Effect of equation of state and composition on relativistic flows

dc.contributor.author	Chattopadhyay, I.
dc.contributor.author	S. Mandal, S.
dc.contributor.author	Ghosh, H.
dc.contributor.author	Garain, S.
dc.contributor.author	Kumar, Rajiv
dc.contributor.author	Ryu, D.
dc.date.accessioned	2015-07-21T09:57:24Z
dc.date.available	2015-07-21T09:57:24Z
dc.date.issued	2012
dc.identifier.uri	http://hdl.handle.net/123456789/1147
dc.description.abstract	The thermal state of the fluid is governed by the ratio of the thermal and the rest energy. This brings the composition of the fluid into the picture. The fluid composed of lighter particles (e.g: electron-positron pair plasma) at same temperature, is more relativistic compared to fluids with finite baryon loading, but this is not necessarily true when baryon poor transonic fluid are compared with each other. It could be shown that the transonic pair-fluid is the least relativistic. This result has far reaching consequences on accreting flows around compact objects and are expected to have similar e ect on relativistic outflows and explosive events as well.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	asi5-81
dc.subject	Accretion, accretion discs—Jets, outflows and bipolar flows— black hole physics — hydrodynamics — Transonic fluids — shock waves — relativity	en_US
dc.title	Effect of equation of state and composition on relativistic flows	en_US
dc.type	Article	en_US