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Lecture 11 Line Integrals of Vector-Valued Functions (Cont'd)
Lecture 11 Line integrals of vector-valued functions (cont’d) In the previous lecture, we considered the following physical situation: A force, F(x), which is not necessarily constant in space, is acting on a mass m, as the mass moves along a curve C from point P to point Q as shown in the diagram below. z Q P m F(x(t)) x(t) C y x The goal is to compute the total amount of work W done by the force. Clearly the constant force/straight line displacement formula, W = F · d , (1) where F is force and d is the displacement vector, does not apply here. But the fundamental idea, in the “Spirit of Calculus,” is to break up the motion into tiny pieces over which we can use Eq. (1 as an approximation over small pieces of the curve. We then “sum up,” i.e., integrate, over all contributions to obtain W . The total work is the line integral of the vector field F over the curve C: W = F · dx . (2) ZC Here, we summarize the main steps involved in the computation of this line integral: 1. Step 1: Parametrize the curve C We assume that the curve C can be parametrized, i.e., x(t)= g(t) = (x(t),y(t), z(t)), t ∈ [a, b], (3) so that g(a) is point P and g(b) is point Q. From this parametrization we can compute the velocity vector, ′ ′ ′ ′ v(t)= g (t) = (x (t),y (t), z (t)) . (4) 1 2. Step 2: Compute field vector F(g(t)) over curve C F(g(t)) = F(x(t),y(t), z(t)) (5) = (F1(x(t),y(t), z(t), F2(x(t),y(t), z(t), F3(x(t),y(t), z(t))) , t ∈ [a, b] . -
Nonstandard Methods in Analysis an Elementary Approach to Stochastic Differential Equations
Nonstandard Methods in Analysis An elementary approach to Stochastic Differential Equations Vieri Benci Dipartimento di Matematica Applicata June 2008 Vieri Benci (DMA-Pisa) Nonstandard Methods 03/06 1 / 42 In most applications of NSA to analysis, only elementary tools and techniques of nonstandard calculus seems to be necessary. The advantages of a theory which includes infinitasimals rely more on the possibility of making new models rather than in the dimostration techniques. These two points will be illustrated using a-theory in the study of Brownian motion. The aim of this talk is to make two points relative to NSA: Vieri Benci (DMA-Pisa) Nonstandard Methods 03/06 2 / 42 The advantages of a theory which includes infinitasimals rely more on the possibility of making new models rather than in the dimostration techniques. These two points will be illustrated using a-theory in the study of Brownian motion. The aim of this talk is to make two points relative to NSA: In most applications of NSA to analysis, only elementary tools and techniques of nonstandard calculus seems to be necessary. Vieri Benci (DMA-Pisa) Nonstandard Methods 03/06 2 / 42 These two points will be illustrated using a-theory in the study of Brownian motion. The aim of this talk is to make two points relative to NSA: In most applications of NSA to analysis, only elementary tools and techniques of nonstandard calculus seems to be necessary. The advantages of a theory which includes infinitasimals rely more on the possibility of making new models rather than in the dimostration techniques. Vieri Benci (DMA-Pisa) Nonstandard Methods 03/06 2 / 42 The aim of this talk is to make two points relative to NSA: In most applications of NSA to analysis, only elementary tools and techniques of nonstandard calculus seems to be necessary. -
An Introduction to Nonstandard Analysis 11
AN INTRODUCTION TO NONSTANDARD ANALYSIS ISAAC DAVIS Abstract. In this paper we give an introduction to nonstandard analysis, starting with an ultrapower construction of the hyperreals. We then demon- strate how theorems in standard analysis \transfer over" to nonstandard anal- ysis, and how theorems in standard analysis can be proven using theorems in nonstandard analysis. 1. Introduction For many centuries, early mathematicians and physicists would solve problems by considering infinitesimally small pieces of a shape, or movement along a path by an infinitesimal amount. Archimedes derived the formula for the area of a circle by thinking of a circle as a polygon with infinitely many infinitesimal sides [1]. In particular, the construction of calculus was first motivated by this intuitive notion of infinitesimal change. G.W. Leibniz's derivation of calculus made extensive use of “infinitesimal” numbers, which were both nonzero but small enough to add to any real number without changing it noticeably. Although intuitively clear, infinitesi- mals were ultimately rejected as mathematically unsound, and were replaced with the common -δ method of computing limits and derivatives. However, in 1960 Abraham Robinson developed nonstandard analysis, in which the reals are rigor- ously extended to include infinitesimal numbers and infinite numbers; this new extended field is called the field of hyperreal numbers. The goal was to create a system of analysis that was more intuitively appealing than standard analysis but without losing any of the rigor of standard analysis. In this paper, we will explore the construction and various uses of nonstandard analysis. In section 2 we will introduce the notion of an ultrafilter, which will allow us to do a typical ultrapower construction of the hyperreal numbers. -
