Le Sage's theory of gravitation

Le Sage's theory of gravitation

Le Sage's theory of gravitation is the most common name for the kinetic theory of gravity originally proposed by Nicolas Fatio de Duillier in 1690 and later by Georges-Louis Le Sage in 1748. The theory proposed a mechanical explanation for Newton's gravitational force in terms of streams of tiny unseen particles (which Le Sage called ultra-mundane corpuscles) impacting on all material objects from all directions. According to this model, any two material bodies partially shield each other from the impinging corpuscles, resulting in a net imbalance in the pressure exerted by the impacting corpuscles on the bodies, tending to drive the bodies together. This mechanical explanation for gravity never gained widespread acceptance, although it continued to be studied occasionally by physicists until the beginning of the twentieth century, by which time it was generally considered to be conclusively discredited.

Basic theory

but no net directional force (P1). With a second object "B" present, however, a fraction of the particles that would otherwise have struck A from the direction of B is intercepted, so B works as a shield, i.e. from the direction of B, A will be struck by fewer particles than from the opposite direction. Likewise B will be struck by fewer particles from the direction of A than from the opposite direction. One can say that A and B are "shadowing" each other, and the two bodies are pushed toward each other by the resulting imbalance of forces (P2). Thus the apparent attraction between bodies is, according to this theory, actually a diminished push from the direction of other bodies, so the theory is sometimes called "push gravity" or "shadow gravity", although it is more widely referred to as "Lesage gravity".

;Nature of collisions If the collisions of body A and the gravific particles are fully elastic, the intensity of the reflected particles would be as strong as of the incoming ones, so no net directional force would arise. The same is true if a second body B is introduced, where B acts as a shield against gravific particles in the direction of A. The gravific particle C which ordinarily would strike on A is blocked by B, but another particle D which ordinarily would not have struck A, is re-directed by the reflection on B, and therefore replaces C. Thus if the collisions are fully elastic, the reflected particles between A and B would fully compensate any shadowing effect. In order to account for a net gravitational force, it must be assumed that the collisions are not fully elastic, or at least that the reflected particles are slowed, so that their momentum is reduced after the impact. This would result in streams with diminished momentum departing from A, and streams with undiminished momentum arriving at A, so a net directional momentum toward the center of A would arise (P3). Under this assumption, the reflected particles in the two-body case will not fully compensate the shadowing effect, because the reflected flux is weaker than the incident flux.

;Inverse square law Since it is assumed that some or all of the gravific particles converging on an object are either absorbed or slowed by the object, it follows that the intensity of the flux of gravific particles emanating from the direction of a massive object is less than the flux converging on the object. We can imagine this imbalance of momentum flow - and therefore of the force exerted on any other body in the vicinity - distributed over a spherical surface centered on the object (P4). The imbalance of momentum flow over an entire spherical surface enclosing the object is independent of the size of the enclosing sphere, whereas the surface area of the sphere increases in proportion to the square of the radius. Therefore, the momentum imbalance per unit area decreases inversely as the square of the distance.

;Mass proportionalityFrom the premises outlined so far, there arises only a force which is proportional to the surface of the bodies. But gravity is proportional to the masses. To satisfy the need for mass proportionality, the theory posits that a) the basic elements of matter are very small so that gross matter consists mostly of empty space, and b) that the particles are so small, that only a small fraction of them would be intercepted by gross matter. The result is, that the "shadow" of each body is proportional to the surface of every single element of matter. If it is then assumed that the elementary opaque elements of all matter are identical (i.e., having the same ratio of density to area), it will follow that the shadow effect is, at least approximately, proportional to the mass (P5).


Nicolas Fatio presented the first formulation of his thoughts on gravitation in a letter to Christiaan Huygens in the spring of 1690. [Citation | author=Fatio de Duillier, N. | author-link =Nicolas Fatio de Duillier | year= 1690a | contribution =Lettre N° 2570 | contribution-url=http://gallica.bnf.fr/ark:/12148/bpt6k778578/f388.table | editor= Société Hollandaise des Sciences | title=Oeuvres complètes de Christiaan Huygens | volume =9 | place = The Hague | publication-date=1888-1950 | pages =381–389 ] Two days later Fatio read the content of the letter before the Royal Society in London. In the following years Fatio composed several draft manuscripts of his major work "De la Cause de la Pesanteur", but none of this material was published in his lifetime. In 1731 Fatio also sent his theory as a Latin poem, in the style of Lucretius, to the Paris Academy of Science, but it was dismissed. Some fragments of these manuscripts and copies of the poem were later acquired by Le Sage who failed to find a publisher for Fatio's papers.See secondary sources, Prévost (1805)] So it lasted until 1929, [Citation | author=Fatio de Duillier, N. | author-link=Nicolas Fatio de Duillier | year=1701 | contribution=Die wiederaufgefundene Abhandlung von Fatio de Duillier: De la cause de la Pesanteur | contribution-url=http://www.mahag.com/grav/bopp.php | editor=Bopp, Karl | title=Drei Untersuchungen zur Geschichte der Mathematik | periodical=Schriften der Straßburger Wissenschaftlichen Gesellschaft in Heidelberg | volume=10 | location=Berlin & Leipzig | publication-date=1929 | pages=19–66 ] when the only complete copy of Fatio's manuscript was published by Bopp, and in 1949 [Citation | author=Fatio de Duillier, N. | author-link=Nicolas Fatio de Duillier | chapter =De la Cause de la Pesanteur | editor=Gagnebin, Bernard | title=De la Cause de la Pesanteur: Mémoire de Nicolas Fatio de Duillier | journal =Notes and Records of the Royal Society of London | volume =6 | pages =125–160 | year =1743 | publication-date=1949 | chapter-url=http://www.journals.royalsoc.ac.uk/link.asp?id=bn57l77831121738 | doi=10.1098/rsnr.1949.0018 ] Gagnebin used the collected fragments in possession of Le Sage to reconstruct the paper. The Gagnebin edition includes revisions made by Fatio as late as 1743, forty years after he composed the draft on which the Bopp edition was based. However, the second half of the Bopp edition contains the mathematically most advanced parts of Fatio's theory, and were not included by Gagnebin in his edition. For a detailed analysis of Fatio's work, and a comparison between the Bopp and the Gagnebin editions, see ZeheZehe (1980), secondary sources] The following description is mainly based on the Bopp edition.

Features of Fatio's theory

;Fatio's pyramid (Problem I) Fatio assumed that the universe is filled by minute particles, which are moving indiscriminately with very high speed and rectilinearly in all directions. To illustrate his thoughts he used the following example: Suppose an object "C", on which an infinite small plane zz and a sphere centered about "zz" is drawn. Into this sphere Fatio placed the pyramid "PzzQ", in which some particles are streaming in the direction of "zz" and also some particles, which were already reflected by "C" and therefore depart from "zz". Fatio proposed that the mean velocity of the reflected particles is lower and therefore their momentum is weaker than that of the incident particles. The result is "one stream", which pushes all bodies in the direction of "zz". So on one hand the speed of the stream remains constant, but on the other hand at larger proximity to "zz" the density of the stream increases and therefore its intensity is proportional to 1/r². And because one can draw an infinite number of such pyramids around "C", the proportionality applies to the entire range around "C".

;Reduced speedIn order to justify the assumption, that the particles are travelling after their reflection with diminished velocities, Fatio stated the following assumptions:
* Either ordinary matter, or the gravific particles, or both are inelastic, or
* the impacts are fully elastic, but the particles are not absolutely hard, and therefore are in a state of vibration after the impact, and/or
* due to friction the particles begin to rotate after their impacts. These passages are the most incomprehensible parts of Fatio's theory, because he never clearly decided, which sort of collision he actually preferred. However, in the last version of his theory in 1742 he shortened the related passages and ascribed "perfect elasticity or spring force" to the particles and on the other hand "imperfect elasticity" to gross matter, therefore the particles would be reflected with diminished velocities. Additionally, Fatio faced another problem: What is happening if the particles collide with each other? Inelastic collisions would lead to a steady decrease of the particle speed and therefore a decrease of the gravitational force. To avoid this problem, Fatio supposed that the diameter of the particles is very small compared to their mutual distance, so their interactions are very rare.

