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 |