress of 1860 whose subject was chemical notation and atomic weights. Crosland suggested that the first international scientific congress could be considered the meeting convened in Paris on January 20, 1798 for the definition of the metric system.1 In September 1798 there arrived in Paris Bugge from Denmark, van Swinden and Aeneae from Germany, Trallès from Switzerland, Ciscar and Pedrayes from Spain, Balbo, Mascheroni, Multedo, Franchini and Fabbroni from Italy. These scientists joined the several scientists already living in Paris and engaged in the definition of the metric system: Coulomb, Mechain, Delambre, Laplace, Legendre, Lagrange, etc. English and American scientists, however, did not take part in the meeting. The same question could be asked regarding the first national congress in England, in Germany, in Switzerland, in Italy, etc. As far as Italy is concerned, many historians of science would date the first meeting of Italian scientists (Prima Riunione degli Scienziati Italiani) as the one held in Pisa in 1839. This meeting was organised by Carlo Luciano Bonaparte, Napoleon’s nephew, with the co-operation of the mathematician Gaetano Giorgini under the sanction of the Grand Duke of Tuscany Leopold II (Leopold was a member of the Royal Society).2 Participation in the meetings of the Italian scientists, held annually from 1839 for nine years, was high: * This research was made possible by support from C.N.R. -
Libreria Antiquaria Mediolanum
libreria antiquaria mediolanum Via del Carmine, 1 - 20121 milano (italy) tel. (+39) 02.86.46.26.16 - FaX (+39) 02.45.47.43.33 www.libreriamediolanum.com - e-mail: [email protected] 1. (aCCademia dei Gelati). ricreationi amorose de small worm-hole repaired in the blank margin from p. 229, thin marginal gli academici Gelati di bologna. (Follows): Psafone trattato worm-holes repaired in the last 2 ll., touching few letters. unsophisticated co- py. d’amore del medesimo Caliginoso Gelato melchiorre Zoppio. - bologna, per Gio. rossi, 1590. First edition of a rare emblems book with illustrations ascribed to agostino Carracci. two parts in one 12° volume; 96 pp. – 260 pp., 2 ll. with frontispiece and 9 the iconographic apparatus consists of the full-page etched fronti- half-page engraved emblems by agostino Carracci; contemporary limp vellum, spiece with the central emblem and 9 large and beautiful emblems. manuscript title on spine. Frontispiece slightly shaved in the lower margin, a the second part of the volume offers a treatise on love by melchior- re Zoppo. the academy was founded in 1588 by Zoppo himself and collected the most distinguished literary men and scholars of the time; the aca- demy was supported by Pope urbano Viii barberini and its cultural activities lasted until the end of the 18th century. Praz 244: “scarce”. landwehr (romanic) 4. Cicognara 1831. Frati 6471. € 3.800 2. baratotti Galerana (tarabotti arCanGe- la). la semplicità ingannata. - leiden, Gio. Sambix (i.e. Jo- hannes and daniel elzevier), 1654. 12°; 12 leaves, 307 pp. (without final 2 blank ll.); contemporary vellum, manu- script title on spine. -
2 COMPLEX NUMBERS 61 2 Complex Numbers
2 COMPLEX NUMBERS 61 2 Complex numbers Though they don’t exist, per se, complex numbers pop up all over the place when we do science. They are an especially useful mathematical tool in problems dealing with oscillations and waves in light, fluids, magnetic fields, electrical circuits, etc., • stability problems in fluid flow and structural engineering, • signal processing (Fourier transform, etc.), • quantum physics, e.g. Schroedinger’s equation, • ∂ψ i + 2ψ + V (x)ψ =0 , ∂t ∇ which describes the wavefunctions of atomic and molecular systems,. difficult differential equations. • For your revision: recall that the general quadratic equation, ax2 + bx + c =0, has two solutions given by the quadratic formula b √b2 4ac x = − ± − . (85) 2a But