Ordinary Differential Equations
Ordinary Differential Equations for Engineers and Scientists Gregg Waterman Oregon Institute of Technology c 2017 Gregg Waterman This work is licensed under the Creative Commons Attribution 4.0 International license. The essence of the license is that You are free to: Share copy and redistribute the material in any medium or format • Adapt remix, transform, and build upon the material for any purpose, even commercially. • The licensor cannot revoke these freedoms as long as you follow the license terms. Under the following terms: Attribution You must give appropriate credit, provide a link to the license, and indicate if changes • were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use. No additional restrictions You may not apply legal terms or technological measures that legally restrict others from doing anything the license permits. Notices: You do not have to comply with the license for elements of the material in the public domain or where your use is permitted by an applicable exception or limitation. No warranties are given. The license may not give you all of the permissions necessary for your intended use. For example, other rights such as publicity, privacy, or moral rights may limit how you use the material. For any reuse or distribution, you must make clear to others the license terms of this work. The best way to do this is with a link to the web page below. To view a full copy of this license, visit https://creativecommons.org/licenses/by/4.0/legalcode. -
A Brief Tour of Vector Calculus
A BRIEF TOUR OF VECTOR CALCULUS A. HAVENS Contents 0 Prelude ii 1 Directional Derivatives, the Gradient and the Del Operator 1 1.1 Conceptual Review: Directional Derivatives and the Gradient........... 1 1.2 The Gradient as a Vector Field............................ 5 1.3 The Gradient Flow and Critical Points ....................... 10 1.4 The Del Operator and the Gradient in Other Coordinates*............ 17 1.5 Problems........................................ 21 2 Vector Fields in Low Dimensions 26 2 3 2.1 General Vector Fields in Domains of R and R . 26 2.2 Flows and Integral Curves .............................. 31 2.3 Conservative Vector Fields and Potentials...................... 32 2.4 Vector Fields from Frames*.............................. 37 2.5 Divergence, Curl, Jacobians, and the Laplacian................... 41 2.6 Parametrized Surfaces and Coordinate Vector Fields*............... 48 2.7 Tangent Vectors, Normal Vectors, and Orientations*................ 52 2.8 Problems........................................ 58 3 Line Integrals 66 3.1 Defining Scalar Line Integrals............................. 66 3.2 Line Integrals in Vector Fields ............................ 75 3.3 Work in a Force Field................................. 78 3.4 The Fundamental Theorem of Line Integrals .................... 79 3.5 Motion in Conservative Force Fields Conserves Energy .............. 81 3.6 Path Independence and Corollaries of the Fundamental Theorem......... 82 3.7 Green's Theorem.................................... 84 3.8 Problems........................................ 89 4 Surface Integrals, Flux, and Fundamental Theorems 93 4.1 Surface Integrals of Scalar Fields........................... 93 4.2 Flux........................................... 96 4.3 The Gradient, Divergence, and Curl Operators Via Limits* . 103 4.4 The Stokes-Kelvin Theorem..............................108 4.5 The Divergence Theorem ...............................112 4.6 Problems........................................114 List of Figures 117 i 11/14/19 Multivariate Calculus: Vector Calculus Havens 0. -
Appendix a Short Course in Taylor Series
Appendix A Short Course in Taylor Series The Taylor series is mainly used for approximating functions when one can identify a small parameter. Expansion techniques are useful for many applications in physics, sometimes in unexpected ways. A.1 Taylor Series Expansions and Approximations In mathematics, the Taylor series is a representation of a function as an infinite sum of terms calculated from the values of its derivatives at a single point. It is named after the English mathematician Brook Taylor. If the series is centered at zero, the series is also called a Maclaurin series, named after the Scottish mathematician Colin Maclaurin. It is common practice to use a finite number of terms of the series to approximate a function. The Taylor series may be regarded as the limit of the Taylor polynomials. A.2 Definition A Taylor series is a series expansion of a function about a point. A one-dimensional Taylor series is an expansion of a real function f(x) about a point x ¼ a is given by; f 00ðÞa f 3ðÞa fxðÞ¼faðÞþf 0ðÞa ðÞþx À a ðÞx À a 2 þ ðÞx À a 3 þÁÁÁ 2! 3! f ðÞn ðÞa þ ðÞx À a n þÁÁÁ ðA:1Þ n! © Springer International Publishing Switzerland 2016 415 B. Zohuri, Directed Energy Weapons, DOI 10.1007/978-3-319-31289-7 416 Appendix A: Short Course in Taylor Series If a ¼ 0, the expansion is known as a Maclaurin Series. Equation A.1 can be written in the more compact sigma notation as follows: X1 f ðÞn ðÞa ðÞx À a n ðA:2Þ n! n¼0 where n ! is mathematical notation for factorial n and f(n)(a) denotes the n th derivation of function f evaluated at the point a. -
