Heti posta, 1912
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Heti posta, 1912

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Mamås Friedmann, csålé gyertyåval.
Boldog szĂŒletĂ©snapot, Apu!
âLes ReprĂ©sentantsâ sculpture de Gloria Friedmann (2022) dans le cadre de Paris Art Basel au Jardin des Tuileries, octobre 2023.
The Most Important Equation In The Universe
"The first Friedmann equation describes how, based on what is in the universe, its expansion rate will change over time. If you want to know where the Universe came from and where it's headed, all you need to measure is how it is expanding today and what is in it. This equation allows you to predict the rest!"
In 1915, Einstein put forth General Relativity as a new theory of gravity. It reproduced all of Newtonâs earlier successes, solved the problem that Newton couldnât of Mercuryâs orbit, and made a new prediction of bent starlight by large masses, verified during the 1919 solar eclipse. Despite the fact that it included a cosmological constant to keep the Universe static, that didnât deter Soviet physicist Alexander Friedmann from solving Einsteinâs equations for a Universe that was filled with matter and energy, all the way back in 1922. The two generic equations he found, known as the Friedmann equations, immediately related measurable quantities like the amount of matter in the Universe to the expansion or contraction rate, which just years later became validated by Hubbleâs observations. But the young Friedmann never lived to see it; he died of typhoid fever contracted when he was returning from his honeymoon in 1925.
Nearly 100 years later, it still stands as the equation that determines the history and fate of the Universe. Come see why I call it the most important equation in the Universe!
Des Petits Tailleursâ, ELLE France, March 1991Photographer: Friedmann HaussModel: Beverly Peele.

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Portrait of Rose von Rothsorn Friedmann, by Gustav Klimt (1901).
Az igazi Friedmann nem olyan, mint az igazi Trebitsch, nem, egy sĂŒtirĆl van szĂł. NĂ©hĂĄny bejegyzĂ©ssel ezelĆtt ismĂ©t megemlĂtettem, hogy az Or
A hozzĂĄvalĂłk:
30 dkg (kicsit kevesebb, mint mĂĄsfĂ©l guriga) GyĆri Ădes zabkeksz
10 dkg vaj
15 dkg csoki
1,5 dl tejszĂn
1 doboz (20 dkg) natĂșr krĂ©msajt
2 dl tejszĂn
kb. 50 dkg eper
åtlåtszó tortazselé a tetejére
1. A zabkekszet ledarĂĄljuk, összekeverjĂŒk a vajjal, Ă©s 29 cm ĂĄtmĂ©rĆjƱ (Ă©n ekkorĂĄban kĂ©szĂtem, ikeĂĄs) piteformĂĄban egyenletesen elrendezzĂŒk Ășgy, hogy vĂ©gig a peremet is fedje a keksz. 180 fokos sĂŒtĆben 12 percig sĂŒtjĂŒk, majd kivesszĂŒk, hƱlni hagyjuk.
2. A csokit összeolvasztjuk (Ă©n mikrĂłban) a tejszĂnnel. Ăgy szoktam, hogy egy bögrĂ©be tördelem a csokit, råöntöm a tejszĂnt, Ă©s kb. mĂĄsfĂ©l percre teszem a mikrĂłba â a tejszĂn felforr, de ne fusson ki⊠UtĂĄna mĂĄr csak keverem, amĂg a csoki Ă©s a tejszĂn tökĂ©letesen nem elegyedik. A keverĂ©ket a kekszalapra öntöm, kihƱtöm.
3. FelverjĂŒk a tejszĂnt 2 ek cukorral, majd hozzĂĄadjuk a krĂ©msajtot. Eloszlatjuk a csokin.
4. Az epret felszeleteljĂŒk, szĂ©pen elrendezzĂŒk a sajtos krĂ©men, majd befedjĂŒk a leĂrĂĄsnak megfelelĆen elkĂ©szĂtett tortazselĂ©vel.
Minden Ăgy, csak cm tk KekszbĆl, eper helyett mĂĄlnĂĄval Ă©s Dr.Oetker expressz zselatinnal.
Ask Ethan: If the Universe is expanding, why arenât we?
âIf the universe is expanding at rates in excess of the speed of light, why does it not appear to affect our solar system and the planetary distances from the sun, etc.? And why would the relative distances of stars in our galaxy not appear to be increasing... or are they?â
It's a thing of scientific beauty that we've not only been able to determine that the Universe is expanding, but that we've been able to measure the rate of expansion so incredibly well. To better than 90% uniformity, we've determined the expansion rate in all directions and going back billions of years, allowing us to determine what's in the Universe, how that's changed over time, and what its fate is. It's one of the most remarkable achievements of modern science over the last 100 years. But even though the distant galaxies are all expanding away both from us and from one another, not everything in the Universe is expanding. Individual galaxy clusters remain bound; galaxies do not grow; planetary orbits remain constant; stars, planets, humans and even atoms remain the same size. Yet, the fabric of the Universe itself still continues to expand.
Why is this the case? Why don't these smaller-scale objects expand along with the fabric of the Universe, while everything else does? Find out on this week's Ask Ethan!