Summary. There are reference frames for which both stars of binary radio-pulsar

Similar documents
Relativity, Gravitation, and Cosmology

Claudia de Rham July 30 th 2013

Einstein s Ether: E. Annual Motion of the Earth

On the Origin of the Lorentz Transformation

RELG - General Relativity

2.5.1 Static tides Tidal dissipation Dynamical tides Bibliographical notes Exercises 118

A873: Cosmology Course Notes. II. General Relativity

The Einstein field equation in terms of. the Schrödinger equation. The meditation of quantum information

A RULE FOR THE EQUILIBRIUM OF FORCES IN THE HERMITIAN THEORY OF RELATIVITY

2.1 Basics of the Relativistic Cosmology: Global Geometry and the Dynamics of the Universe Part I

The Mathematics of Minkowski Space-Time

Transformation for the energy flux of the electromagnetic wave

On the Gravitational Field of a Mass Point according to Einstein s Theory

9/12/2010. The Four Fundamental Forces of Nature. 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force

Understanding and Testing Relativity

Chapter 4. The Origin Of Modern Astronomy. Is okay to change your phone? From ios to Android From Android to ios

THE FOUNDATIONS OF PHYSICS (SECOND COMMUNICATION)

ASTR 200 : Lecture 30. More Gravity: Tides, GR, and Gravitational Waves

Binary Pulsars and Evidence for Gravitational Radiation

A Theory of Gravitation in Flat Space-Time. Walter Petry

From General Relativity to A Simple-Harmonically Oscillating Universe, and Vice-Versa: A Review

Relativity SPECIAL, GENERAL, AND COSMOLOGICAL SECOND EDITION. Wolfgang Rindler. Professor of Physics The University of Texas at Dallas

ASTR 200 : Lecture 31. More Gravity: Tides, GR, and Gravitational Waves

A5682: Introduction to Cosmology Course Notes. 2. General Relativity

Ordinals and Cardinals: Basic set-theoretic techniques in logic

Gravitational Waves Theory - Sources - Detection

Symmetries and Group Theory in Particle Physics

Gravitational Wave Astronomy Suggested readings: Camp and Cornish, Ann Rev Nucl Part Sci 2004 Schutz, gr-qc/ Kip Thorne WEB course

ASTR 1010 Spring 2016 Study Notes Dr. Magnani

Gravity and action at a distance

Mach, Thirring & Lense, Gödel - getting dizzy in space-time

Physics 171: General Relativity. An Introduction

Inertial Frame frame-dragging

Talking about general relativity Important concepts of Einstein s general theory of relativity. Øyvind Grøn Berlin July 21, 2016

E = mc 2. Inertial Reference Frames. Inertial Reference Frames. The Special Theory of Relativity. Slide 1 / 63. Slide 2 / 63.

Richard A. Mould. Basic Relativity. With 144 Figures. Springer-Verlag New York Berlin Heidelberg London Paris Tokyo Hong Kong Barcelona Budapest

arxiv: v1 [gr-qc] 11 Sep 2014

ON THE RELATIVITY PROBLEM

The Theory of Relativity

Einstein s Ether: D. Rotational Motion of the Earth

A. B. Lahanas University of Athens, Physics Department, Nuclear and Particle Physics Section, Athens , Greece

arxiv:physics/ v2 [physics.gen-ph] 2 Dec 2003

Adding Light to the Gravitational Waves on the Null Cone

Experimental Tests and Alternative Theories of Gravity

The Michelson Morley experiment explained by means of a Higgs Field that rotates around the Solar System

Chapter 18: Studying Space Astronomy: The Original Science

Postulate 2: Light propagates through empty space with a definite speed (c) independent of the speed of the source or of the observer.

