Doing Physics with Quaternions.Pdf
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
A Mathematical Derivation of the General Relativistic Schwarzschild
A Mathematical Derivation of the General Relativistic Schwarzschild Metric An Honors thesis presented to the faculty of the Departments of Physics and Mathematics East Tennessee State University In partial fulfillment of the requirements for the Honors Scholar and Honors-in-Discipline Programs for a Bachelor of Science in Physics and Mathematics by David Simpson April 2007 Robert Gardner, Ph.D. Mark Giroux, Ph.D. Keywords: differential geometry, general relativity, Schwarzschild metric, black holes ABSTRACT The Mathematical Derivation of the General Relativistic Schwarzschild Metric by David Simpson We briefly discuss some underlying principles of special and general relativity with the focus on a more geometric interpretation. We outline Einstein’s Equations which describes the geometry of spacetime due to the influence of mass, and from there derive the Schwarzschild metric. The metric relies on the curvature of spacetime to provide a means of measuring invariant spacetime intervals around an isolated, static, and spherically symmetric mass M, which could represent a star or a black hole. In the derivation, we suggest a concise mathematical line of reasoning to evaluate the large number of cumbersome equations involved which was not found elsewhere in our survey of the literature. 2 CONTENTS ABSTRACT ................................. 2 1 Introduction to Relativity ...................... 4 1.1 Minkowski Space ....................... 6 1.2 What is a black hole? ..................... 11 1.3 Geodesics and Christoffel Symbols ............. 14 2 Einstein’s Field Equations and Requirements for a Solution .17 2.1 Einstein’s Field Equations .................. 20 3 Derivation of the Schwarzschild Metric .............. 21 3.1 Evaluation of the Christoffel Symbols .......... 25 3.2 Ricci Tensor Components ................. -
Schwarzschild Solution to Einstein's General Relativity
Schwarzschild Solution to Einstein's General Relativity Carson Blinn May 17, 2017 Contents 1 Introduction 1 1.1 Tensor Notations . .1 1.2 Manifolds . .2 2 Lorentz Transformations 4 2.1 Characteristic equations . .4 2.2 Minkowski Space . .6 3 Derivation of the Einstein Field Equations 7 3.1 Calculus of Variations . .7 3.2 Einstein-Hilbert Action . .9 3.3 Calculation of the Variation of the Ricci Tenosr and Scalar . 10 3.4 The Einstein Equations . 11 4 Derivation of Schwarzschild Metric 12 4.1 Assumptions . 12 4.2 Deriving the Christoffel Symbols . 12 4.3 The Ricci Tensor . 15 4.4 The Ricci Scalar . 19 4.5 Substituting into the Einstein Equations . 19 4.6 Solving and substituting into the metric . 20 5 Conclusion 21 References 22 Abstract This paper is intended as a very brief review of General Relativity for those who do not want to skimp on the details of the mathemat- ics behind how the theory works. This paper mainly uses [2], [3], [4], and [6] as a basis, and in addition contains short references to more in-depth references such as [1], [5], [7], and [8] when more depth was needed. With an introduction to manifolds and notation, special rel- ativity can be constructed which are the relativistic equations of flat space-time. After flat space-time, the Lagrangian and calculus of vari- ations will be introduced to construct the Einstein-Hilbert action to derive the Einstein field equations. With the field equations at hand the Schwarzschild equation will fall out with a few assumptions. -
The Schwarzschild Metric and Applications 1
The Schwarzschild Metric and Applications 1 Analytic solutions of Einstein's equations are hard to come by. It's easier in situations that e hibit symmetries. 1916: Karl Schwarzschild sought the metric describing the static, spherically symmetric spacetime surrounding a spherically symmetric mass distribution. A static spacetime is one for which there exists a time coordinate t such that i' all the components of g are independent of t ii' the line element ds( is invariant under the transformation t -t A spacetime that satis+es (i) but not (ii' is called stationary. An example is a rotating azimuthally symmetric mass distribution. The metric for a static spacetime has the form where xi are the spatial coordinates and dl( is a time*independent spatial metric. -ross-terms dt dxi are missing because their presence would violate condition (ii'. 