Chapter 7. Covariant Formulation of Electrodynamics Notes: • Most of the Material Presented in This Chapter Is Taken from Jackson, Chap
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Glossary Physics (I-Introduction)
1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay. -
Relativistic Dynamics
Chapter 4 Relativistic dynamics We have seen in the previous lectures that our relativity postulates suggest that the most efficient (lazy but smart) approach to relativistic physics is in terms of 4-vectors, and that velocities never exceed c in magnitude. In this chapter we will see how this 4-vector approach works for dynamics, i.e., for the interplay between motion and forces. A particle subject to forces will undergo non-inertial motion. According to Newton, there is a simple (3-vector) relation between force and acceleration, f~ = m~a; (4.0.1) where acceleration is the second time derivative of position, d~v d2~x ~a = = : (4.0.2) dt dt2 There is just one problem with these relations | they are wrong! Newtonian dynamics is a good approximation when velocities are very small compared to c, but outside of this regime the relation (4.0.1) is simply incorrect. In particular, these relations are inconsistent with our relativity postu- lates. To see this, it is sufficient to note that Newton's equations (4.0.1) and (4.0.2) predict that a particle subject to a constant force (and initially at rest) will acquire a velocity which can become arbitrarily large, Z t ~ d~v 0 f ~v(t) = 0 dt = t ! 1 as t ! 1 . (4.0.3) 0 dt m This flatly contradicts the prediction of special relativity (and causality) that no signal can propagate faster than c. Our task is to understand how to formulate the dynamics of non-inertial particles in a manner which is consistent with our relativity postulates (and then verify that it matches observation, including in the non-relativistic regime). -
Appendix D: the Wave Vector
General Appendix D-1 2/13/2016 Appendix D: The Wave Vector In this appendix we briefly address the concept of the wave vector and its relationship to traveling waves in 2- and 3-dimensional space, but first let us start with a review of 1- dimensional traveling waves. 1-dimensional traveling wave review A real-valued, scalar, uniform, harmonic wave with angular frequency and wavelength λ traveling through a lossless, 1-dimensional medium may be represented by the real part of 1 ω the complex function ψ (xt , ): ψψ(x , t )= (0,0) exp(ikx− i ω t ) (D-1) where the complex phasor ψ (0,0) determines the wave’s overall amplitude as well as its phase φ0 at the origin (xt , )= (0,0). The harmonic function’s wave number k is determined by the wavelength λ: k = ± 2πλ (D-2) The sign of k determines the wave’s direction of propagation: k > 0 for a wave traveling to the right (increasing x). The wave’s instantaneous phase φ(,)xt at any position and time is φφ(,)x t=+−0 ( kx ω t ) (D-3) The wave number k is thus the spatial analog of angular frequency : with units of radians/distance, it equals the rate of change of the wave’s phase with position (with time t ω held constant), i.e. ∂∂φφ k =; ω = − (D-4) ∂∂xt (note the minus sign in the differential expression for ). If a point, originally at (x= xt0 , = 0), moves with the wave at velocity vkφ = ω , then the wave’s phase at that point ω will remain constant: φ(x0+ vtφφ ,) t =++ φ0 kx ( 0 vt ) −=+ ωφ t00 kx The velocity vφ is called the wave’s phase velocity. -
EMT UNIT 1 (Laws of Reflection and Refraction, Total Internal Reflection).Pdf
Electromagnetic Theory II (EMT II); Online Unit 1. REFLECTION AND TRANSMISSION AT OBLIQUE INCIDENCE (Laws of Reflection and Refraction and Total Internal Reflection) (Introduction to Electrodynamics Chap 9) Instructor: Shah Haidar Khan University of Peshawar. Suppose an incident wave makes an angle θI with the normal to the xy-plane at z=0 (in medium 1) as shown in Figure 1. Suppose the wave splits into parts partially reflecting back in medium 1 and partially transmitting into medium 2 making angles θR and θT, respectively, with the normal. Figure 1. To understand the phenomenon at the boundary at z=0, we should apply the appropriate boundary conditions as discussed in the earlier lectures. Let us first write the equations of the waves in terms of electric and magnetic fields depending upon the wave vector κ and the frequency ω. MEDIUM 1: Where EI and BI is the instantaneous magnitudes of the electric and magnetic vector, respectively, of the incident wave. Other symbols