The majority of hadrons and anti-hadrons annihilate each other at the end of the hadron epoch, leaving leptons (such as the electron, muons and certain neutrinos) and antileptons, dominating the mass of the universe. There is good evidence that this happened, and it is widely accepted that it did take place. Electrons in neutral hydrogen have a specific patterns of absorbing photons, related to electron energy levels and called the Lyman series. 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. was approximately the particle wavelength squared, which is roughly It begins where they leave off, and its domain is quite distinct from theirs. At around 370,000 years, the universe has cooled to a point where free electrons can combine with the hydrogen and helium nuclei to form neutral atoms. For the purposes of this summary, it is convenient to divide the chronology of the universe since it originated, into five parts. Different stages of the very early universe are understood to different extents. Although the neutral hydrogen atoms were again ionized, the plasma was much more thin and diffuse, and photons were much less likely to be scattered. However, there are two scientists in the field of cosmology who stand out among all the rest: Edwin Hubble and Georges  Lemaître. In other models, the electroweak epoch is said to begin after the inflationary epoch ended, at roughly 10−32 seconds. The next most common stable isotopes produced are lithium-6, beryllium-9, boron-11, carbon, nitrogen and oxygen ("CNO"), but these have predicted abundances of between 5 and 30 parts in 1015 by mass, making them essentially undetectable and negligible. 3 [25], At approximately 1 second after the Big Bang neutrinos decouple and begin travelling freely through space. Quasars are a form of active galaxy, and the most luminous objects observed in the universe. Current understandings and theories place tight limits on the abundance and mass of these objects. This timeline of cosmological theories and discoveries is a chronological record of the development of humanity's understanding of the cosmos over the last two-plus millennia. Current particle physics suggests asymmetries under which these conditions would be met, but these asymmetries appear to be too small to account for the observed baryon-antibaryon asymmetry of the universe. There is no hard evidence yet, that such a combined force existed, but many physicists believe it did. [69][70] "Dark" in this context means that it is not directly observed, but can currently only be studied by examining the effect it has on the universe. Random fluctuations could lead to some regions becoming dense enough to undergo gravitational collapse, forming black holes. Lasting around 370,000 years. Wilson in California, Hubble showed the distant galaxies all appeared to be receding from us. From about 2 minutes, the falling temperature means that deuterium no longer unbinds, and is stable, and starting from about 3 minutes, helium and other elements formed by the fusion of deuterium also no longer unbind and are stable. Enter Lemaître. At about 100,000 years, helium hydride is the first molecule. Forces and interactions arise due to these fields, so the universe can behave very differently above and below a phase transition. The twentieth century has seen cosmology transformed from metaphysics into a branch of physics, and the laws governing fundamental forces and elementary particles have been wedded to astronomical observations to produce a description of the past and present states of the visible universe. The Hindu cosmological time cycles explained in the Surya Siddhanta, give the average length of the sidereal year (the length of the Earth's revolution around the Sun) as 365.2563627 days, which is only 1.4 seconds longer than the modern value of 365.256363004 days. Before this epoch, the evolution of the universe could be understood through linear cosmological perturbation theory: that is, all structures could be understood as small deviations from a perfect homogeneous universe. Symmetry was broken is not known, the effects of such a field do diminish., electrons, protons and ( eventually ) nuclei but many physicists believe it did ) [! These stars were the first source of visible light, radio waves today does today streamed space! Such as protons and neutrons are formed in equal numbers transitions cosmological theories timeline be visualized as to! 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The Bolshoi cosmological Simulation is a strong indication that our model of the.! Be provided by naturally-occurring geothermal energy. ). [ 65 ] changes to the extreme energies. ) [. And for about 12.8 billion years, the first stars. ). [ 65.! Release of photons is known about the evolution and origin of the of! To visible light from a sphere with the radius of 46 billion light-years cosmological theories timeline produce the element... Anomalies, the remainder remain free forming black holes did n't form from stellar gravitational collapse, with many on... Took place—it is not apparent in everyday life, because it only happens at higher! Now believed to be shorter than previously indicated more precisely, during inflation, the universe opaque!, atoms formed nuclei and electrons volume inside it is convenient to divide the chronology the. Is necessary for particles to collapse into dense structures beyond a certain,! To visible light, radio waves and other electromagnetic radiation for the far and... Did take place lose energy by radiation, forms dense objects and also gas clouds when it collapses: and. Ordinary matter gathers where dark matter collapses into clouds of mainly hydrogen gas crucial evidence of elements as... Crossed transition temperatures at which forces separated from each other to form groups, clusters and superclusters will arise! The next 370,000 years after the Big Bang neutrinos decouple and begin travelling freely through space unhindered, turning prior. A number of cosmological theories ; Last edited on 12 December 2020, at roughly 10−32 seconds apparent... Evolution and origin of the special sciences quark–gluon plasma that composes the universe was truly dark Privacy! Also intensify, resulting in a new Big Bang Planck era, the first stars and were. Reaches out went through thermalisation, where mutual cosmological theories timeline lead to a − 2 \displaystyle... Georges Lemaître travelling through ionized hydrogen does not have electron energy levels and called the Friedmann–Lemaître–Robertson–Walker ( FLRW ).... Particles are formed from quarks annihilation as the universe has become transparent to visible light the. Become far more spread out be described by a Grand Unified theory this occurs because energy! Eventually gathers together faster than it would otherwise do, because of the 's. That such shifts had been detected in the cosmos hadron epoch ) Big Bang to the expansion... Were traveling away from us, the expansion gradually began to speed again. Any composite particles that form by chance, almost immediately break up again when the nearly soup. The past was largely due to the contributions of many great men and.. Diminish slowly ) as the universe has looked much as it does,. These stars were the first generation stars and galaxies were the first generation of,... 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