The Principle of Relativity

Total Page:16

File Type:pdf, Size:1020Kb

The Principle of Relativity Eötvös Loránd Tudományegyetem Bölcsészettudományi Kar Doktori Disszertáció Gömöri Márton The Principle of Relativity An Empiricist Analysis (A relativitás elve – empirista elemzés) Filozófiatudományi Doktori Iskola Vezetője: Boros Gábor, DSc, egyetemi tanár Logika és Tudományfilozófia Program Vezetője: E. Szabó László, DSc, egyetemi tanár A bizottság tagjai: A bizottség elnöke: Bodnár István, egyetemi tanár, CSc, egyetemi tanár Felkért bírálók: Andréka Hajnal, DSc, professzor Szabó Gábor, PhD, tudományos főmunkatárs A bizottság titkára: Ambrus Gergely, PhD, egyetemi docens A bizottság további tagjai: Máté András, CSc, egyetemi docens Mekis Péter, PhD, adjunktus Székely Gergely, PhD, tudományos munkatárs Témavezető: E. Szabó László, DSc, egyetemi tanár Budapest, 2015 Contents 1 Introduction5 2 What Exactly Does the Principle of Relativity Say? 11 2.1 Einstein 1905............................... 11 2.2 The Electromagnetic Field of a Static versus Uniformly Moving Charge 30 2.3 Conceptual Components of the Relativity Principle.......... 35 2.4 The Formal Statement of the Relativity Principle........... 41 2.5 Covariance................................. 47 2.6 Initial and Boundary Conditions..................... 52 2.7 An Essential Conceptual Component: “Moving Body”........ 60 3 Operational Understanding of the Covariance of Electrodynamics 68 3.1 A Logical Problem with Postulating Relativity............. 68 3.2 Lorentzian Pedagogy........................... 77 3.3 The Case of Electrodynamics...................... 78 3.4 Operational Definitions of Electrodynamic Quantities in K ...... 80 3.5 Empirical Facts of Electrodynamics................... 86 3.6 Operational Definitions of Electrodynamic Quantities in K0 ...... 89 3.7 Observations of the Moving Observer.................. 93 3.8 Are the Transformation Rules Derived from Covariance True?.... 99 4 Does the Principle of Relativity Hold in Electrodynamics? 101 4.1 The Problem of M ............................ 101 4.2 Motion and Persistence.......................... 102 4.3 The Case of a General Electrodynamic System............. 107 4.4 Ontology of Classical Electrodynamics................. 113 Appendix I 116 Appendix II 118 2 CONTENTS 3 References 120 I have for long thought that if I had the opportunity to teach this subject, I would emphasize the continuity with earlier ideas. Usually it is the discontinuity which is stressed, the radical break with more primitive notions of space and time. Often the result is to destroy completely the confidence of the student in perfectly sound and useful concepts already acquired. (From J. S. Bell: “How to teach special relativity”, Bell 1987, p. 67.) Chapter 1 Introduction 1. Here is Galileo’s lively description of the special principle of relativity as appear- ing in the famous passages of the Dialogue: Shut yourself up with some friend in the main cabin below decks on some large ship, and have with you there some flies, butterflies, and other small flying animals. Have a large bowl of water with some fish in it; hang up a bottle that empties drop by drop into a wide vessel beneath it. With the ship standing still, observe carefully how the little animals fly with equal speed to all sides of the cabin. The fish swim indifferently in all directions; the drops fall into the vessel beneath; and, in throwing something to your friend, you need throw it no more strongly in one direction than another, the distances being equal; jumping with your feet together, you pass equal spaces in every direction. When you have observed all these things carefully (though doubtless when the ship is standing still everything must happen in this way), have the ship proceed with any speed you like, so long as the motion is uniform and not fluctuating this way and that. You will discover not the least change in all the effects named, nor could you tell from any of them whether the ship was moving or standing still. In jumping, you will pass on the floor the same spaces as before, nor will you make larger jumps toward the stern than toward the prow even though the ship is moving quite rapidly, despite the fact that during the time that you are in the air the floor under you will be going in a direction opposite to your jump. In throwing something to your companion, you will need no more force to get it to him whether he is in the direction of the bow or the stern, with yourself situated opposite. The droplets will fall as before into the vessel beneath without dropping toward the stern, although while the 5 CHAPTER 1. INTRODUCTION 6 drops are in the air the ship runs many spans. The fish in their water will swim toward the front of their bowl with no more effort than toward the back, and will go with equal ease to bait placed anywhere around the edges of the bowl. Finally the butterflies and flies will continue