The Teukolsky–Starobinsky identities in type D vacuum backgrounds with cosmological constant

DOI10.1063/1.527865zbMath0709.53503OpenAlexW2145374493MaRDI QIDQ3492335

Gerardo F. Torres del Castillo

Publication date: 1988

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

Full work available at URL: https://doi.org/10.1063/1.527865

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Differential geometry (53-XX)

Related Items (13)

Killing spinors and separability of Maxwell’s equations ⋮ A comment on differential identities for the Weyl spinor perturbations ⋮ Teukolsky–Starobinsky identities for arbitrary spin ⋮ 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 ⋮ QUASINORMAL MODES AND LATE-TIME TAILS IN THE BACKGROUND OF SCHWARZSCHILD BLACK HOLE PIERCED BY A COSMIC STRING: SCALAR, ELECTROMAGNETIC AND GRAVITATIONAL PERTURBATIONS ⋮ Extremal black hole entropy satisfying the Nernst theorem ⋮ Rarita–Schwinger fields in algebraically special vacuum space-times ⋮ Debye potentials for Maxwell and Dirac fields from a generalization of the Killing–Yano equation ⋮ Spin-3/2 perturbations of algebraically special solutions of the Einstein–Maxwell equations ⋮ The Teukolsky–Starobinsky constants: facts and fictions ⋮ The method of adjoint operators and a symmetry operator for the Maxwell equations in type-D vacuum backgrounds ⋮ Debye potentials for Rarita–Schwinger fields in curved space-times

Cites Work

• Necessary and sufficient conditions for trivial solutions in supergravity
• Space-times with two-index Killing spinors
• The separability of Maxwell’s equations in type-D backgrounds
• A space-time calculus based on pairs of null directions

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