Representation of solutions of evolution equations on a ramified surface by Feynman formulae
We obtain solutions of parabolic second-order differential equations for functions in the class defined on a ramified surface . By using Chernoff's theorem, we prove that such solutions, whenever they exist, can be represented by Lagrangian Feynman formulae, that is, they can be written as limi...
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Published in | Izvestiya. Mathematics Vol. 82; no. 3; pp. 494 - 511 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
Providence
London Mathematical Society, Turpion Ltd and the Russian Academy of Sciences
01.06.2018
IOP Publishing |
Subjects | |
Online Access | Get full text |
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Summary: | We obtain solutions of parabolic second-order differential equations for functions in the class defined on a ramified surface . By using Chernoff's theorem, we prove that such solutions, whenever they exist, can be represented by Lagrangian Feynman formulae, that is, they can be written as limits of integrals over Cartesian powers of the configuration space as the number of factors tends to infinity. |
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ISSN: | 1064-5632 1468-4810 |
DOI: | 10.1070/IM8376 |