How did the Big Bang create the universe?
The 'Big Bang' is what we call the furthest back in time we can trace the Universe's history. We have a solid understanding of what happened fractions of a second after 'time zero', but cannot yet say anything about before.
It would be more accurate to state that "the Big Bang was the beginning of our Universe (and is as far back as we can study it)" rather than that "the Big Bang created the Universe."
'Big Bang' refers to both a specific event at 'time zero' and a period of exponential expansion at the beginning of our universe (remember, it's still expanding!).
We cannot model the universe between t=0 and about t=0.000000000000000000000000000000000001 seconds; although this seems like a tiny amount of time, significant events must have occurred during this fraction of a second!). Our theories break down sufficiently close to "time zero."
After all, the universe continued to cool exponentially after this point, and quarks eventually turned into nucleons (protons and neutrons) and then into atoms, which were then free to gravitationally collapse into stars, galaxies, and planetary systems after light stopped interacting with matter.
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According to the Big Bang theory, the universe began as a singularity, a point of infinite temperature and density. Roughly 13.8 billion years ago, this singularity experienced rapid expansion, which resulted in the formation of all matter, energy, space, and time. Subatomic particles formed as the universe expanded and cooled, eventually forming into stars, galaxies, atoms, and larger cosmic structures over billions of years.
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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.
- How did the Big Bang begin?
- What is Hubble's Law? What is it used for?
- What is it expanding into? Will it ever stop? Will we ever be able to go outside the zone it is expanding into?
- How many parsecs are in an AU?
- Does the Hubble Law imply that the universe is expanding uniformly from Earth or somewhere near it?

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