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Interacting spinor, vector and scalar fields in Bianchi-I space-time: the isotropization problemSummary: "We consider Bianchi-I type universes with interacting spinor, vector and scalar fields
Interaction of the axionic dark matter, dynamic aether, spinor and gravity fields as an origin of oscillations of the fermion effective mass, the axionic dark mater, described by the pseudoscalar field, the spinor field associated with fermion
Nonlinear Spinor and Scalar Fields in the Friedmann's Model of Universe: Problem of Initial Singularity and spinor fields with nonlinear terms being functions of spinor field invariants S2
New symmetries, conserved quantities and gauge nature of a free dirac field corresponding pair of the KGE solutions for a doublet of scalar fields. In this way, we obtain a “spinor
Physical theories in hypercomplex geometric description equivalent to the spinor (Schrödinger-Pauli and Hamilton-Jacobi) equations of mechanics. It is also
Spin and magnetic excitation in chiral model of graphene of the 8-spinor generalization of the scalar chiral model of graphene, we consider the spin and quasi
Entangled Solitons and Einstein-Podolsky-Rosen Correlations in the nonlinear spinor eld model, the Einstein-Podolsky-Rosen (EPR) spin correlation is calculated and shown
ФОТОНЫ КАК СОЛИТОНЫ В КИРАЛЬНОЙ МОДЕЛИ СКИРМА - ФАДДЕЕВА to represent particles as clots of Brioschi16-spinor field within the scope of the Skyrme - Faddeev chiral
The vacuum expectation value of the spinor massive field in the cosmic string spacetimeThe vacuum expectation value of the spinor massive field in the cosmic string spacetime
Pre-geometric structure of quantum and classical particles in terms of quaternion spinorsPre-geometric structure of quantum and classical particles in terms of quaternion spinors
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