Nonlinear spinor fields in Bianchi type-I spacetime reexamined
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Publication:461834
DOI10.1007/S10773-013-1906-7zbMath1297.83062arXiv1302.1354OpenAlexW2012648316MaRDI QIDQ461834
Publication date: 15 October 2014
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1302.1354
Related Items (3)
Nonlinear spinor fields in Bianchi type-III spacetime ⋮ Bianchi type I cosmology with scalar and spinor tachyon ⋮ Nonlinear spinor fields in LRS Bianchi type-I space-time: theory and observation
Cites Work
- Bulk viscous LRS Bianchi-I universe with variable \(G\) and decaying \(\Lambda \)
- LRS Bianchi-I anisotropic cosmological model with dominance of dark energy
- Nonlinear spinor fields and its role in cosmology
- Spinor field and accelerated regimes in cosmology
- Equivalence between the descriptions of cosmological models using a spinor field and a perfect fluid
- Interacting spinor and scalar fields in Bianchi type I universe filled with perfect fluid: Exact self-consistent solutions
- Spinors, inflation, and non-singular cyclic cosmologies
- Spinor model of a perfect fluid and their applications in Bianchi type-I and FRW models
- Dark energy model with variable \(q\) and \(\omega\) in LRS Bianchi-II space-time
- Quantum Theory of Fields and Elementary Particles
- Lorentz Invariance and the Gravitational Field
- Noether symmetry for non-minimally coupled fermion fields
- Nonlinear spinor field in Bianchi type-I Universe filled with perfect fluid: Exact self-consistent solutions
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Inflationary universe: A possible solution to the horizon and flatness problems
- Doubts and hopes in quantumelectrodynamics
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