17.6: Wrapping It Up 17 - Cosmological Parameter Estimation
- Page ID
- 31499
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Scientists working with supernova, CMB, and large-scale structure data have determined to high precision the ingredients making up the Universe. From these data, scientists have constructed a pie chart depicting the matter and energy budget of the Universe (Figure A.17.9).
In this activity, you will use data from various cosmological measurements in order to determine the values of several cosmological values: the amount of matter (Ωm), which is comprised of regular baryonic matter and cold dark matter, and the amount of dark energy (ΩDE).
You should notice that there are constraints on Ωm and ΩDE from three different measurements:
- Supernovae (SNe, blue region)
- The cosmic microwave background (CMB, orange region)
- Large-scale structure baryon acoustic oscillations (BAO, green region)
Click on each cosmological source to pull up confidence regions for the measurement.
For a given source, the combination of Ωm and ΩDE has a 68% chance of falling within the smallest region, 95% chance of falling within the next larger region, and a 99% chance of falling within the entire shaded region. A 99% confidence region means that the true value will lie outside the region only 1% of the time. In other words, we are 99% confident that the true value lies inside the region bounded by the contour.
Part I: Individual Measurements
1. Plot the BAO measurement. With 99% confidence, what is the range of values for Ωm?
Cannot determine from this data
0.15 – 0.30
0.15 – 0.45
0.20 – 0.40
0.25 – 0.45
2. With 68% confidence, what is the range of values for Ωm from BAO alone?
Cannot determine from this data
0.15 – 0.30
0.15 – 0.45
0.20 – 0.40
0.25 – 0.45
3. Within 68% confidence, what is the range of values for ΩDE from BAO alone?
Cannot determine from this data
0.15 – 0.45
0.20 – 0.40
0.60 – 0.80
4. Overall, with 99% accuracy, do measurements from BAO alone constrain Ωm, ΩDE, or both?
m"> constrains only Ωm
DE"> constrains only ΩDE
constrains both
5. Now click the measurements from the CMB only to constrain the region of possible values for Ωm and ΩDE. Overall, with 99% accuracy, does this measurement alone constrain Ωm, ΩDE, or both?
m"> constrains only Ωm
DE"> constrains only ΩDE
constrains both
6. Now click the measurements from the supernovae (SNe) only to constrain the region of possible values for Ωm and ΩDE. Overall, with 99% accuracy, does this measurement alone constrain Ωm, ΩDE, or both?
m"> constrains only Ωm
DE"> constrains only ΩDE
constrains both
Part II: Combining measurements
1. As you click to add additional cosmological measurement sources, the size of the overlapping region
increases
decreases
stays the same
2. Combing the confidence regions of both the BAO and CMB, with 68% confidence, what is the range of values for Ωm?
cannot determine from this data
0.22 – 0.39
0.29 – 0.32
3. Combing the confidence regions of both the BAO and CMB measurement, are Ωm and ΩDE constrained to within 99% confidence?
m"> constrains only Ωm
DE"> constrains only ΩDE
constrains both
4. Click on various combinations of BAO, CMB, and SNe. Which pair of measurements gives the smallest range of values for Ωm?
BAO+CMB
BAO+SNe
CMB+SNe
5. Which pair of measurements gives the smallest range of values for ΩDE?
BAO+CMB
BAO+SNe
CMB+SNe
6. With all three measurements checked, you should see a set of gray/black confidence regions. What is your best estimate of the matter density fraction, Ωm from all measurements combined?
7. What is the best estimate of the dark energy density fraction, ΩDE from all measurements combined?
8. You should also see a line labeled “flat,” which denotes the region of this plot where the total density, Ω, is equal to 1. In other words, Ωm + ΩDE = 1. If the combined values of Ωm and ΩDE fall below and to the left of this line, what type of Universe would that indicate?
a flat universe
one that will expand forever
one that will collapse eventually
9. The gray region indicates that the best fit for the geometry of the Universe is:
flat (Ω = 1)
1)"> spherical (Ω > 1)
saddle-shaped (Ω < 1)