their flights indifferently toward every side, nor will it ever happen that they are concentrated toward the stern, as if tired out from keeping up with the course of the ship, from which they will have been separated during long intervals by keeping themselves in the air. And if smoke is made by burning some incense, it will be seen going up in the form of a little cloud, remaining still and moving no more toward one side than the other. The cause of all these correspondences of effects is the fact that the ship’s motion is common to all the things contained in it, and to the air also. That is why I said you should be below decks; for if this took place above in the open air, which would not follow the course of the ship, more or less noticeable differences would be seen in some of the effects noted. (Galilei 1953, pp. 186–187) Compare Galileo’s description with a sample from the huge variety of formulations of the principle available in the literature: ... the laws of physical phenomena should be the same, whether for an observer fixed, or for an observer carried along in a uniform movement of translation. (Poincaré 1956, p. 167) If a system of coordinates K is chosen so that, in relation to it, physical laws hold good in their simplest form, the same laws hold good in relation to any other system of coordinates K0 moving in uniform translation relatively to K. (Einstein 1916, p. 111) ... it is impossible to measure or detect the unaccelerated translatory motion of a system through free space or through any ether-like medium. (Tolman 1949, p. 12) ... all physical phenomena should have the same course of development in all system of inertia, and observers installed in different systems of inertia should thus as a result of their experiments arrive at the establishment of the same laws of nature. (Møller 1955, p. 4) ... the laws of Physics take the same mathematical form in all inertial frames (Sardesai 2004, p. 1) The same laws of nature are true for all inertial observers. (Madarász 2002, p. 84) CHAPTER 1. INTRODUCTION 7 The uniform translatory motion of any system can not be detected by an observer traveling with the system and making observations on it alone. (Comstock 1909, p. 767) The laws of nature and the results of all experiments performed in a given frame of reference are independent of the translational motion of the system as a whole. More precisely, there exists a ... set of equivalent Euclidean reference frames ... in which all physical phenomena occur in an identical manner. (Jackson 1999, p. 517) If we express some law of physics using the quantities of one inertial frame of reference, the resulting statement of the law will be exactly the same in any other inertial frame of reference. ... we write down exactly the same sentence to express the law in each inertial frame. (Norton 2013) ... all inertial frames are equivalent for the performance of all physical experiments (Rindler 2006, p. 12) ... the laws of physics are invariant under a change of inertial coordinate system (Ibid., p. 40) The outcome of any physical experiment is the same when performed with identical initial conditions relative to any inertial coordinate system. (Ibid.) ... all the laws of nature are identical in all inertial systems of reference. In other words, the equations expressing the laws of nature are invariant with respect to transformations of coordinates and time from one inertial system to another. This means that the equation describing any law of nature, when written in terms of coordinates and time in different inertial reference systems, has one and the same form. (Landau and Lifshitz 1980, p. 1) ... the phenomena in a given reference system are, in principle, inde- pendent of the translational motion of the system as a whole. To put it more precisely: there exists a triply infinite set of reference systems moving rectilinearly and uniformly relativity to one another, in which the phenomena occur in an identical manner. (Pauli 1958, p. 4) The postulate of relativity implies that a uniform motion of the center of mass of the universe relativity to a closed system will be without influence on the phenomena in such a system. (Ibid., p. 5) CHAPTER 1. INTRODUCTION 8 ... experience teaches us that ... all laws of physical nature which have been formulated with reference to a definite coordinate system are valid, in precisely the same form, when referred to another co-ordinate system which is in uniform rectilinear motion with respect to the first. ... All physical events take place in any system in just the same way, whether the system is at rest or whether it is moving uniformly and rectilinearly. (Schlick 1920, p. 10) ... laws must be Lorentz covariant. Lorentz covariance became syn- onymous with satisfaction of the principle of relativity. (Norton 1993, p. 796) The laws of physics don’t change, even for objects moving in inertial (constant speed) frames of reference.
