Cosmology Challenges: Dark Matter, Dark Energy, Galaxy Formation

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SUMMARY

The forum discussion centers on the challenges in cosmology, specifically regarding dark matter, dark energy, and galaxy formation as outlined in the paper "New Frontiers in Cosmology and Galaxy Formation" by Richard Ellis and Joseph Silk. Key challenges include understanding the nature of the dark sector, the timing and mechanisms of galaxy formation during the epoch of reionization, and reconciling observational discrepancies with the dark matter-driven model of galaxy assembly. The discussion emphasizes the need for improved observational probes and theoretical refinement to address these issues.

PREREQUISITES
  • Understanding of dark matter and dark energy concepts
  • Familiarity with galaxy formation processes during the epoch of reionization
  • Knowledge of ultra luminous infrared galaxies (ULIRGs)
  • Proficiency in observational astrophysics techniques
NEXT STEPS
  • Research advanced observational techniques for probing dark matter and dark energy
  • Study the mechanisms of galaxy formation and evolution during the epoch of reionization
  • Explore the implications of ULIRGs on galaxy assembly theories
  • Investigate the role of chemical signatures in understanding galaxy formation
USEFUL FOR

Astronomers, astrophysicists, and researchers focused on cosmology, particularly those interested in the complexities of dark matter, dark energy, and galaxy formation processes.

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http://arxiv.org/PS_cache/arxiv/pdf/0712/0712.2865v1.pdf

New Frontiers in Cosmology and Galaxy Formation: Challenges for the Future
Authors: Richard Ellis (Caltech), Joseph Silk (Oxford)
Comments: To appear in "Structure Formation in the Universe", ed. Chabrier, G., Cambridge University Press. High resolution version on this http URL
Subjects: Astrophysics (astro-ph)

(Abridged) Cosmology faces three distinct challenges in the next decade. (1) The dark sector, both dark matter and dark energy, dominates the Universe. Key questions include determining the nature of both. Improved observational probes are crucial. (2) Galaxy formation was initiated at around the epoch of reionization: we need to understand how and when as well as to develop probes of earlier epochs. (3) Our simple dark matter-driven picture of galaxy assembly is seemingly at odds with several observational results, including the presence of ULIRGS at high z, the `downsizing' signature, chemical signatures of alpha-element ratios and suggestions that merging may not be important in defining the Hubble sequence. Understanding the physical implications is a major challenge for theorists and refiniing the observational uncertainties a major goal for observers.

The thing that interests me is the (what is the universe made of) question, and the finding or lack of of what is proposed.
 
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IMO this is 24 carat pure gold mainstream cosmology.
I've the highest respect for Joe Silk and am proud to have met him.
I went and bothered him with a question in his office one time when he was at UCBerkeley.

thanks to your flagging this I added it to the bibliography
lets get the URL for the abstract and also for the high-resolution version
the short abstract is here
http://arxiv.org/abs/0712.2865
the high-resolution version is here on Ellis' Caltech server
http://www.astro.caltech.edu/~rse/chamonix.pdf

An ULIRG is an ultra luminous infrared galaxy
ULIRGs are believed to be places where a lot of star-formation is going on.
 
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