Einsteinian$528036$ - meaning and definition. What is Einsteinian$528036$
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What (who) is Einsteinian$528036$ - definition

RIEMANNIAN OR PSEUDO-RIEMANNIAN DIFFERENTIABLE MANIFOLD WHOSE RICCI TENSOR IS PROPORTIONAL TO THE METRIC
Einsteinian manifold; Einstein metric; Einstein space; Kähler-Einstein manifold; Kahler-Einstein manifold; Kaehler-Einstein manifold; Einstein metrics

Einstein manifold         
In differential geometry and mathematical physics, an Einstein manifold is a Riemannian or pseudo-Riemannian differentiable manifold whose Ricci tensor is proportional to the metric. They are named after Albert Einstein because this condition is equivalent to saying that the metric is a solution of the vacuum Einstein field equations (with cosmological constant), although both the dimension and the signature of the metric can be arbitrary, thus not being restricted to Lorentzian manifolds (including the four-dimensional Lorentzian manifolds usually studied in general relativity).
Einstein         
  • Start of a speech by Albert Einstein made on 11 April 1943 for the United Jewish Appeal (recording by Radio Universidad Nacional de La Plata, Argentina)
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"Ladies (coughs) and gentlemen, our age is proud of the progress it has made in man's intellectual development. The search and striving for truth and knowledge is one of the highest of man's qualities ..."
  • 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" />
  • Eddington]]'s photograph of a [[solar eclipse]].
  • Einstein's ''[[Matura]]'' certificate, 1896<ref group=note name=MaturaScore />
  • Einstein's official portrait after receiving the 1921 Nobel Prize in Physics
  • Einstein in 1947
  • Hollywood]] premiere of ''[[City Lights]]'', January 1931
  • Salvation Army]] band before a performance at the [[Rose Bowl Parade]], in California, 1926.
  • Albert Einstein and [[Mileva Marić]] Einstein, 1912
  • Einstein in 1893 (age&nbsp;14)
  • Einstein at the age of three in 1882
  • Einstein at his office, [[University of Berlin]], 1920
  • Einstein during his visit to the United States
  • US citizenship]] certificate from judge [[Phillip Forman]]
  • Albert Einstein's landing card (26 May 1933), when he landed in [[Dover]] (United Kingdom) from [[Ostend]] (Belgium) to visit [[Oxford]]
  • Heinrich Goldschmidt]] is at the left, [[Ole Colbjørnsen]] in the center and [[Jørgen Vogt]] sits behind Ilse Einstein.
  • 1933}})
  • Portrait of Einstein taken in 1935 at Princeton
  • [[Olympia Academy]] founders: [[Conrad Habicht]], [[Maurice Solovine]] and Albert Einstein
  • Einstein with his second wife, Elsa, in 1921
  • Einstein in 1904 (age&nbsp;25)
  • Albert Einstein with his wife [[Elsa Einstein]] and Zionist leaders, including the future president of Israel, [[Chaim Weizmann]], his wife [[Vera Weizmann]], [[Menahem Ussishkin]], and Ben-Zion Mossinson on arrival in New York City in 1921
  • Albert Einstein at a session of the [[International Committee on Intellectual Cooperation]] ([[League of Nations]]) of which he was a member from 1922 to 1932
  • Millikan]] and [[Georges Lemaître]] at the [[California Institute of Technology]] in January 1933
  • Newspaper headline on 4 May 1935
  • Einstein and [[Niels Bohr]], 1925
  • The photoelectric effect. Incoming photons on the left strike a metal plate (bottom), and eject electrons, depicted as flying off to the right.
  • The 1927 [[Solvay Conference]] in Brussels, a gathering of the world's top physicists. Einstein is in the center.
GERMAN-BORN THEORETICAL PHYSICIST; DEVELOPER OF THE THEORY OF RELATIVITY (1879–1955)
Einstein; Albert Eienstein; Albert Einstien; Albert einstein; Einstien; Einsteinian; Einsetein; Albert Enstein; Albert Einstein's; Einstein, Albert; Albert Enstien; Alber Enstien; Albert Einstin; A. Einstein; Alber Einstein; Einstein (physicist); Albrecht Einstein; Albert eintein; Chasing a light beam; I want to go when I want. It is tasteless to prolong life artificially. I have done my share, it is time to go. I will do it elegantly.
['??nst??n]
¦ noun informal a genius.
Origin
the name of the German-born physicist Albert Einstein (1879-1955).
Special relativity         
  • Figure 5–4. Comparison of the measured length contraction of a cube versus its visual appearance.
