Difference between revisions of "Theoretical Investigation of Dark Matter"
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** [http://arxiv.org/PS_cache/astro-ph/pdf/0007/0007165v1.pdf Hot Dark Matter in Cosmology(article)] | ** [http://arxiv.org/PS_cache/astro-ph/pdf/0007/0007165v1.pdf Hot Dark Matter in Cosmology(article)] | ||
** [http://prd.aps.org/pdf/PRD/v54/i12/p7129_1 Accretion of cold and hot dark matter onto cosmic string filaments(article)] | ** [http://prd.aps.org/pdf/PRD/v54/i12/p7129_1 Accretion of cold and hot dark matter onto cosmic string filaments(article)] | ||
| + | |||
| + | == 5th Question (MACHO) == | ||
| + | * How to predict their abundance? | ||
| + | ** | ||
Revision as of 17:55, 22 July 2011
1st Question (Supersymmetry)
- What makes us require supersymmetry & How this symmetry predicts supersymmetry partners?
2rd Question (New formula for gravity)
- New mechanism and interpretation for gravitational force
3th Question (Large structure)
- How dark matter affects on early universe for formation of large structures in Universe?
- Alternative theory of gravity explains large structure formation
- Dark matter and Large Scale Structure
- Comparison of Normal Matter and Dark Matter's Large Scale Structure
- Dark Matter & Inflation (article)
- Formation of galaxies and large-scale structure with cold dark matter(article)
- Dark matter and Large-scale structure(article)
4th Question (Hot dark matter)
- What's the role of hot dark matter?
5th Question (MACHO)
- How to predict their abundance?