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Diagram regarding the confirmation of gravitomagnetism by Gravity Probe B

Gravitoelectromagnetism, abbreviated GEM, refers to a set of formal analogies between the equations for electromagnetism and relativistic gravitation; specifically: between Maxwell's field equations and an approximation, valid under certain conditions, to the Einstein field equations for general relativity. Gravitomagnetism is a widely used term referring specifically to the kinetic effects of gravity, in analogy to the magnetic effects of moving electric charge. The most common version of GEM is valid only far from isolated sources, and for slowly moving test particles.

The analogy and equations differing only by some small factors were first published in 1893, before general relativity, by Oliver Heaviside as a separate theory expanding Newton's law.[1][better source needed]



This approximate reformulation of gravitation as described by general relativity in the weak field limit makes an apparent field appear in a frame of reference different from that of a freely moving inertial body. This apparent field may be described by two components that act respectively like the electric and magnetic fields of electromagnetism, and by analogy these are called the gravitoelectric and gravitomagnetic fields, since these arise in the same way around a mass that a moving electric charge is the source of electric and magnetic fields. The main consequence of the gravitomagnetic field, or velocity-dependent acceleration, is that a moving object near a rotating massive object will experience acceleration not predicted by a purely Newtonian (gravitoelectric) gravity field. More subtle predictions, such as induced rotation of a falling object and precession of a spinning object are among the last basic predictions of general relativity to be directly tested.

Indirect validations of gravitomagnetic effects have been derived from analyses of relativistic jets. Roger Penrose had proposed a frame dragging mechanism for extracting energy and momentum from rotating black holes.[2] Reva Kay Williams, University of Florida, developed a rigorous proof that validated Penrose's mechanism.[3] Her model showed how the Lense–Thirring effect could account for the observed high energies and luminosities of quasars and active galactic nuclei; the collimated jets about their polar axis; and the asymmetrical jets (relative to the orbital plane).[4] All of those observed properties could be explained in terms of gravitomagnetic effects.[5] Williams' application of Penrose's mechanism can be applied to black holes of any size.[6] Relativistic jets can serve as the largest and brightest form of validations for gravitomagnetism.

A group at Stanford University is currently[when?] analyzing data from the first direct test of GEM, the Gravity Probe B satellite experiment, to see whether they are consistent with gravitomagnetism.[citation needed] The Apache Point Observatory Lunar Laser-ranging Operation also plans to observe gravitomagnetism effects.[citation needed]

Physical analogues of fields[7]
Gravitomagnetism — gravitomagnetic field H due to (total) angular momentum J
... or, equivalently, current I, same field profile, and field generation due to rotation. 
Fluid mechanics — rotational fluid drag of a solid sphere immersed in fluid, analogous directions and senses of rotation as magnetism, analogous interaction to frame dragging for the gravitomagnetic interaction. 


According to general relativity, the gravitational field produced by a rotating object (or any rotating mass–energy) can, in a particular limiting case, be described by equations that have the same form as in classical electromagnetism. Starting from the basic equation of general relativity, the Einstein field equation, and assuming a weak gravitational field or reasonably flat spacetime, the gravitational analogs to Maxwell's equations for electromagnetism, called the "GEM equations", can be derived. GEM equations compared to Maxwell's equations in SI units are:[8][9]

GEM equations Maxwell's equations


Lorentz forceEdit

For a test particle whose mass m is "small", in a stationary system, the net (Lorentz) force acting on it due to a GEM field is described by the following GEM analog to the Lorentz force equation:

GEM equation EM equation


Poynting vectorEdit

The GEM Poynting vector compared to the electromagnetic Poynting vector is given by[10]

GEM equation EM equation

Scaling of fieldsEdit

The literature does not adopt a consistent scaling for the gravitoelectric and gravitomagnetic fields, making comparison tricky. For example, to obtain agreement with Mashhoon's writings, all instances of Bg in the GEM equations must be multiplied by −½ c and Eg by −1. These factors variously modify the analogues of the equations for the Lorentz force. No scaling choice allows all the GEM and EM equations to be perfectly analogous. The discrepancy in the factors arises because the source of the gravitational field is the second order stress–energy tensor, as opposed to the source of the electromagnetic field being the first order four-current tensor. This difference becomes clearer when one compares non-invariance of relativistic mass to electric charge invariance. This can be traced back to the spin-2 character of the gravitational field, in contrast to the electromagnetism being a spin-1 field.[11] (See relativistic wave equations for more on "spin-1" and "spin-2" fields).

