Separation of spin 0, 1/2, 1 field equations in Lemaître-Tolman-Bondi cosmological model with cosmological constant
DOI10.1007/S10773-013-1795-9zbMath1284.83059OpenAlexW2049743315MaRDI QIDQ2443987
Publication date: 8 April 2014
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-013-1795-9
cosmological constantscalar field equationvariable separationparametric solutionsLemaître-Tolman-Bondi cosmology
Relativistic cosmology (83F05) Quantum field theory on curved space or space-time backgrounds (81T20) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Methods of quantum field theory in general relativity and gravitational theory (83C47)
Cites Work
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- Massive fields of arbitrary spin in curved space-times
- Weyl spinor and solution of massless free field equations
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- Inhomogeneous Cosmological Models
- Effect of Inhomogeneity on Cosmological Models
- Spherically Symmetrical Models in General Relativity
- Quantum Fields in Curved Space
- Dirac equation in Lemaître-Tolman-Bondi models
- The expanding universe
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