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The universe began with a turbulently charged explosion from a minuscule core, thrusting rapidly toward its outside limits; thus, the life cycle of the cosmos commenced. This cycle continues today. The three possibilities of this expanding universe are that the universe is “open,” “flat,” or “closed.” An open universe means that the universe will continue to expand at an ever-increasing rate forever. If the universe is flat, then the expansion rate will slow down, but the universe will never collapse. Instead, all movement will end in an eternal frozen waste. If the universe is closed, then it will expand only until it reaches a certain point, at which the process will be reversed and the universe will shrink until it collapses.

In the universe, dark energy overwhelms everyday gravity and outweighs the visible universe by a factor of 10 to 1. If the big bang model of the universe is right, the universe is expanding, and if there is enough mass in the universe, at some point the expansion will halt and gravitational forces will cause the universe to collapse on itself. However, if there is insufficient matter, the universe will expand forever and will eventually cool off completely to die a slow death. This would be the end point of a closed universe. If, and only if, there is sufficient mass to halt the expansion, or Hubble flow, movement will be reversed. Instead of galaxies moving rapidly outward, they would move back toward the center. If the existing diffusion velocity of the universe, in units of kilometers per second per mega parsec, slows in relation to the apparent velocity of recession of a galaxy to its distance from the Milky Way, this would mean the universe is aging. If this end result occurs, the big crunch would create the conditions for a new big bang.

It had been postulated that the universe began about 15 billion years ago with a big bang, starting from an infinitesimally small point of “not anything at all” in the empty space of “nothing” in which matter and time did not exist. A very small point of matter appeared and then exploded and began expanding outward at an ever-increasing tempo. This was only the beginning, and it is still expanding today. As the universe expands, more and more matter is shaped into more complex forms. If the universe is a flat universe, then everything will stop and die in cold empty darkness. If it is a closed universe, then it will collapse in on itself.

The big crunch theory, as outlined by Alexander Friedmann (1888–1925), states that if the density of matter in the universe is sufficiently large, gravitational forces between the matter will eventually cause the universe to stop expanding; then it will start falling back in. It will eventually end in a second cataclysmic event such as the big bang. The big crunch theory is completely dependent upon whether or not matter is dense enough in the universe. If astronomers correctly calculated the quantity of matter in all visible stars and galaxies, this would be too litde to stop expansion, let alone start contraction.

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