How to Compute Line Integrals Scalar Line Integral Vector Line Integral
How to Compute Line Integrals Northwestern, Spring 2013 Computing line integrals can be a tricky business. First, there's two types of line integrals: scalar line integrals and vector line integrals. Although these are related, we compute them in different ways. Also, there's two theorems flying around, Green's Theorem and the Fundamental Theorem of Line Integrals (as I've called it), which give various other ways of computing line integrals. Knowing what to use when and where and why can be confusing, so hopefully this will help to keep things straight. I won't say much about what line integrals mean geometrically or otherwise. Hopefully this is something you have some idea about from class or the book, but I'm always happy to talk about this more in office hours. Here the focus is on computation. Key Point: When you are trying to apply one of these techniques, make sure the technique you are using is actually applicable! (This was a major source of confusion on Quiz 5.) Scalar Line Integral • Arises when integrating a function f over a curve C. • Notationally, is always denoted by something like Z f ds; C where the s in ds is just a normal s, as opposed to ds or d~s. • To compute, find parametric equations x(t); a ≤ t ≤ b for C and use Z Z b f ds = f(x(t)) kx0(t)k dt: C a • In the special case where f is the constant function 1, Z ds = arclength of C: C • For scalar line integrals, the orientation (i.e. -
Line Integrals
Line Integrals Kenneth H. Carpenter Department of Electrical and Computer Engineering Kansas State University September 12, 2008 Line integrals arise often in calculations in electromagnetics. The evaluation of such integrals can be done without error if certain simple rules are followed. This rules will be illustrated in the following. 1 Definitions 1.1 Definite integrals In calculus, for functions of one dimension, the definite integral is defined as the limit of a sum (the “Riemann” integral – other kinds are possible – see an advanced calculus text if you are curious about this :). Z b X f(x)dx = lim f(ξi)∆xi (1) ∆xi!0 a i where the ξi is a value of x within the incremental ∆xi, and all the incremental ∆xi add up to the length along the x axis from a to b. This is often pictured graphically as the area between the curve drawn as f(x) and the x axis. 1 EECE557 Line integrals – supplement to text - Fall 2008 2 1.2 Evaluation of definite integrals in terms of indefinite inte- grals The fundamental theorem of integral calculus relates the indefinite integral to the definite integral (with certain restrictions as to when these exist) as Z b dF f(x)dx = F (b) − F (a); when = f(x): (2) a dx The proof of eq.(2) does not depend on having a < b. In fact, R b f(x)dx = R a a − b f(x)dx follows from the values of ∆xi being signed so that ∆xi equals the value of x on the side of the increment next to b minus the value of x on the side of the increment next to a. -
256B Algebraic Geometry
256B Algebraic Geometry David Nadler Notes by Qiaochu Yuan Spring 2013 1 Vector bundles on the projective line This semester we will be focusing on coherent sheaves on smooth projective complex varieties. The organizing framework for this class will be a 2-dimensional topological field theory called the B-model. Topics will include 1. Vector bundles and coherent sheaves 2. Cohomology, derived categories, and derived functors (in the differential graded setting) 3. Grothendieck-Serre duality 4. Reconstruction theorems (Bondal-Orlov, Tannaka, Gabriel) 5. Hochschild homology, Chern classes, Grothendieck-Riemann-Roch For now we'll introduce enough background to talk about vector bundles on P1. We'll regard varieties as subsets of PN for some N. Projective will mean that we look at closed subsets (with respect to the Zariski topology). The reason is that if p : X ! pt is the unique map from such a subset X to a point, then we can (derived) push forward a bounded complex of coherent sheaves M on X to a bounded complex of coherent sheaves on a point Rp∗(M). Smooth will mean the following. If x 2 X is a point, then locally x is cut out by 2 a maximal ideal mx of functions vanishing on x. Smooth means that dim mx=mx = dim X. (In general it may be bigger.) Intuitively it means that locally at x the variety X looks like a manifold, and one way to make this precise is that the completion of the local ring at x is isomorphic to a power series ring C[[x1; :::xn]]; this is the ring where Taylor series expansions live. -
Partial Differential Equations I: Basics and Separable Solutions
