Timeline of gravitational physics and relativity

Timeline of gravitational physics and general relativity

Before 1500

• 3rd century BC - Aristarchus of Samos proposes heliocentric model,^[1] 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 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 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 arrives a mathematical formulation of the law of falling objects based on his earlier experiments.
• 1608 – Galileo Galilei discovers the parabolic arc of projectiles through experiment.
• 1609 - Johannes Kepler describes to motion of planets around the Sun, now known as Kepler's laws of planetary motion.
• 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
• 1686 – Isaac Newton uses a fixed length pendulum with weights of varying composition to test the weak equivalence principle 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 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.
• 1876 – William Kingdon Clifford suggests that the motion of matter may be due to changes in the geometry of space
• 1882 – Simon Newcomb observes a 43 arcsecond per century excess precession of Mercury's orbit
• 1887 – Albert A. Michelson and Edward W. Morley in their experiment do not detect the ether drift
• 1889 – Loránd Eötvös uses a torsion balance to test the weak equivalence principle to 1 part in one billion
• 1893 – Ernst Mach states Mach's principle; first constructive attack on the idea of Newtonian absolute space
• 1898 – Henri Poincaré states that simultaneity is relative
• 1899 – Hendrik Antoon Lorentz published Lorentz transformations

1900s

• 1904 – Henri Poincaré presents the principle of relativity for electromagnetism
• 1905 – Albert Einstein completes his theory of special relativity and states the law of mass-energy conservation: E=mc²
• 1907 – Albert Einstein introduces the principle of equivalence of gravitation and inertia and uses it to predict the gravitational redshift
• 1915 – Albert Einstein completes his theory of general relativity. The new theory explains Mercury's strange motions that baffled Urbain Le Verrier.
• 1915 – Karl Schwarzschild publishes the Schwarzschild metric 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 shows that the field equations of general relativity admit wavelike solutions
• 1918 – J. Lense and Hans Thirring find the gravitomagnetic precession of gyroscopes in the equations of general relativity
• 1919 – Arthur Eddington 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
• 1937 – Fritz Zwicky states that galaxies could act as gravitational lenses
• 1937 – Albert Einstein, Leopold Infeld, 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 introduces sticky bead argument,
• 1957 – John Wheeler discusses the breakdown of classical general relativity near singularities and the need for quantum gravity
• 1959: Pound–Rebka experiment, first precision test of gravitational redshift,
• 1959: Lluís Bel introduces Bel–Robinson tensor and the Bel decomposition of the Riemann tensor,
• 1959: Arthur Komar introduces the Komar mass,
• 1959: Richard Arnowitt, Stanley Deser and Charles W. Misner developed ADM formalism.

1960s

• 1960: Martin Kruskal and George Szekeres independently introduce the Kruskal–Szekeres coordinates for the Schwarzschild vacuum,
• 1960: Shapiro effect confirmed,
• 1960: Thomas Matthews and Allan R. Sandage associate 3C 48 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: Joseph Weber reports observation of gravitational waves (a claim now generally discounted),
• 1960: Ivor M. Robinson and Andrzej Trautman discover the Robinson-Trautman null dust solution^[2]
• 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,
• 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 introduce the ADM reformulation and global hyperbolicity,
• 1962: Yvonne Choquet-Bruhat 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, Peter Roll, and R. Krotkov use a torsion fiber balance to test the weak equivalence principle to 2 parts in 100 billion
• 1963: Roy Kerr discovers the Kerr vacuum solution of Einstein's field equations,
• 1963: Redshifts of 3C 273 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 Gravitational 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 spacetimes,
• 1965: Kerr and Alfred Schild introduce Kerr-Schild spacetimes,
• 1965: Subrahmanyan Chandrasekhar determines a stability criterion,
• 1965: Arno Penzias and Robert Wilson discover the cosmic microwave background radiation,
• 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 and Antony Hewish discover pulsars,
• 1967: Robert H. Boyer and R. W. Lindquist introduce Boyer–Lindquist coordinates for the Kerr vacuum,
• 1967: Bryce DeWitt publishes on canonical quantum gravity,
• 1967: Werner Israel proves the no-hair theorem,
• 1967: Kenneth Nordtvedt develops PPN formalism,
• 1967: Mendel Sachs 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 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 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: Penrose proposes the (weak) cosmic censorship hypothesis 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, and Evgeny Lifshitz 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 waves,
• 1971: Peter C. Aichelburg and Roman U. Sexl introduce the Aichelburg–Sexl ultraboost,
• 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,
• 1971: Harrison and Estabrook algorithm for solving systems of PDEs,
• 1971: James W. York 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 propose the four laws of black hole mechanics,
• 1972: Sachs introduces optical scalars 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 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, Kip S. Thorne and John A. Wheeler 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,
• 1973: Geroch introduces the GHP formalism,
• 1974: Russell Hulse and Joseph Hooton Taylor, Jr. discover the Hulse–Taylor binary pulsar,
• 1974: James W. York 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,
• 1974: Hawking discovers Hawking radiation,
• 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 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 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 using the inverse scattering transform; the first gravitational solitons,
• 1979: Richard Schoen and Shing-Tung Yau prove the positive mass theorem.
• 1979 – Dennis Walsh, Robert Carswell, and Ray Weymann discover the gravitationally lensed quasar Q0957+561

After 1980

• 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%
• 2007 – End of Gravity Probe B experiment.
• 2015 – Laser Interferometer Gravitational-Wave Observatory (LIGO) is the first to directly detect gravitational waves.

See also

• Timeline of black hole physics

References

1. "Agar.io". agar.io. Retrieved 2016-04-08.
2. "Spherical Gravitational Waves". Cdsads.u-strasbg.fr. Retrieved 2012-07-20.

External links

• Timeline of relativity and gravitation (Tomohiro Harada, Department of Physics, Rikkyo University)
• Timeline of General Relativity and Cosmology from 1905