Research and Reviews: Journal of Pure and Applied Physics. Further Remarks on the Oscillating Universe: an Explicative Approach

Relativity. Physics April 2002 Lecture 8. Einstein at 112 Mercer St. 11 Apr 02 Physics 102 Lecture 8 1

A FUNDAMENTAL PRINCIPLE OF RELATIVITY. By Douglas L. Weller ABSTRACT

The structure of spacetime. Eli Hawkins Walter D. van Suijlekom

Physics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits. Planetary Motion

Length Contraction on Rotating Disc: an Argument for the Lorentzian Approach to Relativity

D. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified

Gravity and motion A. LOINGER. Dipartimento di Fisica, Università di Milano. Via Celoria, Milano, Italy

Origins of the Universe

THE SPECIAL THEORY OF RELATIVITY

Possibility of Sound Propagation in Vacuums with the Speed of Light

Interference it s importance not only in surveying

An Introduction to Gravitational Waves

Chapter 2 Radiation of an Accelerated Charge

General Relativity. Einstein s Theory of Gravitation. March R. H. Gowdy (VCU) General Relativity 03/06 1 / 26

On The Michelson-Morley Experiment

Apeiron, Vol. 8, No. 2, April

Curved Spacetime... A brief introduction

Massachusetts Institute of Technology Physics Department

Gravity Tests with Radio Pulsars

16. Einstein and General Relativistic Spacetimes

a. exactly 360 b. less than 360 c. more than 360 On Figure 1, draw the Earth the next day and justify your answer above.

arxiv: v1 [gr-qc] 17 May 2008

Aristotle: If a man on top of a mast in a moving ship drops an object, it would fall toward the back of the ship.

Circular Motion and Gravity Lecture 5

Astronomy 182: Origin and Evolution of the Universe

GRAVITATIONAL COLLAPSE

Chapter 26. Relativity

How the theory of relativity came into being (a brief historical sketch)

A critical remark on Planck s model of black body

Special Relativity: The laws of physics must be the same in all inertial reference frames.

RESEARCH PROJECT: Investigation of Relativistic Longitudinal Gauge Fields. and their Interactions. Abstract

HOMEWORK 10. Applications: special relativity, Newtonian limit, gravitational waves, gravitational lensing, cosmology, 1 black holes

Modern Physics. Third Edition RAYMOND A. SERWAY CLEMENT J. MOSES CURT A. MOYER

- Potentials. - Liénard-Wiechart Potentials. - Larmor s Formula. - Dipole Approximation. - Beginning of Cyclotron & Synchrotron

Chapter 2 The Science of Life in the Universe

Universal gravitation

1. Einleitung. 1.1 Organisatorisches. Ziel der Vorlesung: Einführung in die Methoden der Ökonometrie. Voraussetzungen: Deskriptive Statistik

Galileo Galilei. And yet it moves or albeit it does move were the astute words from Galileo Galilei

214 FIRST PROPOSAL OF THE UNIVERSAL SPEED OF VOL See Deutsches Museum München, Archives, HS 5520

Title. Author(s)Greve, Ralf. Issue Date Doc URL. Type. Note. File Information. A material called spacetime

Einstein for Everyone Lecture 6: Introduction to General Relativity

THE PROBLEM WITH SO-CALLED FICTITIOUS FORCES. Abstract

JF Theoretical Physics PY1T10 Special Relativity

Cosmology - Contents

Do You Need to Understand General Relativity to Understand Gravitation?

Light and Relativity

SYNCHROTRON RADIATION

Gravity. Newtonian gravity: F = G M1 M2/r 2

Space, Time and Simultaneity

Charles Keeton. Principles of Astrophysics. Using Gravity and Stellar Physics. to Explore the Cosmos. ^ Springer

Einstein did not derive E=mc 2 from Special Relativity

arxiv: v2 [physics.gen-ph] 16 Mar 2015

Transcription:

