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Superpixel Clustering for Detection of Binary Object Hierarchy Using Modernized Classical Clustering Methods
Kharinov, M.
approaching by piecewise constant approximations by means of iterative clustering of image pixels
Short-Wave Approximation for Macroscopic Cosmology with Higgs Scalar Field
Ignat’ev Y.G., Ignat’ev D.Y.
-wave approximation for perturbations of the scalar Higgs and gravitational fields has been obtained and examined
Optimal control of a perturbed sweeping process via discrete approximations
Cao T.H., Mordukhovich B.S.
with highly irregular data that cannot be treated by means of known results in optimal control theory
Pair production from the vacuum by a weakly inhomogeneous space-dependent electric potential
Gavrilov, Sergey P., Gitman, Dmitri M., Shishmarev, A. A.
in restricted space areas, which means that the fields vanish as jxj → ∞) in the absence of the corresponding
Analytical approximation of 〈φ2〉 for a massive scalar field in static spherically symmetric spacetimes
Sushkov S.
An analytical approximation of 〈φ2〉 for a massive scalar field in a zero-temperature vacuum state
Analytical approximation for 〈φ2〉 of a quantized scalar field in ultrastatic asymptotically flat spacetimes
Popov A.
Analytical approximations for 〈φ2〉 of a quantized scalar field in ultrastatic
Description of Stark Structure of the Elpasolites Cs2NaPrCl6, Cs2NaYCl6 and Cs2NaYBr6
Fomicheva, L., Dunina, E. V., Kornienko, A. A.
, Cs2NaYBr6 crystal systems is performed in the approximation of the weak and anomalous strong
Simulations of magnetic and magnetoelastic properties of Tb 2Ti 2O 7 in paramagnetic phase
Klekovkina V., Zakirov A., Malkin B., Kasatkina L.
charge model of crystal field theory and a mean field approximation. The set of electron
Аппроксимационные неравенства во взвешенных пространствах Орлича
Акгюн Рамазан
APPROXIMATION INEQUALITIES IN WEIGHTED ORLICZ SPACES
Analytical approximation of (φ2) for a massive scalar field in static spherically symmetric spacetimes
Sushkov S.
An analytical approximation of (φ 2) for a massive scalar field in a zero-temperature vacuum state

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