  • Figure 10–3. Concentric spheres, illustrating in 3-space the null geodesics of a 4-dimensional cone in spacetime.
  • Figure 6-2. Newtonian analysis of the elastic collision of a moving particle with an equal mass stationary particle
  • Figure 5–1. Highly simplified diagram of Fizeau's 1851 experiment.
  • Figure 2–1. The primed system is in motion relative to the unprimed system with constant velocity ''v'' only along the ''x''-axis, from the perspective of an observer stationary in the unprimed system. By the [[principle of relativity]], an observer stationary in the primed system will view a likewise construction except that the velocity they record will be −''v''. The changing of the speed of propagation of interaction from infinite in non-relativistic mechanics to a finite value will require a modification of the transformation equations mapping events in one frame to another.
  • M87]] streams out a black-hole-powered jet of electrons and other sub-atomic particles traveling at nearly the speed of light.
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  • Figure 6-3. Relativistic elastic collision between a moving particle incident upon an equal mass stationary particle
  • 1=''v'' = −0.5''c''}} with respect to '''O''', the events occur in the order A, B, C. The white lines, the ''lines of simultaneity'', move from the past to the future in the respective frames (green coordinate axes), highlighting events residing on them. They are the locus of all events occurring at the same time in the respective frame. The gray area is the [[light cone]] with respect to the origin of all considered frames.
  • Figure 4–3. [[Light cone]]
  • Figure 10–2. Three-dimensional dual-cone.
  • Figure 5–2. Illustration of stellar aberration
  • Figure 5–5. Comparison of the measured length contraction of a globe versus its visual appearance, as viewed from a distance of three diameters of the globe from the eye to the red cross.
  • Figure 5–3. Transverse Doppler effect for two scenarios: (a) receiver moving in a circle around the source; (b) source moving in a circle around the receiver.
PHYSICAL THEORY OF MEASUREMENT IN AN INERTIAL FRAME OF REFERENCE PROPOSED IN 1905 BY ALBERT EINSTEIN
Special theory of relativity; Special Relativity; Specialrelativity; Time-Space Conversion Ratio; Theoretical total mass-energy; Sqecial relativity; Consequences of special relativity; Introduction to special relativity; Special Theory of Relativity; Principle of Special Relativity; Principle of special relativity; Theory of special relativity; Special relativity for mathematicians; Special relativity (simplified); Theory of Special Relativity; Special relativity for beginners; Introduction to Special Relativity; Introduction to Special relativity; Consequences of Special Relativity; Intro to special relativity; Einstein's Special Theory Of Relativity; Einstein's Special Theory of Relativity; Theory Of Special Relativity; Relativistic velocities; Super-classical limit; Special theory of Relativity; Introduction to the special theory of relativity; Introduction to special theory of relativity; Special Rel; The Special Theory of Relativity; Einsteinian speed limit; Cosmic speed limit; Special Relativty
In physics, the special theory of relativity, or special relativity for short, is a scientific theory regarding the relationship between space and time. In Albert Einstein's original treatment, the theory is based on two postulates:

Wikipedia

Einstein manifold

In differential geometry and mathematical physics, an Einstein manifold is a Riemannian or pseudo-Riemannian differentiable manifold whose Ricci tensor is proportional to the metric. They are named after Albert Einstein because this condition is equivalent to saying that the metric is a solution of the vacuum Einstein field equations (with cosmological constant), although both the dimension and the signature of the metric can be arbitrary, thus not being restricted to Lorentzian manifolds (including the four-dimensional Lorentzian manifolds usually studied in general relativity). Einstein manifolds in four Euclidean dimensions are studied as gravitational instantons.

If M is the underlying n-dimensional manifold, and g is its metric tensor, the Einstein condition means that

R i c = k g {\displaystyle \mathrm {Ric} =kg}

for some constant k, where Ric denotes the Ricci tensor of g. Einstein manifolds with k = 0 are called Ricci-flat manifolds.