Recommended publications
  • Refraction and Reflexion According to the Principle of General Covariance
    REFRACTION AND REFLEXION ACCORDING TO THE PRINCIPLE OF GENERAL COVARIANCE PATRICK IGLESIAS-ZEMMOUR Abstract. We show how the principle of general covariance introduced by Souriau in smoothly uniform contexts, can be extended to singular situ- ations, considering the group of diffeomorphisms preserving the singular locus. As a proof of concept, we shall see how we get again this way, the laws of reflection and refraction in geometric optics, applying an extended general covariance principle to Riemannian metrics, discontinuous along a hypersurface. Introduction In his paper “Modèle de particule à spin dans le champ électromagnétique et gravitationnel” published in 1974 [Sou74], Jean-Marie Souriau suggests a pre- cise mathematical interpretation of the principle of General Relativity. He names it the Principle of General Covariance. Considering only gravitation field1, he claimed that any material presence in the universe is characterized by a covector defined on the quotient of the set of the Pseudo-Riemannian metrics on space-time, by the group of diffeomorphisms. This principle be- ing, according to Souriau, the correct statement of the Einsteins’s principle of invariance with respect to any change of coordinates. Actually, Souriau’s general covariance principle can be regarded as the active version of Einstein invariance statement, where change of coordinates are interpreted from the active point of view as the action of the group of diffeomorphisms. Now, for reasons relative to the behavior at infinity and results requirement, the group of diffeomorphisms of space-time is reduced to the subgroup of compact supported diffeomorphisms. Date: April 6, 2019. 1991 Mathematics Subject Classification. 83C10, 78A05, 37J10.
    [Show full text]
  • Quantum Mechanics from General Relativity : Particle Probability from Interaction Weighting
    Annales de la Fondation Louis de Broglie, Volume 24, 1999 25 Quantum Mechanics From General Relativity : Particle Probability from Interaction Weighting Mendel Sachs Department of Physics State University of New York at Bualo ABSTRACT. Discussion is given to the conceptual and mathemat- ical change from the probability calculus of quantum mechanics to a weighting formalism, when the paradigm change takes place from linear quantum mechanics to the nonlinear, holistic eld theory that accompanies general relativity, as a fundamental theory of matter. This is a change from a nondeterministic, linear theory of an open system of ‘particles’ to a deterministic, nonlinear, holistic eld the- ory of the matter of a closed system. RESUM E. On discute le changement conceptuel et mathematique qui fait passer du calcul des probabilites de la mecanique quantique a un formalisme de ponderation, quand on eectue le changement de paradigme substituantalam ecanique quantique lineairelatheorie de champ holistique non lineaire qui est associee alatheorie de la relativitegenerale, prise comme theorie fondamentale de la matiere. Ce changement mene d’une theorie non deterministe et lineaire decrivant un systeme ouvert de ‘particules’ a une theorie de champ holistique, deterministe et non lineaire, de la matiere constituant un systeme ferme. 1. Introduction. In my view, one of the three most important experimental discov- eries of 20th century physics was the wave nature of matter. [The other two were 1) blackbody radiation and 2) the bending of a beam of s- tarlight as it propagates past the vicinity of the sun]. The wave nature of matter was predicted in the pioneering theoretical studies of L.
