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{{see also|history of special relativity}}
{{Use dmy dates|date=July 2013}}
{{General relativity sidebar}}

[[General relativity]] (GR) is a [[theory of gravitation]] that was developed by [[Albert Einstein]] between 1907 and 1915, with contributions by many others after 1915. According to general relativity, the observed gravitational attraction between masses results from the warping of space and time by those masses.

Before the advent of general relativity, Newton's law of universal gravitation had been accepted for more than two hundred years as a valid description of the gravitational force between masses, even though Newton himself did not regard the theory as the final word on the nature of gravity. Within a century of Newton's formulation, careful astronomical observation revealed unexplainable variations between the theory and the observations.  Under Newton's model, gravity was the result of an attractive force between massive objects. Although even Newton was bothered by the unknown nature of that force, the basic framework was extremely successful at describing motion.

However, experiments and observations show that Einstein's description accounts for several effects that are unexplained by Newton's law, such as minute anomalies in the orbits of Mercury and other planets. General relativity also predicts novel effects of gravity, such as [[gravitational wave]]s, [[gravitational lensing]] and an effect of gravity on time known as [[gravitational time dilation]]. Many of these predictions have been confirmed by experiment or observation, while others are the subject of ongoing research.

General relativity has developed into an essential tool in modern astrophysics. It provides the foundation for the current understanding of black holes, regions of space where gravitational attraction is so strong that not even light can escape. Their strong gravity is thought to be responsible for the intense radiation emitted by certain types of astronomical objects (such as active galactic nuclei or microquasars). General relativity is also part of the framework of the standard Big Bang model of cosmology.

==Creation of general relativity==

=== Early investigations ===
As Einstein later said, the reason for the development of general relativity was the preference of inertial motion within [[special relativity]], while a theory which from the outset prefers no particular state of motion appeared more satisfactory to him.<ref>Albert Einstein, [http://nobelprize.org/nobel_prizes/physics/laureates/1921/einstein-lecture.html Nobel lecture] in 1921</ref> So, while still working at the patent office in 1907, Einstein had what he would call his "happiest thought". He realized that the [[principle of relativity]] could be extended to gravitational fields.

Consequently, in 1907 he wrote an article (published 1908) on acceleration under [[special relativity]].<ref>{{Citation|author= Einstein, A. | title= Relativitätsprinzip und die aus demselben gezogenen Folgerungen (On the Relativity Principle and the Conclusions Drawn from It)| journal= Jahrbuch der Radioaktivität (Yearbook of Radioactivity) | volume= 4|pages= 411–462}} page 454 (Wir betrachen zwei Bewegung systeme ...)</ref>
In that article, he argued that [[free fall]] is really inertial motion, and that for a freefalling observer the rules of special relativity must apply. This argument is called the [[Equivalence principle]]. In the same article, Einstein also predicted the phenomenon of [[gravitational time dilation]].

In 1911, Einstein published another article expanding on the 1907 article.<ref>{{Citation|last=Einstein |first=Albert |title=Einfluss der Schwerkraft auf die Ausbreitung des Lichtes (On the Influence of Gravity on the Propagation of Light) |journal=Annalen der Physik |year=1911 |volume=35 |pages=898–908 |doi=10.1002/andp.19113401005|bibcode = 1911AnP...340..898E |url=https://zenodo.org/record/1424213 }} (also in ''Collected Papers'' Vol. 3, document 23)</ref>
There, he thought about the case of a uniformly accelerated box not in a gravitational field, and noted that it would be indistinguishable from a box sitting still in an unchanging gravitational field. He used special relativity to see that the rate of clocks at the top of a box accelerating upward would be faster than the rate of clocks at the bottom. He concludes that the rates of clocks depend on their position in a gravitational field, and that the difference in rate is proportional to the gravitational potential to first approximation.