On PSR1913+16 A. LOINGER Dipartimento di Fisica, Università di Milano Via Celoria, 16 20133 Milano, Italy Summary. There are reference frames for which both stars of binary radio-pulsar PSR1913+16 are at rest. As a consequence, PSR1913+16 does not emit gravity waves. (If the accelerated bodies should send out a gravitational radiation, they would represent a class of physically privileged systems. But this is forbidden by general relativity.) PACS. 04.20 General relativity; 04.30 Gravitational waves and radiation: theory; 97.60 Pulsars. 1. I have already discussed critically in previous papers [1], though en passant, the question of the gravitational waves which as it is commonly believed would be sent forth by the binary pulsar PSR1913+16. I wish now to point out a drastic argument against the possibility that the observational data can be interpreted as an indirect proof of a real emission of gravity waves from PSR1913+16. 2. I begin with some consideration on the role of the reference frames in general relativity. At p.268 of Weyl s book Raum-Zeit-Materie [2] we read: Zunächst stellen wir fest, daß der Begriff der Relativbewegung zweier Körper gegeneinander in der allgemeinen Relativitätstheorie ebensowenig einen Sinn hat wie der Begriff der absoluten Bewegung eines einzigen. [ ] Wie die beiden Körper sich auch bewegen mögen, immer kann ich durch Einführung eines geeigneten Koordinatensystems sie beide zusammen auf Ruhe transformieren. page 1 of 6

Let us examine, however, the case of the Earth and of the sky of the fixed stars. Weyl remarks (loc. cit. in [2], p.269): Wohl ist es unberechtig zu sagen, daß die Erde sich relativ zu den Fixsternen drehe; aber sie dreht sich in bezug auf denjenigen Körper, dem am Ort O der Erde selbst gebildet wird von den Lichtstrahlen, die in O von den Fixsternen her zusammenkommen. Das ist ein wesentlicher Unterschied, weil die Lichtstrahlen abhängig sind von dem metrischen Felde, das zwischen der Erde und den Fixsternen herrscht. Wir wollen auch diesen Sternenkompaß [star compass] genau beschreiben. Actually, Weyl demonstrates that we can assert that the Earth rotates with respect to the above star compass, provided that we suppose that the pseudo- Euclidean metric reign at infinity. More generally, Fock [3] tries to specify an entire class of physically privileged frames the harmonic systems, together with the requirement of pseudo-euclidean metric at infinity such that Galilei s motto E pur si muove! is literally true. As a matter of fact, however, no class of privileged frames can exist in general relativity, as it was repeatedly emphasized by Einstein. This means that Weyl s sentences, which we have written at the beginning of this section, have a strict sense, which does not allow any exception or attenuation. 3. Accordingly, let us choose a reference frame for which both stars of PSR1913+16 are at rest. Evidently, an observer Ω dwelling in such a system does not record any emission of gravity waves. 4. The overwhelming majority of the astrophysicists think that the temporal decrease of the revolution period of PSR1913+16 should be ascribed to an emission of gravity waves. Diligent people computed orbital data and masses by page 2 of 6

means of the semi-empirical PPN-method, then utilized some relativistic perturbative formulae. However, the reliability of the results is dubious because, owing to objective difficulties, the employed procedure is rather remote from a precise treatment of the real question, which would imply an accurate solution of the relativistic problem of two bodies of finite masses (the two stars of PSR1913+16). On the other hand, by virtue of the proposition of sect.3, the exact solution cannot yield any gravitational wave. Moreover, I observe that if the accelerated bodies should emit gravity waves, the accelerated frames would be physically privileged. But this is forbidden by general relativity. An objection: An observer like Ω, who dwells in a frame for which two revolving electric charges are at rest, sees the propagation of electromagnetic waves. Answer: Of course. But the existence of the e.m. waves is a consequence of the fact that Maxwell theory (which includes the material equations D = εe and H = (1/µ)B) is, first of all, the theory of the e.m. field (E, B) in a Minkowski space-time: the wave-like character of a given e.m. perturbation is a property valid for all the Galilean systems. The Riemannian formulation is only an extension. Historically, the belief in the physical existence of gravity waves had its origin in the linearized approximation of Einstein equations, which is a rough theory of weak gravitational fields in a given Minkowski space-time. By formal analogy, it seemed also that any accelerated mass point should generate a gravitational radiation. Then, these convictions were extended to perturbative approximations of higher orders. However, the exact non-linear theory does not admit any class of physically privileged frames for which, in particular, the wave-like character of a gravity field is an invariant property. page 3 of 6

