Ghost neutrinos and radiative Kerr metric in Einstein-Cartan gravity
arXiv:gr-qc/0204084
Abstract
Ghost 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.
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