Euler's Calculation of the Sum of the Reciprocals of the Squares
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Math 137 Calculus 1 for Honours Mathematics Course Notes
Math 137 Calculus 1 for Honours Mathematics Course Notes Barbara A. Forrest and Brian E. Forrest Version 1.61 Copyright c Barbara A. Forrest and Brian E. Forrest. All rights reserved. August 1, 2021 All rights, including copyright and images in the content of these course notes, are owned by the course authors Barbara Forrest and Brian Forrest. By accessing these course notes, you agree that you may only use the content for your own personal, non-commercial use. You are not permitted to copy, transmit, adapt, or change in any way the content of these course notes for any other purpose whatsoever without the prior written permission of the course authors. Author Contact Information: Barbara Forrest ([email protected]) Brian Forrest ([email protected]) i QUICK REFERENCE PAGE 1 Right Angle Trigonometry opposite ad jacent opposite sin θ = hypotenuse cos θ = hypotenuse tan θ = ad jacent 1 1 1 csc θ = sin θ sec θ = cos θ cot θ = tan θ Radians Definition of Sine and Cosine The angle θ in For any θ, cos θ and sin θ are radians equals the defined to be the x− and y− length of the directed coordinates of the point P on the arc BP, taken positive unit circle such that the radius counter-clockwise and OP makes an angle of θ radians negative clockwise. with the positive x− axis. Thus Thus, π radians = 180◦ sin θ = AP, and cos θ = OA. 180 or 1 rad = π . The Unit Circle ii QUICK REFERENCE PAGE 2 Trigonometric Identities Pythagorean cos2 θ + sin2 θ = 1 Identity Range −1 ≤ cos θ ≤ 1 −1 ≤ sin θ ≤ 1 Periodicity cos(θ ± 2π) = cos θ sin(θ ± 2π) = sin -
G-Convergence and Homogenization of Some Sequences of Monotone Differential Operators
Thesis for the degree of Doctor of Philosophy Östersund 2009 G-CONVERGENCE AND HOMOGENIZATION OF SOME SEQUENCES OF MONOTONE DIFFERENTIAL OPERATORS Liselott Flodén Supervisors: Associate Professor Anders Holmbom, Mid Sweden University Professor Nils Svanstedt, Göteborg University Professor Mårten Gulliksson, Mid Sweden University Department of Engineering and Sustainable Development Mid Sweden University, SE‐831 25 Östersund, Sweden ISSN 1652‐893X, Mid Sweden University Doctoral Thesis 70 ISBN 978‐91‐86073‐36‐7 i Akademisk avhandling som med tillstånd av Mittuniversitetet framläggs till offentlig granskning för avläggande av filosofie doktorsexamen onsdagen den 3 juni 2009, klockan 10.00 i sal Q221, Mittuniversitetet, Östersund. Seminariet kommer att hållas på svenska. G-CONVERGENCE AND HOMOGENIZATION OF SOME SEQUENCES OF MONOTONE DIFFERENTIAL OPERATORS Liselott Flodén © Liselott Flodén, 2009 Department of Engineering and Sustainable Development Mid Sweden University, SE‐831 25 Östersund Sweden Telephone: +46 (0)771‐97 50 00 Printed by Kopieringen Mittuniversitetet, Sundsvall, Sweden, 2009 ii Tothememoryofmyfather G-convergence and Homogenization of some Sequences of Monotone Differential Operators Liselott Flodén Department of Engineering and Sustainable Development Mid Sweden University, SE-831 25 Östersund, Sweden Abstract This thesis mainly deals with questions concerning the convergence of some sequences of elliptic and parabolic linear and non-linear oper- ators by means of G-convergence and homogenization. In particular, we study operators with oscillations in several spatial and temporal scales. Our main tools are multiscale techniques, developed from the method of two-scale convergence and adapted to the problems stud- ied. For certain classes of parabolic equations we distinguish different cases of homogenization for different relations between the frequen- cies of oscillations in space and time by means of different sets of local problems. -
Generalizations of the Riemann Integral: an Investigation of the Henstock Integral
