1 Electromagnetic Fields and Charges In
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
General Relativity
GENERAL RELATIVITY IAN LIM LAST UPDATED JANUARY 25, 2019 These notes were taken for the General Relativity course taught by Malcolm Perry at the University of Cambridge as part of the Mathematical Tripos Part III in Michaelmas Term 2018. I live-TEXed them using TeXworks, and as such there may be typos; please send questions, comments, complaints, and corrections to [email protected]. Many thanks to Arun Debray for the LATEX template for these lecture notes: as of the time of writing, you can find him at https://web.ma.utexas.edu/users/a.debray/. Contents 1. Friday, October 5, 2018 1 2. Monday, October 8, 2018 4 3. Wednesday, October 10, 20186 4. Friday, October 12, 2018 10 5. Wednesday, October 17, 2018 12 6. Friday, October 19, 2018 15 7. Monday, October 22, 2018 17 8. Wednesday, October 24, 2018 22 9. Friday, October 26, 2018 26 10. Monday, October 29, 2018 28 11. Wednesday, October 31, 2018 32 12. Friday, November 2, 2018 34 13. Monday, November 5, 2018 38 14. Wednesday, November 7, 2018 40 15. Friday, November 9, 2018 44 16. Monday, November 12, 2018 48 17. Wednesday, November 14, 2018 52 18. Friday, November 16, 2018 55 19. Monday, November 19, 2018 57 20. Wednesday, November 21, 2018 62 21. Friday, November 23, 2018 64 22. Monday, November 26, 2018 67 23. Wednesday, November 28, 2018 70 Lecture 1. Friday, October 5, 2018 Unlike in previous years, this course is intended to be a stand-alone course on general relativity, building up the mathematical formalism needed to construct the full theory and explore some examples of interesting spacetime metrics. -
Chapter 13 Curvature in Riemannian Manifolds
Chapter 13 Curvature in Riemannian Manifolds 13.1 The Curvature Tensor If (M, , )isaRiemannianmanifoldand is a connection on M (that is, a connection on TM−), we− saw in Section 11.2 (Proposition 11.8)∇ that the curvature induced by is given by ∇ R(X, Y )= , ∇X ◦∇Y −∇Y ◦∇X −∇[X,Y ] for all X, Y X(M), with R(X, Y ) Γ( om(TM,TM)) = Hom (Γ(TM), Γ(TM)). ∈ ∈ H ∼ C∞(M) Since sections of the tangent bundle are vector fields (Γ(TM)=X(M)), R defines a map R: X(M) X(M) X(M) X(M), × × −→ and, as we observed just after stating Proposition 11.8, R(X, Y )Z is C∞(M)-linear in X, Y, Z and skew-symmetric in X and Y .ItfollowsthatR defines a (1, 3)-tensor, also denoted R, with R : T M T M T M T M. p p × p × p −→ p Experience shows that it is useful to consider the (0, 4)-tensor, also denoted R,givenby R (x, y, z, w)= R (x, y)z,w p p p as well as the expression R(x, y, y, x), which, for an orthonormal pair, of vectors (x, y), is known as the sectional curvature, K(x, y). This last expression brings up a dilemma regarding the choice for the sign of R. With our present choice, the sectional curvature, K(x, y), is given by K(x, y)=R(x, y, y, x)but many authors define K as K(x, y)=R(x, y, x, y). Since R(x, y)isskew-symmetricinx, y, the latter choice corresponds to using R(x, y)insteadofR(x, y), that is, to define R(X, Y ) by − R(X, Y )= + . -
Spacetime Structuralism
Philosophy and Foundations of Physics 37 The Ontology of Spacetime D. Dieks (Editor) r 2006 Elsevier B.V. All rights reserved DOI 10.1016/S1871-1774(06)01003-5 Chapter 3 Spacetime Structuralism Jonathan Bain Humanities and Social Sciences, Polytechnic University, Brooklyn, NY 11201, USA Abstract In this essay, I consider the ontological status of spacetime from the points of view of the standard tensor formalism and three alternatives: twistor theory, Einstein algebras, and geometric algebra. I briefly review how classical field theories can be formulated in each of these formalisms, and indicate how this suggests a structural realist interpre- tation of spacetime. 1. Introduction This essay is concerned with the following question: If it is possible to do classical field theory without a 4-dimensional differentiable manifold, what does this suggest about the ontological status of spacetime from the point of view of a semantic realist? In Section 2, I indicate why a semantic realist would want to do classical field theory without a manifold. In Sections 3–5, I indicate the extent to which such a feat is possible. Finally, in Section 6, I indicate the type of spacetime realism this feat suggests. 2. Manifolds and manifold substantivalism In classical field theories presented in the standard tensor formalism, spacetime is represented by a differentiable manifold M and physical fields are represented by tensor fields that quantify over the points of M. To some authors, this has 38 J. Bain suggested an ontological commitment to spacetime points (e.g., Field, 1989; Earman, 1989). This inclination might be seen as being motivated by a general semantic realist desire to take successful theories at their face value, a desire for a literal interpretation of the claims such theories make (Earman, 1993; Horwich, 1982). -
