Complete sets of functions for perturbations of Robertson–Walker cosmologies and spin 1 equations in Robertson–Walker-type space-times

DOI10.1063/1.529413zbMath0729.53073OpenAlexW2141094727MaRDI QIDQ3353758

Ernest G. Kalnins, Willard jun. Miller

Publication date: 1991

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

Full work available at URL: https://doi.org/10.1063/1.529413

zbMATH Keywords

perturbationswave equationsseparation of variablesRobertson-Walker cosmological models

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of global differential geometry to the sciences (53C80)

Related Items (5)

Spin 2 field equation in expanding universe ⋮ Spin 3/2 field equation: separation and solution in a class of Lemaître-Tolman-Bondi cosmologies ⋮ THE SPECTRUM OF SCALAR FLUCTUATIONS OF A BOUNCING UNIVERSE ⋮ Proca fields interpretation of spin 1 equation in Robertson-Walker space-time ⋮ Small perturbations in general relativity: tensor harmonics of arbitrary symmetry

Cites Work

• Cauchy's problem and Huygens' principle for relativistic higher spin wave equations in an arbitrary curved space-time
• Non-factorizable separable systems and higher-order symmetries of the Dirac operator
• Symmetry operators for neutrino and Dirac fields on curved spacetime
• On transformations between basis vectors of unitarySL 2,C representations

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