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Explore This is what happened immediately after the Big Bang || Part-1 with 3,247 views, 36 likes, and 28 comments. Experience the impact of this video content that has captured audience attention.

This Video explores the evolution of scientific perspectives on the origins and nature of the universe. The journey through the early universe encompasses several key epochs, each marked by distinct events and transformations. Around 13.8 billion years ago, the universe began with the enigmatic moment of the big bang singularity, a point of infinite density and temperature described by Einstein's general theory of relativity. The subsequent Planck epoch, lasting a mere fraction of a second, witnessed the universe in a state of extreme density and temperature, challenging our understanding of physics. The Grand Unification Epoch followed, during which fundamental forces like gravity, electromagnetism, and the strong and weak nuclear forces potentially unified at immensely high energy levels. This epoch gave rise to the electro weak force and saw the emergence of WIMPs, dark matter, and dark energy. The electroweak epoch, occurring around 1 trillion trillion trillionth seconds after the big bang, witnessed the separation of the electro weak force into distinct electro weak and strong nuclear forces. Exotic elementary particles, including W and Z bosons, made their appearance during this epoch. The subsequent Inflationary Epoch, occurring 1 billion trillion trillionths of a second after the big bang, provided a solution to various cosmic mysteries, such as the uniformity of the universe and the absence of magnetic monopoles. Inflation, a rapid volumetric expansion, set the stage for the formation of large-scale structures. The era of supersymmetry in the early universe posits perfect symmetry, suggesting the existence of hidden partner particles for known particles. However, these hidden partners remain elusive due to their potential high energy levels. Thermalization and Electroweak Symmetry Breaking marked the transition from a hot quark-gluon plasma to stable particles, including quarks, leptons, and matter-antimatter pairs. Baryogenesis addressed the observed imbalance of baryons and antibaryons, proposing mechanisms like electroweak baryogenesis and leptogenesis. The Quark Epoch, beginning around ten to the power of negative twelve seconds, witnessed the stabilization of fundamental interactions, paving the way for the emergence of the four fundamental forces: gravity, electromagnetism, the strong nuclear force, and the weak nuclear force. The universe persisted in a chaotic state until the end of this epoch. The Hadron Epoch, from around ten to the power of negative five seconds to 1 second after the Big Bang, marked the formation of hadrons, subatomic particles composed of quarks. Initially, a quark-gluon plasma transitioned to a state where hadrons, including protons and neutrons, could form. Hadron-antihadron pairs annihilated, leaving behind a residue that participated in nucleosynthesis, leading to the formation of elements like hydrogen and helium. Additional Sources: http://www.space.com/13347-big-bang-origins-universe-birth.html https://map.gsfc.nasa.gov/universe/ https://www.space.com/24054-how-old-is-the-universe.html https://www.sciencechannel.com/tv-shows/how-the-universe-works/full-episodes/first-second https://www.mpg.de/7044245/Planck_cmb_universe https://www.space.com/19027-universe-baby-picture-wmap.html https://www.jpl.nasa.gov/news/news.php?release=2014-082 http://hyperphysics.phy-astr.gsu.edu/hbase/Astro/planck.html Other Videos Link:- 1. The fundamental forces of Nature:- https://youtu.be/xU_zuvUiAyQ 2. Particle Physics playlist:- https://www.youtube.com/playlist?list=PLoaw7ytcH-HpwtGoP88SIhmF-7jsGUhPu

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