Generalizations of the Riemann Integral: An Investigation of the Henstock Integral Jonathan Wells May 15, 2011 Abstract The Henstock integral, a generalization of the Riemann integral that makes use of the δ-fine tagged partition, is studied. We first consider Lebesgue’s Criterion for Riemann Integrability, which states that a func- tion is Riemann integrable if and only if it is bounded and continuous almost everywhere, before investigating several theoretical shortcomings of the Riemann integral. Despite the inverse relationship between integra- tion and differentiation given by the Fundamental Theorem of Calculus, we find that not every derivative is Riemann integrable. We also find that the strong condition of uniform convergence must be applied to guarantee that the limit of a sequence of Riemann integrable functions remains in- tegrable. However, by slightly altering the way that tagged partitions are formed, we are able to construct a definition for the integral that allows for the integration of a much wider class of functions. We investigate sev- eral properties of this generalized Riemann integral. We also demonstrate that every derivative is Henstock integrable, and that the much looser requirements of the Monotone Convergence Theorem guarantee that the limit of a sequence of Henstock integrable functions is integrable. This paper is written without the use of Lebesgue measure theory. Acknowledgements I would like to thank Professor Patrick Keef and Professor Russell Gordon for their advice and guidance through this project. I would also like to acknowledge Kathryn Barich and Kailey Bolles for their assistance in the editing process. Introduction As the workhorse of modern analysis, the integral is without question one of the most familiar pieces of the calculus sequence. -
Sequences, Series and Taylor Approximation (Ma2712b, MA2730)
Sequences, Series and Taylor Approximation (MA2712b, MA2730) Level 2 Teaching Team Current curator: Simon Shaw November 20, 2015 Contents 0 Introduction, Overview 6 1 Taylor Polynomials 10 1.1 Lecture 1: Taylor Polynomials, Definition . .. 10 1.1.1 Reminder from Level 1 about Differentiable Functions . .. 11 1.1.2 Definition of Taylor Polynomials . 11 1.2 Lectures 2 and 3: Taylor Polynomials, Examples . ... 13 x 1.2.1 Example: Compute and plot Tnf for f(x) = e ............ 13 1.2.2 Example: Find the Maclaurin polynomials of f(x) = sin x ...... 14 2 1.2.3 Find the Maclaurin polynomial T11f for f(x) = sin(x ) ....... 15 1.2.4 QuestionsforChapter6: ErrorEstimates . 15 1.3 Lecture 4 and 5: Calculus of Taylor Polynomials . .. 17 1.3.1 GeneralResults............................... 17 1.4 Lecture 6: Various Applications of Taylor Polynomials . ... 22 1.4.1 RelativeExtrema .............................. 22 1.4.2 Limits .................................... 24 1.4.3 How to Calculate Complicated Taylor Polynomials? . 26 1.5 ExerciseSheet1................................... 29 1.5.1 ExerciseSheet1a .............................. 29 1.5.2 FeedbackforSheet1a ........................... 33 2 Real Sequences 40 2.1 Lecture 7: Definitions, Limit of a Sequence . ... 40 2.1.1 DefinitionofaSequence .......................... 40 2.1.2 LimitofaSequence............................. 41 2.1.3 Graphic Representations of Sequences . .. 43 2.2 Lecture 8: Algebra of Limits, Special Sequences . ..... 44 2.2.1 InfiniteLimits................................ 44 1 2.2.2 AlgebraofLimits.............................. 44 2.2.3 Some Standard Convergent Sequences . .. 46 2.3 Lecture 9: Bounded and Monotone Sequences . ..... 48 2.3.1 BoundedSequences............................. 48 2.3.2 Convergent Sequences and Closed Bounded Intervals . .... 48 2.4 Lecture10:MonotoneSequences . -
Fundamental Theorems in Mathematics
SOME FUNDAMENTAL THEOREMS IN MATHEMATICS OLIVER KNILL Abstract. An expository hitchhikers guide to some theorems in mathematics. Criteria for the current list of 243 theorems are whether the result can be formulated elegantly, whether it is beautiful or useful and whether it could serve as a guide [6] without leading to panic. The order is not a ranking but ordered along a time-line when things were writ- ten down. Since [556] stated “a mathematical theorem only becomes beautiful if presented as a crown jewel within a context" we try sometimes to give some context. Of course, any such list of theorems is a matter of personal preferences, taste and limitations. The num- ber of theorems is arbitrary, the initial obvious goal was 42 but that number got eventually surpassed as it is hard to stop, once started. As a compensation, there are 42 “tweetable" theorems with included proofs. More comments on the