The following is a
timeline of
gravitational physics
In physics, gravity () is a fundamental interaction which causes mutual attraction between all things with mass or energy. Gravity is, by far, the weakest of the four fundamental interactions, approximately 1038 times weaker than the strong ...
and
general relativity.
Before 1500
* 3rd century BC -
Aristarchus of Samos
Aristarchus of Samos (; grc-gre, Ἀρίσταρχος ὁ Σάμιος, ''Aristarkhos ho Samios''; ) was an ancient Greek astronomer and mathematician who presented the first known heliocentric model that placed the Sun at the center of the k ...
proposes heliocentric model, measures the distance to the Moon and its size
1500s
* 1543 – Nicolaus Copernicus places the Sun at the gravitational center, starting a revolution in science
* 1583 –
Galileo Galilei induces the period relationship of a
pendulum
A pendulum is a weight suspended from a pivot so that it can swing freely. When a pendulum is displaced sideways from its resting, equilibrium position, it is subject to a restoring force due to gravity that will accelerate it back toward the ...
from observations (according to later biographer).
* 1586 –
Simon Stevin demonstrates that two objects of different mass accelerate at the same rate when dropped.
* 1589 – Galileo Galilei describes a
hydrostatic balance
In fluid mechanics, hydrostatic equilibrium (hydrostatic balance, hydrostasy) is the condition of a fluid or plastic solid at rest, which occurs when external forces, such as gravity, are balanced by a pressure-gradient force. In the planetary ...
for measuring
specific gravity.
* 1590 – Galileo Galilei formulates modified
Aristotelean theory of motion (later retracted) based on
density rather than weight of objects.
1600s
* 1602 – Galileo Galilei conducts experiments on pendulum motion.
* 1604 – Galileo Galilei conducts experiments with
inclined planes and induces the law of falling objects.
* 1607 – Galileo Galilei derives a mathematical formulation of the law of falling objects based on his earlier experiments.
* 1608 – Galileo Galilei discovers the
parabolic arc of
projectile
A projectile is an object that is propelled by the application of an external force and then moves freely under the influence of gravity and air resistance. Although any objects in motion through space are projectiles, they are commonly found in ...
s through experiment.
* 1609 –
Johannes Kepler describes the motion of planets around the Sun, now known as
Kepler's laws of planetary motion
In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbit ...
.
* 1640 –
Ismaël Bullialdus suggests an inverse-square gravitational force law.
* 1665 –
Isaac Newton introduces an inverse-square
universal law of gravitation uniting terrestrial and celestial theories of motion and uses it to predict the orbit of the
Moon and the parabolic arc of projectiles.
* 1684 – Isaac Newton proves that
planets moving under an inverse-square force law will obey
Kepler's laws
In astronomy, Kepler's laws of planetary motion, published by Johannes Kepler between 1609 and 1619, describe the orbits of planets around the Sun. The laws modified the heliocentric theory of Nicolaus Copernicus, replacing its circular orbi ...
* 1686 – Isaac Newton uses a fixed length
pendulum
A pendulum is a weight suspended from a pivot so that it can swing freely. When a pendulum is displaced sideways from its resting, equilibrium position, it is subject to a restoring force due to gravity that will accelerate it back toward the ...
with weights of varying composition to test the
weak equivalence principle
In the theory of general relativity, the equivalence principle is the equivalence of gravitational and inertial mass, and Albert Einstein's observation that the gravitational "force" as experienced locally while standing on a massive body (suc ...
to 1 part in 1000
1700s
* 1798 –
Henry Cavendish measures the force of gravity between two masses, leading to the first accurate value for the
gravitational constant
1800s
* 1846 –
Urbain Le Verrier
Urbain Jean Joseph Le Verrier FRS (FOR) HFRSE (; 11 March 1811 – 23 September 1877) was a French astronomer and mathematician who specialized in celestial mechanics and is best known for predicting the existence and position of Neptune using ...
and
John Couch Adams, studying
Uranus' orbit, independently prove that another, farther planet must exist.
Neptune was found at the predicted moment and position.
* 1855 – Le Verrier observes a 35 arcsecond per century excess
precession of
Mercury's
orbit and attributes it to another planet, inside Mercury's orbit. The planet was never found. See
Vulcan
Vulcan may refer to:
Mythology
* Vulcan (mythology), the god of fire, volcanoes, metalworking, and the forge in Roman mythology
Arts, entertainment and media Film and television
* Vulcan (''Star Trek''), name of a fictional race and their home p ...
.