have their usual meanings. For the reflected wave, Similarly, MEDIUM 2: Where ET and BT are the electric and magnetic instantaneous vectors of the transmitted part in medium 2. BOUNDARY CONDITIONS (at z=0) As the free charge on the surface is zero, the perpendicular component of the displacement vector is continuous across the surface. (DIꓕ + DRꓕ ) (In Medium 1) = DTꓕ (In Medium 2) Where Ds represent the perpendicular components of the displacement vector in both the media. Converting D to E, we get, ε1 EIꓕ + ε1 ERꓕ = ε2 ETꓕ ε1 ꓕ +ε1 ꓕ= ε2 ꓕ Since the equation is valid for all x and y at z=0, and the coefficients of the exponentials are constants, only the exponentials will determine any change that is occurring. -
On the Covariant Representation of Integral Equations of the Electromagnetic Field
On the covariant representation of integral equations of the electromagnetic field Sergey G. Fedosin PO box 614088, Sviazeva str. 22-79, Perm, Perm Krai, Russia E-mail: [email protected] Gauss integral theorems for electric and magnetic fields, Faraday’s law of electromagnetic induction, magnetic field circulation theorem, theorems on the flux and circulation of vector potential, which are valid in curved spacetime, are presented in a covariant form. Covariant formulas for magnetic and electric fluxes, for electromotive force and circulation of the vector potential are provided. In particular, the electromotive force is expressed by a line integral over a closed curve, while in the integral, in addition to the vortex electric field strength, a determinant of the metric tensor also appears. Similarly, the magnetic flux is expressed by a surface integral from the product of magnetic field induction by the determinant of the metric tensor. A new physical quantity is introduced – the integral scalar potential, the rate of change of which over time determines the flux of vector potential through a closed surface. It is shown that the commonly used four-dimensional Kelvin-Stokes theorem does not allow one to deduce fully the integral laws of the electromagnetic field and in the covariant notation requires the addition of determinant of the metric tensor, besides the validity of the Kelvin-Stokes theorem is limited to the cases when determinant of metric tensor and the contour area are independent from time. This disadvantage is not present in the approach that uses the divergence theorem and equation for the dual electromagnetic field tensor. -
Instantaneous Local Wave Vector Estimation from Multi-Spacecraft Measurements Using Few Spatial Points T
Instantaneous local wave vector estimation from multi-spacecraft measurements using few spatial points T. D. Carozzi, A. M. Buckley, M. P. Gough To cite this version: T. D. Carozzi, A. M. Buckley, M. P. Gough. Instantaneous local wave vector estimation from multi- spacecraft measurements using few spatial points. Annales Geophysicae, European Geosciences Union, 2004, 22 (7), pp.2633-2641. hal-00317540 HAL Id: hal-00317540 https://hal.archives-ouvertes.fr/hal-00317540 Submitted on 14 Jul 2004 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. Annales Geophysicae (2004) 22: 2633–2641 SRef-ID: 1432-0576/ag/2004-22-2633 Annales © European Geosciences Union 2004 Geophysicae Instantaneous local wave vector estimation from multi-spacecraft measurements using few spatial points T. D. Carozzi, A. M. Buckley, and M. P. Gough Space Science Centre, University of Sussex, Brighton, England Received: 30 September 2003 – Revised: 14 March 2004 – Accepted: 14 April 2004 – Published: 14 July 2004 Part of Special Issue “Spatio-temporal analysis and multipoint measurements in space” Abstract. We introduce a technique to determine instan- damental assumptions, namely stationarity and homogene- taneous local properties of waves based on discrete-time ity. -
Chapter 2 X-Ray Diffraction and Reciprocal Lattice
