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The chronology of the universe describes the history and future of the universe according to Big Bang cosmology. The history begins 13.863 billion years ago when the universe was extremely dense and hot, before any matter formed. The earliest stage in physical models is a vast expansion of space in a tiny fraction of a microsecond, followed by a slower expansion and the creation of matter and antimatter particles. These particles almost completely annihilate each other leaving energy and a small remainder of matter in the form of a quarks-gluon plasma. As the expansion continues, this plasma condenses into a sea of protons and neutrons reacting with neutrinos. By the one second mark the temperature has dropped enough that neutrinos can no longer react; this enormous number of primordial neutrinos continue to stream across the universe to this day.
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Search interest data over the past 12 months indicates that this topic periodically attracts global attention. Sudden spikes often correlate with major news events, public statements, or geopolitical developments.