choice of the theorems is included in an epilogue. For literature on general mathematics, see [193, 189, 29, 235, 254, 619, 412, 138], for history [217, 625, 376, 73, 46, 208, 379, 365, 690, 113, 618, 79, 259, 341], for popular, beautiful or elegant things [12, 529, 201, 182, 17, 672, 673, 44, 204, 190, 245, 446, 616, 303, 201, 2, 127, 146, 128, 502, 261, 172]. For comprehensive overviews in large parts of math- ematics, [74, 165, 166, 51, 593] or predictions on developments [47]. For reflections about mathematics in general [145, 455, 45, 306, 439, 99, 561]. Encyclopedic source examples are [188, 705, 670, 102, 192, 152, 221, 191, 111, 635]. -
A SIMPLE COMPUTATION of Ζ(2K) 1. Introduction in the Mathematical Literature, One Finds Many Ways of Obtaining the Formula
A SIMPLE COMPUTATION OF ζ(2k) OSCAR´ CIAURRI, LUIS M. NAVAS, FRANCISCO J. RUIZ, AND JUAN L. VARONA Abstract. We present a new simple proof of Euler's formulas for ζ(2k), where k = 1; 2; 3;::: . The computation is done using only the defining properties of the Bernoulli polynomials and summing a telescoping series, and the same method also yields integral formulas for ζ(2k + 1). 1. Introduction In the mathematical literature, one finds many ways of obtaining the formula 1 X 1 (−1)k−122k−1π2k ζ(2k) := = B ; k = 1; 2; 3;:::; (1) n2k (2k)! 2k n=1 where Bk is the kth Bernoulli number, a result first published by Euler in 1740. For example, the recent paper [2] contains quite a complete list of references; among them, the articles [3, 11, 12, 14] published in this Monthly. The aim of this paper is to give a new proof of (1) which is simple and elementary, in the sense that it involves only basic one variable Calculus, the Bernoulli polynomials, and a telescoping series. As a bonus, it also yields integral formulas for ζ(2k + 1) and the harmonic numbers. 1.1. The Bernoulli polynomials | necessary facts. For completeness, we be- gin by recalling the definition of the Bernoulli polynomials Bk(t) and their basic properties. There are of course multiple approaches one can take (see [7], which shows seven ways of defining these polynomials). A frequent starting point is the generating function 1 xext X xk = B (t) ; ex − 1 k k! k=0 from which, by the uniqueness of power series expansions, one can quickly obtain many of their basic properties. -
Leonhard Euler - Wikipedia, the Free Encyclopedia Page 1 of 14
Leonhard Euler - Wikipedia, the free encyclopedia Page 1 of 14 Leonhard Euler From Wikipedia, the free encyclopedia Leonhard Euler ( German pronunciation: [l]; English Leonhard Euler approximation, "Oiler" [1] 15 April 1707 – 18 September 1783) was a pioneering Swiss mathematician and physicist. He made important discoveries in fields as diverse as infinitesimal calculus and graph theory. He also introduced much of the modern mathematical terminology and notation, particularly for mathematical analysis, such as the notion of a mathematical function.[2] He is also renowned for his work in mechanics, fluid dynamics, optics, and astronomy. Euler spent most of his adult life in St. Petersburg, Russia, and in Berlin, Prussia. He is considered to be the preeminent mathematician of the 18th century, and one of the greatest of all time. He is also one of the most prolific mathematicians ever; his collected works fill 60–80 quarto volumes. [3] A statement attributed to Pierre-Simon Laplace expresses Euler's influence on mathematics: "Read Euler, read Euler, he is our teacher in all things," which has also been translated as "Read Portrait by Emanuel Handmann 1756(?) Euler, read Euler, he is the master of us all." [4] Born 15 April 1707 Euler was featured on the sixth series of the Swiss 10- Basel, Switzerland franc banknote and on numerous Swiss, German, and Died Russian postage stamps. The asteroid 2002 Euler was 18 September 1783 (aged 76) named in his honor. He is also commemorated by the [OS: 7 September 1783] Lutheran Church on their Calendar of Saints on 24 St. Petersburg, Russia May – he was a devout Christian (and believer in Residence Prussia, Russia biblical inerrancy) who wrote apologetics and argued Switzerland [5] forcefully against the prominent atheists of his time. -
(Sn) Converges to a Real Number S If ∀Ε > 0, ∃Ns.T
