Faster access than browser!Similarities between Black hole and History of general relativity
Black hole and History of general relativity have 27 things in common (in Unionpedia): Albert Einstein, Arthur Eddington, Big Bang, Equivalence principle, Free fall, General relativity, Georges Lemaître, Gravitational lens, Gravitational singularity, Gravitational time dilation, Gravitational wave, Gravity, Hendrik Lorentz, Karl Schwarzschild, Kerr metric, Kerr–Newman metric, Kip Thorne, LIGO, Loop quantum gravity, Martin David Kruskal, Quantum gravity, Quantum mechanics, Reissner–Nordström metric, Roy Kerr, Schwarzschild metric, Spacetime, String theory.
Albert Einstein
Albert Einstein (14 March 1879 – 18 April 1955) was a German-born theoretical physicist who developed the theory of relativity, one of the two pillars of modern physics (alongside quantum mechanics).
Albert Einstein and Black hole · Albert Einstein and History of general relativity ·
Arthur Eddington
Sir Arthur Stanley Eddington (28 December 1882 – 22 November 1944) was an English astronomer, physicist, and mathematician of the early 20th century who did his greatest work in astrophysics.
Arthur Eddington and Black hole · Arthur Eddington and History of general relativity ·
Big Bang
The Big Bang theory is the prevailing cosmological model for the universe from the earliest known periods through its subsequent large-scale evolution.
Big Bang and Black hole · Big Bang and History of general relativity ·
Equivalence principle
In the theory of general relativity, the equivalence principle is any of several related concepts dealing with the equivalence of gravitational and inertial mass, and to Albert Einstein's observation that the gravitational "force" as experienced locally while standing on a massive body (such as the Earth) is the same as the pseudo-force experienced by an observer in a non-inertial (accelerated) frame of reference.
Black hole and Equivalence principle · Equivalence principle and History of general relativity ·
Free fall
In Newtonian physics, free fall is any motion of a body where gravity is the only force acting upon it.
Black hole and Free fall · Free fall and History of general relativity ·
General relativity
General relativity (GR, also known as the general theory of relativity or GTR) is the geometric theory of gravitation published by Albert Einstein in 1915 and the current description of gravitation in modern physics.
Black hole and General relativity · General relativity and History of general relativity ·
Georges Lemaître
Georges Henri Joseph Édouard Lemaître, RAS Associate (17 July 1894 – 20 June 1966) was a Belgian Catholic Priest, astronomer and professor of physics at the Catholic University of Leuven.
Black hole and Georges Lemaître · Georges Lemaître and History of general relativity ·
Gravitational lens
A gravitational lens is a distribution of matter (such as a cluster of galaxies) between a distant light source and an observer, that is capable of bending the light from the source as the light travels towards the observer.
Black hole and Gravitational lens · Gravitational lens and History of general relativity ·
Gravitational singularity
A gravitational singularity or spacetime singularity is a location in spacetime where the gravitational field of a celestial body becomes infinite in a way that does not depend on the coordinate system.
Black hole and Gravitational singularity · Gravitational singularity and History of general relativity ·
Gravitational time dilation
Gravitational time dilation is a form of time dilation, an actual difference of elapsed time between two events as measured by observers situated at varying distances from a gravitating mass.
Black hole and Gravitational time dilation · Gravitational time dilation and History of general relativity ·
Gravitational wave
Gravitational waves are the disturbance in the fabric ("curvature") of spacetime generated by accelerated masses and propagate as waves outward from their source at the speed of light.
Black hole and Gravitational wave · Gravitational wave and History of general relativity ·
Gravity
Gravity, or gravitation, is a natural phenomenon by which all things with mass or energy—including planets, stars, galaxies, and even light—are brought toward (or gravitate toward) one another.
Black hole and Gravity · Gravity and History of general relativity ·
Hendrik 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.
Black hole and Hendrik Lorentz · Hendrik Lorentz and History of general relativity ·
Karl Schwarzschild
Karl Schwarzschild (October 9, 1873 – May 11, 1916) was a German physicist and astronomer.
Black hole and Karl Schwarzschild · History of general relativity and Karl Schwarzschild ·
Kerr metric
The Kerr metric or Kerr geometry describes the geometry of empty spacetime around a rotating uncharged axially-symmetric black hole with a spherical event horizon.
Black hole and Kerr metric · History of general relativity and Kerr metric ·
Kerr–Newman metric
The Kerr–Newman metric is a solution of the Einstein–Maxwell equations in general relativity that describes the spacetime geometry in the region surrounding a charged, rotating mass.
Black hole and Kerr–Newman metric · History of general relativity and Kerr–Newman metric ·
Kip Thorne
Kip Stephen Thorne (born June 1, 1940) is an American theoretical physicist and Nobel laureate, known for his contributions in gravitational physics and astrophysics.
Black hole and Kip Thorne · History of general relativity and Kip Thorne ·
LIGO
The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool.
Black hole and LIGO · History of general relativity and LIGO ·
Loop quantum gravity
Loop quantum gravity (LQG) is a theory of quantum gravity, merging quantum mechanics and general relativity.
Black hole and Loop quantum gravity · History of general relativity and Loop quantum gravity ·
Martin David Kruskal
Martin David Kruskal (September 28, 1925 – December 26, 2006) was an American mathematician and physicist.
Black hole and Martin David Kruskal · History of general relativity and Martin David Kruskal ·
Quantum gravity
Quantum gravity (QG) is a field of theoretical physics that seeks to describe gravity according to the principles of quantum mechanics, and where quantum effects cannot be ignored, such as near compact astrophysical objects where the effects of gravity are strong.
Black hole and Quantum gravity · History of general relativity and Quantum gravity ·
Quantum mechanics
Quantum mechanics (QM; also known as quantum physics, quantum theory, the wave mechanical model, or matrix mechanics), including quantum field theory, is a fundamental theory in physics which describes nature at the smallest scales of energy levels of atoms and subatomic particles.
Black hole and Quantum mechanics · History of general relativity and Quantum mechanics ·
Reissner–Nordström metric
In physics and astronomy, the Reissner–Nordström metric is a static solution to the Einstein-Maxwell field equations, which corresponds to the gravitational field of a charged, non-rotating, spherically symmetric body of mass M. The metric was discovered by Hans Reissner, Hermann Weyl, Gunnar Nordström and G. B. Jeffery.
Black hole and Reissner–Nordström metric · History of general relativity and Reissner–Nordström metric ·
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.
Black hole and Roy Kerr · History of general relativity and Roy Kerr ·
Schwarzschild metric
In Einstein's theory of general relativity, the Schwarzschild metric (also known as the Schwarzschild vacuum or Schwarzschild solution) is the solution to the Einstein field equations that describes the gravitational field outside a spherical mass, on the assumption that the electric charge of the mass, angular momentum of the mass, and universal cosmological constant are all zero.
Black hole and Schwarzschild metric · History of general relativity and Schwarzschild metric ·
Spacetime
In physics, spacetime is any mathematical model that fuses the three dimensions of space and the one dimension of time into a single four-dimensional continuum.
Black hole and Spacetime · History of general relativity and Spacetime ·
String theory
In physics, string theory is a theoretical framework in which the point-like particles of particle physics are replaced by one-dimensional objects called strings.
Black hole and String theory · History of general relativity and String theory ·
The list above answers the following questions
- What Black hole and History of general relativity have in common
- What are the similarities between Black hole and History of general relativity
Black hole and History of general relativity Comparison
Black hole has 287 relations, while History of general relativity has 98. As they have in common 27, the Jaccard index is 7.01% = 27 / (287 + 98).
References
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