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Friedmann and while
" Within the Friedmann – Lemaître – Robertson – Walker ( FLRW ) model, the presently most popular shape of the Universe found to fit observational data according to cosmologists is the infinite flat model, while other FLRW models that fit the data include the Poincaré dodecahedral space and the Picard horn.
This behavior is well studied in the Greater Honeyguide ; some authorities ( following Friedmann, 1955 ) state that it also occurs in the Scaly-throated Honeyguide, while others disagree ( Short and Horne, 2002 ).

Friedmann and with
Whilst in Vienna, working to aid refugees from Nazi Germany, Philby met and fell in love with Litzi Friedmann ( born Alice Kohlmann ), a young Austrian Communist of Hungarian Jewish origins.
Philby and Litzi Friedmann married in February 1933, enabling her to escape to the United Kingdom with Philby two months later.
This animation illustrates a closed Friedmann universe with zero cosmological constant Λ ; such a universe oscillates between a Big Bang and a Big Crunch.
The equation describing how R varies with time is known as the Friedmann equation, after its inventor, Alexander Friedmann.
Later, in 1931, Einstein himself agreed with the results of Friedmann and Lemaître.
However, soon after Einstein developed his static theory, observations by Edwin Hubble indicated that the universe appears to be expanding ; this was consistent with a cosmological solution to the original general-relativity equations that had been found by the mathematician Friedmann.
The idea comes from a perceived need to reconcile Edwin Hubble's observation of an expanding universe ( which was also predicted from Einstein's equations of general relativity by Alexander Friedmann ) with the notion that the universe must be eternally old.
* 2003 of Ingmar Thilo ; with Antonios Safralis ( Faust ), Raphaela Zick ( Mephisto ), Ulrike Dostal ( Helena ), Max Friedmann ( Lynceus ), and others
His mother was Alice Friedmann, an Ashkenazi Viennese Jew with roots in Galicia, and his father was Dr. Samuel Djerassi, a Bulgarian Sephardic Jew.
In this work the Friedmann equations emerge from an elliptic solution of the Vlasov equation coupled with Poisson's equation.
According to the Friedmann – Lemaître – Robertson – Walker metric which is used to model the expanding universe, if at the present time we receive light from a distant object with a redshift of z, then the scale factor at the time the object originally emitted that light is given by the equation.
" His repeated negationist statements on the topic of Nazi genocide brought Degrelle to trial with Violeta Friedmann, a Romanian-born Venezuelan survivor of the camps ; although the lower courts were initially favourable to Degrelle, the Supreme Court of Spain decided that he had brought offence to the memory of the victims, both Jews and non-Jews, and it sentenced him to pay a substantial fine.
They were first derived by Alexander Friedmann in 1922 from Einstein's field equations of gravitation for the Friedmann-Lemaître-Robertson-Walker metric and a fluid with a given mass density and pressure.
The Friedmann equations start with the simplifying assumption that the universe is spatially homogeneous and isotropic, i. e. the Cosmological Principle ; empirically, this is justified on scales larger than ~ 100 Mpc.
Applied to a fluid with a given equation of state, the Friedmann equations yield the time evolution and geometry of the universe as a function of the fluid density.
The first Friedmann equation is often seen in a form with density parameters.
The Friedmann equations can be solved exactly in presence of a perfect fluid with equation of state
* Daniel E. Friedmann, an engineering physicist and CEO of MacDonald, Dettwiler and Associates ( an aerospace corporation ), has demonstrated an alignment between the dates of key events as described in Genesis Chapters 1 and 2 with dates derived from scientific theory and observation, thus solving the perceived discrepancy between the biblical and scientific timelines.
* From 1881 to 1886 Friedmann published, together with Isaac Hirsh Weiss, the monthly Bet Talmud, devoted to rabbinical studies.
The accused were defended by Károly Eötvös, journalist and member of the House of Deputies, with whom were associated the advocates B. Friedmann, Sándor Funták, Max Székely of Budapest, and Ignác Heumann of Nyíregyháza, the seat of the county court before which the case was tried.

