The Inconsistent Equivalence Principle
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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. -
Quantum Mechanical Laws - Bogdan Mielnik and Oscar Rosas-Ruiz
FUNDAMENTALS OF PHYSICS – Vol. I - Quantum Mechanical Laws - Bogdan Mielnik and Oscar Rosas-Ruiz QUANTUM MECHANICAL LAWS Bogdan Mielnik and Oscar Rosas-Ortiz Departamento de Física, Centro de Investigación y de Estudios Avanzados, México Keywords: Indeterminism, Quantum Observables, Probabilistic Interpretation, Schrödinger’s cat, Quantum Control, Entangled States, Einstein-Podolski-Rosen Paradox, Canonical Quantization, Bell Inequalities, Path integral, Quantum Cryptography, Quantum Teleportation, Quantum Computing. Contents: 1. Introduction 2. Black body radiation: the lateral problem becomes fundamental. 3. The discovery of photons 4. Compton’s effect: collisions confirm the existence of photons 5. Atoms: the contradictions of the planetary model 6. The mystery of the allowed energy levels 7. Luis de Broglie: particles or waves? 8. Schrödinger’s wave mechanics: wave vibrations explain the energy levels 9. The statistical interpretation 10. The Schrödinger’s picture of quantum theory 11. The uncertainty principle: instrumental and mathematical aspects. 12. Typical states and spectra 13. Unitary evolution 14. Canonical quantization: scientific or magic algorithm? 15. The mixed states 16. Quantum control: how to manipulate the particle? 17. Measurement theory and its conceptual consequences 18. Interpretational polemics and paradoxes 19. Entangled states 20. Dirac’s theory of the electron as the square root of the Klein-Gordon law 21. Feynman: the interference of virtual histories 22. Locality problems 23. The idea UNESCOof quantum computing and future – perspectives EOLSS 24. Open questions Glossary Bibliography Biographical SketchesSAMPLE CHAPTERS Summary The present day quantum laws unify simple empirical facts and fundamental principles describing the behavior of micro-systems. A parallel but different component is the symbolic language adequate to express the ‘logic’ of quantum phenomena. -
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 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. -
1. Introduction
Beichler (1) Preliminary paper for Vigier IX Conference June 2014 MODERN FYSICS PHALLACIES: THE BEST WAY NOT TO UNIFY PHYSICS JAMES E. BEICHLER Research Institute for Paraphysics, Retired P.O. Box 624, Belpre, Ohio 45714 USA [email protected] Too many physicists believe the ‘phallacy’ that the quantum is more fundamental than relativity without any valid supporting evidence, so the earliest attempts to unify physics based on the continuity of relativity have been all but abandoned. This belief is probably due to the wealth of pro-quantum propaganda and general ‘phallacies in fysics’ that were spread during the second quarter of the twentieth century, although serious ‘phallacies’ exist throughout physics on both sides of the debate. Yet both approaches are basically flawed because both relativity and the quantum theory are incomplete and grossly misunderstood as they now stand. Had either side of the quantum versus relativity controversy sought common ground between the two worldviews, total unification would have been accomplished long ago. The point is, literally, that the discrete quantum, continuous relativity, basic physical geometry, theoretical mathematics and classical physics all share one common characteristic that has never been fully explored or explained – a paradoxical duality between a dimensionless point (discrete) and an extended length (continuity) in any dimension – and if the problem of unification is approached from an understanding of how this paradox relates to each paradigm, all of physics and indeed all of science could be unified under a single new theoretical paradigm. Keywords: unification, single field theory, unified field theory, quantized space-time, five-dimensional space-time, quantum, relativity, hidden variables, Einstein, Kaluza, Klein, Clifford 1. -
Albert Einstein - Wikipedia, the Free Encyclopedia Page 1 of 27
Albert Einstein - Wikipedia, the free encyclopedia Page 1 of 27 Albert Einstein From Wikipedia, the free encyclopedia Albert Einstein ( /ælbərt a nsta n/; Albert Einstein German: [albt a nʃta n] ( listen); 14 March 1879 – 18 April 1955) was a German-born theoretical physicist who developed the theory of general relativity, effecting a revolution in physics. For this achievement, Einstein is often regarded as the father of modern physics.