In Planck unitsEdit

From comparison of GEM equations and Maxwell's equations it is obvious that −1/(4πG) is the gravitational analog of vacuum permittivity ε0. Adopting Planck units normalizes G, c and 1/(4πε0) to 1, thereby eliminating these constants from both sets of equations. The two sets of equations then become identical but for the minus sign preceding 4π in the GEM equations and a factor of four in Ampere's law. These minus signs stem from an essential difference between gravity and electromagnetism: electrostatic charges of the same sign repel each other, whereas masses attract each other. Hence the GEM equations are nearly Maxwell's equations, but with mass (or mass density) substituting for charge (or charge density), and −1/(4πG) replacing the vacuum permittivity ε0. The factor 4π appears in both the GEM and Maxwell equations, because Planck units normalize G and 1/(4πε0) to 1, and not 4πG and ε0.

Higher-order effectsEdit

Some higher-order gravitomagnetic effects can reproduce effects reminiscent of the interactions of more conventional polarized charges. For instance, if two wheels are spun on a common axis, the mutual gravitational attraction between the two wheels will be greater if they spin in opposite directions than in the same direction. This can be expressed as an attractive or repulsive gravitomagnetic component.

Gravitomagnetic arguments also predict that a flexible or fluid toroidal mass undergoing minor axis rotational acceleration (accelerating "smoke ring" rotation) will tend to pull matter through the throat (a case of rotational frame dragging, acting through the throat). In theory, this configuration might be used for accelerating objects (through the throat) without such objects experiencing any g-forces.[12]

Consider a toroidal mass with two degrees of rotation (both major axis and minor-axis spin, both turning inside out and revolving). This represents a "special case" in which gravitomagnetic effects generate a chiral corkscrew-like gravitational field around the object. The reaction forces to dragging at the inner and outer equators would normally be expected to be equal and opposite in magnitude and direction respectively in the simpler case involving only minor-axis spin. When both rotations are applied simultaneously, these two sets of reaction forces can be said to occur at different depths in a radial Coriolis field that extends across the rotating torus, making it more difficult to establish that cancellation is complete.[citation needed]

Modelling this complex behaviour as a curved spacetime problem has yet to be done and is believed to be very difficult.[citation needed]

Gravitomagnetic fields of astronomical objectsEdit

The formula for the gravitomagnetic field Bg near a rotating body can be derived from the GEM equations. It is exactly half of the Lense–Thirring precession rate, and is given by:[citation needed]


where L is the angular momentum of the body. At the equatorial plane, r and L are perpendicular, so their dot product vanishes, and this formula reduces to:


The magnitude of angular momentum of a homogeneous ball-shaped body is:




Therefore, the magnitude of Earth's gravitomagnetic field at its equator is:


where   is Earth's gravity. The field direction coincides with the angular moment direction, i.e. north.

From this calculation it follows that Earth's equatorial gravitomagnetic field is about 1.012×10−14 Hz,[13] or 3.1×10−7 in units of standard gravity (9.81 m/s2) divided by the speed of light. Such a field is extremely weak and requires extremely sensitive measurements to be detected. One experiment to measure such field was the Gravity Probe B mission.


If the preceding formula is used with the pulsar PSR J1748-2446ad (which rotates 716 times per second), assuming a radius of 16 km, and two solar masses, then


equals about 166 Hz. This would be easy to notice. However, the pulsar is spinning at a quarter of the speed of light at the equator, and its radius is only three times more than its Schwarzschild radius. When such fast motion and such strong gravitational fields exist in a system, the simplified approach of separating gravitomagnetic and gravitoelectric forces can be applied only as a very rough approximation.

Lack of invarianceEdit

While Maxwell's equations are invariant under Lorentz transformations, the GEM equations were not. The fact that ρg and jg do not form a four-vector (instead they are merely a part of the stress–energy tensor) is the basis of this problem.[citation needed]

Although GEM may hold approximately in two different reference frames connected by a Lorentz boost, there is no way to calculate the GEM variables of one such frame from the GEM variables of the other, unlike the situation with the variables of electromagnetism. Indeed, their predictions (about what motion is free fall) will probably conflict with each other.

