History of gravitational theory
In physics, theories of gravitation postulate mechanisms of interaction governing the movements of bodies with mass. There have been numerous theories of gravitation since ancient times. Greek philosopher Aristotle (f. 4th century BC) believed that objects tend toward a point due to their inner gravitas (heaviness). Vitruvius (f. 1st century BC) understood that objects fall based on their specific gravity. 5th/6th-century AD Indian mathematician Aryabhata developed a geocentric model incorporating gravity; in the 7th century, Brahmagupta spoke of gravity as an attractive force.
The Aristotelian concept of gravity began to be rejected, initially by Islamic physicists, starting in the 11th century with Ibn Sina's theory of impetus. The following century, Abu'l-Barakāt al-Baghdādī explained gravitational acceleration, describing it as the acceleration of falling bodies by the accumulation of successive increments of power with successive increments of velocity. The works of Ibn Sina and al-Baghdādī were translated into Latin by the 14th century, influencing Jean Buridan and Albert of Saxony. The same century, Oxford's Merton College developed the mean speed theorem.
In the early 17th century, Galileo Galilei found that all objects tend to accelerate equally in free fall. In 1632, he put forth the basic principle of relativity. The existence of the gravitational constant was explored by various researchers from the mid-17th century, helping Isaac Newton formulate his law of universal gravitation. Newton's classical mechanics were superseded in the early 20th century, when Albert Einstein developed the special and general theory of relativity. The force carrier of gravity remains an outlier in the search for a theory of everything, which various models of quantum gravity are candidates for.
Various ancient texts such as the Bible describe some of the everyday effects of gravity; some religious scholars interpret particular scriptures as describing the cosmic force of gravity while not explicitly naming it as such.
In the 4th century BC, the Greek philosopher Aristotle taught that there is no effect or motion without a cause. The cause of the downward motion of heavy bodies, such as the element earth, was related to their nature, which caused them to move downward toward the centre of the universe, which was their natural place. Conversely, light bodies such as the element fire, move by their nature upward toward the inner surface of the sphere of the Moon. Thus in Aristotle's system heavy bodies are not attracted to the Earth by an external force, but tend toward the centre of the universe because of an inner gravitas or heaviness.
The 3rd-century-BC Greek physicist Archimedes discovered the centre of mass of a triangle. He also postulated that if the centres of gravity of two equal weights was not the same, it would be located in the middle of the line that joins them. Two centuries later, the Roman engineer and architect Vitruvius contended in his De architectura that gravity is not dependent on a substance's weight but rather on its 'nature' (cf. specific gravity):
If the quicksilver is poured into a vessel, and a stone weighing one hundred pounds is laid upon it, the stone swims on the surface, and cannot depress the liquid, nor break through, nor separate it. If we remove the hundred pound weight, and put on a scruple of gold, it will not swim, but will sink to the bottom of its own accord. Hence, it is undeniable that the gravity of a substance depends not on the amount of its weight, but on its nature.
In the 6th century, the Byzantine Alexandrian scholar John Philoponus proposed the theory of impetus, which modifies Aristotle's theory that "continuation of motion depends on continued action of a force" by incorporating a causative force which diminishes over time.
Indian mathematician/astronomer Aryabhata (476–550) first identified the force which explains why the Earth's rotation does not cause objects to spin away from it, and developed a geocentric solar system of gravitation. This features an eccentric elliptical model of the planets, where the planets spin on their axes and follow elliptical orbits, the Sun and the Moon revolving around the Earth in epicycles. Indian astronomer and mathematician Brahmagupta (c. 598–c. 668) described gravity as an attractive force and used the term "gurutvākarṣaṇam (गुरुत्वाकर्षणम्)" to describe it.Al-Hamdānī and Al-Biruni quote Brahmagupta as saying:
Disregarding this, we say that the earth on all its sides is the same; all people on the earth stand upright, and all heavy things fall down to the earth by a law of nature, for it is the nature of the earth to attract and to keep things, as it is the nature of water to flow, that of fire to burn, and that of the wind to set in motion. If a thing wants to go deeper down than the earth, let it try. The earth is the only low thing, and seeds always return to it, in whatever direction you may throw them away, and never rise upwards from the earth.
