Dark Energy and the Accelerating Universe (survey)

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SUMMARY

The discussion centers on the invited review titled "Dark Energy and the Accelerating Universe" by Joshua Frieman, Michael Turner, and Dragan Huterer, submitted on March 7, 2008. It highlights the discovery that the Universe's expansion is accelerating, leading to the current cosmological model comprising 4% baryons, 20% dark matter, and 76% dark energy. The review addresses the implications of cosmic acceleration, potential explanations such as the quantum energy of the vacuum, and the necessity for observational probes to further understand dark energy and its connection to General Relativity.

PREREQUISITES
  • Understanding of cosmological models, specifically LCDM (Lambda Cold Dark Matter).
  • Familiarity with concepts of dark energy and its role in cosmic acceleration.
  • Knowledge of General Relativity and its implications for cosmology.
  • Awareness of observational techniques in astrophysics, such as supernova surveys and cosmic microwave background measurements.
NEXT STEPS
  • Research the latest findings on dark energy from the European Space Agency's Euclid mission.
  • Explore the implications of cosmic acceleration on the future of the Universe.
  • Study the observational probes discussed in the review, such as baryon acoustic oscillations.
  • Investigate alternative theories to dark energy, including modifications to General Relativity.
USEFUL FOR

Astronomers, cosmologists, and astrophysicists interested in the current understanding of dark energy and its effects on the Universe's expansion. This discussion is also beneficial for students and researchers looking to grasp the complexities of modern cosmology.

marcus
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http://arxiv.org/abs/0803.0982
Dark Energy and the Accelerating Universe
Joshua Frieman (Chicago/Fermilab), Michael Turner (Chicago), Dragan Huterer (Michigan)
Invited review for Annual Reviews of Astronomy and Astrophysics; 53 pages, 18 figures
(Submitted on 7 Mar 2008)

"The discovery ten years ago that the expansion of the Universe is accelerating put in place the last major building block of the present cosmological model, in which the Universe is composed of 4% baryons, 20% dark matter, and 76% dark energy. At the same time, it posed one of the most profound mysteries in all of science, with deep connections to both astrophysics and particle physics. Cosmic acceleration could arise from the repulsive gravity of dark energy -- for example, the quantum energy of the vacuum -- or it may signal that General Relativity breaks down on cosmological scales and must be replaced. We review the present observational evidence for cosmic acceleration and what it has revealed about dark energy, discuss the various theoretical ideas that have been proposed to explain acceleration, and describe the key observational probes that will shed light on this enigma in the coming years."


Michael Turner is one of the world's top cosmologists. This invited review probably sums up the current mainstream view of dark energy. A good point of reference.
 
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Thanks Marcus, indeed it will be a useful reference.
 
This paper puts the basic concepts of modern cosmology into perspective. I would call it a review paper, and a very good one. LCDM is a model that is affirmed on a daily basis on many fronts.
 

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