[2] He received the 1921 Nobel Prize in Physics "for his services to theoretical physics, and especially for his discovery of the law of the photoelectric effect". [3] The latter was pivotal in establishing quantum theory within physics. Near the beginning of his career, Einstein thought that Newtonian mechanics was no longer enough to reconcile the laws of classical mechanics with the laws of the electromagnetic field. This led to the development of his special theory of relativity. He Albert Einstein in 1921 realized, however, that the principle of relativity could also be extended to gravitational fields, and with his Born 14 March 1879 subsequent theory of gravitation in 1916, he published Ulm, Kingdom of Württemberg, a paper on the general theory of relativity. He German Empire continued to deal with problems of statistical Died mechanics and quantum theory, which led to his 18 April 1955 (aged 76) explanations of particle theory and the motion of Princeton, New Jersey, United States molecules. He also investigated the thermal properties Residence Germany, Italy, Switzerland, United of light which laid the foundation of the photon theory States of light. In 1917, Einstein applied the general theory of relativity to model the structure of the universe as a Ethnicity Jewish [4] whole. -
Introducing Quantum and Statistical Physics in the Footsteps of Einstein: a Proposal †
universe Article Introducing Quantum and Statistical Physics in the Footsteps of Einstein: A Proposal † Marco Di Mauro 1,*,‡ , Salvatore Esposito 2,‡ and Adele Naddeo 2,‡ 1 Dipartimento di Matematica, Universitá di Salerno, Via Giovanni Paolo II, 84084 Fisciano, Italy 2 INFN Sezione di Napoli, Via Cinthia, 80126 Naples, Italy; [email protected] (S.E.); [email protected] (A.N.) * Correspondence: [email protected] † This paper is an extended version from the proceeding paper: Di Mauro, M.; Esposito, S.; Naddeo, A. Introducing Quantum and Statistical Physics in the Footsteps of Einstein: A Proposal. In Proceedings of the 1st Electronic Conference on Universe, online, 22–28 February 2021. ‡ These authors contributed equally to this work. Abstract: Introducing some fundamental concepts of quantum physics to high school students, and to their teachers, is a timely challenge. In this paper we describe ongoing research, in which a teaching–learning sequence for teaching quantum physics, whose inspiration comes from some of the fundamental papers about the quantum theory of radiation by Albert Einstein, is being developed. The reason for this choice goes back essentially to the fact that the roots of many subtle physical concepts, namely quanta, wave–particle duality and probability, were introduced for the first time in one of these papers, hence their study may represent a useful intermediate step towards tackling the final incarnation of these concepts in the full theory of quantum mechanics. An extended discussion of some elementary tools of statistical physics, mainly Boltzmann’s formula for entropy and statistical distributions, which are necessary but may be unfamiliar to the students, is included. -
General Relativity
Institut für Theoretische Physik der Universität Zürich in conjunction with ETH Zürich General Relativity Autumn semester 2016 Prof. Philippe Jetzer Original version by Arnaud Borde Revision: Antoine Klein, Raymond Angélil, Cédric Huwyler Last revision of this version: September 20, 2016 Sources of inspiration for this course include • S. Carroll, Spacetime and Geometry, Pearson, 2003 • S. Weinberg, Gravitation and Cosmology, Wiley, 1972 • N. Straumann, General Relativity with applications to Astrophysics, Springer Verlag, 2004 • C. Misner, K. Thorne and J. Wheeler, Gravitation, Freeman, 1973 • R. Wald, General Relativity, Chicago University Press, 1984 • T. Fliessbach, Allgemeine Relativitätstheorie, Spektrum Verlag, 1995 • B. Schutz, A first course in General Relativity, Cambridge, 1985 • R. Sachs and H. Wu, General Relativity for mathematicians, Springer Verlag, 1977 • J. Hartle, Gravity, An introduction to Einstein’s General Relativity, Addison Wesley, 2002 • H. Stephani, General Relativity, Cambridge University Press, 1990, and • M. Maggiore, Gravitational Waves: Volume 1: Theory and Experiments, Oxford University Press, 2007. • A. Zee, Einstein Gravity in a Nutshell, Princeton University Press, 2013 As well as the lecture notes of • Sean Carroll (http://arxiv.org/abs/gr-qc/9712019), • Matthias Blau (http://www.blau.itp.unibe.ch/lecturesGR.pdf), and • Gian Michele Graf (http://www.itp.phys.ethz.ch/research/mathphys/graf/gr.pdf). 2 CONTENTS Contents I Introduction 5 1 Newton’s theory of gravitation 5 2 Goals of general relativity 6 II Special Relativity 8 3 Lorentz transformations 8 3.1 Galilean invariance . .8 3.2 Lorentz transformations . .9 3.3 Proper time . 11 4 Relativistic mechanics 12 4.1 Equations of motion . 12 4.2 Energy and momentum . -
Einstein's Pathway to the Equivalence Principle 1905-1907