32 MATH 3333{INTERMEDIATE ANALYSIS{BLECHER NOTES 4. Sequences 4.1. Convergent sequences. • A sequence (sn) converges to a real number s if 8 > 0, 9Ns:t: jsn − sj < 8n ≥ N. Saying that jsn−sj < is the same as saying that s− < sn < s+. • If (sn) converges to s then we say that s is the limit of (sn) and write s = limn sn, or s = limn!1 sn, or sn ! s as n ! 1, or simply sn ! s. • If (sn) does not converge to any real number then we say that it diverges. • A sequence (sn) is called bounded if the set fsn : n 2 Ng is a bounded set. That is, there are numbers m and M such that m ≤ sn ≤ M for all n 2 N. This is the same as saying that fsn : n 2 Ng ⊂ [m; M]. It is easy to see that this is equivalent to: there exists a number K ≥ 0 such that jsnj ≤ K for all n 2 N. (See the first lines of the last Section.) Fact 1. Any convergent sequence is bounded. Proof: Suppose that sn ! s as n ! 1. Taking = 1 in the definition of convergence gives that there exists a number N 2 N such that jsn −sj < 1 whenever n ≥ N. Thus jsnj = jsn − s + sj ≤ jsn − sj + jsj < 1 + jsj whenever n ≥ N. Now let M = maxfjs1j; js2j; ··· ; jsN j; 1 + jsjg. We have jsnj ≤ M if n = 1; 2; ··· ;N, and jsnj ≤ M if n ≥ N. So (sn) is bounded. • A sequence (an) is called nonnegative if an ≥ 0 for all n 2 N. -
BAIRE ONE FUNCTIONS 1. History Baire One Functions Are Named in Honor of René-Louis Baire (1874- 1932), a French Mathematician
BAIRE ONE FUNCTIONS JOHNNY HU Abstract. This paper gives a general overview of Baire one func- tions, including examples as well as several interesting properties involving bounds, uniform convergence, continuity, and Fσ sets. We conclude with a result on a characterization of Baire one func- tions in terms of the notion of first return recoverability, which is a topic of current research in analysis [6]. 1. History Baire one functions are named in honor of Ren´e-Louis Baire (1874- 1932), a French mathematician who had research interests in continuity of functions and the idea of limits [1]. The problem of classifying the class of functions that are convergent sequences of continuous functions was first explored in 1897. According to F.A. Medvedev in his book Scenes from the History of Real Functions, Baire was interested in the relationship between the continuity of a function of two variables in each argument separately and its joint continuity in the two variables [2]. Baire showed that every function of two variables that is continuous in each argument separately is not pointwise continuous with respect to the two variables jointly [2]. For instance, consider the function xy f(x; y) = : x2 + y2 Observe that for all points (x; y) =6 0, f is continuous and so, of course, f is separately continuous. Next, we see that, xy xy lim = lim = 0 (x;0)!(0;0) x2 + y2 (0;y)!(0;0) x2 + y2 as (x; y) approaches (0; 0) along the x-axis and y-axis respectively. However, as (x; y) approaches (0; 0) along the line y = x, we have xy 1 lim = : (x;x)!(0;0) x2 + y2 2 Hence, f is continuous along the lines y = 0 and x = 0, but is discon- tinuous overall at (0; 0). -
Sequences and Their Limits
Sequences and their limits c Frank Zorzitto, Faculty of Mathematics University of Waterloo The limit idea For the purposes of calculus, a sequence is simply a list of numbers x1; x2; x3; : : : ; xn;::: that goes on indefinitely. The numbers in the sequence are usually called terms, so that x1 is the first term, x2 is the second term, and the entry xn in the general nth position is the nth term, naturally. The subscript n = 1; 2; 3;::: that marks the position of the terms will sometimes be called the index. We shall deal only with real sequences, namely those whose terms are real numbers. Here are some examples of sequences. • the sequence of positive integers: 1; 2; 3; : : : ; n; : : : • the sequence of primes in their natural order: 2; 3; 5; 7; 11; ::: • the decimal sequence that estimates 1=3: :3;:33;:333;:3333;:33333;::: • a binary sequence: 0; 1; 0; 1; 0; 1;::: • the zero sequence: 0; 0; 0; 0;::: • a geometric sequence: 1; r; r2; r3; : : : ; rn;::: 1 −1 1 (−1)n • a sequence that alternates in sign: 2 ; 3 ; 4 ;:::; n ;::: • a constant sequence: −5; −5; −5; −5; −5;::: 1 2 3 4 n • an increasing sequence: 2 ; 3 ; 4 ; 5 :::; n+1 ;::: 1 1 1 1 • a decreasing sequence: 1; 2 ; 3 ; 4 ;:::; n ;::: 3 2 4 3 5 4 n+1 n • a sequence used to estimate e: ( 2 ) ; ( 3 ) ; ( 4 ) :::; ( n ) ::: 1 • a seemingly random sequence: sin 1; sin 2; sin 3;:::; sin n; : : : • the sequence of decimals that approximates π: 3; 3:1; 3:14; 3:141; 3:1415; 3:14159; 3:141592; 3:1415926; 3:14159265;::: • a sequence that lists all fractions between 0 and 1, written in their lowest form, in groups of increasing denominator with increasing numerator in each group: 1 1 2 1 3 1 2 3 4 1 5 1 2 3 4 5 6 1 3 5 7 1 2 4 5 ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ;::: 2 3 3 4 4 5 5 5 5 6 6 7 7 7 7 7 7 8 8 8 8 9 9 9 9 It is plain to see that the possibilities for sequences are endless. -
Infinitesimals
Infinitesimals: History & Application Joel A. Tropp Plan II Honors Program, WCH 4.104, The University of Texas at Austin, Austin, TX 78712 Abstract. An infinitesimal is a number whose magnitude ex- ceeds zero but somehow fails to exceed any finite, positive num- ber. Although logically problematic, infinitesimals are extremely appealing for investigating continuous phenomena. They were used extensively by mathematicians until the late 19th century, at which point they were purged because they lacked a rigorous founda- tion. In 1960, the logician Abraham Robinson revived them by constructing a number system, the hyperreals, which contains in- finitesimals and infinitely large quantities. This thesis introduces Nonstandard Analysis (NSA), the set of techniques which Robinson invented. It contains a rigorous de- velopment of the hyperreals and shows how they can be used to prove the fundamental theorems of real analysis in a direct, natural way. (Incredibly, a great deal of the presentation echoes the work of Leibniz, which was performed in the 17th century.) NSA has also extended mathematics in directions which exceed the scope of this thesis. These investigations may eventually result in fruitful discoveries. Contents Introduction: Why Infinitesimals? vi Chapter 1. Historical Background 1 1.1. Overview 1 1.2. Origins 1 1.3. Continuity 3 1.4. Eudoxus and Archimedes 5 1.5. Apply when Necessary 7 1.6. Banished 10 1.7. Regained 12 1.8. The Future 13 Chapter 2. Rigorous Infinitesimals 15 2.1. Developing Nonstandard Analysis 15 2.2. Direct Ultrapower Construction of ∗R 17 2.3. Principles of NSA 28 2.4. Working with Hyperreals 32 Chapter 3. -
A Compact Introduction to a Generalized Extreme Value Theorem
Ursinus College Digital Commons @ Ursinus College Transforming Instruction in Undergraduate Topology Mathematics via Primary Historical Sources (TRIUMPHS) Summer 2017 A Compact Introduction to a Generalized Extreme Value Theorem Nicholas A. Scoville Ursinus College, [email protected] Follow this and additional works at: https://digitalcommons.ursinus.edu/triumphs_topology Part of the Curriculum and Instruction Commons, Educational Methods Commons, Geometry and Topology Commons, Higher Education Commons, and the Science and Mathematics Education Commons Click here to let us know how access to this document benefits ou.y Recommended Citation Scoville, Nicholas A., "A Compact Introduction to a Generalized Extreme Value Theorem" (2017). Topology. 5. https://digitalcommons.ursinus.edu/triumphs_topology/5 This Course Materials is brought to you for free and open access by the Transforming Instruction in Undergraduate Mathematics via Primary Historical Sources (TRIUMPHS) at Digital Commons @ Ursinus College. It has been accepted for inclusion in Topology by an authorized administrator of Digital Commons @ Ursinus College. For more information, please contact [email protected]. A Compact Introduction to a Generalized Extreme Value Theorem Nicholas A. Scoville∗ April 19, 2021 1 Introduction Compactness is a concept that is often introduced in a first course in analysis or topology, but one which students in those courses often find to be considerably difficult. Not only can it be challenging to figure out what the standard definition is saying, it can be even more of a mystery tofigure out what possessed someone to write down such a definition in the first place. In this project, we look back to when compactness was first defined (albeit slightly differently than it is today) tosee what use it had then and, more importantly, the role it continues to play in mathematics today.