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HOW WILL OUR UNIVERSE END!?

The Big Crunch Theory

By Michael PoePublished 3 years ago 3 min read
HOW WILL OUR UNIVERSE END!?
Photo by NASA on Unsplash

Unveiling the Impending End of our Universe:

The universe is a vast expanse filled with countless galaxies, stars, and mysteries that continue to captivate the human imagination. Among the various theories proposed to understand the ultimate destiny of our universe, the Big Crunch Theory stands as a thought-provoking concept. In this essay, we will delve into the intriguing world of the Big Crunch Theory, exploring its origins, implications, and the implications it holds for the future of our cosmos.

What is the Big Crunch theory? This theory has its roots in Einstein's theory of general relativity. Everything in life follows an ebb and flow; when one event occurs, the opposite is likely to occur. If the Big Bang caused the expansion of the universe, then eventually the opposite will become true. Once the universe has reached its largest size, it will begin to be collapsed in on itself and form a massive black hole-containing all matter. So, this theory is not great news for those who are a class or for bacon lovers. Expansion and contraction: According to the Big Crunch Theory, the universe's expansion will eventually slow and then reverse. The universe would eventually collapse in on itself as a result of this contraction phase.

Consequences of Contraction: As the universe shrinks, galaxies, stars, and finally all matter would converge, creating the "Big Crunch," a highly energetic and dense state.

The Ending: The Big Crunch would bring the universe to an end, maybe to be followed by a fresh cycle of expansion and contraction that would create a brand-new universe.

Observational Hints: In order to find proof of a possible Big Crunch, scientists examine the pace of cosmic expansion and the distribution of matter. However, nothing of these data has conclusively supported nor refuted this idea.

The Big Crunch Theory is put to the test by the discovery of dark energy, a mysterious force that is responsible for the universe's present, accelerated expansion. Its presence raises the probability that our universe will have a different outcome.

Inherent to the Big Crunch theory is the potential for catastrophic events. As the universe expands, it becomes heavier and more dense. This increased gravity could eventually cause everything in the cosmos to collapse back together into a big crunch. However, scientists don't fully understand all of the factors involved in the expansion of the universe. One unknown factor is dark energy. If there's enough dark energy present, then the forces of gravity might once again overpower everything else, preventing a Big Crunch from occurring. On the other hand, if there's not enough dark energy, then gravity will eventually take over and cause the universe to undergo a cataclysmic collapse known as the Big Crunch.

Some people believe that the increasing rates of expansion of dark energy could be a sign of the beginning of the Big Crunch, but in 2015 it was suggested that this is the last gasp of the expanding universe. In about fifty-billion years, the contraction will begin, and scientists are still not sure how things will end. There are three possible outcomes: the Big Crunch, in which every piece of matter returns to its origins; a new universe; or cosmic chaos. If this has happened before, we may be living through it now – and there's nothing we can do to stop it.

The Big Crunch Theory presents a fascinating perspective on the fate of the universe, envisioning a cyclical pattern of expansion and contraction. While observational evidence and the discovery of dark energy pose challenges to this theory, it continues to stimulate scientific discourse and spark curiosity about the ultimate destiny of our cosmos. Whether the Big Crunch is a plausible future or if alternate scenarios like Heat Death or the Big Rip hold true, the exploration of these theories deepens our understanding of the universe and our place within it.

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Michael Poe

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