2008, VOLUME 3 PROGRESS IN PHYSICS
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Editorial Board Dmitri Rabounski (Editor-in-Chief) I. I. Haranas and M. Harney Detection of the Relativistic Corrections to the Gravita- [email protected] tional Potential using a Sagnac Interferometer ...... 3 Florentin Smarandache R. T. Cahill Resolving Spacecraft Earth-Flyby Anomalies with Measured Light Speed [email protected] Anisotropy ...... 9 Larissa Borissova [email protected] F.Smarandache and V.Christianto The Neutrosophic Logic View to Schrodinger’s¨ Cat Stephen J. Crothers Paradox, Revisited ...... 16 [email protected] P.Wagener A Classical Model of Gravitation ...... 21 Postal address A. A. Ungar On the Origin of the Dark Matter/Energy in the Universe and the Pioneer Chair of the Department Anomaly...... 24 of Mathematics and Science, P.-M.Robitaille A Critical Analysis of Universality and Kirchhoff’s Law: A Return to University of New Mexico, Stewart’s Law of Thermal Emission ...... 30 200 College Road, Gallup, NM 87301, USA P.-M.Robitaille Blackbody Radiation and the Carbon Particle ...... 36 A. Khazan The Roleˆ of the Element Rhodium in the Hyperbolic Law of the Periodic Table of Elements...... 56 Copyright c Progress in Physics, 2007 V.Chrisatianto and F.Smarandache What Gravity Is. Some Recent Considerations. . . .63 All rights reserved. The authors of the ar- U. K.W. Neumann Models for Quarks and Elementary Particles — Part III: What is ticles do hereby grant Progress in Physics non-exclusive, worldwide, royalty-free li- the Nature of the Gravitational Field? ...... 68 cense to publish and distribute the articles in U. K.W. Neumann Models for Quarks and Elementary Particles — Part IV: How Much accordance with the Budapest Open Initia- Do We Know of This Universe? ...... 71 tive: this means that electronic copying, dis- tribution and printing of both full-size ver- A. Sharma The Generalized Conversion Factor in Einstein’s Mass-Energy Equation. . . . .76 sion of the journal and the individual papers E. A. Isaeva On the Necessity of Aprioristic Thinking in Physics ...... 84 published therein for non-commercial, aca- 230-238 demic or individual use can be made by any S. M. Diab and S. A. Eid Potential Energy Surfaces of the Even-Even U Iso- user without permission or charge. The au- topes...... 87 thors of the articles published in Progress in Physics retain their rights to use this journal LETTERS as a whole or any part of it in any other pub- E. Goldfain A Brief Note on “Un-Particle” Physics ...... 93 lications and in any way they see fit. Any part of Progress in Physics howsoever used F.Smarandache International Injustice in Science ...... 94 in other publications must include an appro- priate citation of this journal.
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Detection of the Relativistic Corrections to the Gravitational Potential using a Sagnac Interferometer
Ioannis Iraklis Haranas and Michael Harneyy Department of Physics and Astronomy, York University, 314A Petrie Building, North York, Ontario, M3J-1P3, Canada E-mail: [email protected] y841 North 700 West, Pleasant Grove, Utah, 84062, USA E-mail: [email protected]
General Relativity predicts the existence of relativistic corrections to the static Newto- nian potential which can be calculated and verified experimentally. The idea leading to quantum corrections at large distances is that of the interactions of massless parti- cles which only involve their coupling energies at low energies. In this short paper we attempt to propose the Sagnac intrerferometric technique as a way of detecting the rela- tivistic correction suggested for the Newtonian potential, and thus obtaining an estimate for phase difference using a satellite orbiting at an altitude of 250 km above the surface of the Earth.