23ote: The Kerr metric, which describes the spacetime outside a rotating ( axisymmetric mass distribution, contains a term ∝ dt d.] To preser)e spherical symmetry& dl( can be distorted from the flat-space metric only in the radial direction. In 5at space, (1) r is the distance from the origin and (2) 6r( is the area of a sphere. Let's de+ne r such that (2) remains true but (1) can be violated. Then, A,xi' A,r) in cases of spherical symmetry. The Ricci tensor for this metric is diagonal, with components S/ 10.1 /rimes denote differentiation with respect to r. The region outside the spherically symmetric mass distribution is empty. 9 The vacuum Einstein equations are R = 0. To find A,r' and B,r'# (. -
Embeddings and Time Evolution of the Schwarzschild Wormhole
Embeddings and time evolution of the Schwarzschild wormhole Peter Collasa) Department of Physics and Astronomy, California State University, Northridge, Northridge, California 91330-8268 David Kleinb) Department of Mathematics and Interdisciplinary Research Institute for the Sciences, California State University, Northridge, Northridge, California 91330-8313 (Received 26 July 2011; accepted 7 December 2011) We show how to embed spacelike slices of the Schwarzschild wormhole (or Einstein-Rosen bridge) in R3. Graphical images of embeddings are given, including depictions of the dynamics of this nontraversable wormhole at constant Kruskal times up to and beyond the “pinching off” at Kruskal times 61. VC 2012 American Association of Physics Teachers. [DOI: 10.1119/1.3672848] I. INTRODUCTION because the flow of time is toward r 0. Therefore, to under- stand the dynamics of the Einstein-Rosen¼ bridge or Schwarzs- 1 Schwarzschild’s 1916 solution of the Einstein field equa- child wormhole, we require a spacetime that includes not tions is perhaps the most well known of the exact solutions. only the two asymptotically flat regions associated with In polar coordinates, the line element for a mass m is Eq. (2) but also the region near r 0. For this purpose, the maximal¼ extension of Schwarzschild 1 2m 2m À spacetime by Kruskal7 and Szekeres,8 along with their global ds2 1 dt2 1 dr2 ¼À À r þ À r coordinate system,9 plays an important role. The maximal extension includes not only the interior and exterior of the r2 dh2 sin2 hd/2 ; (1) þ ð þ Þ Schwarzschild black hole [covered by the coordinates of Eq. -
Equivalence Principle (WEP) of General Relativity Using a New Quantum Gravity Theory Proposed by the Authors Called Electro-Magnetic Quantum Gravity Or EMQG (Ref
WHAT ARE THE HIDDEN QUANTUM PROCESSES IN EINSTEIN’S WEAK PRINCIPLE OF EQUIVALENCE? Tom Ostoma and Mike Trushyk 48 O’HARA PLACE, Brampton, Ontario, L6Y 3R8 [email protected] Monday April 12, 2000 ACKNOWLEDGMENTS We wish to thank R. Mongrain (P.Eng) for our lengthy conversations on the nature of space, time, light, matter, and CA theory. ABSTRACT We provide a quantum derivation of Einstein’s Weak Equivalence Principle (WEP) of general relativity using a new quantum gravity theory proposed by the authors called Electro-Magnetic Quantum Gravity or EMQG (ref. 1). EMQG is manifestly compatible with Cellular Automata (CA) theory (ref. 2 and 4), and is also based on a new theory of inertia (ref. 5) proposed by R. Haisch, A. Rueda, and H. Puthoff (which we modified and called Quantum Inertia, QI). QI states that classical Newtonian Inertia is a property of matter due to the strictly local electrical force interactions contributed by each of the (electrically charged) elementary particles of the mass with the surrounding (electrically charged) virtual particles (virtual masseons) of the quantum vacuum. The sum of all the tiny electrical forces (photon exchanges with the vacuum particles) originating in each charged elementary particle of the accelerated mass is the source of the total inertial force of a mass which opposes accelerated motion in Newton’s law ‘F = MA’. The well known paradoxes that arise from considerations of accelerated motion (Mach’s principle) are resolved, and Newton’s laws of motion are now understood at the deeper quantum level. We found that gravity also involves the same ‘inertial’ electromagnetic force component that exists in inertial mass. -