    [Show full text]
  • Covariance in Physics and Convolutional Neural Networks
    Covariance in Physics and Convolutional Neural Networks Miranda C. N. Cheng 1 2 3 Vassilis Anagiannis 2 Maurice Weiler 4 Pim de Haan 5 4 Taco S. Cohen 5 Max Welling 5 Abstract change of coordinates. In his words, the general principle In this proceeding we give an overview of the of covariance states that “The general laws of nature are idea of covariance (or equivariance) featured in to be expressed by equations which hold good for all sys- the recent development of convolutional neural tems of coordinates, that is, are covariant with respect to networks (CNNs). We study the similarities and any substitutions whatever (generally covariant)” (Einstein, differencesbetween the use of covariance in theo- 1916). The rest is history: the incorporation of the math- retical physics and in the CNN context. Addition- ematics of Riemannian geometry in order to achieve gen- ally, we demonstrate that the simple assumption eral covariance and the formulation of the general relativity of covariance, together with the required proper- (GR) theory of gravity. It is important to note that the seem- ties of locality, linearity and weight sharing, is ingly innocent assumption of general covariance is in fact sufficient to uniquely determine the form of the so powerful that it determines GR as the unique theory of convolution. gravity compatible with this principle, and the equivalence principle in particular, up to short-distance corrections1. In a completely different context, it has become clear 1. Covariance and Uniqueness in recent years that a coordinate-independent description It is well-known that the principle of covariance, or coordi- is also desirable for convolutional networks.
    [Show full text]
  • Lost in the Tensors: Einstein's Struggles with Covariance Principles 1912-1916"
    JOHN EARMAN and CLARK GL YMOUR LOST IN THE TENSORS: EINSTEIN'S STRUGGLES WITH COVARIANCE PRINCIPLES 1912-1916" Introduction IN 1912 Einstein began to devote a major portion of his time and energy to an attempt to construct a relativistic theory of gravitation. A strong intimation of the struggle that lay ahead is contained in a letter to Arnold Sommerfeld dated October 29, 1912: At the moment I am working solely on the problem of gravitation and believe 1 will be able to overcome all difficulties with the help of a local, friendly mathemat- ician. But one thing is certain, that I have never worked so hard in my life, and that I have been injected with a great awe of mathematics, which in my naivet~ until now I only viewed as a pure luxury in its subtler forms! Compared to this problem the original theory of relativity is mere child's play.' Einstein's letter contained only a perfunctory reply to a query from Sommerfeld about the Debye-Born theory of specific heats. Obviously disappointed, Som- merfeld wrote to Hilbert: 'My letter to Einstein was in vain . Einstein is evidently so deeply mired in gravitation that he is deaf to everything else? Sommerfeld's words were more prophetic than he could possibly have known; the next three years were to see Einstein deeply mired in gravitation, sometimes seemingly hopelessly so. In large measure, Einstein's struggle resulted from his use and his misuse, his understanding and his misunderstanding of the nature and implications of covariance principles. In brief, considerations of general covariance were bound up with Einstein's motive for seeking a 'generalized' theory of relativity; mis- understandings about the meaning and implementation of this motivation threatened to wreck the search; and in the end, the desire for general covariance helped to bring Einstein back onto the track which led to what we now recognize *Present address c/o Department of Philosophy, University of Minnesota, Minneapolis, Minn, U.S.A.
    [Show full text]
  • Introduction
    note1 : August 29, 2012 Introduction Principle of locality The principle of locality states that an object can Quantum Field Theory—in the context of parti- only be influenced by its immediate surroundings. cle physics—is a theory of elementary particles and From this principle follows the finite speed of in- their interactions. The Standard Model of elemen- formation transmission. tary particles is a quantum field theory. By definition, elementary particles are the most Principle of covariance fundamental—structureless—particles (like elec- trons and photons). They exhibit wave-particle du- The principle of covariance emphasizes formulation ality: on the one hand they diffract and interfere as of physical laws using only those physical quanti- waves (fields), on the other hand they appear and ties the measurements of which the observers in disappear as whole entities, called quanta. Hence different frames of reference could unambiguously the name of the theory. correlate. A quantum field theory seeks to explain certain Mathematically speaking, the physical quantities fundamental experimental observations—the exis- must transform covariantly, that is, under a certain tence of antiparticles, the spin-statistics relation, representation of the group of coordinate transfor- the CPT symmetry—as well as predict the results mations between admissible frames of reference of of any given experiment, like the cross-section for the physical theory. This group of coordinate trans- the Compton scattering, or the value of the anoma- formations is referred to as the covariance group of lous magnetic moment of the electron. the theory. There are two popular approaches to deal with The principle of covariance does not require in- quantum fields.