1 Introduction only involve their coupling energies at low energies, some- thing that it is known from the theory of General Relativity, The potential acting between to masses M and m that sepa- even though at short distances the theory of quantum grav- r G~ rated from their centers by a distance is: ity differs resulting to finite correction of the order, O c3r3 . GMm The existence of a universal long distance quantum correction V (r) = ; r (1) to the Newtonian potential should be relevant for a wide class of gravity theories. It is well known that the ultraviolet be- s where the Newton’s constant of gravitation. This potential haviour of Einstein’s pure gravity can be improved, if higher is of course only approximately valid [1]. For large masses derivative contributions to the action are added, which in four and or large velocities the theory of General Relativity pre- dimensions take the form: dicts that there exist relativistic corrections which can be cal- 2 culated and also verified experimentally [2]. In the micro- R R + R ; (2) scopic distance domain, we could expect that quantum me- where and are dimensionless coupling constants. What chanics, would predict a modification in the gravitational po- makes the difference is that the resulting classical and quan- tential in the same way that the radiative corrections of quan- tum corrections to gravity are expected to significantly alter tum electrodynamics leads to a similar modification of the the gravitational potential at short distances comparable to Coulombic interaction [3]. q ` = G~ = 35 Even though the theory of General Relativity constitutes that of Planck length P c3 10 m, but it should not a very well defined classical theory, it is still not possible to really affect its behaviour at long distances. At long distances combine it with quantum mechanics in order to create a sat- is the structure of the Einstein-Hilbert action that actually de- isfied theory of quantum gravity. One of the basic obstacles termines that. At this point we should mentioned that some that prevent this from happening is that General Relativity of the calculation to the corrections of the Newtonian gravi- does not actually fit the present paradigm for a fundamental tational potential result in the absence of a cosmological con- theory that of a renormalizable quantum field theory. Gravita- stant which usually complicates the perturbative treatment tional fields can be successfully quantized on smooth-enough to a significant degree due to the need to expand about a non- space-times [4], but the form of gravitational interactions is flat background. such that they induce unwanted divergences which can not In one loop amplitude computation one needs to calculate be absorbed by the renormalization of the parameters of the all first order corrections in G, which will include both the G2m2 G~ minimal General Relativity [5]. Somebody can introduce new relativistic O c2 and the quantum mechanical O c3 coupling constants and absorb the divergences then, one is corrections to the classical Newtonian potential [6]. unfortunately led to an infinite number of free parameters. In spite the difficulty above quantum gravity calculations can 2 The corrections to the potential predict long distance quantum corrections. The main idea leading to quantum corrections at large dis- Our goal is not to present the details of the one loop treat- tances is due to the interactions of massless particles which ment that leads to the corrections of the Newtonian gravita-
Ioannis I. Haranas and Michael Harney. The Relativistic Corrections to the Gravitational Potential using a Sagnac Interferometer 3 Volume 3 PROGRESS IN PHYSICS July, 2008
tional potential but rather sate the result and then use it in our Therefore equation (4) can be further written: calculations. Valid in order of G2 we have that the corrected GMm potential now becomes [6]: V (r; ) = r GMm G (M + m) 122 G ~ X1 n V (r) = 1 : (3) Re G (M + m) 2 3 2 1 Jn Pn(sin ) = (6a) r 2c r 15c r r 2rc2 n=2 Observing (3) we see that in the correction of the static GMm = [Vo + VJ + VJ + ::: VRelativistic] : Newtonian potential two differentq length scales are involved. r 2 3 G~ 35 First, the Planck length `P = 3 =10 m and second the c Since J2 is 400 larger that any other Jn coefficients, we 2GMn Schwarzschild radii of the heavy sources rsch = c2 . Fur- can disregard them and write the following expression for the thermore there are two independent dimensionless parame- Earth’s potential function including only the relativistic cor- ters which appear in the correction term, and involve the ratio rection and omitting the quantum corrections as being very of these two scales wit respect to the distance r. Presumably small we have: for meaningful results the two length scales are much smaller GM m GM mR2J 3 1 than r. V (r; ) = e + e e 2 sin2 + r r3 2 2 2 G Mem (Me + m) 3 Perturbations due to oblateness J2 + : c2r2 (7)
Because the Earth’s gravitational potential is not that of a Since we propose a satellite in orbit that carries the perfect spherical body, we can approximate its potential as Sagnac instrument it will of a help to express equation (7) for a spherical harmonic expansion of the following form: the potential in terms of the orbital elements. We know that " # sin = sin i sin(f +!) where i is the inclination of the orbit, GMm X1 R n f ! V (r; ) = 1 J e P (sin ) = is the true anomaly and is the argument of the perigee. Ig- r n r n noring long and short periodic terms (those containing ! and n=2 f GMm ) we write (7) in terms of the inclination as follows: = [Vo + VJ + VJ + ::: ] ; (4) r 2 3 GM m 3GM mR2J sin2i 1 V (r; ) = e + e e 2 + 3 where: r 2r 2 3 G2M m (M + m) r = geocentric distance, + e e c2r2 (8) = geocentric latitude. therefore the corresponding total acceleration that a mass m Re = means equatorial radius of the Earth, at r > Re has becomes: P = n Legendre polynomial of degree n and order zero, 1 @ GM m 3GM mR2J Jn = Jn jonal harmonics of order zero, that depend e e e 2 0 gtot = + on the latitude only, m @r r 2r3 2 2 GMm=r sin i 1 G Mem (M + m) and the first term now describes the potential of a + (9) homogeneous sphere and thus refers to Keplerian motion, the 2 3 r2c2 remaining part represents the Earth’s oblateness via the zonal harmonic coefficients and [7] so that: 2 2 9 GMe 9GMeReJ2 sin i 1 V0 = 1 g = + + > tot 2 4 > r 2r 2 3 2 > J R = G2M (M + m) V = 2 e 3 sin2 1 e e J2 + : (10) 2 r > (5) c2r3 > J R 3 > V = 3 e 5 sin3 3 sin ;> J3 2 r 4 Basic Sagnac interferometric theory similarly [8] ) 6 The Sagnac interferometer is based on the Sagnac effect, re- J2 = 1,082.610 : ported by G. Sagnac in 1913 [8]. Two beams are sent in op- 6 (6) J3 = 2.5310 posite directions around the interferometer until they meet
4 Ioannis I. Haranas and Michael Harney. The Relativistic Corrections to the Gravitational Potential using a Sagnac Interferometer July, 2008 PROGRESS IN PHYSICS Volume 3