Table of Contents
Journal of Gravity

Volume 2014, Article ID 415649, 5 pages

http://dx.doi.org/10.1155/2014/415649
Research Article

Gravitational Lagrangians, Mach’s Principle, and the Equivalence Principle in an Expanding Universe

KTH Mechanics, 100 44 Stockholm, Sweden

Received 13 June 2014; Accepted 6 August 2014; Published 17 August 2014

Academic Editor: Kazuharu Bamba

Copyright © 2014 Hanno Essén. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Abstract

Gravitational Lagrangians as derived by Fock for the Einstein-Infeld-Hoffmann approach, and by Kennedy assuming only a fourth rank tensor interaction, contain long range interactions. Here we investigate how these affect the local dynamics when integrated over an expanding universe out to the Hubble radius. Taking the cosmic expansion velocity into account in a heuristic manner it is found that these long range interactions imply Mach’s principle, provided the universe has the critical density, and that mass is renormalized. Suitable higher order additions to the Lagrangians make the formalism consistent with the equivalence principle.

1. Introduction and Outline

We start by presenting the gravitational Lagrangians that form the basis of the present formalism in Section 2. After that we point out how the local equations of motion for a particle will be affected by the long range interactions with the other particles in the universe. Consistency demands that the only quantities that enter are velocities and accelerations relative to the rest of the universe. This is Mach’s principle. After that, in Section 4, the long range effects are calculated by integration over the universe as a whole out to the Hubble radius, where the expansion velocity reaches the speed of light. In Section 5 Mach’s principle is found to be obeyed provided the density is the critical density (). The original masses of the theory then, however, turn out to be renormalized. This problem is dealt with in Section 6 where it is shown that the addition of certain higher order terms in the gravitational coupling constant restores the usual interpretation of mass and the gravitational constant. In this way the formalism as a whole is consistent with both Mach’s principle and the equivalence principle.

2. Gravitational Lagrangians

Fock [1] found the Lagrangian that yields the Einstein-Infeld-Hoffmann (EIH) equations of motion [24]. Modern derivations and discussions of this approach can be found in Landau and Lifshitz [5], Hirondel [6], Nordtvedt [7], Brumberg [8], and Louis-Martinez [9], among others. These are all based on general relativity and Hirondel’s is the shortest.

Here we will, however, focus on the profound work by Kennedy [10] on approximately relativistic interactions and their Lagrangians. Kennedy first derives the (special) relativistic Lagrangian for one particle interacting with another particle with constant given velocity. In a second step one then wishes to combine such Lagrangians into a single two-body Lagrangian, symmetric in the particle indices. To do this it is necessary to expand the Lagrangians in and keep terms to second order only. Even then the desired Lagrangian can, in general, be found only to first order in the coupling constant, the exception being electromagnetism for which the formalism produces the Darwin Lagrangian [11].

Assuming that the interaction is mediated by a fourth rank tensor (presumably the curvature tensor) Kennedy arrives at a two-body Lagrangian, which when generalized to bodies is where Here is the vector from particle to particle , and , and if is to give the Newtonian result we must have contains higher order terms in the gravitational coupling constant , Kennedy’s formalism does not give such terms but the general relativistic EIH-formalism gives To proceed we assume in what follows that does not depend on particle velocities, except via the factor as discussed in (15). It will then not affect the inertia properties of a particle, that is, the generalized momentum.

3. Mach’s Principle

Mach’s principle has been the subject of many publications over the years. Some more recent studies can be found in the volume edited by Barbour and Pfister [12]. Mashhoon et al. [13] and Iorio et al. [14] discuss the gravitomagnetic analogy. Other texts of interest are by Assis [15], Ciufolini and Wheeler [16], Peacock [17], and Cheng [18]. Frame dragging, rotational and translational, and its relation to Mach’s principle and general relativity have been discussed by Grøn et al. [1921], Harris [22], Holstein [23], Hughes [24], Lynden-Bell et al. [25], Martin et al. [26], Nightingale [27, 28], and Vetö [29, 30]. Recent observational support for rotational frame dragging, the Lense-Thirring effect, was found by Everitt et al. [31] using Gravity probe B, but the most accurate confirmation of this effect comes from the study of satellite motion (see [32]).

Here we will interpret Mach’s principle as saying that the equation of motion of a (slow) particle number is of the form where is the acceleration of the universe as a whole. That is, it is in the Newtonian form but only the acceleration relative to the universe as a whole, , is what matters in the equation of motion. The force is from the other particles of the system. We will now show that this result can be obtained from the Lagrangian of (1).