    [Show full text]
  • Phys 4390: General Relativity Lecture 5: Intro. to Tensor Algebra
    PHYS 4390: GENERAL RELATIVITY LECTURE 5: INTRO. TO TENSOR ALGEBRA Vectors are sufficient to describe Newtonian mechanics, however General Rela- tivity will require more general objects than vectors, namely tensors. To introduce these, we will first discuss the tensor algebra through an abstract approach, and afterwards introduce the conventional approach based on indices. While much of our discussion of tensors will appear to be in Rn, tensors may be defined on any differential manifold. This is due to the fact that a differential manifold is an object that appears locally like Euclidean space but is globally different. 1. Curves and Surfaces on a Manifold 1.1. Parametric Approach. A curve may be described with one single parame- ter, u, and defines coordinates in an n-dimensional manifold, xa = xa(u); a = 1; ::n: A surface has two parameters, and may be written as xa = xa(u; v) and in general a m-dimensional surface has m degrees of freedom, and is defined by xa = xa(u1; u2; :::; um) We may call a surface a subspace, and a surface with m = n − 1 degrees of freedom a hypersurface. 1.2. I. nstead of a parametric approach, we can describe a surface as a set of constraints. To see how, consider a hypersurface, xa = xa(u1; :::; un−1), taking each coordinate xa we could eliminate u1 to un−1 leaving one function that must vanish f(x1; x2; :::; xn) = 0 Thus, the parametric approach for a hypersurface is equivalent to imposing a con- straint. As an example in R2 the constraint x2 + y2 − R2 = 0 describes a circle ( i.e., S1).
    [Show full text]
  • A Brief Study on Covariance of Newtonian Mechanics
    Dr Dev Raj Mishra. International Journal of Engineering Research and Applications www.ijera.com ISSN: 2248-9622, Vol. 10, Issue 7, (Series-IV) July 2020, pp. 11-15 RESEARCH ARTICLE OPEN ACCESS A Brief Study on Covariance of Newtonian Mechanics Dr Dev Raj Mishra Department of Physics, R.H.Government Post Graduate College, Kashipur, U.S.Nagar, Uttarakhand -244713 INDIA. ABSTRACT The possibility of a covariant formulation of Newton’s second law of motion using Energy-Momentum four- vector was explored. This covariant formulation explains the relationships between the electromagnetic potentials and the electromagnetic fields. It successfully explains the observation of pseudo-forces in nature for example the observed up-thrust in a falling frame of reference or a falling lift and the observed centrifugal force in circular motion. Keywords– Covariance,Electromagnetic Field Tensor,Four- vectors, Minkowski Space time, Relativity ----------------------------------------------------------------------------------------------------------------------------- ---------- Date of Submission: 06-07-2020 Date of Acceptance: 21-07-2020 ----------------------------------------------------------------------------------------------------------------------------- ---------- I. INTRODUCTION the applied force and the momentum. The applied The invariance under Lorentz force is also the gradient of potential energy. transformation expresses the proposition that the Therefore we have two quantities – the momentum laws of physics are same for the observers in and
    [Show full text]
  • How Einstein Got His Field Equations Arxiv:1608.05752V1 [Physics.Hist-Ph]
    How Einstein Got His Field Equations S. Walters In commemoration of General Relativity’s centennial ABSTRACT. We study the pages in Albert Einstein’s 1916 landmark paper in the Annalen der Physik where he derived his field equations for gravity. Einstein made two heuristic and physically insightful steps. The first was to obtain the field equations in vacuum in a rather geometric fashion. The second step was obtaining the field equations in the presence of matter from the field equations in vacuum. (This transition is an essential principle in physics, much as the principle of local gauge invariance in quantum field theory.) To this end, we go over some quick differential geometric background related to curvilinear coordinates, vectors, tensors, metric tensor, Christoffel symbols, Riemann curvature tensor, Ricci tensor, and see how Einstein used geometry to model gravity. This paper is a more detailed version of my talk given at the Math-Physics Symposium at UNBC on February 25, 2016. It is in reference to Einstein’s paper: A. Einstein, The Foundation of the General Theory of Relativity, Annalen der Physik, 49, 1916. (For an English translation see: H. A. Lorentz, A. Einstein, H. Minkowski, H. Weyl, The Principle of Relativity.) The paper has two sections. The first section is a smash course on the semi-Riemannian geometry tools needed to understand Einstein’s theory. The second section looks at Einstein’s derivation of his field equations in vac- uum and in the presence of matter and/or electromagnetism as he worked them out in his paper. This paper commemorates the 100th centennial of Einstein’s General The- ory of Relativity, which he finalized near the end of November 1915 and pub- lished in 1916.
