Changes

Jump to navigation Jump to search
Line 27: Line 27:  
** [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)]
 +
** [http://www.metapress.com/content/g3x8w86451l82047/fulltext.pdf Dark Matter, Density Perturbations, and Structure Formation (2006)]
 +
** [http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2008.14267.x/pdf Angular momentum and clustering properties of early dark matter haloes]
 +
** [http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2008.13306.x/pdf Consequences of dark matter self-annihilation for galaxy formation]
 +
** [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) ==
63

edits

Navigation menu