Torsion Modified Plasma Screening in Astrophysics

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3322

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.contributor.author	de Andrade, L. C. G	-
dc.date.accessioned	2008-09-02T10:47:15Z	-
dc.date.available	2008-09-02T10:47:15Z	-
dc.date.issued	2000-06	-
dc.identifier.citation	Modern Physics Letters A, Vol. 15, No. 19, pp. 1275 - 1277	en
dc.identifier.issn	0217-7323	-
dc.identifier.uri	http://hdl.handle.net/2248/3322	-
dc.description.abstract	The torsion modified Maxwell–Proca equations when applied to describe a plasma is shown to lead to a correction to the Debye screening length. For hot new born neutron stars the torsion correction is shown to be significant. This effect may provide an indirect evidence for torsion.	en
dc.language.iso	en	en
dc.publisher	World Scientific Publishing Company	en
dc.relation.uri	http://dx.doi.org/10.1142/S021773230000150X	en
dc.relation.uri	http://arxiv.org/pdf/astro-ph/9811116	-
dc.subject	Torsion Modified Maxwell–Proca Equations	en
dc.subject	Plasma	en
dc.subject	Neutron Stars	en
dc.subject	Torsion Correction	en
dc.title	Torsion Modified Plasma Screening in Astrophysics	en
dc.type	Article	en
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