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Impulsive control problems without the frobenius condition
Arutyunov A., Karamzin D., Lobo Pereira F.
In this chapter, the same dynamical system and problem as in the previous chapter are considered
Construction of Multidimensional Vector Fields Whose Projections Onto Coordinate Planes Have Given Topological Structures
Volkov S.V.
The aim of the work is to construct multidimensional vector fields that are represented
Construction of Flat Vector Fields with Prescribed Global Topological Structures
Volkov S.V.
In this paper, we present a method for constructing vector fields whose phase portraits have finite
Spontaneous color polarization as a modus originis of the dynamic aether
Balakin A., Kiselev G.
the multiplet of vector fields. The scenario of the transition to the dynamic aether, which is characterized
Analytical Synthesis of the State Observer of a Bilinear Dynamic System with Vector Input
Asanov A., Dem’yanov D.
© 2019, Allerton Press, Inc. The problem of estimating the state vector of a bilinear dynamic
Relativistic Dynamics of Vector Bosons in the Field of Gravitational Radiation
Balakin A., Kurbanova V.
the dynamical equations for the particle four-velocity and the equations for the polarization four-vector
The extended Einstein-Maxwell-Aether-Axion model: Exact solutions for axionically controlled pp-wave aether modes
, the dynamic unit vector field describing the velocity of an aether, and the pseudoscalar field associated
Construction of Planar Vector Fields with a Nonsimple Critical Point of Prescribed Topological Structure
Volkov S.V.
The problem of constructing n-linear (n ≥ 2) plane vector fields with an isolated critical point
Dynamics of the kinetic energy flux density vector in the lower 200-meter layer of the atmosphere
Krasnenko, Nikolay P., Potekaev, Aleksandr I., Shamanaeva, Luidmila G.
In the report, the diurnal hourly dynamics of the mean and turbulent components of the kinetic
Einstein-aether theory: Dynamics of relativistic particles with spin or polarization in a Gödel-type universe
Balakin A., Popov V.
consider a cosmological model, which describes the evolution of the unit dynamic vector field

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