* 1876 –
William Kingdon Clifford
William Kingdon Clifford (4 May 18453 March 1879) was an English mathematician and philosopher. Building on the work of Hermann Grassmann, he introduced what is now termed geometric algebra, a special case of the Clifford algebra named in hi ...
suggests that the motion of matter may be due to changes in the geometry of space
* 1882 –
Simon Newcomb
Simon Newcomb (March 12, 1835 – July 11, 1909) was a Canadian– American astronomer, applied mathematician, and autodidactic polymath. He served as Professor of Mathematics in the United States Navy and at Johns Hopkins University. Born in ...
observes a 43 arcsecond per century excess precession of Mercury's orbit
* 1887 –
Albert A. Michelson
Albert Abraham Michelson FFRS HFRSE (surname pronunciation anglicized as "Michael-son", December 19, 1852 – May 9, 1931) was a German-born American physicist of Polish/Jewish origin, known for his work on measuring the speed of light and espe ...
and
Edward W. Morley
Edward Williams Morley (January 29, 1838 – February 24, 1923) was an American scientist known for his precise and accurate measurement of the atomic weight of oxygen, and for the Michelson–Morley experiment.
Biography
Morley was born in New ...
in
their famous experiment do not detect the
ether
In organic chemistry, ethers are a class of compounds that contain an ether group—an oxygen atom connected to two alkyl or aryl groups. They have the general formula , where R and R′ represent the alkyl or aryl groups. Ethers can again b ...
drift
* 1889 –
Loránd Eötvös
Baron Loránd Eötvös de Vásárosnamény (or Loránd Eötvös, , '' hu, vásárosnaményi báró Eötvös Loránd Ágoston''; 27 July 1848 – 8 April 1919), also called Baron Roland von Eötvös in English literature, was a Hungarian physicist ...
uses a
torsion balance
A torsion spring is a spring that works by twisting its end along its axis; that is, a flexible elastic object that stores mechanical energy when it is twisted. When it is twisted, it exerts a torque in the opposite direction, proportional ...
to test the
weak equivalence principle
In the theory of general relativity, the equivalence principle is the equivalence of gravitational and inertial mass, and Albert Einstein's observation that the gravitational "force" as experienced locally while standing on a massive body (suc ...
to 1 part in one billion
* 1893 –
Ernst Mach states
Mach's principle
In theoretical physics, particularly in discussions of gravitation theories, Mach's principle (or Mach's conjecture) is the name given by Einstein to an imprecise hypothesis often credited to the physicist and philosopher Ernst Mach. The hypothe ...
; first constructive attack on the idea of Newtonian absolute space
* 1898 –
Henri Poincaré states that simultaneity is relative
* 1899 –
Hendrik Antoon Lorentz
Hendrik Antoon Lorentz (; 18 July 1853 – 4 February 1928) was a Dutch physicist who shared the 1902 Nobel Prize in Physics with Pieter Zeeman for the discovery and theoretical explanation of the Zeeman effect. He also derived the Lorentz t ...
published Lorentz transformations
1900s
* 1902 –
Paul Gerber explains the movement of the perihelion of Mercury using finite speed of gravity. His formula, at least approximately, matches the later model from Einstein's general relativity, but Gerber's theory was incorrect.
* 1904 –
Henri Poincaré presents the principle of relativity for
electromagnetism
In physics, electromagnetism is an interaction that occurs between particles with electric charge. It is the second-strongest of the four fundamental interactions, after the strong force, and it is the dominant force in the interactions of ...
* 1905 –
Albert Einstein
Albert Einstein ( ; ; 14 March 1879 – 18 April 1955) was a German-born theoretical physicist, widely acknowledged to be one of the greatest and most influential physicists of all time. Einstein is best known for developing the theory ...
completes his theory of
special relativity and states the
law of mass-energy conservation: E=mc
2
* 1907 –
Albert Einstein
Albert Einstein ( ; ; 14 March 1879 – 18 April 1955) was a German-born theoretical physicist, widely acknowledged to be one of the greatest and most influential physicists of all time. Einstein is best known for developing the theory ...
introduces the principle of equivalence of gravitation and inertia and uses it to predict the
gravitational redshift
In physics and general relativity, gravitational redshift (known as Einstein shift in older literature) is the phenomenon that electromagnetic waves or photons travelling out of a gravitational well (seem to) lose energy. This loss of energy ...
* 1915 –
Albert Einstein
Albert Einstein ( ; ; 14 March 1879 – 18 April 1955) was a German-born theoretical physicist, widely acknowledged to be one of the greatest and most influential physicists of all time. Einstein is best known for developing the theory ...
completes his theory of
general relativity. The new theory explains
Mercury's strange motions that baffled
Urbain Le Verrier
Urbain Jean Joseph Le Verrier FRS (FOR) HFRSE (; 11 March 1811 – 23 September 1877) was a French astronomer and mathematician who specialized in celestial mechanics and is best known for predicting the existence and position of Neptune using ...