In the 11th century, Persian polymath Ibn Sina (Avicenna) agreed with Philoponus' theory that "the moved object acquires an inclination from the mover" as an explanation for projectile motion. Ibn Sina then published his own theory of impetus in The Book of Healing (c. 1020). Unlike Philoponus, who believed that it was a temporary virtue that would decline even in a vacuum, Ibn Sina viewed it as a persistent, requiring external forces such as air resistance to dissipate it. Ibn Sina made distinction between 'force' and 'inclination' (mayl), and argued that an object gained mayl when the object is in opposition to its natural motion. So he concluded that continuation of motion is attributed to the inclination that is transferred to the object, and that object will be in motion until the mayl is spent. He also claimed that a projectile in a vacuum would not stop unless acted upon, dissenting from the Aristotelian view.
Another 11th-century Persian polymath, Al-Biruni, proposed that heavenly bodies have mass, weight, and gravity, just like the Earth. He criticized both Aristotle and Ibn Sina for holding the view that heavenly bodies lack these properties and that only the Earth has mass, weight and gravity. The 12th-century scholar Al-Khazini suggested that the gravity an object contains varies depending on its distance from the centre of the universe (referring to the centre of the Earth). Al-Biruni and Al-Khazini studied the theory of the centre of gravity, and generalized and applied it to three-dimensional bodies. They also founded the theory of ponderable lever, and created the science of gravity. Fine experimental methods were also developed for determining the specific gravity or specific weight of objects, based the theory of balances and weighing.
In the 12th century, Abu'l-Barakāt al-Baghdādī adopted and modified Avicenna's theory on projectile motion. In his Kitab al-Mu'tabar, Abu'l-Barakat stated that the mover imparts a violent inclination (mayl qasri) on the moved and that this diminishes as the moving object distances itself from the mover. He also gave an explanation for the gravitational acceleration of falling bodies. He proposed an explanation of the acceleration of falling bodies by the accumulation of successive increments of power with successive increments of velocity. According to Shlomo Pines, al-Baghdādī's theory of motion was "the oldest negation of Aristotle's fundamental dynamic law [namely, that a constant force produces a uniform motion], [and is thus an] anticipation in a vague fashion of the fundamental law of classical mechanics [namely, that a force applied continuously produces acceleration]."
The 12th-century Arab polymath Ibn Bajjah proposed that for every force there is always a reaction force. While he did not specify that these forces be equal, it was an early version of the third law of motion which states that for every action there is an equal and opposite reaction. In the 16th century, Al-Birjandi explained the Earth's rotation by developing a hypothesis similar to Galileo Galilei's notion of circular inertia, which he described in an observational test.
In the 14th century, both the French philosopher Jean Buridan and the Merton College of Oxford rejected the Aristotelian concept of gravity.[a] They attributed the motion of objects to an impetus (akin to momentum), which varies according to velocity and mass; Buridan was influenced in this by Ibn Sina's Book of Healing. Buridan and Albert of Saxony (c. 1320–1390) adopted Abu'l-Barakat's theory that the acceleration of a falling body is a result of its increasing impetus. Influenced by Buridan, Albert developed a square law regarding the relationship between the speed of an object in free fall and either the time or space elapsed. He also theorized that mountains and valleys are caused by erosion[b]—displacing the Earth's centre of gravity.[c] Also in this century, the Merton College developed the mean speed theorem, which was proved by Nicole Oresme (c. 1323–1382) and would be influential in later gravitational equations.
Leonardo da Vinci (1452–1519) wrote that the "mother and origin of gravity" is energy. He describes two pairs of physical powers which stem from a metaphysical origin and have an effect on everything: abundance of force and motion, and gravity and resistance. He associates gravity with the 'cold' classical elements, water and earth, and calls its energy infinite. Leonardo did not publish his manuscripts and they had no direct influence on subsequent science. By 1514, Nicolaus Copernicus had written an outline of his heliocentric model, in which he recognized Earth's centre as the centre of both its revolution and the Moon's orbit; his full theory was published in 1534. In 1533, German humanist Petrus Apianus described the exertion of gravity:[d]
Since it is apparent that in the descent [along the arc] there is more impediment acquired, it is clear that gravity is diminished on this account. But because this comes about by reason of the position of heavy bodies, let it be called a positional gravity [i.e. gravitas secundum situm]
Galileo Galilei derived his kinematics from the 14th-century Merton College and Jean Buridan. In the early 17th century, Galileo found that, counter to Aristotle's teachings, all objects in free fall tend to accelerate equally in relation to the duration of their fall. In a 1604 letter to Paolo Sarpi, Galileo correctly hypothesized that the distance of a falling object is proportional to the square of the time elapsed.[f] His Dialogue Concerning the Two Chief World Systems (1632) reiterates the aforementioned theory and puts forth the basic principle of relativity. The latter establishes that the laws of physics are the same in any system moving at a constant speed in a continuous direction.[g] A disciple of Galileo, Evangelista Torricelli reiterated Aristotle's model involving a gravitational centre, adding his view that a system can only be in equilibrium when the common centre itself is unable to fall.
