Graph with Saul and Perlmutter's results

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In summary, the conversation discusses a graph that shows the values of \Omega_m and \Omega_\Lambda. The confusion arises from the fact that the ellipse on the graph is centered on (0.9,1.5) instead of the expected (0.3,0.7). However, the data from different sources, including supernovae, the cosmic microwave background, and galaxy clusters, all agree on the values of \Omega_m and \Omega_\Lambda being 0.3 and 0.7 respectively, leading to the concordance model. This is an important concept in understanding dark energy and is being studied through the SuperNovae Acceleration Probe (SNAP) mission.
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Niles
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Hi guys

Please take a look at this familiar graph: http://www.iop.org/EJ/article/1538-3881/116/3/1009/980111.fg7.html

I've read about how the data got conceived and all, but I can't see why that graph indicates that [tex]\Omega_m=0.3[/tex] and [tex]\Omega_\Lambda=0.7[/tex]? :confused:
 
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This is the point where the major axis of the inner solid ellipse crosses the line representing total omega = 1.
 
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Is the confusion due to the fact that the ellipse is actually centered on something crazy, like (0.9,1.5) rather than the (0.3,0.7) you expected? As mathman pointed out, the key point is that (0.3,0.7) is where the ellipse crosses total omega=1.

The reason that this is important however is because of the rest of the data. The SN alone leave you with the large ellipse, but have a look at http://snap.lbl.gov/images/omlam.jpg" figure. It shows the way three important data sets, SN, the CMB and galaxy cluster constrain the parameters. As can be see, the CMB basically tells you that omega=1, but doesn't say what the breakup of that is, the SN tell you that the break up is (0.3,0.7) if omega=1 and the clusters tell you independently that omega matter =0.3.

It is the fact that these and other data sets agree independantly, i.e. the contours all cross at a point, that we call this the concordance model. This figure is from the SuperNovae Acceleration Probe (SNAP) website. This is a planned space mission to study dark energy. Note the tiny region they hope to constrain the parameters to!
 
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1. What is the significance of Saul and Perlmutter's results?

Saul and Perlmutter's results are significant because they were the first to provide strong evidence for the accelerating expansion of the universe. Their research paved the way for further studies on dark energy and its role in the expansion of the universe.

2. How did Saul and Perlmutter's results impact our understanding of the universe?

Saul and Perlmutter's results showed that the expansion of the universe is not slowing down as previously believed, but rather accelerating. This discovery challenged the existing theories and led to the development of new models to explain the acceleration, such as the concept of dark energy.

3. What methods did Saul and Perlmutter use to obtain their results?

Saul and Perlmutter used a technique called Type Ia supernova cosmology to study the brightness and distance of distant galaxies. By measuring the light from these supernovae, they were able to determine the rate of expansion of the universe and its acceleration.

4. What were the key findings of Saul and Perlmutter's research?

The key findings of Saul and Perlmutter's research were that the expansion of the universe is accelerating, contrary to previous beliefs, and that this acceleration is likely caused by a mysterious force known as dark energy. They also found that the universe is expanding at an increasingly rapid rate.

5. How has Saul and Perlmutter's research impacted the field of cosmology?

Saul and Perlmutter's research has had a significant impact on the field of cosmology by providing evidence for the existence of dark energy and the accelerating expansion of the universe. This discovery has led to further studies and theories on the nature of dark energy and its role in the universe's expansion.

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