what happens when the discriminant is negative? For instance, consider x2 2x +2=0 . (86) − Its solutions are 2 ( 2)2 4 1 2 2 √ 4 x = ± − − × × = ± − 2 1 2 p × = 1 √ 1 . ± − 2 COMPLEX NUMBERS 62 These two solutions are evidently not real numbers! However, if we put that aside and accept the existence of the square root of minus one, written as i = √ 1 , (87) − then the two solutions, 1+ i and 1 i, live in the set of complex numbers. The − quadratic equation now can be factorised as z2 2z +2=(z 1 i)(z 1+ i)=0 , − − − − and to be able to factorise every polynomial is a very useful thing, as we shall see. 2.1 Complex algebra 2.1.1 Definitions A complex number z takes the form z = x + iy , (88) where x and y are real numbers and i is the imaginary unit satisfying i2 = 1 . -
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. -
Hyperbolic Functions Certain Combinations of the Exponential
Hyperbolic Functions Certain combinations of the exponential function occur so often in physical applications that they are given special names. Specifically, half the difference of ex and e−x is defined as the hyperbolic sine function and half their sum is the hyperbolic cosine function. These functions are denoted as follows: ex − e−x ex + e−x sinh x = and cosh x = . (1.1) 2 2 The names of the hyperbolic functions and their notations bear a striking re- semblance to those for the trigonometric functions, and there are reasons for this. First, the hyperbolic functions sinh x and cosh x are related to the curve x2 −y2 = 1, called the unit hyperbola, in much the same way as the trigonometric functions sin x and cos x are related to the unit circle x2 + y2 = 1. Second, for each identity satis- fied by the trigonometric functions, there is a corresponding identity satisfied by the hyperbolic functions — not the same identity, but one very similar. For example, using equations 1.1, we have ex + e−x 2 ex − e−x 2 (cosh x)2 − (sinh x)2 = − 2 2 1 x − x x − x = e2 +2+ e 2 − e2 − 2+ e 2 4 =1. Thus the hyperbolic sine and cosine functions satisfy the identity cosh2 x − sinh2 x =1, (1.2) which is reminiscent of the identity cos2 x + sin2 x = 1 for the trigonometric func- tions. Just as four other trigonometric functions are defined in terms of sin x and cos x, four corresponding hyperbolic functions are defined as follows: sinh x ex − e−x cosh x ex + e−x tanh x = = , cothx = = , cosh x ex + e−x sinh x ex − e−x (1.3) 1 2 1 2 sechx = = , cschx = = . -
Accurate Hyperbolic Tangent Computation
Accurate Hyperbolic Tangent Computation Nelson H. F. Beebe Center for Scientific Computing Department of Mathematics University of Utah Salt Lake City, UT 84112 USA Tel: +1 801 581 5254 FAX: +1 801 581 4148 Internet: [email protected] 20 April 1993 Version 1.07 Abstract These notes for Mathematics 119 describe the Cody-Waite algorithm for ac- curate computation of the hyperbolic tangent, one of the simpler elementary functions. Contents 1 Introduction 1 2 The plan of attack 1 3 Properties of the hyperbolic tangent 1 4 Identifying computational regions 3 4.1 Finding xsmall ::::::::::::::::::::::::::::: 3 4.2 Finding xmedium ::::::::::::::::::::::::::: 4 4.3 Finding xlarge ::::::::::::::::::::::::::::: 5 4.4 The rational polynomial ::::::::::::::::::::::: 6 5 Putting it all together 7 6 Accuracy of the tanh() computation 8 7 Testing the implementation of tanh() 9 List of Figures 1 Hyperbolic tangent, tanh(x). :::::::::::::::::::: 2 2 Computational regions for evaluating tanh(x). ::::::::::: 4 3 Hyperbolic cosecant, csch(x). :::::::::::::::::::: 10 List of Tables 1 Expected errors in polynomial evaluation of tanh(x). ::::::: 8 2 Relative errors in tanh(x) on Convex C220 (ConvexOS 9.0). ::: 15 3 Relative errors in tanh(x) on DEC MicroVAX 3100 (VMS 5.4). : 15 4 Relative errors in tanh(x) on Hewlett-Packard 9000/720 (HP-UX A.B8.05). ::::::::::::::::::::::::::::::: 15 5 Relative errors in tanh(x) on IBM 3090 (AIX 370). :::::::: 15 6 Relative errors in tanh(x) on IBM RS/6000 (AIX 3.1). :::::: 16 7 Relative errors in tanh(x) on MIPS RC3230 (RISC/os 4.52). :: 16 8 Relative errors in tanh(x) on NeXT (Motorola 68040, Mach 2.1). -
