Nonlinear spinor fields in Bianchi type-III spacetime
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Publication:293026
DOI10.1007/s10773-015-2864-zzbMath1338.81302arXiv1603.04623OpenAlexW2146891265WikidataQ126010052 ScholiaQ126010052MaRDI QIDQ293026
Publication date: 9 June 2016
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1603.04623
Quantum field theory on curved space or space-time backgrounds (81T20) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20)
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Cites Work
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- Nonlinear spinor fields and its role in cosmology
- Nonlinear spinor fields in Bianchi type-I spacetime reexamined
- Spinor field and accelerated regimes in cosmology
- Equivalence between the descriptions of cosmological models using a spinor field and a perfect fluid
- Bianchi type III models with anisotropic dark energy
- Exact spatially homogeneous cosmologies
- 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
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Cosmological constant -- the weight of the vacuum
- A discussion on Dirac field theory, no-go theorems and renormalizability
- Big bounce from spin and torsion
- Spinor model of a perfect fluid and their applications in Bianchi type-I and FRW models
- Bianchi type III anisotropic dark energy models with constant deceleration parameter
- Some Bianchi type III string cosmological models with bulk viscosity
- The dynamics of quintessence, the quintessence of dynamics
- Anisotropic cosmological models with a perfect fluid and a \(\Lambda\) term
- Dirac spinors in Bianchi-I f(R)-cosmology with torsion
- Massive String Cosmology in Bianchi Type III Space-Time with Electromagnetic Field
- Lorentz Invariance and the Gravitational Field
- A note on tilted Bianchi type VI h models: the type III bifurcation
- Noether symmetry for non-minimally coupled fermion fields
- Nonlinear spinor field in Bianchi type-I Universe filled with perfect fluid: Exact self-consistent solutions
- WMAP and the generalized Chaplygin gas
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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