;CondensationFatio thought for a long time that, since corpuscles approach material bodies at a higher speed than they recede from them (after reflection), there would be a progressive accumulation of corpuscles near material bodies (an effect which he called "condensation). However, he later realized that although the incoming corpuscles are quicker, they are spaced fruther apart than are the reflected corpuscles, so the inward and outward flow rates are the same. Hence there is no secular accumulation of corpuscles, i.e., the density of the reflected corpuscles remains constant. Fatio also noted that, by increasing both the velocity and the elasticity of the corpuscles, the difference between the speeds of the incoming and reflected corpuscles (and hence the difference in densities) can be made arbitrarily small while still maintaining the same effective gravitational force. ;Porosity of gross matterIn order to ensure mass proportionality, Fatio assumed that gross matter is extremely permeable to the flux of corpuscles. He sketched 3 models to justify this assumption:
* He assumed that matter is an accumulation of small "balls" whereby their diameter compared with their distance among themselves is "infinitely" small. But he rejected this proposal, because under this condition the bodies would approach each other and therefore wouldn't remain stable.
* Then he assumed that the balls could be connected through bars or lines and would form some kind of crystal lattice. However, he rejected this model too - if several atoms are together, the gravific fluid isn't able to penetrate this structure equally in all direction, and therefore mass proportionality is impossible.
* At the end Fatio also removed the balls and only left the lines or the net. By making them "infinitely" smaller than their distance among themselves, thereby a maximum penetration capacity could be achieved.

;Pressure force of the particles (Problem II)Already in 1690 Fatio assumed, that the "push force" exerted by the particles on a plain surface is the sixth part of the force, which would be produced if all particles are lined up normal to the surface. Fatio now gave a proof of this proposal by determination of the force, which is exerted by the particles on a certain point zz. He derived the formula "p=ρv²zz/6". This solution is very similar to the formula known in the kinetic theory of gases "p=ρv²/3", which was found by Daniel Bernoulli in 1738. This was the first time that a solution analogous to the similar result in kinetic theory was pointed out - long "before" the basic concept of the latter theory was developed. However, Bernoulli's value is twice as large as Fatio's one, because according to Zehe, Fatio only calculated the value "mv" for the change of impulse after the collision, but not "2mv" and therefore got the wrong result. (His result is only correct in the case of totally inelastic collisions.) Fatio tried to use his solution not only for explaining gravitation, but for explaining the behaviour of gases as well. He tried to construct a thermometer, which should indicate the "state of motion" of the air molecules and therefore estimate the temperature. But Fatio (unlike Bernoulli) didn't "identify" heat and the movements of the air particles - he used another fluid, which should be responsible for this effect. It is also unknown, whether Bernoulli was influenced by Fatio or not.

;Infinity (Problem III)In this chapter Fatio examines the connections between the term "infinity" and its relations to his theory. Fatio often justified his considerations with the fact that different phenomena are "infinitely smaller or larger" than others and so many problems can be reduced to an undetectable value. For example the diameter of the bars is infinitely smaller than their distance to each other; or the speed of the particles is infinitely larger than those of gross matter; or the speed difference between reflected and non-reflected particles is infinitely small.

;Resistance of the medium (Problem IV)This is the mathematically most complex part of Fatio's theory. There he tried to estimate the resistance of the particle streams for moving bodies. Supposing "u" is the velocity of gross matter, "v" is the velocity of the gravific particles and "ρ" the density of the medium. In the case "v << u" and "ρ = const." Fatio stated that the resistance is "ρu²". In the case "v >> u" and "ρ = const." the resistance is "4/3ρuv". Now, Newton stated that the lack of resistance to the orbital motion requires an extreme sparseness of any medium in space. So Fatio decreased the density of the medium and stated, that to maintain sufficient gravitational force this reduction must be compensated by changing v "inverse proportional to the square root of the density". This follows from Fatio's particle pressure, which is proportional to "ρv²". According to Zehe, Fatio's attempt to increase v to a very high value would actually leave the resistance very small compared with gravity, because the resistance in Fatio's model is proportional to "ρuv" but gravity (i.e. the particle pressure) is proportional to "ρv²".

Reception of Fatio's theory

Fatio was in communication with some of the most famous scientists of his time.

There was a strong personal relationship between Isaac Newton and Fatio in the years 1690 to 1693. Newton's statements on Fatio's theory differed widely. For example, after describing the necessary conditions for a mechanical explanation of gravity, he wrote in an (unpublished) note in his own printed copy of the "Principia" in 1692:"The unique hypothesis by which gravity can be explained is however of this kind, and was first devised by the most ingenious geometer Mr. N. Fatio." On the other hand, Fatio himself stated that although Newton had commented privately that Fatio's theory was the best possible "mechanical" explanation of gravity, he also acknowledged that Newton tended to believe that the true explanation of gravitation was not mechanical. Also, Gregory noted in his "Memoranda": "Mr. Newton and Mr. Halley laugh at Mr. Fatio’s manner of explaining gravity." This was allegedly noted by him in December 28, 1691. However, the real date is unknown, because both ink and feather which were used, differ from the rest of the page. After 1694, the relationship between the two men cooled down.

Christiaan Huygens was the first person informed by Fatio of his theory, but never accepted it. Fatio believed he had convinced Huygens of the consistency of his theory, but Huygens denied this in a letter to Gottfried Leibniz. There was also a short correspondence between Fatio and Leibniz on the theory. Leibniz criticized Fatio's theory for demanding empty space between the particles, which was rejected by him (Leibniz) on philosophical grounds. Jakob Bernoulli expressed an interest in Fatio's Theory, and urged Fatio to write his thoughts on gravitation in a complete manuscript, which was actually done by Fatio. Bernoulli then copied the manuscript, which now resides in the university library of Basel, and was the base of the Bopp edition.

Nevertheless, Fatio's theory remained largely unknown with a few exceptions like Cramer and Le Sage, because he never was able to formally publish his works and he fell under the influence of a group of religious fanatics called the "French prophets" (which belonged to the camisards) and therefore his public reputation was ruined.

Cramer and Redeker

In 1731 the Swiss mathematician Gabriel Cramer published a dissertation, [Citation | author=Cramer, G. | author-link=Gabriel Cramer | year=1731 | title=Theses Physico-Mathematicae de Gravitate (Dissertation) | place=Geneva ] at the end of which appeared a sketch of a theory very similar to Fatio's - including net structure of matter, analogy to light, shading - but without mentioning Fatio's name. It was known to Fatio that Cramer had access to a copy of his main paper, so he accused Cramer of only repeating his theory without understanding it. It was also Cramer who informed Le Sage about Fatio's theory in 1749. In 1736 the German physician Franz Albert Redeker also published a similar theory. [Citation | author=Redeker, F. A. | year=1736 | title=De cause gravitatis meditatio | periodical=Lemgoviae ex officina Meyeriana] Any connection between Redeker and Fatio is unknown.