Also the [[Gravitational lensing|deflection of light]] by massive bodies was predicted. Although the approximation was crude, it allowed him to calculate that the deflection is nonzero. German astronomer [[Erwin Finlay-Freundlich]] publicized Einstein's challenge to scientists around the world.<ref name="Crelinston_1">Crelinsten, Jeffrey. "[http://www.pupress.princeton.edu/titles/8165.html Einstein's Jury: The Race to Test Relativity]". ''[[Princeton University Press]].'' 2006. Retrieved on 13 March 2007. {{ISBN|978-0-691-12310-3}}</ref> This urged astronomers to detect the deflection of light during a [[solar eclipse]], and gave Einstein confidence that the scalar theory of gravity proposed by [[Gunnar Nordström]] was incorrect. But the actual value for the deflection that he calculated was too small by a factor of two, because the approximation he used doesn't work well for things moving at near the speed of light. When Einstein finished the full theory of general relativity, he would rectify this error and predict the correct amount of light deflection by the sun.

Another of Einstein's notable thought experiments about the nature of the gravitational field is that of the rotating disk (a variant of the [[Ehrenfest paradox]]). He imagined an observer performing experiments on a rotating turntable. He noted that such an observer would find a different value for the mathematical constant π than the one predicted by Euclidean geometry. The reason is that the radius of a circle would be measured with an uncontracted ruler, but, according to special relativity, the circumference would seem to be longer because the ruler would be contracted. Since Einstein believed that the laws of physics were local, described by local fields, he concluded from this that spacetime could be locally curved. This led him to study [[Riemannian geometry]], and to formulate general relativity in this language.

===Developing general relativity===
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| image1    = 1919 eclipse positive.jpg
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| caption1  = [[Arthur Stanley Eddington|Eddington]]'s photograph of a solar eclipse, which confirmed Einstein's theory that light "bends".

| image2    = 19191125 A New Physics Based on Einstein - The New York Times.png
| caption2  = ''The New York Times'' reported confirmation of "the Einstein theory" (specifically, the bending of light by gravitation) based on 29 May 1919 eclipse observations in Principe (Africa) and Sobral (Brazil), after the findings were presented on 6 November 1919 to a joint meeting in London of the [[Royal Society]] and the [[Royal Astronomical Society]].<ref name=NYTimes_19191125>{{cite news |title=A New Physics, Based on Einstein |url=https://newspaperarchive.com/new-york-times-nov-25-1919-p-17/ |work=The New York Times |date=25 November 1919 |page=17}}</ref> ([https://timesmachine.nytimes.com/timesmachine/1919/11/25/96868705.html?pageNumber=17 Full text])
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In 1912, Einstein returned to Switzerland to accept a professorship at his ''alma mater'', the ETH. Once back in Zurich, he immediately visited his old ETH classmate [[Marcel Grossmann]], now a professor of mathematics, who introduced him to Riemannian geometry and, more generally, to [[differential geometry]]. On the recommendation of Italian mathematician [[Tullio Levi-Civita]], Einstein began exploring the usefulness of [[general covariance]] (essentially the use of [[tensor]]s) for his gravitational theory. For a while Einstein thought that there were problems with the approach, but he later returned to it and, by late 1915, had published his [[general theory of relativity]] in the form in which it is used today.<ref>O'Connor, J.J. and E.F. Robertson (1996), "[http://www-history.mcs.st-and.ac.uk/HistTopics/General_relativity.html General relativity]". ''[http://www-history.mcs.st-and.ac.uk/Indexes/Math_Physics.html Mathematical Physics index]'', [http://www.st-andrews.ac.uk/maths/ School of Mathematics and Statistics], [http://www.st-andrews.ac.uk/ University of St. Andrews], Scotland, May, 1996. Retrieved 2015-02-04.</ref> This theory explains gravitation as distortion of the structure of [[spacetime]] by matter, affecting the [[inertia]]l motion of other matter.

During World War I, the work of [[Central Powers]] scientists was available only to Central Powers academics, for national security reasons. Some of Einstein's work did reach the United Kingdom and the United States through the efforts of the Austrian [[Paul Ehrenfest]] and physicists in the Netherlands, especially 1902 Nobel Prize-winner [[Hendrik Lorentz]] and [[Willem de Sitter]] of [[Leiden University]]. After the war ended, Einstein maintained his relationship with Leiden University, accepting a contract as an ''[[Professor#Netherlands|Extraordinary Professor]]''; for ten years, from 1920 to 1930, he travelled to the Netherlands regularly to lecture.<ref>{{Citation|url=http://www.lorentz.leidenuniv.nl/history/einstein/einstein.html|title=Two friends in Leiden|accessdate=11 June 2007}}</ref>