The relation of the distance of objects in free fall to the square of the time taken was confirmed by Francesco Maria Grimaldi and Giovanni Battista Riccioli between 1640 and 1650. They also made a calculation of the gravitational constant by recording the oscillations of a pendulum.
In 1644, René Descartes proposed that no empty space can exist; a continuum of matter would cause every motion to be curvilinear. Centrifugal force causes refined matter to lift away from a central vortex, where crude objects remain due to inertia.[h] In 1671, Robert Hooke speculated that gravitation is the result of bodies emitting waves in the aether.[i]Nicolas Fatio de Duillier (1690) and Georges-Louis Le Sage (1748) proposed a corpuscular model using some sort of screening or shadowing mechanism. In 1784, Le Sage posited that gravity could be a result of the collision of atoms, and in the early 19th century, he expanded Daniel Bernoulli's theory of corpuscular pressure to the universe as a whole. A similar model was later created by Hendrik Lorentz (1853–1928), who used electromagnetic radiation instead of corpuscles.
English mathematician Isaac Newton utilized Descartes' argument that curvilinear motion constrains inertia, and in 1675, argued that aether streams attract all bodies to one another.[j] Newton (1717) and Leonhard Euler (1760) proposed a model in which the aether loses density near mass, leading to a net force acting on bodies. Mechanistic models fell out of favor because most of them lead to an unacceptable amount of drag, which was not observed. Others violate the energy conservation law and are incompatible with modern thermodynamics.
As a result of Robert Hooke's suggestion that there is a gravitational force which depends on the inverse square of the distance, Isaac Newton was able to mathematically derive Kepler's three kinematic laws of planetary motion, including the elliptical orbits for the six then-known planets and the Moon. To prove his inverse-square law, he needed an accurate measure of the gravitational constant. This was first performed by Henry Cavendish in 1797.[k]
In 1687, Newton published Philosophiæ Naturalis Principia Mathematica, which hypothesizes the inverse-square law of universal gravitation. In his own words:
I deduced that the forces which keep the planets in their orbs must be reciprocally as the squares of their distances from the centres about which they revolve; and thereby compared the force requisite to keep the moon in her orb with the force of gravity at the surface of the earth; and found them to answer pretty nearly.
Newton's original formula was:
where the symbol means "is proportional to". To make this into an equal-sided formula or equation, there needed to be a multiplying factor or constant that would give the correct force of gravity no matter the value of the masses or distance between them. This gravitational constant was first accurately measured in 1797 by Henry Cavendish.[k]
Newton's theory enjoyed its greatest success when it was used to predict the existence of Neptune based on motions of Uranus that could not be accounted by the actions of the other planets. Calculations by John Couch Adams and Urbain Le Verrier both predicted the general position of the planet. Le Verrier's sent his position to Johann Gottfried Galle, asking him to verify; in the same night, Galle spotted Neptune near the position Le Verrier had predicted.
Years later, it was another discrepancy in a planet's orbit that showed Newton's theory to be inaccurate. By the end of the 19th century, it was known that the orbit of Mercury could not be accounted for entirely under Newtonian gravity, and all searches for another perturbing body (such as a planet orbiting the Sun even closer than Mercury) were fruitless. This issue was resolved in 1915 by Einstein's general theory of relativity, which accounted for the discrepancy in Mercury's orbit, thereby superseding Newton's theory. However, most modern non-relativistic gravitational calculations still use Newton's equations because they are easier to work with and sufficiently accurate for many everyday applications.