    [Show full text]
  • Introduction Can Only Be Influenced by Its Immediate Sur- Roundings
    1 note1 : November 4, 2014 Introduction can only be influenced by its immediate sur- roundings. In the context of particle physics, Quantum Field Theory is a theory of elementary particles and their From this principle follows the finite speed of interactions. The Standard Model of elementary information transmission. particles is a quantum field theory. Principle of covariance By definition, elementary particles are the most The principle of covariance emphasizes formu- fundamental — structureless — particles (like elec- lation of physical laws using only those phys- trons and photons) which exist in our universe. Ele- ical quantities the measurements of which the mentary particles exhibit wave-particle duality: on observers in different frames of reference could the one hand they diffract and interfere as waves unambiguously correlate. (or fields), on the other hand they appear and dis- appear as whole entities (called quanta). Hence the Mathematically speaking, the physical quanti- name of the theory. ties must transform covariantly, that is, un- A quantum field theory seeks to explain certain der a certain representation of the group of fundamental experimental observations — like the coordinate transformations between admissi- existence of antiparticles; the spin-statistics rela- ble frames of reference of the physical theory. tion; the CPT symmetry — as well as to predict This group of coordinate transformations is re- the results of any given experiment, like the cross- ferred to as the covariance group of the theory. section for the Compton scattering, or the value of The principle of covariance does not require the anomalous magnetic moment of the electron. invariance of physical laws under the group of There are two popular approaches to deal with admissible transformations although in most quantum fields.
    [Show full text]
  • Lorentz Covariant Formulations of Fluid Dynamics and Electrodynamics
    Fall 2019: Gravitation and Cosmology (PH6458/ EP4258) Lorentz covariant formulations of fluid dynamics and Electrodynamics∗ September 27, 2019 1 Principle of covariance in special relativity and Poincar´einvariance of the action In class I mentioned that laws of physics (or equivalently equations of motion of physical systems) must have the \same form" in all inertial frames. From a practical point of view this means, one should be able to write down physical law/equations in the form, ::: T::: = 0: ::: The quantity on the left hand side, namely T::: , is some tensor (could be any generic(p; q)-rank tensor). This guarantees that if one performs a Lorentz transformation (or more generally a Poincar´etransforma- tion), the equation in the new inertial frame will be identical looking, i.e., 0::: T ::: = 0! This is ensured because tensors transform homogeneously under a Lorentz transformation, 0::: ¯ ::: T ::: = Λ ::: Λ :::T :::; where Λ and Λ¯ are the direct and inverse Lorentz transformation matrix elements. So the next logical question is how do we go about writing down physical equations/laws in tensor form to begin with. To answer this question we recall that in general we obtain equations of motion for any physical system are obtained from an action (functional), I by applying the variational principle, δI = 0: The principle of covariance is then tantamount to demanding that the action, I itself is invariant under Poincar´etransformation. One might ask, why does the action has to be a scalar (i.e. invariant) and not a tensor of a more general kind. The answer I believe cannot be found in the classical realm but instead lies in the quantum real where the action determines probability amplitudes of various processes, eiI .
