Scalar and vector fields

Similar documents
Math 5BI: Problem Set 9 Integral Theorems of Vector Calculus

Lecture 4-1 Physics 219 Question 1 Aug Where (if any) is the net electric field due to the following two charges equal to zero?

PLANAR KINETICS OF A RIGID BODY FORCE AND ACCELERATION

DIVERGENCE AND CURL THEOREMS

The Divergence Theorem Stokes Theorem Applications of Vector Calculus. Calculus. Vector Calculus (III)

Maxwell s equations for electrostatics

송석호 ( 물리학과 )

PRACTICE PROBLEMS. Please let me know if you find any mistakes in the text so that i can fix them. 1. Mixed partial derivatives.

MULTIVARIABLE INTEGRATION

Mathematical Notes for E&M Gradient, Divergence, and Curl

free space (vacuum) permittivity [ F/m]

ES.182A Topic 44 Notes Jeremy Orloff

l=0 The expansion coefficients can be determined, for example, by finding the potential on the z-axis and expanding that result in z.

Chapter 23: Gauss Law. PHY2049: Chapter 23 1

Welcome. to Electrostatics

Lecture 15 Perfect Conductors, Boundary Conditions, Method of Images

Kinematics (2) - Motion in Three Dimensions

Physics Will Farmer. May 5, Physics 1120 Contents 2

Chapter 21. Electric Fields

ENGI 4430 Multiple Integration Cartesian Double Integrals Page 3-01

1 + f 2 x + f 2 y dy dx, where f(x, y) = 2 + 3x + 4y, is

Lecture 13: Electromagnetic Theory Professor D. K. Ghosh, Physics Department, I.I.T., Bombay. Poisson s and Laplace s Equations

Basics of Electromagnetics Maxwell s Equations (Part - I)

Summary: Applications of Gauss Law

The fundamental theorem of calculus for definite integration helped us to compute If has an anti-derivative,

ELECTROMAGNETIC WAVES

Time-varying electromagnetic field

3 Chapter. Gauss s Law

Electric Flux. If we know the electric field on a Gaussian surface, we can find the net charge enclosed by the surface.

ENGI Multiple Integration Page 8-01

f dr. (6.1) f(x i, y i, z i ) r i. (6.2) N i=1

Notes on Vector Calculus

Second Year Electromagnetism Summer 2018 Caroline Terquem. Vacation work: Problem set 0. Revisions

Magnetostatics. Lecture 23: Electromagnetic Theory. Professor D. K. Ghosh, Physics Department, I.I.T., Bombay

Chapter 21 Chapter 23 Gauss Law. Copyright 2014 John Wiley & Sons, Inc. All rights reserved.

r r 1 r r 1 2 = q 1 p = qd and it points from the negative charge to the positive charge.

Physics 208, Spring 2016 Exam #3

Some Important Concepts and Theorems of Vector Calculus

Radiation Integrals and Auxiliary Potential Functions

SUMMARY PHYSICS 707 Electrostatics. E(x) = 4πρ(x) and E(x) = 0 (1)

Multivariable Calculus

Practice Problems for Exam 3 (Solutions) 1. Let F(x, y) = xyi+(y 3x)j, and let C be the curve r(t) = ti+(3t t 2 )j for 0 t 2. Compute F dr.

Mathematical Tripos Part IA Lent Term Example Sheet 1. Calculate its tangent vector dr/du at each point and hence find its total length.

Chapter 25. Electric Potential

Math 350 Solutions for Final Exam Page 1. Problem 1. (10 points) (a) Compute the line integral. F ds C. z dx + y dy + x dz C

10.8 Further Applications of the Divergence Theorem

Handout 6: Rotational motion and moment of inertia. Angular velocity and angular acceleration

Concepts in Engineering Mathematics: Lecture 39

MULTIVARIABLE INTEGRATION

Final Exam. Monday March 19, 3:30-5:30pm MAT 21D, Temple, Winter 2018

ENERGY IN ELECTROSTATICS

ELE3310: Basic ElectroMagnetic Theory

Rotational Kinematics and Dynamics. UCVTS AIT Physics

Rotational & Rigid-Body Mechanics. Lectures 3+4

Electromagnetic. G. A. Krafft Jefferson Lab Jefferson Lab Professor of Physics Old Dominion University TAADI Electromagnetic Theory

INTRODUCTION. Introduction. Discrete charges: Electric dipole. Continuous charge distributions. Flux of a vector field

Preliminary Exam: Electromagnetism, Thursday January 12, :00-12:00

Two small balls, each of mass m, with perpendicular bisector of the line joining the two balls as the axis of rotation:

Overview of vector calculus. Coordinate systems in space. Distance formula. (Sec. 12.1)

(a) Consider a sphere of charge with radius a and charge density ρ(r) that varies with radius as. ρ(r) = Ar n for r a

EQUATIONS OF MOTION: NORMAL AND TANGENTIAL COORDINATES (Section 13.5)

where the last equality follows from the divergence theorem. Now since we did this for an arbitrary volume τ, it must hold locally:

3/22/2016. Chapter 27 Gauss s Law. Chapter 27 Preview. Chapter 27 Preview. Chapter Goal: To understand and apply Gauss s law. Slide 27-2.

