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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/561

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DC Field	Value	Language
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
Appears in Collections:	BASI Publications

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