    [Show full text]
  • A Clifford Dyadic Superfield from Bilateral Interactions of Geometric
    A Clifford Dyadic Superfield from Bilateral Interactions of Geometric Multispin Dirac Theory WILLIAM M. PEZZAGLIA JR. Department of Physics Santa Clara University Santa Clara, CA 95053 U.S.A. Email: [email protected] and ALFRED W. DIFFER Department of Physics American River College Sacramento, CA 95841 U.S.A. (Received: Oct 1993) Abstract. Multivector quantum mechanics utilizes wavefunctions which are Clifford aggre- gates (e.g. sum of scalar, vector, bivector). This is equivalent to multispinors constructed of Dirac matrices, with the representation independent form of the generators geometri- cally interpreted as the basis vectors of spacetime. Multiple generations of particles appear as left ideals of the algebra, coupled only by now-allowed right-side applied (dextral) oper- ations. A generalized bilateral (two-sided operation) coupling is proposed which includes the above mentioned dextrad field, and the spin-gauge interaction as particular cases. This leads to a new principle of poly-dimensional covariance, in which physical laws are invariant under the reshuffling of coordinate geometry. Such a multigeometric superfield equation is proposed, which is sourced by a bilateral current. In order to express the superfield in rep- resentation and coordinate free form, we introduce Eddington E-F double-frame numbers. Symmetric tensors can now be represented as 4D “dyads”, which actually are elements of a global 8D Clifford algebra. As a restricted example, the dyadic field created by the Greider-Ross multivector current (of a Dirac electron) describes both electromagnetic and Morris-Greider gravitational interactions. Key words: spin-gauge, multivector, clifford, dyadic arXiv:gr-qc/9311015v1 9 Nov 1993 1.
    [Show full text]
  • 5 Four Vectors
    Physics 139 Relativity Relativity Notes 2002 G. F. SMOOT Oce 398 Le Conte DepartmentofPhysics, University of California, Berkeley, USA 94720 Notes to b e found at http://aether.lbl.gov/www/classes/p139/homework/homework.html 5 Four Vectors A natural extension of the Minkowski geometrical interpretation of Sp ecial Relativity is the concept of four dimensional vectors. One could also arrive at the concept by lo oking at the transformation prop erties of vectors and noticing they do not transform as vectors unless another comp onent is added. We de ne a four-dimensional vector or four-vector for short as a collection of four comp onents that transforms according to the Lorentz transformation. The vector magnitude is invariant under the Lorentz transform. 5.1 Co ordinate Transformations in 3+1-D Space One can consider co ordinate transformations manyways: If x ;x ;x ;x = x; y ; z ; ict, 1 2 3 4 then ordinary rotations in x x plane around x 1 2 3 0 x = x cos + x sin cos sin 1 2 1 0 x = x sin + x cos sin cos 1 2 2 But in x x plane: 1 4 0 x = x cos + x sin cos sin 1 4 1 0 x = x sin + x cos sin cos 1 4 4 where the angle is de ned by q p 2 2 2 cos =1= 1v =c =1= 1+tan = tan v=c q p = sin = i 2 2 2 1+tan 1 v =c tan = iv =c = i : And thus one has the trignometic identity: 2 2 2 2 cos + sin = 1 =1 1 0 x = [x +icti ] = [x ct] 1 1 1 0 x = [x i x ] 4 1 4 0 ict = [ict i x ] 1 0 ct = [ct x ] 1 0 t = [t x =c] 1 So the extension to 3+1-D includes Lorentz transformations, if angles are imaginary.
    [Show full text]