Note that the GEM equations are invariant under translations and spatial rotations, just not under boosts and more general curvilinear transformations. Maxwell's equations can be formulated in a way that makes them invariant under all of these coordinate transformations.

See alsoEdit


  1. ^ O. Heaviside (1893). "A gravitational and electromagnetic analogy". The Electrician. 31: 81–82. 
  2. ^ R. Penrose (1969). "Gravitational collapse: The role of general relativity". Rivista de Nuovo Cimento. Numero Speciale 1: 252–276. Bibcode:1969NCimR...1..252P. 
  3. ^ R.K. Williams (1995). "Extracting x rays, Ύ rays, and relativistic ee+ pairs from supermassive Kerr black holes using the Penrose mechanism". Physical Review. 51 (10): 5387–5427. Bibcode:1995PhRvD..51.5387W. PMID 10018300. doi:10.1103/PhysRevD.51.5387. 
  4. ^ R.K. Williams (2004). "Collimated escaping vortical polar ee+ jets intrinsically produced by rotating black holes and Penrose processes". The Astrophysical Journal. 611 (2): 952–963. Bibcode:2004ApJ...611..952W. arXiv:astro-ph/0404135 . doi:10.1086/422304. 
  5. ^ R.K. Williams (2005). "Gravitomagnetic field and Penrose scattering processes". Annals of the New York Academy of Sciences. 1045. pp. 232–245. 
  6. ^ R.K. Williams (2001). "Collimated energy–momentum extraction from rotating black holes in quasars and microquasars using the Penrose mechanism". AIP Conference Proceedings. 586. pp. 448–453. Bibcode:2001AIPC..586..448W. arXiv:astro-ph/0111161 . doi:10.1063/1.1419591. 
  7. ^ Gravitation and Inertia, I. Ciufolini and J.A. Wheeler, Princeton Physics Series, 1995, ISBN 0-691-03323-4
  8. ^ B. Mashhoon; F. Gronwald; H.I.M. Lichtenegger (1999). "Gravitomagnetism and the Clock Effect". Lect.Notes Phys. 562: 83–108. Bibcode:2001LNP...562...83M. arXiv:gr-qc/9912027 . doi:10.1007/3-540-40988-2_5. 
  9. ^ S.J. Clark; R.W. Tucker (2000). "Gauge symmetry and gravito-electromagnetism". Classical and Quantum Gravity. 17 (19): 4125–4157. Bibcode:2000CQGra..17.4125C. arXiv:gr-qc/0003115 . doi:10.1088/0264-9381/17/19/311. 
  10. ^ B. Mashhoon (2008). "Gravitoelectromagnetism: A Brief Review". Bibcode:2003gr.qc....11030M. arXiv:gr-qc/0311030 . 
  11. ^ B. Mashhoon (2000). "Gravitoelectromagnetism". Reference Frames and Gravitomagnetism - Proceedings of the XXIII Spanish Relativity Meeting. Bibcode:2001rfg..conf..121M. arXiv:gr-qc/0011014 . doi:10.1142/9789812810021_0009. 
  12. ^ R.L. Forward (1963). "Guidelines to Antigravity". American Journal of Physics. 31 (3): 166–170. Bibcode:1963AmJPh..31..166F. doi:10.1119/1.1969340. 
  13. ^*pi*radius+of+Earth*earth+gravity%2F(5*c^2*day)

Further readingEdit


  • J. B. Hartle (2002). Gravity: An Introduction to Einstein's General Relativity. Addison-Wesley. pp. 296, 303. ISBN 9780805386622. 
  • S. Carroll (2003). Spacetime and Geometry: An Introduction to General Relativity. Addison-Wesley. p. 281. ISBN 9780805387322. 
  • J.A. Wheeler (1990). "Gravity's next prize: Gravitomagnetism". A journey into gravity and spacetime. Scientific American Library. pp. 232–233. ISBN 0-7167-5016-3. 
  • L. Iorio (ed.) (2007). Measuring Gravitomagnetism: A Challenging Enterprise. Nova. ISBN 1-60021-002-3. 


External linksEdit