Ghost neutrinos and radiative Kerr metric in Einstein-Cartan gravity

Simple item page
dc.creatorde Andrade, L. C. Garcia
dc.date2002-04-28
dc.date.accessioned2026-07-07T03:26:49Z
dc.date.available2026-07-07T03:26:49Z
dc.descriptionGhost neutrinos in radiative Kerr spacetime endowed with totally skew-symmetric Cartan contortion is presented. The computations are made by using the Newman-Penrose (NP) calculus. The model discussed here maybe useful in several astrophysical applications specially in black hole astrophysics.
dc.descriptionLatex file
dc.identifierhttps://arxiv.org/abs/gr-qc/0204084
dc.identifierhttp://arxiv.org/abs/gr-qc/0204084
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34196
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleGhost neutrinos and radiative Kerr metric in Einstein-Cartan gravity
dc.typetext

Files

Collections

arXiv