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 10â32 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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