| dc.contributor.author | Okeng'o, G O | |
| dc.contributor.author | D, Bertacca | |
| dc.contributor.author | Maartens, R | |
| dc.contributor.author | Malo, J O | |
| dc.date.accessioned | 2015-06-19T14:47:41Z | |
| dc.date.available | 2015-06-19T14:47:41Z | |
| dc.date.issued | 2015 | |
| dc.identifier.citation | Conference oral paper presented during the Fourth East-African Astronomy Workshop 31 st June - 4thJuly 2014, Kigali Institute of Education, Rwanda.- Paper submitted for publication in proceedings in mid- 2015 | en_US |
| dc.identifier.uri | http://hdl.handle.net/11295/85228 | |
| dc.description.abstract | We present a model for structure formation in the Universe where a weakly clustered "free" fluid component is continually accreted by a strongly clustered "halo" fluid component made up of cold dark matter halos. We discuss the cosmological implications of such treatment, comparing our results to the standard model | en_US |
| dc.language.iso | en | en_US |
| dc.title | Testing Structure Formation in the Universe via Coupled Matter Fluids | en_US |
| dc.type | Other | en_US |
| dc.type.material | en | en_US |