Generalizations of the Kerr-Newman Solution
Generalizations of the Kerr-Newman solution Contents 1 Topics 663 1.1 ICRANetParticipants. 663 1.2 Ongoingcollaborations. 663 1.3 Students ............................... 663 2 Brief description 665 3 Introduction 667 4 Thegeneralstaticvacuumsolution 669 4.1 Line element and field equations . 669 4.2 Staticsolution ............................ 671 5 Stationary generalization 673 5.1 Ernst representation . 673 5.2 Representation as a nonlinear sigma model . 674 5.3 Representation as a generalized harmonic map . 676 5.4 Dimensional extension . 680 5.5 Thegeneralsolution ........................ 683 6 Static and slowly rotating stars in the weak-field approximation 687 6.1 Introduction ............................. 687 6.2 Slowly rotating stars in Newtonian gravity . 689 6.2.1 Coordinates ......................... 690 6.2.2 Spherical harmonics . 692 6.3 Physical properties of the model . 694 6.3.1 Mass and Central Density . 695 6.3.2 The Shape of the Star and Numerical Integration . 697 6.3.3 Ellipticity .......................... 699 6.3.4 Quadrupole Moment . 700 6.3.5 MomentofInertia . 700 6.4 Summary............................... 701 6.4.1 Thestaticcase........................ 702 6.4.2 The rotating case: l = 0Equations ............ 702 6.4.3 The rotating case: l = 2Equations ............ 703 6.5 Anexample:Whitedwarfs. 704 6.6 Conclusions ............................. 708 659 Contents 7 PropertiesoftheergoregionintheKerrspacetime 711 7.1 Introduction ............................. 711 7.2 Generalproperties ......................... 712 7.2.1 The black hole case (0 < a < M) ............. 713 7.2.2 The extreme black hole case (a = M) .......... 714 7.2.3 The naked singularity case (a > M) ........... 714 7.2.4 The equatorial plane . 714 7.2.5 Symmetries and Killing vectors . 715 7.2.6 The energetic inside the Kerr ergoregion . -
Weyl Metrics and Wormholes
Prepared for submission to JCAP Weyl metrics and wormholes Gary W. Gibbons,a;b Mikhail S. Volkovb;c aDAMTP, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK bLaboratoire de Math´ematiqueset Physique Th´eorique,LMPT CNRS { UMR 7350, Universit´ede Tours, Parc de Grandmont, 37200 Tours, France cDepartment of General Relativity and Gravitation, Institute of Physics, Kazan Federal University, Kremlevskaya street 18, 420008 Kazan, Russia E-mail: [email protected], [email protected] Abstract. We study solutions obtained via applying dualities and complexifications to the vacuum Weyl metrics generated by massive rods and by point masses. Rescal- ing them and extending to complex parameter values yields axially symmetric vacuum solutions containing singularities along circles that can be viewed as singular mat- ter sources. These solutions have wormhole topology with several asymptotic regions interconnected by throats and their sources can be viewed as thin rings of negative tension encircling the throats. For a particular value of the ring tension the geometry becomes exactly flat although the topology remains non-trivial, so that the rings liter- ally produce holes in flat space. To create a single ring wormhole of one metre radius one needs a negative energy equivalent to the mass of Jupiter. Further duality trans- formations dress the rings with the scalar field, either conventional or phantom. This gives rise to large classes of static, axially symmetric solutions, presumably including all previously known solutions for a gravity-coupled massless scalar field, as for exam- ple the spherically symmetric Bronnikov-Ellis wormholes with phantom scalar. The multi-wormholes contain infinite struts everywhere at the symmetry axes, apart from arXiv:1701.05533v3 [hep-th] 25 May 2017 solutions with locally flat geometry. -
5 Schwarzschild Metric 1 Rµν − Gµνr = Gµν = Κt Μν 2 Where 1 Gµν = Rµν − Gµνr 2 Einstein Thought It Would Never Be Solved