In 1917, several astronomers accepted Einstein's 1911 challenge from Prague. The [[Mount Wilson Observatory]] in California, U.S., published a solar [[spectroscopic]] analysis that showed no gravitational redshift.<ref>{{Citation |last =Crelinsten |first =Jeffrey |title =Einstein's Jury: The Race to Test Relativity |isbn =978-0-691-12310-3 |publisher =Princeton University Press |pages =103–108 |year =2006 |url =https://archive.org/details/einsteinsjuryrac00crel |accessdate =13 March 2007 |ref = }}</ref> In 1918, the [[Lick Observatory]], also in California, announced that it too had disproved Einstein's prediction, although its findings were not published.<ref>{{Citation |last =Crelinsten |first =Jeffrey |title =Einstein's Jury: The Race to Test Relativity |isbn =978-0-691-12310-3 |publisher =Princeton University Press |pages =114–119 |year =2006 |url =https://archive.org/details/einsteinsjuryrac00crel |accessdate =13 March 2007 }}</ref>

However, in May 1919, a team led by the British astronomer [[Arthur Stanley Eddington]] claimed to have confirmed Einstein's prediction of [[gravitational lensing|gravitational deflection of starlight]] by the sun while photographing a solar eclipse with dual expeditions in [[Sobral, Ceará|Sobral]], northern Brazil, and [[Príncipe]], a west African island.<ref name="Crelinston_1"/> Nobel laureate [[Max Born]] praised general relativity as the "greatest feat of human thinking about nature";<ref>{{Citation |title = The genius of space and time
|url = http://books.guardian.co.uk/reviews/scienceandnature/0,,1571826,00.html |publisher = The Guardian |date = 17 September 2005 |accessdate = 31 March 2007 | location=London | first=PD | last=Smith}}</ref> fellow laureate [[Paul Dirac]] was quoted saying it was "probably the greatest scientific discovery ever made".<ref name="schmidhuber">[[Jürgen Schmidhuber]]. "[http://www.idsia.ch/~juergen/einstein.html Albert Einstein (1879–1955) and the 'Greatest Scientific Discovery Ever']". 2006. Retrieved on 4 October 2006.</ref>

There have been claims that scrutiny of the specific photographs taken on the Eddington expedition showed the experimental uncertainty to be comparable to the same magnitude as the effect Eddington claimed to have demonstrated, and that a 1962 British expedition concluded that the method was inherently unreliable.<ref name="Eddington">{{Citation|last = Andrzej |first = Stasiak |year = 2003 |title = Myths in science |journal = EMBO Reports |volume = 4 |issue = 3 |page = 236|doi =10.1038/sj.embor.embor779 |pmc = 1315907 }}</ref> The deflection of light during a solar eclipse was confirmed by later, more accurate observations.<ref>See the table in MathPages [http://www.mathpages.com/rr/s6-03/6-03.htm Bending Light]</ref> Some resented the newcomer's fame, notably among some German physicists, who later started the ''[[Deutsche Physik]]'' (German Physics) movement.<ref name="Hentschel">{{Citation |last = Hentschel |first = Klaus and Ann M. |year = 1996 |title = Physics and National Socialism: An Anthology of Primary Sources |pages = xxi |publisher = Birkhaeuser Verlag |isbn = 3-7643-5312-0 |nopp = true}}</ref><ref>For a discussion of astronomers' attitudes and debates about relativity, see {{Citation |last = Crelinsten |first = Jeffrey |title = Einstein's Jury: The Race to Test Relativity |publisher = Princeton University Press |year = 2006 |isbn = 0-691-12310-1 |url = https://archive.org/details/einsteinsjuryrac00crel }}, especially chapters 6, 9, 10 and 11.</ref>

