Dirac equation in Lemaître-Tolman-Bondi models
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Publication:5931054
DOI10.1023/A:1001950718322zbMath0976.83078MaRDI QIDQ5931054
Publication date: 2 May 2001
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Relativistic cosmology (83F05) Spinor and twistor methods in general relativity and gravitational theory; Newman-Penrose formalism (83C60) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (6)
Massive field equations of arbitrary spin in Schwarzschild geometry: separation induced by spin-\(\frac{3}{2}\) case ⋮ Spin 3/2 field equation: separation and solution in a class of Lemaître-Tolman-Bondi cosmologies ⋮ Separation of spin 0, 1/2, 1 field equations in Lemaître-Tolman-Bondi cosmological model with cosmological constant ⋮ Aspects of solutions of massive spin-3/2 equation in Schwarzschild space-time ⋮ Solution of the Dirac equation in expanding universes ⋮ The Dirac equation in Schwarzschild black hole coupled to a stationary electromagnetic field
Cites Work
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- Second quantization of the Dirac field: Normal modes in the Robertson-Walker space-time
- Massive fields of arbitrary spin in curved space-times
- Nonconservation of the net current of Dirac particles in Tolman-Bondi and Robertson-Walker geometries
- An Approach to Gravitational Radiation by a Method of Spin Coefficients
- Recent advances in the use of separation of variables methods in general relativity
- Inhomogeneous Cosmological Models
- Effect of Inhomogeneity on Cosmological Models
- The Dirac equation in the Robertson–Walker space–time
- On the compatibility of relativistic wave equations in riemann spaces
- Spherically Symmetrical Models in General Relativity
- Quantum Fields in Curved Space
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