On a Complex Spacetime Frame : New Foundation for Physics and Mathematics
On a complex spacetime frame : new foundation for physics and mathematics Joseph Akeyo Omolo∗ Department of Physics and Materials Science, Maseno University P.O. Private Bag, Maseno, Kenya e-mail: [email protected] March 31, 2016 Abstract This paper provides a derivation of a unit vector specifying the tem- poral axis of four-dimensional space-time frame as an imaginary axis in the direction of light or general wave propagation. The basic elements of the resulting complex four-dimensional spacetime frame are complex four-vectors expressed in standard form as four-component quantities specified by four unit vectors, three along space axes and one along the imaginary temporal axis. Consistent mathematical operations with the complex four-vectors have been developed, which provide extensions of standard vector analysis theorems to complex four-dimensional space- time. The general orientation of the temporal unit vector relative to all the three mutually perpendicular spatial unit vectors leads to ap- propriate modifications of fundamental results describing the invariant length of the spacetime event interval, time dilation, mass increase with speed and relativistic energy conservation law. Contravariant and co- variant forms have been defined, providing appropriate definition of the invariant length of a complex four-vector and appropriate definitions of complex tensors within the complex four-dimensional spacetime frame, thus setting a new geometrical framework for physics and mathematics. 1 Introduction Four-dimensional space-time frame is the natural reference frame for de- scribing the general dynamics of physical systems. Its basic elements are ∗Regular Associate, Abdus Salam ICTP: 2001-2006 1 four-vectors, which are suitable for expressing field equations and associ- ated physical quantities in consistent forms. -
Deformations with Maximal Supersymmetries Part 2: Off-Shell Formulation
Deformations with maximal supersymmetries part 2: off-shell formulation The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Chang, Chi-Ming et al. “Deformations with Maximal Supersymmetries Part 2: Off-Shell Formulation.” Journal of High Energy Physics 2016.4 (2016): n. pag. As Published http://dx.doi.org/10.1007/JHEP04(2016)171 Publisher Springer Berlin Heidelberg Version Final published version Citable link http://hdl.handle.net/1721.1/103304 Terms of Use Creative Commons Attribution Detailed Terms http://creativecommons.org/licenses/by/4.0/ Published for SISSA by Springer Received: February 26, 2016 Accepted: April 23, 2016 Published: April 28, 2016 Deformations with maximal supersymmetries part 2: JHEP04(2016)171 off-shell formulation Chi-Ming Chang,a Ying-Hsuan Lin,a Yifan Wangb and Xi Yina aJefferson Physical Laboratory, Harvard University, Cambridge, MA 02138, U.S.A. bCenter for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, U.S.A. E-mail: [email protected], [email protected], [email protected], [email protected] Abstract: Continuing our exploration of maximally supersymmetric gauge theories (MSYM) deformed by higher dimensional operators, in this paper we consider an off- shell approach based on pure spinor superspace and focus on constructing supersymmetric deformations beyond the first order. In particular, we give a construction of the Batalin- Vilkovisky action of an all-order non-Abelian Born-Infeld deformation of MSYM in the non-minimal pure spinor formalism. We also discuss subtleties in the integration over the pure spinor superspace and the relevance of Berkovits-Nekrasov regularization. -
Spacetime As a Feynman Diagram: the Connection Formulation