===General covariance and the hole argument===
By 1912, Einstein was actively seeking a theory in which [[gravitation]] was explained as a [[geometric]] phenomenon. At the urging of [[Tullio Levi-Civita]], Einstein began by exploring the use of [[general covariance]] (which is essentially the use of curvature [[tensors]]) to create a gravitational theory.  However, in 1913 Einstein abandoned that approach, arguing that it is inconsistent based on the "[[hole argument]]".  In 1914 and much of 1915, Einstein was trying to create [[field equations]] based on another approach.  When that approach was proven to be inconsistent, Einstein revisited the concept of general covariance and discovered that the hole argument was flawed.<ref>{{Cite journal|title = Arch and scaffold: How Einstein found his field equations|journal = Physics Today|date = 2015-11-01|issn = 0031-9228|pages = 30–36|volume = 68|issue = 11|doi = 10.1063/PT.3.2979|language = en|first = Michel|last = Janssen|first2 = Jürgen|last2 = Renn|bibcode = 2015PhT....68k..30J }}</ref>

===The development of the Einstein field equations===
{{main|Einstein field equations}}
When Einstein realized that general covariance was actually tenable, he quickly completed the development of the field equations that are named after him. However, he made a now-famous mistake. The field equations he published in October 1915 were

:<math>R_{\mu\nu} =  T_{\mu\nu}\,</math>,

where <math>R_{\mu\nu}</math> is the [[Ricci tensor]], and <math>T_{\mu\nu}</math> the [[energy–momentum tensor]]. This predicted the non-[[Classical mechanics|Newtonian]] [[perihelion precession]] of [[Mercury (planet)|Mercury]], and so had Einstein very excited.  However, it was soon realized that they were inconsistent with the local [[conservation of energy–momentum]] unless the universe had a constant density of mass–energy–momentum.  In other words, air, rock and even a vacuum should all have the same density.  This inconsistency with observation sent Einstein back to the drawing board.  However, the solution was all but obvious, and on 25 November 1915 Einstein presented the actual Einstein field equations to the [[Prussian Academy of Sciences]]:<ref>{{cite book |last=Pais |first=Abraham |authorlink=Abraham Pais |page=239 |title=Subtle is the Lord : The Science and the Life of Albert Einstein: The Science and the Life of Albert Einstein |publisher=Oxford University Press |year=1982 |isbn=9780191524028 |chapter-url=https://books.google.com/books?id=KdaiZDaB7TgC&pg=PA239 |chapter=14. The Field Equations of Gravitation}}</ref>

:<math>R_{\mu\nu} - {1\over 2}R g_{\mu\nu} = T_{\mu\nu}</math>,

where <math>R</math> is the [[Ricci scalar]] and <math>g_{\mu\nu}</math> the [[metric tensor]]. With the publication of the field equations, the issue became one of solving them for various cases and interpreting the solutions.  This and experimental verification have dominated general relativity research ever since.

===Einstein and Hilbert===
{{See also|Relativity priority dispute}}
Although Einstein is credited with finding the field equations, the German mathematician [[David Hilbert]] published them in an article before Einstein's article. This has resulted in accusations of [[plagiarism]] against Einstein, although not from Hilbert, and assertions that the field equations should be called the "Einstein–Hilbert field equations".  However, Hilbert did not press his claim for priority and some{{Who|date=October 2010}} have asserted that Einstein submitted the correct equations before Hilbert amended his own work to include them. This suggests that Einstein developed the correct field equations first, though Hilbert may have reached them later independently (or even learned of them afterwards through his correspondence with Einstein).<ref>Leo Corry, Jürgen Renn, John Stachel: "Belated Decision in the Hilbert-Einstein Priority Dispute",  SCIENCE, Vol. 278, 14 November 1997 – [http://www.tau.ac.il/~corry/publications/articles/science.html article text]</ref> However, others have criticized those assertions.<ref>[http://physics.unr.edu/faculty/winterberg/Hilbert-Einstein.pdf Friedwart Winterberg's response to the Cory-Renn-Stachel paper] {{webarchive|url=https://web.archive.org/web/20060209205126/http://www.physics.unr.edu/faculty/winterberg/Hilbert-Einstein.pdf |date=9 February 2006 }} as printed in "Zeitschrift für Naturforschung" [http://www.znaturforsch.com/c59a.htm 59a], 715–719.</ref>

===Sir Arthur Eddington===
In the early years after Einstein's theory was published, [[Arthur Eddington|Sir Arthur Eddington]] lent his considerable prestige in the British scientific establishment in an effort to champion the work of this German scientist.  Because the theory was so complex and abstruse (even today it is popularly considered the pinnacle of scientific thinking; in the early years it was even more so), it was rumored that only three people in the world understood it.  There was an illuminating, though probably apocryphal, anecdote about this.  As related by [[Ludwik Silberstein]],<ref>John Waller (2002), ''Einstein's Luck'', Oxford University Press, {{ISBN|0-19-860719-9}}</ref> during one of Eddington's lectures he asked "Professor Eddington, you must be one of three persons in the world who understands  general relativity."  Eddington paused, unable to answer. Silberstein continued "Don't be modest, Eddington!" Finally, Eddington replied "On the contrary, I'm trying to think who the third person is."