The equation of motion for particle is given by All terms involving accelerations will occur on the left-hand side here, so this is what we need to calculate. Calculation gives (assuming does not depend on velocities) for the generalized momentum . We now investigate under what circumstances one finds that , that is, Mach’s principle as stated in (7).

4. Summing over an Expanding Universe

Now assume that particle 1 is in a homogeneous isotropic expanding universe of (constant rest mass/energy) density and with Hubble parameter . The particles are then replaced by mass elements of position and velocity . Here is an overall velocity of the universe relative to the origin, and we assume that it is small compared to the speed of light (). We can then replace the sum in (9) with an integral and get Clearly one can not assume that for all , but because of the isotropy these velocities will not appear in the Lagrangian after the integration, and we will only be interested in the effective Lagrangian for slow particles in the expanding universe.

We now calculate the integral on the right-hand side. Introduce spherical coordinates and do the integration over the visible universe. At the radius of the visible universe the Hubble expansion leads to recession at the speed of light, (see Figure 1). The volume element in spherical coordinates is . Without loss of generality we assume that . Since , where , the scalar product term becomes The integrations over the sphere of radius will make the terms involving vanish for symmetry reasons, since these are multiplied by . Nothing depends on the angle in the integral so the term multiplying also vanishes. Two different integrals then remain to be calculated: first and then due to the scalar product term. Here the -integral is . In a previous study (see [33]) the mass/energy density in the integral was taken constant, , with the result that the integral evaluated to . It is, however, physically more natural to assume that it is the rest mass/energy density that is constant. The expansion with radial speed then means that one should use the special relativistic factor to get the contributing mass/energy from a shell of radius ; that is, we put . This gives The result of the radial integration is then a factor of 2 larger than what was found previously [33], when the mass/energy density was simply assumed constant. One notes that Gogberashvili [34] has obtained this factor of two in a different but seemingly more arbitrary way.

415649.fig.001
Figure 1: This figure illustrates the central point particle of mass in a homogeneous isotropic Hubble expanding universe with constant rest mass/energy density . The radial speed is and at the Hubble radius the speed is , the speed of light. In the Lagrangian we assume that the particle has velocity and that the expanding sphere of density has overall translational velocity .

5. Generalized Momentum Density Dependence

Using the above results (10) gives us Note that the quantity using , can be expressed as where is the critical density and where is standard notation in cosmology for the ratio of the density to the critical density; see Harvey [35]. In cosmology using general relativity and the assumption of an expanding homogeneous, isotropic universe one finds that the mass/energy density is the one that makes (three-dimensional) space flat [18, 36]. corresponds to the mass of the universe inside the Hubble radius being such that the Hubble radius is equal to the Schwarzschild radius .

The generalized momentum (16) of particle 1 now becomes Returning to my formulation of Mach’s principle in (7) it is seen to be realized with this if . For this value of the density ratio the generalized momentum is So, for the acceleration in Newton’s second law is relative to the acceleration of the universe as a whole. One also notes that the “bare” mass has been “renormalized” to .

6. The Principle of Equivalence

Let us now consider two slow particles near each other but far from all other local masses in the universe. As above we can sum over the expanding universe to get the influence of all the distant bodies on the two particles of interest. The result will be that their inertial masses are renormalized as found above. Assuming that the density is the critical density only the accelerations relative to the rest of the universe as a whole are relevant.

If, however, we now invoke the principle of equivalence, that is, the equality of the inertial and gravitational masses, we run into a problem (it can be proved that inertial and gravitational mass must be proportional within classical mechanics [37]). The effective Lagrangian for two slow particles near each other will be given by of (2) as modified by the cosmologically integrated of (3) and should thus be with . This will not give the correct local Newtonian equations of motion unless we reinterpret , but if we do that we have to redo the cosmological integrations and we are running in circles.

To get away from this problem it is clear that somehow also the gravitational masses must be renormalized by the cosmological integrations. It is easy to see that one way of doing this is to change of (4) to This clearly results in if the summations/integrations are done in the same way as in Section 4. If we really change we will also change and we have not achieved anything. Instead the changes can be incorporated as higher order terms in , with the same net result.

Such a correction is consistent with Kennedy [10] approach since it leads to correction terms of (5) proportional to and . These are seen to be When the entire universe is included such corrections are not small. With this choice of the entire formalism is consistent with Mach’s principle, the critical density, and the equivalence principle.