Spacetime as a Feynman diagram: the connection formulation Michael P. Reisenberger Theoretical Physics Group, Blackett Laboratory, Imperial College, London, SW7 2BZ, UK. Center for Gravitational Physics and Geometry, The Pennsylvania State University, 104 Davey Lab, University Park, PA16802-6300, USA [email protected] Carlo Rovelli Physics Department, University of Pittsburgh, Pittsburgh, PA 15260, USA. Centre de Physique Th´eorique, CNRS Luminy, 13288 Marseille, France [email protected] March 3, 2000 Abstract Spin foam models are the path integral counterparts to loop quantized canonical theories. In the last few years several spin foam models of gravity have been proposed, most of which live on finite simplicial lattice spacetime. The lattice truncates the presumably infinite set of gravitational degrees of freedom down to a finite set. Models that can accomodate an infinite set of degrees of freedom and that are independent of any background simplicial structure, or indeed any a priori spacetime topology, can be obtained from the lattice models by summing them over all lattice spacetimes. Here we show that this sum can be realized as the sum over Feynman diagrams of a quantum 1 field theory living on a suitable group manifold, with each Feynman diagram defining a particular lattice spacetime. We give an explicit formula for the action of the field theory corresponding to any given spin foam model in a wide class which includes several gravity mod- els. Such a field theory was recently found for a particular gravity model [1]. Our work generalizes this result as well as Boulatov’s and Ooguri’s models of three and four dimensional topological field theo- ries, and ultimately the old matrix models of two dimensional systems with dynamical topology. -
Eienstein Field Equations and Heisenberg's Principle Of
International Journal of Scientific and Research Publications, Volume 2, Issue 9, September 2012 1 ISSN 2250-3153 EIENSTEIN FIELD EQUATIONS AND HEISENBERG’S PRINCIPLE OF UNCERTAINLY THE CONSUMMATION OF GTR AND UNCERTAINTY PRINCIPLE 1DR K N PRASANNA KUMAR, 2PROF B S KIRANAGI AND 3PROF C S BAGEWADI ABSTRACT: The Einstein field equations (EFE) or Einstein's equations are a set of 10 equations in Albert Einstein's general theory of relativity which describe the fundamental interaction (e&eb) of gravitation as a result of space time being curved by matter and energy. First published by Einstein in 1915 as a tensor equation, the EFE equate spacetime curvature (expressed by the Einstein tensor) with (=) the energy and momentum tensor within that spacetime (expressed by the stress–energy tensor).Both space time curvature tensor and energy and momentum tensor is classified in to various groups based on which objects they are attributed to. It is to be noted that the total amount of energy and mass in the Universe is zero. But as is said in different context, it is like the Bank Credits and Debits, with the individual debits and Credits being conserved, holistically, the conservation and preservation of Debits and Credits occur, and manifest in the form of General Ledger. Transformations of energy also take place individually in the same form and if all such transformations are classified and written as a Transfer Scroll, it should tally with the total, universalistic transformation. This is a very important factor to be borne in mind. Like accounts are classifiable based on rate of interest, balance standing or the age, we can classify the factors and parameters in the Universe, be it age, interaction ability, mass, energy content. -
Noncommutative Quantum Gravity
Noncommutative Quantum Gravity J. W. Moffat Department of Physics, University of Toronto, Toronto, Ontario M5S 1A7, Canada Abstract The possible role of gravity in a noncommutative geometry is investi- gated. Due to the Moyal *-product of fields in noncommutative geometry, it is necessary to complexify the metric tensor of gravity. We first consider the possibility of a complex Hermitian, nonsymmetric gµν and discuss the problems associated with such a theory. We then introduce a complex symmetric (non-Hermitian) metric, with the associated complex connec- tion and curvature, as the basis of a noncommutative spacetime geometry. The spacetime coordinates are in general complex and the group of local gauge transformations is associated with the complex group of Lorentz transformations CSO(3, 1). A real action is chosen to obtain a consistent set of field equations. A Weyl quantization of the metric associated with the algebra of noncommuting coordinates is employed. 