Friedmann and for
According to observations of structures larger than solar systems, as well as Big Bang cosmology interpreted under the Friedmann equations and the FLRW metric, dark matter accounts for 23 % of the mass-energy content of the observable universe.
In 1972 Friedmann and Roblin authored a paper in Science titled " Gene therapy for human genetic disease?
That leads to a single form for the metric tensor, called the Friedmann – Lemaître – Robertson – Walker metric
Gamow studied under Alexander Friedmann for some time in Leningrad, until Friedmann died in 1925.
* Friedmann – Lemaître – Robertson – Walker metric for information about the most popular cosmological model
The Friedmann – Lemaître – Robertson – Walker metric that is necessary for the Big Bang and Steady State models emerged in the decade after the development of Einstein's general relativity and was accepted as a model for the universe after Edwin Hubble's discovery of his eponymous law.
Writing for the journal Neurotica in 1951, Dr. Rudolph Friedmann studied the stories so intensely for analytic psychosexual imagery that Dwight Macdonald was moved to include the essay in his 1960 anthology of parodies as a sincere but inadvertent example of the form.
The equations for negative spatial curvature were given by Friedmann in 1924.
There are two independent Friedmann equations for modeling a homogeneous, isotropic universe.
Some cosmologists call the second of these two equations the Friedmann acceleration equation and reserve the term Friedmann equation for only the first equation.
An expression for the critical density is found by assuming Λ to be zero ( as it is for all basic Friedmann universes ) and setting the normalised spatial curvature, k, equal to zero.
( He had used Friedländer as a pen name for several of his publications, but had not used his family name Friedmann since his student days.
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.

Friedmann and critical
The density parameter,, is defined as the ratio of the actual ( or observed ) density to the critical density of the Friedmann universe.
Friedmann has devoted himself chiefly to the editing of old Midrashim, to which he has added critical notes and valuable introductions.

Friedmann and Midrash
Midrash Sifre, Numbers 2 Friedmann, p. 2a ).

Friedmann and early
The cosmological solutions of general relativity were found by Alexander Friedmann in the early 1920s.

Friedmann and .
The governing equations had been formulated by Alexander Friedmann.
Ten years later, Alexander Friedmann, a Russian cosmologist and mathematician, derived the Friedmann equations from Albert Einstein's equations of general relativity, showing that the Universe might be expanding in contrast to the static Universe model advocated by Einstein at that time.
During the 1930s other ideas were proposed as non-standard cosmologies to explain Hubble's observations, including the Milne model, the oscillatory Universe ( originally suggested by Friedmann, but advocated by Albert Einstein and Richard Tolman ) and Fritz Zwicky's tired light hypothesis.
* Yohanan Friedmann: Classification of Unbelievers in Sunnī Muslim Law and Tradition.
The most well-noted of these are object-relative clauses, object Wh-questions, and topicalized structures ( placing the topic at the beginning of the sentence ).< ref name =" Friedmann "> Friedmann, Naama, Aviah Gvion, and Rama Novogrodsky.
This is readily described by the expanding cosmological solutions found by Friedmann in 1922, which do not require a cosmological constant.
The best-known exact solutions, and also those most interesting from a physics point of view, are the Schwarzschild solution, the Reissner – Nordström solution and the Kerr metric, each corresponding to a certain type of black hole in an otherwise empty universe, and the Friedmann – Lemaître – Robertson – Walker and de Sitter universes, each describing an expanding cosmos.
Bach in Leipzig, such as Wilhelm Friedmann Bach, Carl Philipp Emmanuel Bach and Johann Friedrich Agricola, as well as those composers who performed under his direction in Leipzig ( Christoph Graupner, Johann David Heinichen and Johann Georg Pisendel ), composers of the Berlin lieder school, and finally, his numerous pupils, none of whom, however, became major composers.
* 1888 – Alexander Friedmann, Russian physicist and mathematician ( d. 1925 )
Peter Wright, former senior MI5 officer, said in his 1987 book that Litzi Friedmann was " almost certainly the person who recruited him to the Soviet cause.
In February 1934, Philby married Alice ( Litzi ) Friedmann, an Austrian communist whom he had met in Vienna.
* Ronald Friedmann: Klaus Fuchs.
These observations corroborated Alexander Friedman's 1922 work, in which he derived the famous Friedmann equations.
In cosmology, the Cardassian expansion is a modification to the Friedmann equations.

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