In the late 19th century, Lord Kelvin pondered the possibility of a theory of everything. He proposed that every body pulsates, which might be an explanation of gravitation and electric charges. However, his ideas were largely mechanistic and required the existence of the aether, which the Michelson–Morley experiment failed to detect in 1887. This, combined with Mach's principle, led to gravitational models which feature action at a distance.
In 1905, Albert Einstein published a series of papers in which he established the special theory of relativity and the fact that mass and energy are equivalent. In 1907, in what he described as "the happiest thought of my life", Einstein realized that someone who is in free fall experiences no gravitational field. In other words, gravitation is exactly equivalent to acceleration. Between 1911 and 1915, Einstein developed this idea, initially stated as the equivalence principle, into his general theory of relativity, which fuses the three dimensions of space and the one dimension of time into the four-dimensional fabric of spacetime. However, it does not unify gravity with quanta—individual particles of energy, which Einstein himself had postulated the existence of in 1905.
In 1914, Gunnar Nordström attempted to unify gravity and electromagnetism in his theory of five-dimensional gravitation.[l] This was superseded by general relativity in 1919, when gravitational lensing around a solar eclipse was observed by Arthur Eddington. Thereafter, German mathematician Theodor Kaluza promoted the idea of general relativity with a fifth dimension, which in 1921 Swedish physicist Oskar Klein gave a physical interpretation of in a prototypical string theory, a possible model of quantum gravity and potential theory of everything.
Einstein's field equations include a cosmological constant to account for the alleged staticity of the universe. However, Edwin Hubble observed in 1929 that the universe appears to be expanding. By the 1930s, Paul Dirac developed the hypothesis that gravitation should slowly and steadily decrease over the course of the history of the universe. Alan Guth and Alexei Starobinsky proposed in 1980 that cosmic inflation in the very early universe could have been driven by a negative pressure field, a concept later coined 'dark energy'—found in 2013 to have composed around 68.3% of the early universe.
In 1922, Jacobus Kapteyn proposed the existence of dark matter, an unseen force that moves stars in galaxies at higher velocities than gravity alone accounts for. It was found in 2013 to have comprised 26.8% of the early universe. Along with dark energy, dark matter is an outlier in Einstein's relativity, and an explanation for its apparent effects is a requirement for a successful theory of everything.
In 1957, Hermann Bondi proposed that negative gravitational mass (combined with negative inertial mass) would comply with the strong equivalence principle of general relativity and Newton's laws of motion. Bondi's proof yielded singularity-free solutions for the relativity equations.
In general relativity, the effects of gravitation are ascribed to spacetime curvature instead of to a force. The starting point for general relativity is the equivalence principle, which equates free fall with inertial motion. The issue that this creates is that free-falling objects can accelerate with respect to each other. To deal with this difficulty, Einstein proposed that spacetime is curved by matter, and that free-falling objects are moving along locally straight paths in curved spacetime. More specifically, Einstein and David Hilbert discovered the field equations of general relativity, which relate the presence of matter and the curvature of spacetime. These field equations are a set of 10 simultaneous, non-linear, differential equations. The solutions of the field equations are the components of the metric tensor of spacetime, which describes its geometry. The geodesic paths of spacetime are calculated from the metric tensor.
Notable solutions of the Einstein field equations include:
- The Schwarzschild solution, which describes spacetime surrounding a spherically symmetrical non-rotating uncharged massive object. For objects with radii smaller than the Schwarzschild radius, this solution generates a black hole with a central singularity.
- The Reissner–Nordström solution, in which the central object has an electrical charge. For charges with a geometrized length less than the geometrized length of the mass of the object, this solution produces black holes with an event horizon surrounding a Cauchy horizon.
- The Kerr solution for rotating massive objects. This solution also produces black holes with multiple horizons.
- The cosmological Robertson–Walker solution, which predicts the expansion of the universe.
General relativity has enjoyed much success because its predictions (not called for by older theories of gravity) have been regularly confirmed. For example:
- General relativity accounts for the anomalous perihelion precession of Mercury.
- Gravitational lensing was first confirmed in 1919, and has more recently been strongly confirmed through the use of a quasar which passes behind the Sun as seen from the Earth.