.
* 1915 –
Karl Schwarzschild publishes the
Schwarzschild metric
In Einstein's theory of general relativity, the Schwarzschild metric (also known as the Schwarzschild solution) is an
exact solution to the Einstein field equations that describes the gravitational field outside a spherical mass, on the assumpti ...
about a month after Einstein published his general theory of relativity. This was the first solution to the Einstein field equations other than the trivial flat space solution.
* 1916 –
Albert Einstein
Albert Einstein ( ; ; 14 March 1879 – 18 April 1955) was a German-born theoretical physicist, widely acknowledged to be one of the greatest and most influential physicists of all time. Einstein is best known for developing the theory ...
shows that the field equations of general relativity admit wavelike solutions
* 1918 –
Josef Lense and
Hans Thirring
Hans Thirring (March 23, 1888 – March 22, 1976) was an Austrian theoretical physicist, professor, and father of the physicist Walter Thirring. He won the Haitinger Prize of the Austrian Academy of Sciences in 1920.
Together with the mathemat ...
find the gravitomagnetic precession of
gyroscopes in the equations of general relativity
* 1919 –
Arthur Eddington
Sir Arthur Stanley Eddington (28 December 1882 – 22 November 1944) was an English astronomer, physicist, and mathematician. He was also a philosopher of science and a populariser of science. The Eddington limit, the natural limit to the lumi ...
leads a
solar eclipse expedition which claims to detect gravitational deflection of light by the Sun
* 1921 –
Theodor Kaluza demonstrates that a five-dimensional version of Einstein's equations unifies
gravitation and
electromagnetism
In physics, electromagnetism is an interaction that occurs between particles with electric charge. It is the second-strongest of the four fundamental interactions, after the strong force, and it is the dominant force in the interactions of ...
* 1937 –
Fritz Zwicky states that
galaxies could act as
gravitational lenses
* 1937 – Albert Einstein,
Leopold Infeld
Leopold Infeld (20 August 1898 – 15 January 1968) was a Polish physicist who worked mainly in Poland and Canada (1938–1950). He was a Rockefeller fellow at Cambridge University (1933–1934) and a member of the Polish Academy of Sciences.
E ...
, and
Banesh Hoffmann show that the geodesic equations of general relativity can be deduced from its field equations
1950s
* 1953 –
P. C. Vaidya Newtonian time in general relativity, Nature, 171, p260.
* 1956 –
John Lighton Synge publishes the first relativity text emphasizing
spacetime diagrams and
geometrical methods,
* 1957 –
Felix A. E. Pirani uses
Petrov classification to understand
gravitational radiation,
* 1957 –
Richard Feynman
Richard Phillips Feynman (; May 11, 1918 – February 15, 1988) was an American theoretical physicist, known for his work in the path integral formulation of quantum mechanics, the theory of quantum electrodynamics, the physics of the superfl ...
introduces
sticky bead argument
In general relativity, the sticky bead argument is a simple thought experiment designed to show that gravitational radiation is indeed predicted by general relativity, and can have physical effects. These claims were not widely accepted prior to ab ...
,
* 1957 –
John Wheeler discusses the breakdown of classical general relativity near
singularities and the need for
quantum gravity
Quantum gravity (QG) is a field of theoretical physics that seeks to describe gravity according to the principles of quantum mechanics; it deals with environments in which neither gravitational nor quantum effects can be ignored, such as in the vi ...
* 1959 –
Pound–Rebka experiment
The Pound–Rebka experiment was an experiment in which gamma rays were emitted from the top of a tower and measured by a receiver at the bottom of the tower. The purpose of the experiment was to test Albert Einstein's theory of general relativit ...
, first precision test of gravitational redshift,
* 1959 – Lluís Bel introduces
Bel–Robinson tensor In general relativity and differential geometry, the Bel–Robinson tensor is a tensor defined in the abstract index notation by:
:T_=C_C_ ^ _ ^ + \frac\epsilon_^ \epsilon_^_ C_ C_^_^
Alternatively,
:T_ = C_C_ ^ _ ^ - \frac g_ C_ C^_^
where C_ is ...
and the
Bel decomposition of the
Riemann tensor
In the mathematical field of differential geometry, the Riemann curvature tensor or Riemann–Christoffel tensor (after Bernhard Riemann and Elwin Bruno Christoffel) is the most common way used to express the curvature of Riemannian manifolds. ...