18 Partial Differential Equations I: Basics and Separable Solutions We now turn our attention to differential equations in which the “unknown function to be deter- mined” — which we will usually denote by u — depends on two or more variables. Hence the derivatives are partial derivatives with respect to the various variables. (By the way, it may be a good idea to quickly review the A Brief Review of Elementary Ordinary Differential Equations, Appendex A of these notes. We will be using some of the material discussed there.) 18.1 Intro and Examples Simple Examples If we have a horizontally stretched string vibrating up and down, let u(x, t) the vertical position at time t of the bit of string at horizontal position x , = and make some almost reasonable assumptions regarding the string, the universe and the laws of physics, then we can show that u(x, t) satisfies ∂2u ∂2u c2 0 ∂t2 − ∂x2 = where c is some positive constant dependent on the physical properties of the stretched string. This equation is called the one-dimensional wave equation (with no external forces). If, instead, we have a uniform one-dimensional heat conducting rod along the X–axis and let u(x, t) the temperature at time t of the bit of rod at horizontal position x , = then, after applying suitable assumptions about heat flow, etc., we get the one-dimensional heat equation ∂u ∂2u κ f (x, t) . ∂t − ∂x2 = Here, κ is a positive constant dependent on the material properties of the rod, and f (x, t) describes the thermal contributions due to heat sources and/or sinks in the rod. -
Zero and Triviality Andreas Haida1 and Tue Trinh2 1 ELSC, HUJI, Jerusalem, IL 2 Leibniz-ZAS, Berlin, DE Corresponding Author: Tue Trinh ([email protected])
a journal of Haida, Andreas and Tue Trinh. 2020. Zero and general linguistics Glossa triviality. Glossa: a journal of general linguistics 5(1): 116. 1–14. DOI: https://doi.org/10.5334/gjgl.955 RESEARCH Zero and triviality Andreas Haida1 and Tue Trinh2 1 ELSC, HUJI, Jerusalem, IL 2 Leibniz-ZAS, Berlin, DE Corresponding author: Tue Trinh ([email protected]) This paper takes issue with Bylinina & Nouwen’s (2018) hypothesis that the numeral zero has the basic weak meaning of ‘zero or more.’ We argue, on the basis of empirical observation and theoretical consideration, that this hypothesis implies that exhaustification can circum- vent L-triviality, and that exhaustification cannot circumvent L-triviality. We also provide some experimental results to support our argument. Keywords: numerals; modification; exhaustification; L-Triviality 1 Theses and antitheses 1.1 Exhaustification The aim of this squib is to discuss some issues regarding the hypothesis about zero put for- ward by Bylinina & Nouwen (2018). These authors assume that numerals have the weak, ‘at least’ meaning as basic and the strengthened, ‘exactly’ meaning as derived by way of exhaustification, and propose thatzero be considered no different from other numerals in this respect.1 This is illustrated by (1a) and (1b). (1) a. Zero students smoked | ⟦students⟧ ⟦smoked⟧ | ≥ 0 ‘the number of students⟺ who smoked is zero or greater’ ⋂ b. EXH [Zero students smoked] | ⟦students⟧ ⟦smoked⟧ | ≥ 0 | ⟦students⟧ ⟦smoked⟧ | ≥| 1 ‘the number of students who smoked⟺ is zero and not greater’ ⋂ ∧ ⋂ Before we go on, let us be explicit about the notion of exhaustification which we will adopt for the purpose of this discussion. -
Arxiv:1509.06425V4 [Math.AG] 9 Dec 2017 Nipratrl Ntegoercraiaino Conformal of Gen Realization a Geometric the (And in Fact Role This Important Trivial
TRIVIALITY PROPERTIES OF PRINCIPAL BUNDLES ON SINGULAR CURVES PRAKASH BELKALE AND NAJMUDDIN FAKHRUDDIN Abstract. We show that principal bundles for a semisimple group on an arbitrary affine curve over an algebraically closed field are trivial, provided the order of π1 of the group is invertible in the ground field, or if the curve has semi-normal singularities. Several consequences and extensions of this result (and method) are given. As an application, we realize conformal blocks bundles on moduli stacks of stable curves as push forwards of line bundles on (relative) moduli stacks of principal bundles on the universal curve. 1. Introduction It is a consequence of a theorem of Harder [Har67, Satz 3.3] that generically trivial principal G-bundles on a smooth affine curve C over an arbitrary field k are trivial if G is a semisimple and simply connected algebraic group. When k is algebraically closed and G reductive, generic triviality, conjectured by Serre, was proved by Steinberg[Ste65] and Borel–Springer [BS68]. It follows that principal bundles for simply connected semisimple groups over smooth affine curves over algebraically closed fields are trivial. This fact (and a generalization to families of bundles [DS95]) plays an important role in the geometric realization of conformal blocks for smooth curves as global sections of line bundles on moduli-stacks of principal bundles on the curves (see the review [Sor96] and the references therein). An earlier result of Serre [Ser58, Th´eor`eme 1] (also see [Ati57, Theorem 2]) implies that this triviality property is true if G “ SLprq, and C is a possibly singular affine curve over an arbitrary field k.