Einstein's Pathway to the Equivalence Principle 1905-1907 Galina Weinstein Between 1905 and 1907, Einstein first tried to extend the special theory of relativity in such a way so as to explain gravitational phenomena. This was the most natural and simplest path to be taken. These investigations did not fit in with Galileo's law of free fall. This law, which may also be formulated as the law of the equality of inertial and gravitational mass, was illuminating Einstein, and he suspected that in it must lie the key to a deeper understanding of inertia and gravitation. He imagined an observer freely falling from the roof of a house; for the observer there is during the fall – at least in his immediate vicinity – no gravitational field. If the observer lets go of any bodies, they remain relative to him, in a state of rest or uniform motion, regardless of their particular chemical and physical nature. The observer is therefore justified in interpreting his state as being "at rest". Newton realized that Galileo's law of free fall is connected with the equality of the inertial and gravitational mass; however, this connection was accidental. Einstein said that Galileo's law of free fall can be viewed as Newton's equality between inertial and gravitational mass, but for him the connection was not accidental. Einstein's 1907 breakthrough was to consider Galileo's law of free fall as a powerful argument in favor of expanding the principle of relativity to systems moving non- uniformly relative to each other. Einstein realized that he might be able to generalize the principle of relativity when guided by Galileo's law of free fall; for if one body fell differently from all others in the gravitational field, then with the help of this body an observer in free fall (with all other bodies) could find out that he was falling in a gravitational field. -
Arxiv:2105.04329V2 [Gr-Qc] 12 Jul 2021
Inductive rectilinear frame dragging and local coupling to the gravitational field of the universe L.L. Williams∗ Konfluence Research Institute, Manitou Springs, Colorado N. Inany School of Natural Sciences University of California, Merced Merced, California (Dated: 11 July 2021) There is a drag force on objects moving in the background cosmological metric, known from galaxy cluster dynamics. The force is quite small over laboratory timescales, yet it applies in principle to all moving bodies in the universe. It means it is possible for matter to exchange momentum and energy with the gravitational field of the universe, and that the cosmological metric can be determined in principle from local measurements on moving bodies. The drag force can be understood as inductive rectilinear frame dragging. This dragging force exists in the rest frame of a moving object, and arises from the off-diagonal components induced in the boosted-frame metric. Unlike the Kerr metric or other typical frame-dragging geometries, cosmological inductive dragging occurs at uniform velocity, along the direction of motion, and dissipates energy. Proposed gravito-magnetic invariants formed from contractions of the Riemann tensor do not appear to capture inductive dragging effects, and this might be the first identification of inductive rectilinear dragging. 1. INTRODUCTION The freedom of a general coordinate transformation allows a local Lorentz frame to be defined sufficiently locally around a point in curved spacetime. In this frame, also called an inertial frame, first derivatives of the metric vanish, and therefore the connections vanish, and gravitational forces on moving bodies vanish. Yet the coordinate freedom cannot remove all second derivatives of the metric, and so components of the Riemann tensor can be non-zero locally where the connections are zero. -
New Light on the Einstein-Hilbert Priority Question
J. Astrophys. Astr. (1999) 20, 91–101 New Light on the Einstein-Hilbert Priority Question John Stachel, Department of Physics and Center for Einstein Studies, Boston University, 590 Commonwealth Avenue, Boston, Massachusetts 02215 USA. email:[email protected] 1. Introduction This talk is based on the joint work with Leo Corry and Jürgen Renn.1 The develop- ment of general relativity may be compared to a traditional three-act play: I (1907-1908): The formulation of the equivalence principle; II (1912-1913): The choice of the metric tensor field as the appropriate relativistic generalization of the scalar Newtonian gravitational potential; III (1913-1915): The search for the correct field equations for the metric tensor field. The first two acts were essentially monologues starring Albert Einstein. The third act was a dialogue between Einstein and David Hilbert, the leading Göttingen mathe- matician. I have told the story of all three acts from Einstein's point of view elsewhere in some detail,2 so I shall be brief in reviewing the first two acts. But I must say more about the third act, since this is where Hilbert entered the story and the priority question between them arose. Acts I and II. In 1907, Einstein prepared a review article on the principle of relativity and its consequences for the various branches of physics.3 In the course of the review, he discussed the question of a relativistic theory of gravitation.4 It was clear from the outset that the Newtonian theory would have to be modified, since it is based on the concept of a force between pairs of particles that depends on the distance between them at some moment of time.