,
* 1959 –
Arthur Komar introduces the
Komar mass,
* 1959 –
Richard Arnowitt,
Stanley Deser and
Charles W. Misner
Charles W. Misner (; born June 13, 1932) is an American physicist and one of the authors of ''Gravitation''. His specialties include general relativity and cosmology. His work has also provided early foundations for studies of quantum gravity an ...
developed
ADM formalism.
1960s
* 1960 –
Martin Kruskal
Martin David Kruskal (; September 28, 1925 – December 26, 2006) was an American mathematician and physicist. He made fundamental contributions in many areas of mathematics and science, ranging from plasma physics to general relativity and ...
and
George Szekeres
George Szekeres AM FAA (; 29 May 1911 – 28 August 2005) was a Hungarian–Australian mathematician.
Early years
Szekeres was born in Budapest, Hungary, as Szekeres György and received his degree in chemistry at the Technical University of ...
independently introduce the
Kruskal–Szekeres coordinates for the
Schwarzschild vacuum,
* 1960 –
Shapiro effect confirmed,
* 1960 – Thomas Matthews and
Allan R. Sandage
Allan Rex Sandage (June 18, 1926 – November 13, 2010) was an American astronomer. He was Staff Member Emeritus with the Carnegie Observatories in Pasadena, California. He determined the first reasonably accurate values for the Hubble const ...
associate
3C 48
3C48 is a quasar discovered in 1960; it was the second source conclusively identified as such.
3C48 was the first source in the Third Cambridge Catalogue of Radio Sources for which an optical identification was found by Allan Sandage and Thomas ...
with a point-like optical image, show radio source can be at most 15 light minutes in diameter,
* 1960 –
Carl H. Brans and
Robert H. Dicke introduce
Brans–Dicke theory, the first viable alternative theory with a clear physical motivation,
* 1960 –
Ivor M. Robinson and
Andrzej Trautman discover the Robinson-Trautman
null dust solution
* 1961 –
Pascual Jordan and
Jürgen Ehlers develop the ''kinematic decomposition'' of a
timelike congruence,
* 1960 –
Robert Pound and
Glen Rebka test the gravitational redshift predicted by the equivalence principle to approximately 1%
* 1962 –
Roger Penrose and
Ezra T. Newman introduce the
Newman–Penrose formalism,
* 1962 – Ehlers and
Wolfgang Kundt classify the symmetries of
Pp-wave spacetimes,
* 1962: –
Joshua Goldberg and
Rainer K. Sachs prove the
Goldberg–Sachs theorem
The Goldberg–Sachs theorem is a result in Einstein's theory of general relativity about vacuum solutions of the Einstein field equations relating the existence of a certain type of congruence with algebraic properties of the Weyl tensor.
More ...
,
* 1962 – Ehlers introduces
Ehlers transformations, a new
solution generating method,
* 1962 –
Cornelius Lanczos introduces the
Lanczos potential for the
Weyl tensor,
* 1962 –
Richard Arnowitt,
Stanley Deser, and
Charles W. Misner
Charles W. Misner (; born June 13, 1932) is an American physicist and one of the authors of ''Gravitation''. His specialties include general relativity and cosmology. His work has also provided early foundations for studies of quantum gravity an ...
introduce the
ADM reformulation and
global hyperbolicity,
* 1962 –
Yvonne Choquet-Bruhat
Yvonne Choquet-Bruhat (; born 29 December 1923) is a French mathematician and physicist. She has made seminal contributions to the study of Einstein's general theory of relativity, by showing that the Einstein equations can be put into the form ...
on Cauchy problem and global hyperbolicity,
* 1962 – Istvan Ozsvath and
Englbert Schücking rediscover the
circularly polarized monochromomatic gravitational wave,
* 1962 –
Hans Adolph Buchdahl discovers
Buchdahl's theorem,
* 1962 –
Hermann Bondi introduces
Bondi mass,
* 1962 –
Robert Dicke
Robert Henry Dicke (; May 6, 1916 – March 4, 1997) was an American astronomer and physicist who made important contributions to the fields of astrophysics, atomic physics, cosmology and gravity. He was the Albert Einstein Professor in Scien ...
,
Peter Roll, and
R. Krotkov use a torsion fiber balance to test the weak equivalence principle to 2 parts in 100 billion,
* 1962 -
Hermann Bondi, M. G. van der Burg, A. W. Metzner, and
Rainer K. Sachs introduce the
asymptotic symmetry group of
asymptotically flat, Lorentzian spacetimes at null (''i.e.'', light-like) infinity.
* 1963 –
Roy Kerr
Roy Patrick Kerr (; born 16 May 1934) is a New Zealand mathematician who discovered the Kerr geometry, an exact solution to the Einstein field equation of general relativity. His solution models the gravitational field outside an uncharged ...
discovers the
Kerr vacuum solution of
Einstein's field equations
In the general theory of relativity, the Einstein field equations (EFE; also known as Einstein's equations) relate the geometry of spacetime to the distribution of matter within it.