7. Conclusions

Summarizing we find that the Lagrangians and together, after integration over the expanding universe, give a generalized momentum for a particle that only depends on the velocity of the particle relative to the universe as a whole, when the density is the critical density. The inertial mass is, however, renormalized to be larger than the naked mass. The Newtonian gravitational forces arising from Lagrangian then no longer obey the principle of equivalence, unless one reinterprets , but this would require reinterpreting . Instead the introduction of of (24) solves the problem. Together with and integrations over the expanding universe results in the renormalized gravitational masses that agree with the renormalized inertial masses. The principle of equivalence is thus saved (to Newtonian order).

The fact that only is consistent with Mach’s principle in the above formalism is interesting but could, of course, be an accident due to canceling errors. Other authors have obtained similar results by completely different routes [26, 30, 34]. We note that we have not used general relativity at all in the above considerations. Kennedy [10] derives his gravitational Lagrangian only assuming special relativity and a fourth rank tensor interaction. His Lagrangian, however, is the same as the EIH-Lagrangian except for terms of higher order in the coupling constant . We note that general relativity gives a different such higher order term (see (6)) than the one obtained here using the equivalence principle. To add the corresponding physical effect to our theory we can simply add the term (6) with the masses interpreted as renormalized according to our prescription above. The full Lagrangian would have terms up to order .

Conflict of Interests

The author declares that there is no conflict of interests regarding the publication of this paper.

Acknowledgment

The author is grateful to Professor Vetö for insisting that is the value consistent with Mach’s principle.