Le Sage

The first exposition of his theory, "Essai sur l'origine des forces mortes", was sent by Le Sage to the Academy of Sciences at Paris in 1748, but it was never published. According to Le Sage, "after" creating and sending his essay he was informed on the theories of Fatio, Cramer and Redeker. In 1756 for the first time one of his expositions of the theory was published, [Citation | author=Le Sage, G.-L. | author-name=Georges-Louis Le Sage |year =1756 | title=Letter à une académicien de Dijon.. | journal=Mercure de France | pages=153–171] and in 1758 he sent a more detailed exposition, "Essai de Chymie Méchanique", to a competition to the Academy of Sciences in Rouen. [Citation | author=Le Sage, G.-L. | author-link=Georges-Louis Le Sage| year=1761 | title=Essai de Chymie Méchanique | publisher=Not published - private print | url=http://gallica.bnf.fr/ark:/12148/bpt6k110507m] In this paper he tried to explain both the nature of gravitation and chemical affinities. The exposition of the theory which became accessible to a broader public, "Lucrèce Newtonien" (1784), in which the correspondence with Lucretius’ concepts was fully developed. [Citation | author=Le Sage, G.-L. | author-link=Georges-Louis Le Sage | title =Lucrèce Newtonien | journal=Memoires de l’Academie Royale des Sciences et Belles Lettres de Berlin | volume = | issue = | pages = 404–432 | year =1784 | url=http://bibliothek.bbaw.de/bibliothek-digital/digitalequellen/schriften/anzeige/index_html?band=03-nouv/1782&seite:int=0495 An English translation appears in Citation | author=Le Sage, G.-L. | author-link=Georges-Louis Le Sage | contribution =The Newtonian Lucretius | year= 1898 | editor= Langley, Samuel P. | editor-link= Samuel Pierpont Langley| title=| periodical=Annual Report of the Board of Regents of the Smithsonian Institution | pages = 139–160 | publication-date=June 30, 1898] Another exposition of the theory was published from Le Sage's notes posthumously by Pierre Prévost in 1818. [Citation | author=Le Sage, G.-L. | author-link=Georges-Louis Le Sage | year=1818 | chapter=Physique Mécanique des Georges-Louis Le Sage | editor=Prévost, Pierre | editor-link=Pierre Prévost | title=Deux Traites de Physique Mécanique | place=Geneva & Paris | publisher=J.J. Paschoud | pages=1–186 | chapter-url=http://resolver.sub.uni-goettingen.de/purl?PPN521099943]

Le Sage's basic concept

Le Sage discussed the theory in great detail and he proposed quantitative estimates for some of the theory's parameters.
* He called the gravitational particles "ultramundane corpuscles", because he supposed them to originate beyond our known universe. The distribution of the ultramundane flux is isotropic and the laws of its propagation are very similar to that of light.
* Le Sage argued that no gravitational force would arise if the matter-particle-collisions are perfectly elastic . So he proposed that the particles and the basic constituents of matter are "absolutely hard" and asserted that this implies a complicated form of interaction, completely inelastic in the direction normal to the surface of the ordinary matter, and perfectly elastic in the direction tangential to the surface. He then commented that this implies the mean speed of scattered particles is 2/3 of their incident speed. To avoid inelastic collisions between the particles, he supposed that their diameter is very small relative to their mutual distance.
* That resistance of the flux is proportional to uv (where v is the velocity of the particles and u that of gross matter) and gravity is proportional to v², so the ratio resistance/gravity can be made arbitrarily small by increasing v. Therefore he suggested that the ultramundane corpuscles might move at the speed of light, but after further consideration he adjusted this to 105 times the speed of light.
* To maintain mass proportionality, ordinary matter consists of cage-like structures, in which their diameter is only the 107th part of their mutual distance. Also the "bars", which constitute the cages, were small (around 1020 times as long as thick) relative to the dimensions of the cages, so the particles can travel through them nearly unhindered.
* Le Sage also attempted to use the shadowing mechanism to account for the forces of cohesion, and for forces of different strengths, by positing the existence of multiple species of ultramundane corpuscles of different sizes, as illustrated in Figure 9.Le Sage said that he was the first one, who drew all consequences from the theory and also Prévost said that Le Sage's theory was more developed than Fatio's theory. However, by comparing the two theories and after a detailed analysis of Fatio's papers (which also were in possession of Le Sage) Zehe judged that Le Sage contributed nothing essentially new and he often didn't reach Fatio's level.

Reception of Le Sage's theory

Le Sage’s ideas were not well-received during his day, except for some of his friends and associates like Pierre Prévost, Charles Bonnet, Jean-André Deluc and Simon Lhuilier. They mentioned and described Le Sage's theory in their books and papers, which were used by their contemporaries as a secondary source for Le Sage's theory (because of the lack of published papers by Le Sage himself) .

;Euler, Bernoulli, and Boscovich
Leonhard Euler once remarked that Le Sage's model was "infinitely better" than that of all other authors, and that all objections are balanced out in this model, but later he said the analogy to light had no weight for him, because he believed in the wave nature of light. After further consideration, Euler came to disapprove of the model, and he wrote to Le Sage: [Wolf (1852), secondary sources]

Daniel Bernoulli was pleased by the similarity of Le Sage's model and his own thoughts on the nature of gases. However, Bernoulli himself was the opinion that his own kinetic theory of gases was only a speculation, and likewise he regarded Le Sage's theory as highly speculative. [Evanes (2002), secondary sources]

Roger Joseph Boscovich pointed out, that Le Sage's theory is the first one, which actually can explain gravity by mechanical means. However, he rejected the model because of the enormous and unused quantity of ultramundane matter. John Playfair described Boscovich's arguments by saying:

A very similar argument was later given by Maxwell (see the sections below). Additionally, Boscovich denied the existence of all contact and immediate impulse at all, but proposed repulsive and attractive actions at a distance.

;Lichtenberg, Kant, and Schelling
Georg Christoph Lichtenberg's [Citation | author=Lichtenberg, G. C. | author-link =Georg Christoph Lichtenberg | title =Aufzeichnungen über die Theorie der Schwere von G.L. Le Sage | editor= Zehe, H. & Hinrichs, W.| periodical =Nachrichten der Akademie der Wissenschaften zu Göttingen, II. mathematisch-physikalische Klasse | number =1 | year =2003] knowledge of Le Sage's theory was based on "Lucrece Newtonien" and a summary by Prévost. Lichtenberg originally believed (like Descartes) that every explanation of natural phenomena must be based on rectilinear motion and impulsion, and Le Sage's theory fulfilled these conditions. In 1790 he expressed in one of his papers his enthusiasm for the theory, believing that Le Sage's theory embraces all of our knowledge and makes any further dreaming on that topic useless. He went on by saying: "If it is a dream, it is the greatest and the most magnificent which was ever dreamed..." and that we can fill with it a gap in our books, which can only be filled by a dream. [Lichtenberg, in German: "Ist es ein Traum, so ist es der größte und erhabenste der je ist geträumt worden, und womit wir eine Lücke in unseren Büchern ausfüllen können, die nur durch einen Traum ausgefüllt werden kann".]

He often referred to Le Sage's theory in his lectures on physics at the University of Göttingen. However, around 1796 Lichtenberg changed his views after being persuaded by the arguments of Immanuel Kant, who criticized any kind of theory that attempted to replace attraction with impulsion. [Citation | author=Kant, I. | author-link =Immanuel Kant | title =Metaphysische Anfangsgründe der Naturwissenschaft | pages =Dynamik, Lehrsatz 5 | year =1786 | url =http://philosophiebuch.de/metannat.htm] Kant pointed out that the very existence of spatially extended configurations of matter, such as particles of non-zero radius, implies the existence of some sort of binding force to hold the extended parts of the particle together. Now, that force cannot be explained by the push from the gravitational particles, because those particles too must hold together in the same way. To avoid this circular reasoning, Kant asserted that there must exist a fundamental attractive force. This was precisely the same objection that had always been raised against the impulse doctrine of Descartes in the previous century, and had led even the followers of Descartes to abandon that aspect of his philosophy.

