The Role of Space-Time Curvature in the Study of Plasma Processes near Neutron Stars and Black Holes

dc.contributor.author	Prasanna, A. R
dc.date.accessioned	2005-08-20T04:13:46Z
dc.date.available	2005-08-20T04:13:46Z
dc.date.issued	1978-12
dc.identifier.citation	BASI, Vol. 6, No. 4, pp. 88-91	en
dc.identifier.uri	http://hdl.handle.net/2248/561
dc.description.abstract	As neutron stars and black holes are very compact massive objects with possibly high magnetic fields, their surrounding space-time curvature should be treated important while considering plasma processes for explaining radiation emission nearby such objects. In this essay, we make a case for considering plasma processes on curved geometry (general relativistic framework), through considering detailed orbits of charged particles in ellectromagnetic fields on Schwarzschild and Kerr background	en
dc.format.extent	641735 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Stars	en
dc.subject	Black Holes	en
dc.title	The Role of Space-Time Curvature in the Study of Plasma Processes near Neutron Stars and Black Holes	en
dc.type	Article	en