Chapter 2 X-ray diffraction and reciprocal lattice I. Waves 1. A plane wave is described as Ψ(x,t) = A ei(k⋅x-ωt) A is the amplitude, k is the wave vector, and ω=2πf is the angular frequency. 2. The wave is traveling along the k direction with a velocity c given by ω=c|k|. Wavelength along the traveling direction is given by |k|=2π/λ. 3. When a wave interacts with the crystal, the plane wave will be scattered by the atoms in a crystal and each atom will act like a point source (Huygens’ principle). 4. This formulation can be applied to any waves, like electromagnetic waves and crystal vibration waves; this also includes particles like electrons, photons, and neutrons. A particular case is X-ray. For this reason, what we learn in X-ray diffraction can be applied in a similar manner to other cases. II. X-ray diffraction in real space – Bragg’s Law 1. A crystal structure has lattice and a basis. X-ray diffraction is a convolution of two: diffraction by the lattice points and diffraction by the basis. We will consider diffraction by the lattice points first. The basis serves as a modification to the fact that the lattice point is not a perfect point source (because of the basis). 2. If each lattice point acts like a coherent point source, each lattice plane will act like a mirror. θ θ θ d d sin θ (hkl) -1- 2. The diffraction is elastic. In other words, the X-rays have the same frequency (hence wavelength and |k|) before and after the reflection. -
Basic Four-Momentum Kinematics As
L4:1 Basic four-momentum kinematics Rindler: Ch5: sec. 25-30, 32 Last time we intruduced the contravariant 4-vector HUB, (II.6-)II.7, p142-146 +part of I.9-1.10, 154-162 vector The world is inconsistent! and the covariant 4-vector component as implicit sum over We also introduced the scalar product For a 4-vector square we have thus spacelike timelike lightlike Today we will introduce some useful 4-vectors, but rst we introduce the proper time, which is simply the time percieved in an intertial frame (i.e. time by a clock moving with observer) If the observer is at rest, then only the time component changes but all observers agree on ✁S, therefore we have for an observer at constant speed L4:2 For a general world line, corresponding to an accelerating observer, we have Using this it makes sense to de ne the 4-velocity As transforms as a contravariant 4-vector and as a scalar indeed transforms as a contravariant 4-vector, so the notation makes sense! We also introduce the 4-acceleration Let's calculate the 4-velocity: and the 4-velocity square Multiplying the 4-velocity with the mass we get the 4-momentum Note: In Rindler m is called m and Rindler's I will always mean with . which transforms as, i.e. is, a contravariant 4-vector. Remark: in some (old) literature the factor is referred to as the relativistic mass or relativistic inertial mass. L4:3 The spatial components of the 4-momentum is the relativistic 3-momentum or simply relativistic momentum and the 0-component turns out to give the energy: Remark: Taylor expanding for small v we get: rest energy nonrelativistic kinetic energy for v=0 nonrelativistic momentum For the 4-momentum square we have: As you may expect we have conservation of 4-momentum, i.e. -
Electromagnetic Particles Guy Michel Stephan
Electromagnetic particles Guy Michel Stephan To cite this version: Guy Michel Stephan. Electromagnetic particles. 2017. hal-01446417 HAL Id: hal-01446417 https://hal.archives-ouvertes.fr/hal-01446417 Preprint submitted on 2 Feb 2017 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. Electromagnetic particles. G.M. St´ephan 26, Chemin de Quo Vadis 22730, Tregastel email : [email protected] 25 janvier 2017 R´esum´e The covariant derivative of the 4-components electromagnetic potential in a flat Minkowski space- time is split into its antisymmetric and symmetric parts. While the former is well known to describe the electromagnetic field, we show that the latter describes the associated particles. When symmetry principles are applied to the invariants in operations of the Poincar´egroup, one finds equations which describe the structure of the particles. Both parts of the tensor unify the concept of matter-wave duality. Charge and mass are shown to be associated to the potential. 1 Introduction. When Born and Infeld published their work[1] on the foundations of non linear electromagnetism in the year 1934, their aim was to describe the electron and more generally the physical world from a purely electromagnetic theory. -
Linear Elastodynamics and Waves