5. Many physicists believe that the good accordance of the observational data concerning the PSR1913+16 with the numerical results yielded by PPN-method plus perturbative formulae is a confirmation of the theoretical validity of the procedure. But this is an epistemological mistake: an empirical agreement does not imply a conceptual adequacy. A convincing example: by means of a clever use of cycles and epicycles the followers of the Ptolemaic system calculated the planetary orbits with a very good accuracy (with the only exception of Mercury s orbit). 6. In the last twenty years, several detailed papers on perturbative treatments of Einstein equations in vacuo, R ik = 0, have been published. It seems that if the background space-time possesses symmetries, and the perturbations respect them, the perturbative approach is misleading. However, without the constraints represented by symmetries, the perturbation theory seems to be reliable. As it is a priori obvious from the theory of the characteristics by Levi- Civita, there exist solutions which are formally of an undulatory type, but any wave-like character is illusive [1]. PARTHIAN S ARROW Let us suppose that our observer Ω (see sect.3) is a believer in the existence of the gravity waves. He wishes to calculate the watts of gravitational radiation emitted by the rest of the universe, which revolves around him. Ω is a learned man, he reads at pp.359 and 360 of Fock s treatise [3] that, as a consequence of a well-known approximate formula the order of magnitude of the power of the gravity radiation sent out by Jupiter, e.g., in its motion around the Sun is given by B 2 /(2 10 39 c 4 ) g s 1, where B mωv 2 ; m 2 10 30 g is Jupiter s mass; page 4 of 6

ω 2 10 8 s 1 is Jupiter s angular velocity of revolution; v 2 /c 2 2 10 9, if v is Jupiter s mean linear velocity, ( v = ω r ). Substituting these numerical values, we obtain B 2 /(2 10 39 c 4 ) 5 10 12 g s 1 =ˆ 450 watt. Fock s remarks that the power of the solar electromagnetic radiation is 4 10 12 g s 1, i.e. about 10 24 times greater. The observer Ω imitates Fock s computation and substitutes in Fock s formula some reasonable estimates of the total mass of the world and of its mean radius; for ω, of course, no problem. Ω is a very rich man and possesses Michelson interferometers with kilometric arms and suspended mirrors. Do you think that he will be successful in detecting the gravitational radiation which in accordance with his belief should be emitted by the rest of the universe? (Our hero Ω had read in Pauli s book [4] that Einstein equations with cosmological term admit of a unique solution in vacuo, which is regular everywhere: g ik 0. Now as Pauli remarked this implies Mach s relativity of the inertial forces, in particular that a purely kinematical rotation does not exist.) page 5 of 6

REFERENCES [1] LOINGER A., http://xxx.lanl.gov/abs/astro-ph/9810137 (October 8th, 1998); http://xxx.lanl.gov/abs/astro-ph/9904207 (April 20th, 1999); http://xxx.lanl.gov/abs/astro-ph/9906058 (June 3rd, 1999); http://xxx.lanl.gov/abs/gr-qc/9909091 (September 30th, 1999); http://xxx.lanl.gov/abs/astro-ph/9912507 (December 23rd, 1999). [2] WEYL H., Raum, Zeit, Materie, Siebente Auflage (Springer-Verlag, Berlin, etc.) 1988. [3] FOCK V., The Theory of Space, Time and Gravitation, Second Revised Edition (Pergamon Press, Oxford, etc.) 1964, passim. [4] PAULI W., Teoria della Relatività (Boringhieri, Torino) 1958, sect.62. page 6 of 6