1 Introduction The concept of a quantized spacetime was proposed by Snyder [1], and has received much attention over the past few years [2-6]. There has been renewed interest recently in noncommutative field theory, since it makes its appearance in string theory, e.g. noncommutative gauge theories describe the low energy excitations of open strings on D-branes in a background two-form B field [5,7-12]. Noncommutative Minkowski space is defined in terms of spacetime coordinates xµ, µ =0, ...3, which satisfy the following commutation relations [xµ, xν ]= iθµν , (1) arXiv:hep-th/0007181v2 25 Sep 2000 where θµν is an antisymmetric tensor. In what follows, we can generally extend the results to higher dimensions µ =0, ...d. -
Euclidean Closed Linear Transformations of Complex Spacetime and Generally of Complex Spaces of Dimension Four Endowed with the Same Or Different Metric
Journal of Physics: Conference Series PAPER • OPEN ACCESS Related content - A simple example of type-[N] otimes Euclidean Closed Linear Transformations of [N]HH-spaces admitting twisting null geodesic congruence Complex Spacetime and generally of Complex Adam Chudecki and Maciej Przanowski - Distributional sources for Newman's Spaces of dimension four endowed with the Same holomorphic Coulomb field Gerald Kaiser or Different Metric - The generalized good cut equation T M Adamo and E T Newman To cite this article: Spyridon Vossos and Elias Vossos 2016 J. Phys.: Conf. Ser. 738 012048 Recent citations - Explanation of Rotation Curves in Galaxies View the article online for updates and enhancements. and Clusters of them, by Generalization of Schwarzschild Metric and Combination with MOND, eliminating Dark Matter Spyridon Vossos and Elias Vossos This content was downloaded from IP address 131.169.4.70 on 11/01/2018 at 22:43 5th International Conference on Mathematical Modeling in Physical Sciences (IC-MSquare 2016) IOP Publishing Journal of Physics: Conference Series 738 (2016) 012048 doi:10.1088/1742-6596/738/1/012048 Euclidean Closed Linear Transformations of Complex Spacetime and generally of Complex Spaces of dimension four endowed with the Same or Different Metric Spyridon Vossos1, 3 and Elias Vossos2 1Chemist, 2Physicist, School of Science, National and Kapodistrian University of Athens, Panepistimiopolis, GR15784 Zografos, Athens, Hellas E-mail: [email protected] Keywords: 5th Euclidean postulate, complex space, Einstein equations, Euclidean complex relativistic mechanics, Euclidean metric, general relativity, human senses, isometry, linear spacetime transformation, Lorentz matrix, Lorentz metric, Lorentz transformation, Minkowski space, Schwarzschild metric, spacetime, special relativity, real space, universal speed, velocity, Vossos matrix, Vossos transformation. -
Lecture Notes PX421: Relativity and Electrodynamics
Lecture Notes PX421: Relativity and Electrodynamics Y.A. Ramachers, University of Warwick Draft date April 11, 2014 Contents Contents i 1 Full Special Relativity 3 1.1 Homogeneityandisotropyofspace . 3 1.2 Introducingthetimeparameter . 5 1.2.1 Excursion: ’What is a group and why is it interesting here?.. 6 1.3 ThewaybeyondGalileanrelativity . 8 1.4 Derivation of the Lorentz transformation . .... 9 1.4.1 Linearity and absence of change of direction . .. 9 1.4.2 Invarianceundertimereflection . 10 1.4.3 Identityassumption. 11 1.4.4 Finish deriving the one-dimensional Lorentz transformations . 12 1.4.5 Whataboutothervelocitiesthanc?. 13 1.4.6 Three-dimensional Lorentz transformations . .... 13 1.4.7 First glimpse at a compact way of writing Lorentz transfor- mations .............................. 15 1.4.8 Exercises.............................. 16 1.5 ExcursionTensorAnalysis . 17 1.5.1 Introduction............................ 17 1.5.2 Workingwithtensors. 20 1.5.3 Transformations. 30 1.5.4 BacktoLorentztransformations. 33 i ii CONTENTS 1.5.5 Exercises.............................. 36 2 Applications: Mechanics 39 2.1 ProperTime................................ 40 2.2 Four-velocity ............................... 41 2.2.1 Exercises.............................. 