Another German philosopher, Friedrich Wilhelm Joseph Schelling, rejected Le Sage's model because its mechanistic materialism was incompatible with Schelling's very idealistic and anti-materialistic philosophy. [Citation | author=Schelling, F.W.J. | author-link =Friedrich Wilhelm Joseph Schelling | title =Ideen zu einer Philosophie der Natur (2. book, 3. chapter) | year =1797 | url =http://books.google.com/books?id=7SQCAAAAQAAJ]

;LaplacePartly in consideration of Le Sage's theory, Pierre-Simon Laplace undertook to determine the necessary speed of gravity in order to be consistent with astronomical observations. He calculated that the speed must be “at least a hundred millions of times greater than that of light”, in order to avoid unacceptably large inequalities due to aberration effects in the lunar motion. [Citation | author=Laplace, P.-S. | author-link =Pierre-Simon Laplace | title =A Treatise in Celestial Mechanics | volume =4, Book 10, Chapter 7 | place =Chelsea - New York, 1966 | year =1805/1966] This was taken by most researchers, including Laplace, as support for the Newtonian concept of instantaneous action at a distance, and to indicate the implausibility of any model such as Le Sage's. Laplace also argued that to maintain mass-proportionality the upper limit for earth's molecular surface area is at the most the ten-millionth of earth surface. To Le Sage's disappointment, Laplace never directly mentioned Le Sage's theory in his works.

Kinetic theory

Because the theories of Fatio, Cramer and Redeker were not widely known, Le Sage's exposition of the theory enjoyed a resurgence of interest in the latter half of the nineteenth century, coinciding with the development of the kinetic theory.

;LeraySince Le Sage's particles must lose speed when colliding with ordinary matter (in order to produce a net gravitational force), a huge amount of energy must be converted to internal energy modes. If those particles have no internal energy modes, the excess energy can only be absorbed by ordinary matter. Addressing this problem, P. Leray [Citation | author=Leray, P. | title =Theorie nouvelle de la gravitation | journal =Comptes Rendus | volume =69 | pages =615–621 | year =1869 | url=http://gallica.bnf.fr/ark:/12148/bpt6k30260/f617.item] proposed a particle model (perfectly similar to Le Sage's) in which he asserted that the absorbed energy is used by the bodies to produce magnetism and heat. He suggested, that this might be an answer for the question of where the energy output of the stars comes from.

;Kelvin and TaitLe Sage's "own" theory became a subject of re-newed interest in the latter part of the 19th century following a paper published by Kelvin in 1873. [Citation | author=Thomson, William (Lord Kelvin) | author-link=William Thomson, 1st Baron Kelvin | title =On the ultramundane corpuscles of Le Sage | journal =Phil. Mag. | volume =45 | pages =321–332 | year =1873 | url =http://www.hti.umich.edu/cgi/t/text/pageviewer-idx?idno=aat1571.0005.001&c=umhistmath&seq=81&size=s&view=image] Unlike Leray, who treated the heat problem imprecisely, Kelvin stated that the absorbed energy represents a very high heat, sufficient to vaporize any object in a fraction of a second. So Kelvin re-iterated an idea that Fatio had originally proposed in the 1690s for attempting to deal with the thermodynamic problem inherent in Le Sage's theory. He proposed that the excess heat might be absorbed by internal energy modes of the particles themselves, based on his proposal of the vortex-nature of matter. In other words, the original translational kinetic energy of the particles is transferred to internal energy modes, chiefly vibrational or rotational, of the particles. Appealing to Clausius's proposition that the energy in any particular mode of a gas molecule tends toward a fixed ratio of the total energy, Kelvin went on to suggest that the "energized" but slower moving particles would subsequently be restored to their original condition due to collisions (on the cosmological scale) with other particles. Kelvin also asserted that it would be possible to extract limitless amounts of free energy from the ultramundane flux, and described a perpetual motion machine to accomplish this. (The flaw in Kelvin's reasoning was that Clausius's proposition would apply only if ordinary matter was in thermodynamic equilibrium with the ultramundane flux - in which case there would no net gravitational effect.)

Subsequently, Peter Guthrie Tait called the Le Sage theory the only plausible explanation of gravitation which has been propounded at that time. He went on by saying:

Kelvin himself, however, was not optimistic that Le Sage's theory could ultimately give a satisfactory account of phenomena. After his brief paper in 1873 noted above, he never returned to the subject, except to make the following comment:

Samuel Tolver Preston [Citation | author=Preston, S. T.| title =On some dynamical conditions applicable to LeSage’s theory of gravitation | journal =Phil. Mag., fifth ser. | volume =4 | pages =206–213 (pt. 1) and 364–375 (pt. 2) | year =1877] illustrated that many of the postulates introduced by Le Sage concerning the gravitational particles, such as rectilinear motion, rare interactions, "etc"., could be collected under the single notion that they behaved (on the cosmological scale) as the particles of a gas with an extremely long mean free path. Preston also accepted Kelvin's proposal of internal energy modes of the particles. He illustrated Kelvin's model by comparing it with the collision of a steel ring and an anvil - the anvil wouldn't be shaken very much, but the steel ring would be in a state of vibration and therefore departs with diminished velocity. He also argued, that the mean free path of the particles is at least the distance between the planets - on longer distances the particles regain their translational energy due collisions with each other, so he concluded that on longer distances there would be no attraction between the bodies, "independent of their size". Paul Drude suggested that this could possibly be a connection with some theories of Carl Gottfried Neumann and Hugo von Seeliger, who proposed some sort of absorption of gravity in open space. [Drude (1897), secondary sources]

;MaxwellA review of the Kelvin-Le Sage theory was published by James Clerk Maxwell in the Ninth Edition of the Encyclopaedia Britannica under the title "Atom" in 1875. [Citation | author=Maxwell, J. C. | author-link =James Clerk Maxwell | contribution=Atom | editor=none| title=Encyclopedia Britannica | edition =9th | volume =3 | pages =38–47 | year =1875 | contribution-url =http://www.archive.org/details/encyclopediabrit03newyrich ] After describing the basic concept of the theory he wrote (with sarcasm according to Aronson):Aronson (1960), secondary sources]

Maxwell commented on Kelvin’s suggestion of different energy modes of the particles that this implies the gravitational particles are not simple primitive entities, but rather systems, with their own internal energy modes, which must be held together by (unexplained) forces of attraction. He argues that the temperature of bodies must tend to approach that at which the average kinetic energy of a molecule of the body would be equal to the average kinetic energy of an ultra-mundane particle and he states that the latter quantity must be much greater than the former and concludes that ordinary matter should be incinerated within seconds under the Le Sage bombardment. He wrote:

Maxwell also argued that the theory requires "an enormous expenditure of external power" and therefore violating the conservation of energy as the fundamental principle of nature. Preston responded to Maxwell's criticism by arguing that the kinetic energy of each individual simple particle could be made arbitrarily low by positing a sufficiently low mass (and higher number density) for the particles. But this issue later was discussed in a more detailed way by Poincaré, who showed that the thermodynamic problem within Le Sage models remained unresolved.

;Isenkrahe, Rysanik, du Bois-Reymond
Caspar Isenkrahe presented his model in a variety of publications between 1879-1915. [Citation | author=Isenkrahe, C. | author-link=Caspar Isenkrahe | year=1879 | title=Das Räthsel von der Schwerkraft: Kritik der bisherigen Lösungen des Gravitationsproblems und Versuch einer neuen auf rein mechanischer Grundlage | place=Braunschweig | publisher=Friedrich Vieweg und Sohn] His basic assumptions were very similar to those of Le Sage and Preston, but he gave a more detailed application of the kinetic theory. However, by asserting that the velocity of the corpuscles after collision was reduced without any corresponding increase in the energy of any other object, his model violated the conservation of energy. He noted that there is a connection between the weight of a body and its density (because any decrease in the density of an object reduces the internal shielding) so he went on to assert that warm bodies should be heavier than colder ones (related to the effect of thermal expansion).

