Is the Fate of the Universe Truly Determined by Dark Energy?

In summary, the recent study published by the BBC has shown that the ultimate fate of the Universe is still unknown, as we do not fully understand the nature of dark energy. However, the findings are consistent with the theory of constant dark energy, with an equation of state of p = -\rho or w = -1. Further studies and data from various sources have resulted in a range of 0.23 < [itex]\Omega_m < 0.33 and −1.12 < w < −0.82 for the cosmological constraints. This brings us closer to understanding the fate of the Universe, but further research is still needed.
  • #1
skydivephil
474
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The BBc just publsihed this story:
http://www.bbc.co.uk/news/science-environment-11030889

The conclusion is:
"Professor Priyamvada Natarajan of Yale University, a leading cosmologist and co-author of this study, said that the findings finally proved "exactly what the fate of the Universe will be". "

Surely this is premature? Until we udnerstand what dark energy is we can't say its a contsant and if its not constant it may die down or even reverse and so the ultimate fate of the unvierse is still unknown.
 
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  • #2
Constant dark energy/cosmology constant has equation of state [itex]p = -\rho[itex], i.e., [itex]w = -1[/itex]. While it cannot be ruled out that w will remain constant, this paper's result is consistent (with smaller error bands than before) with constant [itex]w = -1[/itex].

From the Science article's abstract:
Combining our cosmological constraints with those from x-ray clusters and the Wilkinson Microwave Anisotropy Probe 5-year data gives Wm = 0.25 T0.05 and w = −0.97 +- 0.07

From the end of the article:
Our results—when combined with the results from WMAP5 (40), the supernovae “Gold sample” (4), the Supernovae Legacy Survey (SNLS) (41), the ESSENCE Supernova Survey (SNEssence) (42), and the BAO peak from the Sloan Digital Sky Survey (SDSS) (16)—give 0.23 < [itex]\Omega_m[/itex] < 0.33 and −1.12 < w < −0.82 at the 99% confidence level.
 

FAQ: Is the Fate of the Universe Truly Determined by Dark Energy?

1. What is the BBC galactic lens?

The BBC galactic lens, also known as the Bullet Cluster, is a cosmic phenomenon where two galaxy clusters have collided and their gravitational forces have bent the light from the galaxies behind them, creating a "lens" effect.

2. What is dark energy?

Dark energy is a theoretical form of energy that is believed to make up about 68% of the total energy in the universe. It is thought to be responsible for the accelerating expansion of the universe.

3. How does the BBC galactic lens help us understand dark energy?

By studying the BBC galactic lens, scientists have been able to measure the amount of dark matter and normal matter in the clusters, as well as the amount of dark energy in the universe. This has provided valuable insights into the nature of dark energy and its effects on the universe.

4. What is the significance of the BBC galactic lens in cosmology?

The BBC galactic lens is significant in cosmology because it provides evidence for the existence of dark matter and dark energy, which are two of the biggest mysteries in modern physics. It also helps to support the theory of cosmic inflation and the Big Bang theory.

5. How does the BBC galactic lens impact our understanding of the universe?

Studying the BBC galactic lens has given scientists a better understanding of the composition of the universe and how it has evolved over time. It has also helped to refine our understanding of dark energy and its role in the expansion of the universe.

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