References

  1. V. Fock, The Theory of Space Time and Gravitation, Pergamon Press, London, UK, 1959. View at MathSciNet
  2. A. Einstein, L. Infeld, and B. Hoffmann, “The gravitational equations and the problem of motion,” Annals of Mathematics, vol. 39, no. 1, pp. 65–100, 1938. View at Publisher · View at Google Scholar · View at MathSciNet
  3. A. Eddington and G. L. Clark, “Clark. The problem of n bodies in general relativity theory,” Proceedings of the Royal Society A, vol. 166, pp. 465–475, 1938. View at Google Scholar
  4. L. Infeld and J. Plebański, Motion and Relativity, Pergamon, Oxford, UK, 1960. View at MathSciNet
  5. L. D. Landau and E. M. Lifshitz, The Classical Theory of Fields, Vol. 2, Pergamon Press, Oxford, UK, 4th edition, 1975. View at MathSciNet
  6. D. Hirondel, “Special relativity in general relativity?” Journal of Mathematical Physics, vol. 15, no. 9, pp. 1471–1473, 1973. View at Google Scholar · View at Scopus
  7. K. Nordtvedt, “A post-newtonian gravitational lagrangian formalism for celestial body dynamics in metric graivity,” Astrophysical Journal, vol. 297, Article ID 390404, pp. 390–404, 1985. View at Google Scholar
  8. V. Brumberg, “On derivation of EIH (Einstein-Infeld-Hoffman) equations of motion from the linearized metric of general relativity theory,” Celestial Mechanics & Dynamical Astronomy, vol. 99, no. 3, pp. 245–252, 2007. View at Publisher · View at Google Scholar · View at MathSciNet · View at Scopus
  9. D. J. Louis-Martinez, “Relativistic action-at-a-distance description of gravitational interactions?” Physical Review D, vol. 86, no. 4, Article ID 045009, pp. 1–11, 2012. View at Publisher · View at Google Scholar · View at Scopus
  10. F. J. Kennedy, “Approximately relativistic interactions,” The American Journal of Physics, vol. 40, pp. 63–74, 1972. View at Google Scholar
  11. C. G. Darwin, “The dynamical motions of charged particles,” Philosophical Magazine Series 6, vol. 39, no. 233, pp. 537–551, 1920. View at Publisher · View at Google Scholar
  12. J. B. Barbour and H. Pfister, Eds., Mach's Principle: From Newton's Bucket to Quantum Gravity, Birkhäuser, Boston, Mass, USA, 1995.
  13. B. Mashhoon, F. Gronwald, and H. I. M. Lichtenegger, “Gravitomagnetism and the clock effect,” in Gyros, Clocks, Interferometers…: Testing Relativistic Graviy in Space, C. Lämmerzahl, C. W. F. Everitt, and F. W. Hehl, Eds., vol. 562 of Lecture Notes in Physics, pp. 83–108, Springer, Berlin, Germany, 2001. View at Publisher · View at Google Scholar
  14. L. Iorio, H. I. M. Lichtenegger, M. L. Ruggiero, and C. Corda, “Phenomenology of the Lense-Thirring effect in the solar system,” Astrophysics and Space Science, vol. 331, pp. 351–395, 2011. View at Google Scholar
  15. A. K. T. Assis, Relational Mechanics, Apeiron, Montreal, Canada, 1999.
  16. I. Ciufolini and J. A. Wheeler, Gravitation and Inertia, Princeton Series in Physics, Princeton University Press, Princeton, NJ, USA, 1995. View at MathSciNet
  17. J. A. Peacock, Cosmological Physics, Cambridge University Press, Cambridge, Mass, USA, 1999.
  18. T. Cheng, Relativity, Gravitation and Cosmology: A Basic Introduction, Oxford University Press, 2nd edition, 2010. View at MathSciNet
  19. Ø. G. Grøn and E. Eriksen, “Translational inertial dragging,” General Relativity and Gravitation, vol. 21, no. 2, pp. 105–124, 1989. View at Publisher · View at Google Scholar · View at MathSciNet
  20. H. I. Hartman and C. Nissim-Sabat, “Reply to “the principle of relativity and inertial dragging” by Ø. G. Grøn,” American Journal of Physics, vol. 77, no. 4, pp. 381–382, 2009. View at Google Scholar
  21. Ø. G. Grøn, “The principle of relativity and inertial dragging,” American Journal of Physics, vol. 77, no. 4, pp. 373–380, 2009. View at Google Scholar
  22. E. G. Harris, “Analogy between general relativity and electromagnetism for slowly moving particles in weak gravitational fields,” American Journal of Physics, vol. 59, no. 5, pp. 421–425, 1991. View at Publisher · View at Google Scholar · View at MathSciNet
  23. B. R. Holstein, “Gyroscope precession and general relativity,” The American Journal of Physics, vol. 69, no. 12, pp. 1248–1256, 2001. View at Publisher · View at Google Scholar · View at Scopus
  24. R. J. Hughes, “On Feynman's proof of the Maxwell equations,” The American Journal of Physics, vol. 60, no. 4, pp. 301–306, 1992. View at Publisher · View at Google Scholar · View at MathSciNet
  25. D. Lynden-Bell, J. Bicák, and J. Katz, “On accelerated inertial frames in gravity and electromagnetism,” Annals of Physics, vol. 271, no. 1, pp. 1–22, 1999. View at Publisher · View at Google Scholar · View at MathSciNet · View at Scopus
  26. J. Martin, A. F. Ranada, and A. Tiemblo, “On Mach's principle: inertia as gravitation,” http://arxiv.org/abs/gr-qc/0703141v1.
  27. J. David Nightingale, “Specific physical consequences of Mach's principle,” American Journal of Physics, vol. 45, pp. 376–379, 1977. View at Google Scholar
  28. J. David Nightingale and J. R. Ray, “Comment on ‘Specific physical consequences of Mach’s principle’,” American Journal of Physics, vol. 46, p. 586, 1978. View at Google Scholar
  29. B. Vetö, “Gravity probe B experiment and gravitomagnetism,” European Journal of Physics, vol. 31, no. 5, pp. 1123–1130, 2010. View at Publisher · View at Google Scholar · View at Scopus
  30. B. Vetö, “Gravitomagnetic field of the universe and Coriolis force on the rotating Earth,” European Journal of Physics, vol. 32, no. 5, pp. 1323–1329, 2011. View at Publisher · View at Google Scholar · View at Scopus
  31. C. W. F. Everitt, D. B. Debra, B. W. Parkinson et al., “Gravity probe B: final results of a space experiment to test general relativity,” Physical Review Letters, vol. 106, Article ID 221101, 2011. View at Publisher · View at Google Scholar · View at Scopus
  32. I. Clutolini and E. C. Pavils, “A confirmation of the general relativistic prediction of the Lens-Thirring effect,” Nature, vol. 431, pp. 958–960, 2004. View at Publisher · View at Google Scholar · View at Scopus
  33. H. Essen, “Mechanics, cosmology and Mach's principle,” European Journal of Physics, vol. 34, pp. 139–145, 2013. View at Google Scholar
  34. M. Gogberashvili, “On the dynamics of the ensemble of particles in the thermodynamic model of gravity,” http://arxiv.org/abs/1309.0376v1.
  35. A. Harvey, “Dark energy and the cosmological constant: a brief introduction,” European Journal of Physics, vol. 30, no. 4, pp. 877–889, 2009. View at Publisher · View at Google Scholar · View at Scopus
  36. T. F. Jordan, “Cosmology calculations almost without general relativity,” American Journal of Physics, vol. 73, pp. 653–662, 2005. View at Google Scholar
  37. A. E. Chubykalo and S. J. Vlaev, “Theorem on the proportionality of inertial and gravitational masses in classical mechanics,” European Journal of Physics, vol. 19, no. 1, pp. 1–6, 1998. View at Publisher · View at Google Scholar · View at Zentralblatt MATH · View at Scopus