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Non-minimally coupled nonlinear spinor field in FRW cosmology in the evolution of the Universe when it is non-minimally coupled to the gravitational one. We considered a few

Interacting self-consistent system of spinor and gravitational fields in the evolution of the Universe when it is non-minimally coupled to the gravitational one. If the spinor field

Non-minimal coupling of photons and axions propagation of electromagnetic waves non-minimally coupled to the gravitational and axion fields. We focus

Non-minimal pp-wave Einstein-Yang-Mills-Higgs model: Color cross-effects induced by curvature interacting with curvature. The influence of the non-minimal coupling on the test particle motion

Non-minimal Einstein-Maxwell theory: The Fresnel equation and the Petrov classification of a trace-free susceptibility tensor
for electromagnetic waves non-minimally coupled to space-time curvature, based on analysis of the susceptibility

Non-minimal coupling of photons and axions propagation of electromagnetic waves non-minimally coupled to the gravitational and axion fields. We focus

Non-minimal pp-wave Einstein-Yang-Mills-Higgs model: Color cross-effects induced by curvature interacting with curvature. The influence of the non-minimal coupling on the test particle motion

Non-minimally coupled nonlinear spinor field in Bianchi type-I cosmology of the corresponding Universe also differs. For example, while a linear spinor field with non-minimal coupling or a

Non-minimal coupling for the gravitational and electromagnetic fields: A general system of equations fields. The procedure is based on a non-minimal nonlinear extension of the standard Einstein

Electromagnetic waves in an axion-active relativistic plasma non-minimally coupled to gravity for a non-minimal coupling of the gravitational, electromagnetic and pseudoscalar (axion) fields in a

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