In another model A. Rysanek in 1887 [Citation | author=Rysanek, A. | journal =Repert. Exp. Phys. | volume =24 | pages =90–115 | year =1887] also gave a careful analysis, including an application of Maxwell's law of the particle velocities in a gas. He distinguished between a gravitational and a luminiferous aether. This separation of those two mediums was necessary, because according to his calculations the absence of any drag effect in the orbit of Neptune implies a lower limit for the particle velocity of 5 · 1019 cm/sec. He (like Leray) argued that the absorbed energy is converted into heat, which might be transferred into the luminiferous aether and/or is used by the stars to maintain their energy output. However, these qualitative suggestions were unsupported by any quantitative evaluation of the amount of heat actually produced.

In 1888 Paul David Gustav du Bois-Reymond argued against Le Sage's model, partly because the predicted force of gravity in Le Sage's theory is not strictly proportional to mass. In order to achieve exact mass proportionality as in Newton's theory (which implies no shielding or saturation effects and an infinitely porous structure of matter), the ultramundane flux must be infinitely intense. Du Bois-Reymond rejected this as absurd. In addition, du Bois-Reymond like Kant observed that Le Sage's theory cannot meet its goal, because it invokes concepts like "elasticity" and "absolute hardness" etc., which (in his opinion) can only be explained by means of attractive forces. The same problem arises for the cohesive forces in molecules. As a result, the basic intent of such models, which is to dispense with elementary forces of attraction, is impossible. [Citation | author=du Bois-Reymond, P. D. G. | author-link =Paul David Gustav du Bois-Reymond | title =Ueber die Unbegreiflichkeit der Fernkraft | journal =Naturwissenschaftliche Rundschau | volume =3 | issue =14 | pages =169–176 | year =1888 | url =http://www.digizeitschriften.de/resolveppn/GDZPPN001069322]

Wave models

;Keller and BoisbaudranIn 1863 F.A.E. and Em. Keller [Citation | author=Keller, F.A.E & Keller, Ém. | title =Mémoire sur la cause de la pesanteur et des effets attribués à l'attraction universelle | journal =Comptes Rendus | volume =56 | pages =530–533 | year =1863 | url=http://gallica.bnf.fr/ark:/12148/bpt6k3013s/f530.item] presented a theory by using a Le Sage type mechanism in combination with longitudinal waves of the aether. They supposed that those waves are propagating in every direction and losing some of their momentum after the impact on bodies, so between two bodies the pressure exerted by the waves is weaker than the pressure around them. In 1869 L. de Boisbaudran [Citation | author=de Boisbaudran, L. | title =Note sur la théorie de la pesanteur | journal =Comptes Rendus | volume =69 | pages =703–705 | year =1869 | url=http://gallica.bnf.fr/ark:/12148/bpt6k30260/f705.item] presented the same model as Leray (including absorption and the production of heat etc.), but like Keller he replaced the particles with longitudinal waves of the aether.

;LorentzAfter these attempts other authors substituted electromagnetic radiation for Le Sage’s particles early 1900s. This was in connection with the Lorentz ether theory and the electron theory of that time, in which the electrical constitution of matter was assumed.

In 1900 Hendrik Lorentz [Citation | author=Lorentz, H. A. | author-link =Hendrik Lorentz | title =Considerations on Gravitation | journal =Proc. Acad. Amsterdam | volume =2 | pages =559–574 | year =1900 | url =http://www.historyofscience.nl/search/detail.cfm?pubid=260&view=image&startrow=1] wrote, that Le Sage's particle model is not consistent with the electron theory of his time. But the detection that trains of electromagnetic waves could produce some pressure in combination with the penetrating power of Röntgen rays (now called x-rays), led him to the conclusion, that nothing is speaking against the possible existence of an even more penetrating radiation then x-rays, which could replace Le Sage's particles. Lorentz showed that an attractive force between charged particles (which might be taken to model the elementary subunits of matter) would indeed arise, but only if the incident energy were entirely absorbed. This was the same fundamental problem which had afflicted the particle models. So Lorentz wrote:

In 1922 [Citation | author=Lorentz, H. A. | author-link =Hendrik Lorentz | title=Lectures On Theoretical Physics| publisher=Macmillan and Co. | year=1922, English translation: 1927 | place= London | url=http://www.archive.org/details/lecturesontheore031600mbp] Lorentz first examined Martin Knudsen's investigation on rarefied gases and in connection with that he discussed Le Sage's particle model, followed by a summary of his own electromagnetic Le Sage model - but he repeated his conclusion from 1900: Without absorption no gravitational effect.

In 1913 David Hilbert referred to Lorentz's theory and criticised it by arguing that no force in the form 1/r² can arise, if the mutual distance of the atoms is large enough when compared with their wavelength. [Corry (1999), secondary sources]

;J.J. ThomsonIn 1904 J. J. Thomson [Citation | author=Thomson, J. J. | author-link =J. J. Thomson | title =Electricity and matter | place=Westminster | publisher=Archibald Constable & Co., Ltd. | year =1904 | url =http://www.archive.org/details/electricitymatte00thomiala] considered a Le Sage-type model in which the primary ultramundane flux consisted of a hypothetical form of radiation much more penetrating even than x-rays. He argued that Maxwell's heat problem might be avoided by assuming that the absorbed energy is not be converted into heat, but "re-radiated" in a still more penetrating form. He noted that this process possibly can explain where the energy of radioactive substances is coming from - however, he stated that an internal cause of radioactivity is more probable. In 1911 Thomson went back to this subject in his article "Matter" in the Encyclopædia Britannica Eleventh Edition. [Citation | author=Thomson, J. J. | author-link =J. J. Thomson | contribution= | periodical =Encyclopædia Britannica Eleventh Edition | pages =891–895 | year =1911] There he stated, that this form of secondary radiation is somewhat analogous to how the passage of electrified particles through matter causes the radiation of the even more penetrating x-rays. He remarked:

;Tommasina and Brush

Unlike Lorentz and Thomson, Thomas Tommasina [Citation | author=Tommasina, T. | title =La Physique de la Gravitation | place=Paris | publisher=Gauthier-Villars | year =1928] between 1903 and 1928 suggested long wavelength radiation to explain gravity, and short wave-length radiation for explaining the cohesive forces of matter. Charles F. Brush [Citation | author=Brush, C. F. | author-link =Charles F. Brush | title =A kinetic theory of gravitation | journal =Nature | volume =86 | pages =130–132 | year =1911 | doi=10.1038/086130a0] in 1911 also proposed long wavelength radiation. But he later revised his view and changed to extremely short wavelengths.

