Difference between revisions of "Theoretical Investigation of Dark Matter"

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** [http://prd.aps.org/pdf/PRD/v60/i2/e023518 Superheavy Dark matter from Thermal inflation(article)]
 
** [http://prd.aps.org/pdf/PRD/v60/i2/e023518 Superheavy Dark matter from Thermal inflation(article)]
 
** [http://www.springerlink.com/content/t96436233384k5n3/fulltext.pdf  Dark Matter & Inflation (article)]
 
** [http://www.springerlink.com/content/t96436233384k5n3/fulltext.pdf  Dark Matter & Inflation (article)]
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** [http://www.metapress.com/content/g3x8w86451l82047/fulltext.pdf Dark Matter, Density Perturbations, and Structure Formation (2006)]
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** [http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2008.14267.x/pdf Angular momentum and clustering properties of early dark matter haloes]
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** [http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2008.13306.x/pdf Consequences of dark matter self-annihilation for galaxy formation]
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** [http://www.jstor.org/stable/pdfplus/3075636.pdf?acceptTC=true The formation of the first star in the universe]
  
 
== 4th Question (Hot dark matter) ==
 
== 4th Question (Hot dark matter) ==

Revision as of 12:29, 25 July 2011

1st Question (Supersymmetry)

2rd Question (New formula for gravity)

3th Question (Large structure)

4th Question (Hot dark matter)

5th Question (Dark Matter and Reionization)