Difference between revisions of "Observational Basis for Dark Matter"
Jump to navigation
Jump to search
Line 1: | Line 1: | ||
==Background Information on Dark Matter== | ==Background Information on Dark Matter== | ||
===Questions for the Web=== | ===Questions for the Web=== | ||
− | {| style="background-color:rgb( | + | {| style="background-color:rgb(180,200,255); -moz-box-shadow:0px 0px 5px black; -webkit-box-shadow:0px 0px 5px black; border-radius:8px; -moz-border-radius:8px" |
− | |- style="background-color:rgb( | + | |- style="background-color:rgb(200,230,255); height:75px" |
! Questions | ! Questions | ||
! Sources with Possible Answers | ! Sources with Possible Answers |
Revision as of 13:43, 22 July 2011
Background Information on Dark Matter
Questions for the Web
Questions | Sources with Possible Answers |
---|---|
1. How can we be sure dark matter exists? |
|
2. What are the possible candidates for the particles that actually make up dark matter? |
|
3. What are the properties of WIMPs, and how can they be detected? |
|
4. What ongoing research is being done to detect and experiment with dark matter? |
|
5. Where do we think all the super-symmetric particles are? |