Later assessments

;DarwinIn 1905 George Darwin subsequently calculated the gravitational force between two bodies at extremely close range to determine if geometrical effects would lead to a deviation from Newton’s law. [Citation | author=Darwin, G. H. | author-link =George Darwin | title =The analogy between Lesage’s theory of gravitation and the repulsion of light | journal =Proc. Royal Soc. | volume =76 | pages =387–410 | year =1905 | url=http://visualiseur.bnf.fr/CadresFenetre?O=NUMM-56169&I=402&M=imageseule | doi=10.1098/rspa.1905.0042] Here Darwin replaced Le Sage's cage-like units of ordinary matter with microscopic hard spheres of uniform size. He concluded that only in the instance of perfectly inelastic collisions (zero reflection) would Newton’s law stand up, thus reinforcing the thermodynamic problem of Le Sage's theory. Also, such a theory is only valid if the normal "and" the tangential components of impact are totally inelastic (contrary to Le Sage's scattering mechanism), and the elementary particles are exactly of the same size. He went on to say that the emission of light is the exact converse of the absorption of Le Sage's particles. A body with different surface temperatures will move in the direction of the colder part. In a later review of gravitational theories Darwin briefly described Le Sage's theory and said he gave the theory serious consideration, but then wrote:

;PoincaréPartially based on the calculations of Darwin, an important criticism was given by Henri Poincaré in 1908. [Citation | author=Poincaré, H. | author-link =Henri Poincaré | title =La dynamique de l'électron | journal =Revue générale des sciences pures et appliquées | volume =19 | pages =386–402 | year =1908 | url =http://www.univ-nancy2.fr/poincare/bhp/pdf/hp1908rg.pdf An English translation appears in: Citation | author=Poincaré, H. | author-link =Henri Poincaré | title =Science and Methode| publisher =Courier Dover Publications Science | year =2003 | isbn=0486432696 ] He concluded that the attraction is proportional to Ssqrt{ ho}v, where "S" is earth's molecular surface area, "v" is the velocity of the particles, and ρ is the density of the medium. Following Laplace he argued that to maintain mass-proportionality the upper limit for "S" is at the most a ten-millionth of the earth's surface. Now, drag (i.e. the resistance of the medium) is proportional to "Sρv" and therefore the ratio of drag to attraction is inversely proportional to "Sv". To reduce drag Poincaré calculated a lower limit for "v" = 24 · 1017 times the speed of light. So there are lower limits for "Sv" and v, and a upper limit for "S" and with those values one can calculate the produced heat, which is proportional to "Sρv3". The calculation shows that earth's temperature would rise by 1026 degrees per second. Poincaré noticed, "that the earth could not long stand such a regime." Poincaré also analyzed some wave models (Tommasina and Lorentz), remarking that they suffered the same problems as the particle models. To reduce drag, superluminal wave velocities were necessary, and they would still be subject to the heating problem. After describing a similar re-radiation model like Thomson he concluded: "Such are the complicated hypotheses to which we are led when we seek to make Le Sage's theory tenable".

He also stated that if in Lorentz' model the absorbed energy is fully converted into heat, this would raise earth's temperature by 1013 degrees per second. Poincaré then went on to consider Le Sage's theory in the context of the "new dynamics" that had been developed at the end of the 19th and beginning of the 20th centuries, specifically recognizing the relativity principle. For a particle theory he remarked that "it is difficult to imagine a law of collision compatible with the principle of relativity", and the problems of drag and heating remain.

Predictions and criticism

Matter and particles

;Porosity of matterA basic prediction of the theory is the extreme porosity of matter. As supposed by Fatio and Le Sage in 1690/1758 (and before them, Huygens) matter must consist mostly of empty space so that the very small particles can penetrate the bodies nearly undisturbed and therefore every single part of matter can take part in the gravitational interaction. This prediction has been (in some respects) confirmed over the course of the time. Indeed, matter consists mostly of empty space and certain particles like neutrinos can pass through matter nearly unhindered. However, the image of elementary particles as classical entities who interact directly, determined by their shapes and sizes (in the sense of the net structure proposed by Fatio/Le Sage and the equisized spheres of Isenkrahe/Darwin), is not consistent with current understanding of elementary particles. The Lorentz/Thomson proposal of electrical charged particles as the "basic constituents" of matter is inconsistent with current physics as well.

;Cosmic radiationEvery Le Sage-type model assumes the existence of a space-filling isotropic flux or radiation of enormous intensity and penetrating capability. This has some similarity to the cosmic microwave background radiation (CMBR) discovered in the 20th century. CMBR is indeed a space-filling and fairly isotropic flux, but its intensity is extremely small, as is its penetrating capability. The flux of neutrinos, emanating from (for example) the sun, possesses the penetrating properties envisaged by Le Sage for his ultramundane corpuscles, but this flux is not isotropic (since individual stars are the main sources of neutrinos) and the intensity is even less than that of the CMBR. Of course, neither the CMBR nor neutrinos propagate at superluminal speeds, which is another necessary attribute of Le Sage’s particles. From a more modern point of view, discarding the simple “push” concept of Le Sage, the suggestion that the neutrino (or some other particle similar to the neutrino) might be the mediating particle in a quantum field theory of gravitation was considered and disproved by Feynman. [Citation | author=Feynman, R. P. | author-link =Richard Feynman | title =Feynman Lectures on Gravitation | pages =23–28 | year =1995 | publisher=Addison-Wesley]

Gravitational shielding

Although matter is postulated to be very sparse in the Fatio-Le Sage theory, it cannot be perfectly transparent, because in that case no gravitational force would exist. However, the lack of perfect transparency leads to problems: with sufficient mass the amount of shading produced by two pieces of matter becomes less than the sum of the shading that each of them would produce separately, due to the overlap of their shadows (P10, above). This hypothetical effect, called gravitational shielding, implies that addition of matter does not result in a direct proportional increase in the gravitational mass. Therefore, in order to be viable, Fatio and Le Sage postulated that the shielding effect is so small as to be undetectable, which requires that the interaction cross-section of matter must be extremely small (P10, below). This places an extremely high lower-bound on the intensity of the flux required to produce the observed force of gravity. According to standard physics any form of gravitational shielding is a violation of the equivalence principle and therefore is inconsistent with general relativity. [Citation | author=Bertolami, O. & Paramos, J. & Turyshev, S. G. | contribution =General Theory of Relativity: Will it survive the next decade? | editor=H. Dittus, C. Laemmerzahl, S. Turyshev | periodical =Lasers, Clocks, and Drag-Free: Technologies for Future Exploration in Space and Tests of Gravity | pages =27–67 | year =2006 | contribution-url=http://arxiv.org/abs/gr-qc/0602016v2] For more historical information on the connection between gravitational shielding and Le Sage gravity, see Martins, [Martin (1999), secondary sources] [Martins (2002), secondary sources] and Borzeszkowski et al. [Borzeskkowski et al. (2004), secondary sources]

Since Isenkrahe's proposal on the connection between density, temperature and weight was based purely on the anticipated effects of changes in material "density", and since temperature at a given density can be increased or decreased, Isenkrahe's comments do not imply any fundamental relation between temperature and gravitation. (There actually "is" a relation between temperature and gravitation, as well as between binding energy and gravitation, but these actual effects have nothing to do with Isenkrahe's proposal. See the section below on "Coupling to Energy".) Regarding the prediction of a relation between gravitation and density, all experimental evidence indicates that there is no such relation.

Speed of gravity

;DragAccording to Le Sage's theory, an isolated body is subjected to drag if it is in motion relative to the unique isotropic frame of the ultramundane flux (i.e., the frame in which the speed of the ultramundane corpuscles is the same in all directions). This is due to the fact that, if a body is in motion, the particles striking the body from the front have a higher speed (relative to the body) than those striking the body from behind - this effect will act to "decrease" the distance between the sun and the earth. The magnitude of this drag is proportional to vu, where v is the speed of the particles and u is the speed of the body, whereas the characteristic force of gravity is proportional to v2, so the ratio of drag to gravitational force is proportional to u/v. Thus for a given characteristic strength of gravity, the amount of drag for a given speed u can be made arbitrarily small by increasing the speed v of the ultramundane corpuscles. However, in order to reduce the drag to an acceptable level (i.e., consistent with observation) in terms of classical mechanics, the speed v must be many orders of magnitude greater than the speed of light. This makes Le Sage theory fundamentally incompatible with the modern science of mechanics based on special relativity, according to which no particle (or wave) can exceed the speed of light. In addition, even if superluminal particles were possible, the effective temperature of such a flux would be sufficient to incinerate all ordinary matter in a fraction of a second.

