Nonlinear integroparabolic equations on unbounded domains: existence of classical solutions with special properties (Q2760736)
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scientific article; zbMATH DE number 1682265
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Nonlinear integroparabolic equations on unbounded domains: existence of classical solutions with special properties |
scientific article; zbMATH DE number 1682265 |
Statements
13 December 2001
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nonlinear ultraparabolic equation of the Fokker-Plank type
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boundary-value problem
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second-order parabolic equation
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0.9186436
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0.91285783
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0.9082274
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0.9081563
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0.90650177
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Nonlinear integroparabolic equations on unbounded domains: existence of classical solutions with special properties (English)
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Under consideration is the following parabolic equation: NEWLINE\[NEWLINE \frac{\partial \rho}{\partial t}= \frac{\partial^2 \rho}{\partial \omega^2} + \varepsilon \frac{\partial^2 \rho}{\partial \theta^2} - F(\omega) \frac{\partial \rho}{\partial \theta} + \frac{\partial }{\partial \omega}(F\rho)- \Omega \frac{\partial \rho}{\partial \omega} -K_s(\theta,t) \frac{\partial \rho}{\partial \omega},\;\tag{1} NEWLINE\]NEWLINE where \((\theta,\omega,t,\Omega)\in Q=[0,2\pi]\times {\mathbb R} \times [0,T]\times [-G,G]\), \(\varepsilon>0\), NEWLINE\[NEWLINE K_s(\theta,t)= \int_{-\infty}^{\infty}\int_{-\infty}^{\infty}\int_{0}^{2\pi} g(\Omega)\sin(\varphi-\theta)\rho(\varphi,\omega,t,\Omega) d\varphi d\omega d\Omega, NEWLINE\]NEWLINE and \(F(\omega)\) is a given function of a Hölder class. Equation (1) is a parabolic regularization of the nonlinear ultraparabolic equation of the Fokker-Plank type which arises in physics. The equation is furnished with the following boundary and initial conditions: NEWLINE\[NEWLINE (\rho,\rho_{\theta})|_{\theta=0}=(\rho,\rho_{\theta})|_{\theta=2\pi},\;\;\rho|_{t=0}=\rho_0(\theta,\omega,\Omega). \tag{2} NEWLINE\]NEWLINE Using a priori bounds and the method of successive approximations, the authors establish the existence and uniqueness theorem for classical solutions to problem (1), (2), i.e., a solution belongs to some Hölder space in \(Q\). Moreover, under the corresponding conditions on the initial data, it is shown that a constructed solution is exponentially decreasing in \(\omega\), nonnegative, and the equality NEWLINE\[NEWLINE \int_0^{2\pi}\int_{-\infty}^{\infty} \rho(\theta,\omega,t,\Omega) d\omega d\theta=1 NEWLINE\]NEWLINE holds whenever NEWLINE\[NEWLINE \int_0^{2\pi}\int_{-\infty}^{\infty}\rho_0(\theta,\omega,\Omega) d\omega d\theta=1 .NEWLINE\]
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