5 Schwarzschild metric 1 Rµν − gµνR = Gµν = κT µν 2 where 1 Gµν = Rµν − gµνR 2 Einstein thought it would never be solved. His equation is a second order tensor equation - so represents 16 separate equations! Though the symmetry properties means there are ’only’ 10 independent equations!! But the way to solve it is not in full generality, but to pick a real physical situation we want to represent. The simplest is static curved spacetime round a spherically symmetric mass while the rest of spacetime is empty. Schwarzchild did this by guessing the form the metric should have c2dτ 2 = A(r)c2dt2 − B(r)dr2 − r2dθ2 − r2 sin2 θdφ2 so the gµν are not functions of t - field is static. And spherically symmetric as surfaces with r, t constant have ds2 = r2(dθ2 + sin2θdφ2). Then we can form the Lagrangian and write down the Euler lagrange equations. Then by comparision with the geodesic equations we get the Christoffel symbols in terms of the unknown functions A and B and their radial derivatives dA/dr = A′ and dB/dr = B′. We can use these to form the Ricci tensor components as this is just defined from the christoffel sym- bols and their derivatives. And for EMPTY spacetime then Rµν = 0 NB just because the Ricci tensor is zero DOES NOT means that the Riemann curvature tensor components are zero (ie no curvature)!! Setting Rνµ = 0 means that the equations are slightly easier to solve when recast into the alternative form 1 Rαβ = κ(T αβ − gαβT ) 2 empty space means all the RHS is zero, so we do simply solve for Rαβ = 0. -
PPN Formalism
PPN formalism Hajime SOTANI 01/07/2009 21/06/2013 (minor changes) University of T¨ubingen PPN formalism Hajime Sotani Introduction Up to now, there exists no experiment purporting inconsistency of Einstein's theory. General relativity is definitely a beautiful theory of gravitation. However, we may have alternative approaches to explain all gravitational phenomena. We have also faced on some fundamental unknowns in the Universe, such as dark energy and dark matter, which might be solved by new theory of gravitation. The candidates as an alternative gravitational theory should satisfy at least three criteria for viability; (1) self-consistency, (2) completeness, and (3) agreement with past experiments. University of T¨ubingen 1 PPN formalism Hajime Sotani Metric Theory In only one significant way do metric theories of gravity differ from each other: ! their laws for the generation of the metric. - In GR, the metric is generated directly by the stress-energy of matter and of nongravitational fields. - In Dicke-Brans-Jordan theory, matter and nongravitational fields generate a scalar field '; then ' acts together with the matter and other fields to generate the metric, while \long-range field” ' CANNOT act back directly on matter. (1) Despite the possible existence of long-range gravitational fields in addition to the metric in various metric theories of gravity, the postulates of those theories demand that matter and non-gravitational fields be completely oblivious to them. (2) The only gravitational field that enters the equations of motion is the metric. Thus the metric and equations of motion for matter become the primary entities for calculating observable effects. -
The Singular Perturbation in the Analysis of Mode I Fracture
Available at Applications and Applied http://pvamu.edu/aam Mathematics: Appl. Appl. Math. ISSN: 1932-9466 An International Journal (AAM) Vol. 9, Issue 1 (June 2014), pp. 260-271 Evaluation of Schwarz Child’s Exterior and Interior Solutions in Bimetric Theory of Gravitation M. S. Borkar* Post Graduate Department of Mathematics Mahatma Jyotiba Phule Educational Campus R T M Nagpur University Nagpur – 440 033 (India) [email protected] P. V. Gayakwad Project Fellow under Major Research Project R T M Nagpur University Nagpur – 440 033 (India) [email protected] *Corresponding author Received: May 29, 2013; Accepted: February 6, 2014 Abstract In this note, we have investigated Schwarz child’s exterior and interior solutions in bimetric theory of gravitation by solving Rosen’s field equations and concluded that the physical singularities at r 0 and at r 2M do not appear in our solution. We have ruled out the discrepancies between physical singularity and mathematical singularity at r 2M and proved that the Schwarzschild exterior solution is always regular and does not break-down at r 2M. Further, we observe that the red shift of light in our model is much stronger than that of Schwarz child’s solution in general relativity and other geometrical and physical aspects are studied. Keywords: Relativity and gravitational theory; Space-time singularities MSC (2010) No.: 83C15, 83C75 260 AAM: Intern. J., Vol. 9, Issue 1 (June 2014) 261 1. Introduction Shortly after Einstein (1915) published his field equations of general theory of relativity, Schwarzschild (1916) solved the first and still the most important exact solution of the Einstein vacuum field equations which represents the field outside a spherical symmetric mass in otherwise empty space. -
