Deformation Methods of Functionally Defined Objects using Perturbation Functions

Author(s):  
Sergey Vyatkin ◽  
Anatoliy Snigur ◽  
Alexandr Romanyuk ◽  
Pavlo Mykhaylov ◽  
Mykola Nechyporuk ◽  
...  
2021 ◽  
Author(s):  
Pavlo Mykhaylov ◽  
Sergey Vyatkin ◽  
Roman Chekhmestruk ◽  
Ivan Perun ◽  
Tetiana Korobeinikova

Author(s):  
Joram Lindenstrauss ◽  
David Preiss ◽  
Tiˇser Jaroslav

This chapter describes smooth variational principles (of Ekeland type) as infinite two-player games. These variational principles are based on a simple but careful recursive choice of points where certain functions that change during the process have values close to their infima. Like many other recursive constructions, the choice has a natural description using the language of infinite two-player games with perfect information. The chapter first considers the perturbation game used in Theorem 7.2.1 to formulate an abstract version of the variational principle before showing how to specialize it to more standard formulations. It then examines the bimetric variant of the smooth variational principle, along with the perturbation functions that are relatively simple. It concludes with an assessment of cases when completeness and lower semicontinuity hold only in a bimetric sense.


2018 ◽  
Vol 1015 ◽  
pp. 032115 ◽  
Author(s):  
S I Vyatkin ◽  
A N Romanyuk ◽  
L A Savytska ◽  
T I Troianovska ◽  
N V Dobrovolska

1993 ◽  
Vol 132 ◽  
pp. 241-253
Author(s):  
R. Spurzem

AbstractA reinvestigation of the linear perturbation theory is presented, which examines the hydrostatic readjustment of an isolated self-gravitating gas sphere to a redistribution of energy. The here presented model describes a stellar system by the common equations of gas in hydrostatic equilibrium but with the effect of the anisotropic velocity distribution on the pressure gradient. We take as equilibrium models the singular isothermal solution with and without anisotropy. The total variation of the Boltzmann entropy resulting from a perturbation of the system caused by a redistribution of heat (i.e. r.m.s. kinetic energy of the stars) is calculated for anisotropic solutions to first order as well as to second order for the isotropic equilibrium. The extremized eigenfunctions which represent the entropy and anisotropy perturbation functions, are determined analytically. They exhibit gravothermal behaviour in the central region where heat is removed. It is also found that the anisotropy readjusts non-thermally in the sense that the system departs from isotropy although the total entropy increases.


2021 ◽  
Author(s):  
Pavlo Mykhaylov ◽  
Sergey Vyatkin ◽  
Roman Chekhmestruk ◽  
Ivan Perun ◽  
Tetiana Korobeinikova ◽  
...  

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