==Solutions==
{{refimprove|section|date=November 2017}}<!--most of section has no citations-->
=== The Schwarzschild solution ===
Since the field equations are [[non-linear]], Einstein assumed that they were unsolvable.{{citation needed|date=February 2016}}  However, [[Karl Schwarzschild]] discovered in 1915 and published in 1916<ref>{{Harvnb|Schwarzschild|1916a}}, {{Harvnb|Schwarzschild|1916b}}</ref> an exact solution for the case of a spherically symmetric [[spacetime]] surrounding a massive object in [[spherical coordinates]]. This is now known as the [[Schwarzschild solution]]. Since then, many other exact solutions have been found.

===The expanding universe and the cosmological constant===
{{main|Cosmological constant}}
In 1922, [[Alexander Friedmann]] found a solution in which the universe may expand or contract, and later [[Georges Lemaître]] derived a solution for an expanding universe.  However, Einstein believed that the universe was apparently static, and since a static cosmology was not supported by the general relativistic field equations, he added a [[cosmological constant]] Λ to the field equations, which became

:<math>R_{\mu\nu} - {1\over 2}R g_{\mu\nu} + \Lambda g_{\mu\nu} = T_{\mu\nu}</math>.

This permitted the creation of [[Einstein's static universe|steady-state solutions]], but they were unstable: the slightest perturbation of a static state would result in the universe expanding or contracting. In 1929, [[Edwin Hubble]] found evidence for the idea that the universe is expanding. This resulted in Einstein dropping the cosmological constant, referring to it as "the biggest blunder in my career". At the time, it was an [[ad hoc]] hypothesis to add in the cosmological constant, as it was only intended to justify one result (a static universe).

===More exact solutions===
Progress in solving the field equations and understanding the solutions has been ongoing.  The solution for a spherically symmetric charged object was discovered by Reissner and later rediscovered by Nordström, and is called the [[Reissner–Nordström black hole|Reissner–Nordström solution]].  The black hole aspect of the Schwarzschild solution was very controversial, and Einstein did not believe that singularities could be real.  However, in 1957 (two years after Einstein's death in 1955), [[Martin Kruskal]] published a proof that black holes are called for by the Schwarzschild Solution.  Additionally, the solution for a rotating massive object was obtained by [[Roy Kerr]] in the 1960s and is called the [[Kerr solution]].  The [[Kerr–Newman solution]] for a rotating, charged massive object was published a few years later.

==Testing the theory==
{{Main|Tests of general relativity|Gravitational wave observation}}
The perihelion precession of Mercury was the first evidence that general relativity is correct. [[Arthur Stanley Eddington]]'s 1919 expedition confirmed Einstein's prediction for the deflection of light by the Sun during the total [[solar eclipse of 29 May 1919]] which helped to cement the status of general relativity as a true theory. Since then many observations have confirmed the correctness of general relativity. These include studies of [[binary pulsar]]s, observations of radio signals passing the limb of the Sun, and even the [[global positioning system]].

