Numerical simulation of astrophysical plasma with relativistic equation of state

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