The exact solutions to an Einstein-Dirac-Maxwell system with Sasakian quasi-Killing spinors on 4D spacetimes

TL;DR

This paper constructs exact solutions to an Einstein-Dirac-Maxwell system on 4D Sasakian spacetimes, revealing models with magnetic fields and spinors derived from quasi-Killing spinors, with implications for cosmic magnetic phenomena.

Contribution

It introduces a method to find exact solutions involving Sasakian quasi-Killing spinors and analyzes their properties in Einstein-Dirac-Maxwell systems.

Findings

Found solutions with contact magnetic fields on Sasakian spacetimes

Identified models satisfying and violating the weak energy condition

Introduced the Sasakian frame for analyzing spinor properties

Abstract

Exact solutions to an Einstein-Maxwell(E-D-M) system with an electric current are simple models of global cosmic magnetic phenomena in the universe. In this paper, we consider an E-D-M system with two chiral spinors $ \psi^\pm$ coupled with a gauge field $ A$ and an electromagnetic field $F=dA$. We construct a family of exact solutions to the E-D-M system on four-dimensional static Sasakian spacetimes. The electromagnetic field in the solutions is a contact magnetic field, and the chiral spinors are induced from Sasakian quasi-Killing spinors. We find closed universe models whose weak energy condition holds and open universe models whose weak energy condition is violated. In this study, we introduce the Sasakian frame, which is used to prospectively discuss the properties of Sasakian quasi-Killing spinors. A simple description of Sasakian quasi-Killing spinors of a certain type is obtained.