Della Matematica Del Settecento: I Logaritmi Dei Numeri Negativi
Periodico di Matematiche VII, 2, 2/3 (1994), 95-106 Una “controversia” della matematica del Settecento: i logaritmi dei numeri negativi GIORGIO T. BAGNI I LOGARITMI DEI NUMERI NEGATIVI Una delle prime raccomandazioni sollecitamente affidate, nelle aule della scuola secondaria superiore, dagli insegnanti agli allievi in procinto di affrontare gli esercizi sui logaritmi è di imporre che l’argomento di ogni logaritmo sia (strettamente) positivo. Un’incontestabile, categorica “legge” della quale gli allievi non possono non tenere conto è infatti: non esistono (nell’àmbito dei numeri reali) i logaritmi dei numeri non positivi. È forse interessante ricordare che tale “legge” ha un’importante collocazione nella storia della matematica: uno dei problemi lungamente e vivacemente discussi dai matematici del Settecento, infatti, è proprio la natura dei logaritmi dei numeri negativi [16] [24]. Nella presente nota, riassumeremo le posizioni degli studiosi che intervengono nell’aspra “controversia”, sottolineando le caratteristiche di sorprendente vitalità presenti in non poche posizioni [3] [5]. Questione centrale nella storia dei logaritmi [8] [9] [10] [23] [29] [30], il problema della natura dei logaritmi dei numeri negativi viene sollevato da una lettera di Gottfried Wilhelm Leibniz a Jean Bernoulli, datata 16 marzo 1712 [17] [20], e vede coinvolti alcuni dei più celebri matematici del XVIII secolo. Gli studiosi sono infatti divisi in due schieramenti, apertamente contrapposti: da un lato, molti matematici sostengono l’opinione di Leibniz, poi ripresa da Euler [11] [19], Walmesley [31] ed in Italia, tra gli altri, da Fontana [13] [14] e da Franceschinis [15], secondo la quale i logaritmi dei numeri negativi devono essere interpretati come quantità immaginarie. -
Diffusion of Innovations Dynamics, Biological Growth and Catenary Function
Working Paper Series, N. 1, March 2015 Diffusion of innovations dynamics, biological growth and catenary function Static and dynamic equilibria Renato Guseo Department of Statistical Sciences University of Padua Italy Abstract: The catenary function has a well-known role in determining the shape of chains and cables supported at their ends under the force of grav- ity. This enables design using a specific static equilibrium over space. Its reflected version, the catenary arch, allows the construction of bridges and arches exploiting the dual equilibrium property under uniform compression. In this paper, we emphasize a further connection with well-known aggregate biological growth models over time and the related diffusion of innovation key paradigms (e.g., logistic and Bass distributions over time) that determine self- sustaining evolutionary growth dynamics in naturalistic and socio-economic contexts. Moreover, we prove that the `local entropy function', related to a logistic distribution, is a catenary and vice versa. This special invariance may be explained, at a deeper level, through the Verlinde's conjecture on the origin of gravity as an effect of the entropic force. Keywords: Hyperbolic cosine, Catenary, Logistic model, Bass models. Final version (2015-03-18) Submitted to Physica A 1-11; third revision 6-14. Diffusion of innovations dynamics, biological growth and catenary function Contents 1 Introduction 1 2 The catenary: Definition and main characteristics 3 2.1 Some historical aspects . 4 2.2 Architecture and Gaud´ı . 4 2.3 Classic and weighted catenary . 5 3 Some growth models 6 3.1 Logistic distribution . 7 3.2 Bass's distribution . 7 4 Catenary and diffusion models 9 4.1 Static and dynamic equilibria .