;AberrationAs shown by Laplace, another possible Le Sage effect is orbital aberration due to finite speed of gravity. Unless the Le Sage particles are moving at speeds much greater than the speed of light, as Le Sage and Kelvin supposed, there is a time delay in the interactions between bodies (the transit time). In the case of orbital motion this results in each body reacting to a retarded position of the other, which creates a leading force component. Contrary to the drag effect, this component will act to accelerate both objects away from each other. In order to maintain stable orbits, the effect of gravity must either propagate much faster than the speed of light or must not be a purely central force. This has been suggested by many as a conclusive disproof of any Le Sage type of theory. In contrast, general relativity is consistent with the lack of appreciable aberration identified by Laplace, because even though gravity propagates at the speed of light in general relativity, the expected aberration is almost exactly cancelled by velocity-dependent terms in the interaction. [Citation | author=Carlip, S. | title =Aberration and the Speed of Gravity | journal= Pys. Lett. A | volume =167 | pages =81–87 | year =1999 | url =http://www.arxiv.org/abs/gr-qc/9909087]

Range of gravity

In many particle models, such as Kelvin's, the range of gravity is limited due to the nature of particle interactions amongst themselves. The range is effectively determined by the rate that the proposed "internal modes" of the particles can eliminate the momentum defects ("shadows") that are created by passing through matter. Such predictions as to the effective range of gravity will vary and are dependent upon the specific aspects and assumptions as to the modes of interactions that are available during particle interactions. However, for this class of models the observed large-scale structure of the cosmos constrains such dispersion to those that will allow for the aggregation of such immense gravitational structures.


;AbsorptionAs noted in the historical section, a major problem for every Le Sage model is the energy and heat issue. As Maxwell and Poincaré showed, inelastic collisions lead to a vaporization of matter within fractions of a second and the suggested solutions were not convincing. For example, Aronson gave a simple proof of Maxwell's assertion:

Likewise Isenkrahe's violation of the energy conservation law is unacceptable, and Kelvin's application of Clausius' theorem leads (as noted by Kelvin himself) to some sort of perpetual motion mechanism. The suggestion of a secondary re-radiation mechanism for wave models attracted the interest of JJ Thomson, but was not taken very seriously by either Maxwell or Poincaré, because it entails a gross violation of the second law of thermodynamics (huge amounts of energy spontaneously being converted from a colder to a hotter form), which is one of the most solidly established of all physical laws.

The energy problem has also been considered in relation to the idea of mass accretion in connection with the Expanding Earth theory. Among the early theorists to link mass increase in some sort of push gravity model to Earth expansion were Yarkovsky and Hilgenberg. [Citation | editor=Scalera, G. and Jacob, K.-H. | title =Why expanding Earth? – A book in honour of O.C. Hilgenberg | year =2003 | place=Rome | publisher= INGV] The idea of mass accretion and the expanding earth theory are not currently considered to be viable by mainstream scientists. This is because, among other reasons, according to the principle of mass-energy equivalence, if the Earth was absorbing the energy of the ultramundane flux at the rate necessary to produce the observed force of gravity (i.e. by using the values calculated by Poincaré), its mass would be doubling in each fraction of a second.

;Coupling to energyBased on observational evidence, it is now known that gravity interacts with all forms of energy, and not just with mass. The electrostatic binding energy of the nucleus, the energy of weak interactions in the nucleus, and the kinetic energy of electrons in atoms, all contribute to the gravitational mass of an atom, as has been confirmed to high precision in Eötvös type experiments. [Citation | author=Carlip, S. | title =Kinetic Energy and the Equivalence Principle | journal =Am. J. Phys. | volume =65 | pages =409–413 | year =1997 | url =http://arxiv.org/abs/gr-qc/9909014] This means, for example, that when the atoms of a quantity of gas are moving more rapidly, the gravitation of that gas increases. Le Sage's theory does not predict any such effect, nor does any of the known variants of Le Sage's theory.

Non-Gravitational applications and analogies

;Mock gravity
Lyman Spitzer in 1941 [cite journal | author=Spitzer, L. | authorlink=Lyman Spitzer | title=The dynamics of the interstellar medium; II. Radiation pressure | journal=The Astrophysical Journal | year=1941 | volume=94 | pages=232–244 | url=http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1941ApJ....94..232S | doi=10.1086/144328] calculated, that absorption of radiation between two dust particles lead to a net attractive force which varies proportional to 1/r² (evidently he was unaware of Le Sage's shadow mechanism and especially Lorentz's considerations on radiation pressure and gravity). George Gamow, who called this effect "mock gravity", proposed in 1949 [cite journal | author=Gamow, George | authorlink=George Gamow | title=On relativistic cosmogony | journal=Reviews of modern physics | year=1949 | volume=21 | pages=367–373 | doi= 10.1103/RevModPhys.21.367] that after the big bang the temperature of the electrons has dropped faster than the temperature of the background radiation. Absorption of the radiation lead to a Lesage mechanism between the electrons, which might had an important role in the process of galaxy formation shortly after the big bang. However, this proposal was disproved by Field in 1971 [cite journal | author=Field, G. B. | title=Instability and waves driven by radiation in interstellar space and in cosmological models | journal=The Astrophysical Journal | year=1971 | volume=165 | pages=29–40
url=http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ApJ...165...29F | doi=10.1086/150873
] , who showed that this effect was much too small, because electrons and the radiation were nearly in thermal equilibrium. Hogan and White proposed in 1986 [cite journal | author=Hogan, C.J. | title=Mock gravity and cosmic structure | journal=The Astrophysical Journal | year=1989 | volume=340 | pages=1–10 | url=http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ApJ...340....1H | doi=10.1086/167371] that mock gravity might have influenced the galaxy formation by absorption of pregalactic starlight. But it was shown by Wang and Field [cite journal | author=Wang, B. and Field, G.B. | title=Galaxy formation by mock gravity with dust? | journal=The Astrophysical Journal | year=1989 | volume=346 | pages=3–11 | url=http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ApJ...346....3W | doi=10.1086/167981] that any form of mock gravity is incapable of producing enough force to influence the galaxy formation.

;PlasmaThe Le Sage mechanism also has been identified as a significant factor in the behavior of dusty plasma. A.M. Ignatov [cite journal | author=Ignatov, A.M. | title=Lesage gravity in dusty plasma | journal=Plasma Physics Reports | year=1996 | volume=22 | issue=7 | pages=585–589] has shown that an attractive force arises between two dust grains suspended in an isotropic collisionless plasma due to inelastic collisions between ions of the plasma and the grains of dust. This attractive force is inversely proportional to the square of the distance between dust grains, and can counterbalance the Coulomb repulsion between dust grains.

;Vacuum energyIn quantum field theory the existence of virtual particles is proposed, which lead to the so called Casimir effect. Casimir calculated that between two plates only particles with specific wavelengths should be counted when calculating the vacuum energy. Therefore the energy density between the plates is less if the plates are close together, leading to a net attractive force between the plates. However, the conceptual framework of this effect is very different from the theory of Fatio and Le Sage.

Recent activity

The re-examination of Le Sage's theory in the 19th century identified several closely interconnected problems with the theory. These relate to excessive heating, frictional drag, shielding, and gravitational aberration. The recognition of these problems, in conjunction with a general shift away from mechanical based theories, resulted in a progressive loss of interest in Le Sage’s theory. Ultimately in the twentieth century Le Sage’s theory was eclipsed by Einstein’s theory of general relativity.