The equations were published by Einstein in 1915 in the for ...
,
* 1963 – Redshifts of
3C 273
3C 273 is a quasar located in the constellation of Virgo. It was the first quasar ever to be identified.
It is the optically brightest quasar in the sky from Earth ( m ~12.9), and one of the closest with a redshift, ''z'', of 0.158. A luminosi ...
and other quasars show they are very distant; hence very luminous,
* 1963 – Newman, T. Unti and L.A. Tamburino introduce the
NUT vacuum solution,
* 1963 –
Roger Penrose introduces
Penrose diagrams and
Penrose limits,
* 1963 – First
Texas Symposium on Relativistic Astrophysics held in Dallas, 16–18 December,
* 1964 – R. W. Sharp and Misner introduce the
Misner–Sharp mass,
* 1964 –
M. A. Melvin discovers the
Melvin electrovacuum solution (aka the ''Melvin magnetic universe''),
* 1964 –
Irwin Shapiro predicts a
gravitational time delay of radiation travel as a test of general relativity
* 1965 – Roger Penrose proves first of the
singularity theorems,
* 1965 – Newman and others discover the Kerr–Newman electrovacuum solution,
* 1965 – Penrose discovers the structure of the light cones in
gravitational plane wave
In general relativity, a gravitational plane wave is a special class of a vacuum pp-wave spacetime, and may be defined in terms of Brinkmann coordinates by
ds^2= (u)(x^2-y^2)+2b(u)xyu^2+2dudv+dx^2+dy^2
Here, a(u), b(u) can be any smooth functions ...
spacetimes,
* 1965 – Kerr and
Alfred Schild
Alfred Schild (September 7, 1921 – May 24, 1977) was a leading Austrian American physicist, well known for his contributions to the Golden age of general relativity (1960–1975).
Biography
Schild was born in Istanbul on September 7, 1921. His ...
introduce
Kerr-Schild spacetime,
* 1965 –
Subrahmanyan Chandrasekhar
Subrahmanyan Chandrasekhar (; ) (19 October 1910 – 21 August 1995) was an Indian-American theoretical physicist who spent his professional life in the United States. He shared the 1983 Nobel Prize for Physics with William A. Fowler for " ...
determines a stability criterion,
* 1965 –
Arno Penzias
Arno Allan Penzias (; born April 26, 1933) is an American physicist, radio astronomer and Nobel laureate in physics. Along with Robert Woodrow Wilson, he discovered the cosmic microwave background radiation, which helped establish the Big Bang ...
and
Robert Wilson discover the
cosmic microwave background radiation
In Big Bang cosmology the cosmic microwave background (CMB, CMBR) is electromagnetic radiation that is a remnant from an early stage of the universe, also known as "relic radiation". The CMB is faint cosmic background radiation filling all space ...
,
* 1965 –
Joseph Weber puts the first Weber bar
gravitational wave detector into operation
* 1966 – Sachs and
Ronald Kantowski discover the
Kantowski-Sachs dust solution,
* 1967 –
Jocelyn Bell
Dame Susan Jocelyn Bell Burnell (; Bell; born 15 July 1943) is an astrophysicist from Northern Ireland who, as a postgraduate student, discovered the first radio pulsars in 1967. The discovery eventually earned the Nobel Prize in Physics i ...
and
Antony Hewish
Antony Hewish (11 May 1924 – 13 September 2021) was a British radio astronomer who won the Nobel Prize for Physics in 1974 (together with fellow radio-astronomer Martin Ryle) for his role in the discovery of pulsars. He was also awarded the ...
discover
pulsars
A pulsar (from ''pulsating radio source'') is a highly magnetized rotating neutron star that emits beams of electromagnetic radiation out of its magnetic poles. This radiation can be observed only when a beam of emission is pointing toward Ea ...
,
* 1967 –
Robert H. Boyer and
R. W. Lindquist introduce
Boyer–Lindquist coordinates In the mathematical description of general relativity, the Boyer–Lindquist coordinates are a generalization of the coordinates used for the metric of a Schwarzschild black hole that can be used to express the metric of a Kerr black hole.
The H ...
for the Kerr vacuum,
* 1967 –
Bryce DeWitt
Bryce Seligman DeWitt (January 8, 1923 – September 23, 2004), was an American theoretical physicist noted for his work in gravitation and quantum field theory.