Review of Vector Analysis in Cartesian Coordinates

Gauss s Law & Potential

Sept , 17, 23, 29, 37, 41, 45, 47, , 5, 13, 17, 19, 29, 33. Exam Sept 26. Covers Sept 30-Oct 4.

Lecture 3. Electric Field Flux, Gauss Law

Electric field lines are perpendicular to the equipotential lines

1 Fundamentals of laser energy absorption

Chapter 24. Gauss s Law

Non-Maxwell Static Solutions for ECE Electromagnetism

CURRENT MATERIAL: Vector Calculus.

Electrostatics : Electric Field & Potential

Electromagnetic Field Theory (EMT)

Week 7: Integration: Special Coordinates

Tutorial 3 - Solutions Electromagnetic Waves

Chapter 24. Gauss s Law

FLUX OF VECTOR FIELD INTRODUCTION

Chapter 8. Conservation Laws. 8.3 Magnetic Forces Do No Work

Lecture 17 - The Secrets we have Swept Under the Rug

V Relation to Physics

Lectures in Discrete Differential Geometry 2 Surfaces

Calculus I Sample Final exam

CH 24. Electric Potential

Vectors and Fields. Vectors versus scalars

TUTORIAL 4. Proof. Computing the potential at the center and pole respectively,

Electric Flux and Gauss Law

9.4 Vector and Scalar Fields; Derivatives

D = 2(2) 3 2 = 4 9 = 5 < 0

PLANAR KINETIC EQUATIONS OF MOTION (Section 17.2)

Physics 2212 GH Quiz #2 Solutions Spring 2015

Chapter 1. Introduction to Electrostatics

E&M. 1 Capacitors. January 2009

PHYSICS. Chapter 24 Lecture FOR SCIENTISTS AND ENGINEERS A STRATEGIC APPROACH 4/E RANDALL D. KNIGHT

Real Analysis III. (MAT312β) Department of Mathematics University of Ruhuna. A.W.L. Pubudu Thilan

Lecture 9 Electric Flux and Its Density Gauss Law in Integral Form

Multivector Calculus

CURRENT MATERIAL: Vector Calculus.

Physics 3323, Fall 2016 Problem Set 2 due Sep 9, 2016

Electrodynamics PHY712. Lecture 4 Electrostatic potentials and fields. Reference: Chap. 1 & 2 in J. D. Jackson s textbook.

Transcription:

Scalar and vector fields What is a field in mathematics? Roughly speaking a field defines how a scalar-valued or vectorvalued quantity varies through space. We usually work with scalar and vector fields. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 1

Motivating examples A flat circular metal plate of radius 1 m is located with its centre at the origin of R 2 and heated with a blow-torch. At each point (x y) of the unit disc denote the temperature of the disc by T (x y) which is a scalar-valued function. T (x y) is an instance of a scalar field defined on a region of two-dimensional space. The above example could be extended to R 3 by replacing the disk with a ball. In this case we d have a scalar field T (x y z) defined over the unit ball in R 3. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 2

A positive point charge of Q coul is located at the origin of R 3. The force exerted on the test charge of 1 coul at the point (x y z) is defined according to Coulomb s law of electrostatics viz. Q 4πɛ 0 r 2 r := x 2 + y 2 + z 2. This force is denoted by E(x y z) and it is called the electrostatic field which is defined for all (x y z) 0 (or R 3 \{0}). This vector-valued function is an instance of a vector field defined everywhere in three-dimensional space R 3 except for the origin. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 3

Suppose that some electric charge is continuously distributed throughout some fixed region D R 3. For some point (x y z) D define a small sphere of radius 0 < ɛ 1 volume V ɛ and enclosed (total) charge Q ɛ. If it exists the limit ρ(x y z) = lim ɛ 0 Q ɛ /V ɛ defines the charge density at the point (x y z). If the limit exists for each and every point (x y z) D then we have a scalar field ρ(x y z) defined over D. Effectively ρ(x y z) gives the quantity of charge per unit volume concentrated at (x y z) that is ρ describes the local concentration of charge at each point in the region D. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 4

Let D = R 3 so that the charge is spread everywhere in space. For an arbitrary region Ω R 3 the total charge enclosed within Ω must be given by Q = ρ(x y z) dxdydz = ρ dv. Ω The above relation can be used to obtain a very important result called the continuity equation which describes the movement of charge through space. Ω Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 5

Suppose that the charge in the fixed region D is in motion. In particular at each point (x y z) D the charge moves past that point with a velocity v(x y z) (which is a vector). For each (x y z) D define which is also a vector. J(x y z) := ρ(x y z) v(x y z) This vector-valued function is a vector field defined everywhere in the region D and called the current density field. The dimensions of J are coul m 3 m sec = coul m 2 sec = amps m 2 Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 6

