What parameter of the present universe, more than any other, is considered to be critical in determining the ultimate fate of the universe?

Answer 1

The rate of expansion of the universe.

The question has been whether the universe is an open system, closed system, or static system. If the universe's density was exactly 1, it would be a static system, or what is known as a steady state universe. If the universe's density was less than 1, on the other hand, it would be a closed system that would undergo alternating episodes of contraction (Big Crushes) and expansion (Big Bangs).

The universe is an open system, and the increasing rate of expansion seen in 1998 suggests that the universe's density is greater than 1. The universe will therefore continue to expand until maximum entropy is reached, which will ultimately lead to the universe's heat death.

The universe is an open system of matter, and energy is not the only thing that exists. The rate of expansion of the universe is crucial in determining the density of the universe and its ultimate fate. The empirical evidence indicates that the universe will ultimately meet its heat death.

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Answer 2

The density parameter, commonly represented by the symbol Ω (Omega), is the parameter of the current universe that is thought to be most important in determining its final destiny.

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Answer from HIX Tutor

When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.

When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.

When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.

When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.

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