Life
He was born Carl Bryce Seligman, but he and his three brothers, including th ...
publishes on canonical
quantum gravity
Quantum gravity (QG) is a field of theoretical physics that seeks to describe gravity according to the principles of quantum mechanics; it deals with environments in which neither gravitational nor quantum effects can be ignored, such as in the vi ...
,
* 1967 –
Werner Israel
Werner Israel, (October 4, 1931 – May 18, 2022) was a physicist, author, researcher, and professor at the University of Victoria.
Biography
Born in Berlin, Germany and raised in Cape Town, South Africa, he first received his B.Sc. in 1951 an ...
proves the
no-hair theorem,
* 1967 –
Kenneth Nordtvedt
Kenneth Leon Nordtvedt is an American physicist. He was born on April 16, 1939, in Chicago, Illinois. Nordtvedt graduated from the Massachusetts Institute of Technology (1960) and Stanford University (Ph.D., 1964) and was a junior fellow in the ...
develops
PPN formalism,
* 1967 –
Mendel Sachs
Mendel Sachs (; April 13, 1927 – May 5, 2012) was an American theoretical physicist. His scientific work includes the proposal of a unified field theory that brings together the weak force, strong force, electromagnetism, and gravity.
Biograph ...
publishes factorization of Einstein's field equations,
* 1967 –
Hans Stephani discovers the
Stephani dust solution,
* 1968 –
F. J. Ernst discovers the
Ernst equation,
* 1968 –
B. Kent Harrison discovers the
Harrison transformation, a solution-generating method,
* 1968 –
Brandon Carter
Brandon Carter, (born 1942) is an Australian theoretical physicist, best known for his work on the properties of black holes and for being the first to name and employ the anthropic principle in its contemporary form. He is a researcher at the ...
solves the geodesic equations for Kerr–Newmann electrovacuum,
* 1968 –
Hugo D. Wahlquist discovers the
Wahlquist fluid,
* 1968 – Irwin Shapiro presents the first detection of the Shapiro delay
* 1968 –
Kenneth Nordtvedt
Kenneth Leon Nordtvedt is an American physicist. He was born on April 16, 1939, in Chicago, Illinois. Nordtvedt graduated from the Massachusetts Institute of Technology (1960) and Stanford University (Ph.D., 1964) and was a junior fellow in the ...
studies a possible violation of the weak equivalence principle for self-gravitating bodies and proposes a new test of the weak equivalence principle based on observing the relative motion of the Earth and Moon in the Sun's gravitational field
* 1969 –
William B. Bonnor introduces the
Bonnor beam,
* 1969 –
Joseph Weber reports observation of
gravitational waves
Gravitational waves are waves of the intensity of gravity generated by the accelerated masses of an orbital binary system that propagate as waves outward from their source at the speed of light. They were first proposed by Oliver Heaviside i ...
(a claim now generally discounted),
* 1969 – Penrose proposes the (weak)
cosmic censorship hypothesis The weak and the strong cosmic censorship hypotheses are two mathematical conjectures about the structure of gravitational singularities arising in general relativity.
Singularities that arise in the solutions of Einstein's equations are typically ...
and the
Penrose process,
* 1969 –
Stephen W. Hawking proves area theorem for black holes,
* 1969 – Misner introduces the
mixmaster universe,
1970s
* 1970 –
Frank J. Zerilli derives the
Zerilli equation,
* 1970 –
Vladimir A. Belinskiǐ,
Isaak Markovich Khalatnikov
Isaak Markovych Khalatnykov ( uk, Ісаа́к Ма́ркович Хала́тников; 17 October 1919 – 9 January 2021) was a leading Soviet theoretical physicist who has made significant contributions to many areas of theoretical physics, ...
, and
Evgeny Lifshitz
Evgeny Mikhailovich Lifshitz (russian: Евге́ний Миха́йлович Ли́фшиц; February 21, 1915, Kharkiv, Russian Empire – October 29, 1985, Moscow, Russian SFSR) was a leading Soviet physicist and brother of the physicist ...
introduce the
BKL conjecture,
* 1970 – Chandrasekhar pushes on to 5/2 post-Newtonian order,
* 1970 – Hawking and Penrose prove trapped surfaces must arise in black holes,
* 1970 – the
Kinnersley-Walker photon rocket,
* 1970 –
Peter Szekeres introduces
colliding plane wave
In physics, a collision is any event in which two or more bodies exert forces on each other in a relatively short time. Although the most common use of the word ''collision'' refers to incidents in which two or more objects collide with great fo ...
s,
* 1971 –
Peter C. Aichelburg and
Roman U. Sexl introduce the
Aichelburg–Sexl ultraboost
In general relativity, the Aichelburg–Sexl ultraboost is an exact solution which models the spacetime of an observer moving towards or away from a spherically symmetric gravitating object at nearly the speed of light. It was introduced by Pe ...