The Confrontation Between General Relativity and Experiment
The Confrontation between General Relativity and Experiment Clifford M. Will Department of Physics University of Florida Gainesville FL 32611, U.S.A. email: [email protected]fl.edu http://www.phys.ufl.edu/~cmw/ Abstract The status of experimental tests of general relativity and of theoretical frameworks for analyzing them are reviewed and updated. Einstein’s equivalence principle (EEP) is well supported by experiments such as the E¨otv¨os experiment, tests of local Lorentz invariance and clock experiments. Ongoing tests of EEP and of the inverse square law are searching for new interactions arising from unification or quantum gravity. Tests of general relativity at the post-Newtonian level have reached high precision, including the light deflection, the Shapiro time delay, the perihelion advance of Mercury, the Nordtvedt effect in lunar motion, and frame-dragging. Gravitational wave damping has been detected in an amount that agrees with general relativity to better than half a percent using the Hulse–Taylor binary pulsar, and a growing family of other binary pulsar systems is yielding new tests, especially of strong-field effects. Current and future tests of relativity will center on strong gravity and gravitational waves. arXiv:1403.7377v1 [gr-qc] 28 Mar 2014 1 Contents 1 Introduction 3 2 Tests of the Foundations of Gravitation Theory 6 2.1 The Einstein equivalence principle . .. 6 2.1.1 Tests of the weak equivalence principle . .. 7 2.1.2 Tests of local Lorentz invariance . .. 9 2.1.3 Tests of local position invariance . 12 2.2 TheoreticalframeworksforanalyzingEEP. ....... 16 2.2.1 Schiff’sconjecture ................................ 16 2.2.2 The THǫµ formalism ............................. -
Doing Physics with Quaternions
Doing Physics with Quaternions Douglas B. Sweetser ©2005 doug <[email protected]> All righs reserved. 1 INDEX Introduction 2 What are Quaternions? 3 Unifying Two Views of Events 4 A Brief History of Quaternions Mathematics 6 Multiplying Quaternions the Easy Way 7 Scalars, Vectors, Tensors and All That 11 Inner and Outer Products of Quaternions 13 Quaternion Analysis 23 Topological Properties of Quaternions 28 Quaternion Algebra Tool Set Classical Mechanics 32 Newton’s Second Law 35 Oscillators and Waves 37 Four Tests of for a Conservative Force Special Relativity 40 Rotations and Dilations Create the Lorentz Group 43 An Alternative Algebra for Lorentz Boosts Electromagnetism 48 Classical Electrodynamics 51 Electromagnetic Field Gauges 53 The Maxwell Equations in the Light Gauge: QED? 56 The Lorentz Force 58 The Stress Tensor of the Electromagnetic Field Quantum Mechanics 62 A Complete Inner Product Space with Dirac’s Bracket Notation 67 Multiplying quaternions in Polar Coordinate Form 69 Commutators and the Uncertainty Principle 74 Unifying the Representations of Integral and Half−Integral Spin 79 Deriving A Quaternion Analog to the Schrödinger Equation 83 Introduction to Relativistic Quantum Mechanics 86 Time Reversal Transformations for Intervals Gravity 89 Unified Field Theory by Analogy 101 Einstein’s vision I: Classical unified field equations for gravity and electromagnetism using Riemannian quaternions 115 Einstein’s vision II: A unified force equation with constant velocity profile solutions 123 Strings and Quantum Gravity 127 Answering Prima Facie Questions in Quantum Gravity Using Quaternions 134 Length in Curved Spacetime 136 A New Idea for Metrics 138 The Gravitational Redshift 140 A Brief Summary of Important Laws in Physics Written as Quaternions 155 Conclusions 2 What Are Quaternions? Quaternions are numbers like the real numbers: they can be added, subtracted, multiplied, and divided.