Temperature Dependence Viscosity of the Neutron Star Matter
| dc.contributor.advisor | Wetro, Legesse (PhD) | |
| dc.contributor.author | Belay, Atakalti | |
| dc.date.accessioned | 2018-06-19T07:43:13Z | |
| dc.date.accessioned | 2023-11-09T11:27:35Z | |
| dc.date.available | 2018-06-19T07:43:13Z | |
| dc.date.available | 2023-11-09T11:27:35Z | |
| dc.date.issued | 2010-06 | |
| dc.description.abstract | In this work, we review the basics of both ideal and non ideal uid dynamics. Funda- mental principles of uid dynamics,solution of nonlinear Boltzmann equation, transport coe cients, and moment transfer, are discussed. To solve the collision integral we have used the concept of time reversal symmetry. The basic equations governing uid motion , energy and momentum are discussed. The in uence of viscosity and its time and tem- perature dependency in uid motion is also discussed. These concepts are then applied systematically in Neutron star matter to obtain the general balance equation and to in- vestigate the motion of uid particles between two parallel planes moving with a constant relative velocity . Di erence between ideal and non ideal uids are discussed | en_US |
| dc.identifier.uri | http://10.90.10.223:4000/handle/123456789/1540 | |
| dc.language.iso | en | en_US |
| dc.publisher | Addis Ababa University | en_US |
| dc.subject | The Neutron Star Matter | en_US |
| dc.title | Temperature Dependence Viscosity of the Neutron Star Matter | en_US |
| dc.type | Thesis | en_US |