,
* 1971 – Introduction of the
Khan–Penrose vacuum, a simple explicit colliding plane wave spacetime,
* 1971 –
Robert H. Gowdy introduces the
Gowdy vacuum solutions (cosmological models containing circulating gravitational waves),
* 1971 –
Cygnus X-1, the first solid black hole candidate, discovered by
Uhuru satellite,
* 1971 –
William H. Press discovers black hole ringing by
numerical simulation
Computer simulation is the process of mathematical modelling, performed on a computer, which is designed to predict the behaviour of, or the outcome of, a real-world or physical system. The reliability of some mathematical models can be dete ...
,
* 1971 – Harrison and Estabrook algorithm for solving systems of PDEs,
* 1971 –
James W. York
James W. York Jr. (born July 3, 1939 in Raleigh, North Carolina) is an American mathematical physicist who contributed to the theory of general relativity. In any physical theory, it is important to understand when solutions to the fundamental fiel ...
introduces
conformal method generating initial data for ADM initial value formulation,
* 1971 –
Robert Geroch introduces
Geroch group and a
solution generating method,
* 1972 –
Jacob Bekenstein proposes that black holes have a non-decreasing
entropy which can be identified with the area,
* 1972 – Carter, Hawking and
James M. Bardeen
James Maxwell Bardeen (May 9, 1939 – June 20, 2022) was an American physicist, well known for his work in general relativity, particularly his role in formulating the laws of black hole mechanics. He also discovered the Bardeen vacuum, an e ...
propose the four
laws of black hole mechanics,
* 1972 – Sachs introduces
optical scalars In general relativity, optical scalars refer to a set of three scalar functions \ describing the propagation of a geodesic null congruence.Eric Poisson. ''A Relativist's Toolkit: The Mathematics of Black-Hole Mechanics''. Cambridge: Cambridge Uni ...
and proves
peeling theorem,
* 1972 –
Rainer Weiss proposes concept of interferometric gravitational wave detector,
* 1972 – J. C. Hafele and R. E. Keating perform
Hafele–Keating experiment,
* 1972 –
Richard H. Price studies
gravitational collapse with numerical simulations,
* 1972 –
Saul Teukolsky
Saul Arno Teukolsky (born August 2, 1947) is a theoretical astrophysicist and a professor of Physics and Astronomy at Caltech and Cornell University. His major research interests include general relativity, relativistic astrophysics, and computa ...
derives the
Teukolsky equation,
* 1972 –
Yakov B. Zel'dovich predicts the transmutation of electromagnetic and gravitational radiation,
* 1973 – P. C. Vaidya and L. K. Patel introduce the
Kerr–Vaidya null dust solution,
* 1973 – Publication by
Charles W. Misner
Charles W. Misner (; born June 13, 1932) is an American physicist and one of the authors of ''Gravitation''. His specialties include general relativity and cosmology. His work has also provided early foundations for studies of quantum gravity an ...
,
Kip S. Thorne
Kip Stephen Thorne (born June 1, 1940) is an American theoretical physicist known for his contributions in gravitational physics and astrophysics. A longtime friend and colleague of Stephen Hawking and Carl Sagan, he was the Richard P. F ...
and
John A. Wheeler
John Archibald Wheeler (July 9, 1911April 13, 2008) was an American theoretical physicist. He was largely responsible for reviving interest in general relativity in the United States after World War II. Wheeler also worked with Niels Bohr in e ...
of the treatise ''
Gravitation'', the first modern textbook on general relativity,
* 1973 – Publication by
Stephen W. Hawking and
George Ellis of the monograph ''
The Large Scale Structure of Space-Time
''The'' () is a grammatical article in English, denoting persons or things already mentioned, under discussion, implied or otherwise presumed familiar to listeners, readers, or speakers. It is the definite article in English. ''The'' is the ...
'',
* 1973 – Geroch introduces the
GHP formalism,
* 1974 –
Russell Hulse
Russell Alan Hulse (born November 28, 1950) is an American physicist and winner of the Nobel Prize in Physics, shared with his thesis advisor Joseph Hooton Taylor Jr., "''for the discovery of a new type of pulsar, a discovery that has opened up ...
and
Joseph Hooton Taylor, Jr. discover the
Hulse–Taylor binary pulsar,
* 1974 –
James W. York
James W. York Jr. (born July 3, 1939 in Raleigh, North Carolina) is an American mathematical physicist who contributed to the theory of general relativity. In any physical theory, it is important to understand when solutions to the fundamental fiel ...
and Niall Ó Murchadha present the analysis of the initial value formulation and examine the stability of its solutions,
* 1974 – R. O. Hansen introduces
Hansen–Geroch multipole moments,
* 1974: –
Tullio Regge introduces the
Regge calculus In general relativity, Regge calculus is a formalism for producing simplicial approximations of spacetimes that are solutions to the Einstein field equation. The calculus was introduced by the Italian theoretician Tullio Regge in 1961. Available ( ...