42 2.3 Relativistickinematicsessentials. ..... 43 2.3.1 Exercises.............................. 45 2.4 Energy-mass equivalence derivation, Einstein 1906 . ........ 46 2.5 Waves ................................... 48 2.5.1 Lightraysandtakingphotos. 50 2.5.2 Exercises.............................. 52 2.6 Linear acceleration in special relativity . ...... 53 2.6.1 Kinematicsincoordinatelanguage . 56 2.6.2 Rindlercoordinates . 58 2.6.3 Exercises.............................. 62 3 Applications: Electromagnetism 63 3.1 Reminderondifferentialoperators. .. 64 3.2 BacktotheMaxwellequations . 65 3.3 Frompotentialstofields . 67 3.3.1 Exercises.............................. 69 3.4 ParticleDynamics............................. 70 3.4.1 Exercises.............................. 71 3.5 Conservationlawsforfields . -
The Metaphysics of Physics the Speed of Darkness
Lewis - 954 – THE METAPHYSICS OF PHYSICS THE SPEED OF DARKNESS (S.O.D.) ONE THOUSAND STEPS TO CHAOS CHAPTER XXXXV THE PHYSICS AND METAPHYSICS OF SYMMETRICS AXIOMS OF SIMPLEXITY (THE SIMPLE & THE COMPLEX) The Physics of Symmetry (Symmetrics-Transformatics: The First 313 Simplexity Axioms). Before I can interpret the complexities of the combination of Symmetrics and Asymmetrics (Non-Symmetrics: The Grand Synthesis-Unification-De- Unification) in an Infinite, Unbounded, (open-closed) Universe; it is necessary to sum up the known facts of the Symmetric, Infinite, Unbounded Universe as interpreted by Physicists and Cosmologists in the 20th and 21st Century. Infinitism, Transformatics, Reverseamatics, Asymmetrics (Non-Symmetrics) and the Metaphysics of Structural Cosmology will be derived in the last 687 Axioms after I take a look at the special case of Symmetry (Axioms 1-313). 1. In the last decade there has been an attempt to merge GUT Theory (Grand Unification Theory) with TOE Theory (Theory of Everything) by combining their counterparts GUUT Theory (Grand Un-Unified Theory) and TON Theory (Theory of Nothing or Lewis - 955 - Theory of S.O.D. - Speed of Darkness Theory) incorporating SMGT Theory (Super Modern Gravitational Theory, which also includes the Forces and Interactions over and above the four know Forces), in order to discover the solution to all the major Interactions along with their minor Constituents. (See Axioms 314-1,000 on Asymmetrics and Non-Symmetrics). A discussion of the Chronons, the Quanta of Time, Chronodynamics and their special relationships to Symmetrics, Asymmetrics (Non-Symmetrics) and to the S-Wave Quanta, is reserved for the later Axioms. -
Oxford Physics Department Notes on General Relativity Steven Balbus
Oxford Physics Department Notes on General Relativity Steven Balbus Version: January 25, 2017 1 These notes are intended for classroom use. There is little here that is original, but a few results are. If you would like to quote from these notes and are unable to find an original literature reference, please contact me by email first. Thank you in advance for your cooperation. Steven Balbus 2 Recommended Texts Hobson, M. P., Efstathiou, G., and Lasenby, A. N. 2006, General Relativity: An Introduction for Physicists, (Cambridge: Cambridge University Press) Referenced as HEL06. A very clear, very well-blended book, admirably covering the mathematics, physics, and astrophysics of GR. Excellent presentation of black holes and gravitational radiation. The explanation of the geodesic equation and the affine connection is very clear and enlightening. Not so much on cosmology, though a nice introduction to the physics of inflation. Overall, my favourite text on this topic. (The metric has a different sign convention in HEL06 compared with Weinberg 1972 & MTW [see below], as well as these notes. Be careful.) Weinberg, S. 1972, Gravitation and Cosmology. Principles and Applications of the General Theory of Relativity, (New York: John Wiley) Referenced as W72. What is now the classic reference by the great man, but lacking any discussion whatsoever of black holes, and almost nothing on the geometrical interpretation of the equations. The author is explicit in his aversion to anything geometrical: gravity is a field theory with a mere geometrical \analogy" according to Weinberg. But there is no way to make sense of the equations, in any profound sense, without immersing onself in geometry.