
TL;DR
This paper provides an approximate, axisymmetric, time-dependent solution to the Einstein-Dirac equations, modeling a massive fermion with its gravitational field and analyzing its conserved quantities.
Contribution
It introduces a novel approximate solution to the Einstein-Dirac equations describing a fermion with self-gravity, expanding understanding of fermionic matter in curved spacetime.
Findings
Solution describes a massive fermion with its gravitational field
Metric approaches flat spacetime at infinity
Conserved quantities have been calculated
Abstract
We present an approximate solution to the minimally coupled Einstein-Dirac equations. We interpret the solution as describing a massive fermion coexisting with its own gravitational field. The solution is axisymmetric but is time dependent. The metric approaches that of a flat spacetime at the spatial infinity. We have calculated a variety of conserved quantities in the system.
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