,
* 1974 – Hawking discovers
Hawking radiation
Hawking radiation is theoretical black body radiation that is theorized to be released outside a black hole's event horizon because of relativistic quantum effects. It is named after the physicist Stephen Hawking, who developed a theoretical arg ...
,
* 1975 – Chandrasekhar and
Steven Detweiler compute
quasinormal modes,
* 1975 – Szekeres and D. A. Szafron discover the
Szekeres–Szafron dust solutions,
* 1976 – Penrose introduces
Penrose limits (every null geodesic in a Lorentzian spacetime behaves like a plane wave),
* 1976 –
Gravity Probe A
Gravity Probe A (GP-A) was a space-based experiment to test the equivalence principle, a feature of Einstein's theory of relativity. It was performed jointly by the Smithsonian Astrophysical Observatory and the National Aeronautics and Space ...
experiment confirmed slowing the flow of time caused by gravity matching the predicted effects to an accuracy of about 70 parts per million.
* 1976 –
Robert Vessot and
Martin Levine use a
hydrogen maser
A maser (, an acronym for microwave amplification by stimulated emission of radiation) is a device that produces coherent electromagnetic waves through amplification by stimulated emission. The first maser was built by Charles H. Townes, Jame ...
clock on a
Scout D rocket to test the gravitational redshift predicted by the equivalence principle to approximately 0.007%
* 1978 – Penrose introduces the notion of a ''thunderbolt'',
* 1978 – Belinskiǐ and Zakharov show how to solve
Einstein's field equations
In the general theory of relativity, the Einstein field equations (EFE; also known as Einstein's equations) relate the geometry of spacetime to the distribution of matter within it.
The equations were published by Einstein in 1915 in the for ...
using the
inverse scattering transform In mathematics, the inverse scattering transform is a method for solving some non-linear partial differential equations. The method is a non-linear analogue, and in some sense generalization, of the Fourier transform, which itself is applied to sol ...
; the first
gravitational solitons,
* 1979 –
Richard Schoen and
Shing-Tung Yau prove the
positive mass theorem.
* 1979 –
Dennis Walsh,
Robert Carswell Robert Carswell may refer to:
* Robert Carswell, Baron Carswell (1934–2023), British law lord
* Robert Carswell (cricketer) (born 1936), New Zealand cricketer
* Robert Carswell (MP) for Wallingford (UK Parliament constituency)
* Robert Carswel ...
, and
Ray Weymann discover the gravitationally lensed
quasar Q0957+561
1980s
* 1982 –
Joseph Taylor and
Joel Weisberg show that the rate of energy loss from the binary
pulsar PSR B1913+16 agrees with that predicted by the general relativistic quadrupole formula to within 5%
2000s
* 2002 – First data collection of the
Laser Interferometer Gravitational-Wave Observatory
The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool. Two large ...
(LIGO).
* 2005 – The first
stable numerical solutions of a binary black hole orbit are calculated independently by three different research groups.
* 2007 – End of
Gravity Probe B experiment.
* 2015 – Advanced
LIGO reports the first direct detections of gravitational waves (
GW150914 and
GW151226).
* 2017 – Advanced
LIGO and
Fermi Gamma-ray Space Telescope constrain the speed of gravity to 1 part in
of the speed of light with
GW170817.
* 2019 – The
Event Horizon Telescope
The Event Horizon Telescope (EHT) is a large telescope array consisting of a global network of radio telescopes. The EHT project combines data from several very-long-baseline interferometry (VLBI) stations around Earth, which form a combined arr ...
images the shadow of
supermassive black hole M87*
* 2022 - The
James Webb Space Telescope
The James Webb Space Telescope (JWST) is a space telescope which conducts infrared astronomy. As the largest optical telescope in space, its high resolution and sensitivity allow it to view objects too old, distant, or faint for the Hubble Spa ...
publishes its
first image, showing gravitational lensing by the
SMACS 0723 galaxy cluster.
See also
*
Timeline of black hole physics
*
Timeline of special relativity and the speed of light
References
External links
Timeline of relativity and gravitation(Tomohiro Harada, Department of Physics, Rikkyo University)
{{DEFAULTSORT:Timeline Of Gravitational Physics And Relativity
Astrophysics
Gravity
Gravitational physics and relativity