How Cosmic Inflation Flattened the Universe
Interactive Video
•
Physics, Science, Business
•
11th Grade - University
•
Practice Problem
•
Hard
Wayground Content
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10 questions
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1.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the horizon problem in cosmology?
The universe's expansion rate is too slow.
Distant parts of the universe appear to have been in contact.
The universe is not expanding at all.
The universe's temperature is too high.
2.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
How is the curvature of the universe measured?
By analyzing the color of stars.
By calculating the mass of galaxies.
By measuring the angles of triangles in space.
By observing the speed of light.
3.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What does the flatness problem suggest about the universe?
The universe is expanding too quickly.
The universe should not be flat if only gravity is considered.
The universe is shrinking.
The universe is perfectly spherical.
4.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the main idea behind cosmic inflation?
The universe is cooling down.
The universe has always been static.
The universe expanded rapidly in its early moments.
The universe is contracting.
5.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
How does inflation solve the horizon and flatness problems?
By stopping the universe's expansion entirely.
By rapidly expanding the universe to smooth out irregularities.
By increasing the universe's temperature.
By slowing down the universe's expansion.
6.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What role does the cosmological constant play in the universe's expansion?
It drives the expansion of the universe.
It causes the universe to contract.
It has no effect on the universe.
It allows for a static universe.
7.
MULTIPLE CHOICE QUESTION
30 sec • 1 pt
What is the relationship between the cosmological constant and dark energy?
They are unrelated concepts.
The cosmological constant describes the effect of dark energy.
The cosmological constant causes the universe to collapse.
Dark energy prevents the universe from expanding.
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