Debye potentials for Rarita–Schwinger fields in curved space-times

DOI10.1063/1.528312zbMath0681.76119OpenAlexW2155236527MaRDI QIDQ4730970

Gerardo F. Torres del Castillo

Publication date: 1989

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.528312

zbMATH Keywords

Einstein-Maxwell equationsEinstein vacuum field equationsbackground space-timecomplete solution of the Rarita-Schwinger equationcomplex scalar potentialsmethod of adjoint operators

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (6)

Perturbations of solutions of the Einstein–Maxwell equations with a null background electromagnetic field ⋮ Spin-3/2 fields in flat space-time ⋮ Gravitational perturbations of type-D vacuum space–times with cosmological constant ⋮ Killing spinors and separability of Rarita–Schwinger’s equation in type {2,2} backgrounds ⋮ Solution of the Dirac equation on the Bertotti-Robinson metric ⋮ Self-adjoint operators and conserved currents

Cites Work

• The Teukolsky–Starobinsky identities in type D vacuum backgrounds with cosmological constant
• Perturbations of solutions of the Einstein equations with sources
• Rarita–Schwinger fields in algebraically special vacuum space-times

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