a. Which areas (H, I, J, K, L, or M) are the accelerating universes? (As opposed to the expansion staying steady or decelerating.) b. Which area (H, I, J, K, L, or M) represents a flat universe with a matter density parameter of 1.0? c. Which area (H, I, J, K, L, or M) represents a universe containing 76% Dark Energy? d. Which area (H, I, J, K, L, or M) represents the universe that Supernova Type la, galaxy cluster, and CMB data results indicate we are in? e. Which area (H, I, J, K, L, or M) represents the universe that will someday have a "Big Crunch"? f. What force opposes the acceleration of the Universe? g. What causes the acceleration of the Universe?

Elements Of Electromagnetics
7th Edition
ISBN:9780190698614
Author:Sadiku, Matthew N. O.
Publisher:Sadiku, Matthew N. O.
ChapterMA: Math Assessment
Section: Chapter Questions
Problem 1.1MA
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Directions
Part 1: Due Thursday at 9pm. Answer the questions below.
Dark energy density parameter ₁
2.5
2.0
1.5
1.0
0.5
0.0
-0.5
-1.0
Gray area: No Big Bang
(density of matter could
never have been infinite)
0.0
K
Expansion is speeding up
Expansion is slowing down
This model,
for which
m=1.00, and
A=0.00, has
been ruled out
by observations.
Universe expands forever
Universe recollapses
M
Universe is closed
Universe is open
0.5 1.0
1.5
2.0
Matter density parameter m
2.5
a. Which areas (H, I, J, K, L, or M) are the accelerating universes? (As opposed to the expansion staying steady or decelerating.)
b. Which area (H, I, J, K, L, or M) represents a flat universe with a matter density parameter of 1.0?
c. Which area (H, I, J, K, L, or M) represents a universe containing 76% Dark Energy?
d. Which area (H, I, J, K, L, or M) represents the universe that Supernova Type la, galaxy cluster, and CMB data results indicate we are in?
e. Which area (H, I, J, K, L, or M) represents the universe that will someday have a "Big Crunch"?
f. What force opposes the acceleration of the Universe?
g. What causes the acceleration of the Universe?
Transcribed Image Text:Directions Part 1: Due Thursday at 9pm. Answer the questions below. Dark energy density parameter ₁ 2.5 2.0 1.5 1.0 0.5 0.0 -0.5 -1.0 Gray area: No Big Bang (density of matter could never have been infinite) 0.0 K Expansion is speeding up Expansion is slowing down This model, for which m=1.00, and A=0.00, has been ruled out by observations. Universe expands forever Universe recollapses M Universe is closed Universe is open 0.5 1.0 1.5 2.0 Matter density parameter m 2.5 a. Which areas (H, I, J, K, L, or M) are the accelerating universes? (As opposed to the expansion staying steady or decelerating.) b. Which area (H, I, J, K, L, or M) represents a flat universe with a matter density parameter of 1.0? c. Which area (H, I, J, K, L, or M) represents a universe containing 76% Dark Energy? d. Which area (H, I, J, K, L, or M) represents the universe that Supernova Type la, galaxy cluster, and CMB data results indicate we are in? e. Which area (H, I, J, K, L, or M) represents the universe that will someday have a "Big Crunch"? f. What force opposes the acceleration of the Universe? g. What causes the acceleration of the Universe?
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