Torsion modified Plasma Screening in Astrophysics

Simple item page
dc.creatorSivaram, C.
dc.creatorde Andrade, L. C. Garcia
dc.date1998-11-07
dc.date.accessioned2026-07-07T02:28:59Z
dc.date.available2026-07-07T02:28:59Z
dc.descriptionThe 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.
dc.description5 pages latex file
dc.identifierhttps://arxiv.org/abs/astro-ph/9811116
dc.identifierhttp://arxiv.org/abs/astro-ph/9811116
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13291
dc.subjectAstrophysics
dc.titleTorsion modified Plasma Screening in Astrophysics
dc.typetext

Files

Collections

arXiv