- The expansion of the universe (predicted by the Robertson–Walker metric) was confirmed by Edwin Hubble in 1929.
- The prediction that time runs slower at lower potentials has been confirmed by the Pound–Rebka experiment, the Hafele–Keating experiment, and the GPS.
- The time delay of light passing close to a massive object was first identified by Irwin Shapiro in 1964 in interplanetary spacecraft signals.
- Gravitational radiation has been indirectly confirmed through studies of binary pulsars such as PSR 1913+16.
Several decades after the discovery of general relativity, it was realized that it cannot be the complete theory of gravity because it is incompatible with quantum mechanics. Later it was understood that it is possible to describe gravity in the framework of quantum field theory like the other fundamental forces. In this framework, the attractive force of gravity arises due to exchange of virtual gravitons, in the same way as the electromagnetic force arises from exchange of virtual photons. This reproduces general relativity in the classical limit, but only at the linearized level and postulating that the conditions for the applicability of Ehrenfest theorem holds, which is not always the case. Moreover, this approach fails at short distances of the order of the Planck length.
Theoretical models such as string theory and loop quantum gravity are current candidates for a possible 'theory of everything'.
- This was interpreted as deriving the weight of objects from the pressure of the air below them.
- Leonardo da Vinci tested this theory by observing trace fossils, which he used to argue against the myth of a universal flood.
- Furthermore, he hypothesized that the planet is in equilibrium when its centre of gravity coincides with that of its mass.
- Physicist Pierre Duhem erroneously attributes this to Jordanus Nemorarius, whom he calls the "precursor of Leonardo". Leonardo alludes to Jordanus in his notebooks, but not to any of his theories.
- Some historians consider this to have been a thought experiment rather than a physical test as there is little evidence that it actually took place.
- The distance traversed in successive equal intervals of time is calculated with a triangular model whose width (representing maximum velocity) increases by two for every equal section of height (representing time elapsed). This is in part anticipated by the Merton rule.
- This principle provided the basic framework for Newton's laws of motion and is central to Einstein's special theory of relativity.
- Christiaan Huygens utilized aspects of Descartes' theory in 1690.
- James Challis repeated this assumption in 1869.
- Bernhard Riemann made a similar argument in 1853.
- Many sources incorrectly state that this was the first measurement of G (or the Earth's density). There were previous measurements, chiefly by Bouguer (1740) and Maskelyne (1774), but they were very inaccurate.
- In string theory, dimensions exceeding four allow for the existence of parallel realities—which along with the anthropic principle, help to explain the statistical near-impossibility of our fine-tuned universe.
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Using a whole body of mathematical methods (not only those inherited from the antique theory of ratios and infinitesimal techniques, but also the methods of the contemporary algebra and fine calculation techniques), Muslim scientists raised statics to a new, higher level. The classical results of Archimedes in the theory of the centre of gravity were generalized and applied to three-dimensional bodies, the theory of ponderable lever was founded and the 'science of gravity' was created and later further developed in medieval Europe. The phenomena of statics were studied by using the dynamic approach so that two trends – statics and dynamics – turned out to be inter-related within a single science, mechanics. The combination of the dynamic approach with Archimedean hydrostatics gave birth to a direction in science which may be called medieval hydrodynamics. [...] Numerous fine experimental methods were developed for determining the specific weight, which were based, in particular, on the theory of balances and weighing. The classical works of al-Biruni and al-Khazini can by right be considered as the beginning of the application of experimental methods in medieval science.
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Force arises from dearth or abundance; it is the child of physical motion, and the grandchild of spiritual motion, and the mother and origin of gravity. Gravity is limited to the elements of water and earth; but his force is unlimited, and by it infinite worlds might be moved if instruments could be made by which the force be generated.
Force, with physical motion, and gravity, with resistance, are the four external powers on which all actions of mortals depend.
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Der englische Physiker und Nobelpreisträger Dirac hat ... vor über dreißig Jahren die Vermutung begründet, dass sich das universelle Maß der Schwerkraft im Laufe der Geschichte des Universums außerordentlich langsam, aber stetig verringert." English: "The English physicist and Nobel laureate Dirac has ..., more than thirty years ago, substantiated the assumption that the universal strength of gravity decreases very slowly, but steadily over the course of the history of the universe.
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