[[File:Black hole - Messier 87 crop max res.jpg|alt=|thumb|right|First image of the event horizon of a black hole ([[M87*]]) captured by the Event Horizon Telescope<ref name="NYT-20190410">{{cite news |last=Overbye |first=Dennis |authorlink=Dennis Overbye |title=Black Hole Picture Revealed for the First Time – Astronomers at last have captured an image of the darkest entities in the cosmos |url=http://www.nytimes.com/2019/04/10/science/black-hole-picture.html?comments#permid=31473598 |date=April 10, 2019 |work=[[The New York Times]] |accessdate=April 10, 2019 }}</ref><ref name="APJL-20190410">{{cite journal |author=The Event Horizon Telescope Collaboration |title=First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole |date=April 10, 2019 |journal=[[The Astrophysical Journal Letters]] |volume=87 |pages=L1 |number=1 |doi=10.3847/2041-8213/ab0ec7 |doi-access=free }}</ref><ref name="NASA-20190410">{{cite news |last=Landau |first=Elizabeth |title=Black Hole Image Makes History |url=https://www.jpl.nasa.gov/news/news.php?feature=7372 |date=April 10, 2019 |work=[[NASA]] |accessdate=April 10, 2019 }}</ref>]]
The theory predicts [[gravitational waves]], which are ripples in the [[curvature]] of [[spacetime]] that propagate as [[wave]]s, travelling outward from the source. They were first detected in September 2015 by the [[Advanced LIGO]] team from the [[Stellar collision]] of a [[Binary black hole]] of [[black hole]]s, adding another confirmation of the theory 100 years after it was published.<ref name="Discovery 2016">{{cite journal |title=Einstein's gravitational waves found at last |journal=Nature News| url=http://www.nature.com/news/einstein-s-gravitational-waves-found-at-last-1.19361 |date=11 February 2016 |last=Castelvecchi |first=Davide |last2=Witze |first2=Witze |doi=10.1038/nature.2016.19361  |accessdate=2016-02-11 }}</ref><ref name='Abbot'>{{cite journal |title=Observation of Gravitational Waves from a Binary Black Hole Merger| authors=B. P. Abbott et al. (LIGO Scientific Collaboration and Virgo Collaboration)| journal=Physical Review Letters| year=2016| volume=116|issue=6| doi=10.1103/PhysRevLett.116.061102|arxiv = 1602.03837 |bibcode = 2016PhRvL.116f1102A | pmid=26918975 | pages=061102}}</ref><ref name='NSF'>{{cite web|title = Gravitational waves detected 100 years after Einstein's prediction {{!}} NSF - National Science Foundation|url = https://www.nsf.gov/news/news_summ.jsp?cntn_id=137628|website = www.nsf.gov|access-date = 2016-02-11}}</ref>

The first image of a black hole, the supermassive one at the center of galaxy [[Messier 87]], was published by the [[Event Horizon Telescope|Event Horizon Telescope Collaboration]] on 10 April 2019.<ref>
* {{Cite journal |author=Shep Doeleman, on behalf of the EHT Collaboration |date=April 2019|url=https://iopscience.iop.org/journal/2041-8205/page/Focus_on_EHT |title=Focus on the First Event Horizon Telescope Results |journal=The Astrophysical Journal Letters |access-date=2019-04-10}}
* {{Cite news|url=https://www.nytimes.com/2019/04/10/science/black-hole-picture.html|title=Black Hole Picture Revealed for the First Time|last=Overbye|first=Dennis|date=2019-04-10|work=The New York Times|access-date=2019-04-10|language=en-US|issn=0362-4331}}</ref>

==Alternative theories==
{{Main|Alternatives to general relativity}}
There have been various attempts to find modifications to general relativity. The most famous of these are the [[Brans–Dicke theory]] (also known as [[scalar-tensor theory]]), and [[Bimetric gravity|Rosen's bimetric theory]]. Both of these theories proposed changes to the field equations of general relativity, and both suffer from these changes permitting the presence of bipolar gravitational radiation. As a result, Rosen's original theory has been refuted by observations of binary pulsars. As for Brans–Dicke (which has a tunable parameter ''ω'' such that ''ω = ∞'' is the same as general relativity), the amount by which it can differ from general relativity has been severely constrained by these observations.

In addition, general relativity is inconsistent with [[quantum mechanics]], the physical theory that describes the wave–particle duality of matter, and quantum mechanics does not currently describe gravitational attraction at relevant (microscopic) scales. There is a great deal of speculation in the physics community as to the modifications that might be needed to both general relativity and quantum mechanics in order to unite them consistently. The speculative theory that unites general relativity and quantum mechanics is usually called [[quantum gravity]], prominent examples of which include [[String Theory]] and [[Loop Quantum Gravity]].

