MGD Dirac Stars
Roldão da Rocha
Abstract
The method of geometric deformation (MGD) is here employed to study compact stellar configurations, which are solutions of the effective Einstein–Dirac coupled field equations on fluid branes. Non-linear, self-interacting, fermionic fields are then employed to derive MGD Dirac stars, whose properties are analyzed and discussed. The MGD Dirac star maximal mass is shown to increase as a specific function of the spinor self-interaction coupling constant, in a realistic model involving the most strict phenomenological current bounds for the brane tension.
Topics & Concepts
PhysicsDirac (video compression format)Dirac equationStarsSpinor fieldCoupling (piping)Function (biology)SpinorField (mathematics)Star (game theory)Mathematical physicsDeformation (meteorology)Dirac spinorDirac operatorDirac seaPhenomenological modelBraneClassical mechanicsCurrent (fluid)Dirac algebraVector fieldField equationWave functionBlack Holes and Theoretical PhysicsCosmology and Gravitation TheoriesPulsars and Gravitational Waves Research