WebDuring decoupling, about 400,000 years after the Big Bang, the temperature was finally low enough (about 3,000 K) for neutral atoms to form. Before then, the universe was largely …
What existed before the Big Bang? - BBC Future
WebA. beginning of particle production, about .0001 seconds into the universe. B. end of the Planck Era, about 10-43 seconds after the Big Bang. C. end of the Inflationary Epoch, … WebSelect one: A. decoupling Event, about a million years after the Big Bang. B. end of the Inflationary Epoch, about 10-32 seconds into creation. C. beginning of particle production, about .0001 seconds into the universe. D. end of the Planck Era, about 10-43 seconds after the Big Bang. E. end of electron production, about a minute after creation. how to report inventory on taxes
The Creation of Helium - University of Oregon
WebMay 30, 2024 · Hydrogen formed pretty much instantly and even helium (with nuclei containing 2 protons) formed in relatively short order (part of a process referred to as Big Bang nucleosynthesis). As this hydrogen and helium began to form in the early universe, there were some areas where it was denser than in others. WebAfter the Big Bang, the universe was like a hot soup of particles (i.e. protons, neutrons, and electrons). When the universe started cooling, the protons and neutrons began combining into ionized atoms of hydrogen (and eventually some helium). These ionized atoms of hydrogen and helium attracted electrons, turning them into neutral atoms - which … The recombination epoch begins at around 18,000 years, as electrons are combining with helium nuclei to form He+ . At around 47,000 years, [2] as the universe cools, its behavior begins to be dominated by matter rather than radiation. At around 100,000 years, after the neutral helium atoms form, helium hydride is the … See more The chronology of the universe describes the history and future of the universe according to Big Bang cosmology. Research published in 2015 estimates the earliest stages of the universe's existence as taking place 13.8 See more The Standard Model of cosmology is based on a model of spacetime called the Friedmann–Lemaître–Robertson–Walker (FLRW) metric. A metric provides a measure of distance between objects, and the FLRW metric is the exact solution of Einstein field equations See more After cosmic inflation ends, the universe is filled with a hot quark–gluon plasma, the remains of reheating. From this point onwards the … See more The universe has appeared much the same as it does now, for many billions of years. It will continue to look similar for many more billions of years into the future. Based upon the … See more Chronology in five stages For the purposes of this summary, it is convenient to divide the chronology of the universe since it See more During the earliest moments of cosmic time, the energies and conditions were so extreme that current knowledge can only suggest possibilities, which may turn out to be incorrect. To … See more 370 thousand to about 1 billion years after the Big Bang Dark Ages After recombination and decoupling, the universe was transparent and had cooled enough to allow light to travel long distances, but there … See more how to report involuntary conversion on 4797