==More about history of general relativity==
[[Kip Thorne]] identifies the "golden age of general relativity" as the period roughly from 1960 to 1975 during which the study of [[general relativity]],<ref>{{cite book |title=The future of theoretical physics and cosmology: celebrating Stephen Hawking's 60th birthday |chapter=Warping spacetime |first1=Kip |last1=Thorne |publisher=Cambridge University Press |year=2003 |isbn=0-521-82081-2 |page=74 |url=https://books.google.com/books?id=yLy4b61rfPwC}} [https://books.google.com/books?id=yLy4b61rfPwC&pg=PA74 Extract of page 74]</ref> which had previously been regarded as something of a curiosity, entered the mainstream of [[theoretical physics]].<ref>In [[Black holes and time warps]], chapter 7 "The Golden Age" Kip Thorne writes: ''The black holes [Subrahmanyan Chandrasekhar] was analyzing were radically different beasts from those of the early 1960s, when physicists had begun to embrace the concept of a black hole. The intervening decade had been a golden age of black-hole research, an era that revolutionized our understanding of general relativity’s predictions.''</ref> During this period, many of the concepts and terms which continue to inspire the imagination of gravitation researchers and the general public were introduced, including [[black hole]]s and '[[gravitational singularity]]'.  At the same time, in a closely related development, the study of [[physical cosmology]] entered the mainstream and the [[Big Bang]] became well established.

[[Fulvio Melia]] refers frequently to the "golden age of relativity" in his book ''Cracking the Einstein Code''. [[Andrzej Trautman]] hosted a relativity conference in [[Warsaw]] in 1962 to which Melia refers:
:General relativity moved very successfully from that meeting in Warsaw, hot on the heels of the [[Pound–Rebka experiment]], and entered its golden age of discovery that lasted into the mid-1970s.<ref>[[Fulvio Melia]] (2009) ''Cracking the Einstein Code'', page 50, [[University of Chicago Press]] {{ISBN|9780226519517}}</ref>
[[Roy Kerr]], protagonist of the book, contributed an Afterword, saying of the book: "It is a remarkable piece of writing capturing beautifully the period we now refer to as the golden age of relativity."<ref>[[Roy Kerr]] (2009) Afterword, ''Cracking the Einstein Code'', page 127</ref>

==See also==
*[[Contributors to general relativity]]
*[[Golden age of cosmology]]
*[[Golden age of physics]]
*[[Mach's principle]]
*[[W. K. Clifford#Premonition of relativity]]

==Notes==
{{reflist}}

==References==
*{{cite book | author=Pais, Abraham | title=Subtle is the lord: the science and life of Albert Einstein | location=Oxford | publisher=Oxford University Press | year=1982 | isbn=0-19-853907-X | url=https://archive.org/details/subtleislordscie00pais }}
* {{cite journal | last1 = Einstein | first1 = A. | authorlink2 = Marcel Grossmann | last2 = Grossmann | first2 = M. | year = 1913 | title = Entwurf einer verallgemeinerten Relativitätstheorie und einer Theorie der Gravitation |trans-title= Outline of a Generalized Theory of Relativity and of a Theory of Gravitation | url = | journal = Zeitschrift für Mathematik und Physik | volume = 62 | issue = | pages = 225–261 }}
*''Einstein and the Changing Worldviews of Physics'' (editors—Lehner C., Renn J., Schemmel M.) 2012 ([[Birkhäuser]]).
* [http://www.bun.kyoto-u.ac.jp/~suchii/gen.GR.html Genesis of general relativity series].
* {{Citation
|last=Schwarzschild
|first=Karl
|authorlink=Karl Schwarzschild
|title=Über das Gravitationsfeld eines Massenpunktes nach der Einsteinschen Theorie
|journal=Sitzungsber. Preuss. Akad. D. Wiss.
|date=1916a
 |pages=189–196
}}
* {{Citation
|last=Schwarzschild
|first=Karl
|authorlink=Karl Schwarzschild
|title=Über das Gravitationsfeld einer Kugel aus inkompressibler Flüssigkeit nach der Einsteinschen Theorie
|journal=Sitzungsber. Preuss. Akad. D. Wiss.
|pages=424–434
|date=1916b
}}

==External links==
*{{Wikisource-inline|The Foundation of the Generalised Theory of Relativity}}

[[Category:General relativity| ]]
[[Category:History of physics|General relativity]]
[[Category:Albert Einstein]]