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Bookmark or Share- Rip, Crunch, Freeze: The Three Fates of our Universe – Hadron - IMSAIt’s Crunch Time: The Big Crunch. If the k parameter exceeds 0, then the density of the universe will be greater than it’s critical mass density and gravity will take over as the main driving force. Eventually gravity will overpower the force of dark energy, a constant value in our universe. There are two possible outcomes that could result ...
- Crunch, rip, freeze or decay — how will the Universe end? - NatureThe Big Crunch. Astrophysicists long considered the most likely denouement to be a reversal of the Big Bang — the Big Crunch. Outside our cosmic neighbourhood, every galaxy is zooming away from ...
- Ultimate fate of the universe - WikipediaThe Big Crunch. The vertical axis can be considered as expansion or contraction with time. The Big Crunch hypothesis is a symmetric view of the ultimate fate of the universe. Just as the theorized Big Bang started as a cosmological expansion, this theory assumes that the average density of the universe will be enough to stop its expansion and ...
- WMAP- Fate of the Universe - NASAThe “Big Crunch” The evolution of the universe is determined by a struggle between the momentum of expansion and the pull (or push!) of gravity. The current rate of expansion is measured by the Hubble Constant, while the strength of gravity depends on the density and pressure of the matter in the universe. If the pressure of the matter is ...
- How the Big Crunch Theory Works | HowStuffWorksAlthough How the Big Bang Theory Works covers the origin of the universe in detail, it will be useful to cover the basics here. The short version goes like this: About 15 billion years ago, all matter and energy was bottled up in an incredibly small region known as a singularity.In an instant, this single point of super-dense material began to expand at an astonishingly rapid rate.
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