Linear Elastodynamics and Waves M. Destradea, G. Saccomandib aSchool of Electrical, Electronic, and Mechanical Engineering, University College Dublin, Belfield, Dublin 4, Ireland; bDipartimento di Ingegneria Industriale, Universit`adegli Studi di Perugia, 06125 Perugia, Italy. Contents 1 Introduction 3 2 Bulk waves 6 2.1 Homogeneous waves in isotropic solids . 8 2.2 Homogeneous waves in anisotropic solids . 10 2.3 Slowness surface and wavefronts . 12 2.4 Inhomogeneous waves in isotropic solids . 13 3 Surface waves 15 3.1 Shear horizontal homogeneous surface waves . 15 3.2 Rayleigh waves . 17 3.3 Love waves . 22 3.4 Other surface waves . 25 3.5 Surface waves in anisotropic media . 25 4 Interface waves 27 4.1 Stoneley waves . 27 4.2 Slip waves . 29 4.3 Scholte waves . 32 4.4 Interface waves in anisotropic solids . 32 5 Concluding remarks 33 1 Abstract We provide a simple introduction to wave propagation in the frame- work of linear elastodynamics. We discuss bulk waves in isotropic and anisotropic linear elastic materials and we survey several families of surface and interface waves. We conclude by suggesting a list of books for a more detailed study of the topic. Keywords: linear elastodynamics, anisotropy, plane homogeneous waves, bulk waves, interface waves, surface waves. 1 Introduction In elastostatics we study the equilibria of elastic solids; when its equilib- rium is disturbed, a solid is set into motion, which constitutes the subject of elastodynamics. Early efforts in the study of elastodynamics were mainly aimed at modeling seismic wave propagation. With the advent of electron- ics, many applications have been found in the industrial world. -
1 Fundamental Solutions to the Wave Equation 2 the Pulsating Sphere
1 Fundamental Solutions to the Wave Equation Physical insight in the sound generation mechanism can be gained by considering simple analytical solutions to the wave equation. One example is to consider acoustic radiation with spherical symmetry about a point ~y = fyig, which without loss of generality can be taken as the origin of coordinates. If t stands for time and ~x = fxig represent the observation point, such solutions of the wave equation, @2 ( − c2r2)φ = 0; (1) @t2 o will depend only on the r = j~x − ~yj. It is readily shown that in this case (1) can be cast in the form of a one-dimensional wave equation @2 @2 ( − c2 )(rφ) = 0: (2) @t2 o @r2 The general solution to (2) can be written as f(t − r ) g(t + r ) φ = co + co : (3) r r The functions f and g are arbitrary functions of the single variables τ = t± r , respectively. ± co They determine the pattern or the phase variation of the wave, while the factor 1=r affects only the wave magnitude and represents the spreading of the wave energy over larger surface as it propagates away from the source. The function f(t − r ) represents an outwardly co going wave propagating with the speed c . The function g(t + r ) represents an inwardly o co propagating wave propagating with the speed co. 2 The Pulsating Sphere Consider a sphere centered at the origin and having a small pulsating motion so that the equation of its surface is r = a(t) = a0 + a1(t); (4) where ja1(t)j << a0. -
Electromagnetic Forces and Internal Stresses in Dielectric Media
PHYSICAL REVIEW E 85, 046606 (2012) Electromagnetic forces and internal stresses in dielectric media Winston Frias* and Andrei I. Smolyakov Department of Physics and Engineering Physics, University of Saskatchewan, 116 Science Place Saskatoon, SK S7N 5E2, Canada (Received 16 August 2011; revised manuscript received 26 January 2012; published 23 April 2012) The macroscopic electromagnetic force on dielectric bodies and the related problem of the momentum conservation are discussed. It is argued that different forms of the momentum conservation and, respectively, different forms of the force density, correspond to the different ordering in the macroscopic averaging procedure. Different averaging procedures and averaging length scale assumptions result in expressions for the force density with vastly different force density profiles which can potentially be detected experimentally by measuring the profiles of the internal stresses in the medium. The expressions for the Helmholtz force is generalized for the dissipative case. It is shown that the net (integrated) force on the body in vacuum is the same for Lorentz and Helmholtz expressions in all configuration. The case of a semi-infinite medium is analyzed and it is shown that explicit assumptions on the boundary conditions at infinity remove ambiguity in the force on the semi-infinite dielectric. DOI: 10.1103/PhysRevE.85.046606 PACS number(s): 03.50.De I. INTRODUCTION This article is organized as follows. In Sec. II, the problem of the momentum exchange and the force is explored from Electromagnetic forces on charged particles result in an the microscopic point of view. In Sec. III, the Abraham and overall force imparted on a body that is called radiation Minkowski expressions for the momentum and the stress (ponderomotive) pressure.