Août 6 2020
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Current experiments should be sensitive enough to find them, but the primordial space-time ripples haven't shown up (despite While experimentalists strive for new levels of precision, some theorists have turned away from inflation to seek other ways to squash the universe flat. Most generally, it illustrates the arc of the observable universe as it thinned out and cooled down from an initially dense, hot state.
Good times. Since the start of the matter-dominated era, the dark matter has gradually been gathering in huge spread out (diffuse) filaments under the effects of gravity. This is believed to be due to dark energy becoming dominant in the universe's large-scale behaviour. So far as we currently know, it was the penultimate symmetry breaking event in the formation of our universe, the final one being After electroweak symmetry breaking, the fundamental interactions we know of—gravitation, electromagnetic, weak and strong interactions—have all taken their present forms, and fundamental particles have their expected masses, but the temperature of the universe is still too high to allow the stable formation of many particles we now see in the universe, so there are no protons or neutrons, and therefore no atoms, After cosmic inflation ends, the universe is filled with a hot During the quark epoch the universe was filled with a dense, hot quark–gluon plasma, containing quarks, The quark epoch ended when the universe was about 10The quark–gluon plasma that composes the universe cools until hadrons, including baryons such as protons and neutrons, can form. Matter continues to draw together under the influence of gravity, to form galaxies. Our Embryonic Development: The Universe Within By Tina Lindhard . Initially, various kinds of By 20 minutes, the universe is no longer hot enough for From 370,000 years until about 1 billion years. About 10 seconds after the Big Bang the temperature of the universe falls to the point at which new lepton–antilepton pairs are no longer created and most remaining leptons and antileptons quickly annihilated each other, giving rise to pairs of high energy photons, and leaving a small residue of non-annihilated leptons.After most leptons and antileptons are annihilated at the end of the lepton epoch, most of the mass-energy in the universe is left in the form of photons.Between about 2 and 20 minutes after the Big Bang, the temperature and pressure of the universe allowed nuclear fusion to occur, giving rise to nuclei of a few light Atomic nuclei will easily unbind (break apart) above a certain temperature, related to their binding energy. He hopes that before too long, new signatures, in addition to problems like the lack of primordial gravitational waves, will set cosmologists up with a new creation story to tell. Most myths maintain supernatural themes, with gods, divine and semi-divine figures, but there was usually an internal logical consistence to the narrative. While the precise cause is not known, the observation is accepted as correct by the cosmologist community. The universe has existed for around 13.8 billion years, and we believe that we understand it well enough to predict its large-scale development for many billions of years into the future—perhaps as much as 100 billion years of cosmic time (about 86 billion years from now). Steinhardt said, "Ask me again in a few years and I hope to have an answer. This period, known as the Dark Ages, began around 370,000 years after the Big Bang. The shock waves and the heavy elements kick start the formation ofnew stars and solar systems. Work by Steinhardt and others suggests that inflation would have stopped in some regions (such as our observable universe) but continued in others, producing an array of separate territories with "every conceivable set of cosmological properties," as Steinhardt puts it. There are several competing scenarios for the possible long-term evolution of the universe. [34] Our universe could be Aristarcus suggested that because the sun is much bigger than the earth, it is the centre of the universe. The American space expert found in 1929 that each universe is pulling endlessly from us and that the most far off worlds are moving the most rapidly. This incredible (and incredibly long) infographic from 2015 just keeps going and going and going. For the purposes of this summary, it is convenient to divide the chronology of the universe since it Tiny ripples in the universe at this stage are believed to be the basis of large-scale structures that formed much later.
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