dc.contributor.author | Chattopadhyay, Indranil | |
dc.contributor.author | Ryu, Dongsu | |
dc.contributor.author | Jang, Hanbyul | |
dc.date.accessioned | 2015-04-24T07:06:01Z | |
dc.date.available | 2015-04-24T07:06:01Z | |
dc.date.issued | 2013 | |
dc.identifier.uri | http://hdl.handle.net/123456789/982 | |
dc.description.abstract | In this paper we incorporate the relativistic equation of state of multi-species fluid in relativistic hydrodynamic code. We show that in the trans-relativistic temperature regime, composition plays a very important role in the temporal evolution of relativistic hydrodynamics. We show this for shock tube tests, as well as, relativistic jets. | en_US |
dc.language.iso | en_US | en_US |
dc.publisher | ASI | en_US |
dc.relation.ispartofseries | ASI;9-13 | |
dc.subject | Hydrodynamics — methods | en_US |
dc.subject | Numerical-relativity | en_US |
dc.title | Numerical simulation of astrophysical plasma with relativistic equation of state | en_US |
dc.type | Article | en_US |