In 1965 Richard Feynman examined the Fatio/Lesage mechanism, primarily as an example of an attempt to explain a "complicated" physical law (in this case, Newton's inverse-square law of gravity) in terms of simpler primitive operations without the use of complex mathematics, and also as an example of a failed theory. He notes that the mechanism of "bouncing particles" reproduces the inverse-square force law and that "the strangeness of the mathematical relation will be very much reduced", but then notes that the scheme "does not work", because of the drag it predicts would be experienced by moving bodies, "so that is the end of that theory". [Citation | author=Feynman, R. P. | author-link =Richard Feynman | title = The Character of Physical Law, The 1964 Messenger Lectures | pages =37–39 | year =1967 | isbn=0-262-56003-8 ]

Although it is not regarded as a viable theory within the mainstream scientific community, there are occasional attempts to re-habilitate the theory outside the mainstream, including those of Radzievskii and Kagalnikova (1960), [Citation | author=Radzievskii, V.V. and Kagalnikova, I.I. | title =The nature of gravitation | journal =Vsesoyuz. Astronom.-Geodezich. Obsch. Byull. | volume =26 | issue =33 | pages =3–14 | year =1960 A rough English translation appeared in a U.S. government technical report: FTD TT64 323; TT 64 11801 (1964), Foreign Tech. Div., Air Force Systems Command, Wright-Patterson AFB, Ohio (reprinted in "Pushing Gravity")] Shneiderov (1961), [Citation | author=Shneiderov, A. J. | title =On the internal temperature of the earth | journal =Bollettino di Geofisica Teorica ed Applicata | volume =3 | pages =137–159 | year =1961] Buonomano and Engels (1976), [Citation | author=Buonomano, V. & Engel, E. | title =Some speculations on a causal unification of relativity, gravitation, and quantum mechanics | journal =Int. J. Theor. Phys. | volume =15 | pages =231–246 | year =1976 | doi=10.1007/BF01807095] Adamut (1982), [Citation | author=Adamut, I. A. | title =The screen effect of the earth in the TETG. Theory of a screening experiment of a sample body at the equator using the earth as a screen | journal =Nuovo Cimento C | volume =5 | pages =189–208 | year =1982 | doi=10.1007/BF02509010] Jaakkola (1996), [Citation | author=Jaakkola, T. | title =Action-at-a-distance and local action in gravitation: discussion and possible solution of the dilemma | journal =Apeiron | volume =3 | issue=3-4 | pages =61–75 | year =1996 | url =http://redshift.vif.com/JournalFiles/Pre2001/V03NO3PDF/V03N3JAA.PDF] Tom Van Flandern (1999), [Citation | author=Van Flandern, T. | author-link =Tom Van Flandern | title =Dark Matter, Missing Planets and New Comets | edition = 2 | pages =Chapters 2–4 | year =1999 | place =Berkeley | publisher=North Atlantic Books ] and Edwards (2007). [Citation | author=Edwards, M .R. | title =Photon-Graviton Recycling as Cause of Gravitation | journal =Apeiron | volume =14 | issue=3| pages =214–233 | year =2007 | url =http://redshift.vif.com/JournalFiles/V14NO3PDF/V14N3EDW.PDF] A variety of Le Sage models and related topics are discussed in Edwards, et al. [Citation | editor=Edwards, M. R.| title =Pushing Gravity: New Perspectives on Le Sage's Theory of Gravitation | place=Montreal | publisher =C. Roy Keys Inc. | year =2002]

Primary sources

econdary sources

* English summary of Prévost (1805).

External links

* Mathpages: [http://www.mathpages.com/home/kmath131/kmath131.htm LeSage's Shadows] , [http://www.mathpages.com/home/kmath426/kmath426.htm Omni-Directional Flux] , [http://www.mathpages.com/home/kmath610/kmath610.htm Kinetic Pressure and Tetrode’s Star] , [http://www.mathpages.com/home/kmath041/kmath041.htm Nicolas Fatio and the Cause of Gravity] , [http://www.mathpages.com/home/kmath181/kmath181.htm Fatio, Le Sage and the camisards] , [http://www.mathpages.com/home/kmath209/kmath209.htm Historical Assessments of the Fatio-Lesage Theory]

* Halton Arp: [http://www.haltonarp.com/articles/the_observational_impetus_for_le_sage_gravity The Observational Impetus for Le Sage Gravity]
* Auffray, J.-P.: [http://arxiv.org/abs/physics/0611300 Preston on E=mc²] and [http://arxiv.org/abs/physics/0608289 Dual origin of E=mc²]
* Borg Xavier : [http://blazelabs.com/f-g-intro.asp Electromagnetic radiation pressure (EMRP) gravity theory - Blaze Labs Research]
* Buonomano, V.: [http://arxiv.org/abs/physics/0210032 Co-Operative Phenomena as a Physical Paradigm for Special Relativity, Gravitation and Quantum Mechanics]
* Edwards, et al.: [http://redshift.vif.com/BookBlurbs/PushingGravity.htm Pushing Gravity]
* Mingst, B. & Stowe, P.: [http://www.mountainman.com.au/le_sage.htm Derivation of Newtonian Gravitation from LeSage's Attenuation]
* Popescu, I.I.: [http://www.geocities.com/iipopescu/ether_and_etherons.html Ether and Etherons]
* Tom Van Flandern: [http://www.metaresearch.org/cosmology/gravity/possiblenewpropertiesofgravity.asp Possible new properties of gravity]

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  • Gravitation — hält die Planeten auf ihren Bahnen um die Sonne (nicht maßstabsgetreu) Die Gravitation (von lateinisch gravitas, Schwere), ist eine der vier Grundkräfte der Physik. Sie bewirkt die gegenseitige Anziehung von Massen. Gravitation besitzt… …   Deutsch Wikipedia

  • Le-Sage-Gravitation — Die Le Sage Gravitation ist eine einfache mechanische Gravitationserklärung, die das Gravitationsgesetz von Newton begründen sollte. Sie wurde von Nicolas Fatio de Duillier (1690) und Georges Louis Le Sage (1748) entworfen. Da Fatios Arbeit… …   Deutsch Wikipedia

  • LeSage-Gravitation — Die Le Sage Gravitation ist eine einfache mechanische Gravitationserklärung, die das Gravitationsgesetz von Newton begründen sollte. Sie wurde von Nicolas Fatio de Duillier (1690) und Georges Louis Le Sage (1748) entworfen. Da Fatios Arbeit… …   Deutsch Wikipedia

  • Le Sage-Gravitation — Die Le Sage Gravitation ist eine einfache mechanische Gravitationserklärung, die das Gravitationsgesetz von Newton begründen sollte. Sie wurde von Nicolas Fatio de Duillier (1690) und Georges Louis Le Sage (1748) entworfen. Da Fatios Arbeit… …   Deutsch Wikipedia

  • Georges-Louis Le Sage — (* June 13, 1724 in Geneva, † November 9 1803 in Geneva) was a physicist and is most known for his theory of gravitation, for his invention of an electric telegraph and his anticipation of the kinetic theory of gases. Life and education Le Sage… …   Wikipedia

  • Teoría de la gravitación de Le Sage — La Teoría de la gravitación de Le Sage, referida también con el nombre de teoría cinética de la gravitación fue concebida originariamente por Nicolas Fatio de Duillier en 1690 y desarrollada ulteriormente por Georges Louis Le Sage en 1748. La… …   Wikipedia Español

  • Mechanical explanations of gravitation — (or kinetic theories of gravitation) are attempts to explain the action of gravity by aid of basic mechanical processes, such as pressure forces caused by pushes, and without the use of any action at a distance. These theories were developed from …   Wikipedia

  • Georges-Louis Le Sage — (* 13. Juni 1724 in Genf; † 9. November 1803 ebenda), war ein Genfer Physiker und Lehrer der Mathematik. Er ist bekannt geworden durch die nach ihm benannte Le Sage Gravitation, für seine Erfindung eines der ers …   Deutsch Wikipedia

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