Let S be a plane with area A and let n be the unit vector normal to S. Let us assume for simplicity that ρ(x y z) and v(x y z) are constant in space namely ρ(x y z) = ρ v(x y z) = v for all (x y z) D. Then the current density field J(x y z) is position independent and given by J = ρ v. Moreover if n and v are collinear then the speed of the charge is given by v = v = n v. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 7

Now let us fix some small time interval t > 0. Since v n the total volume of space that crosses S in the time t must be Av t. Then the total charge Q which flows across S in the time t must be equal to Q = (Av t)ρ when v and n are collinear. The above relation can also be rewritten as Q = (A t)(v n)ρ. Yet what happens when v and n are not collinear? Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 8

Suppose for example that v is tangential to S. Then v is orthogonal to the unit vector n which implies v n = 0. Then the total charge Q that crosses S in the time t is Q = (A t) (v n) ρ = 0. }{{} 0 Intuitively since the direction of charge movement is along S and not through it there can be no charge crossing S. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 9

Finally suppose v has an arbetrary orientation. Then we can express v as v = v 1 + v 2 where v 1 n while v 2 n. In this case the total charge that crosses S in the time t is given by Q = (Av 1 t)ρ. But v 1 is just the projection of v along n viz. v 1 = v n. Therefore the total charge Q becomes Q = (A t)(v n)ρ when the charge velocity v is in a general direction. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 1

The quantity I = Q/ t is the total current passing through the surface S and it can be expressed as I = Q/ t = A(n v)ρ = A(ρv) n = A(J n). Conclusion The total current I through the surface S is the product of the area A of S and the inner product J n of the current density J with the unit normal n to S. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 1

Now let us allow v and ρ (and hence J) to vary in space. Then for an infinitesimally small surface ds with infinitesimally small area da J(x y z) is effectively constant as (x y z) varies through ds. Then the infinitesimal current passing through the infinitesimal surface ds with unit normal n(x y z) is given by di = (J(x y z) n(x y z)) da. Thus knowing the vector field J(x y z) we can calculate the current di flowing across a small planar surface ds with area da and unit normal vector n(x y z) at a point (x y z) ds. Later we shall see that charge and current density are absolutely essential to the formulation of Maxwell s equations of electromagnetism. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 1

Vector and scalar fields Definition A vector field comprises a specified region D R 3 called the domain of the vector field together with a function or mapping F : D R 3 which assigns to each point (x y z) D the vector F(x y z) R 3. The vector field F(x y z) can be defined in terms of its scalar components F 1 (x y z) F 2 (x y z) and F 3 (x y z) along the coordinates x y z respectively. Given the standard i j k axes one has F(x y z) = F 1 (x y z)i + F 2 (x y z)j + F 3 (x y z)k. Definition A scalar field comprises a specified region D R 3 called the domain of the scalar field together with a function or mapping f : D R which assigns to each point (x y z) D the real number f(x y z). Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 1

Vector and scalar fields (cont.) Definition A vector field F : D R 3 is called a C 1 -vector field when for each i = 1 2 3 the partial derivatives F i (x y z) x F j (x y z) y F k (x y z) z all exist and are continuous functions of (x y z) D. Definition A vector field F : D R 3 is called a C 2 -vector field when F is a C 1 vector field and for each i = 1 2 3 the partial derivatives 2 F i (x y z) x 2 2 F i (x y z) x y 2 F j (x y z) y 2 2 F j (x y z) y z 2 F k (x y z) z 2 2 F k (x y z) x z all exist and are continuous functions of (x y z) D. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 1

Vector and scalar fields (cont.) Definition A scalar field f : D R is called a C 1 -scalar field when the partial derivatives f(x y z) f(x y z) f(x y z) x y z all exist and are continuous functions of (x y z) D. Definition A scalar field f : D R is called a C 2 -scalar field when f is a C 1 scalar field and the partial derivatives 2 f(x y z) x 2 2 f(x y z) x y 2 f(x y z) y 2 2 f(x y z) y z 2 f(x y z) z 2 2 f(x y z) x z all exist and are continuous functions of (x y z) D. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 1

Vector and scalar fields (cont.) A standard result from elementary calculus says that when F : D R 3 is a C 2 -vector field then we always have for i = 1 2 3. 2 F i (x y z) x y 2 F i (x y z) y z 2 F i (x y z) x z = 2 F i (x y z) y x = 2 F i (x y z) z y = 2 F i (x y z) z x The same rules of exchangeability of the order of differentiation apply to scalar vector fields. Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 1

Vector and scalar fields (cont.) Both vector and scalar fields can vary with time t. Such time-varying vector and scalar fields are denoted by F(x y z t) and f(x y z t) respectively. A time-varying vector field is one in which for each fixed instant t we just have a vector field which maps each (x y z) D into the vector F(x y z t) R 3. Similarly a time varying scalar field is one in which for each fixed instant t we just have a scalar field which maps each (x y z) D into the real number f(x y z t). Department of ECE Fall 2014 ECE 206: Advanced Calculus 2 1